{"as_of":"2026-08-14T17:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:01c67327c243a4a3bdec313635dd9de777ec7b158799cae5d4e5aec453f9265a","coverage":[{"denominator":92,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":92,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T05:28:09.169393Z","state":"measured"},{"denominator":94,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":94,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+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":"2026-05-18T12:44:55.766757Z","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":"2026-05-18T12:46:23.699326Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"cited_work":{"arxiv_id":"1909.01278","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.01278","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Dietrich and K","venue":null,"work_id":"d0d53c0b-cf96-416f-a83c-3f93eb27ed54","year":2019},"citing_paper":{"arxiv_id":"2509.25838","last_updated":"2026-04-16T18:51:06Z","snapshot_observed_at":"2026-07-06T22:31:10.099674Z","submitted_at":"2025-09-30T06:23:26Z","title":"Bulk viscosity from neutron decays to dark baryons in neutron star matter","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-05-18T12:44:55.766757Z"},"links":{"cited_paper":"/paper/1909.01278","citing_paper":"/paper/2509.25838"},"observation_digest":"sha256:d87099a94af3c5d66f5f263b19320a5a4b9b8b7e31ce2659ecda9b56976c4feb","observation_id":"01522c5d-d4ec-4975-9114-8d7bb6503c4d","resolution":{"observed_at":"2026-05-18T12:46:23.702358Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"cited_work":{"arxiv_id":"1909.01278","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.01278","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Dietrich and K","venue":null,"work_id":"d0d53c0b-cf96-416f-a83c-3f93eb27ed54","year":2019},"citing_paper":{"arxiv_id":"2604.02413","last_updated":"2026-04-02T18:00:00Z","snapshot_observed_at":"2026-08-11T00:29:23.416387Z","submitted_at":"2026-04-02T18:00:00Z","title":"The Black Hole Mass Gap as a New Probe of Millicharged Particles","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-13T21:01:01.821843Z"},"links":{"cited_paper":"/paper/1909.01278","citing_paper":"/paper/2604.02413"},"observation_digest":"sha256:7dfe4fe0e025a6199866dad3ebd4e46481a5b7fab22f1d7a9423ae8a7ec7e458","observation_id":"50694df1-ca03-4cbf-a4e5-c5b4bf187e37","resolution":{"observed_at":"2026-05-13T21:03:19.802078Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1909.01278/citation-record","integrity":"/paper/1909.01278/integrity","json":"/paper/1909.01278/citation-record.json","paper":"/paper/1909.01278"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-14T05:28:08.730181Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.730181Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:597c788ccd31ab455a337cc8417e61cb502ea4ffc8e8b6e48ba7412ea0ff6197","observation_id":"27cee86d-2dbc-4d84-8760-41c64f3fc7c2","resolution":{"observed_at":"2026-08-14T05:28:08.730181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11581","last_updated":"2018-10-15T17:59:04Z","snapshot_observed_at":"2026-08-13T07:04:27.028955Z","submitted_at":"2018-05-29T16:56:13Z","title":"GW170817: Measurements of Neutron Star Radii and Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11581","snapshot_observed_at":"2026-08-14T05:28:08.736760Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.736760Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:0730f9279e6c46f122502436942b07a8379f36e71f821680f4097b797b1859f1","observation_id":"d6ec141f-9696-4da1-95bb-14b81a9929d9","resolution":{"observed_at":"2026-08-14T05:28:08.736760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11579","last_updated":"2019-01-22T19:56:03Z","snapshot_observed_at":"2026-07-06T06:41:51.126097Z","submitted_at":"2018-05-29T16:55:48Z","title":"Properties of the binary neutron star merger GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11579","snapshot_observed_at":"2026-08-14T05:28:08.742504Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.742504Z"},"links":{"cited_paper":"/paper/1805.11579","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:ab5da23ac10e6380e59ab7e5941cbb0e4af636addd16da6b69880ed0bd0788e8","observation_id":"52935251-4ece-4577-900c-4c8551d930f5","resolution":{"observed_at":"2026-08-14T05:28:08.742504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-08-14T05:28:08.748313Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.748313Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:ce2819599ab909edb3da0f728a9d8acf8e336a53bf9d8ea211f51fb10bf142fd","observation_id":"666f1e78-3d51-4e63-a1a2-188a9b8bd6d1","resolution":{"observed_at":"2026-08-14T05:28:08.748313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05834","last_updated":"2017-11-02T11:19:17Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:57:19Z","title":"Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05834","snapshot_observed_at":"2026-08-14T05:28:08.754038Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.754038Z"},"links":{"cited_paper":"/paper/1710.05834","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:9da9b756f656f4af8325b28b235abc9ecd594394e7a0bd3ae7affcfe4a67b1f8","observation_id":"4ba03c69-56e2-49fd-8533-4226ccb19c85","resolution":{"observed_at":"2026-08-14T05:28:08.754038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05833","last_updated":"2017-10-24T12:03:18Z","snapshot_observed_at":"2026-08-02T02:15:12.749442Z","submitted_at":"2017-10-16T16:57:18Z","title":"Multi-messenger Observations of a Binary Neutron Star Merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05833","snapshot_observed_at":"2026-08-14T05:28:08.760589Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.760589Z"},"links":{"cited_paper":"/paper/1710.05833","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:d27308c1317b4e31a0e65c17c6273b184001fd60a22b6337276673d21f90c943","observation_id":"0daccb31-2b1c-4da9-af41-cad7a4bcb349","resolution":{"observed_at":"2026-08-14T05:28:08.760589Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05452","last_updated":"2017-10-16T16:57:35Z","snapshot_observed_at":"2026-08-05T05:30:21.316562Z","submitted_at":"2017-10-16T16:57:35Z","title":"Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05452","snapshot_observed_at":"2026-08-14T05:28:08.767500Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.767500Z"},"links":{"cited_paper":"/paper/1710.05452","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:c7c7f47436b5a8275e8ad612ac46742c0d15ee946caa1072d79f51e948a18d9d","observation_id":"495b0bbd-357a-43d8-908c-f0d9e7a863ff","resolution":{"observed_at":"2026-08-14T05:28:08.767500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.07456","last_updated":"2016-07-25T20:03:51Z","snapshot_observed_at":"2026-07-06T05:04:52.078932Z","submitted_at":"2016-07-25T20:03:51Z","title":"Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run","version":1},"cited_work":{"arxiv_id":"1607.07456","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.07456","snapshot_observed_at":"2026-08-14T05:28:10.448730Z","title":"Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run","venue":"astro-ph.HE","work_id":"f25b87eb-0dd6-4270-93af-1bcf2ed4dc20","year":2016},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.773380Z"},"links":{"cited_paper":"/paper/1607.07456","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:4a1a24c49e83986d78dd0557d2867e35c2fc484809d249f5758c862cddda4395","observation_id":"75ab9c40-b7cd-4e54-928b-5b09c690db29","resolution":{"observed_at":"2026-08-14T05:28:10.453884Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.07885","last_updated":"2017-10-17T11:34:15Z","snapshot_observed_at":"2026-07-06T05:56:46.045868Z","submitted_at":"2017-08-21T18:00:00Z","title":"Double