{"as_of":"2026-08-22T05:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f1221e159dab050af4dfa97c12e37474fbe6e7392fe12ef1682f74182a36c2a0","coverage":[{"denominator":155,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T00:39:49.564567Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-01T06:16:24.888925Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"cited_work":{"arxiv_id":"2607.05208","doi":"10.48550/arxiv.2607.05208","metadata_source":"pith","pith_arxiv_id":"2607.05208","snapshot_observed_at":"2026-08-01T06:16:24.888925Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","venue":"astro-ph.GA","work_id":"c9eed13d-76b7-4672-8c6d-ff2a3302242b","year":2026},"citing_paper":{"arxiv_id":"2607.26177","last_updated":"2026-07-28T18:36:46Z","snapshot_observed_at":"2026-08-18T15:30:47.043177Z","submitted_at":"2026-07-28T18:36:46Z","title":"How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations","version":1},"reference_index":264,"source":"arxiv_source","source_observed_at":"2026-08-01T00:39:49.564567Z"},"links":{"cited_paper":"/paper/2607.05208","citing_paper":"/paper/2607.26177"},"observation_digest":"sha256:5ae2f9a5c6f0719df5a7a460267fa47ed92face0dbd2d435895cda08a0bea3c5","observation_id":"652d7c7b-0e7b-406a-9a78-d5fb78bac3ca","resolution":{"observed_at":"2026-08-01T00:41:15.127047Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2607.05208/citation-record","integrity":"/paper/2607.05208/integrity","json":"/paper/2607.05208/citation-record.json","paper":"/paper/2607.05208"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ace18b","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.3847/2041-8213/ace18b , keywords =","venue":"The Astrophysical Journal Letters","work_id":"a197123b-8ce4-4b8d-bee2-547822fc0224","year":2041},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:2bdff74849fcad764cab8861ac3ba66c2e78e52117ab2fa00af1c99d97c9f56c","observation_id":"7686baa8-87ba-46b1-a95e-bbb8af1e9e52","resolution":{"observed_at":"2026-07-07T23:34:19.417820Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:19.653746+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:19.653746+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/acdac6","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.3847/2041-8213/acdac6 , keywords =","venue":"The Astrophysical Journal Letters","work_id":"c4e36d40-1bdc-46a1-8190-df81b311338c","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:4fc0cb213607bea2a3b34cd6cd2af6b7f2a4346a3162141cccab4f4efd073717","observation_id":"32eb11a6-ed40-444f-bfb3-6034d044bd43","resolution":{"observed_at":"2026-07-07T23:34:19.215924Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:19.486152+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:19.486152+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2025.10066","doi":"10.1017/pasa.2025.10066","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"good enough","venue":"Publications of the Astronomical Society of Australia","work_id":"1c678313-dcdb-4d74-8e92-fa34d254d2ac","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:271136c4f645d19e3b253b025be25c4f89a26f83931935010a01b2bcc82d3df3","observation_id":"45d0692c-b4cc-4883-97c3-5f12b708d27e","resolution":{"observed_at":"2026-07-07T23:34:19.259324Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:04.5278+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:04.5278+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202346844","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.354897Z","title":"Arumugam, P","venue":"Astronomy & Astrophysics","work_id":"467bd3f3-d1db-4832-b5f5-99b895f3a8f8","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:14269e7a394da1a3b350372b8addde8f991550d33d2ad819e18dbaebe771afb1","observation_id":"a2c858c2-94d3-48be-8acb-30bb34aa6ed2","resolution":{"observed_at":"2026-07-07T23:34:19.357194Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-20T15:23:18.914168+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-20T15:23:18.914168+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/acdd02","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Reardon and Andrew Zic and Ryan M","venue":"The Astrophysical Journal Letters","work_id":"d9a50e82-9ea2-4a36-a530-f9d12ab303e3","year":2041},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:fa15212a92dd1b293986642877f6430ab08ce98a9d73fdd92e10c3c9cee66ccc","observation_id":"39c4dc70-3f4f-4c25-8711-2097283a3c84","resolution":{"observed_at":"2026-07-07T23:34:19.187709Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-08T04:08:18.043711+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-08T04:08:18.043711+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1674-4527/acdfa5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Searching for the Nano-Hertz Stochastic Gravitational Wave Background with the Chinese Pulsar Timing Array Data Release I.Res","venue":"Research in Astronomy and Astrophysics","work_id":"1d737179-87a2-4325-842f-89fe528f0f92","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:2a2d3d6d5df5c79314c829de9cb3aa092a7b517f7f22382cb529eb2c7a893747","observation_id":"859be1a8-84e8-404f-a7c9-369409fcc0ea","resolution":{"observed_at":"2026-07-07T23:34:19.279562Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-08T04:08:18.139982+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-08T04:08:18.139982+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.17549","last_updated":"2025-08-31T19:43:33Z","snapshot_observed_at":"2026-08-18T22:50:27.630354Z","submitted_at":"2025-04-24T13:40:06Z","title":"Premature supermassive black hole mergers in cosmological simulations of structure formation","version":2},"cited_work":{"arxiv_id":"2504.17549","doi":"10.1093/mnras/staf1336","metadata_source":"pith","pith_arxiv_id":"2504.17549","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Premature supermassive black hole mergers in cosmological simulations of structure formation","venue":"astro-ph.GA","work_id":"d85b8f14-3a8e-4822-87e1-a211f1450084","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2504.17549","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8aa520019cf8022e289173f43100f96d24dbfea1ffde3e3d4dbc26b7b7526b34","observation_id":"3a50eda8-444b-4e83-8769-7951ea5d0e24","resolution":{"observed_at":"2026-07-07T23:34:19.359919Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:05.768732+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:05.768732+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.703978Z","title":"Nature , keywords =","venue":null,"work_id":"8b32132a-b560-46fd-801a-323af9559233","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:c8bac8ff8c5390743a581d8335d7c97b0f24d6075c3f441348f58594009830f2","observation_id":"fdcffbed-e996-49c7-9921-0d703879223e","resolution":{"observed_at":"2026-07-07T23:34:19.705544Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stx1638","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Taylor , title =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"4ff5f007-1a7d-4b5a-a14a-e2e04a7c4d51","year":2017},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:1fb64498f536fdaaa9dd36752880b20039d0a4c7810f5e5e5489a9964394a938","observation_id":"b56ba1fc-54bc-40f9-80d3-540954a4d171","resolution":{"observed_at":"2026-07-07T23:34:19.369231Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:25.034865+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:25.034865+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stw2452","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Z., Blecha, L., & Hernquist, L","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"a65c369c-95fe-4042-939d-9ca940400cb7","year":2017},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:3b498a24d8b28cc85e422e0ceedcb1468123ab5378256ef1ea562716a50baa0a","observation_id":"efb05793-e1df-4894-b3a4-6d0ef243bf0b","resolution":{"observed_at":"2026-07-07T23:34:19.171532Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:24.915577+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:24.915577+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.01024","last_updated":"2025-02-03T03:37:56Z","snapshot_observed_at":"2026-08-19T07:01:29.715257Z","submitted_at":"2025-02-03T03:37:56Z","title":"The Gravitational Wave Background from Massive Black Holes in the ASTRID Simulation","version":1},"cited_work":{"arxiv_id":"2502.01024","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.01024","snapshot_observed_at":"2026-07-07T23:34:19.536661Z","title":"The Gravitational Wave Background from Massive Black Holes in the ASTRID