{"as_of":"2026-08-21T08:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:13e9ae37b8633ff0d4dbc21337304a8db5b179660f2010a74deae874401bd05e","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":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T10:15:09.043524Z","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":"2026-07-03T09:57:55.787412Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":"1804.03145","doi":null,"metadata_source":"pith","pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-07-03T09:57:55.787412Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","venue":"hep-ph","work_id":"09534ea4-5282-47b5-91bb-0f0a5f68f1de","year":2018},"citing_paper":{"arxiv_id":"2411.17186","last_updated":"2026-04-14T07:48:14Z","snapshot_observed_at":"2026-08-16T13:57:20.338729Z","submitted_at":"2024-11-26T07:51:07Z","title":"Scalar-Induced Electromagnetic Radiation: Comparison with Axion-Like Particles and Implications for Modified Gravity","version":4},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-23T16:49:32.959724Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2411.17186"},"observation_digest":"sha256:43360260050ab908664a2bd9954fad3a55a13f11b5b1207820a71f21a4b78848","observation_id":"5c000802-8920-4aaa-bb2e-07a2438dcff1","resolution":{"observed_at":"2026-05-23T16:53:12.962479Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-08-12T10:15:09.043524Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.19441","last_updated":"2024-12-18T14:32:30Z","snapshot_observed_at":"2026-08-16T11:08:36.843050Z","submitted_at":"2024-11-29T02:53:27Z","title":"Indirect detection of the QCD axion","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T10:15:09.043524Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2411.19441"},"observation_digest":"sha256:4635854d23a218382bc81d848a7a297e123ce35307704aac51e375c3ce551e4b","observation_id":"235861c8-4ce7-4173-9f25-de42c8d5e80f","resolution":{"observed_at":"2026-08-12T10:15:09.043524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-08-07T14:01:03.087317Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.20450","last_updated":"2025-05-26T18:43:50Z","snapshot_observed_at":"2026-08-18T20:09:06.677912Z","submitted_at":"2025-05-26T18:43:50Z","title":"Searching for Axion Dark Matter Near Relaxing Magnetars","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T14:01:03.087317Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2505.20450"},"observation_digest":"sha256:0aa58bc9267bfc51841106cc7432a4648912bd93927cf6f4940c6cd15311aacd","observation_id":"432174dd-1060-4920-8215-49130fad4aa1","resolution":{"observed_at":"2026-08-07T14:01:03.087317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-08-06T19:18:33.624680Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.06178","last_updated":"2025-07-08T17:00:03Z","snapshot_observed_at":"2026-08-15T21:39:35.755145Z","submitted_at":"2025-07-08T17:00:03Z","title":"Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter?","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T19:18:33.624680Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2507.06178"},"observation_digest":"sha256:0cacd68c80c4c29e4b5eb3e608a6c079e8a5c81b51a2819dc0a702d88baed83e","observation_id":"6345e454-b680-4718-98f5-13b2359bafab","resolution":{"observed_at":"2026-08-06T19:18:33.624680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-08-06T15:21:59.176003Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.16609","last_updated":"2025-07-22T14:07:46Z","snapshot_observed_at":"2026-08-20T13:15:39.058128Z","submitted_at":"2025-07-22T14:07:46Z","title":"Gravitational Wave Scattering on Magnetic Fields","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T15:21:59.176003Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2507.16609"},"observation_digest":"sha256:a61b3be1a7ea2a509e59e6aa0006c56074a9c4005def6238593307f47399deea","observation_id":"9dcd60e2-d17a-49fc-b264-44b4d8f13ffb","resolution":{"observed_at":"2026-08-06T15:21:59.176003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-08-06T15:00:24.291472Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.17384","last_updated":"2025-07-23T10:26:46Z","snapshot_observed_at":"2026-08-18T00:48:38.726611Z","submitted_at":"2025-07-23T10:26:46Z","title":"Mass-Gap Neutron Stars from Vector \\texorpdfstring{$f(R)$}{f(R)} Gravity Inflationary