{"as_of":"2026-08-10T01:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c62c93d015e23b9b9e3f5bc67ead5de205b4995583f6bb8c7f72c3e8e24c89da","coverage":[{"denominator":110,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T04:46:13.740292Z","state":"measured"},{"denominator":103,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":103,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T04:46:12.248535Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-06T18:39:50.542934Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.03463","snapshot_observed_at":"2026-08-09T04:46:12.248535Z","title":"Similarly, using methods presented in Finstadet al.[57], Bandopadhyay et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.248535Z"},"links":{"cited_paper":"/paper/2502.03463","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:034505bce5b0cd67134303a7773a05912f49f243fc54f0485762c1769d7059f2","observation_id":"94914e99-5d21-4bdd-8f63-1e69a8888064","resolution":{"observed_at":"2026-08-09T04:46:12.248535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"cited_work":{"arxiv_id":"2502.03463","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.03463","snapshot_observed_at":"2026-08-06T18:39:50.542934Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","venue":"astro-ph.HE","work_id":"aa958a24-24db-4249-9df4-67d616cbed61","year":2025},"citing_paper":{"arxiv_id":"2507.07895","last_updated":"2025-07-10T16:24:17Z","snapshot_observed_at":"2026-08-09T15:59:51.124865Z","submitted_at":"2025-07-10T16:24:17Z","title":"A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T18:39:49.425707Z"},"links":{"cited_paper":"/paper/2502.03463","citing_paper":"/paper/2507.07895"},"observation_digest":"sha256:b11d3590e24ea10e41178299dcaaa24ac416fb3a68ba102ec05e180dfd7a9153","observation_id":"8ad4d401-1595-46b4-9711-5089a531310d","resolution":{"observed_at":"2026-08-06T18:39:50.619435Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.03463","snapshot_observed_at":"2026-07-31T07:22:45.812750Z","title":"Precise and accurate neutron star radius measurements with next-generation gravitational wave detectors","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28438","last_updated":"2026-07-30T16:13:33Z","snapshot_observed_at":"2026-08-03T00:12:06.425303Z","submitted_at":"2026-07-30T16:13:33Z","title":"Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology","version":1},"reference_index":137,"source":"arxiv_source","source_observed_at":"2026-07-31T07:22:45.812750Z"},"links":{"cited_paper":"/paper/2502.03463","citing_paper":"/paper/2607.28438"},"observation_digest":"sha256:cc0feaf0f686dffeb6cb02013a5bcea1e6a973fb5cc0c3e4619c0996b467b6c1","observation_id":"08a40043-155b-4aac-a7da-94ed044ed931","resolution":{"observed_at":"2026-07-31T07:22:45.812750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2502.03463/citation-record","integrity":"/paper/2502.03463/integrity","json":"/paper/2502.03463/citation-record.json","paper":"/paper/2502.03463"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1305.3510","last_updated":"2013-05-15T14:59:02Z","snapshot_observed_at":"2026-07-06T03:13:27.638618Z","submitted_at":"2013-05-15T14:59:02Z","title":"The Nuclear Equation of State and Neutron Star Masses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.3510","snapshot_observed_at":"2026-08-09T04:46:12.256887Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.256887Z"},"links":{"cited_paper":"/paper/1305.3510","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:f0afd8173fbf6cd0129dc8c7159ae9b7d0e8ddeb8fccec87b1ec090dca34a6a2","observation_id":"72fb6385-9981-4136-abed-323878f77e71","resolution":{"observed_at":"2026-08-09T04:46:12.256887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.07820","last_updated":"2015-12-24T14:09:54Z","snapshot_observed_at":"2026-07-06T04:41:02.094698Z","submitted_at":"2015-12-24T14:09:54Z","title":"The Equation of State of Hot, Dense Matter and Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.07820","snapshot_observed_at":"2026-08-09T04:46:12.261259Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.261259Z"},"links":{"cited_paper":"/paper/1512.07820","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:14baf93d203732cbef2aa005d453ad765a9de8e6c37f2dddcd689b40417670f7","observation_id":"2c12330b-197d-4548-a039-70d9e38b627b","resolution":{"observed_at":"2026-08-09T04:46:12.261259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02698","last_updated":"2016-03-08T21:05:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2016-03-08T21:05:49Z","title":"Masses, Radii, and Equation of State of Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02698","snapshot_observed_at":"2026-08-09T04:46:12.349078Z","title":"Özel and P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.349078Z"},"links":{"cited_paper":"/paper/1603.02698","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:63d5d4d5e51804f85a417e6bd3eef52dd589c970eee5fb54630aaf28c10769fc","observation_id":"15fd0045-df35-4c87-b95c-1b20807e0780","resolution":{"observed_at":"2026-08-09T04:46:12.349078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.01081","last_updated":"2016-02-02T20:56:45Z","snapshot_observed_at":"2026-07-06T04:44:55.350506Z","submitted_at":"2016-02-02T20:56:45Z","title":"Measuring the neutron star equation of state using X-ray timing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.01081","snapshot_observed_at":"2026-08-09T04:46:12.436561Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.436561Z"},"links":{"cited_paper":"/paper/1602.01081","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:708bdc685a4f93575fa43f53af78232f127c5dc38af9e4f53f192733ec6c63c9","observation_id":"b12659da-609b-4e3f-be92-18fedfa559d2","resolution":{"observed_at":"2026-08-09T04:46:12.436561Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.04966","last_updated":"2017-12-17T00:07:47Z","snapshot_observed_at":"2026-08-07T05:50:14.787661Z","submitted_at":"2017-07-17T00:23:41Z","title":"From hadrons to quarks in neutron stars: a review","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.04966","snapshot_observed_at":"2026-08-09T04:46:12.522817Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.522817Z"},"links":{"cited_paper":"/paper/1707.04966","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:d6977fb53f8d4f987238aa2fafe9912eb725cf8ba7e6b74ac22644df8685b1e7","observation_id":"7788d139-6e35-43a7-bcf3-711cfe775248","resolution":{"observed_at":"2026-08-09T04:46:12.522817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.03361","last_updated":"2016-10-11T14:29:10Z","snapshot_observed_at":"2026-07-06T05:14:11.208979Z","submitted_at":"2016-10-11T14:29:10Z","title":"Equations of state for supernovae and compact stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.03361","snapshot_observed_at":"2026-08-09T04:46:12.544936Z","title":"Oertel, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.544936Z"},"links":{"cited_paper":"/paper/1610.03361","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:1fe2e27806d134e99cd0eeee8d28fc386353a2b0d9287fbedf4aa0e562d9a05a","observation_id":"846dc623-ec28-432c-be90-3a41cd094694","resolution":{"observed_at":"2026-08-09T04:46:12.544936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.03050","last_updated":"2017-11-30T16:24:12Z","snapshot_observed_at":"2026-08-06T11:41:23.029803Z","submitted_at":"2016-12-09T15:09:32Z","title":"Rotating Stars in Relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.03050","snapshot_observed_at":"2026-08-09T04:46:12.548778Z","title":"Rel.20, 7 (2017), arXiv:1612.03050 [astro-ph.HE]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.548778Z"},"links":{"cited_paper":"/paper/1612.03050","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:94989baa548e5e6699cca493fa8ddaee71324526b0276234c09183465b43f328","observation_id":"b1a16309-6df4-410c-bafb-00ad03ea310f","resolution":{"observed_at":"2026-08-09T04:46:12.548778Z","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":"2026-08-09T04:46:12.552623Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.552623Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:15a0c1d0108f3e9d2d82f038ff976361c3c31056e81c2d8c546b8c593e4c6666","observation_id":"8077d8dc-944f-4a34-99bf-fd0b00b7612e","resolution":{"observed_at":"2026-08-09T04:46:12.552623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05705","last_updated":"2019-12-12T00:04:41Z","snapshot_observed_at":"2026-07-31T21:20:48.579404Z","submitted_at":"2019-12-12T00:04:41Z","title":"PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05705","snapshot_observed_at":"2026-08-09T04:46:12.555750Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.555750Z"},"links":{"cited_paper":"/paper/1912.05705","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:5212711832e47b23508939f608db70f6556dbe4ff7b02bbf6d00426a8ea286a0","observation_id":"30423196-8814-488c-ae1d-2d00a41cd08d","resolution":{"observed_at":"2026-08-09T04:46:12.555750Z","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":"2026-08-09T04:46:12.559263Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.559263Z"},"links":{"cited_paper":"/paper/2105.06979","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:521865e51efec71905612915a6788872cf82373eb47a3b27b56180989b3e5f01","observation_id":"3b020bf6-5eaa-4acb-8cce-01e75c53a658","resolution":{"observed_at":"2026-08-09T04:46:12.559263Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.11031","last_updated":"2020-04-17T13:55:45Z","snapshot_observed_at":"2026-07-06T08:46:37.972284Z","submitted_at":"2019-12-23T18:51:21Z","title":"Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.11031","snapshot_observed_at":"2026-08-09T04:46:12.562580Z","title":"Raaijmakers