{"as_of":"2026-08-23T09:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:46f4c27c7f50f56645fc0a3d14e4a2120220fd1149581986a61404e939ec2561","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":"2026-08-23T06:30:58.430688+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":"2026-08-16T05:25:17.239051Z","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":"2026-07-04T07:49:39.067014Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":"1709.09120","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-07-04T07:49:39.067014Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","venue":"astro-ph.HE","work_id":"302161aa-49b6-4868-9dda-e0b0fded78ea","year":2017},"citing_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},"reference_index":167,"source":"pdf_text","source_observed_at":"2026-05-12T01:58:58.813686Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/1710.05832"},"observation_digest":"sha256:4fce19326f50ffcf124fec438a5d6a9c3188e395664871a83eaaaba1178d3fd4","observation_id":"237199d3-7737-48ec-84d6-084aa37245e5","resolution":{"observed_at":"2026-05-12T01:58:58.894601Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-08-14T14:26:03.946262Z","title":"Nättilä, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03213","last_updated":"2019-08-08T18:00:00Z","snapshot_observed_at":"2026-08-17T11:08:47.456109Z","submitted_at":"2019-08-08T18:00:00Z","title":"Gravitational Waves from Holographic Neutron Star Mergers","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T14:26:03.946262Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/1908.03213"},"observation_digest":"sha256:3661456beb3031f4adbd418934bd25d9057b55d22818be84ad001846c8531455","observation_id":"1e919a8c-11ea-49f8-ad8a-4ff1609c3e57","resolution":{"observed_at":"2026-08-14T14:26:03.946262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-08-16T05:25:17.239051Z","title":"N¨ attil¨ a, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.20825","last_updated":"2025-09-07T19:39:37Z","snapshot_observed_at":"2026-08-16T17:27:28.635325Z","submitted_at":"2025-04-29T14:46:04Z","title":"Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T05:25:17.239051Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/2504.20825"},"observation_digest":"sha256:fe90723d284f3ac94104b819d1d8e4a89b4a8d0e6df421cf6d9e5c7e1ede138f","observation_id":"1efe7168-12c8-4ca7-af3c-bfdd5681c065","resolution":{"observed_at":"2026-08-16T05:25:17.239051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":"1709.09120","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-07-04T07:49:39.067014Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","venue":"astro-ph.HE","work_id":"302161aa-49b6-4868-9dda-e0b0fded78ea","year":2017},"citing_paper":{"arxiv_id":"2512.02484","last_updated":"2026-05-10T08:00:41Z","snapshot_observed_at":"2026-08-06T13:32:17.046475Z","submitted_at":"2025-12-02T07:18:55Z","title":"Properties of Stable Massive Quark Stars in Holography","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-17T03:04:38.141280Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/2512.02484"},"observation_digest":"sha256:6edb455d3cb872ba309192cd0dd81b87eb2d6d80cae7ce08897e974d8fa5e734","observation_id":"3d8e3e44-b83c-4f22-ae45-1fad754a1826","resolution":{"observed_at":"2026-05-17T03:08:56.890982Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":"1709.09120","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-07-04T07:49:39.067014Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","venue":"astro-ph.HE","work_id":"302161aa-49b6-4868-9dda-e0b0fded78ea","year":2017},"citing_paper":{"arxiv_id":"2605.14264","last_updated":"2026-05-14T02:08:14Z","snapshot_observed_at":"2026-08-14T09:17:29.993109Z","submitted_at":"2026-05-14T02:08:14Z","title":"The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius","version":1},"reference_index":114,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/2605.14264"},"observation_digest":"sha256:2a236d0697bdca7fd435b44cc9951c244848e5a6d1a1baf56d9a0e2bd60eac75","observation_id":"2920aa9b-e1ba-48b2-bcd2-1476205c0d41","resolution":{"observed_at":"2026-05-15T02:33:31.652352Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":"1709.09120","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-07-04T07:49:39.067014Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","venue":"astro-ph.HE","work_id":"302161aa-49b6-4868-9dda-e0b0fded78ea","year":2017},"citing_paper":{"arxiv_id":"2605.18731","last_updated":"2026-05-18T17:53:13Z","snapshot_observed_at":"2026-08-19T07:00:07.100695Z","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":17,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/2605.18731"},"observation_digest":"sha256:82de2c927daa97efa9a1611f7df2378483c3fbccf975bab70f609f271efbd048","observation_id":"dc6e63c9-e3ce-4123-bae7-096f70956785","resolution":{"observed_at":"2026-05-20T08:58:09.366488Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":"1709.09120","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-07-04T07:49:39.067014Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","venue":"astro-ph.HE","work_id":"302161aa-49b6-4868-9dda-e0b0fded78ea","year":2017},"citing_paper":{"arxiv_id":"2606.21435","last_updated":"2026-06-19T13:51:27Z","snapshot_observed_at":"2026-08-06T05:56:14.769876Z","submitted_at":"2026-06-19T13:51:27Z","title":"Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis","version":1},"reference_index":144,"source":"pdf_text","source_observed_at":"2026-06-26T12:50:53.032717Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/2606.21435"},"observation_digest":"sha256:c703e15014e9206f3e9c7344ec4d4338fa8347bc90169a28ef7d6c3f45ffe28f","observation_id":"55e8c17e-0861-49f4-b4c8-9025ff45bf24","resolution":{"observed_at":"2026-07-04T07:49:39.068426Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.09120","snapshot_observed_at":"2026-07-12T00:24:01.284884Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03721","last_updated":"2026-07-04T06:04:04Z","snapshot_observed_at":"2026-08-16T00:10:42.094855Z","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":85,"source":"arxiv_source","source_observed_at":"2026-07-12T00:24:01.284884Z"},"links":{"cited_paper":"/paper/1709.09120","citing_paper":"/paper/2607.03721"},"observation_digest":"sha256:16e9eaa8495fc256e04f715790ba03f5b86ca44d25166f11ba04f00820ce68e1","observation_id":"0c1cc199-9b63-47f1-b5cd-3dd7355dbd4a","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"}}],"links":{"evidence":"/evidence","html":"/paper/1709.09120/citation-record","integrity":"/paper/1709.09120/integrity","json":"/paper/1709.09120/citation-record.json","paper":"/paper/1709.09120"},"outbound":[],"paper":{"arxiv_id":"1709.09120","last_updated":"2017-09-26T16:36:01Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-20T01:01:24.394917Z","submitted_at":"2017-09-26T16:36:01Z","title":"Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1709.09120."}