{"as_of":"2026-08-13T06:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6dd2b9f76aa5820cd9879490d38dd7abe769446a6b65eaaf84413478298de190","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":"2026-08-13T06:31:53.387327+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":"2026-08-10T16:31:09.783809Z","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":"2026-07-04T07:29:39.585691Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2112.08413","last_updated":"2022-07-03T07:41:52Z","snapshot_observed_at":"2026-08-07T17:46:26.384153Z","submitted_at":"2021-12-15T19:02:31Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.08413","snapshot_observed_at":"2026-08-10T16:31:09.783809Z","title":"Turbulent magnetic field amplification in binary neutron star mergers,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.13154","last_updated":"2025-01-22T19:00:01Z","snapshot_observed_at":"2026-08-11T03:41:24.633293Z","submitted_at":"2025-01-22T19:00:01Z","title":"Implications of Magnetic Flux-Disk Mass Correlation in Black Hole-Neutron Star Mergers for GRB sub-populations","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T16:31:09.783809Z"},"links":{"cited_paper":"/paper/2112.08413","citing_paper":"/paper/2501.13154"},"observation_digest":"sha256:6c0b4fb5ae67791559e1e775f1472b7a49776a7726e97c4202483b0bbc2a7ac3","observation_id":"19abccf9-5000-402d-9c32-26e609865bb5","resolution":{"observed_at":"2026-08-10T16:31:09.783809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.08413","last_updated":"2022-07-03T07:41:52Z","snapshot_observed_at":"2026-08-07T17:46:26.384153Z","submitted_at":"2021-12-15T19:02:31Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":"2112.08413","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.08413","snapshot_observed_at":"2026-07-04T07:29:39.585691Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","venue":null,"work_id":"e50d01d2-32a1-4141-8d01-8f3d85d36fcf","year":2022},"citing_paper":{"arxiv_id":"2510.00114","last_updated":"2026-04-30T00:58:48Z","snapshot_observed_at":"2026-08-11T00:38:13.064325Z","submitted_at":"2025-09-30T18:00:11Z","title":"Chiral effects and Joule heating in hot and dense matter","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-18T11:24:20.786689Z"},"links":{"cited_paper":"/paper/2112.08413","citing_paper":"/paper/2510.00114"},"observation_digest":"sha256:a5a577fc4ec597449773a78e9acc7db78aea698447e3ed82c9f01636eb71b806","observation_id":"78a8b954-7e26-4563-b523-61e3bd5d85c4","resolution":{"observed_at":"2026-05-18T11:26:18.601146Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:31:53.387327+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.08413","last_updated":"2022-07-03T07:41:52Z","snapshot_observed_at":"2026-08-07T17:46:26.384153Z","submitted_at":"2021-12-15T19:02:31Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":"2112.08413","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.08413","snapshot_observed_at":"2026-07-04T07:29:39.585691Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","venue":null,"work_id":"e50d01d2-32a1-4141-8d01-8f3d85d36fcf","year":2022},"citing_paper":{"arxiv_id":"2605.30548","last_updated":"2026-05-28T20:30:13Z","snapshot_observed_at":"2026-08-12T13:30:50.158867Z","submitted_at":"2026-05-28T20:30:13Z","title":"Magnetic Eruption and Nucleosynthesis in GR{\\nu}MHD Simulations of Spinning Neutron Star Mergers","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-06-29T05:38:27.204444Z"},"links":{"cited_paper":"/paper/2112.08413","citing_paper":"/paper/2605.30548"},"observation_digest":"sha256:9e51d671047433d1471e02bc452345e0b7a6acf696e9de87f0e4791a0f9a298c","observation_id":"e9a794c5-9834-41c6-bb11-e70fe774df7b","resolution":{"observed_at":"2026-06-29T05:43:08.394092Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:31:53.387327+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.08413","last_updated":"2022-07-03T07:41:52Z","snapshot_observed_at":"2026-08-07T17:46:26.384153Z","submitted_at":"2021-12-15T19:02:31Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":"2112.08413","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.08413","snapshot_observed_at":"2026-07-04T07:29:39.585691Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","venue":null,"work_id":"e50d01d2-32a1-4141-8d01-8f3d85d36fcf","year":2022},"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":142,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/2112.08413","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:b865e43f279e8525341be36ac0012a5b7f1c327434b39d990fbc2f9901c3fe20","observation_id":"8cc04109-d0ef-4056-9c83-a247f7c4c84b","resolution":{"observed_at":"2026-07-03T07:37:45.117030Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:31:53.387327+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.08413","last_updated":"2022-07-03T07:41:52Z","snapshot_observed_at":"2026-08-07T17:46:26.384153Z","submitted_at":"2021-12-15T19:02:31Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":"2112.08413","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.08413","snapshot_observed_at":"2026-07-04T07:29:39.585691Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","venue":null,"work_id":"e50d01d2-32a1-4141-8d01-8f3d85d36fcf","year":2022},"citing_paper":{"arxiv_id":"2606.21659","last_updated":"2026-06-19T18:03:14Z","snapshot_observed_at":"2026-08-06T21:24:26.336014Z","submitted_at":"2026-06-19T18:03:14Z","title":"Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-26T13:20:12.147520Z"},"links":{"cited_paper":"/paper/2112.08413","citing_paper":"/paper/2606.21659"},"observation_digest":"sha256:bf7e856c879796e18f32d4111ef3873935432d18baa5b5a9d02bb722456bb441","observation_id":"90a8fe61-5852-4937-aac9-0876183467b3","resolution":{"observed_at":"2026-07-04T07:29:39.587210Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:31:53.387327+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.08413","last_updated":"2022-07-03T07:41:52Z","snapshot_observed_at":"2026-08-07T17:46:26.384153Z","submitted_at":"2021-12-15T19:02:31Z","title":"Turbulent magnetic field amplification in binary neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.08413","snapshot_observed_at":"2026-07-31T14:28:12.694657Z","title":"Palenzuela, R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.24457","last_updated":"2026-07-27T13:58:46Z","snapshot_observed_at":"2026-08-09T04:12:41.741905Z","submitted_at":"2026-07-27T13:58:46Z","title":"Transport Properties of the MRI in Differentially Rotating Neutron Stars","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-31T14:28:12.694657Z"},"links":{"cited_paper":"/paper/2112.08413","citing_paper":"/paper/2607.24457"},"observation_digest":"sha256:983c7bb3c5a68ec3931c5b3a8aa59418449877d4abedae6b192e102ffff8c9b2","observation_id":"c2bfb55c-1875-4ea4-b3bc-24503c7b284c","resolution":{"observed_at":"2026-07-31T14:28:12.694657Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2112.08413/citation-record","integrity":"/paper/2112.08413/integrity","json":"/paper/2112.08413/citation-record.json","paper":"/paper/2112.08413"},"outbound":[],"paper":{"arxiv_id":"2112.08413","last_updated":"2022-07-03T07:41:52Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-07T17:46:26.384153Z","submitted_at":"2021-12-15T19:02:31Z","title":"Turbulent magnetic field amplification in binary neutron star mergers"},"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":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2112.08413."}