{"as_of":"2026-08-18T05:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bc983c6cf03e46cb330c48287014d9c48fb0bb9f4d0d75d3624122c3bd0691af","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:44:03.643237Z","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":"2026-07-04T07:49:39.898128Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-08-10T16:45:20.202439Z","title":"Bednarek, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.12905","last_updated":"2025-06-02T08:26:49Z","snapshot_observed_at":"2026-08-16T00:10:28.609111Z","submitted_at":"2025-01-22T14:33:08Z","title":"The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T16:45:20.202439Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2501.12905"},"observation_digest":"sha256:b10a497fed7833052ca44f9fd5101ed9b22ffedb23c822163a2c0994434e4a0c","observation_id":"d9da9643-40fc-4c06-8158-6f20ae335cbc","resolution":{"observed_at":"2026-08-10T16:45:20.202439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-08-16T05:44:03.643237Z","title":"Bednarek, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2504.19962","last_updated":"2025-07-09T09:30:24Z","snapshot_observed_at":"2026-08-18T00:00:34.274176Z","submitted_at":"2025-04-28T16:33:55Z","title":"Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-16T05:44:03.643237Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2504.19962"},"observation_digest":"sha256:498c0ab1f77dca5c852309124ba3c0efbc24d483cfd1a1e181c5490a27b4c36b","observation_id":"539ff4ae-df47-4da5-bf31-75f9dcdfcdbf","resolution":{"observed_at":"2026-08-16T05:44:03.643237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-08-06T10:19:22.334185Z","title":"Bednarek, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.00236","last_updated":"2026-06-23T06:11:02Z","snapshot_observed_at":"2026-08-12T18:34:14.675852Z","submitted_at":"2025-08-01T00:47:10Z","title":"Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T10:19:22.334185Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2508.00236"},"observation_digest":"sha256:f0c87569da4f118ea5e9cb65b7d9e70acf859d74da52fc97b732fcc7150ba81a","observation_id":"48737cfc-9137-4ea8-8ab5-93fca9bcfa9e","resolution":{"observed_at":"2026-08-06T10:19:22.334185Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-08-03T20:20:19.470532Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.20378","last_updated":"2026-06-28T03:18:05Z","snapshot_observed_at":"2026-08-16T23:47:23.753728Z","submitted_at":"2025-11-25T14:59:28Z","title":"Toward a Unified Understanding of the Dense Matter Equation of State","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-03T20:20:19.470532Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2511.20378"},"observation_digest":"sha256:f165b731076def5e2cf91a9c878b466781fb9e139b2ae8b452a4e18679a1c31b","observation_id":"5a246a3f-203e-4668-828b-b985ec5c61b3","resolution":{"observed_at":"2026-08-03T20:20:19.470532Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":"1111.6942","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-07-04T07:49:39.898128Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","venue":"astro-ph.SR","work_id":"52b604e9-54b8-49e6-adff-5a67385b543b","year":2011},"citing_paper":{"arxiv_id":"2606.21617","last_updated":"2026-06-19T17:21:27Z","snapshot_observed_at":"2026-08-13T14:50:21.420397Z","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":8,"source":"pdf_text","source_observed_at":"2026-06-26T12:34:28.137843Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2606.21617"},"observation_digest":"sha256:a2ec50cf0bd0e3b8ae0da5fc08db75e0379be953d3f844757de205c15faba7aa","observation_id":"943e52da-a6fa-4df2-a5bc-8c8c91540e82","resolution":{"observed_at":"2026-07-04T07:49:39.899321Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-07-13T04:22:12.472403Z","title":"Bednarek, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.09255","last_updated":"2026-07-10T10:10:02Z","snapshot_observed_at":"2026-08-14T14:33:49.972316Z","submitted_at":"2026-07-10T10:10:02Z","title":"Accelerator neutrinos as a probe of in-medium hyperon potentials","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-13T04:22:12.472403Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2607.09255"},"observation_digest":"sha256:9b8b895b09c9d26fa665de58941f9b812fb1d4d079dd6029fa91438d9f7888a7","observation_id":"5812cae6-17eb-4607-8850-2d4a83c40fcf","resolution":{"observed_at":"2026-07-13T04:22:12.472403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-07-13T04:14:25.041579Z","title":"Bednarek, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.09273","last_updated":"2026-07-10T10:42:23Z","snapshot_observed_at":"2026-08-13T10:45:22.204358Z","submitted_at":"2026-07-10T10:42:23Z","title":"Neutrino-induced hyperon final-state interactions as constraints on the in-medium hyperon potential","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-13T04:14:25.041579Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2607.09273"},"observation_digest":"sha256:cd9890645706f2aec81c333dc39de39c454dd36da862d7ac44b46498de44294a","observation_id":"8683cf02-ba2c-4411-b115-d4040a0c06dc","resolution":{"observed_at":"2026-07-13T04:14:25.041579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.6942","snapshot_observed_at":"2026-07-13T04:12:01.548194Z","title":"Bednarek, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.09280","last_updated":"2026-07-10T10:49:02Z","snapshot_observed_at":"2026-08-14T14:43:06.613199Z","submitted_at":"2026-07-10T10:49:02Z","title":"In-medium hyperon potentials and the quarkyonic hyperon onset: charged $\\Sigma$'s in $\\beta$-equilibrium and the neutrino connection","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-13T04:12:01.548194Z"},"links":{"cited_paper":"/paper/1111.6942","citing_paper":"/paper/2607.09280"},"observation_digest":"sha256:e823889a59984e55b34cd28a635976294b8c3e2bce360451a790bfa91b562666","observation_id":"d1beb470-47f0-4f71-89f9-398d99f8d0c1","resolution":{"observed_at":"2026-07-13T04:12:01.548194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1111.6942/citation-record","integrity":"/paper/1111.6942/integrity","json":"/paper/1111.6942/citation-record.json","paper":"/paper/1111.6942"},"outbound":[],"paper":{"arxiv_id":"1111.6942","last_updated":"2011-11-29T19:30:32Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-17T22:40:35.902884Z","submitted_at":"2011-11-29T19:30:32Z","title":"Hyperons in neutron-star cores and two-solar-mass pulsar"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1111.6942."}