et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.562580Z"},"links":{"cited_paper":"/paper/1912.11031","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:ef0d53918fa0e7f68b5c0a4ed38229206f5090aedb9e13211222d43844343426","observation_id":"3954eae9-a76c-4b22-b7b0-020556c196ee","resolution":{"observed_at":"2026-08-09T04:46:12.562580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05703","last_updated":"2019-12-12T00:04:39Z","snapshot_observed_at":"2026-07-06T08:43:58.019943Z","submitted_at":"2019-12-12T00:04:39Z","title":"A NICER view of PSR J0030+0451: Implications for the dense matter equation of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05703","snapshot_observed_at":"2026-08-09T04:46:12.566176Z","title":"Raaijmakers et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.566176Z"},"links":{"cited_paper":"/paper/1912.05703","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:4dc510d3ae320c3b356922bf19c9da2a3552c92e07e91b8a0caf6af455bca18c","observation_id":"e34c6a75-1b04-47c4-a2ec-85060a0cf027","resolution":{"observed_at":"2026-08-09T04:46:12.566176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06981","last_updated":"2021-06-13T12:25:31Z","snapshot_observed_at":"2026-08-08T20:36:46.404172Z","submitted_at":"2021-05-14T17:33:34Z","title":"Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06981","snapshot_observed_at":"2026-08-09T04:46:12.570017Z","title":"Raaijmakers, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.570017Z"},"links":{"cited_paper":"/paper/2105.06981","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:434fed9a5dc8f822f3d7bfcc425b3c4a711b8fce34a1ece25a67336ff258e413","observation_id":"2892f338-a334-4f1e-8d8a-50f179b5035b","resolution":{"observed_at":"2026-08-09T04:46:12.570017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05706","last_updated":"2019-12-12T00:04:42Z","snapshot_observed_at":"2026-07-06T08:43:58.019943Z","submitted_at":"2019-12-12T00:04:42Z","title":"Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-ray Data Set","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05706","snapshot_observed_at":"2026-08-09T04:46:12.574638Z","title":"Bogdanov et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.574638Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:bc5ecb65bcfb8bfba5ac8df926bc22e699387d8d29a739d6721c7c22ded045ff","observation_id":"7cc6b4d3-c067-4292-b803-2ffb93d587a0","resolution":{"observed_at":"2026-08-09T04:46:12.574638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05707","last_updated":"2019-12-12T00:04:43Z","snapshot_observed_at":"2026-07-06T08:43:58.019943Z","submitted_at":"2019-12-12T00:04:43Z","title":"Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05707","snapshot_observed_at":"2026-08-09T04:46:12.579132Z","title":"Bogdanov et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.579132Z"},"links":{"cited_paper":"/paper/1912.05707","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:ea36e17ab37d30a15c50350c9e29b65bdce711cd1dab6a56e9837be6162dc046","observation_id":"48c0567d-1e3a-4efd-b25c-31641a87db67","resolution":{"observed_at":"2026-08-09T04:46:12.579132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.1762","last_updated":"2011-06-17T16:16:20Z","snapshot_observed_at":"2026-07-06T02:24:36.604135Z","submitted_at":"2011-03-09T11:41:27Z","title":"Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.1762","snapshot_observed_at":"2026-08-09T04:46:12.582748Z","title":"Roca-Maza, M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.582748Z"},"links":{"cited_paper":"/paper/1103.1762","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:9d03c241ddc222c957362f7cbbc4c88d99a66f2d7d3ad79af11c29408f281ea3","observation_id":"b7e07c47-5505-4ab8-a9d7-94670df3256d","resolution":{"observed_at":"2026-08-09T04:46:12.582748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06615","last_updated":"2017-12-15T08:37:25Z","snapshot_observed_at":"2026-08-04T22:10:42.743579Z","submitted_at":"2017-11-17T16:23:42Z","title":"Neutron skins and neutron stars in the multi-messenger era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.06615","snapshot_observed_at":"2026-08-09T04:46:12.604026Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.604026Z"},"links":{"cited_paper":"/paper/1711.06615","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:b3ee2c6a9cf6b19ace3fec570401daa8f850565026b7253c17f7fafd57c607ee","observation_id":"e5f6103c-2a2c-4f17-ae9f-e873474057f3","resolution":{"observed_at":"2026-08-09T04:46:12.604026Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.03193","last_updated":"2021-03-31T18:26:09Z","snapshot_observed_at":"2026-08-09T02:26:57.176739Z","submitted_at":"2021-01-08T19:28:16Z","title":"Implications of PREX-II on the equation of state of neutron-rich matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.03193","snapshot_observed_at":"2026-08-09T04:46:12.645635Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.645635Z"},"links":{"cited_paper":"/paper/2101.03193","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:4065d3b44ee8e5a0bb07ab7e85a832c9ed31e3f163ffd98baf259dc64a5eedc6","observation_id":"9ec3ffb6-188c-4638-b540-fde9339a3fab","resolution":{"observed_at":"2026-08-09T04:46:12.645635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-09T04:46:12.702738Z","title":"(LIGOScientific, Virgo),GW170817: Observation of Gravitational Waves from a Binary Neu- tron Star Inspiral, Phys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.702738Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:77bbfa6abdb6cc3510ecebee4a519f6db4a1cc0cd08ca6eceb251dac6ef75d0a","observation_id":"83175557-c5aa-4d08-b0c5-701371db26b3","resolution":{"observed_at":"2026-08-09T04:46:12.702738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.01761","last_updated":"2020-04-07T09:39:44Z","snapshot_observed_at":"2026-08-09T10:14:45.078058Z","submitted_at":"2020-01-06T19:54:55Z","title":"GW190425: Observation of a Compact Binary Coalescence with Total Mass $\\sim 3.4 M_{\\odot}$","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.01761","snapshot_observed_at":"2026-08-09T04:46:12.760092Z","title":"(LIGOScientific, Virgo),GW190425: Observation of a Compact Binary Coalescence with To- tal Mass ∼ 3.4M⊙, Astrophys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.760092Z"},"links":{"cited_paper":"/paper/2001.01761","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:3f4907d7ede4a45eb8ff81c70fe07223d8f7773fa4327b68f3ae3387f80292b8","observation_id":"5a80ff76-094f-4209-bcfb-587d6404752c","resolution":{"observed_at":"2026-08-09T04:46:12.760092Z","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":"2026-07-06T02:11:23.670680Z","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":"2026-08-09T04:46:12.780871Z","title":"Aasiet al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.780871Z"},"links":{"cited_paper":"/paper/1411.4547","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:81b2253af21dc8cc3a9a28916342ec5d52cef4e072387e31150041ed6318e371","observation_id":"9d76a389-49c1-4442-98ac-62c39cf90c12","resolution":{"observed_at":"2026-08-09T04:46:12.780871Z","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":"2026-07-06T02:11:23.670680Z","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":"2026-08-09T04:46:12.785313Z","title":"Acerneseet