{"as_of":"2026-08-16T18:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7ee7da6b0edadc49507be406d8e69300824a8a18988d7fdd650a0e11adb5a945","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:43:40.278521Z","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":"2026-05-21T11:15:02.231026Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2206.12910","last_updated":"2022-06-26T15:48:10Z","snapshot_observed_at":"2026-08-16T16:50:18.776540Z","submitted_at":"2022-06-26T15:48:10Z","title":"Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.12910","snapshot_observed_at":"2026-08-16T12:43:40.278521Z","title":"Jizba and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.12205","last_updated":"2025-09-05T12:05:34Z","snapshot_observed_at":"2026-08-16T12:33:11.569499Z","submitted_at":"2025-04-16T15:54:06Z","title":"Barrow and Tsallis entropies after the DESI DR2 BAO data","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T12:43:40.278521Z"},"links":{"cited_paper":"/paper/2206.12910","citing_paper":"/paper/2504.12205"},"observation_digest":"sha256:d74d3bf4f61f1dee194e13f9a65918d3377ced2b8e12adb647d5b396dc0a80d4","observation_id":"e6c2b17e-7a7c-4335-8dfd-80fb1d7d0d3f","resolution":{"observed_at":"2026-08-16T12:43:40.278521Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.12910","last_updated":"2022-06-26T15:48:10Z","snapshot_observed_at":"2026-08-16T16:50:18.776540Z","submitted_at":"2022-06-26T15:48:10Z","title":"Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.12910","snapshot_observed_at":"2026-08-03T23:47:54.300441Z","title":"Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.04613","last_updated":"2026-05-28T12:22:43Z","snapshot_observed_at":"2026-08-14T01:16:08.433886Z","submitted_at":"2025-11-06T18:05:18Z","title":"Effective matter sectors from modified entropies","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T23:47:54.300441Z"},"links":{"cited_paper":"/paper/2206.12910","citing_paper":"/paper/2511.04613"},"observation_digest":"sha256:114e81d8bc332f8873e8905b3515da6dd1c536b4d4fdf7004262aad3ed07116a","observation_id":"9d318cdc-2efa-49bf-887c-809448178780","resolution":{"observed_at":"2026-08-03T23:47:54.300441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.12910","last_updated":"2022-06-26T15:48:10Z","snapshot_observed_at":"2026-08-16T16:50:18.776540Z","submitted_at":"2022-06-26T15:48:10Z","title":"Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data","version":1},"cited_work":{"arxiv_id":"2206.12910","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.12910","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Jizba and G","venue":null,"work_id":"efe79348-52b5-4da9-96d4-3c62a8489aab","year":2022},"citing_paper":{"arxiv_id":"2603.03568","last_updated":"2026-05-20T08:27:13Z","snapshot_observed_at":"2026-08-14T08:56:51.368017Z","submitted_at":"2026-03-03T22:54:28Z","title":"Observational constraints on Luciano-Saridakis entropic cosmology","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-21T11:14:52.779018Z"},"links":{"cited_paper":"/paper/2206.12910","citing_paper":"/paper/2603.03568"},"observation_digest":"sha256:2146b7b6a9ba9f8c23d91d8774440d428773b9b73d0faaee01e537e3261e9721","observation_id":"5f627bab-c535-48d0-b85d-4c5b7aff7ffb","resolution":{"observed_at":"2026-05-21T11:15:02.232976Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.12910","last_updated":"2022-06-26T15:48:10Z","snapshot_observed_at":"2026-08-16T16:50:18.776540Z","submitted_at":"2022-06-26T15:48:10Z","title":"Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.12910","snapshot_observed_at":"2026-08-15T14:31:40.591949Z","title":"Jizba and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.10495","last_updated":"2026-08-11T05:11:44Z","snapshot_observed_at":"2026-08-16T02:55:57.101369Z","submitted_at":"2026-08-11T05:11:44Z","title":"The generalized second law as a thermodynamic selection criterion for dynamical dark energy","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-15T14:31:40.591949Z"},"links":{"cited_paper":"/paper/2206.12910","citing_paper":"/paper/2608.10495"},"observation_digest":"sha256:6c274938a4968c6b13ce7df4098e27c3f7714c8151e122cb04403b50d6ca8b03","observation_id":"9516e648-9360-4689-b8ac-616f7dc6315c","resolution":{"observed_at":"2026-08-15T14:31:40.591949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2206.12910/citation-record","integrity":"/paper/2206.12910/integrity","json":"/paper/2206.12910/citation-record.json","paper":"/paper/2206.12910"},"outbound":[],"paper":{"arxiv_id":"2206.12910","last_updated":"2022-06-26T15:48:10Z","latest_version":1,"primary_category":"hep-th","snapshot_observed_at":"2026-08-16T16:50:18.776540Z","submitted_at":"2022-06-26T15:48:10Z","title":"Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2206.12910."}