{"as_of":"2026-08-10T08:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:927b8362be247c7608d2288a553f9b1db159ac1bd37b4b8be83c224f6e69acdd","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T04:46:13.168402Z","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":"2026-05-16T14:16:32.875090Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2001.01747","last_updated":"2020-01-06T19:19:48Z","snapshot_observed_at":"2026-08-10T07:28:55.089898Z","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":"2001.01747","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2001.01747","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Wysocki, R","venue":null,"work_id":"9a556a4f-a69b-4203-9b1b-69cdd6c1f45e","year":2001},"citing_paper":{"arxiv_id":"2007.05579","last_updated":"2022-03-18T17:26:01Z","snapshot_observed_at":"2026-08-09T13:59:48.109437Z","submitted_at":"2020-07-10T19:25:03Z","title":"Inferring the properties of a population of compact binaries in presence of selection effects","version":4},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-24T13:43:48.580253Z"},"links":{"cited_paper":"/paper/2001.01747","citing_paper":"/paper/2007.05579"},"observation_digest":"sha256:3ea8f47e11254c9e722141c6f201cce9feeb002073d7a27d602187d0f09d8926","observation_id":"76a6c004-e2dc-48e0-9523-94c6f84e45e1","resolution":{"observed_at":"2026-05-09T04:54:56.292695Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.01747","last_updated":"2020-01-06T19:19:48Z","snapshot_observed_at":"2026-08-10T07:28:55.089898Z","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":"2001.01747","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2001.01747","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Wysocki, R","venue":null,"work_id":"9a556a4f-a69b-4203-9b1b-69cdd6c1f45e","year":2001},"citing_paper":{"arxiv_id":"2111.03634","last_updated":"2025-01-30T17:06:46Z","snapshot_observed_at":"2026-08-04T10:06:39.982302Z","submitted_at":"2021-11-05T17:35:45Z","title":"The population of merging compact binaries inferred using gravitational waves through GWTC-3","version":5},"reference_index":134,"source":"pdf_text","source_observed_at":"2026-05-16T14:16:32.822374Z"},"links":{"cited_paper":"/paper/2001.01747","citing_paper":"/paper/2111.03634"},"observation_digest":"sha256:647a335baf9b9d3e43bb7cd8651f961e6cf3b0462bf3004ef83283576cef0061","observation_id":"4698b252-6d6e-4fb1-97fd-c085832a58d2","resolution":{"observed_at":"2026-05-16T14:16:32.877231Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.01747","last_updated":"2020-01-06T19:19:48Z","snapshot_observed_at":"2026-08-10T07:28:55.089898Z","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":"sha256:2325a8c1d9a059d7392841fb4e03787ce2c054db5ca1243736fc8486941dfe2c","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":{"arxiv_id":"2001.01747","last_updated":"2020-01-06T19:19:48Z","snapshot_observed_at":"2026-08-10T07:28:55.089898Z","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":"2026-08-08T23:01:14.434152Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2502.04278","last_updated":"2025-12-10T21:58:15Z","snapshot_observed_at":"2026-08-08T22:53:09.338057Z","submitted_at":"2025-02-06T18:25:34Z","title":"Probing Spin-Orbit Resonances with the Binary Black Hole Population","version":2},"reference_index":2020,"source":"pdf_text","source_observed_at":"2026-08-08T23:01:14.434152Z"},"links":{"cited_paper":"/paper/2001.01747","citing_paper":"/paper/2502.04278"},"observation_digest":"sha256:47b1751bf74f682f08d7a82e8577f9e3a1bae0d17e156c0af3c32011c6c14a14","observation_id":"fd8e741c-8e63-42c2-b705-fded4a52becf","resolution":{"observed_at":"2026-08-08T23:01:14.434152Z","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":"2026-08-10T07:28:55.089898Z","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":"2026-08-03T16:47:28.177486Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.12130","last_updated":"2026-05-30T20:45:32Z","snapshot_observed_at":"2026-08-09T15:07:11.303571Z","submitted_at":"2025-12-13T01:49:43Z","title":"Inference of Neutron Star Mass Distributions and the Dense Matter Equation of State from Multi-messenger Observations","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-03T16:47:28.177486Z"},"links":{"cited_paper":"/paper/2001.01747","citing_paper":"/paper/2512.12130"},"observation_digest":"sha256:8011062c79b7acd6566d2ec032c15527bea7b777d4165b946b7ac248c195a153","observation_id":"8c2010fb-0ce8-4576-bbf5-27a62e5d200b","resolution":{"observed_at":"2026-08-03T16:47:28.177486Z","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":"2026-08-10T07:28:55.089898Z","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":"2026-08-02T11:36:02.258688Z","title":"Inferring the neutron star equation of state simultaneously with the population of merging neutron stars,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2606.14229","last_updated":"2026-07-24T07:15:23Z","snapshot_observed_at":"2026-08-10T00:52:40.152165Z","submitted_at":"2026-06-12T08:11:12Z","title":"Fortifying gravitational-wave population inference with normalizing flows","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-02T11:36:02.258688Z"},"links":{"cited_paper":"/paper/2001.01747","citing_paper":"/paper/2606.14229"},"observation_digest":"sha256:ff7beb0a9766ec46599812e8780128d6bbdfe27421db398f174921118ad3dfb5","observation_id":"2e73e799-5a0f-411c-b418-30b017565e2f","resolution":{"observed_at":"2026-08-02T11:36:02.258688Z","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":"2026-08-10T07:28:55.089898Z","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":"2026-07-31T07:22:46.253634Z","title":"Inferring the neutron star equation of state simultaneously with the population of merging neutron stars","venue":null,"work_id":null,"year":2020},"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":276,"source":"arxiv_source","source_observed_at":"2026-07-31T07:22:46.253634Z"},"links":{"cited_paper":"/paper/2001.01747","citing_paper":"/paper/2607.28438"},"observation_digest":"sha256:2a933407d8fa29b667bb59b9e84ca29d5f8b654432872e5de85526999751cd2e","observation_id":"c4314b3f-9f09-4887-80fd-f8bb1796b75a","resolution":{"observed_at":"2026-07-31T07:22:46.253634Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2001.01747/citation-record","integrity":"/paper/2001.01747/integrity","json":"/paper/2001.01747/citation-record.json","paper":"/paper/2001.01747"},"outbound":[],"paper":{"arxiv_id":"2001.01747","last_updated":"2020-01-06T19:19:48Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-10T07:28:55.089898Z","submitted_at":"2020-01-06T19:19:48Z","title":"Inferring the neutron star equation of state simultaneously with the population of merging 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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2001.01747."}