neutron stars: merger rates revisited","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.07885","snapshot_observed_at":"2026-08-14T05:28:08.778461Z","title":"Chruslinska, K","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.778461Z"},"links":{"cited_paper":"/paper/1708.07885","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:f00a5d158a94a59ecf34a49467539d679f20fececfe3687c0fc330729298e2a7","observation_id":"153c2f17-e01b-4840-961f-ae63a423817c","resolution":{"observed_at":"2026-08-14T05:28:08.778461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.784814Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.784814Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:8776d7f2991a34abff9df2d9c8a88e6ea6a08bdec532b2dc3f74bc14a5bd1da3","observation_id":"b40546fe-0947-47a1-aeed-164d52ef56af","resolution":{"observed_at":"2026-08-14T05:28:08.784814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.790071Z","title":"Vafa and E","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.790071Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:0825d87cae5c32d7dfc122178725f60ad017604f2640037347ba4c84942bc72e","observation_id":"ea93597b-d8d8-4a42-be2b-288e0b3e0414","resolution":{"observed_at":"2026-08-14T05:28:08.790071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.02669","last_updated":"2023-11-19T20:25:04Z","snapshot_observed_at":"2026-08-14T17:47:23.407408Z","submitted_at":"2018-12-06T17:11:32Z","title":"TASI Lectures on the Strong CP Problem and Axions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.02669","snapshot_observed_at":"2026-08-14T05:28:08.795337Z","title":"Hook, PoS T ASI2018, 004 (2019), 1812.02669","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.795337Z"},"links":{"cited_paper":"/paper/1812.02669","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:d7b1cc8ecf650976df82c6d947ded9866a6a81f440381a255a2cb0174fabf561","observation_id":"bb855f57-b947-44dd-8a17-fbf3e7f03008","resolution":{"observed_at":"2026-08-14T05:28:08.795337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.800963Z","title":"Svrcek and E","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.800963Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:aca0509dd3879f8414e37e77180eebe0f5989b67475042f6916cfd692b910e7d","observation_id":"abcf0acb-8108-4e56-be6d-2808893b4b95","resolution":{"observed_at":"2026-08-14T05:28:08.800963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.805449Z","title":null,"venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.805449Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:4d46036e42dd416c2e19960a9e8d515288b922497252a2936ee46631b26945bf","observation_id":"6aee6fd3-791f-498a-a987-9d18a4db16bb","resolution":{"observed_at":"2026-08-14T05:28:08.805449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.810099Z","title":"Preskill, M","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.810099Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:12f9b31aa048edf587ca8b25e9a2938a96e8dca89fc8b9e715171d1ab2717a70","observation_id":"57a5d8d4-c4e1-4cdf-9503-66dc8a47ec2f","resolution":{"observed_at":"2026-08-14T05:28:08.810099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.814771Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.814771Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:3d0b8b309811a679f617f1c418a4d0a4ebe917ecd4f4c3c342e432f8e0ffd3c5","observation_id":"4934c717-6dae-415f-87a7-5d11ec9df6bb","resolution":{"observed_at":"2026-08-14T05:28:08.814771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.819469Z","title":"Dine and W","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.819469Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:046e55ab9d17dfb141b7baa86c8078efc9ea5ddea7cc534b8627f416e7350fd8","observation_id":"680c60db-8c43-45b8-a9c4-20d8bb027f7a","resolution":{"observed_at":"2026-08-14T05:28:08.819469Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.07633","last_updated":"2016-06-15T09:26:10Z","snapshot_observed_at":"2026-07-06T04:34:18.606343Z","submitted_at":"2015-10-26T20:14:39Z","title":"Axion Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.07633","snapshot_observed_at":"2026-08-14T05:28:08.823839Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.823839Z"},"links":{"cited_paper":"/paper/1510.07633","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:d36ea9f06db18ae89990ccb3d42e0822d070390155e6ba4ea306484ef1902906","observation_id":"47020706-756b-4863-9498-9e55cb12f031","resolution":{"observed_at":"2026-08-14T05:28:08.823839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.829004Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.829004Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:e595bde1188928de241efe9a3edb69ce3382a0dfc3c76a0d7e0a5a9909587148","observation_id":"3f1b249d-e559-4bd8-bdce-2a3e6190506f","resolution":{"observed_at":"2026-08-14T05:28:08.829004Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.833690Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.833690Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:67d9fb07a87eaf74e7a31d78924509bdcd335d609feeb816151340bba6774487","observation_id":"83b292e5-0ff0-4622-9adf-668362040322","resolution":{"observed_at":"2026-08-14T05:28:08.833690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.838261Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.838261Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:8e95dac7c3fd401b9c3269e3ad64a081bc64ce8affda96f9b6d26ee84364a743","observation_id":"201cc9d8-0b6c-4e01-a3a2-38823e6fe593","resolution":{"observed_at":"2026-08-14T05:28:08.838261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9903472","last_updated":"1999-03-24T14:19:27Z","snapshot_observed_at":"2026-07-07T04:32:32.802594Z","submitted_at":"1999-03-24T14:19:27Z","title":"Particle Physics from Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9903472","snapshot_observed_at":"2026-08-14T05:28:08.842701Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.842701Z"},"links":{"cited_paper":"/paper/hep-ph/9903472","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:67a8b1cde00eb8ed5e9c3b318a1a9af97b79793d3c7b09dda3bd426c2a4e5be8","observation_id":"8ad549b6-abf3-4e84-b05b-547d38a6dfa0","resolution":{"observed_at":"2026-08-14T05:28:08.842701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.847651Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.847651Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:e7394e85bfb29edb79156f8af789f00795447059382a6550aa8a4fdc944f23bf","observation_id":"49b176df-89e9-4f66-820d-3daf4cbc1641","resolution":{"observed_at":"2026-08-14T05:28:08.847651Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9807476","last_updated":"1998-12-03T17:10:40Z","snapshot_observed_at":"2026-07-07T04:30:13.067582Z","submitted_at":"1998-07-23T13:03:08Z","title":"Helioseismological constraint on solar axion emission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9807476","snapshot_observed_at":"2026-08-14T05:28:08.852358Z","title":"Schlattl, A","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.852358Z"},"links":{"cited_paper":"/paper/hep-ph/9807476","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:a0b3033331d0ed589d088ddeefa6371cce62d9a1e3aefd2b6c71f295bb229160","observation_id":"9fcb2944-2a24-417c-a340-2302e791056b","resolution":{"observed_at":"2026-08-14T05:28:08.852358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.856968Z","title":"Isern