Simulation","venue":"astro-ph.GA","work_id":"1271b74c-87a0-438f-a172-1f4d229e1d27","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2502.01024","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:b7b55ab5980247960164d206ab73aea641eff53165ecd5814b9614d95f3f8526","observation_id":"682c60f8-c06c-40ae-b02a-57434927676f","resolution":{"observed_at":"2026-07-07T23:34:19.539079Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.05410","last_updated":"2022-02-11T01:59:44Z","snapshot_observed_at":"2026-08-19T11:13:23.351108Z","submitted_at":"2022-02-11T01:59:44Z","title":"An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation","version":1},"cited_work":{"arxiv_id":"2202.05410","doi":"10.1093/mnras/stac388","metadata_source":"pith","pith_arxiv_id":"2202.05410","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation","venue":"astro-ph.GA","work_id":"4393dc51-877d-494e-ab75-02292055b2ef","year":2022},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2202.05410","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:1bf17224f726a951c848f1eb1c31aaae5bc87866cf5c258c86bab3d439383b1a","observation_id":"8b894468-c3b4-4b89-b4f7-e9b941fa25cc","resolution":{"observed_at":"2026-07-07T23:34:19.327464Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:06.978149+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:06.978149+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.05064","last_updated":"2018-07-06T10:25:30Z","snapshot_observed_at":"2026-08-14T19:26:08.957235Z","submitted_at":"2018-04-13T18:00:00Z","title":"The FABLE simulations: A feedback model for galaxies, groups and clusters","version":2},"cited_work":{"arxiv_id":"1804.05064","doi":"10.1093/mnras/sty1780","metadata_source":"doi_reference","pith_arxiv_id":"1804.05064","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"A., Puchwein E., Shen S., Sijacki D., 2018, @doi [ ] 10.1093/mnras/sty1780 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.479.5385H 479","venue":"astro-ph.GA","work_id":"7e70aadf-3ac8-455b-bcd2-db79710ae0ed","year":2018},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"cited_paper":"/paper/1804.05064","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:ac4e3d79eb4e21e2b676bce45bd69bbc7232a7a862392c916b7c69dbf8c5ae05","observation_id":"0a598a3e-7da6-462f-a447-b338cb961ce8","resolution":{"observed_at":"2026-07-07T23:34:19.419996Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:07.287875+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:07.287875+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.00013","last_updated":"2019-08-16T14:25:37Z","snapshot_observed_at":"2026-08-19T15:53:03.628623Z","submitted_at":"2019-04-30T18:00:00Z","title":"The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations","version":2},"cited_work":{"arxiv_id":"1905.00013","doi":"10.1093/mnras/stz2301","metadata_source":"pith","pith_arxiv_id":"1905.00013","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations","venue":"astro-ph.CO","work_id":"05cfc1ca-0f31-43c6-879c-6ff620ef794f","year":2019},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.00013","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:37c43fa6207a2808ec0922a9b4cd1b5dee2ef90c4246297593a6068ca38f915b","observation_id":"f4a7177f-3fe0-4279-8828-8b66c30d4c5c","resolution":{"observed_at":"2026-07-07T23:34:19.146632Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:07.644284+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:07.644284+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.12367","last_updated":"2020-07-25T11:21:10Z","snapshot_observed_at":"2026-08-14T17:24:46.352710Z","submitted_at":"2019-11-27T19:00:01Z","title":"The baryon content of groups and clusters of galaxies in the FABLE simulations","version":2},"cited_work":{"arxiv_id":"1911.12367","doi":null,"metadata_source":"pith","pith_arxiv_id":"1911.12367","snapshot_observed_at":"2026-07-07T23:34:19.370551Z","title":"The baryon content of groups and clusters of galaxies in the FABLE simulations","venue":"astro-ph.GA","work_id":"805841c9-386f-4279-a10e-507ce8a42a90","year":2019},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1911.12367","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:d732372db610c5c5a9c54a7fa2954a7f172e9beb15eb92c248c362b8b5f8c46c","observation_id":"5e49a0ef-1d83-40ef-a951-0d4a2566ff35","resolution":{"observed_at":"2026-07-07T23:34:19.372099Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staf1435","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Bigwood, M","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"119f391e-49d2-43c7-99ba-3d423f3b30ef","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8f3809cce21ba27390ab13efbe6dc70eb89f4c5ede2a6bbc3707b74ceaaaf6a1","observation_id":"16bbc1bb-7ee7-43e8-9035-40e3f048eda4","resolution":{"observed_at":"2026-07-07T23:34:19.387024Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:08.275678+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:08.275678+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac5f0b","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"H., Rantala, A., et al","venue":"The Astrophysical Journal","work_id":"49a88ec2-5b3e-45ee-af22-0ff44c9d9f16","year":2022},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:bb5e138fccd203093b839b553261794f7b1dcf48886f62047c2addf49ffa799c","observation_id":"8576f081-10fa-45c2-87ab-1148b8dbfa13","resolution":{"observed_at":"2026-07-07T23:34:19.564703Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:08.58095+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:08.58095+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0264-9381/30/22/224014","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Insights into the astrophysics of supermassive black hole binaries from pulsar timing observations , volume=","venue":"Classical and Quantum Gravity","work_id":"0a322541-9ac2-4336-a2d2-45b8e661c490","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:050927c20059be8dd7f8084de33c94b79a98e49674bbbbef2c7111d76577e8bb","observation_id":"e90735ed-5f29-4799-9aeb-df36072e3f51","resolution":{"observed_at":"2026-07-07T23:34:19.561141Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:08.857921+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:08.857921+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stx1093","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Monthly Notices of the Royal Astronomical Society , volume =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"47715c28-023d-44c5-b32c-3d073d7efd30","year":2017},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:06d308836b9eafe21b9338e5331123ff49317a8f2e088d31e4a9b0d793305cfc","observation_id":"2639fb4b-c3b8-4299-bf71-46289c4b015a","resolution":{"observed_at":"2026-07-07T23:34:19.287092Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:09.096995+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:09.096995+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202452562","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"Astronomy and Astrophysics","work_id":"5306b938-8a21-4688-9347-5c118017595f","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:f19a41212056e470eb5d81cc3b80d440903216cd2898128db16323efe0d430f0","observation_id":"214ca7b8-5c70-4364-9d5f-6916f84c4e45","resolution":{"observed_at":"2026-07-07T23:34:19.439042Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:09.390574+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:09.390574+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2005","doi":"10.1111/j.1365-2966.2005","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"A., okas E","venue":null,"work_id":"fbe25bd0-9403-4539-b873-fcf6743fba70","year":2005},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:fb282aebac098c088991da685217f4968d35fae1a5a569b0fbd516a128cc97bd","observation_id":"b48fea4e-734e-440e-86ab-7aa12143a905","resolution":{"observed_at":"2026-07-07T23:34:19.284830Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/151796","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:16:47.715138Z","title":"M., Press W","venue":"The Astrophysical Journal","work_id":"1cd6e75e-7b2e-40f9-9322-31ed7900a66d","year":1972},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:ecd6b164d62c9c27bfa077b208d89385ac09f6db7ded790c368f06e9a6af282d","observation_id":"47363478-fbd1-40ca-ad9e-202761cd26ea","resolution":{"observed_at":"2026-07-07T23:34:19.309764Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:14.924321+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:14.924321+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2012","doi":"10.1111/j.1365-2966.2012","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"and Shibahashi , H","venue":null,"work_id":"91cc99ad-bdb6-42b2-afbd-e26dad5ec964","year":2012},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:c12a23091e5129414dfdae8f0160fc18665d797a0fd99de86fcc9494bcc74aad","observation_id":"d6a1f381-877f-4f91-8d66-a137d16ab096","resolution":{"observed_at":"2026-07-07T23:34:19.296384Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-13T20:49:50.088461+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T20:49:50.088461+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504097","last_updated":"2005-04-06T08:50:45Z","snapshot_observed_at":"2026-08-05T05:39:13.755503Z","submitted_at":"2005-04-05T07:08:11Z","title":"Simulating the joint evolution of quasars, galaxies and their large-scale distribution","version":2},"cited_work":{"arxiv_id":"astro-ph/0504097","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0504097","snapshot_observed_at":"2026-07-10T19:37:33.835133Z","title":"Simulating the joint evolution of quasars, galaxies and their large-scale distribution","venue":"astro-ph","work_id":"d7c52e22-1d67-45cc-9512-2834a57ec6ad","year":2005},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0504097","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:6bcc124a37269872228b45d783646a55d4c234f1fbe129704e7a6e3743802b2b","observation_id":"4177ae13-d891-4d19-adcc-746387743865","resolution":{"observed_at":"2026-07-07T23:34:19.422547Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.00693","last_updated":"2023-09-01T18:27:16Z","snapshot_observed_at":"2026-08-20T09:22:08.320559Z","submitted_at":"2023-09-01T18:27:16Z","title":"Comparing recent PTA results on the nanohertz stochastic gravitational wave background","version":1},"cited_work":{"arxiv_id":"2309.00693","doi":"10.48550/arxiv.2309.00693","metadata_source":"pith","pith_arxiv_id":"2309.00693","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Agazieet al.