al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.785313Z"},"links":{"cited_paper":"/paper/1408.3978","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7cd45ca6178ca08430a47b8f6ac1672eb84e6ebf5038aa41672da07f6c9163e9","observation_id":"b0fdda48-6623-4085-87fb-8ef38b2bc5ad","resolution":{"observed_at":"2026-08-09T04:46:12.785313Z","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":"2026-08-09T04:46:12.789040Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.789040Z"},"links":{"cited_paper":"/paper/1710.05834","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:8eb8284c7102f05595b77f820e9955960bf616327defa62b7bd31b7c71bc0ea4","observation_id":"a2c7a51a-a590-47ac-bfee-af1c0c98c31a","resolution":{"observed_at":"2026-08-09T04:46:12.789040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03647","last_updated":"2017-12-24T17:36:18Z","snapshot_observed_at":"2026-07-06T06:08:41.171622Z","submitted_at":"2017-11-09T23:34:10Z","title":"GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03647","snapshot_observed_at":"2026-08-09T04:46:12.792119Z","title":"Radice, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.792119Z"},"links":{"cited_paper":"/paper/1711.03647","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:5e5591bd66293706376aa05ff79ee933ccb810dc102d643e7d452398419e495a","observation_id":"c2e79f92-db5e-431c-abdd-b8b92882c11a","resolution":{"observed_at":"2026-08-09T04:46:12.792119Z","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":"2026-07-06T07:20:42.045092Z","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":"2026-08-09T04:46:12.796171Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.796171Z"},"links":{"cited_paper":"/paper/1812.04803","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:1e1dbdc14ec222b241c9f6a0b0228b0ae6a1cc7db395be7de8b832752ec0eb14","observation_id":"95c0ff4f-9e5a-49ce-a30b-2d9b07f6f0e8","resolution":{"observed_at":"2026-08-09T04:46:12.796171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.10002","last_updated":"2019-04-22T18:00:09Z","snapshot_observed_at":"2026-07-06T07:47:38.383855Z","submitted_at":"2019-04-22T18:00:09Z","title":"Constraints on the Neutron Star Equation of State from GW170817","version":1},"cited_work":{"arxiv_id":"1904.10002","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.10002","snapshot_observed_at":"2026-08-09T04:46:14.892341Z","title":"Constraints on the Neutron Star Equation of State from GW170817","venue":"astro-ph.HE","work_id":"48e053a6-9749-4c54-b563-8bafddee5a80","year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.799219Z"},"links":{"cited_paper":"/paper/1904.10002","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:5e7d7099ba65aaa32e8eed83433a80dca2e65fc32d87f8701d0962708715d0bc","observation_id":"795a8436-09db-4ef7-9378-2bb60c458dc3","resolution":{"observed_at":"2026-08-09T04:46:14.983772Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10352","last_updated":"2020-03-24T17:32:24Z","snapshot_observed_at":"2026-08-10T00:46:34.433694Z","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":"2026-08-09T04:46:12.802529Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.802529Z"},"links":{"cited_paper":"/paper/1908.10352","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:f96afcc58afd56ad9c60da873fcf50dc3525ebc393c7c732715a4dc4ab8aa7d1","observation_id":"5c5dd4f4-27a7-4e27-876b-0451edab9ac5","resolution":{"observed_at":"2026-08-09T04:46:12.802529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.03750","last_updated":"2024-08-08T06:24:41Z","snapshot_observed_at":"2026-07-06T17:12:38.536345Z","submitted_at":"2024-01-08T09:21:34Z","title":"Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.03750","snapshot_observed_at":"2026-08-09T04:46:12.805696Z","title":"Breschi, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.805696Z"},"links":{"cited_paper":"/paper/2401.03750","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:9ef5518d2fea7067bca75d012e65ca2775c786060324a1b38d4f2fef27ad9dcb","observation_id":"edd49ba8-5eec-4894-85ab-0c4c0e257bf5","resolution":{"observed_at":"2026-08-09T04:46:12.805696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04172","last_updated":"2025-04-15T09:06:55Z","snapshot_observed_at":"2026-08-09T09:44:05.199128Z","submitted_at":"2024-02-06T17:27:09Z","title":"From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.04172","snapshot_observed_at":"2026-08-09T04:46:12.809078Z","title":"Koehn et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.809078Z"},"links":{"cited_paper":"/paper/2402.04172","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:c35e8eaf99e7d5dc9f3eac7977ec5a4af4bb190d57cd1c9b5e5ab6912940d4ab","observation_id":"a697d90f-1bf6-416b-aea0-6170079f8b00","resolution":{"observed_at":"2026-08-09T04:46:12.809078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.13485","last_updated":"2021-10-06T16:35:29Z","snapshot_observed_at":"2026-07-06T10:44:56.707503Z","submitted_at":"2021-02-26T15:25:39Z","title":"Bayesian analysis of multimessenger M-R data with interpolated hybrid EoS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.13485","snapshot_observed_at":"2026-08-09T04:46:12.812271Z","title":"Ayriyan, D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.812271Z"},"links":{"cited_paper":"/paper/2102.13485","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:ddc2fa6f6e0b2460152ea97c86f38633a3252f1ae4ec09418a6d3e2a88710fe6","observation_id":"19cd6d5c-382a-4041-b3ec-92836d01de00","resolution":{"observed_at":"2026-08-09T04:46:12.812271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.07744","last_updated":"2020-11-08T20:29:17Z","snapshot_observed_at":"2026-08-10T00:48:38.856384Z","submitted_at":"2020-04-16T16:29:02Z","title":"Direct Astrophysical Tests of Chiral Effective Field Theory at Supranuclear Densities","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.07744","snapshot_observed_at":"2026-08-09T04:46:12.815204Z","title":"Essick, I","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.815204Z"},"links":{"cited_paper":"/paper/2004.07744","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:32d995b43178498cfc146227c381eb2012715bae8148b741d775acfe17f9e703","observation_id":"3e7bebe5-e3be-490e-9325-3077d2e4f55a","resolution":{"observed_at":"2026-08-09T04:46:12.815204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.00562","last_updated":"2020-02-03T05:20:07Z","snapshot_observed_at":"2026-07-06T08:54:25.868963Z","submitted_at":"2020-02-03T05:20:07Z","title":"Effects of symmetry energy on the radius and tidal deformability of neutron stars in relativistic mean-field model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.00562","snapshot_observed_at":"2026-08-09T04:46:12.850987Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.850987Z"},"links":{"cited_paper":"/paper/2002.00562","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:14f2805e5d852ea9f6dcc13dfdceba2efafd59266c54f933fc6a96fb6202dbd4","observation_id":"31637bf7-8cdf-477f-9b97-56970487aba5","resolution":{"observed_at":"2026-08-09T04:46:12.850987Z","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":"2026-08-09T04:46:12.912596Z","title":"Akutsu et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.912596Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:bace93d7f216223d7f68407b40358585e92e1fe260c4d7f763cdb2e1d645de2e","observation_id":"dc9f1844-0f1f-4cd1-921c-b8a610124848","resolution":{"observed_at":"2026-08-09T04:46:12.912596Z","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":"2026-08-09T04:46:12.973784Z","title":"Barsotti, L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.973784Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7629801f13d9773e582e179b6b1019169d1d04b42c69874c94710d68fd2e8a00","observation_id":"ba60167b-9415-4e47-be5d-53f98b8b28a2","resolution":{"observed_at":"2026-08-09T04:46:12.973784Z","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":"2026-08-09T04:46:12.996230Z","title":"Fritschel, K","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.996230Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:9209141f05831637c31abf1dd9337c69b08ee2bc7146fa5002af4ae454ad6dca","observation_id":"27f6fe38-ce50-4225-82ca-d9ca9913a57f","resolution":{"observed_at":"2026-08-09T04:46:12.996230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04833","last_updated":"2019-07-10T17:27:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2019-07-10T17:27:49Z","title":"Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04833","snapshot_observed_at":"2026-08-09T04:46:12.999042Z","title":"Reitze et al., Cosmic Explorer: The U.S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.999042Z"},"links":{"cited_paper":"/paper/1907.04833","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:d0a60090715ba590982583507bfcd295de0ae0de0bac62e2bc5a27ed9b73fb37","observation_id":"c27a41cf-3151-4ce6-8b0c-7c90172def44","resolution":{"observed_at":"2026-08-09T04:46:12.999042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09882","last_updated":"2021-10-06T14:54:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-09-20T23:34:33Z","title":"A Horizon Study for Cosmic Explorer: Science, Observatories, and Community","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.09882","snapshot_observed_at":"2026-08-09T04:46:13.002815Z","title":"Evans