Deformations","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T15:00:24.291472Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2507.17384"},"observation_digest":"sha256:6134f3def3565d8b4a3b609c15cab0c7b487fca87087ad74e1eb23412bc7599a","observation_id":"fda9373e-0f93-45cd-8b84-6268a3aea141","resolution":{"observed_at":"2026-08-06T15:00:24.291472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":"1804.03145","doi":null,"metadata_source":"pith","pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-07-03T09:57:55.787412Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","venue":"hep-ph","work_id":"09534ea4-5282-47b5-91bb-0f0a5f68f1de","year":2018},"citing_paper":{"arxiv_id":"2606.25537","last_updated":"2026-06-24T08:13:20Z","snapshot_observed_at":"2026-08-02T10:33:53.318398Z","submitted_at":"2026-06-24T08:13:20Z","title":"Probing the Fundamental Nature of Particle Dark Matter","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2606.25537"},"observation_digest":"sha256:a8de090a28cbe9a59f7de54ef6006f56fc79827b18a14974329200fa6e19a270","observation_id":"6c1c0838-0dca-4b83-86d0-36d91afc0c5c","resolution":{"observed_at":"2026-06-25T21:38:29.524601Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":"1804.03145","doi":null,"metadata_source":"pith","pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-07-03T09:57:55.787412Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","venue":"hep-ph","work_id":"09534ea4-5282-47b5-91bb-0f0a5f68f1de","year":2018},"citing_paper":{"arxiv_id":"2606.31476","last_updated":"2026-06-30T10:51:32Z","snapshot_observed_at":"2026-08-15T20:44:04.400802Z","submitted_at":"2026-06-30T10:51:32Z","title":"Landau-Zener formula and resonant axion conversion in neutron star magnetospheres","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-01T05:03:19.549528Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2606.31476"},"observation_digest":"sha256:8b57b6266e40730bc45e8593d58ed72e186379248a48629e8fcb014a435d4329","observation_id":"3dc49384-e209-46af-82f1-0d661b4b92f0","resolution":{"observed_at":"2026-07-01T10:45:43.197392Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":"1804.03145","doi":null,"metadata_source":"pith","pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-07-03T09:57:55.787412Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","venue":"hep-ph","work_id":"09534ea4-5282-47b5-91bb-0f0a5f68f1de","year":2018},"citing_paper":{"arxiv_id":"2607.02232","last_updated":"2026-07-02T14:32:02Z","snapshot_observed_at":"2026-08-15T03:03:26.935670Z","submitted_at":"2026-07-02T14:32:02Z","title":"Sideband Structure of Axion Electrodynamics","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-03T09:54:33.386737Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2607.02232"},"observation_digest":"sha256:90d009c3e67312126966046a4becd907e5f9e2074f7c5de70c92cfea2bb1bc83","observation_id":"afc08c77-38fc-4bd8-b372-57e0f64151f0","resolution":{"observed_at":"2026-07-03T09:57:55.789303Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-07-12T05:03:41.498841Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.03078","last_updated":"2026-07-03T08:11:20Z","snapshot_observed_at":"2026-08-15T15:21:29.964018Z","submitted_at":"2026-07-03T08:11:20Z","title":"Galactic Centre Pulsars with the SKAO","version":1},"reference_index":126,"source":"arxiv_source","source_observed_at":"2026-07-12T05:03:41.498841Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2607.03078"},"observation_digest":"sha256:90538b01bb2665d89b9e216665a317da132a37839e455df879e562ceffb151bb","observation_id":"c768276d-53bc-44ed-acc2-d4cf712b6dc8","resolution":{"observed_at":"2026-07-12T05:03:41.498841Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03145","snapshot_observed_at":"2026-08-05T00:40:10.692611Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.00589","last_updated":"2026-08-01T10:57:38Z","snapshot_observed_at":"2026-08-14T23:51:42.269955Z","submitted_at":"2026-08-01T10:57:38Z","title":"Gamma Rays from ALP-Photon Conversion and Inverse Compton Reprocessing in Neutron Star Magnetospheres","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-05T00:40:10.692611Z"},"links":{"cited_paper":"/paper/1804.03145","citing_paper":"/paper/2608.00589"},"observation_digest":"sha256:be6d4aaedf9d66e3adf6372750773135317da7c87391b65f2a047f72b4efcbce","observation_id":"746e18b2-398c-4c8f-bb34-b6398829af0a","resolution":{"observed_at":"2026-08-05T00:40:10.692611Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1804.03145/citation-record","integrity":"/paper/1804.03145/integrity","json":"/paper/1804.03145/citation-record.json","paper":"/paper/1804.03145"},"outbound":[],"paper":{"arxiv_id":"1804.03145","last_updated":"2018-04-09T18:00:01Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-17T17:19:31.843044Z","submitted_at":"2018-04-09T18:00:01Z","title":"Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres"},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:1804.03145."}