and E","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.856968Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:9d3493f66b070f109de72b06d1f3ec7db717c287a782a9703a5621769a6b9c1b","observation_id":"da4e58b9-0b2a-487e-9816-3842f53582eb","resolution":{"observed_at":"2026-08-14T05:28:08.856968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0611350","last_updated":"2006-11-28T12:29:51Z","snapshot_observed_at":"2026-07-07T04:13:06.058372Z","submitted_at":"2006-11-28T12:29:51Z","title":"Astrophysical Axion Bounds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0611350","snapshot_observed_at":"2026-08-14T05:28:08.861353Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.861353Z"},"links":{"cited_paper":"/paper/hep-ph/0611350","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:fdac9839703f77e409423df17d8b63c76f43d6ee73ee4a757613321fd8f8beef","observation_id":"b1771567-ee2b-4504-b4f3-540f9092b63a","resolution":{"observed_at":"2026-08-14T05:28:08.861353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.866014Z","title":null,"venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.866014Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:4fa73b7897128d8525ca26682ceab1d7541a1beddf5891afe88bc02204ec2410","observation_id":"90d26cf6-ac6f-4528-b80f-d5a053234e43","resolution":{"observed_at":"2026-08-14T05:28:08.866014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.700626Z","title":"Raffelt and D","venue":null,"work_id":"8b5a4349-9d27-4677-ad38-a04e7dabd49f","year":1988},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.870279Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:84aa64dac4197b2f1739198e9654c3456c894d9432ff6431fbe6a8147789a3dc","observation_id":"a8a29795-9fb7-4eba-8ea7-5dfaa5381a50","resolution":{"observed_at":"2026-08-14T05:28:10.705507Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.685877Z","title":null,"venue":null,"work_id":"8d3e3d05-123f-4f79-b9e4-1ee495bfeac1","year":1988},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.874737Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:2a59243da699a47e1e930b544789fe8ee5cefc26a95025e1dfdf51ee3c25cf98","observation_id":"a6d58165-8673-43cf-95ab-87368efa891f","resolution":{"observed_at":"2026-08-14T05:28:10.690543Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.670067Z","title":"Mayle, J","venue":null,"work_id":"dd32367e-6453-4ae2-b5b9-fc51a3857bbe","year":1988},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.879167Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:f2339ca84fe7c6aba5d99f1e4f03783fe00f85c44af06429b715f54c884a45ec","observation_id":"1fb95952-2375-4acc-9969-d81538f8efd0","resolution":{"observed_at":"2026-08-14T05:28:10.675737Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.655591Z","title":"Mayle, J","venue":null,"work_id":"bbc66be8-79bf-4767-aa9f-2914512d1712","year":1989},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.883920Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:69fa8ed90f8478284226fb174a119054bc7b84408cd09a59b8fff07c5c667d63","observation_id":"5743b068-c7f5-4531-8c28-3d6789e820d4","resolution":{"observed_at":"2026-08-14T05:28:10.660183Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.640638Z","title":"Burrows, M","venue":null,"work_id":"83d8eb6a-9153-4c10-afee-5057894ac80a","year":1989},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.888427Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:3bdc58e92bd6e2c6218c0247032227c8016a57e88501622e934f7b5b73425c19","observation_id":"36b0a610-bd9f-4f8a-a2d4-8e64296f681c","resolution":{"observed_at":"2026-08-14T05:28:10.645512Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:08.892872Z","title":"Burrows, M","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.892872Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:199e1661e35282f36c9031c85769d944a6073d6da0d341a8c25c1f8d1014e597","observation_id":"56c05237-5c7f-4278-a415-57c0437bfb94","resolution":{"observed_at":"2026-08-14T05:28:08.892872Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9612222","last_updated":"1996-12-23T17:27:00Z","snapshot_observed_at":"2026-08-11T10:44:48.843866Z","submitted_at":"1996-12-23T17:27:00Z","title":"A Fresh Look at Axions and SN 1987A","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9612222","snapshot_observed_at":"2026-08-14T05:28:08.897315Z","title":"Keil, H.-T","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.897315Z"},"links":{"cited_paper":"/paper/astro-ph/9612222","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:91ca54e62cc42fa53f792c199939c4ecac4a6bda847a8098dee682fcae08b43c","observation_id":"45f412ad-f75d-4481-a175-926e906fd127","resolution":{"observed_at":"2026-08-14T05:28:08.897315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00993","last_updated":"2018-09-17T04:50:13Z","snapshot_observed_at":"2026-07-06T06:26:20.207918Z","submitted_at":"2018-03-02T18:46:17Z","title":"Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.00993","snapshot_observed_at":"2026-08-14T05:28:08.902251Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.902251Z"},"links":{"cited_paper":"/paper/1803.00993","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:79add99014727a37efa49a9b3d1e0090e5f5c92058b36785a8d533a27d1291c6","observation_id":"4982b258-0875-48f0-a95f-c11549492a09","resolution":{"observed_at":"2026-08-14T05:28:08.902251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.5487","last_updated":"2012-09-18T17:03:42Z","snapshot_observed_at":"2026-07-06T02:54:27.204840Z","submitted_at":"2012-08-27T20:00:05Z","title":"Importance of cooling in triggering the collapse of hypermassive neutron stars","version":2},"cited_work":{"arxiv_id":"1208.5487","doi":null,"metadata_source":"pith","pith_arxiv_id":"1208.5487","snapshot_observed_at":"2026-08-14T05:28:10.253579Z","title":"Importance of cooling in triggering the collapse of hypermassive neutron stars","venue":"astro-ph.HE","work_id":"406bf037-7cde-4eb5-9b13-50b51919fc25","year":2012},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.907025Z"},"links":{"cited_paper":"/paper/1208.5487","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:29a0b238c15281375a15ceef72ff40a97524979c576177809741b4612e448074","observation_id":"b42ef0a5-d17f-4eb1-94c9-b4dfe0f04f4c","resolution":{"observed_at":"2026-08-14T05:28:10.258681Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.04138","last_updated":"2019-04-10T14:48:02Z","snapshot_observed_at":"2026-08-14T17:31:31.758159Z","submitted_at":"2019-01-14T05:35:44Z","title":"When Did the Remnant of GW170817 Collapse to a Black Hole?