{"as_of":"2026-08-06T16:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:941d17f980ff76c6225eb8517cc2b85bcfa012eeea2432ad3eb4354b261ace44","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T00:06:27.198555Z","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":"2026-06-29T03:53:04.896849Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-07-14T21:55:54.028883Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2603.13030","last_updated":"2026-07-01T15:32:03Z","snapshot_observed_at":"2026-07-14T21:55:53.060873Z","submitted_at":"2026-03-13T14:42:17Z","title":"Floquet Dissipative Phase Transitions","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-14T21:55:54.028883Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2603.13030"},"observation_digest":"sha256:652516c2c6282655ae628cc2312454854c7d6f809b53a3a43a2da918a929f453","observation_id":"74026f32-1c5b-44aa-a255-41b1dd24fc91","resolution":{"observed_at":"2026-07-14T21:55:54.028883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":"1603.02702","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-06-29T03:53:04.896849Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","venue":"astro-ph.CO","work_id":"79513547-8da6-472c-b1cf-55ad281a9771","year":2016},"citing_paper":{"arxiv_id":"2605.16483","last_updated":"2026-05-15T18:00:00Z","snapshot_observed_at":"2026-07-06T23:27:38.955917Z","submitted_at":"2026-05-15T18:00:00Z","title":"The limits of feedback from active galactic nuclei","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-20T16:13:17.171905Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2605.16483"},"observation_digest":"sha256:979f2356c7b6b42225a4e679b11f60a3322c4bd3a5987b4587628942619d9db2","observation_id":"c2302f96-b750-4ea9-86fc-e956b155aa11","resolution":{"observed_at":"2026-05-20T16:13:34.343736Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":"1603.02702","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-06-29T03:53:04.896849Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","venue":"astro-ph.CO","work_id":"79513547-8da6-472c-b1cf-55ad281a9771","year":2016},"citing_paper":{"arxiv_id":"2605.16501","last_updated":"2026-05-15T18:00:35Z","snapshot_observed_at":"2026-08-02T17:09:21.567607Z","submitted_at":"2026-05-15T18:00:35Z","title":"Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2605.16501"},"observation_digest":"sha256:b26257d3990be7dfe6193fe1e9ea78bc1122c71d17a7f18fbafae1c277c75dd4","observation_id":"e704c636-4b39-44c9-820e-28b9e05fd0fe","resolution":{"observed_at":"2026-05-20T16:03:33.462244Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":"1603.02702","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-06-29T03:53:04.896849Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","venue":"astro-ph.CO","work_id":"79513547-8da6-472c-b1cf-55ad281a9771","year":2016},"citing_paper":{"arxiv_id":"2606.10679","last_updated":"2026-06-09T10:32:19Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:32:19Z","title":"Balancing bias, baryons, and scale cuts in LSST 3x2pt analysis","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2606.10679"},"observation_digest":"sha256:f97a18b713e83d6e0bbfb22ff08331c370c534dd06cab49497f08bb95ffaac63","observation_id":"9ae6b4e5-66f1-4482-950b-b73ea2d27076","resolution":{"observed_at":"2026-06-27T14:00:59.901033Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":"1603.02702","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-06-29T03:53:04.896849Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","venue":"astro-ph.CO","work_id":"79513547-8da6-472c-b1cf-55ad281a9771","year":2016},"citing_paper":{"arxiv_id":"2606.19463","last_updated":"2026-06-17T18:01:34Z","snapshot_observed_at":"2026-08-05T03:47:10.189563Z","submitted_at":"2026-06-17T18:01:34Z","title":"On the later evolution of observationally selected protocluster candidates at $z\\,{\\gtrsim}\\,5$","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2606.19463"},"observation_digest":"sha256:4137870de5cb630d31f0e899de8f0061b71da11ce89e740934e779841e7bb8b7","observation_id":"db303ea6-538a-4531-a87c-2505400e0a20","resolution":{"observed_at":"2026-06-26T20:09:57.730125Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":"1603.02702","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-06-29T03:53:04.896849Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","venue":"astro-ph.CO","work_id":"79513547-8da6-472c-b1cf-55ad281a9771","year":2016},"citing_paper":{"arxiv_id":"2606.26445","last_updated":"2026-06-24T23:14:13Z","snapshot_observed_at":"2026-08-02T06:35:29.874763Z","submitted_at":"2026-06-24T23:14:13Z","title":"Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium","version":1},"reference_index":160,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2606.26445"},"observation_digest":"sha256:358d894e2409e45911cb54059ca959e1ad10df93b567e36b0e8eca0f11369f39","observation_id":"e73fc2de-32f3-41ce-a46d-b29d3d1b59f0","resolution":{"observed_at":"2026-06-27T01:00:20.760274Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":"1603.02702","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-06-29T03:53:04.896849Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","venue":"astro-ph.CO","work_id":"79513547-8da6-472c-b1cf-55ad281a9771","year":2016},"citing_paper":{"arxiv_id":"2606.27714","last_updated":"2026-06-26T04:44:56Z","snapshot_observed_at":"2026-08-01T17:32:21.309572Z","submitted_at":"2026-06-26T04:44:56Z","title":"Fast Radio