{"as_of":"2026-08-16T16:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2d3cf9bd42fe8c993f91c2ec7cba02b074f279d9ed086b63c7e10db789367018","coverage":[{"denominator":60,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":60,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:44:03.697029Z","state":"measured"},{"denominator":61,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":61,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-22T09:20:09.976842Z","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":"2026-05-22T09:21:20.871654Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"cited_work":{"arxiv_id":"2504.19962","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.19962","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Approximating neutron-star radii us- ing gravitational-wave only measurements with sym- bolic regression","venue":null,"work_id":"edea5639-928b-46e0-930f-daed95ccaa7b","year":2025},"citing_paper":{"arxiv_id":"2605.21593","last_updated":"2026-05-20T18:00:05Z","snapshot_observed_at":"2026-08-01T21:26:03.431639Z","submitted_at":"2026-05-20T18:00:05Z","title":"Predicting intermediate-mass black hole formation in star clusters with machine learning","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-05-22T09:20:09.976842Z"},"links":{"cited_paper":"/paper/2504.19962","citing_paper":"/paper/2605.21593"},"observation_digest":"sha256:0ca14a641af75fd1c140412fd21fc95ed7808fd1bdc3ba0bef7e849649024798","observation_id":"881db6aa-6970-491a-99ae-e561c18cf812","resolution":{"observed_at":"2026-05-22T09:21:20.874418Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2504.19962/citation-record","integrity":"/paper/2504.19962/integrity","json":"/paper/2504.19962/citation-record.json","paper":"/paper/2504.19962"},"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":"2026-08-16T05:44:03.323010Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.323010Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:3dbd9f370135c697e673c940bd5518e92b65336e479c9a6cbe429e635c3c9948","observation_id":"7baf4264-65bf-4d6a-bbc0-e29cd6af5684","resolution":{"observed_at":"2026-08-16T05:44:03.323010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.4547","last_updated":"2014-11-17T16:55:23Z","snapshot_observed_at":"2026-08-12T13:34:30.122295Z","submitted_at":"2014-11-17T16:55:23Z","title":"Advanced LIGO","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.4547","snapshot_observed_at":"2026-08-16T05:44:03.330403Z","title":"Aasiet al., Advanced LIGO, Classical and Quantum Gravity32, 074001 (2015), arXiv:1411.4547 [gr-qc]","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.330403Z"},"links":{"cited_paper":"/paper/1411.4547","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:15037c576aef10f474c226ecfde2bd529fe2c9e3e4833eab8bcaadef0fb436b7","observation_id":"ab18049d-b04b-4dbe-a0e4-0bffa65efc66","resolution":{"observed_at":"2026-08-16T05:44:03.330403Z","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":"2026-08-16T05:44:05.121198Z","title":"mass limit 50 % 90 % LVC This work LVC This work 8 9 10 11 12 13 14 15 R, R [km] 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 Parametrized EOS, no max","venue":null,"work_id":"a3863a31-3cd9-4fca-a192-14abf7b1e673","year":2021},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.317176Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:fbc1331dbfc03fdaf47b82bf22a355f4b14a87e0c8f352a681b2eedbe02b972e","observation_id":"09bec610-7694-4af1-bc80-93d17a6fb80f","resolution":{"observed_at":"2026-08-16T05:44:05.127369Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05833","last_updated":"2017-10-24T12:03:18Z","snapshot_observed_at":"2026-08-15T08:46:24.571654Z","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":"2026-08-16T05:44:03.349228Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.349228Z"},"links":{"cited_paper":"/paper/1710.05833","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:ca62253f0ab6bd84e22d29fb310da7f011b2e2254d918d23aaa1e99f5871a4d6","observation_id":"a6b069e1-d320-465e-acf1-e0923e7e6c29","resolution":{"observed_at":"2026-08-16T05:44:03.349228Z","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":"2026-08-16T05:44:03.356629Z","title":"Haensel, A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.356629Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:5f960c47b574d67ddce5c6faae93847424e7b1896c3324c503c631e52101a846","observation_id":"459a313b-8ab3-41dd-a4c3-3025c1825899","resolution":{"observed_at":"2026-08-16T05:44:03.356629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3978","last_updated":"2014-10-16T13:24:29Z","snapshot_observed_at":"2026-08-12T13:34:29.588273Z","submitted_at":"2014-08-18T11:19:22Z","title":"Advanced