{"as_of":"2026-08-18T03:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f5f7a1995ce5093673cb4c81e4b42bf35c1c55df28e4fc272d32ea620cbc19c1","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T12:22:44.063878Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":40,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2203.12586","doi":"10.1038/s41598-022-19540-7","metadata_source":"pith","pith_arxiv_id":"2203.12586","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Pieroni, A","venue":"astro-ph.CO","work_id":"d401672b-33bb-4fb1-a216-91137f5327d4","year":2022},"citing_paper":{"arxiv_id":"2303.15923","last_updated":"2023-06-17T10:49:26Z","snapshot_observed_at":"2026-08-08T01:52:18.464766Z","submitted_at":"2023-03-28T12:29:33Z","title":"Science with the Einstein Telescope: a comparison of different designs","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-17T21:43:29.760310Z"},"links":{"cited_paper":"/paper/2203.12586","citing_paper":"/paper/2303.15923"},"observation_digest":"sha256:198e02d59a8814c68e2d30db8db283aa473ce131b30cc03e7e469245c5c2aac4","observation_id":"f989af81-a2e1-4660-8c43-d0e636b7cb50","resolution":{"observed_at":"2026-05-17T21:43:29.981008Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.12586","snapshot_observed_at":"2026-08-07T12:22:44.063878Z","title":"Pieroni, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.24695","last_updated":"2025-05-30T15:18:51Z","snapshot_observed_at":"2026-08-14T11:06:36.478622Z","submitted_at":"2025-05-30T15:18:51Z","title":"Likelihoods for Stochastic Gravitational Wave Background Data Analysis","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:44.063878Z"},"links":{"cited_paper":"/paper/2203.12586","citing_paper":"/paper/2505.24695"},"observation_digest":"sha256:3bd010223b0591cde591bfd00f44d82394b3ae83e34cabcdaa35d13c75a01771","observation_id":"edc88fdf-fa8d-4614-9d4c-d680102d2b7f","resolution":{"observed_at":"2026-08-07T12:22:44.063878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.12586","snapshot_observed_at":"2026-08-06T22:29:59.157074Z","title":"Pieroni, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.21530","last_updated":"2026-06-24T11:29:49Z","snapshot_observed_at":"2026-08-13T11:49:17.024024Z","submitted_at":"2025-06-26T17:50:19Z","title":"Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T22:29:59.157074Z"},"links":{"cited_paper":"/paper/2203.12586","citing_paper":"/paper/2506.21530"},"observation_digest":"sha256:81bce5da317e83bfbe9712db1e6f8ae74745eee7ab4f602a012f9e894ba03f9f","observation_id":"ae98e178-f66a-4b84-a52b-053a5664343b","resolution":{"observed_at":"2026-08-06T22:29:59.157074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2203.12586","doi":"10.1038/s41598-022-19540-7","metadata_source":"pith","pith_arxiv_id":"2203.12586","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Pieroni, A","venue":"astro-ph.CO","work_id":"d401672b-33bb-4fb1-a216-91137f5327d4","year":2022},"citing_paper":{"arxiv_id":"2509.04028","last_updated":"2026-05-19T16:22:50Z","snapshot_observed_at":"2026-08-16T05:15:05.633771Z","submitted_at":"2025-09-04T09:04:42Z","title":"Primordial black holes versus their impersonators at gravitational wave observatories","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-21T22:15:03.407886Z"},"links":{"cited_paper":"/paper/2203.12586","citing_paper":"/paper/2509.04028"},"observation_digest":"sha256:97cd1c100fe9e4e07a6f7e61d5902457f25c885d142cd2e8ebf15b2a413bfa43","observation_id":"f5dba79c-364e-4a21-956a-a85e8e076ea3","resolution":{"observed_at":"2026-05-21T22:15:42.229476Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2203.12586","doi":"10.1038/s41598-022-19540-7","metadata_source":"pith","pith_arxiv_id":"2203.12586","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Pieroni, A","venue":"astro-ph.CO","work_id":"d401672b-33bb-4fb1-a216-91137f5327d4","year":2022},"citing_paper":{"arxiv_id":"2604.11871","last_updated":"2026-04-13T18:00:00Z","snapshot_observed_at":"2026-08-14T13:30:23.001709Z","submitted_at":"2026-04-13T18:00:00Z","title":"Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-10T15:27:10.838625Z"},"links":{"cited_paper":"/paper/2203.12586","citing_paper":"/paper/2604.11871"},"observation_digest":"sha256:32417ea2f1d0f1a31f4cc975cb50995823f681088ed3faad6a1a459e8fbad837","observation_id":"c28d4c51-6b78-4a75-8c76-0a37844a5a20","resolution":{"observed_at":"2026-05-11T10:31:03.156155Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2203.12586","doi":"10.1038/s41598-022-19540-7","metadata_source":"pith","pith_arxiv_id":"2203.12586","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Pieroni, A","venue":"astro-ph.CO","work_id":"d401672b-33bb-4fb1-a216-91137f5327d4","year":2022},"citing_paper":{"arxiv_id":"2607.07120","last_updated":"2026-07-08T08:02:30Z","snapshot_observed_at":"2026-08-08T06:28:48.615790Z","submitted_at":"2026-07-08T08:02:30Z","title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","version":1},"reference_index":262,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2203.12586","citing_paper":"/paper/2607.07120"},"observation_digest":"sha256:4c50190d6df2a7ab95a13a2ada3d8d2f5e5257a99a561a630df9ef4de8205a88","observation_id":"93476ede-7458-41c5-a169-4489ee0f5179","resolution":{"observed_at":"2026-07-09T20:06:29.153887Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.12586","snapshot_observed_at":"2026-08-01T09:38:48.453887Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.27311","last_updated":"2026-07-29T18:00:00Z","snapshot_observed_at":"2026-08-14T05:21:21.489405Z","submitted_at":"2026-07-29T18:00:00Z","title":"Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-01T09:38:48.453887Z"},"links":{"cited_paper":"/paper/2203.12586","citing_paper":"/paper/2607.27311"},"observation_digest":"sha256:40fa4e2c03a765d3ed977edab0d303a671147bcc033ea55a4d53e91510b26f0a","observation_id":"1f3305e3-9ebc-4b8b-9cab-8f5d8214edd2","resolution":{"observed_at":"2026-08-01T09:38:48.453887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2203.12586/citation-record","integrity":"/paper/2203.12586/integrity","json":"/paper/2203.12586/citation-record.json","paper":"/paper/2203.12586"},"outbound":[],"paper":{"arxiv_id":"2203.12586","last_updated":"2022-11-17T14:20:06Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T17:12:17.671418Z","submitted_at":"2022-03-23T17:52:11Z","title":"Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2203.12586."}