[International Pulsar Timing Array],Comparing recent PTA results on the nanohertz stochastic gravitational wave background,Astrophys","venue":"astro-ph.HE","work_id":"9a4c3027-c074-4c91-bc50-4446b6b13549","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2309.00693","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:d8507536d4b943d247b0c9663cfc9f9857dc668e9047750356f72100751849c9","observation_id":"63c14bee-6959-4df1-90ca-78a4dbc8043a","resolution":{"observed_at":"2026-07-07T23:34:19.151465Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2009","doi":"10.1111/j.1365-2966.2009","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607","venue":null,"work_id":"23562d5d-936a-4b08-a6f0-15466b0fcd7c","year":2009},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:02f3a6ab8a363b1d29d7f7342c74d777bed61950b2c49956febaf3a0783ca626","observation_id":"5b4fd1da-3010-4fbe-b762-c694a719655a","resolution":{"observed_at":"2026-07-07T23:34:19.478106Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/183954","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"The Astrophysical Journal","work_id":"bcb4beca-226f-4339-ad3b-95e05e5a3b8b","year":1983},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:b49d23762ffd4a1b960fd59c510874e4df18300631ab71a1182828218bde9d28","observation_id":"722882ed-89b3-4d76-9ab2-77a774ed28fb","resolution":{"observed_at":"2026-07-07T23:34:19.316610Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-08T04:08:17.982642+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-08T04:08:17.982642+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.719414Z","title":"Nature , keywords =","venue":null,"work_id":"e4702540-728f-4ce4-84b4-1cf1183ac562","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:04b6f5412d58b71f876c75659a3b2f6edccf3c13278b8545f549dc1dce685a60","observation_id":"289d74e8-1d76-4946-b0b5-56d5796de234","resolution":{"observed_at":"2026-07-07T23:34:19.720893Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.713555Z","title":"The Astronomical Journal , keywords =","venue":null,"work_id":"5b26479c-a97d-4b7c-afa0-b748b313ba80","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:15756835c8f11e6566a21c77f1b3dfcd39b8c775b63523ec90ffdc3232b1fc57","observation_id":"f26a0af1-d778-4310-9867-ab3d6679caf2","resolution":{"observed_at":"2026-07-07T23:34:19.715166Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1304.7762","last_updated":"2013-04-29T19:58:33Z","snapshot_observed_at":"2026-08-21T20:46:38.414542Z","submitted_at":"2013-04-29T19:58:33Z","title":"Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies","version":1},"cited_work":{"arxiv_id":"1304.7762","doi":"10.1146/annurev-astro-082708-101811","metadata_source":"doi_reference","pith_arxiv_id":"1304.7762","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"C., 2013, @doi [ ] 10.1146/annurev-astro-082708-101811 , http://adsabs.harvard.edu/abs/2013ARA","venue":"astro-ph.CO","work_id":"d31a6d9c-0123-4707-9480-1dc7c1ed440a","year":2013},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"cited_paper":"/paper/1304.7762","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:6f7e08fa055acdb6e3ff1a2f6d00743ad81215b2e09abe54b3d5a6149262c441","observation_id":"78a01efc-2b9f-47ae-90b4-9238c0ceee8a","resolution":{"observed_at":"2026-07-07T23:34:19.475017Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:25.974677+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:25.974677+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.723580Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":"45ba2ed1-f1a6-4354-871d-947257562da8","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:4fa4c91da8f7be4fff1aa2c3c7cb74edddac0763beff89c54951417b071ce874","observation_id":"21d4d37a-e2e3-42eb-be8f-ee38bb770b46","resolution":{"observed_at":"2026-07-07T23:34:19.725116Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/342308","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2002, ApJ, 578, 90, doi: 10.1086/342308","venue":"The Astrophysical Journal","work_id":"8d1aaa84-713a-4aee-95e9-3d8f885eea67","year":2002},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:e13cf7275727c2251775251b4e1fa7269e0ab1ba8c9f2f67e3070b8f322e0892","observation_id":"7d31d8d7-2cf7-471f-9bc1-e1e659f1667f","resolution":{"observed_at":"2026-07-07T23:34:19.167374Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:10.783377+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:10.783377+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.705969Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":"e977890d-3ad1-4eff-950e-c83fe049eef6","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:7b0506e79d586e1cbeba79b14191684d4fa1958f84d5557a527aefa572a08f43","observation_id":"f34387a9-297a-4639-b28d-f0719eacceea","resolution":{"observed_at":"2026-07-07T23:34:19.707579Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.707958Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":"b6fcad58-725a-4e70-9641-4ba9bac82dde","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:c9efde3beee87e253f8c30f1d75831bd77d0264e0fde8b082263b579f9dd64c0","observation_id":"25a06598-d2d3-4229-b015-80984acecc87","resolution":{"observed_at":"2026-07-07T23:34:19.709502Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.709783Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":"8cb3cd54-3aee-4c4f-a815-750edd59b32b","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:557db8042cae544df26b4615beddec27acdca9191a6fabb95d868cf9edce0915","observation_id":"bcc61745-d40c-438e-ae24-c2edf4c18336","resolution":{"observed_at":"2026-07-07T23:34:19.711209Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.711661Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":"b90c4bc1-c870-4f86-91b0-c830d37557eb","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8877d6982e58a49cdf99109245ed6ba825f6e0e3629fc39ff77c7d97c23541a4","observation_id":"3c94dca8-bbc2-4fae-a928-e0aa451f8a54","resolution":{"observed_at":"2026-07-07T23:34:19.713141Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.731730Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":"4d4cf59c-4114-4a47-a376-fdff3b4b561d","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:6691fc14e55a12adb5e1efa56424f853590214c188cd4864bf8587eda1eae5b5","observation_id":"7a34aa6a-80d2-41e8-bda0-fb80b75ebe42","resolution":{"observed_at":"2026-07-07T23:34:19.733769Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/183.3.341","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.194122Z","title":"keywords =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"5b99fb29-3881-48a2-87e3-925aa0ee5e6b","year":1978},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:e8ec00cd36a0e89382df072581c0b9d93c85ca87ec92a2b8b3419dc4d083a247","observation_id":"1e755172-54dd-4a55-9f38-4a5f7369be8c","resolution":{"observed_at":"2026-07-07T23:34:19.195705Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-08T07:38:12.560807+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-08T07:38:12.560807+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0411104","last_updated":"2004-12-17T18:43:54Z","snapshot_observed_at":"2026-07-07T00:45:49.880615Z","submitted_at":"2004-11-04T08:12:30Z","title":"The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2","version":2},"cited_work":{"arxiv_id":"astro-ph/0411104","doi":"10.1086/427183","metadata_source":"pith","pith_arxiv_id":"astro-ph/0411104","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2","venue":"astro-ph","work_id":"50dfe882-35a0-4b40-b35d-3edd6826097c","year":2004},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0411104","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:7df0fc3df4548a8c2d09fc32429eca5f6b4425f6c6f4c1b1097aa33fefda57a5","observation_id":"643f28e3-91ea-40b2-9f05-09a1e55c22d2","resolution":{"observed_at":"2026-07-07T23:34:19.299205Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:11.013598+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:11.013598+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0712.0416","last_updated":"2007-12-05T20:17:31Z","snapshot_observed_at":"2026-08-15T10:26:25.676486Z","submitted_at":"2007-12-04T00:46:48Z","title":"Galaxy Mergers at z>1 in the HUDF: Evidence for a Peak in the Major Merger Rate of Massive Galaxies","version":2},"cited_work":{"arxiv_id":"0712.0416","doi":"10.1086/527463","metadata_source":"pith","pith_arxiv_id":"0712.0416","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Galaxy