{"as_of":"2026-08-07T19:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:206491318a02246a62dcbbbc053caec9f8a53c97d47084a2feed1212c2c64342","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T19:01:56.496354Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T14:58:32.849380Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-08-06T19:01:56.496354Z","title":"Seeding 9 Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.07171","last_updated":"2025-07-23T03:00:43Z","snapshot_observed_at":"2026-08-06T23:19:55.408091Z","submitted_at":"2025-07-09T18:00:01Z","title":"Little Red Dots from Small-Scale Primordial Black Hole Clustering","version":2},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-08-06T19:01:56.496354Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2507.07171"},"observation_digest":"sha256:563acc98876ef8faf19843cb901f1dfd7162da5b9e65cdab3f76f71fb4a6e87c","observation_id":"3388effc-d25f-4565-a238-66497ab0e826","resolution":{"observed_at":"2026-08-06T19:01:56.496354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":"2010.15132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-03T14:58:32.849380Z","title":"Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons","venue":null,"work_id":"1ebe8695-afc5-4bc5-842f-14260f1bd426","year":2021},"citing_paper":{"arxiv_id":"2509.25325","last_updated":"2026-04-14T18:06:24Z","snapshot_observed_at":"2026-07-06T22:31:10.099674Z","submitted_at":"2025-09-29T18:00:03Z","title":"Direct Collapse Black Hole Candidates from Decaying Dark Matter","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-18T12:06:32.865011Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2509.25325"},"observation_digest":"sha256:c9b7fbd7738ddfc05f9e9c1ecebe171ee69c65786c8f69727747f49b81f7a560","observation_id":"8767e8f7-9a60-4f4b-94bd-c1ea9054f008","resolution":{"observed_at":"2026-05-18T12:11:22.531976Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":"2010.15132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-03T14:58:32.849380Z","title":"Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons","venue":null,"work_id":"1ebe8695-afc5-4bc5-842f-14260f1bd426","year":2021},"citing_paper":{"arxiv_id":"2601.17117","last_updated":"2026-04-25T12:29:32Z","snapshot_observed_at":"2026-07-06T22:42:52.947644Z","submitted_at":"2026-01-23T19:00:02Z","title":"Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-05-16T11:34:12.521105Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2601.17117"},"observation_digest":"sha256:b2044e5fb02c0e3bdd7f9e7574f2107a8b47dca04b59af23db527702586a7bd0","observation_id":"a9c6edc6-625a-404a-a3f5-c6ba0e3b191f","resolution":{"observed_at":"2026-05-16T11:37:49.049567Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":"2010.15132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-03T14:58:32.849380Z","title":"Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons","venue":null,"work_id":"1ebe8695-afc5-4bc5-842f-14260f1bd426","year":2021},"citing_paper":{"arxiv_id":"2604.01684","last_updated":"2026-06-29T23:15:37Z","snapshot_observed_at":"2026-08-03T00:41:35.054539Z","submitted_at":"2026-04-02T06:39:39Z","title":"Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-05-13T21:21:21.468999Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2604.01684"},"observation_digest":"sha256:515c07fbdfd46699904f48ff4863effae4e4bb6f11b6342ed91bddb1a73d6f5a","observation_id":"d0b428e4-6ccd-4cc1-bd6a-6a432e8be00d","resolution":{"observed_at":"2026-05-13T21:23:17.508810Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":"2010.15132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-03T14:58:32.849380Z","title":"Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons","venue":null,"work_id":"1ebe8695-afc5-4bc5-842f-14260f1bd426","year":2021},"citing_paper":{"arxiv_id":"2604.08647","last_updated":"2026-04-09T17:59:18Z","snapshot_observed_at":"2026-08-01T03:59:27.972333Z","submitted_at":"2026-04-09T17:59:18Z","title":"Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-10T16:51:41.665607Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2604.08647"},"observation_digest":"