Virgo: a 2nd generation interferometric gravitational wave detector","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3978","snapshot_observed_at":"2026-08-16T05:44:03.339068Z","title":"Acerneseet al., Advanced Virgo: a second-generation interferometric gravitational wave detector, Classical and Quantum Gravity32, 024001 (2015), arXiv:1408.3978 [gr-qc]","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.339068Z"},"links":{"cited_paper":"/paper/1408.3978","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:60fc35e8e9de73dbc995beaedc8a072a4ec21e46f0954436f9e2843827b31cbe","observation_id":"b099c4ae-d407-4b7c-b2f3-7de20197be81","resolution":{"observed_at":"2026-08-16T05:44:03.339068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06979","last_updated":"2021-05-14T17:33:32Z","snapshot_observed_at":"2026-08-08T20:42:33.884209Z","submitted_at":"2021-05-14T17:33:32Z","title":"The Radius of PSR J0740+6620 from NICER and XMM-Newton Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06979","snapshot_observed_at":"2026-08-16T05:44:03.369779Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.369779Z"},"links":{"cited_paper":"/paper/2105.06979","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:3298352b6d9dc5dc028103a7665aa03c241e806c21ee26fdc43306671b8728da","observation_id":"55914e04-9de5-4c8d-a396-10fa86f12579","resolution":{"observed_at":"2026-08-16T05:44:03.369779Z","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":"2026-08-16T05:44:05.067773Z","title":null,"venue":null,"work_id":"7b857c20-6f3a-47da-a539-68a85a8f7ba1","year":2012},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.376648Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:788184dea28a04096f0298791d12d5bf85c4e90b65ed4210d52a6b9316bf7512","observation_id":"2e62adaf-68ab-472e-a8cc-8235e0f19fbe","resolution":{"observed_at":"2026-08-16T05:44:05.073852Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:05.088509Z","title":"Andersson,Gravitational-Wave Astronomy: Explor- ing the Dark Side of the Universe(Oxford University Press, 2019)","venue":null,"work_id":"6e567021-3b1c-49c7-9606-c4b480309cf3","year":2019},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.363567Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:14a2146d4e57756a55d965365165589082b72ff5c34f18673281eb4817b12a66","observation_id":"8fb66ba6-d6e5-4183-9cc8-ad47fd2f046d","resolution":{"observed_at":"2026-08-16T05:44:05.094846Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.07687","last_updated":"2018-03-20T23:08:55Z","snapshot_observed_at":"2026-08-14T19:34:10.319128Z","submitted_at":"2018-03-20T23:08:55Z","title":"Tidal deformability from GW170817 as a direct probe of the neutron star radius","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.07687","snapshot_observed_at":"2026-08-16T05:44:03.389278Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.389278Z"},"links":{"cited_paper":"/paper/1803.07687","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:052695540e327dedb39decc7d8995fccb4541afb5ef5aa6ce49277a6b6f234cb","observation_id":"98bbaf20-cd53-401a-b872-ba92d561a726","resolution":{"observed_at":"2026-08-16T05:44:03.389278Z","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":"2026-08-16T05:44:05.015760Z","title":null,"venue":null,"work_id":"dbee02a0-b905-47c9-b438-907a46cecf3a","year":2018},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.396167Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:caebdaa57a8e8c43b60636d376bb96f181513a58d797c519b11411d6fbc55592","observation_id":"d2ca9192-9415-4051-9d14-28a9114e4458","resolution":{"observed_at":"2026-08-16T05:44:05.022499Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:05.035853Z","title":null,"venue":null,"work_id":"925c6d68-65d9-497f-9fa7-869637f092ea","year":2018},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.383434Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:d225f863d060fffc51483c5a3c6c986a32b8403734f57e5d73d968ef914c0b93","observation_id":"54f57631-1a17-4b3c-b55e-d7d036316a6f","resolution":{"observed_at":"2026-08-16T05:44:05.041977Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1528","last_updated":"2017-11-30T16:53:50Z","snapshot_observed_at":"2026-08-15T00:26:19.755098Z","submitted_at":"2013-03-06T21:00:03Z","title":"I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1528","snapshot_observed_at":"2026-08-16T05:44:03.409817Z","title":"Yagi and N","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.409817Z"},"links":{"cited_paper":"/paper/1303.1528","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:bbe447bbc1ab52765e49295d173204405870174a7f3af763d7360b5661364f72","observation_id":"d116d36f-a6d5-4093-ad43-445e92bde8cd","resolution":{"observed_at":"2026-08-16T05:44:03.409817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03221","last_updated":"2018-05-22T12:38:51Z","snapshot_observed_at":"2026-08-14T19:27:42.187440Z","submitted_at":"2018-04-09T20:25:47Z","title":"Measuring the neutron star tidal deformability with equation-of-state-independent relations and gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03221","snapshot_observed_at":"2026-08-16T05:44:03.416463Z","title":"Chatziioannou, C.