Mergers at z>1 in the HUDF: Evidence for a Peak in the Major Merger Rate of Massive Galaxies","venue":"astro-ph","work_id":"2d0591f7-bd24-4865-9a05-96ddb504f761","year":2007},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0712.0416","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:467e071e08c47e9872d624eeb78f355d854c84493bd38f2e01e1d3f321f2ef05","observation_id":"8d8cb14a-d8b6-44f7-add2-70ba0e5ecbcf","resolution":{"observed_at":"2026-07-07T23:34:19.277465Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:11.260722+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:11.260722+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.12188","last_updated":"2019-03-28T18:00:13Z","snapshot_observed_at":"2026-08-15T09:15:38.426796Z","submitted_at":"2019-03-28T18:00:13Z","title":"Observational constraints on the merger history of galaxies since $z\\approx6$: Probabilistic galaxy pair counts in the CANDELS fields","version":1},"cited_work":{"arxiv_id":"1903.12188","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.12188","snapshot_observed_at":"2026-07-10T17:27:26.503636Z","title":"Observational constraints on the merger history of galaxies since $z\\approx6$: Probabilistic galaxy pair counts in the CANDELS fields","venue":"astro-ph.GA","work_id":"7b7205c3-09b6-4db2-80df-302d267eb81b","year":2019},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1903.12188","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:2afb666aced6f3ae16cb249c7778c6545c367935044996d23c95980b619cbf3a","observation_id":"2bdd45b3-8081-42eb-868a-4bd83915149f","resolution":{"observed_at":"2026-07-07T23:34:19.365242Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.03067","last_updated":"2025-03-09T08:30:15Z","snapshot_observed_at":"2026-08-20T13:37:03.284750Z","submitted_at":"2023-10-04T18:00:01Z","title":"GA-NIFS: High number of dual active galactic nuclei at z~3","version":3},"cited_work":{"arxiv_id":"2310.03067","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.03067","snapshot_observed_at":"2026-07-07T23:34:19.380720Z","title":"2023, arXiv e-prints","venue":"astro-ph.GA","work_id":"f909f54c-81c9-4360-8459-ae00bd256424","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2310.03067","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:7e926d15e5bbf970888c5f661a2b9350298b69ee928973c6073bf287569eadac","observation_id":"04e04212-82ac-4ef4-b705-e7db20d748ff","resolution":{"observed_at":"2026-07-07T23:34:19.382254Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.03589","last_updated":"2024-08-22T10:09:55Z","snapshot_observed_at":"2026-08-17T16:18:31.280481Z","submitted_at":"2023-12-06T16:29:25Z","title":"GA-NIFS: JWST discovers an offset AGN 740 million years after the Big Bang","version":2},"cited_work":{"arxiv_id":"2312.03589","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.03589","snapshot_observed_at":"2026-07-07T23:34:19.488056Z","title":"GA-NIFS: JWST discovers an offset AGN 740 million years after the Big Bang","venue":"astro-ph.GA","work_id":"8b9c2929-5ee7-4a52-b6fc-84dfd16c06cf","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2312.03589","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:879079d9f26afda2a4c07fd6b28a0f9ac3b7be50b620fe40521218635728f56b","observation_id":"69cb4f10-debb-4e5e-beba-aefeaace0553","resolution":{"observed_at":"2026-07-07T23:34:19.489547Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.06647","last_updated":"2023-06-21T16:03:09Z","snapshot_observed_at":"2026-08-16T15:55:38.200782Z","submitted_at":"2023-02-13T19:20:16Z","title":"GA-NIFS: A massive black hole in a low-metallicity AGN at $z\\sim5.55$ revealed by JWST/NIRSpec IFS","version":2},"cited_work":{"arxiv_id":"2302.06647","doi":"10.48550/arxiv.2302.06647","metadata_source":"pith","pith_arxiv_id":"2302.06647","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.GA","work_id":"49e36f92-daa1-44f6-9b9f-64d6ed3cfb1b","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2302.06647","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:592da072cc493981903fd6175ee25f144ae9da3054be4006f4d2f865235fd99c","observation_id":"d82c39b0-7e90-4147-a5ed-5c644eee01bd","resolution":{"observed_at":"2026-07-07T23:34:19.499470Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/777/1/64","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Comerford and Kyle Schluns and Jenny E","venue":"The Astrophysical Journal","work_id":"5595b841-5d3b-460b-96a1-bd9b25856561","year":2013},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:ca62736076678d71c497393c455ec2a617fc01a921f5ea41b557aec538521931","observation_id":"dc9f5cea-060f-45b2-a8e3-9b383e2e291a","resolution":{"observed_at":"2026-07-07T23:34:19.334403Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:12.522449+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:12.522449+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/504825","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Rodriguez and G","venue":"The Astrophysical Journal","work_id":"95550cc7-393b-4146-9a16-e64fcafcf711","year":2006},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:03e1b25f167c46d75953571c27331215b8582f07f6fb9707e8a3def9a0f498d3","observation_id":"9f028dc0-241e-40eb-8676-f47f7a4e1152","resolution":{"observed_at":"2026-07-07T23:34:19.237764Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:29.337228+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:29.337228+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/acf7c5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"D., Greene, J","venue":"The Astrophysical Journal Letters","work_id":"7c495197-d617-46d3-b657-6cbb200de933","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:eb2c7e00198d84c3c64b49ac704dba34abb342dd5b5c391caa9d439b65c7678a","observation_id":"5e74f127-25f9-49e5-8adb-c09bf3b42f43","resolution":{"observed_at":"2026-07-07T23:34:19.210107Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-20T15:23:38.277687+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-20T15:23:38.277687+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.07396","last_updated":"2023-10-09T09:17:31Z","snapshot_observed_at":"2026-08-17T12:16:52.316890Z","submitted_at":"2023-05-12T11:48:17Z","title":"GMP-selected dual and lensed AGNs: selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, KECK/OSIRIS, and LBT/LUCI","version":2},"cited_work":{"arxiv_id":"2305.07396","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.07396","snapshot_observed_at":"2026-07-07T23:34:19.373335Z","title":"GMP-selected dual and lensed AGNs: selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, KECK/OSIRIS, and LBT/LUCI","venue":"astro-ph.GA","work_id":"b74a5aaf-a2bd-4957-8ffb-18f6a9471c03","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2305.07396","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:4502ba31a3cc11a17a26882a6aa113ba603e22738a1d3b30b2504b10a2c07cd6","observation_id":"e5e21a94-72a0-460f-b648-1897899625f2","resolution":{"observed_at":"2026-07-07T23:34:19.374632Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06756","last_updated":"2023-12-11T19:00:01Z","snapshot_observed_at":"2026-08-17T14:11:39.798743Z","submitted_at":"2023-12-11T19:00:01Z","title":"Where are NANOGrav's big black holes?","version":1},"cited_work":{"arxiv_id":"2312.06756","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.06756","snapshot_observed_at":"2026-07-07T23:34:19.335760Z","title":"Sato-Polito, M","venue":"astro-ph.CO","work_id":"f9bc693e-f7b3-4d4f-a028-06a37cff38fb","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2312.06756","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:a6715ae049c400335a6344cbb62a4a456d7a3607ab6fd0aaa10aedad7367ebb5","observation_id":"2508f600-e8a7-4b25-8dc6-e7956a662b63","resolution":{"observed_at":"2026-07-07T23:34:19.337826Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.111.023043","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Physical review. D/Physical review. D.","work_id":"eaa16aec-b288-4896-a2cb-d221a75ea7d8","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:ba6ec50f58e0b0492b527f59a23542c6b2875a6600f033daa7f2c85d405f063e","observation_id":"5fb2ad43-9a54-47b4-b139-088db6baba86","resolution":{"observed_at":"2026-07-07T23:34:19.200544Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:13.81575+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:13.81575+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.11671","last_updated":"2021-11-23T09:41:23Z","snapshot_observed_at":"2026-08-16T18:00:50.486802Z","submitted_at":"2021-08-26T09:36:47Z","title":"Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background","version":2},"cited_work":{"arxiv_id":"2108.11671","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.11671","snapshot_observed_at":"2026-07-09T20:06:29.683905Z","title":"Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background","venue":"astro-ph.GA","work_id":"ba639cba-fd51-4025-8f57-8f3d55b4d9a4","year":2021},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2108.11671","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:362a1d9b6a01a25f625237df5009acc1a3dfbbf4719b3e9a1c3e5fe430aecf06","observation_id":"3400aa85-76e2-4366-ae88-c70c373abdd5","resolution":{"observed_at":"2026-07-07T23:34:19.343272Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2008","doi":"10.1111/j.1365-2966.2008.12689.x","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"T., Ogilvie