{"as_of":"2026-08-09T12:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d341cf6f458c90f61878128a767743be3ffffd5353b881e8ce4d8b0639702f92","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":"2026-08-09T06:31:02.800959+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":"2026-08-07T14:46:34.940251Z","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":"2026-07-04T05:19:35.258533Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2009.08722","last_updated":"2020-09-18T09:54:20Z","snapshot_observed_at":"2026-07-06T09:56:44.318762Z","submitted_at":"2020-09-18T09:54:20Z","title":"Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.08722","snapshot_observed_at":"2026-08-07T14:46:34.940251Z","title":"Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.17947","last_updated":"2025-05-23T14:24:05Z","snapshot_observed_at":"2026-08-08T21:45:31.184340Z","submitted_at":"2025-05-23T14:24:05Z","title":"Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T14:46:34.940251Z"},"links":{"cited_paper":"/paper/2009.08722","citing_paper":"/paper/2505.17947"},"observation_digest":"sha256:3ade04f7e103efe626360bd2164ce648bb31034d05f9b91c2bf09c0db28a68b9","observation_id":"e1fd84aa-5e0c-4b0e-a8a5-7208c218ce4e","resolution":{"observed_at":"2026-08-07T14:46:34.940251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.08722","last_updated":"2020-09-18T09:54:20Z","snapshot_observed_at":"2026-07-06T09:56:44.318762Z","submitted_at":"2020-09-18T09:54:20Z","title":"Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars","version":1},"cited_work":{"arxiv_id":"2009.08722","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2009.08722","snapshot_observed_at":"2026-07-04T05:19:35.258533Z","title":"Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars,","venue":null,"work_id":"3b84ce36-099d-42a1-b213-bd475a1e03d3","year":2020},"citing_paper":{"arxiv_id":"2606.20931","last_updated":"2026-06-18T20:48:17Z","snapshot_observed_at":"2026-08-08T16:54:14.186569Z","submitted_at":"2026-06-18T20:48:17Z","title":"Scattering, Hawking Radiation and Neutrino Energy Deposition in Euler-Heisenberg Black Holes Surrounded by Perfect Fluid Dark Matter","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-26T16:07:02.887025Z"},"links":{"cited_paper":"/paper/2009.08722","citing_paper":"/paper/2606.20931"},"observation_digest":"sha256:0590db1891f71aa8bf80654f5a58d299597a3f69c55096dc8585730c188f42dc","observation_id":"66ed04f1-c2da-4d52-bc3b-91e3ac833cf0","resolution":{"observed_at":"2026-07-04T05:19:35.260531Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2009.08722/citation-record","integrity":"/paper/2009.08722/integrity","json":"/paper/2009.08722/citation-record.json","paper":"/paper/2009.08722"},"outbound":[],"paper":{"arxiv_id":"2009.08722","last_updated":"2020-09-18T09:54:20Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T09:56:44.318762Z","submitted_at":"2020-09-18T09:54:20Z","title":"Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2009.08722."}