{"as_of":"2026-08-12T09:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d1efe1535cf0a8cc9024cda9d421e2b24b1c91d7e5f09cd8d6c48d52aad70285","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T04:37:09.379899Z","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":"2026-08-10T19:48:57.681024Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2310.15214","last_updated":"2024-01-12T17:26:17Z","snapshot_observed_at":"2026-08-12T09:17:19.962256Z","submitted_at":"2023-10-23T18:00:00Z","title":"Can prompt cusps of WIMP dark matter be detected as individual gamma-ray sources?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.15214","snapshot_observed_at":"2026-08-11T04:37:09.379899Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.18736","last_updated":"2024-12-25T01:49:18Z","snapshot_observed_at":"2026-08-11T05:32:42.947994Z","submitted_at":"2024-12-25T01:49:18Z","title":"Revisiting the search for dark matter subhalos using the Fermi-LAT 4FGL-DR4 catalog","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T04:37:09.379899Z"},"links":{"cited_paper":"/paper/2310.15214","citing_paper":"/paper/2412.18736"},"observation_digest":"sha256:ea48bdfc05f75d50c917bb367c01a4337b6d6058270d1264c27cc0731191befa","observation_id":"145cfdeb-23b5-420e-ad6b-0dc178893cc6","resolution":{"observed_at":"2026-08-11T04:37:09.379899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.15214","last_updated":"2024-01-12T17:26:17Z","snapshot_observed_at":"2026-08-12T09:17:19.962256Z","submitted_at":"2023-10-23T18:00:00Z","title":"Can prompt cusps of WIMP dark matter be detected as individual gamma-ray sources?","version":2},"cited_work":{"arxiv_id":"2310.15214","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.15214","snapshot_observed_at":"2026-08-10T19:48:57.681024Z","title":"Can prompt cusps of WIMP dark matter be detected as individual gamma-ray sources?","venue":"astro-ph.CO","work_id":"a8925f96-f17e-4427-8d1d-85e0860e6e2f","year":2023},"citing_paper":{"arxiv_id":"2501.09789","last_updated":"2025-01-16T19:00:01Z","snapshot_observed_at":"2026-08-10T23:26:49.092566Z","submitted_at":"2025-01-16T19:00:01Z","title":"Detecting dark matter sub-halos in the Galactic plane with the Cherenkov Telescope Array Observatory","version":1},"reference_index":137,"source":"pdf_text","source_observed_at":"2026-08-10T19:48:57.641662Z"},"links":{"cited_paper":"/paper/2310.15214","citing_paper":"/paper/2501.09789"},"observation_digest":"sha256:e2cf4649d3f93b7a29178cc0d8a844bd0fe12aef1f024e4713167742c8c7a2f4","observation_id":"def73607-175c-401f-aeb5-51fdce553289","resolution":{"observed_at":"2026-08-10T19:48:57.687258Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2310.15214/citation-record","integrity":"/paper/2310.15214/integrity","json":"/paper/2310.15214/citation-record.json","paper":"/paper/2310.15214"},"outbound":[],"paper":{"arxiv_id":"2310.15214","last_updated":"2024-01-12T17:26:17Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-12T09:17:19.962256Z","submitted_at":"2023-10-23T18:00:00Z","title":"Can prompt cusps of WIMP dark matter be detected as individual gamma-ray sources?"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.15214."}