G","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"a585747b-4fbc-4555-a22d-a4a769e4179d","year":2008},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:72e4fed7b6124b45fec07bf34ae86eb4b6ad76f2700b9ce24c7f28abe288c4e3","observation_id":"773eac71-ae44-4294-9bc0-dfdac92f15a4","resolution":{"observed_at":"2026-07-07T23:34:19.441894Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2009","doi":"10.1111/j.1365-2966.2009","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607","venue":null,"work_id":"23562d5d-936a-4b08-a6f0-15466b0fcd7c","year":2009},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:be9ff8287a5ecbe7e64472b3c4cb4f1561b254c5e0a4783d26f349b147126f15","observation_id":"ec916d8a-79a9-4c4a-b54a-42ead130652d","resolution":{"observed_at":"2026-07-07T23:34:19.450053Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.725790Z","title":"The Astrophysical Journal Letters , keywords =","venue":null,"work_id":"55483662-c162-4992-a7a7-3e3c00b8c7b9","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:008ad0b79a1096118890ee7cded0e424d11da634643b194e0c23f6f03d0c2199","observation_id":"52d75cf6-3ead-4b67-8c67-215563853503","resolution":{"observed_at":"2026-07-07T23:34:19.727324Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1301.7184","last_updated":"2013-01-30T10:19:15Z","snapshot_observed_at":"2026-08-15T00:30:39.653952Z","submitted_at":"2013-01-30T10:19:15Z","title":"A black-hole mass measurement from molecular gas kinematics in NGC4526","version":1},"cited_work":{"arxiv_id":"1301.7184","doi":"10.1038/nature11819","metadata_source":"pith","pith_arxiv_id":"1301.7184","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"A black-hole mass measurement from molecular gas kinematics in NGC4526","venue":"astro-ph.CO","work_id":"a27b37c5-6c6d-47d5-8bff-d7075aeda2b8","year":2013},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1301.7184","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:188ccc6507f1fbb1d5900dcc8c117515074bf89d5a08662956c7412ec4f891bc","observation_id":"23f80233-8bd2-4303-901f-bc170f636c00","resolution":{"observed_at":"2026-07-07T23:34:19.509744Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:14.603493+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:14.603493+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.0816","last_updated":"2012-05-03T20:12:03Z","snapshot_observed_at":"2026-08-15T04:11:07.253710Z","submitted_at":"2012-05-03T20:12:03Z","title":"A Stellar Dynamical Mass Measurement of the Black Hole in NGC 3998 from Keck Adaptive Optics Observations","version":1},"cited_work":{"arxiv_id":"1205.0816","doi":"10.1088/0004-637x/753/1/79","metadata_source":"pith","pith_arxiv_id":"1205.0816","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"A Stellar Dynamical Mass Measurement of the Black Hole in NGC 3998 from Keck Adaptive Optics Observations","venue":"astro-ph.CO","work_id":"7cb0902e-9ae3-4eef-8fff-bc5cbcaae5fb","year":2012},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1205.0816","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:3fa9020d70cfee39680cdfc17ccc4efac17bf38e88ed140c3eeb3524ac4bcd03","observation_id":"5ff5cdda-37ee-49d4-b09e-c0153cac1dae","resolution":{"observed_at":"2026-07-07T23:34:19.220300Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:14.861535+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:14.861535+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.05917","last_updated":"2015-06-19T08:52:25Z","snapshot_observed_at":"2026-08-14T22:43:47.641996Z","submitted_at":"2015-06-19T08:52:25Z","title":"A Measurement of the Black-Hole Mass in NGC 1097 using ALMA","version":1},"cited_work":{"arxiv_id":"1506.05917","doi":"10.1088/0004-637x/806/1/39","metadata_source":"pith","pith_arxiv_id":"1506.05917","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"A Measurement of the Black-Hole Mass in NGC 1097 using ALMA","venue":"astro-ph.GA","work_id":"2f38460b-ab87-4c23-ab9f-5e45e346a8e6","year":2015},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1506.05917","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:855e38b2791f84c344073e81d1390d06c49d8d21facd11778ceae32abb26da3a","observation_id":"1a178fcd-fd65-4381-a3bd-b002588cefd5","resolution":{"observed_at":"2026-07-07T23:34:19.141713Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:15.114719+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:15.114719+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2006","doi":"10.1111/j.1365-2966.2006","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"and Yang , J","venue":null,"work_id":"7ef6cf0d-0877-424d-9dec-97ef68ca2212","year":2006},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:4f1f79a8c5fc99ef717fad904acb669fce2698c654e381271aaaa5a599cb02d4","observation_id":"1140719a-4ac0-4f49-a971-e68a054a94e0","resolution":{"observed_at":"2026-07-07T23:34:19.330174Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9704099","last_updated":"1997-04-11T15:36:36Z","snapshot_observed_at":"2026-08-17T09:34:27.729410Z","submitted_at":"1997-04-11T15:36:36Z","title":"A Search for \"Dwarf\" Seyfert Nuclei. IV. Nuclei with Broad H-alpha Emission","version":1},"cited_work":{"arxiv_id":"astro-ph/9704099","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9704099","snapshot_observed_at":"2026-07-07T23:34:19.569608Z","title":"A Search for \"Dwarf\" Seyfert Nuclei. IV. Nuclei with Broad H-alpha Emission","venue":"astro-ph","work_id":"2fdd40e7-b060-4f38-9dee-78d24a5be8c8","year":1997},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/9704099","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:0cd1cd2bd47099afc8a60d3b50bda1cd839dce0ed271473a7823c62f55d0af8d","observation_id":"341eb5cd-433f-4eda-8b70-a6f99e5d2a95","resolution":{"observed_at":"2026-07-07T23:34:19.574254Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0502551","last_updated":"2005-03-06T23:55:29Z","snapshot_observed_at":"2026-07-07T00:48:22.191947Z","submitted_at":"2005-02-25T21:29:10Z","title":"Radio Sources in Low-Luminosity Active Galactic Nuclei.IV. Radio Luminosity Function, Importance of Jet Power, and Radio Properties of the Complete Palomar Sample","version":2},"cited_work":{"arxiv_id":"astro-ph/0502551","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0502551","snapshot_observed_at":"2026-07-07T23:34:19.344671Z","title":"Radio Sources in Low-Luminosity Active Galactic Nuclei.IV. Radio Luminosity Function, Importance of Jet Power, and Radio Properties of the Complete Palomar Sample","venue":"astro-ph","work_id":"afc42621-92b3-40c3-a26f-8b9907b39a14","year":2005},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0502551","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:e15531dcf42add4bf241cd69045270f13f18ad896e3e848a609e62da4e67df33","observation_id":"1f5abc90-be81-418c-9add-71e877e40175","resolution":{"observed_at":"2026-07-07T23:34:19.346276Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9905012","last_updated":"1999-05-03T18:18:39Z","snapshot_observed_at":"2026-07-07T01:25:56.760989Z","submitted_at":"1999-05-03T18:18:39Z","title":"The Spectral Energy Distributions of Low-Luminosity Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":"astro-ph/9905012","doi":"10.1086/307137","metadata_source":"pith","pith_arxiv_id":"astro-ph/9905012","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Spectral Energy Distributions of Low-Luminosity Active Galactic Nuclei","venue":"astro-ph","work_id":"d16a111b-9e2c-45e8-8f32-b981e865934a","year":1999},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/9905012","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:22206124e18f12edf723cfba63363342357073741b16660302ec714a1c2da162","observation_id":"c0067d96-6e15-4b62-9f60-ddd26f448a94","resolution":{"observed_at":"2026-07-07T23:34:19.155202Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:16.253692+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:16.253692+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0209607","last_updated":"2002-09-30T06:54:29Z","snapshot_observed_at":"2026-07-07T00:28:47.808242Z","submitted_at":"2002-09-30T06:54:29Z","title":"Chandra Snapshot Observations of Low-Luminosity AGNs with a Compact Radio Source","version":1},"cited_work":{"arxiv_id":"astro-ph/0209607","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0209607","snapshot_observed_at":"2026-07-07T23:34:19.462661Z","title":"Chandra Snapshot Observations of Low-Luminosity AGNs with a Compact Radio Source","venue":"astro-ph","work_id":"9c88f97e-8159-4966-addc-1a8cf40cf83d","year":2002},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0209607","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:f28b8efa1b08736272e13c6842dee31ade9e4587f7d3eefcb443855fc79b6920","observation_id":"6b415b81-45c1-4ee1-afe3-cc78e955b711","resolution":{"observed_at":"2026-07-07T23:34:19.464128Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2004","doi":"10.1111/j.1365-2966.2004","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"M., Papadakis