{"as_of":"2026-08-07T09:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cb459e464c2ff2d085714dc9cb22d8e0c4034394d86eb13985163b006951888e","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-18T17:26:22.291821Z","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":"2026-05-18T17:26:40.205186Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2101.00372","last_updated":"2021-01-02T05:20:28Z","snapshot_observed_at":"2026-08-07T00:28:42.536337Z","submitted_at":"2021-01-02T05:20:28Z","title":"Analysing the radio flux density profile of the M31 galaxy: a possible dark matter interpretation","version":1},"cited_work":{"arxiv_id":"2101.00372","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.00372","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Chan, C.F","venue":null,"work_id":"aa564263-0d79-4829-985c-4c170ff37cdd","year":2021},"citing_paper":{"arxiv_id":"2509.08043","last_updated":"2026-04-28T15:42:07Z","snapshot_observed_at":"2026-08-02T01:57:59.727904Z","submitted_at":"2025-09-09T18:00:01Z","title":"Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-18T17:26:22.291821Z"},"links":{"cited_paper":"/paper/2101.00372","citing_paper":"/paper/2509.08043"},"observation_digest":"sha256:1065816b9ed1bc10e8c3e3b1fadcd4f505f4bc8370ceabbf1567810858a762a1","observation_id":"181bde83-36d2-4d42-9870-041a2588c653","resolution":{"observed_at":"2026-05-18T17:26:40.207255Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2101.00372/citation-record","integrity":"/paper/2101.00372/integrity","json":"/paper/2101.00372/citation-record.json","paper":"/paper/2101.00372"},"outbound":[],"paper":{"arxiv_id":"2101.00372","last_updated":"2021-01-02T05:20:28Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-07T00:28:42.536337Z","submitted_at":"2021-01-02T05:20:28Z","title":"Analysing the radio flux density profile of the M31 galaxy: a possible dark matter interpretation"},"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 1 inbound Pith citation observation for arXiv:2101.00372."}