{"as_of":"2026-08-10T05:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3e4773c6ae23739afdd69da2b225c6aeb0da08d6817debfec4c7cb2e6f25d79a","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T04:46:13.252845Z","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":"2026-05-22T01:40:54.128614Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2306.04626","last_updated":"2023-09-06T20:20:07Z","snapshot_observed_at":"2026-07-06T15:39:53.141172Z","submitted_at":"2023-06-07T17:54:24Z","title":"Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.04626","snapshot_observed_at":"2026-08-09T04:46:13.252845Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:13.252845Z"},"links":{"cited_paper":"/paper/2306.04626","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:99275a942bff94287cf85aefc81175f8116f37558d5c7ec232821c12c8c96e52","observation_id":"6d9eab2b-c20a-4a31-a738-7d0ce110a90a","resolution":{"observed_at":"2026-08-09T04:46:13.252845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04626","last_updated":"2023-09-06T20:20:07Z","snapshot_observed_at":"2026-07-06T15:39:53.141172Z","submitted_at":"2023-06-07T17:54:24Z","title":"Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars","version":2},"cited_work":{"arxiv_id":"2306.04626","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.04626","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"bdcccd02-6d24-4d3b-9846-51a08f5cfffc","year":2023},"citing_paper":{"arxiv_id":"2505.16929","last_updated":"2026-04-14T09:24:59Z","snapshot_observed_at":"2026-07-06T21:28:43.610849Z","submitted_at":"2025-05-22T17:22:16Z","title":"Properties of the neutron star crust informed by nuclear structure data","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-05-22T01:36:22.187463Z"},"links":{"cited_paper":"/paper/2306.04626","citing_paper":"/paper/2505.16929"},"observation_digest":"sha256:ff7259427984818ab488260b07c9c1df21e8f7d20f24fe611c0d0d4d1e1d8ff3","observation_id":"84846ae3-3c7f-49c0-b13a-a5e9d6738ed1","resolution":{"observed_at":"2026-05-22T01:40:54.131358Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04626","last_updated":"2023-09-06T20:20:07Z","snapshot_observed_at":"2026-07-06T15:39:53.141172Z","submitted_at":"2023-06-07T17:54:24Z","title":"Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars","version":2},"cited_work":{"arxiv_id":"2306.04626","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.04626","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"bdcccd02-6d24-4d3b-9846-51a08f5cfffc","year":2023},"citing_paper":{"arxiv_id":"2508.15912","last_updated":"2026-05-18T20:05:07Z","snapshot_observed_at":"2026-07-31T16:58:10.911812Z","submitted_at":"2025-08-21T18:18:26Z","title":"$f$-mode Oscillations for Hyperons and H-dibaryons in Neutron Stars","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-21T22:06:40.449540Z"},"links":{"cited_paper":"/paper/2306.04626","citing_paper":"/paper/2508.15912"},"observation_digest":"sha256:cb91698e10e372a2d6d971b05634c9a46a56aadfaeb9325cc430559cf3eefa61","observation_id":"c817fb27-3796-4945-8662-71335665cd47","resolution":{"observed_at":"2026-05-21T22:10:42.539528Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2306.04626/citation-record","integrity":"/paper/2306.04626/integrity","json":"/paper/2306.04626/citation-record.json","paper":"/paper/2306.04626"},"outbound":[],"paper":{"arxiv_id":"2306.04626","last_updated":"2023-09-06T20:20:07Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T15:39:53.141172Z","submitted_at":"2023-06-07T17:54:24Z","title":"Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2306.04626."}