{"as_of":"2026-08-13T21:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:873599d37da476cf5ccdf323cc27e1fe2890f56d38771f3982d194ef47108d1e","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T00:26:46.301506Z","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":"2026-05-11T11:36:00.748286Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"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":"2026-08-12T19:17:59.970016Z","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":"sha256:4a3235f3569e448c74beed61a21b18b46a06e0919ae862adaad7222022eac741","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":"1912.05706","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":"2026-08-06T16:22:45.268202Z","title":"Bogdanov et al., Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State withN ICER","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.14255","last_updated":"2025-12-10T17:44:25Z","snapshot_observed_at":"2026-08-09T06:22:32.264848Z","submitted_at":"2025-07-18T11:19:45Z","title":"Probing of EoS with clusters and hypernuclei","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T16:22:45.268202Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2507.14255"},"observation_digest":"sha256:de56fbbae894bf8174dcb4609e3816156f6c1faec22f3e087f0567f00f06cb1b","observation_id":"6401b450-ef06-4123-86a5-12376364f58c","resolution":{"observed_at":"2026-08-06T16:22:45.268202Z","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":"2026-08-04T19:51:05.370545Z","title":"Bogdanov et al., Astrophys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.09061","last_updated":"2025-09-10T23:58:36Z","snapshot_observed_at":"2026-08-09T04:48:06.095863Z","submitted_at":"2025-09-10T23:58:36Z","title":"Study on the equation-of-state with light clusters and hypernuclei","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-04T19:51:05.370545Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2509.09061"},"observation_digest":"sha256:7cb9fe8393e50d649d8f796fabf6de62f179dbdaf04f96a6d855275efef904da","observation_id":"65ce39b4-76a1-438d-af4e-41902354c33b","resolution":{"observed_at":"2026-08-04T19:51:05.370545Z","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":"1912.05706","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05706","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equa- tion of State withN ICER. I. The Millisecond Pulsar X-Ray Data Set","venue":null,"work_id":"6ebf2a6d-8764-44d4-9afb-eed50300c25b","year":2019},"citing_paper":{"arxiv_id":"2604.11710","last_updated":"2026-04-13T16:44:22Z","snapshot_observed_at":"2026-08-11T00:27:57.240735Z","submitted_at":"2026-04-13T16:44:22Z","title":"A bright flare in the obscured state of GRS 1915+105 as seen by NICER and Swift","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-10T14:51:22.160440Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2604.11710"},"observation_digest":"sha256:bf930bd5f014697007cabbf2afd1d8c12bbc301beb9f9104ec8ff5f92094c8d4","observation_id":"f1bc9a66-4f49-4215-9b85-600d0b601389","resolution":{"observed_at":"2026-05-11T11:31:01.012369Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"1912.05706","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05706","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equa- tion of State withN ICER. I. The Millisecond Pulsar X-Ray Data Set","venue":null,"work_id":"6ebf2a6d-8764-44d4-9afb-eed50300c25b","year":2019},"citing_paper":{"arxiv_id":"2604.13208","last_updated":"2026-06-08T11:02:34Z","snapshot_observed_at":"2026-08-12T21:42:28.738288Z","submitted_at":"2026-04-14T18:30:45Z","title":"Axial Oscillations of Viscous Neutron Stars","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-10T14:26:31.751897Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2604.13208"},"observation_digest":"sha256:08bfdfe1cca97690b60cd8f3d45fb62706ce8db7fa3733242358f31a17724937","observation_id":"004242b0-8d93-4a6a-99bc-0d07f3bbd648","resolution":{"observed_at":"2026-05-11T11:36:00.750411Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-07-12T00:24:01.284884Z","title":null,"venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.03721","last_updated":"2026-07-04T06:04:04Z","snapshot_observed_at":"2026-08-08T10:04:04.593895Z","submitted_at":"2026-07-04T06:04:04Z","title":"A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-07-12T00:24:01.284884Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2607.03721"},"observation_digest":"sha256:8d63b2c5772130114a4cf522971cca24328884e76217983969174905447b645a","observation_id":"7b4c6568-7550-4cae-bf05-af09d1d8b7f0","resolution":{"observed_at":"2026-07-12T00:24:01.284884Z","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":"2026-08-01T03:47:24.546007Z","title":null,"venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.27664","last_updated":"2026-07-30T04:21:23Z","snapshot_observed_at":"2026-08-04T07:39:35.858439Z","submitted_at":"2026-07-30T04:21:23Z","title":"Proof of Concept Measurements of Laterally Graded Multilayers for Soft X-ray Spectropolarimetry","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-01T03:47:24.546007Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2607.27664"},"observation_digest":"sha256:cb37dca814e7285b76dceedb7792a225ba2949e5adfc5cf51bd0c31ea0939494","observation_id":"5351e962-e4ed-431f-8333-87ebf73c6b2a","resolution":{"observed_at":"2026-08-01T03:47:24.546007Z","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":"2026-08-11T00:26:46.301506Z","title":"Bogdanovet al., Astrophys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.07698","last_updated":"2026-08-07T18:40:24Z","snapshot_observed_at":"2026-08-13T20:13:36.064763Z","submitted_at":"2026-08-07T18:40:24Z","title":"Fast and Accurate Prediction of Neutron Star Structure with Deep Neural Networks","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T00:26:46.301506Z"},"links":{"cited_paper":"/paper/1912.05706","citing_paper":"/paper/2608.07698"},"observation_digest":"sha256:5e2e9874cdc2e21e6b006b0118eb67169001892fad99ca6b25646c4faa170c49","observation_id":"d51fae5d-1d73-4795-8847-fb1a680513a5","resolution":{"observed_at":"2026-08-11T00:26:46.301506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1912.05706/citation-record","integrity":"/paper/1912.05706/integrity","json":"/paper/1912.05706/citation-record.json","paper":"/paper/1912.05706"},"outbound":[],"paper":{"arxiv_id":"1912.05706","last_updated":"2019-12-12T00:04:42Z","latest_version":1,"primary_category":"astro-ph.HE","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"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1912.05706."}