{"as_of":"2026-08-12T20:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e668ecc7f7dc6dee5a822ac9968d9847fa4ba6c326a743894f8f35e3eda78769","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":"2026-08-12T06:34:41.77262+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":"2026-08-11T18:36:00.945146Z","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":"2026-07-09T20:06:29.647466Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1805.09371","last_updated":"2018-10-17T18:23:38Z","snapshot_observed_at":"2026-08-07T23:31:10.494645Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.09371","snapshot_observed_at":"2026-08-11T18:36:00.945146Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.07846","last_updated":"2025-02-18T23:12:56Z","snapshot_observed_at":"2026-08-12T17:38:30.171061Z","submitted_at":"2024-12-10T19:00:05Z","title":"Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:00.945146Z"},"links":{"cited_paper":"/paper/1805.09371","citing_paper":"/paper/2412.07846"},"observation_digest":"sha256:9e4437a0a37aa5849a6e5dc6556ad92558e8b7b3031dc4b7274b70a16f32a6c7","observation_id":"bcd436b2-d477-418a-801b-a692179abeaa","resolution":{"observed_at":"2026-08-11T18:36:00.945146Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.09371","last_updated":"2018-10-17T18:23:38Z","snapshot_observed_at":"2026-08-07T23:31:10.494645Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.09371","snapshot_observed_at":"2026-08-03T20:20:20.189580Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.20378","last_updated":"2026-06-28T03:18:05Z","snapshot_observed_at":"2026-08-06T06:55:09.797555Z","submitted_at":"2025-11-25T14:59:28Z","title":"Toward a Unified Understanding of the Dense Matter Equation of State","version":2},"reference_index":272,"source":"pdf_text","source_observed_at":"2026-08-03T20:20:20.189580Z"},"links":{"cited_paper":"/paper/1805.09371","citing_paper":"/paper/2511.20378"},"observation_digest":"sha256:9c463b4bb80a0ff0625e9fd55b80da719004c4514b990a0d7ef21b27c162ef7b","observation_id":"438b3022-4f2a-498d-9b72-808b3bd492d6","resolution":{"observed_at":"2026-08-03T20:20:20.189580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.09371","last_updated":"2018-10-17T18:23:38Z","snapshot_observed_at":"2026-08-07T23:31:10.494645Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","version":2},"cited_work":{"arxiv_id":"1805.09371","doi":null,"metadata_source":"pith","pith_arxiv_id":"1805.09371","snapshot_observed_at":"2026-07-09T20:06:29.647466Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","venue":"astro-ph.HE","work_id":"b7c7438b-9d14-4ede-96ba-58c15db8870a","year":2018},"citing_paper":{"arxiv_id":"2606.11299","last_updated":"2026-06-09T18:00:02Z","snapshot_observed_at":"2026-08-12T15:48:11.069118Z","submitted_at":"2026-06-09T18:00:02Z","title":"A magnetar formation in binary neutron star merger","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/1805.09371","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:aece8cf9e5e3e9cad10ed7d4bf912044e5e70c2b389456d1406a5f9bcf5c5265","observation_id":"6cfe7ac3-ba4b-4d40-a6cd-87d52fac59bb","resolution":{"observed_at":"2026-07-03T07:37:44.722688Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.09371","last_updated":"2018-10-17T18:23:38Z","snapshot_observed_at":"2026-08-07T23:31:10.494645Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.09371","snapshot_observed_at":"2026-07-12T05:14:58.841553Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03045","last_updated":"2026-07-03T07:34:46Z","snapshot_observed_at":"2026-08-03T21:49:18.542361Z","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":54,"source":"arxiv_source","source_observed_at":"2026-07-12T05:14:58.841553Z"},"links":{"cited_paper":"/paper/1805.09371","citing_paper":"/paper/2607.03045"},"observation_digest":"sha256:12232b11fce8dd9df4b6bdbeb81ab9f4d64165e7bf9f29e33210a6fb5593f2a8","observation_id":"d1abce07-eeb1-49aa-aba8-e758a50e307c","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":"1805.09371","last_updated":"2018-10-17T18:23:38Z","snapshot_observed_at":"2026-08-07T23:31:10.494645Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","version":2},"cited_work":{"arxiv_id":"1805.09371","doi":null,"metadata_source":"pith","pith_arxiv_id":"1805.09371","snapshot_observed_at":"2026-07-09T20:06:29.647466Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations","venue":"astro-ph.HE","work_id":"b7c7438b-9d14-4ede-96ba-58c15db8870a","year":2018},"citing_paper":{"arxiv_id":"2607.07120","last_updated":"2026-07-08T08:02:30Z","snapshot_observed_at":"2026-08-08T06:28:48.615790Z","submitted_at":"2026-07-08T08:02:30Z","title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","version":1},"reference_index":216,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1805.09371","citing_paper":"/paper/2607.07120"},"observation_digest":"sha256:8decad0c3be013edb13190229e37d82409d5e2b4e67a48019f7dee6247be6fcc","observation_id":"f79f43a5-6418-4667-a12e-070d5cf700c7","resolution":{"observed_at":"2026-07-09T20:06:29.648757Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1805.09371/citation-record","integrity":"/paper/1805.09371/integrity","json":"/paper/1805.09371/citation-record.json","paper":"/paper/1805.09371"},"outbound":[],"paper":{"arxiv_id":"1805.09371","last_updated":"2018-10-17T18:23:38Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-07T23:31:10.494645Z","submitted_at":"2018-05-23T18:31:07Z","title":"Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1805.09371."}