{"as_of":"2026-08-11T19:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:597b98613a3767097697f71431f04491ba4e831b62814bf1c7ac75389e9966e3","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":"2026-08-11T06:34:44.6726+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":"2026-08-11T14:29:01.341045Z","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":"2026-05-12T00:41:18.988335Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1305.7197","last_updated":"2013-05-30T18:35:18Z","snapshot_observed_at":"2026-07-06T03:14:44.470940Z","submitted_at":"2013-05-30T18:35:18Z","title":"Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.7197","snapshot_observed_at":"2026-08-11T14:29:01.341045Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.12002","last_updated":"2025-07-16T07:57:02Z","snapshot_observed_at":"2026-08-11T14:20:36.315671Z","submitted_at":"2024-12-16T17:31:22Z","title":"Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons","version":2},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-08-11T14:29:01.341045Z"},"links":{"cited_paper":"/paper/1305.7197","citing_paper":"/paper/2412.12002"},"observation_digest":"sha256:edbd6166da159c4f16b901dd7a980e8f2f52ed00b2001b062876ff76ec145fcd","observation_id":"8de087fe-aa71-45e3-9e9c-f5d17b44372a","resolution":{"observed_at":"2026-08-11T14:29:01.341045Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.7197","last_updated":"2013-05-30T18:35:18Z","snapshot_observed_at":"2026-07-06T03:14:44.470940Z","submitted_at":"2013-05-30T18:35:18Z","title":"Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.7197","snapshot_observed_at":"2026-08-10T16:33:19.613606Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.613606Z"},"links":{"cited_paper":"/paper/1305.7197","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:4dde1eb6af13e510acc2c90ea46c04286de6b3d14c8a94465ce89d2b97c20750","observation_id":"c708d623-c6d7-4a94-8e74-a44b66f6b6ad","resolution":{"observed_at":"2026-08-10T16:33:19.613606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.7197","last_updated":"2013-05-30T18:35:18Z","snapshot_observed_at":"2026-07-06T03:14:44.470940Z","submitted_at":"2013-05-30T18:35:18Z","title":"Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.7197","snapshot_observed_at":"2026-08-05T11:42:10.888512Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.02325","last_updated":"2025-09-02T13:51:14Z","snapshot_observed_at":"2026-08-10T10:07:32.224439Z","submitted_at":"2025-09-02T13:51:14Z","title":"Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model","version":1},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-08-05T11:42:10.888512Z"},"links":{"cited_paper":"/paper/1305.7197","citing_paper":"/paper/2509.02325"},"observation_digest":"sha256:caad24b713dfe8b20e4da2eee0dc3624e56a557d5ac5e27f9cc7a8e93dc307b9","observation_id":"45ddba0e-fe89-42e4-b34c-9b86396459d5","resolution":{"observed_at":"2026-08-05T11:42:10.888512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.7197","last_updated":"2013-05-30T18:35:18Z","snapshot_observed_at":"2026-07-06T03:14:44.470940Z","submitted_at":"2013-05-30T18:35:18Z","title":"Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.7197","snapshot_observed_at":"2026-08-04T18:11:08.778273Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.10150","last_updated":"2025-09-12T11:25:29Z","snapshot_observed_at":"2026-08-11T15:46:07.422801Z","submitted_at":"2025-09-12T11:25:29Z","title":"Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-04T18:11:08.778273Z"},"links":{"cited_paper":"/paper/1305.7197","citing_paper":"/paper/2509.10150"},"observation_digest":"sha256:dc8cede72ceafe5d3dd71b843e09bdcdd2698ea90b144cce59bc2c5eeacfd946","observation_id":"80e62f4f-e9ff-4b25-8e7f-000be39574cf","resolution":{"observed_at":"2026-08-04T18:11:08.778273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.7197","last_updated":"2013-05-30T18:35:18Z","snapshot_observed_at":"2026-07-06T03:14:44.470940Z","submitted_at":"2013-05-30T18:35:18Z","title":"Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state","version":1},"cited_work":{"arxiv_id":"1305.7197","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1305.7197","snapshot_observed_at":"2026-07-04T18:38:38.724744Z","title":null,"venue":null,"work_id":"03208761-6db2-4c93-a30f-d4b3912f3ebb","year":2013},"citing_paper":{"arxiv_id":"2605.03305","last_updated":"2026-05-05T02:49:02Z","snapshot_observed_at":"2026-07-06T23:16:15.509235Z","submitted_at":"2026-05-05T02:49:02Z","title":"Non-radial pulsations of gravitationally coupled two-fluid neutron stars in general relativity","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-07T14:48:53.601422Z"},"links":{"cited_paper":"/paper/1305.7197","citing_paper":"/paper/2605.03305"},"observation_digest":"sha256:0652a254d7f9b2c163ce807bad80c397705e8954b3b9f9a212e7ee1589abe735","observation_id":"d3fb37a0-9d8c-4252-a55c-c7b9e422576a","resolution":{"observed_at":"2026-07-04T18:38:38.724744Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1305.7197/citation-record","integrity":"/paper/1305.7197/integrity","json":"/paper/1305.7197/citation-record.json","paper":"/paper/1305.7197"},"outbound":[],"paper":{"arxiv_id":"1305.7197","last_updated":"2013-05-30T18:35:18Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T03:14:44.470940Z","submitted_at":"2013-05-30T18:35:18Z","title":"Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1305.7197."}