-J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.416463Z"},"links":{"cited_paper":"/paper/1804.03221","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:1eb5062411decc88827ac5c46a413672aafac7167805037c589ef062a7db2924","observation_id":"eac12293-00f8-497c-bf65-14e7734d84e8","resolution":{"observed_at":"2026-08-16T05:44:03.416463Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.03168","last_updated":"2020-11-12T00:13:49Z","snapshot_observed_at":"2026-08-13T18:26:06.117457Z","submitted_at":"2020-06-04T23:23:02Z","title":"Neutron star tidal deformability and equation of state constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.03168","snapshot_observed_at":"2026-08-16T05:44:03.402739Z","title":"Chatziioannou, Neutron-star tidal deformability and equation-of-state constraints, General Relativity and Gravitation52, 109 (2020), arXiv:2006.03168 [gr-qc]","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.402739Z"},"links":{"cited_paper":"/paper/2006.03168","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:28ca0d45267ada86de2772a629007e4d9994f5755fa5a830f4206542c420de06","observation_id":"972f4aa6-2068-4c00-ac42-ef86f2a624f3","resolution":{"observed_at":"2026-08-16T05:44:03.402739Z","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":"2026-08-16T05:44:04.995817Z","title":"Fujimoto, K","venue":null,"work_id":"87c5a92b-fae1-4952-8d8e-8d4ba14c8d28","year":2020},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.429184Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:ada03cdf8c73e04f817b1119134b1d52120eed1c4aec9eccdd0a94580eced55b","observation_id":"9674b223-ce7d-42d9-94ed-27821f98927b","resolution":{"observed_at":"2026-08-16T05:44:05.002031Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.07194","last_updated":"2020-06-29T13:44:09Z","snapshot_observed_at":"2026-08-13T22:27:39.471158Z","submitted_at":"2020-06-11T13:04:47Z","title":"Neural networks reconstruction of the dense-matter equation of state from neutron-star parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.07194","snapshot_observed_at":"2026-08-16T05:44:03.436888Z","title":"Morawski and M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.436888Z"},"links":{"cited_paper":"/paper/2006.07194","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:514f5f15bd925c2d86bcaeee4050020447a761494a1da0d8845dd2861c68a02c","observation_id":"34705a73-2d91-4ce2-a1a3-f66e2b403e5e","resolution":{"observed_at":"2026-08-16T05:44:03.436888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04557","last_updated":"2019-03-12T07:21:48Z","snapshot_observed_at":"2026-08-14T17:17:21.561113Z","submitted_at":"2019-02-12T18:58:46Z","title":"Inferring neutron star properties from GW170817 with universal relations","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04557","snapshot_observed_at":"2026-08-16T05:44:03.422269Z","title":"Kumar and P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.422269Z"},"links":{"cited_paper":"/paper/1902.04557","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:3dc1f350d2bf325df3fc135ef4fbcd3ec5c6e41606c8eedf7cf0a38cb111f4c8","observation_id":"5cbd6ffe-a309-43ff-be03-7e6a75f1bdc9","resolution":{"observed_at":"2026-08-16T05:44:03.422269Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.07442","last_updated":"2024-02-12T00:19:51Z","snapshot_observed_at":"2026-08-16T15:34:19.990029Z","submitted_at":"2023-05-09T22:38:34Z","title":"Deducing Neutron Star Equation of State from Telescope Spectra with Machine-learning-derived Likelihoods","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.07442","snapshot_observed_at":"2026-08-16T05:44:03.449537Z","title":"Farrell, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.449537Z"},"links":{"cited_paper":"/paper/2305.07442","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:5eddaac406e04293827fa675a150338e6aef74f3002d6eda88496d0441ff9a4e","observation_id":"057053c7-a4ab-49e4-b07f-f70c2b104a0a","resolution":{"observed_at":"2026-08-16T05:44:03.449537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.11227","last_updated":"2024-04-17T14:59:50Z","snapshot_observed_at":"2026-08-16T14:59:09.813692Z","submitted_at":"2023-09-20T11:38:56Z","title":"Insights into neutron star equation of state by machine learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.11227","snapshot_observed_at":"2026-08-16T05:44:03.456643Z","title":"Guo, J.