{"as_of":"2026-08-07T20:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1fad48a3237479c1cc530eb122e0ac16b63c8e0bcede288528f9db5f389c8c21","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":"2026-08-07T06:34:17.273281+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":"2026-08-06T18:50:28.603126Z","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":"2026-07-02T19:07:18.348246Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2408.07740","last_updated":"2024-12-19T00:09:51Z","snapshot_observed_at":"2026-07-06T19:00:48.581359Z","submitted_at":"2024-08-14T18:00:01Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","version":2},"cited_work":{"arxiv_id":"2408.07740","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.07740","snapshot_observed_at":"2026-07-02T19:07:18.348246Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","venue":null,"work_id":"84dd1ed2-e2ef-4edd-9af5-9b4bf9011cde","year":2024},"citing_paper":{"arxiv_id":"2412.20932","last_updated":"2026-04-29T14:21:41Z","snapshot_observed_at":"2026-07-06T20:14:40.579474Z","submitted_at":"2024-12-30T13:22:39Z","title":"Weak nuclear decays deep-underground as a probe of axion dark matter","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-23T06:51:36.769360Z"},"links":{"cited_paper":"/paper/2408.07740","citing_paper":"/paper/2412.20932"},"observation_digest":"sha256:9063bbbd6f886c944786d07706544926961f9d95997cbb167640d0d760ebcd2c","observation_id":"73948ac3-3a20-42a6-b17c-4412b6f25441","resolution":{"observed_at":"2026-05-23T06:52:39.932823Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07740","last_updated":"2024-12-19T00:09:51Z","snapshot_observed_at":"2026-07-06T19:00:48.581359Z","submitted_at":"2024-08-14T18:00:01Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.07740","snapshot_observed_at":"2026-08-06T18:50:28.603126Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.07482","last_updated":"2026-07-26T11:09:56Z","snapshot_observed_at":"2026-08-07T19:21:01.037377Z","submitted_at":"2025-07-10T07:11:20Z","title":"Probing Fundamental Constant Oscillation in the Galactic Center with S-Star Spectroscopy","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T18:50:28.603126Z"},"links":{"cited_paper":"/paper/2408.07740","citing_paper":"/paper/2507.07482"},"observation_digest":"sha256:f37f7db418b7faafe759e8e49989131352126897952902d012889f513edf9d8d","observation_id":"7b2a45d3-48c9-4af2-bd82-a78d2ad3794a","resolution":{"observed_at":"2026-08-06T18:50:28.603126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07740","last_updated":"2024-12-19T00:09:51Z","snapshot_observed_at":"2026-07-06T19:00:48.581359Z","submitted_at":"2024-08-14T18:00:01Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","version":2},"cited_work":{"arxiv_id":"2408.07740","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.07740","snapshot_observed_at":"2026-07-02T19:07:18.348246Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","venue":null,"work_id":"84dd1ed2-e2ef-4edd-9af5-9b4bf9011cde","year":2024},"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":37,"source":"pdf_text","source_observed_at":"2026-05-21T21:38:33.685810Z"},"links":{"cited_paper":"/paper/2408.07740","citing_paper":"/paper/2509.25305"},"observation_digest":"sha256:2b1d050b7c4180f6769ef6417b8d7c77c7ff3f45be93d2088cbe50356cca552c","observation_id":"5d5b7fff-f5d8-4a27-8e29-da5c70abe748","resolution":{"observed_at":"2026-05-21T21:40:40.491681Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07740","last_updated":"2024-12-19T00:09:51Z","snapshot_observed_at":"2026-07-06T19:00:48.581359Z","submitted_at":"2024-08-14T18:00:01Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","version":2},"cited_work":{"arxiv_id":"2408.07740","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.07740","snapshot_observed_at":"2026-07-02T19:07:18.348246Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","venue":null,"work_id":"84dd1ed2-e2ef-4edd-9af5-9b4bf9011cde","year":2024},"citing_paper":{"arxiv_id":"2602.18392","last_updated":"2026-05-22T12:43:26Z","snapshot_observed_at":"2026-08-06T17:12:27.313063Z","submitted_at":"2026-02-20T17:57:15Z","title":"RadioAxion results on the search for axion dark matter under Gran Sasso","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-25T07:27:56.158622Z"},"links":{"cited_paper":"/paper/2408.07740","citing_paper":"/paper/2602.18392"},"observation_digest":"sha256:26886d839924536b820fb59cee855ec3a15dac47f2603f8efe54d32544b42011","observation_id":"ac6bd971-6097-4844-b9c8-550ef5c5fc02","resolution":{"observed_at":"2026-05-25T07:30:27.745004Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07740","last_updated":"2024-12-19T00:09:51Z","snapshot_observed_at":"2026-07-06T19:00:48.581359Z","submitted_at":"2024-08-14T18:00:01Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","version":2},"cited_work":{"arxiv_id":"2408.07740","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2408.07740","snapshot_observed_at":"2026-07-02T19:07:18.348246Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling","venue":null,"work_id":"84dd1ed2-e2ef-4edd-9af5-9b4bf9011cde","year":2024},"citing_paper":{"arxiv_id":"2606.07742","last_updated":"2026-06-05T18:00:04Z","snapshot_observed_at":"2026-07-06T23:47:19.773490Z","submitted_at":"2026-06-05T18:00:04Z","title":"Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-27T21:37:55.919953Z"},"links":{"cited_paper":"/paper/2408.07740","citing_paper":"/paper/2606.07742"},"observation_digest":"sha256:c37fabce524db4ebea1877347f8a988826ccf93ea04e33ceb8e8fd21852a52f2","observation_id":"6616bffa-639a-4239-bca1-f2717f3f8417","resolution":{"observed_at":"2026-07-02T19:07:18.350062Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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/2408.07740/citation-record","integrity":"/paper/2408.07740/integrity","json":"/paper/2408.07740/citation-record.json","paper":"/paper/2408.07740"},"outbound":[],"paper":{"arxiv_id":"2408.07740","last_updated":"2024-12-19T00:09:51Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-07-06T19:00:48.581359Z","submitted_at":"2024-08-14T18:00:01Z","title":"Constraining Light QCD Axions with Isolated Neutron Star Cooling"},"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 5 inbound Pith citation observations for arXiv:2408.07740."}