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.04138","snapshot_observed_at":"2026-08-14T05:28:08.911671Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.911671Z"},"links":{"cited_paper":"/paper/1901.04138","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:aebbf6c510438e5066900c638d592bfbff261015405122bf31d5908d283fe17d","observation_id":"5b9624d0-8514-47da-af50-7a60afd3f22f","resolution":{"observed_at":"2026-08-14T05:28:08.911671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.09320","last_updated":"2017-10-25T16:11:09Z","snapshot_observed_at":"2026-08-13T04:05:42.720049Z","submitted_at":"2017-10-25T16:11:09Z","title":"Search for post-merger gravitational waves from the remnant of the binary neutron star merger GW170817","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.09320","snapshot_observed_at":"2026-08-14T05:28:08.916325Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.916325Z"},"links":{"cited_paper":"/paper/1710.09320","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:f5a4e13bf0f2c5d009a473b42415d79a08e684b8301c234373ff137926be6abc","observation_id":"30be91a7-9581-4514-9bda-17a40c90486a","resolution":{"observed_at":"2026-08-14T05:28:08.916325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0302301","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.198356Z","title":"Rosswog and M","venue":null,"work_id":"650115bd-56a9-4977-9653-805131c9d6a1","year":2003},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.921337Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:8cfbb480e271ce7e8b97b12163dd08ddec1bce36655fec99e78d9b4cbc9482ba","observation_id":"b5783782-460f-4730-b09b-b158c46c0625","resolution":{"observed_at":"2026-08-14T05:28:10.206129Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0806.4380","last_updated":"2008-06-26T20:00:25Z","snapshot_observed_at":"2026-07-06T01:39:34.416146Z","submitted_at":"2008-06-26T20:00:25Z","title":"Neutrino signatures and the neutrino-driven wind in Binary Neutron Star Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.4380","snapshot_observed_at":"2026-08-14T05:28:08.925605Z","title":"Dessart, C","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.925605Z"},"links":{"cited_paper":"/paper/0806.4380","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:c8f1e819c14341fea3419bb147693665750a37257c7c39528e05367ecef3ec67","observation_id":"f495d6f5-493a-45ae-baa5-d58e0bb80dd0","resolution":{"observed_at":"2026-08-14T05:28:08.925605Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.2125","last_updated":"2011-06-24T03:23:51Z","snapshot_observed_at":"2026-07-06T02:27:34.105640Z","submitted_at":"2011-05-11T08:53:17Z","title":"Gravitational waves and neutrino emission from the merger of binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.2125","snapshot_observed_at":"2026-08-14T05:28:08.930027Z","title":"Sekiguchi, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.930027Z"},"links":{"cited_paper":"/paper/1105.2125","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:7f6c31369d01b3f8d45177bc231e277881b517abcdc15d66d74a601d3e27be77","observation_id":"f2274a79-6072-4960-846a-01a602b1e487","resolution":{"observed_at":"2026-08-14T05:28:08.930027Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.4953","last_updated":"2013-10-02T15:08:26Z","snapshot_observed_at":"2026-07-06T03:16:25.257171Z","submitted_at":"2013-06-20T18:32:07Z","title":"Implementation of a simplified approach to radiative transfer in general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.4953","snapshot_observed_at":"2026-08-14T05:28:08.934529Z","title":"Galeazzi, W","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.934529Z"},"links":{"cited_paper":"/paper/1306.4953","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:2e65f563b27c2af551b07013e62d592e9d04b6e7ac1b1db1f3db243c15e603c7","observation_id":"495c3120-86ff-4c8d-b50a-8095226d7533","resolution":{"observed_at":"2026-08-14T05:28:08.934529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1121","last_updated":"2014-06-19T19:19:08Z","snapshot_observed_at":"2026-08-04T09:23:53.517600Z","submitted_at":"2014-05-06T01:32:48Z","title":"Neutron star-black hole mergers with a nuclear equation of state and neutrino cooling: Dependence in the binary parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1121","snapshot_observed_at":"2026-08-14T05:28:08.939133Z","title":"Foucart, M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.939133Z"},"links":{"cited_paper":"/paper/1405.1121","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:834d8a53c4cdc12ef0e35c798ddfe86b6b2075625d2a07ea2b8a5e5cbe399c5c","observation_id":"094f4e6b-2c1a-4919-bea5-3398731c51d0","resolution":{"observed_at":"2026-08-14T05:28:08.939133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.3680","last_updated":"2014-05-09T15:36:29Z","snapshot_observed_at":"2026-08-04T04:31:19.774761Z","submitted_at":"2014-03-14T19:41:42Z","title":"Magnetized Neutron Stars With Realistic Equations of State and Neutrino Cooling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.3680","snapshot_observed_at":"2026-08-14T05:28:08.944591Z","title":"Neilsen, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.944591Z"},"links":{"cited_paper":"/paper/1403.3680","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:cbe9400c798d1749c370e8f5ea5ab95520a3646600f7ecb6e754db829ad9403e","observation_id":"da8b7f07-d039-44b4-8ac1-32dd0a5f6183","resolution":{"observed_at":"2026-08-14T05:28:08.944591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.01607","last_updated":"2015-05-07T07:35:19Z","snapshot_observed_at":"2026-08-10T03:31:43.290630Z","submitted_at":"2015-05-07T07:35:19Z","title":"Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.01607","snapshot_observed_at":"2026-08-14T05:28:08.949461Z","title":"Palenzuela, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.949461Z"},"links":{"cited_paper":"/paper/1505.01607","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:effb3d64f1694e4f1b1a971029d694701d732b68cde7b13eb198713199cd47f7","observation_id":"21d1ed14-dd37-459d-ae70-0d1c2fd36e0e","resolution":{"observed_at":"2026-08-14T05:28:08.949461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.00501","last_updated":"2016-03-01T21:44:59Z","snapshot_observed_at":"2026-08-09T09:14:42.045565Z","submitted_at":"2016-03-01T21:44:59Z","title":"Unequal mass binary neutron star mergers and multimessenger signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.00501","snapshot_observed_at":"2026-08-14T05:28:08.954213Z","title":"Lehner, S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.954213Z"},"links":{"cited_paper":"/paper/1603.00501","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:36e83d5f71e6b7219e4866bfdfa64c0afaf101b24d7919c35d51512b38de4f1f","observation_id":"ad1bdd2a-a002-428d-89ed-ef5c12dc8d41","resolution":{"observed_at":"2026-08-14T05:28:08.954213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.02349","last_updated":"2018-06-06T18:00:02Z","snapshot_observed_at":"2026-08-04T05:45:16.472954Z","submitted_at":"2018-06-06T18:00:02Z","title":"Evaluating radiation transport errors in merger simulations using a Monte-Carlo algorithm","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.02349","snapshot_observed_at":"2026-08-14T05:28:08.958958Z","title":"Foucart, M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.958958Z"},"links":{"cited_paper":"/paper/1806.02349","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:a556044ca9ca4311b519b415fee9be9408cdf85848233b29f4549d2f2ac164ff","observation_id":"0190b3ac-4b8a-412f-93ca-c3454dbc9bc1","resolution":{"observed_at":"2026-08-14T05:28:08.958958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.06311","last_updated":"2017-10-04T14:42:49Z","snapshot_observed_at":"2026-08-13T17:52:36.444745Z","submitted_at":"2017-06-20T08:27:59Z","title":"Gravitational wave searches for ultralight bosons with LIGO and LISA","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.06311","snapshot_observed_at":"2026-08-14T05:28:08.963760Z","title":"Brito, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.963760Z"},"links":{"cited_paper":"/paper/1706.06311","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:29dba1eb68d477e5c490c7389216d6604cc2fe5ca1a142d00fa1171f5f37be0c","observation_id":"f8d98eac-f570-4f2d-a4c5-27a318d9b0f8","resolution":{"observed_at":"2026-08-14T05:28:08.963760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.06789","last_updated":"2018-05-23T16:36:32Z","snapshot_observed_at":"2026-07-06T05:23:31.105251Z","submitted_at":"2016-12-20T18:11:58Z","title":"Ultra-Light