I","venue":null,"work_id":"cc97efa9-0c9d-45a7-ba7f-7bcd7663f68e","year":2004},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:4ae91ac542e9cf618b8574708eba5c6c5365fce6a43301e145aa98689ae80ab7","observation_id":"75ffb8e4-3c0f-4c33-a3bc-f32daf0a0bfa","resolution":{"observed_at":"2026-07-07T23:34:19.431199Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2007","doi":"10.1111/j.1365-2966.2007","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Mignone and Jonathan C","venue":null,"work_id":"93665276-ce05-4d2b-9ee4-0f0fe85b05b8","year":2007},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:3dc7190cd9c0d8c34c30d6ada4cf5e7c54a1e11acddf5d6f23a9b6d3fcbeb570","observation_id":"442d99a1-b8d5-403a-986a-101345099086","resolution":{"observed_at":"2026-07-07T23:34:19.305023Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0705.0020","last_updated":"2007-04-30T21:40:31Z","snapshot_observed_at":"2026-08-15T10:41:50.061867Z","submitted_at":"2007-04-30T21:40:31Z","title":"The Mass Function of Active Black Holes in the Local Universe","version":1},"cited_work":{"arxiv_id":"0705.0020","doi":null,"metadata_source":"pith","pith_arxiv_id":"0705.0020","snapshot_observed_at":"2026-07-07T23:34:19.291439Z","title":"The Mass Function of Active Black Holes in the Local Universe","venue":"astro-ph","work_id":"5f1c14a0-d7cc-4308-bda5-9dbc7c0c254f","year":2007},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0705.0020","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:5c95fa2533fcca06f123098bce0010b3b75e1faf3e8ce1e290dfcef9befed152","observation_id":"c2c67bc3-66ba-45c4-8e1e-05c6896c15e1","resolution":{"observed_at":"2026-07-07T23:34:19.292979Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.735972Z","title":"Annual Review of Astronomy and Astrophysics , keywords =","venue":null,"work_id":"afeb0544-e8d7-416c-a570-a9cf6ef1d9ed","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:2fa4d086a0a12772bfb79310148ed257b3d306663e538e9bf8103e5623ff0cb5","observation_id":"df959d60-b132-47fe-8dbe-758ec6b39ebb","resolution":{"observed_at":"2026-07-07T23:34:19.737719Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.717501Z","title":"Monthly Notices of the Royal Astronomical Society , keywords =","venue":null,"work_id":"7b24f101-a689-4b7b-9db7-2c42f155b45c","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:2e35429c5103533480f81b53851891435ad619f84518e00b28d53e8d56233b3c","observation_id":"165f216a-5d38-46dd-92da-1b872973c790","resolution":{"observed_at":"2026-07-07T23:34:19.719147Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03872","last_updated":"2024-12-04T16:26:25Z","snapshot_observed_at":"2026-08-16T14:12:14.081639Z","submitted_at":"2024-03-06T17:25:26Z","title":"A dormant, overmassive black hole in the early Universe","version":2},"cited_work":{"arxiv_id":"2403.03872","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.03872","snapshot_observed_at":"2026-07-07T23:34:19.451365Z","title":"Juodžbalis et al., Nature636, 594 (2024), 2403.03872","venue":"astro-ph.GA","work_id":"f7b2cc8f-08b7-4793-b901-5b3ba2a38065","year":2024},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2403.03872","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:f87d05ed37192463fb472395edb18db38d3f57f63e76645e2e0c4aaf3dcbeb51","observation_id":"7ac554b2-fdcb-4d4e-9a30-fc02bd8bb82f","resolution":{"observed_at":"2026-07-07T23:34:19.452822Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ad0158","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"The Astrophysical Journal Letters","work_id":"0ac81360-dcbd-4f9a-9449-959e920da819","year":2041},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:adb2db2c5e029ac24434d3b9c201786ee93ed651237911e6d136ca60abd281ef","observation_id":"cb8e9a23-5441-402d-8b06-61cd24673350","resolution":{"observed_at":"2026-07-07T23:34:19.180033Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:08:45.680485+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:08:45.680485+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/s41550-023-02111-9","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.531255Z","title":"2024, Nature Astron., 8, 126, 10.1038/s41550-023-02111-9","venue":"Nature Astronomy","work_id":"82db6d4d-d0e2-4ebb-8e7d-70fd6bfc8adc","year":2024},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:5a9d3adc43728007c1cd867b9a76c6e101c7be79b3120bbdec0fb9579233c323","observation_id":"4c3f46d6-febb-41ce-b8a4-a3205d8550f0","resolution":{"observed_at":"2026-07-07T23:34:19.536085Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:17.476385+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:17.476385+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202347640","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.172258Z","title":"keywords =","venue":"Astronomy & Astrophysics","work_id":"0d3a9d0f-1d41-4f5a-8484-1f6c6e42069b","year":2024},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:c89a41bfbef334b1438cfac371cb70d54278cd8d5fc7a7a8a1b952732ad07496","observation_id":"da68087f-afc5-4c47-8ce9-e33ea5b36e11","resolution":{"observed_at":"2026-07-07T23:34:19.175795Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:08:44.207012+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:08:44.207012+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"8711.2002","doi":"10.1046/j.1365-8711.2002.04944.x","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and LeBlanc , F","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"fc06b3ca-a49a-40e5-a61e-b9d148b54d70","year":2002},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:13a6a918b00e8b7826b581944f57ac07fa2b90b1c8e5e154f77ddfc7ce577249","observation_id":"e7d47e99-68df-442b-b99b-e8c7adf65eba","resolution":{"observed_at":"2026-07-07T23:34:19.243702Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1012.3213","last_updated":"2010-12-15T02:21:15Z","snapshot_observed_at":"2026-08-15T04:59:58.011116Z","submitted_at":"2010-12-15T02:21:15Z","title":"The Radiative Efficiency of Accretion Flows in Individual AGN","version":1},"cited_work":{"arxiv_id":"1012.3213","doi":null,"metadata_source":"pith","pith_arxiv_id":"1012.3213","snapshot_observed_at":"2026-07-07T23:34:19.375865Z","title":"The Radiative Efficiency of Accretion Flows in Individual AGN","venue":"astro-ph.CO","work_id":"f206ac81-f2c9-4df9-bdd7-9425568fab5b","year":2010},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1012.3213","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:270137c4748ea4f1429f4373912a31f835faec10b1838e40205cf06b3aa90577","observation_id":"bbab2c9e-0cbe-470d-a5d7-af586616c564","resolution":{"observed_at":"2026-07-07T23:34:19.377521Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.727609Z","title":"2001 , eprint=","venue":null,"work_id":"c2c2c300-bcc9-4e04-926f-5367eecd535a","year":2001},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:66b35a89aeff254f7347889446416c14aaac08283f1a3c8c2ac8c15b6251c539","observation_id":"c310baa4-ea48-45f2-b4da-dcf63b35f64f","resolution":{"observed_at":"2026-07-07T23:34:19.729165Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.730049Z","title":"2025 , eprint=","venue":null,"work_id":"dc15fd67-7518-4931-acf9-20081a055086","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:643de880d8ccd73ddec5f66e4964b26773ff6b34370e44be3906a5687b35c9d8","observation_id":"3a0a7d67-ea8a-469b-867a-764a248f4bd4","resolution":{"observed_at":"2026-07-07T23:34:19.731455Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ae2480","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal","work_id":"b1f53a5e-2a29-40d5-bda9-1e52b82b78d4","year":2026},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:f41e2d4fc3f1f486d8a5a5df3a3fb6f917b9250e3aa95de0b7ef21ab6767e7c3","observation_id":"1c962f51-6ad7-4c35-ac1a-4f9ec0c6646d","resolution":{"observed_at":"2026-07-07T23:34:19.213486Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-15T02:08:26.954545+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-15T02:08:26.954545+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.18179","last_updated":"2024-10-23T18:00:02Z","snapshot_observed_at":"2026-08-16T21:58:26.451258Z","submitted_at":"2024-10-23T18:00:02Z","title":"Impact of the observation frequency coverage on the significance of a gravitational wave background detection in PTA data","version":1},"cited_work":{"arxiv_id":"2410.18179","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.18179","snapshot_observed_at":"2026-07-07T23:34:19.443068Z","title":"Impact of the observation frequency coverage on the significance of a gravitational wave background detection in PTA