{"as_of":"2026-08-05T04:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:af1b8d412d060515a9827f4e90541386c154842bb1309060ccb2fd6259ceacc6","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":"2026-08-04T06:34:03.388597+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":"2026-08-03T13:44:09.577717Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-04T07:49:39.911657Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1111.6049","last_updated":"2012-04-27T14:37:52Z","snapshot_observed_at":"2026-07-06T02:38:13.099660Z","submitted_at":"2011-11-25T16:48:20Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","version":3},"cited_work":{"arxiv_id":"1111.6049","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.6049","snapshot_observed_at":"2026-07-04T07:49:39.911657Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","venue":"astro-ph.HE","work_id":"da19da2e-c704-44c2-9800-bd4c54bcdd1b","year":2011},"citing_paper":{"arxiv_id":"1907.03549","last_updated":"2019-07-05T10:16:33Z","snapshot_observed_at":"2026-07-06T08:05:48.377851Z","submitted_at":"2019-07-05T10:16:33Z","title":"Anisotropic strange quark stars with a non-linear equation-of-state","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-25T02:25:09.067764Z"},"links":{"cited_paper":"/paper/1111.6049","citing_paper":"/paper/1907.03549"},"observation_digest":"sha256:3f11e4431e29de76e2ebf7231711f84a3f59857839bef3ed9d0b6a13fc3e5e12","observation_id":"5f7b5472-1a6d-4e20-b372-dd1b0079821d","resolution":{"observed_at":"2026-05-25T02:25:14.592719Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6049","last_updated":"2012-04-27T14:37:52Z","snapshot_observed_at":"2026-07-06T02:38:13.099660Z","submitted_at":"2011-11-25T16:48:20Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","version":3},"cited_work":{"arxiv_id":"1111.6049","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.6049","snapshot_observed_at":"2026-07-04T07:49:39.911657Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","venue":"astro-ph.HE","work_id":"da19da2e-c704-44c2-9800-bd4c54bcdd1b","year":2011},"citing_paper":{"arxiv_id":"2504.18764","last_updated":"2026-04-20T20:15:29Z","snapshot_observed_at":"2026-07-06T21:15:02.308553Z","submitted_at":"2025-04-26T01:56:18Z","title":"Symmetry Energy Expansion with Strange Dense Matter","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-22T18:20:24.680116Z"},"links":{"cited_paper":"/paper/1111.6049","citing_paper":"/paper/2504.18764"},"observation_digest":"sha256:aa01e5b9f6cd868b419519c81c7478ba1eb827141b9cacdb8f3df3306ecafc81","observation_id":"57e82cf2-3cf6-4fec-9d0c-28bb9508f1ca","resolution":{"observed_at":"2026-05-22T18:21:55.403878Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6049","last_updated":"2012-04-27T14:37:52Z","snapshot_observed_at":"2026-07-06T02:38:13.099660Z","submitted_at":"2011-11-25T16:48:20Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","version":3},"cited_work":{"arxiv_id":"1111.6049","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.6049","snapshot_observed_at":"2026-07-04T07:49:39.911657Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","venue":"astro-ph.HE","work_id":"da19da2e-c704-44c2-9800-bd4c54bcdd1b","year":2011},"citing_paper":{"arxiv_id":"2511.07567","last_updated":"2026-04-14T18:19:15Z","snapshot_observed_at":"2026-07-06T22:35:27.050353Z","submitted_at":"2025-11-10T19:22:59Z","title":"Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-17T23:10:30.793407Z"},"links":{"cited_paper":"/paper/1111.6049","citing_paper":"/paper/2511.07567"},"observation_digest":"sha256:8bcb94e2303328329a35a06de3fb222c6bf8ae33317a00282b729d53c7c3409e","observation_id":"eed6fa80-5f5a-4514-9e3a-7df8148c65d8","resolution":{"observed_at":"2026-05-17T23:12:12.083872Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6049","last_updated":"2012-04-27T14:37:52Z","snapshot_observed_at":"2026-07-06T02:38:13.099660Z","submitted_at":"2011-11-25T16:48:20Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6049","snapshot_observed_at":"2026-08-03T13:44:09.577717Z","title":"Weissenborn, D","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2512.23477","last_updated":"2026-07-06T15:41:51Z","snapshot_observed_at":"2026-08-03T13:44:07.338883Z","submitted_at":"2025-12-29T14:01:25Z","title":"Compact star and compact star matter properties from a baryonic extended linear sigma model with explicit chiral symmetry breaking","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T13:44:09.577717Z"},"links":{"cited_paper":"/paper/1111.6049","citing_paper":"/paper/2512.23477"},"observation_digest":"sha256:0b4ebf57560aded101886cd170c01bfaaa6539ce5b818d60b7d2c630a8e59932","observation_id":"483db9c7-5f61-4c43-8db3-e3b87187f909","resolution":{"observed_at":"2026-08-03T13:44:09.577717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6049","last_updated":"2012-04-27T14:37:52Z","snapshot_observed_at":"2026-07-06T02:38:13.099660Z","submitted_at":"2011-11-25T16:48:20Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","version":3},"cited_work":{"arxiv_id":"1111.6049","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.6049","snapshot_observed_at":"2026-07-04T07:49:39.911657Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials","venue":"astro-ph.HE","work_id":"da19da2e-c704-44c2-9800-bd4c54bcdd1b","year":2011},"citing_paper":{"arxiv_id":"2606.21617","last_updated":"2026-06-19T17:21:27Z","snapshot_observed_at":"2026-07-06T23:56:35.743669Z","submitted_at":"2026-06-19T17:21:27Z","title":"Hyperonic equation of state for neutron stars: A systematic Bayesian comparison of density-dependent and non-linear relativistic mean-field models","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-26T12:34:28.137843Z"},"links":{"cited_paper":"/paper/1111.6049","citing_paper":"/paper/2606.21617"},"observation_digest":"sha256:be17da72d0ee771b1fc2384c519a873303891a1d6536c93231e12a86db752da6","observation_id":"572d2374-a75a-4be8-90ec-e85c9401188c","resolution":{"observed_at":"2026-07-04T07:49:39.912841Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1111.6049/citation-record","integrity":"/paper/1111.6049/integrity","json":"/paper/1111.6049/citation-record.json","paper":"/paper/1111.6049"},"outbound":[],"paper":{"arxiv_id":"1111.6049","last_updated":"2012-04-27T14:37:52Z","latest_version":3,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T02:38:13.099660Z","submitted_at":"2011-11-25T16:48:20Z","title":"Hyperons and massive neutron stars: the role of hyperon potentials"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1111.6049."}