sha256:f53b3b9cde76b151509144edf9d72c811e01c54cd3376844ab21d14cbb813ae5","observation_id":"3c7d72c8-56c1-4d02-b340-d89693296d5c","resolution":{"observed_at":"2026-05-11T08:00:58.916418Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":"2010.15132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-03T14:58:32.849380Z","title":"Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons","venue":null,"work_id":"1ebe8695-afc5-4bc5-842f-14260f1bd426","year":2021},"citing_paper":{"arxiv_id":"2605.31335","last_updated":"2026-05-29T14:16:44Z","snapshot_observed_at":"2026-08-02T13:53:50.544392Z","submitted_at":"2026-05-29T14:16:44Z","title":"Gravothermal Collapse: Robust Against Baryonic Feedback","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-06-28T20:58:05.796638Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2605.31335"},"observation_digest":"sha256:e7fa1281dc6b9675a83ba4dc6d1725b444c0ebd347e3abba46652546409e7b2f","observation_id":"fd202ee8-2d86-443a-ba6b-3404f178261c","resolution":{"observed_at":"2026-07-01T20:36:11.612335Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":"2010.15132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-03T14:58:32.849380Z","title":"Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons","venue":null,"work_id":"1ebe8695-afc5-4bc5-842f-14260f1bd426","year":2021},"citing_paper":{"arxiv_id":"2606.12909","last_updated":"2026-06-11T05:08:09Z","snapshot_observed_at":"2026-07-06T23:51:45.306189Z","submitted_at":"2026-06-11T05:08:09Z","title":"SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$\\mathcal{V}$","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-27T06:50:27.397229Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2606.12909"},"observation_digest":"sha256:794119406da4cd4dfd7e0964ff2e748691643691617822e7d5d892dc3467ac8b","observation_id":"6dcfd9e3-592c-412f-9a56-b77e820a6bd0","resolution":{"observed_at":"2026-07-03T14:58:32.850949Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":"2010.15132","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-03T14:58:32.849380Z","title":"Seeding Supermassive Black Holes with Self-interacting Dark Matter: A Unified Scenario with Baryons","venue":null,"work_id":"1ebe8695-afc5-4bc5-842f-14260f1bd426","year":2021},"citing_paper":{"arxiv_id":"2607.02151","last_updated":"2026-07-02T13:26:31Z","snapshot_observed_at":"2026-08-06T16:24:28.071885Z","submitted_at":"2026-07-02T13:26:31Z","title":"Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-03T06:49:14.051341Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2607.02151"},"observation_digest":"sha256:24d6784f6f974c2863c41702c2472267c8292253a83b8b534aed06f37a4199ec","observation_id":"b048106e-6511-48a7-918a-05701faccce5","resolution":{"observed_at":"2026-07-03T06:57:42.781246Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.15132","snapshot_observed_at":"2026-07-11T06:38:02.275303Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.05504","last_updated":"2026-07-06T18:00:03Z","snapshot_observed_at":"2026-08-05T04:28:37.214862Z","submitted_at":"2026-07-06T18:00:03Z","title":"A Novel Implementation of Self-Interacting Dark Matter in AREPO","version":1},"reference_index":168,"source":"arxiv_source","source_observed_at":"2026-07-11T06:38:02.275303Z"},"links":{"cited_paper":"/paper/2010.15132","citing_paper":"/paper/2607.05504"},"observation_digest":"sha256:7bc20a0b6a40e2994775ef600d406f62ad8517cb53c12c3ef8c08353bf42f651","observation_id":"e38a866f-7b74-4f14-93fd-b5e88915c2a3","resolution":{"observed_at":"2026-07-11T06:38:02.275303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2010.15132/citation-record","integrity":"/paper/2010.15132/integrity","json":"/paper/2010.15132/citation-record.json","paper":"/paper/2010.15132"},"outbound":[],"paper":{"arxiv_id":"2010.15132","last_updated":"2025-04-28T18:40:31Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T10:09:30.922063Z","submitted_at":"2020-10-28T18:00:03Z","title":"Seeding Supermassive Black Holes with Self-Interacting Dark Matter: A Unified Scenario with Baryons"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2010.15132."}