{"as_of":"2026-08-08T02:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7e1502297802a4280896fbced63de04e56d277c9c1a49b1430d967a550d22946","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T15:59:42.962112Z","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":"2026-06-30T20:45:03.744012Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-08-06T15:59:42.962112Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.14591","last_updated":"2025-07-23T11:04:42Z","snapshot_observed_at":"2026-08-07T04:42:34.896430Z","submitted_at":"2025-07-19T12:27:51Z","title":"Properties of compact objects in quadratic non-metricity gravity","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T15:59:42.962112Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2507.14591"},"observation_digest":"sha256:624beffbb9c0fd17f3ba073696e6fcbbf56a2f9501b7f67192fea61533258bb1","observation_id":"19458779-9ddd-4a4f-be37-40939300dcec","resolution":{"observed_at":"2026-08-06T15:59:42.962112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-08-06T15:00:21.595621Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.17384","last_updated":"2025-07-23T10:26:46Z","snapshot_observed_at":"2026-08-07T00:53:51.103153Z","submitted_at":"2025-07-23T10:26:46Z","title":"Mass-Gap Neutron Stars from Vector \\texorpdfstring{$f(R)$}{f(R)} Gravity Inflationary Deformations","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T15:00:21.595621Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2507.17384"},"observation_digest":"sha256:3c304000830dafb7273964a00f192a8b4c11e982337950abd554d5598996ccb2","observation_id":"a6627d05-6ff7-41a1-9f51-88a1e34ebf94","resolution":{"observed_at":"2026-08-06T15:00:21.595621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-08-04T16:52:12.670992Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.11647","last_updated":"2026-07-31T01:59:15Z","snapshot_observed_at":"2026-08-07T00:46:29.520625Z","submitted_at":"2025-09-15T07:35:34Z","title":"A no-go theorem in bumblebee vector-tensor cosmology","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-04T16:52:12.670992Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2509.11647"},"observation_digest":"sha256:6c88e2f6b24e9e04813ea88cc0bb3effe6bf781eb43662b6ed65fc6cb802182b","observation_id":"9e55caea-4cec-4c54-8232-72a92b6c43dd","resolution":{"observed_at":"2026-08-04T16:52:12.670992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":"1912.05202","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-06-30T20:45:03.744012Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges","venue":null,"work_id":"c4db0c9f-f699-4200-86b6-b006c8746697","year":2020},"citing_paper":{"arxiv_id":"2509.25305","last_updated":"2026-05-15T10:25:52Z","snapshot_observed_at":"2026-07-06T22:31:10.099674Z","submitted_at":"2025-09-29T18:00:00Z","title":"$\\phi$-Dwarfs: White Dwarfs probe Quadratically Coupled Scalars","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-21T21:38:33.685810Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2509.25305"},"observation_digest":"sha256:c528408374df1e50d816eb878e856b23b44e55e0336a320adee7cb2a30596e92","observation_id":"095fcca0-27ca-4e25-944e-3c158c7b8a2d","resolution":{"observed_at":"2026-05-21T21:40:40.502730Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":"1912.05202","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-06-30T20:45:03.744012Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges","venue":null,"work_id":"c4db0c9f-f699-4200-86b6-b006c8746697","year":2020},"citing_paper":{"arxiv_id":"2601.17848","last_updated":"2026-04-08T09:51:55Z","snapshot_observed_at":"2026-07-06T22:42:57.796038Z","submitted_at":"2026-01-25T14:10:38Z","title":"Three dimensional black bounces in $f(R)$ gravity","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-16T11:22:15.942852Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2601.17848"},"observation_digest":"sha256:defac112eb8c0b753af23edc2bbd9fa77373c81f43a5e98a37cb4203cc5416b5","observation_id":"38a34e97-30af-4526-b512-27a36088037f","resolution":{"observed_at":"2026-05-16T11:22:48.073401Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":"1912.05202","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-06-30T20:45:03.744012Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges","venue":null,"work_id":"c4db0c9f-f699-4200-86b6-b006c8746697","year":2020},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-02T14:17:03.153933Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-06-30T20:41:44.418504Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:7b5393ac6ead369802d3354136ec9698928dd16b7f3514fb3815ad4a71146154","observation_id":"bf39ce9b-d6c7-4027-b805-863488f4e3ad","resolution":{"observed_at":"2026-06-30T20:45:03.745689Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-08-02T14:17:05.056207Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.14711","last_updated":"2026-07-22T06:49:38Z","snapshot_observed_at":"2026-08-02T14:17:03.153933Z","submitted_at":"2026-05-14T11:29:03Z","title":"Black holes and neutron stars in massive Hellings-Nordtvedt theory","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-02T14:17:05.056207Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2605.14711"},"observation_digest":"sha256:39fd376caa9c2342fabb373050ac7aa2a8d9269c8cb1ac58201c9df085c76581","observation_id":"fc3c1a4f-dfbc-4d1b-8d6d-344b2c9cc0a2","resolution":{"observed_at":"2026-08-02T14:17:05.056207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":"1912.05202","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-06-30T20:45:03.744012Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges","venue":null,"work_id":"c4db0c9f-f699-4200-86b6-b006c8746697","year":2020},"citing_paper":{"arxiv_id":"2605.19731","last_updated":"2026-07-22T00:32:36Z","snapshot_observed_at":"2026-08-02T13:44:04.267230Z","submitted_at":"2026-05-19T12:05:32Z","title":"Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-20T04:20:10.592465Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2605.19731"},"observation_digest":"sha256:2a74dbc0ee6a2340e521248b6079d5458b9419caa8dcebf061ba55d691b335be","observation_id":"95cee662-9333-4bbd-a519-a69a4d6e7548","resolution":{"observed_at":"2026-05-20T04:23:03.843636Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-08-02T13:44:07.833396Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2605.19731","last_updated":"2026-07-22T00:32:36Z","snapshot_observed_at":"2026-08-02T13:44:04.267230Z","submitted_at":"2026-05-19T12:05:32Z","title":"Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-02T13:44:07.833396Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2605.19731"},"observation_digest":"sha256:608c7180fe4debd5f3d90b26778c820600efbc8a290f08cf4e457b053fd0363a","observation_id":"178841a2-abc8-4d55-bd2a-69b4ea8cf689","resolution":{"observed_at":"2026-08-02T13:44:07.833396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges","version":2},"cited_work":{"arxiv_id":"1912.05202","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05202","snapshot_observed_at":"2026-06-30T20:45:03.744012Z","title":"Stellar structure models in modified theories of gravity: Lessons and challenges","venue":null,"work_id":"c4db0c9f-f699-4200-86b6-b006c8746697","year":2020},"citing_paper":{"arxiv_id":"2605.27170","last_updated":"2026-05-26T15:26:35Z","snapshot_observed_at":"2026-07-06T23:36:53.330986Z","submitted_at":"2026-05-26T15:26:35Z","title":"Regular black hole solutions and the quark chemical potential at the QCD phase transition","version":1},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-06-29T15:52:43.514424Z"},"links":{"cited_paper":"/paper/1912.05202","citing_paper":"/paper/2605.27170"},"observation_digest":"sha256:9f4485177c1315973a65eb75fc196ee70d755f5242c461f2a845704d4ed1f4f4","observation_id":"3e31d52f-321a-46db-b208-1bab6d238fec","resolution":{"observed_at":"2026-06-29T16:13:36.388929Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1912.05202/citation-record","integrity":"/paper/1912.05202/integrity","json":"/paper/1912.05202/citation-record.json","paper":"/paper/1912.05202"},"outbound":[],"paper":{"arxiv_id":"1912.05202","last_updated":"2020-07-08T12:49:23Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T08:43:39.917391Z","submitted_at":"2019-12-11T09:41:57Z","title":"Stellar structure models in modified theories of gravity: lessons and challenges"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1912.05202."}