Dark Matter Resonates with Binary Pulsars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.06789","snapshot_observed_at":"2026-08-14T05:28:08.968782Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.968782Z"},"links":{"cited_paper":"/paper/1612.06789","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:d4a7b966ed6a895ebf44513033ad41f04c48ad8dee44410d2aa603176b2ed047","observation_id":"972dc204-d83c-43fa-ae91-259e20835795","resolution":{"observed_at":"2026-08-14T05:28:08.968782Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01958","last_updated":"2020-03-30T15:20:02Z","snapshot_observed_at":"2026-08-14T17:16:58.924913Z","submitted_at":"2019-04-02T09:25:38Z","title":"Axion resonances in binary pulsar systems","version":4},"cited_work":{"arxiv_id":"1904.01958","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.01958","snapshot_observed_at":"2026-08-14T05:28:09.981534Z","title":"Axion resonances in binary pulsar systems","venue":"astro-ph.CO","work_id":"b57a3ad3-c795-45d4-99e6-3e50c63860f1","year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.973483Z"},"links":{"cited_paper":"/paper/1904.01958","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:57ab596ecb7fe83a65bba19b64f1576c17d9811d3401c901d44a69f3523820d5","observation_id":"2287224b-222e-452b-9e1a-6bdc6d5deaa8","resolution":{"observed_at":"2026-08-14T05:28:09.986444Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.08464","last_updated":"2017-08-28T18:00:08Z","snapshot_observed_at":"2026-08-05T15:08:19.924661Z","submitted_at":"2017-08-28T18:00:08Z","title":"Probing axions with neutron star inspirals and other stellar processes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.08464","snapshot_observed_at":"2026-08-14T05:28:08.978219Z","title":"Hook and J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.978219Z"},"links":{"cited_paper":"/paper/1708.08464","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:ac8032070ba0d3bef39d3393e58718f7eb962e75fc8dfc82f05ad1f034c0dc68","observation_id":"f435c4ea-b8ba-4e7f-aab3-b13bdfb4837c","resolution":{"observed_at":"2026-08-14T05:28:08.978219Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.02133","last_updated":"2019-02-28T20:08:41Z","snapshot_observed_at":"2026-07-06T06:48:36.957224Z","submitted_at":"2018-07-05T18:15:00Z","title":"Prospects for axion searches with Advanced LIGO through binary mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.02133","snapshot_observed_at":"2026-08-14T05:28:08.982775Z","title":"Huang, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.982775Z"},"links":{"cited_paper":"/paper/1807.02133","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:5099458614282885ac17d7d242271657207081d4cf7da309777ac37b7b7e8f2a","observation_id":"65760d76-c937-42c1-abf2-174e2f3404ec","resolution":{"observed_at":"2026-08-14T05:28:08.982775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.06570","last_updated":"2021-01-08T08:19:41Z","snapshot_observed_at":"2026-08-11T07:07:02.101103Z","submitted_at":"2015-01-26T21:00:09Z","title":"Superradiance -- the 2020 Edition","version":8},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.06570","snapshot_observed_at":"2026-08-14T05:28:08.987359Z","title":"Brito, V","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.987359Z"},"links":{"cited_paper":"/paper/1501.06570","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:411e07c97b2884aeb14d29073fcab6f2272fb7e1bf79447feeba762b0e1818a7","observation_id":"f765c655-c87e-4bfd-8808-eed0ca97da29","resolution":{"observed_at":"2026-08-14T05:28:08.987359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.00466","last_updated":"2016-01-30T19:16:00Z","snapshot_observed_at":"2026-07-06T04:38:25.327338Z","submitted_at":"2015-12-01T21:00:06Z","title":"Interaction between bosonic dark matter and stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.00466","snapshot_observed_at":"2026-08-14T05:28:08.991965Z","title":"Brito, V","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.991965Z"},"links":{"cited_paper":"/paper/1512.00466","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:d19ec610648190e60a60a284b484a6578fc5881ee4b2ce6a2cb91677d923901b","observation_id":"836d06d1-b346-4175-b76e-04e751d3ade0","resolution":{"observed_at":"2026-08-14T05:28:08.991965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05540","last_updated":"2018-05-15T13:06:46Z","snapshot_observed_at":"2026-08-02T19:29:54.935750Z","submitted_at":"2017-10-16T07:11:00Z","title":"Search for Dark Matter Effects on Gravitational Signals from Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05540","snapshot_observed_at":"2026-08-14T05:28:08.996738Z","title":"Ellis, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:08.996738Z"},"links":{"cited_paper":"/paper/1710.05540","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:9b9647927fe7787b83bf1b70f86083b17fc60c3ff4204cea257ee8c3827a888f","observation_id":"65010d2d-dd5a-4363-acff-563349cfb4ce","resolution":{"observed_at":"2026-08-14T05:28:08.996738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.08551","last_updated":"2019-09-25T08:11:07Z","snapshot_observed_at":"2026-08-14T16:29:09.074832Z","submitted_at":"2019-05-21T11:16:22Z","title":"Gravitational wave signatures of dark matter cores in binary neutron star mergers by using numerical simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.08551","snapshot_observed_at":"2026-08-14T05:28:09.001289Z","title":"Bezares, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.001289Z"},"links":{"cited_paper":"/paper/1905.08551","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:b43e815f4012adcb5d5048795f5dd61d7b19a661473b08b54f880262d89653fe","observation_id":"6d3856d6-6276-464f-a1a6-dc0be1bc90fe","resolution":{"observed_at":"2026-08-14T05:28:09.001289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.5177","last_updated":"2012-01-13T04:31:50Z","snapshot_observed_at":"2026-07-06T02:34:32.759448Z","submitted_at":"2011-09-23T20:00:03Z","title":"The merger of binary white dwarf-neutron stars: Simulations in full general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.5177","snapshot_observed_at":"2026-08-14T05:28:09.005828Z","title":"Paschalidis, Y","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.005828Z"},"links":{"cited_paper":"/paper/1109.5177","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:ebb17a79dac43adf5ba073dd1ff21875edaca14bdde1d9654afcefeb72d72600","observation_id":"bef009c9-28dc-41c5-a78c-84806a2410b2","resolution":{"observed_at":"2026-08-14T05:28:09.005828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111092","last_updated":"2001-11-12T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2001-11-05T17:05:33Z","title":"A unified equation of state of dense matter and neutron star structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111092","snapshot_observed_at":"2026-08-14T05:28:09.010546Z","title":"Douchin and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.010546Z"},"links":{"cited_paper":"/paper/astro-ph/0111092","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:bbdeebc550b0c870dd38442b246eb51b7993867124fc2261d83407793ed7d26d","observation_id":"383d521d-c79b-44c7-9b53-4c0b4c022c8c","resolution":{"observed_at":"2026-08-14T05:28:09.010546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.2163","last_updated":"2008-12-11T14:59:23Z","snapshot_observed_at":"2026-07-06T01:47:44.956336Z","submitted_at":"2008-12-11T14:59:23Z","title":"Constraints