data","venue":"astro-ph.HE","work_id":"89aaa0fd-e964-4102-bc8e-2aab79857910","year":2024},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2410.18179","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:5072ffd718b3a87b2c07c7d8f6576f81bab11b83f848a89715b8aafd1ad4450a","observation_id":"227960c0-58dd-4f07-bc67-097648250506","resolution":{"observed_at":"2026-07-07T23:34:19.444582Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.11946","last_updated":"2023-10-29T05:22:53Z","snapshot_observed_at":"2026-08-17T06:55:00.570708Z","submitted_at":"2023-03-21T15:40:30Z","title":"A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties","version":3},"cited_work":{"arxiv_id":"2303.11946","doi":"10.48550/arxiv.2303.11946","metadata_source":"pith","pith_arxiv_id":"2303.11946","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Harikane, Y","venue":"astro-ph.GA","work_id":"911a8c7e-c9f2-4829-a722-48f54edf78fd","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2303.11946","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:548f0b9e99de3568ea2016c374a62bd733c27ac4ca03e3da17f197a26535f6f0","observation_id":"2d641e23-b216-4870-9ec2-8458b65497a1","resolution":{"observed_at":"2026-07-07T23:34:19.470003Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.13117","last_updated":"2024-03-22T12:51:34Z","snapshot_observed_at":"2026-08-19T21:27:21.813710Z","submitted_at":"2023-09-22T18:00:11Z","title":"Testing strengths, limitations and biases of current Pulsar Timing Arrays detection analyses on realistic data","version":3},"cited_work":{"arxiv_id":"2309.13117","doi":"10.1051/0004-6361/202348084","metadata_source":"pith","pith_arxiv_id":"2309.13117","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Valtolina, G","venue":"astro-ph.HE","work_id":"d2637d72-61a5-4aa0-9402-ffec970c998c","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2309.13117","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8f0f050b542b4219084f01a1d3e585f01bfa75dc8306faa04c0cf32dea6517cb","observation_id":"1437c447-3368-4b1c-a806-dda48524983b","resolution":{"observed_at":"2026-07-07T23:34:19.472690Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:19.643812+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:19.643812+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.05959","last_updated":"2017-03-17T10:57:35Z","snapshot_observed_at":"2026-08-14T21:11:23.005525Z","submitted_at":"2017-03-17T10:57:35Z","title":"Planck confronts large scale structure: methods to quantify discordance","version":1},"cited_work":{"arxiv_id":"1703.05959","doi":"10.1103/physrevd.95.123535","metadata_source":"pith","pith_arxiv_id":"1703.05959","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Planck confronts large scale structure: methods to quantify discordance","venue":"astro-ph.CO","work_id":"6ccf0bf9-ae04-4f21-a885-93bb333644fa","year":2017},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1703.05959","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8584a4177ab12bd5808b3d3e7f8c2c8457b986db684fb93cbf2770b04a795d5c","observation_id":"b7b829b5-abfc-48e5-9ec8-ffcc7a6588f5","resolution":{"observed_at":"2026-07-07T23:34:19.290029Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:19.90168+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:19.90168+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T23:34:19.734237Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":"b9daf205-37ff-4c58-8466-6165d8df41fd","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:ecb9248639ea200f0665a7307f680263dd12f4969a6b8c47b4216ffc73be0535","observation_id":"5aac17db-d70e-476a-a9b3-1e416cbdb80e","resolution":{"observed_at":"2026-07-07T23:34:19.735836Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.2769","last_updated":"2014-09-09T15:06:02Z","snapshot_observed_at":"2026-08-14T23:20:09.598665Z","submitted_at":"2014-09-09T15:06:02Z","title":"Tension between the power spectrum of density perturbations measured on large and small scales","version":1},"cited_work":{"arxiv_id":"1409.2769","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.2769","snapshot_observed_at":"2026-07-07T23:34:19.163276Z","title":"Tension between the power spectrum of density perturbations measured on large and small scales","venue":"astro-ph.CO","work_id":"682f861f-d43a-470a-858a-a2fb7f814505","year":2014},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1409.2769","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8982e07e9bf5cda146705623f0d252251be242ea82b280f849d785188e84bf22","observation_id":"9c039ace-a55b-4074-bcb4-0f8cc330142a","resolution":{"observed_at":"2026-07-07T23:34:19.164851Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.06647","last_updated":"2021-01-05T17:06:36Z","snapshot_observed_at":"2026-08-04T05:11:37.535844Z","submitted_at":"2020-06-11T17:42:09Z","title":"Massive black hole binary inspiral and spin evolution in a cosmological framework","version":3},"cited_work":{"arxiv_id":"2006.06647","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.06647","snapshot_observed_at":"2026-07-07T23:34:19.435306Z","title":"Massive black hole binary inspiral and spin evolution in a cosmological framework","venue":"astro-ph.GA","work_id":"43eabc5c-3ad3-4b8a-adff-71d5fb68328c","year":2020},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2006.06647","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8401983a85135f621a9340e8e5f8bcbb01bf53cb25ebe3837113732fa330684d","observation_id":"a93c6274-79ca-43df-a6ed-f365efdb23f7","resolution":{"observed_at":"2026-07-07T23:34:19.437043Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.5375","last_updated":"2012-11-22T21:00:02Z","snapshot_observed_at":"2026-08-17T04:11:03.850527Z","submitted_at":"2012-11-22T21:00:02Z","title":"Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing band","version":1},"cited_work":{"arxiv_id":"1211.5375","doi":"10.1093/mnrasl/slt034","metadata_source":"pith","pith_arxiv_id":"1211.5375","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Sesana, Mon","venue":"astro-ph.CO","work_id":"2a97949d-aed8-480e-b2bd-9e29e05a0a14","year":2012},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1211.5375","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:b81209e55d47e485ce598a1c4770e5699f0ca1d59d114992ee230c12562e4205","observation_id":"645dbb3c-00b4-4153-b2ab-7cd728b1c335","resolution":{"observed_at":"2026-07-07T23:34:19.399845Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:20.749028+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:20.749028+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stv1214","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Veronesi, B","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"f3b894b8-e7b5-4a59-a885-864dabe735f6","year":2015},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:5620f6ccad8361f04bf8faba6951d74a1ee68ca4ae979c46338885f6ffc68462","observation_id":"5b38a93f-db4d-4478-b324-fc2cd737f4fb","resolution":{"observed_at":"2026-07-07T23:34:19.311742Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:21.060746+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:21.060746+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.07376","doi":"10.48550/arxiv.2510.07376","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"L., Kocevski, D","venue":"ArXiv.org","work_id":"cc65e4d5-1370-4d52-afa3-38089f2c721a","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:e2a1d3630a69f7f0c411a284b11000727ab293fab8455578c5bf07a2745b0676","observation_id":"acd6abf9-2b67-43cf-9712-9a55015e9ba0","resolution":{"observed_at":"2026-07-07T23:34:19.626014Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:48.14683+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:48.14683+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.5297","last_updated":"2014-12-16T01:08:27Z","snapshot_observed_at":"2026-08-14T23:29:41.423018Z","submitted_at":"2014-06-20T07:45:50Z","title":"Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays","version":2},"cited_work":{"arxiv_id":"1406.5297","doi":null,"metadata_source":"pith","pith_arxiv_id":"1406.5297","snapshot_observed_at":"2026-07-07T23:34:19.350396Z","title":"Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays","venue":"astro-ph.CO","work_id":"159f6a5e-71e2-4895-8f8c-3bba67507676","year":2014},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1406.5297","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8e2a009512c8b9ab1296b69ef7f1ef4152ccc1fd69c7f45724071a2a12f3634b","observation_id":"24f0780c-3c33-4d90-90ab-2f14fb6a2010","resolution":{"observed_at":"2026-07-07T23:34:19.351808Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.04902","last_updated":"2020-09-15T11:06:25Z","snapshot_observed_at":"2026-08-13T22:45:36.758558Z","submitted_at":"2020-05-11T07:55:14Z","title":"Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations","version":3},"cited_work":{"arxiv_id":"2005.04902","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.04902","snapshot_observed_at":"2026-07-07T23:34:19.479545Z","title":"Volonteri et al","venue":"astro-ph.GA","work_id":"8895f4c4-8cc8-4dbc-8ee2-546e9f93e489","year":2020},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2005.04902","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:18cea35b85f9b7001f6990d29605522edff9c44f81d0dd685da94f3d3a74f010","observation_id":"1718676c-ef3f-4d2f-91b0-611c4e8e3325","resolution":{"observed_at":"2026-07-07T23:34:19.481078Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.18395","last_updated":"2024-02-05T20:16:43Z","snapshot_observed_at":"2026-08-16T14:48:11.548221Z","submitted_at":"2023-10-27T18:00:01Z","title":"Undermassive Host Galaxies of Five z~6 Luminous Quasars Detected with JWST","version":3},"cited_work":{"arxiv_id":"2310.18395","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.18395","snapshot_observed_at":"2026-07-07T23:34:19.248690Z","title":"Undermassive Host Galaxies of Five z~6 Luminous Quasars Detected with JWST","venue":"astro-ph.GA","work_id":"f9fdab42-8f60-4fbb-ab74-ffceb60133ff","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2310.18395","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:71932b503d486585c1506f1b0a1692caf066fe281181506370ba963e1a6dbc34","observation_id":"be424546-796c-4c8d-b6d2-428ea0928b6b","resolution":{"observed_at":"2026-07-07T23:34:19.255164Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04614","last_updated":"2024-03-28T23:40:11Z","snapshot_observed_at":"2026-08-21T01:01:41.765416Z","submitted_at":"2023-09-08T22:08:51Z","title":"EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\\gtrsim6$","version":2},"cited_work":{"arxiv_id":"2309.04614","doi":"10.48550/arxiv.2309.04614","metadata_source":"pith","pith_arxiv_id":"2309.04614","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Yue, A.