{"as_of":"2026-08-22T19:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:776e491b8d5815ad01adbbd671f5ac8f25b3926b1d45068e5d27cadcca448852","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T04:25:34.993579Z","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":"2026-05-16T11:37:48.807683Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2210.01817","last_updated":"2023-05-24T13:50:42Z","snapshot_observed_at":"2026-08-19T15:23:40.989442Z","submitted_at":"2022-10-04T18:00:04Z","title":"Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.01817","snapshot_observed_at":"2026-08-16T04:25:34.993579Z","title":"Meshveliani, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.01495","last_updated":"2025-07-22T06:50:33Z","snapshot_observed_at":"2026-08-19T10:10:28.280676Z","submitted_at":"2025-05-02T18:00:00Z","title":"Evolution of a black hole cluster in full general relativity","version":2},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-08-16T04:25:34.993579Z"},"links":{"cited_paper":"/paper/2210.01817","citing_paper":"/paper/2505.01495"},"observation_digest":"sha256:1519942d0a8946f07eea8b549f9e3e363152c0e5a1e947c0af5469092fb9494f","observation_id":"e77304d7-d61d-4948-ae64-98a48c69f7bb","resolution":{"observed_at":"2026-08-16T04:25:34.993579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01817","last_updated":"2023-05-24T13:50:42Z","snapshot_observed_at":"2026-08-19T15:23:40.989442Z","submitted_at":"2022-10-04T18:00:04Z","title":"Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.01817","snapshot_observed_at":"2026-08-15T19:14:09.889486Z","title":"Gravothermal collapse of self-interacting dark matter halos as the origin of intermediate mass black holes in Milky Way satellites,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.17641","last_updated":"2025-06-21T08:47:00Z","snapshot_observed_at":"2026-08-21T14:35:25.960164Z","submitted_at":"2025-06-21T08:47:00Z","title":"Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T19:14:09.889486Z"},"links":{"cited_paper":"/paper/2210.01817","citing_paper":"/paper/2506.17641"},"observation_digest":"sha256:551837f7597d7c285505081d63de1562ad5321f4054a370060763e6f8340315a","observation_id":"6b1cebe4-89ef-45e4-a67f-af18a5f241c8","resolution":{"observed_at":"2026-08-15T19:14:09.889486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01817","last_updated":"2023-05-24T13:50:42Z","snapshot_observed_at":"2026-08-19T15:23:40.989442Z","submitted_at":"2022-10-04T18:00:04Z","title":"Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites","version":2},"cited_work":{"arxiv_id":"2210.01817","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.01817","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Meshveliani, J","venue":null,"work_id":"783de212-f42f-4c14-af26-767eb4eedc2b","year":2023},"citing_paper":{"arxiv_id":"2601.17117","last_updated":"2026-04-25T12:29:32Z","snapshot_observed_at":"2026-08-16T07:15:03.867617Z","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":134,"source":"pdf_text","source_observed_at":"2026-05-16T11:34:12.521105Z"},"links":{"cited_paper":"/paper/2210.01817","citing_paper":"/paper/2601.17117"},"observation_digest":"sha256:439628b9135dd7819da9a36e37062eabe1eff6f116185014ec93497770aaad89","observation_id":"e07bf046-6bb3-4ea7-bd25-ae8d3e224bde","resolution":{"observed_at":"2026-05-16T11:37:48.809115Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01817","last_updated":"2023-05-24T13:50:42Z","snapshot_observed_at":"2026-08-19T15:23:40.989442Z","submitted_at":"2022-10-04T18:00:04Z","title":"Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.01817","snapshot_observed_at":"2026-07-31T04:54:06.814642Z","title":"Meshveliani, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28517","last_updated":"2026-07-30T16:55:29Z","snapshot_observed_at":"2026-08-15T23:24:16.872609Z","submitted_at":"2026-07-30T16:55:29Z","title":"Dynamical flattening of halo density cusps by Q-ball dark matter","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-31T04:54:06.814642Z"},"links":{"cited_paper":"/paper/2210.01817","citing_paper":"/paper/2607.28517"},"observation_digest":"sha256:919d1b8fdd001b2e095a9707c8607a6df05e3b67aabf864b02a3cab838ecb2af","observation_id":"b46b83cb-1889-495d-bde3-977f31770447","resolution":{"observed_at":"2026-07-31T04:54:06.814642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2210.01817/citation-record","integrity":"/paper/2210.01817/integrity","json":"/paper/2210.01817/citation-record.json","paper":"/paper/2210.01817"},"outbound":[],"paper":{"arxiv_id":"2210.01817","last_updated":"2023-05-24T13:50:42Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-19T15:23:40.989442Z","submitted_at":"2022-10-04T18:00:04Z","title":"Gravothermal collapse of Self-Interacting Dark Matter halos as the Origin of Intermediate Mass Black Holes in Milky Way satellites"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2210.01817."}