-Y","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.456643Z"},"links":{"cited_paper":"/paper/2309.11227","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:730240e06473820cfed4d432f7870cbfd26226307e0145fb2aab8675089c0ba5","observation_id":"b6bd956a-c7c4-45a8-8ca9-978d2250a4eb","resolution":{"observed_at":"2026-08-16T05:44:03.456643Z","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":"2026-08-16T05:44:04.977676Z","title":"Ferreira, V","venue":null,"work_id":"98c7e317-b4bb-424d-b4cd-effdf02d6843","year":2022},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.443541Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:96d9ed553fbb6b70d159ba37c2c64bc4f62b6a3efad0a17b95fb973db8572a54","observation_id":"93738a17-fc34-4191-b199-eea9f420fc10","resolution":{"observed_at":"2026-08-16T05:44:04.983219Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.03745","last_updated":"2020-05-11T07:33:42Z","snapshot_observed_at":"2026-08-15T01:21:39.016462Z","submitted_at":"2020-05-07T20:47:19Z","title":"Enhancing Gravitational-Wave Science with Machine Learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.03745","snapshot_observed_at":"2026-08-16T05:44:03.470815Z","title":"Cuoco, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.470815Z"},"links":{"cited_paper":"/paper/2005.03745","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:97082fb49adf69a7dc31939659a215bbd88be94fb48c06720192fb9821492f82","observation_id":"77d5ce0b-92e0-4aaa-b9aa-49f8156c561c","resolution":{"observed_at":"2026-08-16T05:44:03.470815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.07406","last_updated":"2024-01-15T00:51:43Z","snapshot_observed_at":"2026-08-16T14:27:35.838262Z","submitted_at":"2024-01-15T00:51:43Z","title":"Machine Learning Applications in Gravitational Wave Astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.07406","snapshot_observed_at":"2026-08-16T05:44:03.477918Z","title":"Stergioulas, Machine Learning Applications in Gravitational Wave Astronomy, arXiv e-prints , arXiv:2401.07406 (2024), arXiv:2401.07406 [gr-qc]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.477918Z"},"links":{"cited_paper":"/paper/2401.07406","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:e3cb5930ebd02928c2d9c92ee1a2c931842d25c226e4f5459f86ac7bc6840175","observation_id":"34f13d76-e410-4221-922a-de033e63e962","resolution":{"observed_at":"2026-08-16T05:44:03.477918Z","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":"2026-08-16T05:44:04.958143Z","title":"Ferreira and M","venue":null,"work_id":"c54c8bf4-3f06-4e15-b7f5-03e6b54fdc13","year":2025},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.463000Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:7d7fd538ee0c8f6ab0e8ed79ef734b473e5340dc87769a901f272d82a2783980","observation_id":"a802cedd-2585-4f22-9874-1bbdb4187874","resolution":{"observed_at":"2026-08-16T05:44:04.963789Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:03.492923Z","title":"Angelis, F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.492923Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:e6701e35445401f6220be3b63be90a907495601db6ada8bfc936ab6a1f052e21","observation_id":"d780f2d4-bb31-4705-83d5-eec433524f47","resolution":{"observed_at":"2026-08-16T05:44:03.492923Z","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":"2026-08-16T05:44:04.926591Z","title":"Tenachi, R","venue":null,"work_id":"ff8d056f-e1e2-45bb-82cf-a66d12eb878a","year":2023},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.499439Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:d2594cf78bc1ecef9c171a52e63ca51c3c589c7c080bdd95643f51489457cf35","observation_id":"aaa79685-feed-4830-b4b7-3e849a2c85ee","resolution":{"observed_at":"2026-08-16T05:44:04.932968Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.15046","last_updated":"2024-12-19T16:52:43Z","snapshot_observed_at":"2026-08-14T03:15:06.261898Z","submitted_at":"2024-12-19T16:52:43Z","title":"Applications of machine learning in gravitational wave research with current interferometric detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.15046","snapshot_observed_at":"2026-08-16T05:44:03.485056Z","title":"Cuoco, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.485056Z"},"links":{"cited_paper":"/paper/2412.15046","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:c00b6c3dc4ef1b71295009df636afee7cb2b2ab507908cd9a53e033bda620020","observation_id":"612dc7fb-8bb2-4c90-9f93-990f1ac34b7e","resolution":{"observed_at":"2026-08-16T05:44:03.485056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.12409","last_updated":"2022-07-25T18:00:00Z","snapshot_observed_at":"2026-08-13T14:57:29.101018Z","submitted_at":"2022-07-25T18:00:00Z","title":"Automated