{"as_of":"2026-08-13T17:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b91373f6cc143ea478ebee54c0da8aaa7d1b870f0ea3118d86257c26cb2077c8","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T11:39:46.418714Z","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":"2026-05-21T21:40:40.445525Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-08-12T11:39:46.418714Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18052","last_updated":"2025-06-25T14:09:04Z","snapshot_observed_at":"2026-08-13T09:48:18.498201Z","submitted_at":"2024-11-27T04:43:31Z","title":"Heating the dark matter halo with dark radiation from supernovae","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T11:39:46.418714Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2411.18052"},"observation_digest":"sha256:21d1c417424e1574706065f6a24eff596d89125b9217d4e040ae58eb99bc0d69","observation_id":"300f1ffe-2951-4f3f-a457-9ee18e75f5f3","resolution":{"observed_at":"2026-08-12T11:39:46.418714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-08-11T13:29:11.169985Z","title":"From Supernovae to Neu- tron Stars: A Systematic Approach to Axion Produc- tion at Finite Density,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13247","last_updated":"2024-12-17T19:00:00Z","snapshot_observed_at":"2026-08-11T13:16:57.714184Z","submitted_at":"2024-12-17T19:00:00Z","title":"Time-delayed gamma-ray signatures of heavy axions from core-collapse supernovae","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T13:29:11.169985Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2412.13247"},"observation_digest":"sha256:67ae766a7c5ea9a2ffe45632e3610971db90bacabdcfa7268a4e9502c6660717","observation_id":"13990f05-48e5-4497-b8cd-39374f849668","resolution":{"observed_at":"2026-08-11T13:29:11.169985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-08-10T20:46:16.347486Z","title":"Springmann, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.07725","last_updated":"2025-05-06T07:41:32Z","snapshot_observed_at":"2026-08-12T03:50:52.414956Z","submitted_at":"2025-01-13T22:24:05Z","title":"In-flight positron annihilation as a probe of feebly interacting particles","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-10T20:46:16.347486Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2501.07725"},"observation_digest":"sha256:a72e486d9dd523349bc2dc3020dc717773b7a66eb48d7fa2a0f9026342bbf7f8","observation_id":"e575a19f-a9db-4b29-abf6-de73eabd8b24","resolution":{"observed_at":"2026-08-10T20:46:16.347486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-08-07T12:20:22.491807Z","title":"Springmann, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.00115","last_updated":"2025-05-30T18:00:01Z","snapshot_observed_at":"2026-08-13T07:53:48.470792Z","submitted_at":"2025-05-30T18:00:01Z","title":"Dark Matter Haloscope with a Disordered Dielectric Absorber","version":1},"reference_index":166,"source":"pdf_text","source_observed_at":"2026-08-07T12:20:22.491807Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2506.00115"},"observation_digest":"sha256:4882ead72f470fd5e23462f977fe6699373fb526ef05de4975c5841bef5badfe","observation_id":"b694778f-52da-4197-8174-3946d8c50b5e","resolution":{"observed_at":"2026-08-07T12:20:22.491807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":"2410.10945","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Springmann, M","venue":null,"work_id":"50fc2ff7-fb5c-47d7-a35c-8ec29fabe772","year":2025},"citing_paper":{"arxiv_id":"2509.13322","last_updated":"2026-03-18T20:26:19Z","snapshot_observed_at":"2026-07-06T22:30:02.223630Z","submitted_at":"2025-09-16T17:59:59Z","title":"Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-18T15:47:12.746339Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2509.13322"},"observation_digest":"sha256:2c1f0ab37645901202c2e5ea01c7469536c8e6cbb85f4239c8139eac389d68f6","observation_id":"46ccac6e-2e82-4835-ad57-e7766aa2e70b","resolution":{"observed_at":"2026-05-18T15:51:34.722511Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":"2410.10945","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Springmann, M","venue":null,"work_id":"50fc2ff7-fb5c-47d7-a35c-8ec29fabe772","year":2025},"citing_paper":{"arxiv_id":"2509.25305","last_updated":"2026-05-15T10:25:52Z","snapshot_observed_at":"2026-07-06T22:31:10.099674Z","submitted_at":"2025-09-29T18:00:00Z","title":"$\\phi$-Dwarfs: White Dwarfs probe Quadratically Coupled Scalars","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-05-21T21:38:33.685810Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2509.25305"},"observation_digest":"sha256:7b1ff864703b1e78b301aa493c9e7d76140bbba244f08fbd34fa669cb93fd20b","observation_id":"6b9552a4-5f36-4866-a0e6-16c8265108a6","resolution":{"observed_at":"2026-05-21T21:40:40.447692Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density","version":2},"cited_work":{"arxiv_id":"2410.10945","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.10945","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Springmann, M","venue":null,"work_id":"50fc2ff7-fb5c-47d7-a35c-8ec29fabe772","year":2025},"citing_paper":{"arxiv_id":"2511.13815","last_updated":"2026-05-02T11:07:26Z","snapshot_observed_at":"2026-08-11T15:21:59.439605Z","submitted_at":"2025-11-17T19:00:00Z","title":"Stripped-Envelope Supernovae for QCD Axion Detection","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-17T21:37:41.394551Z"},"links":{"cited_paper":"/paper/2410.10945","citing_paper":"/paper/2511.13815"},"observation_digest":"sha256:da4b7687f66aeab98ed2bb47c11f443f9a47c6fb323b5ff0eb5748ebd8be09ef","observation_id":"1086480c-fbdc-4209-a074-1d00a076ece0","resolution":{"observed_at":"2026-05-17T21:40:17.937810Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2410.10945/citation-record","integrity":"/paper/2410.10945/integrity","json":"/paper/2410.10945/citation-record.json","paper":"/paper/2410.10945"},"outbound":[],"paper":{"arxiv_id":"2410.10945","last_updated":"2025-02-28T11:00:57Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-12T22:23:25.795957Z","submitted_at":"2024-10-14T18:00:00Z","title":"From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2410.10945."}