{"as_of":"2026-08-16T22:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:28753c83a36cc6107209e32f8b5d94d9abf8c1239cb10fae6b4e11e86922767e","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-31T07:22:45.666157Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-18T08:51:08.638216Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1902.03300","last_updated":"2019-12-12T04:16:15Z","snapshot_observed_at":"2026-08-16T10:33:32.649038Z","submitted_at":"2019-02-08T21:51:51Z","title":"The mass distribution of Galactic double neutron stars","version":4},"cited_work":{"arxiv_id":"1902.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.03300","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J.87618 (Preprint1902.03300)","venue":null,"work_id":"d7b29933-8e80-4eee-bfd7-0e2b710e9534","year":2019},"citing_paper":{"arxiv_id":"2010.14527","last_updated":"2021-03-08T18:36:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-10-27T18:01:31Z","title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","version":3},"reference_index":269,"source":"pdf_text","source_observed_at":"2026-05-13T13:21:02.413921Z"},"links":{"cited_paper":"/paper/1902.03300","citing_paper":"/paper/2010.14527"},"observation_digest":"sha256:06af15218cafcc9eeba227934f4dccacf7c846f2d136e5a2fbbd4c06d3ff044e","observation_id":"323eb39f-0cad-4631-84d3-4a6868d30390","resolution":{"observed_at":"2026-05-13T13:21:02.772839Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.03300","last_updated":"2019-12-12T04:16:15Z","snapshot_observed_at":"2026-08-16T10:33:32.649038Z","submitted_at":"2019-02-08T21:51:51Z","title":"The mass distribution of Galactic double neutron stars","version":4},"cited_work":{"arxiv_id":"1902.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.03300","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J.87618 (Preprint1902.03300)","venue":null,"work_id":"d7b29933-8e80-4eee-bfd7-0e2b710e9534","year":2019},"citing_paper":{"arxiv_id":"2510.05400","last_updated":"2026-05-12T18:57:13Z","snapshot_observed_at":"2026-08-08T20:19:36.745595Z","submitted_at":"2025-10-06T21:46:05Z","title":"Binary Neutron Stars from the Moon: Early Warnings and Precision Science for the Artemis Era","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-18T08:50:34.604521Z"},"links":{"cited_paper":"/paper/1902.03300","citing_paper":"/paper/2510.05400"},"observation_digest":"sha256:a24990b75512028959f25578dc550cd52ff6afe44ae4273a7eaec96261507233","observation_id":"5510a318-0d24-42b6-9dd9-17e2bf1efd23","resolution":{"observed_at":"2026-05-18T08:51:08.641104Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.03300","last_updated":"2019-12-12T04:16:15Z","snapshot_observed_at":"2026-08-16T10:33:32.649038Z","submitted_at":"2019-02-08T21:51:51Z","title":"The mass distribution of Galactic double neutron stars","version":4},"cited_work":{"arxiv_id":"1902.03300","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.03300","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J.87618 (Preprint1902.03300)","venue":null,"work_id":"d7b29933-8e80-4eee-bfd7-0e2b710e9534","year":2019},"citing_paper":{"arxiv_id":"2510.22137","last_updated":"2026-04-17T07:23:37Z","snapshot_observed_at":"2026-08-13T16:08:34.546938Z","submitted_at":"2025-10-25T03:18:25Z","title":"Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-05-18T05:03:14.790179Z"},"links":{"cited_paper":"/paper/1902.03300","citing_paper":"/paper/2510.22137"},"observation_digest":"sha256:7e8e544885b7cf1caefd591f84234afcd3774c1c6dfd6792261d3716c8205fd9","observation_id":"0d7b1063-54fa-43eb-a883-971fe344bb34","resolution":{"observed_at":"2026-05-18T05:05:55.058217Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.03300","last_updated":"2019-12-12T04:16:15Z","snapshot_observed_at":"2026-08-16T10:33:32.649038Z","submitted_at":"2019-02-08T21:51:51Z","title":"The mass distribution of Galactic double neutron stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.03300","snapshot_observed_at":"2026-07-12T05:14:58.841553Z","title":", keywords =","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2607.03045","last_updated":"2026-07-03T07:34:46Z","snapshot_observed_at":"2026-08-13T11:34:49.188005Z","submitted_at":"2026-07-03T07:34:46Z","title":"nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-07-12T05:14:58.841553Z"},"links":{"cited_paper":"/paper/1902.03300","citing_paper":"/paper/2607.03045"},"observation_digest":"sha256:c97e538a9413bac6e8005029a1d0a844766b18b0d15c40298666e29c0787f368","observation_id":"64bb7cc3-43a2-4727-8c38-2bd394ba8568","resolution":{"observed_at":"2026-07-12T05:14:58.841553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.03300","last_updated":"2019-12-12T04:16:15Z","snapshot_observed_at":"2026-08-16T10:33:32.649038Z","submitted_at":"2019-02-08T21:51:51Z","title":"The mass distribution of Galactic double neutron stars","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.03300","snapshot_observed_at":"2026-07-31T07:22:45.666157Z","title":"The mass distribution of Galactic double neutron stars","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.28438","last_updated":"2026-07-30T16:13:33Z","snapshot_observed_at":"2026-08-13T12:07:24.939195Z","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":89,"source":"arxiv_source","source_observed_at":"2026-07-31T07:22:45.666157Z"},"links":{"cited_paper":"/paper/1902.03300","citing_paper":"/paper/2607.28438"},"observation_digest":"sha256:4e8dcf41d29f8e28a976db47eb2a140de21d913be41ac61f5dec284142dd3e88","observation_id":"9e9bf484-b20b-4047-8a70-93f6954e7097","resolution":{"observed_at":"2026-07-31T07:22:45.666157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1902.03300/citation-record","integrity":"/paper/1902.03300/integrity","json":"/paper/1902.03300/citation-record.json","paper":"/paper/1902.03300"},"outbound":[],"paper":{"arxiv_id":"1902.03300","last_updated":"2019-12-12T04:16:15Z","latest_version":4,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T10:33:32.649038Z","submitted_at":"2019-02-08T21:51:51Z","title":"The mass distribution of Galactic double neutron stars"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1902.03300."}