{"as_of":"2026-08-09T20:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4201cc99b9c9b1c5a0d5ab9edccabc7620e6bc5229d92405a05db5c03a678887","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":"2026-08-09T06:31:02.800959+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":"2026-08-09T17:47:56.919655Z","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":"2026-05-20T08:58:09.511424Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"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":"2026-08-09T17:47:56.919655Z","title":"Colloquium : Mea- suring the neutron star equation of state using x-ray timing,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.00819","last_updated":"2025-02-26T10:52:41Z","snapshot_observed_at":"2026-08-09T17:34:22.209737Z","submitted_at":"2025-02-02T15:08:09Z","title":"Kaon Modification in Pion Medium","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-09T17:47:56.919655Z"},"links":{"cited_paper":"/paper/1602.01081","citing_paper":"/paper/2502.00819"},"observation_digest":"sha256:51557308f0fdd35ee9652e8c4c4c8895c09580530719017207c6b0ff8aba755d","observation_id":"d3c3ae1b-3998-4c41-b432-3a4ae1546f96","resolution":{"observed_at":"2026-08-09T17:47:56.919655Z","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":"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":"2026-08-04T15:37:54.707800Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.19933","last_updated":"2026-07-14T09:52:14Z","snapshot_observed_at":"2026-08-08T16:19:56.650266Z","submitted_at":"2025-09-24T09:40:16Z","title":"QFT on rotating boxes at finite temperature","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-04T15:37:54.707800Z"},"links":{"cited_paper":"/paper/1602.01081","citing_paper":"/paper/2509.19933"},"observation_digest":"sha256:89ce6a397037801080f2edcfaa2ce47b02dd209ea0696adb74ac91ed2df1c008","observation_id":"1bfe01fe-41a6-450b-8d36-9fe3befec8c5","resolution":{"observed_at":"2026-08-04T15:37:54.707800Z","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":"2026-08-04T00:40:04.347148Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2601.05999","last_updated":"2026-07-31T19:04:54Z","snapshot_observed_at":"2026-08-06T23:10:54.278432Z","submitted_at":"2026-01-09T18:33:25Z","title":"Constraining Hamiltonians from chiral effective field theory with neutron-star data","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-04T00:40:04.347148Z"},"links":{"cited_paper":"/paper/1602.01081","citing_paper":"/paper/2601.05999"},"observation_digest":"sha256:40f6eeab30d8d33ea986994ba64ffa462fcbe915502c325e96fd85287e83ff39","observation_id":"2946d89b-af55-484f-a600-8737dedf73b7","resolution":{"observed_at":"2026-08-04T00:40:04.347148Z","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":"1602.01081","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.01081","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Measuring the neutron star equation of state using X-ray timing","venue":"astro-ph.HE","work_id":"20cefbbc-f7af-4c94-856e-cdc200e01ab8","year":2016},"citing_paper":{"arxiv_id":"2605.18731","last_updated":"2026-05-18T17:53:13Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-18T17:53:13Z","title":"Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207","version":1},"reference_index":228,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1602.01081","citing_paper":"/paper/2605.18731"},"observation_digest":"sha256:1d14f2820f76bcb26f205f781f213fbb5179a854d85c1f47777b5be009ddbe19","observation_id":"c0062078-67ba-4460-98c1-d6119f147589","resolution":{"observed_at":"2026-05-20T08:58:09.512826Z","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":"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":"2026-07-12T00:24:01.284884Z","title":"Reviews of Modern Physics , keywords =","venue":null,"work_id":null,"year":null},"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":122,"source":"arxiv_source","source_observed_at":"2026-07-12T00:24:01.284884Z"},"links":{"cited_paper":"/paper/1602.01081","citing_paper":"/paper/2607.03721"},"observation_digest":"sha256:5c0b6cbec16926c864dc8740e385b93087180f3f7f57246920f06de95742bcd3","observation_id":"dd756e1a-7d5d-49a0-aa72-fe65bc8fe779","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":"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":"2026-07-14T06:38:48.754265Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.11154","last_updated":"2026-07-13T06:48:40Z","snapshot_observed_at":"2026-08-02T20:10:47.890228Z","submitted_at":"2026-07-13T06:48:40Z","title":"Determination of neutron star radius from pulse profile modeling using profile likelihood","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-14T06:38:48.754265Z"},"links":{"cited_paper":"/paper/1602.01081","citing_paper":"/paper/2607.11154"},"observation_digest":"sha256:4d1cd78e15c19c8c0ddeef5d82b2ee5dab58597c9becd79a27f0444a9946cfae","observation_id":"b9cc448a-530c-4552-86b9-2b677307ee0e","resolution":{"observed_at":"2026-07-14T06:38:48.754265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1602.01081/citation-record","integrity":"/paper/1602.01081/integrity","json":"/paper/1602.01081/citation-record.json","paper":"/paper/1602.01081"},"outbound":[],"paper":{"arxiv_id":"1602.01081","last_updated":"2016-02-02T20:56:45Z","latest_version":1,"primary_category":"astro-ph.HE","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"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1602.01081."}