et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.002815Z"},"links":{"cited_paper":"/paper/2109.09882","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:d0d7732ad3e3cc8f98458c74ef01d8ad6b39f701c87c97171d033a4c75da5831","observation_id":"4fd2eb73-6e91-4aad-85cb-3e4264f6bcf0","resolution":{"observed_at":"2026-08-09T04:46:13.002815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08697","last_updated":"2016-09-11T21:23:08Z","snapshot_observed_at":"2026-08-09T23:53:26.084975Z","submitted_at":"2016-07-29T06:37:47Z","title":"Exploring the Sensitivity of Next Generation Gravitational Wave Detectors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.08697","snapshot_observed_at":"2026-08-09T04:46:13.006122Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.006122Z"},"links":{"cited_paper":"/paper/1607.08697","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:0119cc30e5ac4e5260d63e19ed0f4bac7563d83f02fb159a8b958e7288a05cd6","observation_id":"cb066282-cff8-4f9b-9839-b29d46593cec","resolution":{"observed_at":"2026-08-09T04:46:13.006122Z","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":"2026-08-09T04:46:13.009725Z","title":"Punturo et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.009725Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:48ff8a665ade3d3a1cc66851d2300bc592f9e7df1f215a70a32d6192b66d36a1","observation_id":"1e939257-4458-4499-9e9c-9333104a569c","resolution":{"observed_at":"2026-08-09T04:46:13.009725Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.0908","last_updated":"2010-12-04T12:17:06Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2010-12-04T12:17:06Z","title":"Sensitivity Studies for Third-Generation Gravitational Wave Observatories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.0908","snapshot_observed_at":"2026-08-09T04:46:13.012507Z","title":"Hild et al., Sensitivity Studies for Third-Generation Gravitational Wave Observatories, Class","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.012507Z"},"links":{"cited_paper":"/paper/1012.0908","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:8c273aa3a198f8fa09c31d463244ac3e7edd77cef4b548e1ef7003d91ea8fcde","observation_id":"5ddc0d85-6040-4332-83f6-7ddc48726afd","resolution":{"observed_at":"2026-08-09T04:46:13.012507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.02622","last_updated":"2020-03-24T17:57:53Z","snapshot_observed_at":"2026-08-02T17:41:15.064781Z","submitted_at":"2019-12-05T14:57:00Z","title":"Science Case for the Einstein Telescope","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.02622","snapshot_observed_at":"2026-08-09T04:46:13.016217Z","title":"Maggiore et al","venue":null,"work_id":null,"year":1912},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.016217Z"},"links":{"cited_paper":"/paper/1912.02622","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:d15ab53d2104a5662792930d93b563c14e4cdca14f98f5ff7095574dbce9e35d","observation_id":"fd46db26-6140-4ebb-86e7-76030214b4c9","resolution":{"observed_at":"2026-08-09T04:46:13.016217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10421","last_updated":"2024-02-02T18:48:35Z","snapshot_observed_at":"2026-08-08T19:35:59.639506Z","submitted_at":"2023-07-19T19:15:11Z","title":"Characterizing Gravitational Wave Detector Networks: From A$^\\sharp$ to Cosmic Explorer","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10421","snapshot_observed_at":"2026-08-09T04:46:13.020960Z","title":"Guptaet al., Characterizing gravitational wave detec- tor networks: from A♯ to cosmic explorer, Class","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.020960Z"},"links":{"cited_paper":"/paper/2307.10421","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:106b0e782efbbed6e9f154bb4335934cca9c8be7c1775e6b0281eb5e391be156","observation_id":"d0b7a97c-a213-44ce-9aa2-ed271b6d587b","resolution":{"observed_at":"2026-08-09T04:46:13.020960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506681","last_updated":"2005-06-28T02:41:28Z","snapshot_observed_at":"2026-07-07T00:51:43.193510Z","submitted_at":"2005-06-28T02:41:28Z","title":"Probing the interior of neutron stars with gravitational waves","version":1},"cited_work":{"arxiv_id":"astro-ph/0506681","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0506681","snapshot_observed_at":"2026-08-09T04:46:14.602351Z","title":"Probing the interior of neutron stars with gravitational waves","venue":"astro-ph","work_id":"4ce1a7b7-1849-41e9-b17f-17a81e1b4bea","year":2005},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.024399Z"},"links":{"cited_paper":"/paper/astro-ph/0506681","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:f47130974e0eace25c47bcc1b3aa4a3b0a85a9df9379105b29725f32f562b811","observation_id":"06dfa5e2-0940-41cc-be0e-cbc216db0d1f","resolution":{"observed_at":"2026-08-09T04:46:14.606349Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.05405","last_updated":"2015-07-12T14:53:38Z","snapshot_observed_at":"2026-07-06T04:12:23.710098Z","submitted_at":"2015-03-18T13:39:55Z","title":"Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.05405","snapshot_observed_at":"2026-08-09T04:46:13.027185Z","title":"Agathos, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.027185Z"},"links":{"cited_paper":"/paper/1503.05405","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:0fa4bfa05fc9db37900b714a718892e24e6e3bc763dfbd8efaffdae360a40abb","observation_id":"13d29118-3db6-4ad7-bf40-661b7261ed10","resolution":{"observed_at":"2026-08-09T04:46:13.027185Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.8866","last_updated":"2014-10-31T19:53:25Z","snapshot_observed_at":"2026-07-06T03:59:12.341358Z","submitted_at":"2014-10-31T19:53:25Z","title":"Reconstructing the neutron-star equation of state with gravitational-wave detectors from a realistic population of inspiralling binary neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.8866","snapshot_observed_at":"2026-08-09T04:46:13.031434Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.031434Z"},"links":{"cited_paper":"/paper/1410.8866","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:90676b6f262499aa4963435c3f1f52f74504f64248ede7db53969cec828bccc1","observation_id":"74aa29ca-955b-45ca-ae3a-dbd4e12dfeb0","resolution":{"observed_at":"2026-08-09T04:46:13.031434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.02698","last_updated":"2020-05-26T03:55:07Z","snapshot_observed_at":"2026-08-09T21:19:51.464758Z","submitted_at":"2019-09-06T02:44:32Z","title":"Measuring the neutron star equation of state with gravitational waves: the first forty binary neutron star mergers","version":3},"cited_work":{"arxiv_id":"1909.02698","doi":null,"metadata_source":"pith","pith_arxiv_id":"1909.02698","snapshot_observed_at":"2026-08-09T04:46:14.569254Z","title":"Measuring the neutron star equation of state with gravitational waves: the first forty binary neutron star mergers","venue":"gr-qc","work_id":"88a3799c-e4bd-43a7-9a33-cc3478a2d2ab","year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.034445Z"},"links":{"cited_paper":"/paper/1909.02698","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:0149b2370f1cf2e6cfa68cd30b023091bbeb8d23a0cbb80cda4963d87e501930","observation_id":"d87c6760-29b0-4601-91f2-69b93317380b","resolution":{"observed_at":"2026-08-09T04:46:14.573218Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12529","last_updated":"2018-12-05T18:19:00Z","snapshot_observed_at":"2026-07-06T07:18:06.398264Z","submitted_at":"2018-11-29T23:05:21Z","title":"Non-parametric inference of the neutron star equation of state from gravitational wave observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12529","snapshot_observed_at":"2026-08-09T04:46:13.055424Z","title":"Landry and R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.055424Z"},"links":{"cited_paper":"/paper/1811.12529","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:dde5b882b703f9501e8a2e30f4524b07ee4b7faff43d9505ee11547520683a01","observation_id":"73f352ea-7a80-43b5-becb-556573c6a68c","resolution":{"observed_at":"2026-08-09T04:46:13.055424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.00482","last_updated":"2020-09-25T15:05:53Z","snapshot_observed_at":"2026-08-09T22:30:27.572561Z","submitted_at":"2020-05-01T16:50:58Z","title":"Inferring the maximum and minimum mass of merging neutron stars with gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.00482","snapshot_observed_at":"2026-08-09T04:46:13.113798Z","title":"Chatziioannou and W","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.113798Z"},"links":{"cited_paper":"/paper/2005.00482","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:a75bbf5fb7eec4c7093795bf846d55aa9d78872989a8119400fd901b6d65761a","observation_id":"904092f2-3286-4ac9-a317-ac126ed4ef4b","resolution":{"observed_at":"2026-08-09T04:46:13.113798Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.01747","last_updated":"2020-01-06T19:19:48Z","snapshot_observed_at":"2026-08-09T22:29:13.398010Z","submitted_at":"2020-01-06T19:19:48Z","title":"Inferring