Bursts as Cosmological Probes","version":1},"reference_index":297,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2606.27714"},"observation_digest":"sha256:6ceb787374b7c0bbd96bb7396ad18678fd3ffccc81664c8aa8a8b84678b83e6e","observation_id":"f85c7d77-22ba-4542-bbd6-66af2f51513d","resolution":{"observed_at":"2026-06-29T03:53:04.898347Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":"1603.02702","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-06-29T03:53:04.896849Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","venue":"astro-ph.CO","work_id":"79513547-8da6-472c-b1cf-55ad281a9771","year":2016},"citing_paper":{"arxiv_id":"2606.28099","last_updated":"2026-07-21T07:58:37Z","snapshot_observed_at":"2026-08-04T20:18:41.228751Z","submitted_at":"2026-06-26T13:56:50Z","title":"Thermal Sunyaev-Zel'dovich cross-correlations with unWISE galaxies: disentangling radio contamination, dust properties, and electron pressure","version":1},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2606.28099"},"observation_digest":"sha256:25c4d8d6809b459c5ee2bf47071bc685ee84d3c908a29bf66a2c92bb2d3c0182","observation_id":"0ab97600-cec2-4746-bd7f-63d831367a8c","resolution":{"observed_at":"2026-06-29T03:03:03.782242Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-07-12T07:37:06.339592Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.02704","last_updated":"2026-07-02T18:47:11Z","snapshot_observed_at":"2026-07-29T15:42:46.914291Z","submitted_at":"2026-07-02T18:47:11Z","title":"S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known clusters and groups in DR5 and a pilot study of Abell 4038","version":1},"reference_index":144,"source":"arxiv_source","source_observed_at":"2026-07-12T07:37:06.339592Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2607.02704"},"observation_digest":"sha256:0670e3176a0faf51b969bc726d68e8a3d4e753554d3df71f47d1b359575000f7","observation_id":"6e6381ff-acb2-4159-9cb9-c8fad844b9de","resolution":{"observed_at":"2026-07-12T07:37:06.339592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-08-02T06:10:13.089540Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.13151","last_updated":"2026-07-14T18:01:38Z","snapshot_observed_at":"2026-08-06T10:10:01.626872Z","submitted_at":"2026-07-14T18:01:38Z","title":"Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-02T06:10:13.089540Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2607.13151"},"observation_digest":"sha256:9b0b40c1ec444b5068ecfc1207b80b05e7b7ac58cec92ee98c5c05c1e9c97b08","observation_id":"c432c1fd-3676-4159-b70f-2ba4609694cf","resolution":{"observed_at":"2026-08-02T06:10:13.089540Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-08-01T08:26:28.118434Z","title":"doi:10.1093/mnras/stw2792 , archivePrefix =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.21140","last_updated":"2026-07-23T10:17:57Z","snapshot_observed_at":"2026-08-06T14:23:55.188294Z","submitted_at":"2026-07-23T10:17:57Z","title":"What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba","version":1},"reference_index":261,"source":"arxiv_source","source_observed_at":"2026-08-01T08:26:28.118434Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2607.21140"},"observation_digest":"sha256:e6cc12507a63b435fa604bd32a4046ff148938ba7f3754ae534cd96987424f24","observation_id":"787d9eb5-899c-44fa-bc09-311726da9122","resolution":{"observed_at":"2026-08-01T08:26:28.118434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-07-31T23:49:27.443824Z","title":"and Schaye, Joop and Bird, Simeon and Le Brun, Amandine M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.23339","last_updated":"2026-07-25T19:35:29Z","snapshot_observed_at":"2026-08-02T05:19:25.373749Z","submitted_at":"2026-07-25T19:35:29Z","title":"Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects","version":1},"reference_index":113,"source":"arxiv_source","source_observed_at":"2026-07-31T23:49:27.443824Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2607.23339"},"observation_digest":"sha256:21fb17964c396a9ea3c8e9da51f51db9295c8dc334bc96d99ed235c81b31e00d","observation_id":"b6b0f26a-4313-40d8-8f78-f63ce944c532","resolution":{"observed_at":"2026-07-31T23:49:27.443824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02702","snapshot_observed_at":"2026-08-06T00:06:27.198555Z","title":"doi:10.1093/mnras/stw2792 , archiveprefix =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.03186","last_updated":"2026-08-04T06:26:06Z","snapshot_observed_at":"2026-08-06T15:33:16.815636Z","submitted_at":"2026-08-04T06:26:06Z","title":"The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\\rm X}$--$T$ relation of early-type galaxies","version":1},"reference_index":160,"source":"arxiv_source","source_observed_at":"2026-08-06T00:06:27.198555Z"},"links":{"cited_paper":"/paper/1603.02702","citing_paper":"/paper/2608.03186"},"observation_digest":"sha256:c30a58ef1ecab6ac2b4e741564d097f40bda7f64f1fda2146b049114719a6f7c","observation_id":"966afba6-0647-4295-a32b-1ac25e0af737","resolution":{"observed_at":"2026-08-06T00:06:27.198555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1603.02702/citation-record","integrity":"/paper/1603.02702/integrity","json":"/paper/1603.02702/citation-record.json","paper":"/paper/1603.02702"},"outbound":[],"paper":{"arxiv_id":"1603.02702","last_updated":"2016-11-07T12:16:40Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:09:29Z","title":"The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:1603.02702."}