-C","venue":"astro-ph.GA","work_id":"4adea16f-19e4-4a48-b754-469af04f9d1e","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2309.04614","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:cea07b924cad710da4c163d1bfa6eeedf814f8dd82a90b683ad3f4c0815ed9f1","observation_id":"05f709f4-a52f-41c8-9538-fcb1d71b32a8","resolution":{"observed_at":"2026-07-07T23:34:19.183842Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/s41586-023-06345-5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"D., et al","venue":"Nature","work_id":"8ce56182-51c6-4968-8f74-7db7b8a63bfc","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:2050cb0da0a9ed41481e85bd7b16787cf9019ac3e14003fb0fbdd7c4634c7abf","observation_id":"cae58154-a6dc-4d28-8e05-4b58476d6e1e","resolution":{"observed_at":"2026-07-07T23:34:19.307585Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:08:41.552681+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:08:41.552681+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202452650","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"Astronomy and Astrophysics","work_id":"ad27ba00-7849-463a-91cd-bb315a0cac06","year":2025},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:2830c1078351cbe6d8ad752c673147b826ed26c7c13732f5e8c14a529091763a","observation_id":"07b9c0b3-1732-4489-8be0-e22285c9b4fd","resolution":{"observed_at":"2026-07-07T23:34:19.511770Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T15:20:41.66008+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T15:20:41.66008+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stag086","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"b517c453-9d82-425e-a89c-1369de475992","year":2026},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:4f3a46c2c2ff75e59e56756217b95ad4e3585a8fda50016b51f103e417449c84","observation_id":"15b2e260-a046-4c35-8fd9-d731016b939e","resolution":{"observed_at":"2026-07-07T23:34:19.379458Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:22.916281+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:22.916281+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.12492","last_updated":"2024-01-17T18:51:16Z","snapshot_observed_at":"2026-08-17T16:18:02.459381Z","submitted_at":"2023-05-21T16:01:03Z","title":"A small and vigorous black hole in the early Universe","version":2},"cited_work":{"arxiv_id":"2305.12492","doi":"10.48550/arxiv.2305.12492","metadata_source":"pith","pith_arxiv_id":"2305.12492","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"A small and vigorous black hole in the arly Unverse, arxiv:2305.12492v2, https://doi.org/10.48550/arXiv.2305.12492","venue":"astro-ph.GA","work_id":"90dde65e-d265-43ce-b61e-be8846a2b25d","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2305.12492","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8012addc0fd9d4508e5cf3f875d49e9c60e31185e3f5e4b63577b66eeff34831","observation_id":"7f8ad07d-7eb4-4f05-acb8-f1f2c7b3d919","resolution":{"observed_at":"2026-07-07T23:34:19.396642Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2008","doi":"10.1111/j.1365-2966.2008.12689.x","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"T., Ogilvie G","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"a585747b-4fbc-4555-a22d-a4a769e4179d","year":2008},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:1eee40e51cf5a5e40e5be71cd8a8f07047cc2266ce68ba14f1379dd5dc40b7cc","observation_id":"94628373-b457-4f98-aea4-26a84be24fc0","resolution":{"observed_at":"2026-07-07T23:34:19.433849Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1511.08502","last_updated":"2015-12-09T09:33:42Z","snapshot_observed_at":"2026-08-18T15:15:42.744923Z","submitted_at":"2015-11-26T21:00:06Z","title":"How Big Can a Black Hole Grow?","version":2},"cited_work":{"arxiv_id":"1511.08502","doi":null,"metadata_source":"pith","pith_arxiv_id":"1511.08502","snapshot_observed_at":"2026-07-07T23:34:19.401023Z","title":"How Big Can a Black Hole Grow?","venue":"astro-ph.GA","work_id":"72d15746-7f18-4263-bee7-520e109bc426","year":2015},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1511.08502","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:7d6e0cfd94c5539888cc025689d1762a52c330ba5b961ad060a4fd6aad30c2a2","observation_id":"7a93042c-482d-40c3-a350-061e2bff2534","resolution":{"observed_at":"2026-07-07T23:34:19.402299Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08071","last_updated":"2023-01-19T13:36:20Z","snapshot_observed_at":"2026-08-21T12:01:31.021515Z","submitted_at":"2023-01-19T13:36:20Z","title":"The GRAVITY+ Project: Towards All-sky, Faint-Science, High-Contrast Near-Infrared Interferometry at the VLTI","version":1},"cited_work":{"arxiv_id":"2301.08071","doi":null,"metadata_source":"pith","pith_arxiv_id":"2301.08071","snapshot_observed_at":"2026-07-07T23:34:19.130624Z","title":"The GRAVITY+ Project: Towards All-sky, Faint-Science, High-Contrast Near-Infrared Interferometry at the VLTI","venue":"astro-ph.IM","work_id":"e5558276-e9e7-4592-8b7e-5a6f9c9ce32d","year":2023},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2301.08071","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:21a65c70bc8ef71037de2b99dfe0f662371f88bcd7e2348a43352c56ab87d2ba","observation_id":"c83db13d-838e-4e19-bce5-648a90dca880","resolution":{"observed_at":"2026-07-07T23:34:19.137302Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/s41586-024-07053-4","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"Nature","work_id":"32a4c2cf-5d03-487c-b536-8b8633aa6f18","year":2024},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:8ff29fec710dd255d4d2078b87d3105042d8450b3db7682657dd9db4c1da934b","observation_id":"4596f81c-f081-4f92-b966-bb490e24de9d","resolution":{"observed_at":"2026-07-07T23:34:19.321961Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:46.512178+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:46.512178+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.12237","last_updated":"2022-07-25T14:39:25Z","snapshot_observed_at":"2026-08-16T16:43:33.013455Z","submitted_at":"2022-07-25T14:39:25Z","title":"Evaluating the prevalence of spurious correlations in pulsar timing array datasets","version":1},"cited_work":{"arxiv_id":"2207.12237","doi":null,"metadata_source":"pith","pith_arxiv_id":"2207.12237","snapshot_observed_at":"2026-07-07T23:34:19.353021Z","title":"Evaluating the prevalence of spurious correlations in pulsar timing array datasets","venue":"astro-ph.HE","work_id":"94835c9c-1cc8-4ddf-b080-88ccf01c51ed","year":2022},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2207.12237","citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:0b297d7219b92f80afb1cc9af80164502af4293845051b6d9273fb5a6ac47a71","observation_id":"30c53dfe-6bd8-4570-93e2-aaefb2731a59","resolution":{"observed_at":"2026-07-07T23:34:19.354368Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/s41467-025-65450-3","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Chen, Siyuan and Keane, Evan F","venue":"Nature Communications","work_id":"14f8e132-1b27-4265-a262-1ae9c6d3b121","year":null},"citing_paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-07-07T23:29:47.022382Z"},"links":{"citing_paper":"/paper/2607.05208"},"observation_digest":"sha256:5d04a42bfd33abe0b7f15f0b6bbb9152038e513240744556fbd8b7f3f9f9ad40","observation_id":"6c028f5f-2a2b-4319-b925-85f1fa69b1f7","resolution":{"observed_at":"2026-07-07T23:34:19.557173Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-07-11T19:19:25.091943+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T19:19:25.091943+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2607.05208","last_updated":"2026-07-06T15:26:08Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-02T15:38:18.964748Z","submitted_at":"2026-07-06T15:26:08Z","title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":32,"parse_uncertain":0,"unresolved":0,"verified_exact":53,"verified_fuzzy":15},"total_outbound_references":155},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 100 of 155 outbound references and 1 inbound Pith citation observation for arXiv:2607.05208."}