discovery of interpretable gravitational-wave population models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.12409","snapshot_observed_at":"2026-08-16T05:44:03.513088Z","title":"Wong and M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.513088Z"},"links":{"cited_paper":"/paper/2207.12409","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:0ad463737c646f2ff2cba212b2491878043aededbec2446b4c3d3aefc871454c","observation_id":"96a6f895-9c8e-4ecd-bffb-f96c9a6b00f8","resolution":{"observed_at":"2026-08-16T05:44:03.513088Z","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":"2026-08-16T05:44:04.885524Z","title":null,"venue":null,"work_id":"156e12c0-2d25-420e-8cad-15227a177774","year":2025},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.522062Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:7f090d525450b7121cc0ee377e80a3a00e0ec560c912e6766754a6c23589c41b","observation_id":"a0f1a88d-b95f-4225-b9a7-7c806bc40403","resolution":{"observed_at":"2026-08-16T05:44:04.891528Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:04.906105Z","title":"Saeed and C","venue":null,"work_id":"9b387f45-080f-44c9-9f34-31940b263764","year":2023},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.505905Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:d7d7783b37105efde2ae9980d6e4abdb9720fc25b430d3fc62aa1a86646c1c95","observation_id":"2bf5d87d-7984-4444-a102-e43cd618f7c3","resolution":{"observed_at":"2026-08-16T05:44:04.912739Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.20226","last_updated":"2025-04-16T03:12:30Z","snapshot_observed_at":"2026-08-16T12:54:35.387360Z","submitted_at":"2025-02-27T16:12:52Z","title":"Inferring the Equation of State from Neutron Star Observables via Machine Learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.20226","snapshot_observed_at":"2026-08-16T05:44:03.537112Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.537112Z"},"links":{"cited_paper":"/paper/2502.20226","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:f66ca564069c20fa78755bb4c22071384129e656b66ad4c6de17569ed3057349","observation_id":"0119a697-a64b-4e46-8e20-d77b8bc41a80","resolution":{"observed_at":"2026-08-16T05:44:03.537112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08553","last_updated":"2024-07-11T14:37:05Z","snapshot_observed_at":"2026-08-16T13:35:03.626185Z","submitted_at":"2024-07-11T14:37:05Z","title":"Calibrating global behaviour of equation of state by combining nuclear and astrophysics inputs in a machine learning approach","version":1},"cited_work":{"arxiv_id":"2407.08553","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.08553","snapshot_observed_at":"2026-08-16T05:44:04.228095Z","title":"Calibrating global behaviour of equation of state by combining nuclear and astrophysics inputs in a machine learning approach","venue":"nucl-th","work_id":"40001085-d4be-4a5f-8c66-b1fb1ab8fad8","year":2024},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.543415Z"},"links":{"cited_paper":"/paper/2407.08553","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:3f47725d3f2a3f8646367d8168c6128b58d118d3edaa786cda6d0b0caa34f9f5","observation_id":"ca907bfb-ecb1-4473-b0f2-40960f8d195c","resolution":{"observed_at":"2026-08-16T05:44:04.234605Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.18270","last_updated":"2025-09-12T08:35:18Z","snapshot_observed_at":"2026-08-16T10:18:05.817301Z","submitted_at":"2025-04-25T11:28:20Z","title":"Machine Learning-Based Analytical Expressions for Gray-Body Factors and Application to Primordial Black Holes","version":3},"cited_work":{"arxiv_id":"2504.18270","doi":null,"metadata_source":"pith","pith_arxiv_id":"2504.18270","snapshot_observed_at":"2026-08-16T05:44:04.275664Z","title":"Machine Learning-Based Analytical Expressions for Gray-Body Factors and Application to Primordial Black Holes","venue":"astro-ph.CO","work_id":"8ae820fc-2477-4feb-a2bc-7f466e124b62","year":2025},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.529521Z"},"links":{"cited_paper":"/paper/2504.18270","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:a611052c7ccd980d129209a10a937a9753fb92c471eafebe83706ce44f4ae355","observation_id":"006d53fc-45f7-4ebd-a348-33c968135edd","resolution":{"observed_at":"2026-08-16T05:44:04.282003Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:04.851092Z","title":null,"venue":null,"work_id":"3cc5b4f4-1dd8-4c48-890c-d133e967f61d","year":1939},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.556214Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:511ef36a600e6d92baa816c378deff37e7446284c04c3f86ed359243d897f968","observation_id":"b0dc1031-db50-4634-a715-bb786f01a9d8","resolution":