{"as_of":"2026-08-09T00:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a2cd57421670f94672645bf809b65ee7aff44b34d7c2969bb9f9044d3d29eac1","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T00:43:19.441566Z","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":"2026-07-04T16:19:57.046774Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2107.06804","last_updated":"2021-07-14T16:04:29Z","snapshot_observed_at":"2026-08-06T08:06:41.139452Z","submitted_at":"2021-07-14T16:04:29Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06804","snapshot_observed_at":"2026-07-13T17:23:25.842886Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.26885","last_updated":"2026-05-29T07:50:42Z","snapshot_observed_at":"2026-08-03T05:39:04.714659Z","submitted_at":"2026-03-27T18:02:32Z","title":"TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-13T17:23:25.842886Z"},"links":{"cited_paper":"/paper/2107.06804","citing_paper":"/paper/2603.26885"},"observation_digest":"sha256:70de085367d1affdb6246cd36a41496eb772c3d7a3b836be45cfa2c3da02eb86","observation_id":"8d329019-11d7-4840-8425-9dd965133093","resolution":{"observed_at":"2026-07-13T17:23:25.842886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.06804","last_updated":"2021-07-14T16:04:29Z","snapshot_observed_at":"2026-08-06T08:06:41.139452Z","submitted_at":"2021-07-14T16:04:29Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence","version":1},"cited_work":{"arxiv_id":"2107.06804","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2107.06804","snapshot_observed_at":"2026-07-04T16:19:57.046774Z","title":null,"venue":null,"work_id":"2a94558a-a762-4517-b577-65c1842fe8c4","year":2021},"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":79,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/2107.06804","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:bc1f14ba4d792a8c5b4b45ab4290717cf890de11ae53f3915247a5dff3934646","observation_id":"ac78cae1-2d3a-46d8-9343-2ea17bc5d98e","resolution":{"observed_at":"2026-07-03T07:37:45.066155Z","resolver_source":"arxiv_id","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":"2107.06804","last_updated":"2021-07-14T16:04:29Z","snapshot_observed_at":"2026-08-06T08:06:41.139452Z","submitted_at":"2021-07-14T16:04:29Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence","version":1},"cited_work":{"arxiv_id":"2107.06804","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2107.06804","snapshot_observed_at":"2026-07-04T16:19:57.046774Z","title":null,"venue":null,"work_id":"2a94558a-a762-4517-b577-65c1842fe8c4","year":2021},"citing_paper":{"arxiv_id":"2606.26326","last_updated":"2026-06-24T19:12:40Z","snapshot_observed_at":"2026-08-03T00:30:24.951043Z","submitted_at":"2026-06-24T19:12:40Z","title":"Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-06-26T00:47:21.247516Z"},"links":{"cited_paper":"/paper/2107.06804","citing_paper":"/paper/2606.26326"},"observation_digest":"sha256:bd84637b2b169b69dc5d5c339945a149c6d26d3f15dbdf905264378bf1abc689","observation_id":"55edaf14-e354-440c-b930-43ecb839fd5f","resolution":{"observed_at":"2026-07-04T16:19:57.048411Z","resolver_source":"arxiv_id","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":"2107.06804","last_updated":"2021-07-14T16:04:29Z","snapshot_observed_at":"2026-08-06T08:06:41.139452Z","submitted_at":"2021-07-14T16:04:29Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.06804","snapshot_observed_at":"2026-08-08T00:43:19.441566Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.04092","last_updated":"2026-08-04T18:00:03Z","snapshot_observed_at":"2026-08-08T23:10:59.820760Z","submitted_at":"2026-08-04T18:00:03Z","title":"From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-08T00:43:19.441566Z"},"links":{"cited_paper":"/paper/2107.06804","citing_paper":"/paper/2608.04092"},"observation_digest":"sha256:431f054b80972e9ade70caad44d755908e03bc1aa1f0576c1ab4800bc286efd1","observation_id":"e2ef3e4d-8d56-4185-90bb-cf8aed0dadac","resolution":{"observed_at":"2026-08-08T00:43:19.441566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2107.06804/citation-record","integrity":"/paper/2107.06804/integrity","json":"/paper/2107.06804/citation-record.json","paper":"/paper/2107.06804"},"outbound":[],"paper":{"arxiv_id":"2107.06804","last_updated":"2021-07-14T16:04:29Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-06T08:06:41.139452Z","submitted_at":"2021-07-14T16:04:29Z","title":"Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence"},"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 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2107.06804."}