on a phenomenologically parameterized neutron-star equation of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.2163","snapshot_observed_at":"2026-08-14T05:28:09.015309Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.015309Z"},"links":{"cited_paper":"/paper/0812.2163","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:c2d61c76288493cdad63c548b86e0334c8182c0e134bcc1e2977c49d0a8cca28","observation_id":"4b001427-196e-42d6-bab4-7400d7d593ea","resolution":{"observed_at":"2026-08-14T05:28:09.015309Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.12917","last_updated":"2019-04-10T17:50:33Z","snapshot_observed_at":"2026-08-06T19:10:12.361191Z","submitted_at":"2018-10-30T18:00:01Z","title":"Multimessenger Parameter Estimation of GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.12917","snapshot_observed_at":"2026-08-14T05:28:09.019837Z","title":"Radice and L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.019837Z"},"links":{"cited_paper":"/paper/1810.12917","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:766e7fe7f76ff92143b1c832fc342847bb7024132b1b4c18e27d5fa99af56625","observation_id":"5d981c21-14b1-47be-b5b1-aea8a1ed8878","resolution":{"observed_at":"2026-08-14T05:28:09.019837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.04803","last_updated":"2021-02-04T16:55:12Z","snapshot_observed_at":"2026-08-14T17:44:55.944887Z","submitted_at":"2018-12-12T04:23:11Z","title":"Multi-messenger Bayesian parameter inference of a binary neutron-star merger","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.04803","snapshot_observed_at":"2026-08-14T05:28:09.024589Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.024589Z"},"links":{"cited_paper":"/paper/1812.04803","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:3e2af6b7ca4c01f53a91b2e0eeeb073d1a167e54549fe575adc5d7795cc156ba","observation_id":"2d99d651-aa5e-411e-a3b2-aecf7cc8a260","resolution":{"observed_at":"2026-08-14T05:28:09.024589Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0620","last_updated":"2009-08-05T08:53:41Z","snapshot_observed_at":"2026-08-12T09:44:33.645961Z","submitted_at":"2009-08-05T08:53:41Z","title":"A new numerical method to construct binary neutron star initial data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.0620","snapshot_observed_at":"2026-08-14T05:28:09.029401Z","title":"Tichy, Class.Quant.Grav","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.029401Z"},"links":{"cited_paper":"/paper/0908.0620","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:cd35592801fb0861f0fbbae5ae14a681fbdaef8aa1fc394ee83d2cfa63945e1e","observation_id":"d7f3a672-c229-412f-b040-49e24441fb66","resolution":{"observed_at":"2026-08-14T05:28:09.029401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.5336","last_updated":"2014-11-04T18:16:11Z","snapshot_observed_at":"2026-07-06T02:56:12.187611Z","submitted_at":"2012-09-24T17:00:50Z","title":"Constructing quasi-equilibrium initial data for binary neutron stars with arbitrary spins","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.5336","snapshot_observed_at":"2026-08-14T05:28:09.034392Z","title":"Tichy, Phys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.034392Z"},"links":{"cited_paper":"/paper/1209.5336","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:0d2e9a28ba886faa38e96fabb75d32edda7a4259674fab800953ae1df8ccb08b","observation_id":"a3e9be36-4edd-4142-b08d-0b24e530a8dc","resolution":{"observed_at":"2026-08-14T05:28:09.034392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.07100","last_updated":"2015-07-25T13:24:10Z","snapshot_observed_at":"2026-07-06T04:24:52.856912Z","submitted_at":"2015-07-25T13:24:10Z","title":"Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.07100","snapshot_observed_at":"2026-08-14T05:28:09.039305Z","title":"Dietrich, N","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.039305Z"},"links":{"cited_paper":"/paper/1507.07100","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:f94a35838acc27e0bef58ed1c76adf4f082c5eedcba57426806112dd50b46196","observation_id":"17cfb466-ea75-4229-ab77-8231983dd7e4","resolution":{"observed_at":"2026-08-14T05:28:09.039305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:09.044062Z","title":"Br¨ ugmann, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.044062Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:3fc3c931bd33f0007e4db0bd89f4fd68a59bfd53fc5391a7b26ad5118e97bba0","observation_id":"6a8f1334-d6c9-4a47-b274-e768426b1bfd","resolution":{"observed_at":"2026-08-14T05:28:09.044062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.4751","last_updated":"2011-08-11T09:46:12Z","snapshot_observed_at":"2026-08-10T14:54:20.028364Z","submitted_at":"2011-04-25T16:51:36Z","title":"Numerical relativity simulations of binary neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.4751","snapshot_observed_at":"2026-08-14T05:28:09.048740Z","title":"Thierfelder, S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.048740Z"},"links":{"cited_paper":"/paper/1104.4751","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:4f821fb0097fb247868deecd8c291b86a1400b12b6f7056484f3e89a03ff6402","observation_id":"fedba9db-3152-4ce4-828c-b7bc59abe49b","resolution":{"observed_at":"2026-08-14T05:28:09.048740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.01266","last_updated":"2015-04-06T11:34:31Z","snapshot_observed_at":"2026-08-10T08:49:28.194106Z","submitted_at":"2015-04-06T11:34:31Z","title":"Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.01266","snapshot_observed_at":"2026-08-14T05:28:09.053614Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.053614Z"},"links":{"cited_paper":"/paper/1504.01266","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:28a935d89f66ff6121f95f420e63227f0969799f896d539cc216e168e8e6ae96","observation_id":"d5778f0a-eedc-4a5a-9cbe-d427f5ad8439","resolution":{"observed_at":"2026-08-14T05:28:09.053614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06959","last_updated":"2018-07-18T14:22:20Z","snapshot_observed_at":"2026-07-06T06:50:58.300042Z","submitted_at":"2018-07-18T14:22:20Z","title":"Full 3D Numerical Relativity Simulations of Neutron Star -- Boson Star Collisions with BAM","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06959","snapshot_observed_at":"2026-08-14T05:28:09.058584Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.058584Z"},"links":{"cited_paper":"/paper/1807.06959","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:91d8738b67526bfeaa9c9c0630b4af091995dde2859300352a59305af7e71ba6","observation_id":"669aff30-016b-4a55-94aa-a6b08d645088","resolution":{"observed_at":"2026-08-14T05:28:09.058584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.616584Z","title":"Wilson and G","venue":null,"work_id":"0d8e1610-4e86-4163-aa14-5b743a1b96b5","year":1995},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.062952Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:9954785627e72d964b2920c4b28d011dc209ea85cf9623bf320bcea074b8ac1f","observation_id":"c8070063-0ead-43fb-af13-2d3ccb2b8a3f","resolution":{"observed_at":"2026-08-14T05:28:10.621204Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9601017","last_updated":"1996-03-04T22:51:17Z","snapshot_observed_at":"2026-08-07T21:25:58.817733Z","submitted_at":"1996-01-10T23:28:20Z","title":"Relativistic Numerical Method for Close Neutron Star