{"observed_at":"2026-08-16T05:44:04.856389Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:04.832978Z","title":null,"venue":null,"work_id":"226959cc-3c85-408b-99b1-48a6815dba07","year":1911},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.562532Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:a3d602b0ee1df37e1ae4532fe66c57f120c19ad0bc52afbbc39136897cde43b7","observation_id":"9da6bba1-2895-4a12-850c-05344dc48166","resolution":{"observed_at":"2026-08-16T05:44:04.838480Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:03.549094Z","title":null,"venue":null,"work_id":null,"year":1939},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.549094Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:3fe354e711f67b51050b0ab1d5ec2fecea4dc4a95bcb6e2d317a2aa82f1202d3","observation_id":"a57f3718-6eac-497b-b04c-1f2209fad9de","resolution":{"observed_at":"2026-08-16T05:44:03.549094Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.03797","last_updated":"2017-05-03T18:52:26Z","snapshot_observed_at":"2026-08-14T21:21:15.796317Z","submitted_at":"2017-01-13T19:00:03Z","title":"Upper limit set by causality on the tidal deformability of a neutron star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.03797","snapshot_observed_at":"2026-08-16T05:44:03.573657Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.573657Z"},"links":{"cited_paper":"/paper/1701.03797","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:449ac44d9208dddc86aea2c0bf10deb0ee8e4a22885ac13557a7e4ad09f70d5d","observation_id":"963dd86c-7243-42a7-b7f9-6e5fc07ac6e8","resolution":{"observed_at":"2026-08-16T05:44:03.573657Z","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":"2026-08-16T05:44:05.159605Z","title":null,"venue":null,"work_id":"ba604a54-a67c-46e0-a227-9623e67379f4","year":null},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.302677Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:b219222d412229fb15ff5bf542fbf5d60d29025880795db2e52fadc033d8f800","observation_id":"774270a1-439a-43ea-bcd5-0fe35a7655a2","resolution":{"observed_at":"2026-08-16T05:44:05.165319Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0709.1915","last_updated":"2007-12-07T21:22:23Z","snapshot_observed_at":"2026-08-15T10:32:26.440510Z","submitted_at":"2007-09-12T15:46:16Z","title":"Constraining neutron star tidal Love numbers with gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.1915","snapshot_observed_at":"2026-08-16T05:44:03.568021Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.568021Z"},"links":{"cited_paper":"/paper/0709.1915","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:63e9f8589706ea47804b48ce12cd77e456b9ffd55de44e323e0caddf87bbb97c","observation_id":"20f17968-f395-448f-b266-20e85363e0bc","resolution":{"observed_at":"2026-08-16T05:44:03.568021Z","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":"2026-08-16T05:44:03.591451Z","title":"Bezanson, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.591451Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:1f764e8b968746f6bc60a450d0c4ef63a28559763e8b567467231bf111f507ca","observation_id":"456f6e50-1a51-4c10-96e7-4d0b41f64786","resolution":{"observed_at":"2026-08-16T05:44:03.591451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01582","last_updated":"2023-05-05T17:44:07Z","snapshot_observed_at":"2026-08-15T03:20:28.565133Z","submitted_at":"2023-05-02T16:31:35Z","title":"Interpretable Machine Learning for Science with PySR and SymbolicRegression.jl","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01582","snapshot_observed_at":"2026-08-16T05:44:03.579407Z","title":"Cranmer, Interpretable Machine Learning for Science with PySR and SymbolicRegression.jl, arXiv e-prints , arXiv:2305.01582 (2023), arXiv:2305.01582 [astro- ph.IM]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.579407Z"},"links":{"cited_paper":"/paper/2305.01582","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:d78de600c949efccb22e84e4f65afa9eba4af28839613d71d6591a7b28e355b7","observation_id":"d994e0a6-332f-44b0-b7d1-94ee42eb0689","resolution":{"observed_at":"2026-08-16T05:44:03.579407Z","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":"2026-08-16T05:44:04.814785Z","title":null,"venue":null,"work_id":"f43fd392-7df0-4c84-888e-d56b611db437","year":2025},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.585023Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:98ef8ebd6bb5b7daee5f61754698239e1ecabd7e9d3d1475e51e549a07c4cd88","observation_id":"d7f8c8e8-1982-4f04-82bd-a13cefaa3462","resolution":{"observed_at":"2026-08-16T05:44:04.820432Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-08-16T05:44:03.614373Z","title":"Douchin