the neutron star equation of state simultaneously with the population of merging neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.01747","snapshot_observed_at":"2026-08-09T04:46:13.168402Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.168402Z"},"links":{"cited_paper":"/paper/2001.01747","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:22aa645241fee3e6606c875b5edd1fce931f9882f919eeada27b7d4a29f370fe","observation_id":"09a67515-9500-4ea6-88fc-f170a984af2b","resolution":{"observed_at":"2026-08-09T04:46:13.168402Z","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":"2026-08-09T04:46:12.253115Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.253115Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7306cc0cb2213b45e59d91940830320d21a65767c560cdbc09714e09d41c7b4d","observation_id":"f99f7099-3a82-48a9-b37a-0f56eefe77d5","resolution":{"observed_at":"2026-08-09T04:46:12.253115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.04880","last_updated":"2020-06-02T23:36:06Z","snapshot_observed_at":"2026-08-09T22:32:18.170083Z","submitted_at":"2020-03-10T17:50:27Z","title":"Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.04880","snapshot_observed_at":"2026-08-09T04:46:13.237544Z","title":"Landry, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.237544Z"},"links":{"cited_paper":"/paper/2003.04880","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:b835bf606c925dcd67ce28f90daaa8a7aac850dfe1f25863d49c1fee06215eb4","observation_id":"e7f9ea4b-d45a-4133-b758-3ec896062bdc","resolution":{"observed_at":"2026-08-09T04:46:13.237544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.15745","last_updated":"2021-12-14T21:33:19Z","snapshot_observed_at":"2026-08-04T08:35:17.367175Z","submitted_at":"2021-06-29T22:32:37Z","title":"Hierarchical Inference of Binary Neutron Star Mass Distribution and Equation of State with Gravitational Waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.15745","snapshot_observed_at":"2026-08-09T04:46:13.224116Z","title":"Golomb and C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.224116Z"},"links":{"cited_paper":"/paper/2106.15745","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:45522082bdd285742a7779d1b3644e8dde8f502a44e84044cf3ae82c52d736d6","observation_id":"04e3a077-622f-4ff0-807c-a31096d96bf0","resolution":{"observed_at":"2026-08-09T04:46:13.224116Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.08046","last_updated":"2023-10-29T21:50:10Z","snapshot_observed_at":"2026-07-06T15:16:23.984788Z","submitted_at":"2023-04-17T08:02:10Z","title":"Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.08046","snapshot_observed_at":"2026-08-09T04:46:13.245433Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.245433Z"},"links":{"cited_paper":"/paper/2304.08046","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:6532db56fb122dcf40b7f398fe0ce5f805c8227649b90af01131549ff10c2baf","observation_id":"fb58d3b3-08de-48ec-b00b-4f1b0fefb27b","resolution":{"observed_at":"2026-08-09T04:46:13.245433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.03463","snapshot_observed_at":"2026-08-09T04:46:12.248535Z","title":"Similarly, using methods presented in Finstadet al.[57], Bandopadhyay et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.248535Z"},"links":{"cited_paper":"/paper/2502.03463","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:034505bce5b0cd67134303a7773a05912f49f243fc54f0485762c1769d7059f2","observation_id":"94914e99-5d21-4bdd-8f63-1e69a8888064","resolution":{"observed_at":"2026-08-09T04:46:12.248535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.09740","last_updated":"2019-10-22T02:50:25Z","snapshot_observed_at":"2026-08-09T09:31:43.389159Z","submitted_at":"2019-10-22T02:50:25Z","title":"Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.09740","snapshot_observed_at":"2026-08-09T04:46:13.241056Z","title":"Essick, P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.241056Z"},"links":{"cited_paper":"/paper/1910.09740","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:dc064ea5118cf2f5095dbacfd0a0789a8232fa8f7251e3d6ba5da9b41d80b8a7","observation_id":"a396b3cf-c073-4e8b-8547-e0e5bb722227","resolution":{"observed_at":"2026-08-09T04:46:13.241056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.11756","last_updated":"2022-12-30T17:59:39Z","snapshot_observed_at":"2026-08-08T22:35:36.178264Z","submitted_at":"2022-03-22T14:16:20Z","title":"Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.11756","snapshot_observed_at":"2026-08-09T04:46:13.249178Z","title":"Ghosh, B","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.249178Z"},"links":{"cited_paper":"/paper/2203.11756","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:c3c6183af211b485a384e4451a6113ea5ca06a4809f0bab55b784bde94661fd5","observation_id":"39e3147d-ee59-4dd9-a6d8-6ec13582f8bc","resolution":{"observed_at":"2026-08-09T04:46:13.249178Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04626","last_updated":"2023-09-06T20:20:07Z","snapshot_observed_at":"2026-07-06T15:39:53.141172Z","submitted_at":"2023-06-07T17:54:24Z","title":"Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.04626","snapshot_observed_at":"2026-08-09T04:46:13.252845Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.252845Z"},"links":{"cited_paper":"/paper/2306.04626","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:99275a942bff94287cf85aefc81175f8116f37558d5c7ec232821c12c8c96e52","observation_id":"6d9eab2b-c20a-4a31-a738-7d0ce110a90a","resolution":{"observed_at":"2026-08-09T04:46:13.252845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.16561","last_updated":"2024-04-27T16:23:28Z","snapshot_observed_at":"2026-07-06T16:53:39.713988Z","submitted_at":"2023-11-28T07:02:53Z","title":"Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars","version":2},"cited_work":{"arxiv_id":"2311.16561","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.16561","snapshot_observed_at":"2026-08-09T04:46:14.332496Z","title":"Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars","venue":"gr-qc","work_id":"b9d4689e-2f51-4453-a6b7-cb8632f34ccf","year":2023},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.256184Z"},"links":{"cited_paper":"/paper/2311.16561","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:fbd8042f44c60a0999fc9e7d392f4c223653d337897a602f7445698bd763e373","observation_id":"f3f1d072-5830-4b29-9639-82613a140c47","resolution":{"observed_at":"2026-08-09T04:46:14.424989Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01396","last_updated":"2022-11-02T18:00:04Z","snapshot_observed_at":"2026-08-09T22:49:59.361309Z","submitted_at":"2022-11-02T18:00:04Z","title":"Prospects for a precise equation of state measurement from Advanced LIGO and Cosmic Explorer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.01396","snapshot_observed_at":"2026-08-09T04:46:13.259519Z","title":"Finstad, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.259519Z"},"links":{"cited_paper":"/paper/2211.01396","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:ae0e099e61fc1caa554a1fc5367e01f7343ad7ed2e1402999a5ae40dfc228cf0","observation_id":"8be73dbe-508e-467c-a92d-80f12752a8e6","resolution":{"observed_at":"2026-08-09T04:46:13.259519Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05056","last_updated":"2024-02-07T18:00:48Z","snapshot_observed_at":"2026-08-09T13:30:03.668907Z","submitted_at":"2024-02-07T18:00:48Z","title":"Measuring Neutron Star Radius with second and third generation Gravitational Wave Detector Networks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05056","snapshot_observed_at":"2026-08-09T04:46:13.262739Z","title":"Bandopadhyay, K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.262739Z"},"links":{"cited_paper":"/paper/2402.05056","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:6192c4834559462f5cb4e52f099f8031263723f4cda660128db4eb07704ce176","observation_id":"7ce8f80f-a51f-427b-8e3c-cfb97c0e27d2","resolution":{"observed_at":"2026-08-09T04:46:13.262739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.08583","last_updated":"2018-10-30T18:34:14Z","snapshot_observed_at":"2026-08-06T22:05:14.981103Z","submitted_at":"2018-04-23T17:22:22Z","title":"Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.08583","snapshot_observed_at":"2026-08-09T04:46:13.266124Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.266124Z"},"links":{"cited_paper":"/paper/1804.08583","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:8f9a4d4071ada23cdbde715f4b74a6362056765a945914e98538abf55600bf31","observation_id":"31bc3dd7-22bd-4df0-82fa-df879580f96c","resolution":{"observed_at":"2026-08-09T04:46:13.266124Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.05376","last_updated":"2024-03-26T16:35:38Z","snapshot_observed_at":"2026-07-06T15:52:40.672121Z","submitted_at":"2023-07-10T16:57:18Z","title":"The