Binaries","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9601017","snapshot_observed_at":"2026-08-14T05:28:09.067386Z","title":"Wilson, G","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.067386Z"},"links":{"cited_paper":"/paper/gr-qc/9601017","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:102b7dadf5509bcf21fbc893da027deb8ad388c786bf3df8cfa11f6de34575c5","observation_id":"02847d7d-e9ad-4b51-80a0-87c94413a5e8","resolution":{"observed_at":"2026-08-14T05:28:09.067386Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:09.072460Z","title":"York, James W., Phys.Rev.Lett","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.072460Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:224e42e2cc96283fe838dad84e4000e11c3422806e8e8d866b091cd1fa4f7b6b","observation_id":"c6b6f2fb-131b-42e7-9a25-b367c137658d","resolution":{"observed_at":"2026-08-14T05:28:09.072460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.03805","last_updated":"2016-12-23T14:32:04Z","snapshot_observed_at":"2026-08-08T11:57:18.073229Z","submitted_at":"2016-10-12T17:52:17Z","title":"The initial value problem as it relates to numerical relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.03805","snapshot_observed_at":"2026-08-14T05:28:09.076903Z","title":"Tichy, Rept","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.076903Z"},"links":{"cited_paper":"/paper/1610.03805","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:63baddab05e6b1fedaa45f655dfecd15d6a53a4c3b2cb8f8de009aacd3327acf","observation_id":"5079398d-c5de-4236-a591-b50f433caff4","resolution":{"observed_at":"2026-08-14T05:28:09.076903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.2920","last_updated":"2010-04-27T16:38:50Z","snapshot_observed_at":"2026-07-06T02:04:43.515736Z","submitted_at":"2009-12-15T15:12:17Z","title":"Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.2920","snapshot_observed_at":"2026-08-14T05:28:09.081927Z","title":"Bernuzzi and D","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.081927Z"},"links":{"cited_paper":"/paper/0912.2920","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:8ceac08303eeaf12f5748491eb10b9c45a1229895f423e04a1ea127afca6d871","observation_id":"78aced26-b6c6-40f1-bfe9-0abe3515b947","resolution":{"observed_at":"2026-08-14T05:28:09.081927Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.2901","last_updated":"2012-12-12T17:44:15Z","snapshot_observed_at":"2026-07-06T03:01:52.564460Z","submitted_at":"2012-12-12T17:44:15Z","title":"Compact binary evolutions with the Z4c formulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.2901","snapshot_observed_at":"2026-08-14T05:28:09.086464Z","title":"Hilditch, S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.086464Z"},"links":{"cited_paper":"/paper/1212.2901","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:74a5899d4258163b9e09cce8a49aaebb1a3b733d6b8489391fd8232db4c79ba1","observation_id":"d2f2b3c1-cc1c-47bf-a145-cdbd7e8d49ea","resolution":{"observed_at":"2026-08-14T05:28:09.086464Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.601553Z","title":null,"venue":null,"work_id":"60350da9-c87d-442c-8bb5-4cac3f4e0af8","year":1996},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.091039Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:edb4eb03a4e0d2c925a9c8a06dd8a54ae74298a91916faa17342b961c61627a8","observation_id":"f323203b-e97b-4405-b937-56daf1027153","resolution":{"observed_at":"2026-08-14T05:28:10.606317Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:09.095395Z","title":"Alcubierre, B","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.095395Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:e8eb6298efe81b2ca7091ae724ad00cca44f43b8ce20ecac673c75500f4ef90a","observation_id":"c2eb8a41-d81b-4251-bb7e-8e4813f8fd24","resolution":{"observed_at":"2026-08-14T05:28:09.095395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0605030","last_updated":"2006-06-18T21:58:06Z","snapshot_observed_at":"2026-07-07T03:22:29.311647Z","submitted_at":"2006-05-05T07:16:10Z","title":"How to move a black hole without excision: gauge conditions for the numerical evolution of a moving puncture","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0605030","snapshot_observed_at":"2026-08-14T05:28:09.099772Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.099772Z"},"links":{"cited_paper":"/paper/gr-qc/0605030","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:a88851df45441e5bd2aae21dfd9e6e9a6d31a5f8756fe14a82a36b257faae53d","observation_id":"0449ba19-6914-4519-b157-57028b22fb41","resolution":{"observed_at":"2026-08-14T05:28:09.099772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.586484Z","title":"Borges, M","venue":null,"work_id":"278b86ae-b65f-4860-8c1d-a87faa124a3a","year":2008},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.104466Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:b1eea3792e669f82be9cc62987d7003e05a53e8ae23180a934a604c3699b1a67","observation_id":"f1000d58-1018-4b69-bb2c-3add9510ac72","resolution":{"observed_at":"2026-08-14T05:28:10.591362Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.07999","last_updated":"2016-09-19T08:43:56Z","snapshot_observed_at":"2026-07-06T04:54:16.596411Z","submitted_at":"2016-04-27T09:48:15Z","title":"Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.07999","snapshot_observed_at":"2026-08-14T05:28:09.108998Z","title":"Bernuzzi and T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.108998Z"},"links":{"cited_paper":"/paper/1604.07999","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:6188db2675ba95f61a25f8fef576e94a9d370bf7450d3af9ec2f0277ad338ef4","observation_id":"c707d8ee-3df4-44aa-a1cb-70df931a78f7","resolution":{"observed_at":"2026-08-14T05:28:09.108998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.07965","last_updated":"2018-03-21T15:28:55Z","snapshot_observed_at":"2026-07-06T06:29:30.274650Z","submitted_at":"2018-03-21T15:28:55Z","title":"High-resolution numerical relativity simulations of spinning binary neutron star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.07965","snapshot_observed_at":"2026-08-14T05:28:09.113603Z","title":"Dietrich, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.113603Z"},"links":{"cited_paper":"/paper/1803.07965","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:585993e44f8ff4c3fb5a9d6e31e76f49222ffcdf6127dd8cd9db5ac1adecbe01","observation_id":"b398260b-0266-43b5-8b0b-916024d975c8","resolution":{"observed_at":"2026-08-14T05:28:09.113603Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.09749","last_updated":"2018-08-29T12:13:53Z","snapshot_observed_at":"2026-07-06T06:58:05.236152Z","submitted_at":"2018-08-29T12:13:53Z","title":"Relevance of tidal effects and post-merger dynamics for binary neutron star parameter estimation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.09749","snapshot_observed_at":"2026-08-14T05:28:09.118044Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.118044Z"},"links":{"cited_paper":"/paper/1808.09749","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:1b9e19eac326d74de954e663497fcbfa1eaf199b036ac7eb1674649bcbdb4e3a","observation_id":"b8e25942-26f5-486e-9125-a25b0fe9dff9","resolution":{"observed_at":"2026-08-14T05:28:09.118044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.04877","last_updated":"2018-04-13T10:37:57Z","snapshot_observed_at":"2026-08-09T03:19:22.704783Z","submitted_at":"2018-04-13T10:37:57Z","title":"A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.04877","snapshot_observed_at":"2026-08-14T05:28:09.122628Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.122628Z"},"links":{"cited_paper":"/paper/1804.04877","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:12e34253ac754d5119de9b45cc1fb7adf6bcfd9722d53de15a7902effa36dddf","observation_id":"680e6191-e799-4ebd-bf20-1ef107f68894","resolution":{"observed_at":"2026-08-14T05:28:09.122628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00040","last_updated":"2017-12-27T17:40:14Z","snapshot_observed_at":"2026-07-06T06:07:05.119814Z","submitted_at":"2017-10-31T18:24:17Z","title":"Inferring