{"as_of":"2026-08-08T09:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:60537a3a67d7f5148f1d976bb2f01a7c15372d6e6e37c8174f92fb6c67f8ff92","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T11:41:25.615640Z","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":"2026-07-03T07:37:44.927109Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-05T10:20:21.387268Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-08-07T11:41:25.615640Z","title":"Shibata, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.01679","last_updated":"2025-07-22T14:30:59Z","snapshot_observed_at":"2026-08-08T01:07:42.134930Z","submitted_at":"2025-06-02T13:48:13Z","title":"Neutrino pair annihilation driven jets from black-hole torus systems","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T11:41:25.615640Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/2506.01679"},"observation_digest":"sha256:2a937edb20ff2698e1623b04d2c2fc7e6318784dba02489a7a059d0a75c6fb06","observation_id":"e5328a4e-5d3b-4c65-b017-b1f757d461d5","resolution":{"observed_at":"2026-08-07T11:41:25.615640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-05T10:20:21.387268Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-08-07T11:40:58.943358Z","title":"Shibata, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.02115","last_updated":"2025-06-02T18:00:04Z","snapshot_observed_at":"2026-08-08T01:13:47.825444Z","submitted_at":"2025-06-02T18:00:04Z","title":"The error budget of binary neutron star merger simulations for configurations with high spin","version":1},"reference_index":125,"source":"pdf_text","source_observed_at":"2026-08-07T11:40:58.943358Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/2506.02115"},"observation_digest":"sha256:c60ec7fe6f62ce56b4c31e6c121551ac5446eea72a0c2ed070b12ac2fb2f40ac","observation_id":"b874fbc8-3911-4da8-bb70-b8981d53a7d5","resolution":{"observed_at":"2026-08-07T11:40:58.943358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-05T10:20:21.387268Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-08-06T15:59:41.524477Z","title":"Shibata, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.14591","last_updated":"2025-07-23T11:04:42Z","snapshot_observed_at":"2026-08-08T04:41:41.623118Z","submitted_at":"2025-07-19T12:27:51Z","title":"Properties of compact objects in quadratic non-metricity gravity","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T15:59:41.524477Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/2507.14591"},"observation_digest":"sha256:733e2657da50dc6718cfc4fbb4c8592245b5ddae9acc20f486d20a46e4b4ca82","observation_id":"f0f53dd6-4067-46b0-9276-2ad339ee305c","resolution":{"observed_at":"2026-08-06T15:59:41.524477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-05T10:20:21.387268Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":"1710.07579","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-07-03T07:37:44.927109Z","title":"Modeling GW170817 based on numerical relativity and its implications","venue":"astro-ph.HE","work_id":"6b101f18-1d42-48c2-961a-d116cac40312","year":2017},"citing_paper":{"arxiv_id":"2509.13322","last_updated":"2026-03-18T20:26:19Z","snapshot_observed_at":"2026-07-06T22:30:02.223630Z","submitted_at":"2025-09-16T17:59:59Z","title":"Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-05-18T15:47:12.746339Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/2509.13322"},"observation_digest":"sha256:370d2c40e25c6338842750cde770659b1a3b1afc0f92facc028e7bff06096eba","observation_id":"da83e82f-f1a3-419c-94b2-17ec0dbf1be6","resolution":{"observed_at":"2026-05-18T15:51:34.596330Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-05T10:20:21.387268Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":"1710.07579","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-07-03T07:37:44.927109Z","title":"Modeling GW170817 based on numerical relativity and its implications","venue":"astro-ph.HE","work_id":"6b101f18-1d42-48c2-961a-d116cac40312","year":2017},"citing_paper":{"arxiv_id":"2606.11299","last_updated":"2026-06-09T18:00:02Z","snapshot_observed_at":"2026-08-05T19:03:12.115770Z","submitted_at":"2026-06-09T18:00:02Z","title":"A magnetar formation in binary neutron star merger","version":1},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:69cdea7c0e1520bbd1fe57f8b34db909191ccfc7789588599ad6810209e029d2","observation_id":"71d27885-5106-4be3-b3ac-317091ccd5c3","resolution":{"observed_at":"2026-07-03T07:37:44.928382Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-05T10:20:21.387268Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-08-01T19:22:25.455449Z","title":"Modeling GW170817 based on numerical relativity and its implications","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.17006","last_updated":"2026-07-18T23:43:21Z","snapshot_observed_at":"2026-08-06T15:57:38.180022Z","submitted_at":"2026-07-18T23:43:21Z","title":"The equation of state for neutron stars","version":1},"reference_index":210,"source":"arxiv_source","source_observed_at":"2026-08-01T19:22:25.455449Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/2607.17006"},"observation_digest":"sha256:1be8511edac2536b075f1f6ac17d875cea8208ef00fbdd35ef422cbc05d3597a","observation_id":"6ef10915-8903-4bdc-a53e-d09193321d11","resolution":{"observed_at":"2026-08-01T19:22:25.455449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1710.07579/citation-record","integrity":"/paper/1710.07579/integrity","json":"/paper/1710.07579/citation-record.json","paper":"/paper/1710.07579"},"outbound":[],"paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-05T10:20:21.387268Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1710.07579."}