and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.614373Z"},"links":{"cited_paper":"/paper/astro-ph/0111092","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:e52e2abc53f88accb47a0e292a53c627d06059c381a790bd3a0f986ee232eaab","observation_id":"51b26ff3-701f-410a-8d0e-4824e09c371b","resolution":{"observed_at":"2026-08-16T05:44:03.614373Z","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":"2026-08-16T05:44:04.795290Z","title":null,"venue":null,"work_id":"8eeac1f7-cbb3-444a-8875-9ae1c395e4b3","year":2005},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.599047Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:08485786d7bbe8d5aba88936c7ccd967414e46a4fc82aabcf38329c8f876b7b6","observation_id":"aed8e008-bbcb-4294-80b0-e0bc61bc329f","resolution":{"observed_at":"2026-08-16T05:44:04.801263Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:04.776740Z","title":null,"venue":null,"work_id":"319cebc8-84d8-4065-8956-f2782bde589d","year":1965},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.605409Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:54ab2858d487c96633db84dfdf9fa6bef1eb292ddb5d9ad17bdd989678bbcdaa","observation_id":"0dcef3c9-66dc-4364-a96f-67d8dcdb560d","resolution":{"observed_at":"2026-08-16T05:44:04.782694Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:03.631796Z","title":"Akmal, V","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.631796Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:8ef25ecdf77d3ca5d318f1dcd241ed940c9536ce60fc7dae9c584699afef5a17","observation_id":"f18e5d21-944f-474b-990b-a45d0cc042e6","resolution":{"observed_at":"2026-08-16T05:44:03.631796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/9310003","last_updated":"1993-10-04T16:06:30Z","snapshot_observed_at":"2026-08-15T00:01:09.730887Z","submitted_at":"1993-10-04T16:06:30Z","title":"Experimental Nuclear Masses and the Ground State of Cold Dense Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-th/9310003","snapshot_observed_at":"2026-08-16T05:44:03.620613Z","title":"Haensel and B","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.620613Z"},"links":{"cited_paper":"/paper/nucl-th/9310003","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:eba2c808dcdc8534912242a8f22100477533700771fd9dfea497a349ef215be3","observation_id":"50bc1734-913d-4e63-bf5b-2bccabc6c4a3","resolution":{"observed_at":"2026-08-16T05:44:03.620613Z","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":"2026-08-16T05:44:03.626353Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.626353Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:179b3f1c53692688c9a9aaea5a0cec4358cb5ad14562409bef19c51bc098cd66","observation_id":"4fa441a5-04ec-4f39-8116-4cf834ddfa69","resolution":{"observed_at":"2026-08-16T05:44:03.626353Z","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":"2026-08-16T05:44:04.744032Z","title":null,"venue":null,"work_id":"31f50d61-b7bb-4b8f-904c-89f52f689704","year":1997},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.648951Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:80101c9d95e68a7c47e9815fd78b9fabb7d643854b32dee6c33f789cc5ac63d1","observation_id":"3ba50fe6-f3ac-41cc-9be9-0e6aed86ceaf","resolution":{"observed_at":"2026-08-16T05:44:04.750361Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1009.3840","last_updated":"2010-09-20T14:50:00Z","snapshot_observed_at":"2026-08-15T05:08:20.250325Z","submitted_at":"2010-09-20T14:50:00Z","title":"Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.3840","snapshot_observed_at":"2026-08-16T05:44:03.637167Z","title":"Goriely, N","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.637167Z"},"links":{"cited_paper":"/paper/1009.3840","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:f96db517910d5d78cfd23ad95c346cd2cbacea2c6009835bb33838b888d8aef3","observation_id":"f290dd41-a267-44bd-bd80-a5c933f875f0","resolution":{"observed_at":"2026-08-16T05:44:03.637167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-15T04:27:23.949454Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-08-16T05:44:03.643237Z","title":"Bednarek, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.643237Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:9a3e4e6caf2ccdb79a0002a9884a3d9f79e16d406ef73551df3e7bf2ffb1e100","observation_id":"539ff4ae-df47-4da5-bf31-75f9dcdfcdbf","resolution":{"observed_at":"2026-08-16T05:44:03.643237Z","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":"2026-08-16T05:44:05.140483Z","title":"3 presented the recovered radii for both BNS components, using various assumptions about the EOS; see LIGO-P1800115 for the data behind the