the post-merger gravitational wave emission from binary neutron star coalescences","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00040","snapshot_observed_at":"2026-08-14T05:28:09.127394Z","title":"Chatziioannou, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.127394Z"},"links":{"cited_paper":"/paper/1711.00040","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:b8a1f4632176725432e5570572f81c1e46622305e2cf7be0734f186cfdf99b96","observation_id":"5c0380a0-61d7-432f-9575-f6a81ea49198","resolution":{"observed_at":"2026-08-14T05:28:09.127394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09381","last_updated":"2017-07-18T00:31:50Z","snapshot_observed_at":"2026-07-06T05:16:35.197394Z","submitted_at":"2016-10-28T20:00:05Z","title":"Kilonovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09381","snapshot_observed_at":"2026-08-14T05:28:09.132065Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.132065Z"},"links":{"cited_paper":"/paper/1610.09381","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:fb13e3a9d600470b12b79d323f7d4ee1ecc00b08d0d1ffdd341578a0f00f6e01","observation_id":"86a9ec6b-4d3e-4b8e-8ba1-3ed3906fcf36","resolution":{"observed_at":"2026-08-14T05:28:09.132065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.07235","last_updated":"2016-05-23T22:58:49Z","snapshot_observed_at":"2026-07-06T04:57:19.691523Z","submitted_at":"2016-05-23T22:58:49Z","title":"Kilonova/Macronova Emission from Compact Binary Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.07235","snapshot_observed_at":"2026-08-14T05:28:09.136547Z","title":"Tanaka, Adv","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.136547Z"},"links":{"cited_paper":"/paper/1605.07235","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:1fafd3b1f706233dd969270625e0803bd07b3fbf6c625906b87437a5dea6c818","observation_id":"b02e18af-3217-4776-a2e1-f8cc460db697","resolution":{"observed_at":"2026-08-14T05:28:09.136547Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-13T15:50:34.752283Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-08-14T05:28:09.141053Z","title":"Shibata, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.141053Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:63ba9ce0283d30abfefe226618db3f5e2a9b1c1a4c2d9f4266f60bf2b19bbe62","observation_id":"f5471b8b-1770-478b-b176-9190d3d69df5","resolution":{"observed_at":"2026-08-14T05:28:09.141053Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.11161","last_updated":"2019-05-30T18:58:04Z","snapshot_observed_at":"2026-07-06T07:04:59.871975Z","submitted_at":"2018-09-28T17:48:24Z","title":"Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts and Nucleosynthesis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.11161","snapshot_observed_at":"2026-08-14T05:28:09.145940Z","title":"Radice, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.145940Z"},"links":{"cited_paper":"/paper/1809.11161","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:b18fcdff7edd06f3932b0a9fc73668e377280342cafcd247e34235325c2a2803","observation_id":"46502f01-6c5e-4300-a7f2-f4057247309f","resolution":{"observed_at":"2026-08-14T05:28:09.145940Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.4323","last_updated":"2014-10-23T02:45:03Z","snapshot_observed_at":"2026-08-13T23:24:35.640198Z","submitted_at":"2014-10-16T08:00:34Z","title":"Axion Stars and Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.4323","snapshot_observed_at":"2026-08-14T05:28:09.150541Z","title":"Iwazaki, Phys","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.150541Z"},"links":{"cited_paper":"/paper/1410.4323","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:fc10d1398eff55b404cbda899e7152994258852c895eee7997910efb0e28385f","observation_id":"d252d173-c6f0-478f-a861-8841c22befb5","resolution":{"observed_at":"2026-08-14T05:28:09.150541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.10516","last_updated":"2017-09-29T17:52:57Z","snapshot_observed_at":"2026-07-06T06:02:02.014789Z","submitted_at":"2017-09-29T17:52:57Z","title":"Detecting Axion Stars with Radio Telescopes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.10516","snapshot_observed_at":"2026-08-14T05:28:09.155295Z","title":"Bai and Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.155295Z"},"links":{"cited_paper":"/paper/1709.10516","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:87eb67b17b7a12763abf3d9621631f4a13a974d6320d02a53be95f40120542b3","observation_id":"3af901ef-8473-4e6e-98c3-dda8c3dd64ed","resolution":{"observed_at":"2026-08-14T05:28:09.155295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.04746","last_updated":"2018-08-14T15:25:05Z","snapshot_observed_at":"2026-08-13T21:20:09.134854Z","submitted_at":"2018-08-14T15:25:05Z","title":"Neutron star -- axion star collisions in the light of multi-messenger astronomy","version":1},"cited_work":{"arxiv_id":"1808.04746","doi":null,"metadata_source":"pith","pith_arxiv_id":"1808.04746","snapshot_observed_at":"2026-08-14T05:28:09.222475Z","title":"Neutron star -- axion star collisions in the light of multi-messenger astronomy","venue":"astro-ph.HE","work_id":"823fc6fe-0a35-462d-930e-c85e9a8e3513","year":2018},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.160095Z"},"links":{"cited_paper":"/paper/1808.04746","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:a75a217bd216d413c63814e3589c11962f95b31f714ddf2fd5ec19518ad5da4c","observation_id":"7433a9eb-fe1f-4c73-8081-31d442121810","resolution":{"observed_at":"2026-08-14T05:28:09.229312Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10352","last_updated":"2020-03-24T17:32:24Z","snapshot_observed_at":"2026-08-14T10:43:48.975759Z","submitted_at":"2019-08-27T17:48:59Z","title":"Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.10352","snapshot_observed_at":"2026-08-14T05:28:09.164601Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.164601Z"},"links":{"cited_paper":"/paper/1908.10352","citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:b1d0a5dbe8131241bf4da6071c787c453a68f6184a63f304dc7e44532218202e","observation_id":"9b4c3c9b-7d12-4e0c-acd9-ceb19e1d7136","resolution":{"observed_at":"2026-08-14T05:28:09.164601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:28:10.571809Z","title":null,"venue":null,"work_id":"6a78a8fd-0b10-4248-ae90-31407715f4ed","year":null},"citing_paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-14T05:28:09.169393Z"},"links":{"citing_paper":"/paper/1909.01278"},"observation_digest":"sha256:76d51b6debd861610663e8a7d2f1cc9e2bd62632b7e8fb1a55ccc6cbaf9051b8","observation_id":"4ec7e091-360f-41d2-ae7b-082b2c08593c","resolution":{"observed_at":"2026-08-14T05:28:10.576338Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1909.01278","last_updated":"2019-09-03T16:19:23Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T06:05:42.423046Z","submitted_at":"2019-09-03T16:19:23Z","title":"Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung"},"reference_resolution":{"displayed":92,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":81,"verified_exact":5,"verified_fuzzy":6},"total_outbound_references":92},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 92 of 92 outbound references and 2 inbound Pith citation observations for arXiv:1909.01278."}