{"as_of":"2026-08-09T20:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6aa18e3bea83505bd2b1fb79c068920ff7538c1c8dc656c41b1d3b2ba859eea3","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T12:47:49.802574Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":85,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-04T05:44:58.776848Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.26408","last_updated":"2026-08-03T07:33:44Z","snapshot_observed_at":"2026-08-08T22:42:13.748087Z","submitted_at":"2026-03-27T13:37:13Z","title":"The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T05:44:58.776848Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2603.26408"},"observation_digest":"sha256:e36c2024397c32cb497067b8fabd306a8330048dce56bc1e2228c3f39666fb53","observation_id":"ced9344b-dafd-4752-9f03-31537709daaa","resolution":{"observed_at":"2026-08-04T05:44:58.776848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-07-13T16:48:58.103396Z","title":"Torres-Forn´ e, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-06T23:11:01.859050Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-13T16:48:58.103396Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:63198505f476ff85d43c64c4f90e189f5e615f046118e66079541c30d8e4ebbc","observation_id":"f041db7e-bd5d-4232-b27b-f22a0d0a9eb9","resolution":{"observed_at":"2026-07-13T16:48:58.103396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-04T05:43:27.157799Z","title":"Torres-Forn´ e, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.27680","last_updated":"2026-08-01T10:10:28Z","snapshot_observed_at":"2026-08-06T23:11:01.859050Z","submitted_at":"2026-03-29T13:07:40Z","title":"Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:27.157799Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2603.27680"},"observation_digest":"sha256:14323409c68ba49544a9ce9995442c93adbb175a47d920f47e2ee6af2bed1161","observation_id":"63927295-4987-4ff7-ab58-19556030b97d","resolution":{"observed_at":"2026-08-04T05:43:27.157799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":"1902.10048","doi":"10.1103/physrevlett.123.051102","metadata_source":"pith","pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Torres-Forn´ e, P","venue":"gr-qc","work_id":"72f0db17-f4ba-4553-afb6-bf32fdfa1fcd","year":2019},"citing_paper":{"arxiv_id":"2605.04852","last_updated":"2026-05-06T12:50:31Z","snapshot_observed_at":"2026-07-06T23:17:33.252539Z","submitted_at":"2026-05-06T12:50:31Z","title":"Bayesian parameter estimation for the Core-bounce phase of Rapidly Rotating Core-Collapse Supernovae in real interferometric data","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-08T16:11:03.889445Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2605.04852"},"observation_digest":"sha256:3327fcf5c30c615bb7ef8ed8b039828365528a7e528ca1209fe6e25421d80e5e","observation_id":"95613371-43a4-4151-9eb6-4a1d73c43608","resolution":{"observed_at":"2026-05-11T18:21:09.582410Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":"1902.10048","doi":"10.1103/physrevlett.123.051102","metadata_source":"pith","pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Torres-Forn´ e, P","venue":"gr-qc","work_id":"72f0db17-f4ba-4553-afb6-bf32fdfa1fcd","year":2019},"citing_paper":{"arxiv_id":"2605.04896","last_updated":"2026-05-06T13:27:04Z","snapshot_observed_at":"2026-07-30T01:39:37.333910Z","submitted_at":"2026-05-06T13:27:04Z","title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-08T15:59:11.556246Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2605.04896"},"observation_digest":"sha256:385f758f600150760328fad06954f0e581a2043f72ebf64b7b656d0eab5beaf0","observation_id":"761c00ee-d50c-4a01-a6ec-670e8fd35b06","resolution":{"observed_at":"2026-05-11T18:26:10.724817Z","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":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":"1902.10048","doi":"10.1103/physrevlett.123.051102","metadata_source":"pith","pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Torres-Forn´ e, P","venue":"gr-qc","work_id":"72f0db17-f4ba-4553-afb6-bf32fdfa1fcd","year":2019},"citing_paper":{"arxiv_id":"2607.06664","last_updated":"2026-07-07T18:00:01Z","snapshot_observed_at":"2026-08-07T09:00:48.980402Z","submitted_at":"2026-07-07T18:00:01Z","title":"Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors","version":1},"reference_index":214,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2607.06664"},"observation_digest":"sha256:d2bdedc71b03a035fa4b04d7fadedbea6ebfa348c754a695e6792ecfc5f92225","observation_id":"15dc55b6-8f1a-4bb0-903e-cd28525c96bc","resolution":{"observed_at":"2026-07-11T00:07:40.914625Z","resolver_source":"local_arxiv","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":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-07-14T12:04:34.767477Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.10396","last_updated":"2026-07-11T16:52:32Z","snapshot_observed_at":"2026-08-06T09:29:12.012546Z","submitted_at":"2026-07-11T16:52:32Z","title":"Strongly interacting matter with criticality induced by modified excluded volume in core-collapse supernova simulations","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-14T12:04:34.767477Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2607.10396"},"observation_digest":"sha256:caa86e096c61056a5635f6ead38f0041f4b6e032dbf8446bcf70ab04b6a40f92","observation_id":"85f4cc7f-a3ef-44d2-84b4-2133396cfd73","resolution":{"observed_at":"2026-07-14T12:04:34.767477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-01T04:14:02.879971Z","title":"Universal Relations for Gravitational-Wave Asteroseismology of Protoneutron Stars","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.22909","last_updated":"2026-07-24T20:54:25Z","snapshot_observed_at":"2026-08-08T04:04:33.668623Z","submitted_at":"2026-07-24T20:54:25Z","title":"Universal relations applied to proto-neutron star generated gravitational waves from three-dimensional core collapse supernova simulations","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-01T04:14:02.879971Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2607.22909"},"observation_digest":"sha256:ba65bbefda8895217bc60f2420f26aa83c1a1df1b67afc87078dbd7279900915","observation_id":"781ea33c-b26e-4387-934e-7ea8dae5840d","resolution":{"observed_at":"2026-08-01T04:14:02.879971Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10048","snapshot_observed_at":"2026-08-08T12:47:49.802574Z","title":"Torres-Forn´ e, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.05456","last_updated":"2026-08-05T23:03:42Z","snapshot_observed_at":"2026-08-09T20:11:04.804953Z","submitted_at":"2026-08-05T23:03:42Z","title":"Reconstructing Core-Collapse Supernova Gravitational-Wave Signals with Transdimensional Bayesian Inference","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-08T12:47:49.802574Z"},"links":{"cited_paper":"/paper/1902.10048","citing_paper":"/paper/2608.05456"},"observation_digest":"sha256:a3201a44aa264fc22b3836616a333d005a74ac031221dc924de88fc3442da617","observation_id":"4fa020ef-8499-4e51-8a74-228c172919fb","resolution":{"observed_at":"2026-08-08T12:47:49.802574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1902.10048/citation-record","integrity":"/paper/1902.10048/integrity","json":"/paper/1902.10048/citation-record.json","paper":"/paper/1902.10048"},"outbound":[],"paper":{"arxiv_id":"1902.10048","last_updated":"2021-11-08T15:54:00Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-07T14:15:27.655641Z","submitted_at":"2019-02-26T16:46:05Z","title":"Universal relations for gravitational-wave asteroseismology of proto-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 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1902.10048."}