figure","venue":null,"work_id":"f275f5e7-0bb7-4e3b-b7cf-f222c885ba78","year":null},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.310980Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:4992a55e4c526931d7ac1a5a5f7d9376dc972f7616ebfd47abafcc5341947f82","observation_id":"560994c0-82a7-44c8-a968-0beb98f7964f","resolution":{"observed_at":"2026-08-16T05:44:05.146219Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1209.6160","last_updated":"2012-09-27T08:44:30Z","snapshot_observed_at":"2026-08-15T00:45:11.914723Z","submitted_at":"2012-09-27T08:44:30Z","title":"Existence of hyperons in the pulsar PSRJ1614-2230","version":1},"cited_work":{"arxiv_id":"1209.6160","doi":null,"metadata_source":"pith","pith_arxiv_id":"1209.6160","snapshot_observed_at":"2026-08-16T05:44:03.777224Z","title":"Existence of hyperons in the pulsar PSRJ1614-2230","venue":"nucl-th","work_id":"f456b085-cb1e-4689-a61c-5112c31d0a9d","year":2012},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.654439Z"},"links":{"cited_paper":"/paper/1209.6160","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:2f4ddcd0bc82c8b60cf7db2e7f8d06f2e69a58b499766c96897aa6fae9c0b5b2","observation_id":"250bb98c-db91-4acb-ae5b-2ccc31f6fbce","resolution":{"observed_at":"2026-08-16T05:44:03.900062Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:04.724909Z","title":null,"venue":null,"work_id":"e2a73698-d898-4803-8bfe-0f3e543f22df","year":1971},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.662370Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:232aaaf2bd8613dc6246d894b58b44d2826020dde90b2c2acdfc65a2d3843244","observation_id":"ed8107da-d444-4061-8888-12e46a8abd4e","resolution":{"observed_at":"2026-08-16T05:44:04.730450Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11581","last_updated":"2018-10-15T17:59:04Z","snapshot_observed_at":"2026-08-14T19:09:49.769515Z","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":"2026-08-16T05:44:03.667992Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.667992Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:3bcbfb8182923af609a776b34e5dbae9fbedd006a935df6922f73baa993f6b4e","observation_id":"469d610b-79b7-461f-9544-d1d5c2494972","resolution":{"observed_at":"2026-08-16T05:44:03.667992Z","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":"2026-08-16T05:44:04.703934Z","title":null,"venue":null,"work_id":"6dac4802-9071-438b-91a5-c3f9568d5778","year":2018},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.674082Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:1f172e4b935d76bf9df00153afbda5c7b692ac5a0bc998aab6d95df0052fe554","observation_id":"7e138319-be85-4c3a-8400-96022daab632","resolution":{"observed_at":"2026-08-16T05:44:04.711521Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:03.679037Z","title":"Virtanen, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.679037Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:fabbbf839ab2c320ce40da19b544e6b0bd815d22ad29c51fa653c6c38a6f2059","observation_id":"3060d140-83f6-4b57-9fb9-98bd600e22b8","resolution":{"observed_at":"2026-08-16T05:44:03.679037Z","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":"2026-08-16T05:44:04.669500Z","title":null,"venue":null,"work_id":"5661a414-a2fd-46f1-97a2-bc2469ff44d4","year":null},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.684612Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:1fb2496b3efea29b4ce4db284b76db0f8e47a0b635400e397362e15b3ac6f199","observation_id":"2f5cab51-e461-4814-8b8f-e6fd90b33f7b","resolution":{"observed_at":"2026-08-16T05:44:04.675132Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:04.649906Z","title":"Akiba, S","venue":null,"work_id":"c03a079b-9ec9-42a2-b42d-1d65ef51261e","year":2019},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.691553Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:93fd8a6b0ec2a9b64ebc805c52df8b22b7fba49fdb9b36a386269d1b0d2344b6","observation_id":"79fec894-86f8-4877-9561-21e97e83b036","resolution":{"observed_at":"2026-08-16T05:44:04.655913Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-16T05:44:04.628916Z","title":null,"venue":null,"work_id":"340513eb-d750-4ebe-8bcf-5b6adce67100","year":2025},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.697029Z"},"links":{"citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:8fd903ce09123a949e35b0a73afda821d59faaa5246050bdaf226c28c03ff610","observation_id":"8fb73563-9a3b-4f30-975d-78f1b0dcfd5a","resolution":{"observed_at":"2026-08-16T05:44:04.635325Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T05:36:35.722533Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression"},"reference_resolution":{"displayed":60,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":48,"verified_exact":3,"verified_fuzzy":8},"total_outbound_references":60},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 60 of 60 outbound references and 1 inbound Pith citation observation for arXiv:2504.19962."}