Accuracy of Neutron Star Radius Measurement with the Next Generation of Terrestrial Gravitational-Wave Observatories","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.05376","snapshot_observed_at":"2026-08-09T04:46:13.269600Z","title":"Huxford, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.269600Z"},"links":{"cited_paper":"/paper/2307.05376","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:99561709d283da053cddaafb53e85cb043ca8f6126c87316fe40fc233255002f","observation_id":"9ab53734-06b9-4d4a-9d70-fd6e5c4becfb","resolution":{"observed_at":"2026-08-09T04:46:13.269600Z","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":"2026-08-09T04:46:13.273205Z","title":"Walker, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.273205Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:a4005c793f02c3184eec99597557c6eb3e64314d1e63567be506079c8ba260c8","observation_id":"f0004940-e477-4d4d-8bec-b3fda2be9252","resolution":{"observed_at":"2026-08-09T04:46:13.273205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.0738","last_updated":"2010-10-21T16:50:45Z","snapshot_observed_at":"2026-08-05T08:41:03.979276Z","submitted_at":"2010-09-03T18:33:19Z","title":"Spectral Representations of Neutron-Star Equations of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.0738","snapshot_observed_at":"2026-08-09T04:46:13.276287Z","title":"Lindblom, Spectral Representations of Neutron-Star Equations of State, Phys","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.276287Z"},"links":{"cited_paper":"/paper/1009.0738","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7cc8babf03eec9450379d1cc92e0fbfd652202f3915e3f6823c85dc9fdbab95a","observation_id":"88b7d4ab-6ea3-4073-b8cf-fe9551f29156","resolution":{"observed_at":"2026-08-09T04:46:13.276287Z","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":"2026-08-07T22:20:24.299342Z","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":"2026-08-09T04:46:13.279453Z","title":"(LIGOScientific, Virgo),GW170817: Measurements of neutron star radii and equation of state, Phys","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.279453Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:81f44e8560cc646cab9a868edabceacc9155a203194572ab50b2418e90d4172c","observation_id":"080bc915-8dbc-470b-bc93-6fa4095bcee8","resolution":{"observed_at":"2026-08-09T04:46:13.279453Z","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":"2026-08-09T04:46:13.322335Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.322335Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:514edf835c43c8bbd87b7360036297121ea39684e72143efa1a35bfaf5e8fe5b","observation_id":"ec6ab1bb-49aa-42f7-b6db-c1391c68ac35","resolution":{"observed_at":"2026-08-09T04:46:13.322335Z","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":"2026-08-09T04:46:13.358431Z","title":"Futamase and Y","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.358431Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:754f2e781910e5e5edad6902cd1837f097aa5db233980523b6ad4abbb2ab94c6","observation_id":"ce4e46b0-2403-4353-a819-9bdbccc771e4","resolution":{"observed_at":"2026-08-09T04:46:13.358431Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.1528","last_updated":"2024-07-12T19:24:23Z","snapshot_observed_at":"2026-07-06T03:24:52.562608Z","submitted_at":"2013-10-06T02:23:37Z","title":"Post-Newtonian Theory for Gravitational Waves","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.1528","snapshot_observed_at":"2026-08-09T04:46:13.379715Z","title":"Blanchet, Post-Newtonian Theory for Gravitational Waves, Living Rev","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.379715Z"},"links":{"cited_paper":"/paper/1310.1528","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:849e961452b7de4d3e21e91656eb686b31302d1cd3b62b74a4541fd143817120","observation_id":"e7cf21c1-e38d-4d2d-8515-82ee0bc503ae","resolution":{"observed_at":"2026-08-09T04:46:13.379715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.04914","last_updated":"2016-05-15T17:36:03Z","snapshot_observed_at":"2026-08-08T23:38:42.344031Z","submitted_at":"2016-01-19T13:28:29Z","title":"The Effective Field Theorist's Approach to Gravitational Dynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.04914","snapshot_observed_at":"2026-08-09T04:46:13.412557Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.412557Z"},"links":{"cited_paper":"/paper/1601.04914","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:3561947996af4b6e3a493d23a8a870fa3f7814cfc7f744ed8d03356cf2effeb3","observation_id":"65446373-fea6-4ffa-bc6c-9dc25e3f4c1f","resolution":{"observed_at":"2026-08-09T04:46:13.412557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.01699","last_updated":"2020-06-18T12:54:21Z","snapshot_observed_at":"2026-07-06T06:48:23.889615Z","submitted_at":"2018-07-04T17:58:36Z","title":"Effective Field Theories of Post-Newtonian Gravity: A comprehensive review","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.01699","snapshot_observed_at":"2026-08-09T04:46:13.416412Z","title":"Levi, Effective Field Theories of Post-Newtonian Gravity: A comprehensive review, Rept","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.416412Z"},"links":{"cited_paper":"/paper/1807.01699","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:af868da04ecf82dfbc4e7b2644130275d23303344baf02e0cc7a77388f1ea912","observation_id":"342815a3-9fea-4c54-8c98-e4b7e15111aa","resolution":{"observed_at":"2026-08-09T04:46:13.416412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.2420","last_updated":"2009-03-07T02:10:36Z","snapshot_observed_at":"2026-08-03T22:44:29.548949Z","submitted_at":"2007-11-15T14:44:17Z","title":"Tidal Love numbers of neutron stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.2420","snapshot_observed_at":"2026-08-09T04:46:13.420099Z","title":"Hinderer, Tidal Love numbers of neutron stars, As- trophys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.420099Z"},"links":{"cited_paper":"/paper/0711.2420","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7df66eb25067b7314db3c98d7c791eb2744d3ed814a6fad9f64de85be1aa9481","observation_id":"8099b9e9-ffbb-4db1-85df-f259354bda1e","resolution":{"observed_at":"2026-08-09T04:46:13.420099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.1915","last_updated":"2007-12-07T21:22:23Z","snapshot_observed_at":"2026-07-06T01:33:47.610408Z","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":"2026-08-09T04:46:13.423797Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.423797Z"},"links":{"cited_paper":"/paper/0709.1915","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:588c6aaf732291f9a4c671ed0927a75221ba32ce44eff771b9d60b394e738c09","observation_id":"f453a69a-bfa6-4dad-99c7-bf8eac4b9c30","resolution":{"observed_at":"2026-08-09T04:46:13.423797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.1673","last_updated":"2011-01-09T20:36:19Z","snapshot_observed_at":"2026-07-06T02:21:47.279050Z","submitted_at":"2011-01-09T20:36:19Z","title":"Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.1673","snapshot_observed_at":"2026-08-09T04:46:13.427095Z","title":"Vines, E","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.427095Z"},"links":{"cited_paper":"/paper/1101.1673","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:1b9150cbfa57ced03c247a30c1a5d596cd9e52c326425c5fc6604d2e1fa8b37d","observation_id":"84a5d257-a22e-4734-a431-266d47be9f34","resolution":{"observed_at":"2026-08-09T04:46:13.427095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.5156","last_updated":"2014-02-20T21:57:24Z","snapshot_observed_at":"2026-07-06T03:36:34.006096Z","submitted_at":"2014-02-20T21:57:24Z","title":"Systematic and statistical errors in a bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.5156","snapshot_observed_at":"2026-08-09T04:46:13.430174Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.430174Z"},"links":{"cited_paper":"/paper/1402.5156","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:492e9645df5d85eaf547d89712304a101ae20e5c9f75762cf756cbd7d8453f96","observation_id":"e42a8dc1-8007-49cb-bf5f-e46eff0ac4a9","resolution":{"observed_at":"2026-08-09T04:46:13.430174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9811091","last_updated":"1998-11-26T20:44:21Z","snapshot_observed_at":"2026-07-07T03:29:43.892120Z","submitted_at":"1998-11-26T20:44:21Z","title":"Effective one-body approach to general relativistic two-body dynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9811091","snapshot_observed_at":"2026-08-09T04:46:13.433874Z","title":"Buonanno and