{"as_of":"2026-08-18T08:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5975f8bcca58b819baef14691abbcaf1b6b0700bfeb6ebddf6fe548f8ccd20b2","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:20:27.112564Z","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":"2026-05-13T21:53:19.698154Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2009.07844","last_updated":"2021-01-29T14:36:57Z","snapshot_observed_at":"2026-08-18T04:50:30.678777Z","submitted_at":"2020-09-16T18:00:00Z","title":"The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.07844","snapshot_observed_at":"2026-08-12T11:06:39.693384Z","title":"Robertson, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.18751","last_updated":"2025-09-09T06:20:17Z","snapshot_observed_at":"2026-08-12T10:53:05.939549Z","submitted_at":"2024-11-27T20:55:04Z","title":"Relaxing Constraints on Dark Matter Annihilation Near the Supermassive Black Hole in M87","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T11:06:39.693384Z"},"links":{"cited_paper":"/paper/2009.07844","citing_paper":"/paper/2411.18751"},"observation_digest":"sha256:44d9bf191f41e5902498235537a1913d51e9cdf012e8bd31f1a75438f77cda3c","observation_id":"988d216f-b3d5-4ffa-9b30-f577b6f79071","resolution":{"observed_at":"2026-08-12T11:06:39.693384Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.07844","last_updated":"2021-01-29T14:36:57Z","snapshot_observed_at":"2026-08-18T04:50:30.678777Z","submitted_at":"2020-09-16T18:00:00Z","title":"The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.07844","snapshot_observed_at":"2026-08-15T21:20:27.112564Z","title":"Robertson, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.10451","last_updated":"2025-05-15T16:08:57Z","snapshot_observed_at":"2026-08-18T04:47:09.490817Z","submitted_at":"2025-05-15T16:08:57Z","title":"Constraints on dark matter self-interaction from velocity distribution function in isolated halos","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T21:20:27.112564Z"},"links":{"cited_paper":"/paper/2009.07844","citing_paper":"/paper/2505.10451"},"observation_digest":"sha256:8820c438898bb504bd82abae816e4e0046e6baf38beb6a5d5482c5609d1b91a6","observation_id":"58f9d830-4e6f-4831-84c4-30f9a51763c4","resolution":{"observed_at":"2026-08-15T21:20:27.112564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.07844","last_updated":"2021-01-29T14:36:57Z","snapshot_observed_at":"2026-08-18T04:50:30.678777Z","submitted_at":"2020-09-16T18:00:00Z","title":"The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.07844","snapshot_observed_at":"2026-08-03T06:13:39.296743Z","title":"Robertson, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2601.23264","last_updated":"2026-06-11T13:48:14Z","snapshot_observed_at":"2026-08-14T05:11:55.106926Z","submitted_at":"2026-01-30T18:33:03Z","title":"MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM","version":3},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-03T06:13:39.296743Z"},"links":{"cited_paper":"/paper/2009.07844","citing_paper":"/paper/2601.23264"},"observation_digest":"sha256:db3b21494768781b1811bb5508ee12c2f273ae299b6e610359a8b8273d035b96","observation_id":"81557521-ecac-4647-ad67-a0bb7adfc7cf","resolution":{"observed_at":"2026-08-03T06:13:39.296743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.07844","last_updated":"2021-01-29T14:36:57Z","snapshot_observed_at":"2026-08-18T04:50:30.678777Z","submitted_at":"2020-09-16T18:00:00Z","title":"The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles","version":2},"cited_work":{"arxiv_id":"2009.07844","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.07844","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Robertson, R","venue":null,"work_id":"e0f929cc-de62-48e9-911b-eac83fb9c31f","year":2021},"citing_paper":{"arxiv_id":"2604.01112","last_updated":"2026-04-15T14:41:48Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-01T16:36:52Z","title":"Cosmological zoom-in perturbation theory as a consistent beyond point-particle approximation framework","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-05-13T21:51:38.091879Z"},"links":{"cited_paper":"/paper/2009.07844","citing_paper":"/paper/2604.01112"},"observation_digest":"sha256:ef30707e1b9e3dcd620aedb21050e2cb8cffe38da9a17185d4a2e7e6aebe8f3d","observation_id":"70798516-7dac-440f-bad5-5eb212f733d8","resolution":{"observed_at":"2026-05-13T21:53:19.699301Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.07844","last_updated":"2021-01-29T14:36:57Z","snapshot_observed_at":"2026-08-18T04:50:30.678777Z","submitted_at":"2020-09-16T18:00:00Z","title":"The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.07844","snapshot_observed_at":"2026-07-11T06:38:02.275303Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.05504","last_updated":"2026-07-06T18:00:03Z","snapshot_observed_at":"2026-08-12T23:54:22.345251Z","submitted_at":"2026-07-06T18:00:03Z","title":"A Novel Implementation of Self-Interacting Dark Matter in AREPO","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-11T06:38:02.275303Z"},"links":{"cited_paper":"/paper/2009.07844","citing_paper":"/paper/2607.05504"},"observation_digest":"sha256:4780059c27a725a0a36aca5a30e93b99c41de7cb55c3c553ceb4d02e589d8f62","observation_id":"ed47637c-b520-4706-ba43-5ff2504ba86c","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/2009.07844/citation-record","integrity":"/paper/2009.07844/integrity","json":"/paper/2009.07844/citation-record.json","paper":"/paper/2009.07844"},"outbound":[],"paper":{"arxiv_id":"2009.07844","last_updated":"2021-01-29T14:36:57Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-18T04:50:30.678777Z","submitted_at":"2020-09-16T18:00:00Z","title":"The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2009.07844."}