T","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.433874Z"},"links":{"cited_paper":"/paper/gr-qc/9811091","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:35a955ce6153ff2cd8fd8b2afd7813a24470f6c45dbde29920b59b58575da62b","observation_id":"9a6228cb-a26a-42e9-8c1b-367c3a8739e9","resolution":{"observed_at":"2026-08-09T04:46:13.433874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0001013","last_updated":"2000-05-31T18:17:34Z","snapshot_observed_at":"2026-07-07T03:11:56.819046Z","submitted_at":"2000-01-07T00:04:14Z","title":"Transition from inspiral to plunge in binary black hole coalescences","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0001013","snapshot_observed_at":"2026-08-09T04:46:13.437381Z","title":"Buonanno and T","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.437381Z"},"links":{"cited_paper":"/paper/gr-qc/0001013","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:c6e3f097fe6102f01489d4a7a300f72ec3ff4a3c1ed9cd27fa017419a699a137","observation_id":"9887bb68-3a08-4943-984e-60d041ff347d","resolution":{"observed_at":"2026-08-09T04:46:13.437381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0103018","last_updated":"2001-10-01T14:35:29Z","snapshot_observed_at":"2026-07-07T03:13:50.798072Z","submitted_at":"2001-03-07T08:39:09Z","title":"Coalescence of Two Spinning Black Holes: An Effective One-Body Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0103018","snapshot_observed_at":"2026-08-09T04:46:13.440874Z","title":"Damour, Coalescence of two spinning black holes: an effective one-body approach, Phys","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.440874Z"},"links":{"cited_paper":"/paper/gr-qc/0103018","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:b8bb6550ef9921785fed0f729e96dba0ad55cd1ddaddf51d2cc521e0829caa51","observation_id":"e4d7402c-1a3d-4da3-92b9-a2d180cac40e","resolution":{"observed_at":"2026-08-09T04:46:13.440874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.2867","last_updated":"2011-06-08T20:13:06Z","snapshot_observed_at":"2026-07-06T01:57:39.890051Z","submitted_at":"2009-09-15T20:15:41Z","title":"Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.2867","snapshot_observed_at":"2026-08-09T04:46:13.444265Z","title":"Ajithet al., Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins, Phys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.444265Z"},"links":{"cited_paper":"/paper/0909.2867","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:8f480d6f97289438a34bd84c2db1c12f6439bb36a54617d3b7f233150dc714d0","observation_id":"e066c37e-b217-4007-97f3-2cbabef6b92f","resolution":{"observed_at":"2026-08-09T04:46:13.444265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.3306","last_updated":"2010-08-03T11:41:08Z","snapshot_observed_at":"2026-08-02T03:11:07.740286Z","submitted_at":"2010-05-18T20:00:07Z","title":"Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.3306","snapshot_observed_at":"2026-08-09T04:46:13.448189Z","title":"Santamaria et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.448189Z"},"links":{"cited_paper":"/paper/1005.3306","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:656ad6c11d78f188d7b14c857fc58fc28c15b542f7d47e3fe10f3b4ecf77067c","observation_id":"d6e780b5-ec7a-423b-800a-4022eb7d578a","resolution":{"observed_at":"2026-08-09T04:46:13.448189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.11412","last_updated":"2020-01-30T15:46:20Z","snapshot_observed_at":"2026-08-09T07:25:02.131923Z","submitted_at":"2020-01-30T15:46:20Z","title":"Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.11412","snapshot_observed_at":"2026-08-09T04:46:13.451617Z","title":"Pratten, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.451617Z"},"links":{"cited_paper":"/paper/2001.11412","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:6aec90514095ed017f48ef08c073c7953667abece1dce8c919bfcd5c79c21553","observation_id":"1b438435-a515-47de-8f00-6d17be664ae1","resolution":{"observed_at":"2026-08-09T04:46:13.451617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.02235","last_updated":"2018-04-06T12:37:24Z","snapshot_observed_at":"2026-07-06T06:32:05.310210Z","submitted_at":"2018-04-06T12:37:24Z","title":"Matter imprints in waveform models for neutron star binaries: tidal and self-spin effects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.02235","snapshot_observed_at":"2026-08-09T04:46:13.475789Z","title":"Dietrich et al., Matter imprints in waveform models for neutron star binaries: Tidal and self-spin effects, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.475789Z"},"links":{"cited_paper":"/paper/1804.02235","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7b6faec4ff4ec6e32e145405edfc05c53ad0cd88f17c088f58af95bc9288f1a9","observation_id":"973d3cb0-0786-4154-862d-23337fa091be","resolution":{"observed_at":"2026-08-09T04:46:13.475789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06011","last_updated":"2019-07-19T10:05:00Z","snapshot_observed_at":"2026-08-04T19:08:23.231514Z","submitted_at":"2019-05-15T08:05:10Z","title":"Improving the NRTidal model for binary neutron star systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06011","snapshot_observed_at":"2026-08-09T04:46:13.508739Z","title":"Dietrich, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.508739Z"},"links":{"cited_paper":"/paper/1905.06011","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7c78b2c41c978f2bca4685afefd7218c89992d80bf0b727c637b2beb8bf64528","observation_id":"0ace82b6-900d-4482-8daa-c6e47dbd8bb6","resolution":{"observed_at":"2026-08-09T04:46:13.508739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.07253","last_updated":"2015-09-25T12:59:37Z","snapshot_observed_at":"2026-07-06T04:28:02.506375Z","submitted_at":"2015-08-28T15:58:53Z","title":"Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.07253","snapshot_observed_at":"2026-08-09T04:46:13.560449Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.560449Z"},"links":{"cited_paper":"/paper/1508.07253","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:4d4f84944c171e611e575013acecd683a0735319624e5a65538cc5fe158f7af0","observation_id":"48cc3797-ea55-46e7-bd5f-3231fc2acb96","resolution":{"observed_at":"2026-08-09T04:46:13.560449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.07250","last_updated":"2015-09-25T12:57:10Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2015-08-28T15:55:43Z","title":"Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.07250","snapshot_observed_at":"2026-08-09T04:46:13.634217Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.634217Z"},"links":{"cited_paper":"/paper/1508.07250","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:dbd54eb0dba8acc8eed83e0b67f74147194a044f865963540d19ade7f1de741d","observation_id":"3342ab3d-8438-4af2-b43b-f941a4897b99","resolution":{"observed_at":"2026-08-09T04:46:13.634217Z","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":"2026-08-09T04:46:13.638150Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.638150Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:6ce86bd6146c84cd58978482233df38b2c12f2d17f0d7a87cee6b1f4821c94d5","observation_id":"697b2e5f-91e2-433a-b25d-ad05bca7d8ad","resolution":{"observed_at":"2026-08-09T04:46:13.638150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.00714","last_updated":"2021-06-07T05:14:37Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-06-01T04:46:19Z","title":"Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.00714","snapshot_observed_at":"2026-08-09T04:46:13.641755Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.641755Z"},"links":{"cited_paper":"/paper/2006.00714","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:8cf952ad9a1545f5ee58281d894c02b95a0575d12fc2de195f5ae134210906fd","observation_id":"79a02477-4adf-4c87-b417-102ab2ff7c34","resolution":{"observed_at":"2026-08-09T04:46:13.641755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.02042","last_updated":"2018-11-05T21:35:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-05T21:35:34Z","title":"Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.02042","snapshot_observed_at":"2026-08-09T04:46:13.645522Z","title":"Ashton et al., BILBY: A user-friendly Bayesian in- ference library for gravitational-wave astronomy, Astro- phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.645522Z"},"links":{"cited_paper":"/paper/1811.02042","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:c0ab5743b1d54f5796e89eb04af5b1fc396a3d3c0068a6b1b9dba171b8de708a","observation_id":"013dab42-5e9e-4c89-854e-e03f82ffb6bd","resolution":{"observed_at":"2026-08-09T04:46:13.645522Z","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":"2026-08-09T04:46:13.648723Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.648723Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:f279d64dc4b67500119488fb45c1d634e8dca9013fc5297e51e179b3b5cb607c","observation_id":"5ce47fda-94d2-4fcc-8ecf-0154373c6436","resolution":{"observed_at":"2026-08-09T04:46:13.648723Z","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":"2026-08-09T04:46:13.653079Z","title":"Wette, SWIGLAL: Python and Octave interfaces to the LALSuite gravitational-wave data analysis libraries, SoftwareX12, 100634 (2020)","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.653079Z"},"links":{"citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:fb4ee0f2ed6245568600771493bbaf7a06bb323bb80db0c3f1573def50c7f462","observation_id":"a2d1267a-6b86-496d-9b1d-d0ca731f71cf","resolution":{"observed_at":"2026-08-09T04:46:13.653079Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02180","last_updated":"2019-04-03T18:04:57Z","snapshot_observed_at":"2026-07-06T07:43:43.696691Z","submitted_at":"2019-04-03T18:04:57Z","title":"dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.02180","snapshot_observed_at":"2026-08-09T04:46:13.656189Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.656189Z"},"links":{"cited_paper":"/paper/1904.02180","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:9ffa67e1b134acac070199fe63512c4b836d442d9386644f11467f996b25549c","observation_id":"f77cd6e9-abab-4e39-810d-41ba351e8272","resolution":{"observed_at":"2026-08-09T04:46:13.656189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.4820","last_updated":"2013-02-06T19:53:45Z","snapshot_observed_at":"2026-08-04T01:07:34.569614Z","submitted_at":"2010-07-27T20:43:25Z","title":"Fast Fisher Matrices and Lazy Likelihoods","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.4820","snapshot_observed_at":"2026-08-09T04:46:13.659308Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.659308Z"},"links":{"cited_paper":"/paper/1007.4820","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7960372af281337fbd42874fc325c12c422da6f3f9c7bf16e7835d59fce72902","observation_id":"a20341f6-df82-478b-82d4-31a11c190398","resolution":{"observed_at":"2026-08-09T04:46:13.659308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.02728","last_updated":"2021-09-06T20:43:22Z","snapshot_observed_at":"2026-08-04T23:35:57.697911Z","submitted_at":"2021-09-06T20:43:22Z","title":"Heterodyned Likelihood for Rapid Gravitational Wave Parameter Inference","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.02728","snapshot_observed_at":"2026-08-09T04:46:13.662760Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.662760Z"},"links":{"cited_paper":"/paper/2109.02728","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:907113ed7867d4a0b8a4e23fa4e2e447650bbcbc09b18d9f3a420351f8a57258","observation_id":"c56b3692-b28a-44d5-898a-a72a1d3f5557","resolution":{"observed_at":"2026-08-09T04:46:13.662760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.08792","last_updated":"2018-08-02T14:08:27Z","snapshot_observed_at":"2026-08-02T02:50:47.767629Z","submitted_at":"2018-06-22T18:00:00Z","title":"Relative Binning and Fast Likelihood Evaluation for Gravitational Wave Parameter Estimation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.08792","snapshot_observed_at":"2026-08-09T04:46:13.666181Z","title":"Zackay, L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.666181Z"},"links":{"cited_paper":"/paper/1806.08792","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:7dbb21f610e6c8c649e8f80c5fdebe750d252fc8415ff1869ab78c4558a28741","observation_id":"64ead0eb-efb5-4285-90b4-6d98727383c4","resolution":{"observed_at":"2026-08-09T04:46:13.666181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06009","last_updated":"2023-12-10T21:48:52Z","snapshot_observed_at":"2026-08-06T18:57:41.135022Z","submitted_at":"2023-12-10T21:48:52Z","title":"Accelerated parameter estimation in Bilby with relative binning","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.06009","snapshot_observed_at":"2026-08-09T04:46:13.669930Z","title":"Krishna, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.669930Z"},"links":{"cited_paper":"/paper/2312.06009","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:2d637573e73fb40e5728aef98665e4ad7174f021ddf328c66f8ad1503824c900","observation_id":"e2041915-2768-4955-89cd-e399d70f3273","resolution":{"observed_at":"2026-08-09T04:46:13.669930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.0670","last_updated":"2020-11-24T20:19:46Z","snapshot_observed_at":"2026-07-30T08:36:04.718291Z","submitted_at":"2013-04-02T15:40:39Z","title":"Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA","version":11},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.0670","snapshot_observed_at":"2026-08-09T04:46:13.673438Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.673438Z"},"links":{"cited_paper":"/paper/1304.0670","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:c0ca093802be9931e0b9229e86e74c0c356faa53f2ea85cf55601561a9c32b67","observation_id":"7f30575e-b23c-446c-bda6-6065091c139c","resolution":{"observed_at":"2026-08-09T04:46:13.673438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06059","last_updated":"2015-10-16T15:18:01Z","snapshot_observed_at":"2026-07-06T04:33:44.933216Z","submitted_at":"2015-10-16T15:18:01Z","title":"IndIGO and LIGO-India: Scope and Plans for Gravitational Wave Research and Precision Metrology in India","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06059","snapshot_observed_at":"2026-08-09T04:46:13.677217Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.677217Z"},"links":{"cited_paper":"/paper/1510.06059","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:e6dc2582717542362f62262c65232b9171329c8d475719976b940b3dec0c7d51","observation_id":"618b0819-41a3-4c90-97a0-04f00787f647","resolution":{"observed_at":"2026-08-09T04:46:13.677217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.01716","last_updated":"2021-12-31T19:28:34Z","snapshot_observed_at":"2026-08-04T00:29:41.785513Z","submitted_at":"2021-05-04T19:15:26Z","title":"The Science Case for LIGO-India","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.01716","snapshot_observed_at":"2026-08-09T04:46:13.690083Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.690083Z"},"links":{"cited_paper":"/paper/2105.01716","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:28533e951e3edbd2298c1e9186b5bb6d5cafb8e5aa4617533575b1a449d26348","observation_id":"754c1564-e1e6-474e-b3ff-7fb38dc2ef48","resolution":{"observed_at":"2026-08-09T04:46:13.690083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.10349","last_updated":"2025-05-01T19:11:14Z","snapshot_observed_at":"2026-07-06T19:51:01.075884Z","submitted_at":"2024-11-15T16:51:17Z","title":"The Critical Role of LIGO-India in the Era of Next-Generation Observatories","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.10349","snapshot_observed_at":"2026-08-09T04:46:13.708425Z","title":"Pandey, I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.708425Z"},"links":{"cited_paper":"/paper/2411.10349","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:138ceef2a7f1e4795747aa7d6b7af28d02974781a61e31a84aeb5d7dc240029a","observation_id":"c64e3c2b-0624-4457-88e5-486a83debda8","resolution":{"observed_at":"2026-08-09T04:46:13.708425Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14533","last_updated":"2021-02-25T19:28:33Z","snapshot_observed_at":"2026-08-08T19:36:01.139819Z","submitted_at":"2020-10-27T18:05:06Z","title":"Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.14533","snapshot_observed_at":"2026-08-09T04:46:13.726828Z","title":"Abbott et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.726828Z"},"links":{"cited_paper":"/paper/2010.14533","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:004e9efb74fe2d70b9b7bae40d04107e442bffa8efae0cd28fcdc4eccebc889b","observation_id":"7e791080-68b4-4eb2-a0a2-94055fd2b822","resolution":{"observed_at":"2026-08-09T04:46:13.726828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.01665","last_updated":"2016-05-05T17:43:59Z","snapshot_observed_at":"2026-08-03T17:47:52.719584Z","submitted_at":"2016-05-05T17:43:59Z","title":"The millisecond pulsar mass distribution: Evidence for bimodality and constraints on the maximum neutron star mass","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.01665","snapshot_observed_at":"2026-08-09T04:46:13.740292Z","title":"Antoniadis, T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.740292Z"},"links":{"cited_paper":"/paper/1605.01665","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:60a91cefb90c9e37d2726e0eb610834b9742da31ec0417a4aa593079d80ac47d","observation_id":"6855c2f0-d343-4eb0-9f54-f27fc5506bfa","resolution":{"observed_at":"2026-08-09T04:46:13.740292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":96,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":110},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 110 outbound references and 3 inbound Pith citation observations for arXiv:2502.03463."}