{"as_of":"2026-08-18T03:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:45f1c07652609f67ef9cbce83426e314dc814564bc7a98067eac25bf2cff5a19","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:19:56.317578Z","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":"2026-08-07T11:24:28.751827Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1107.4816","last_updated":"2011-12-24T22:17:35Z","snapshot_observed_at":"2026-08-17T17:14:24.837765Z","submitted_at":"2011-07-25T00:08:44Z","title":"Interacting dark matter and modified holographic Ricci dark energy induce a relaxed Chaplygin gas","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.4816","snapshot_observed_at":"2026-08-16T05:19:56.317578Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.21110","last_updated":"2025-07-19T00:40:01Z","snapshot_observed_at":"2026-08-17T21:33:14.327503Z","submitted_at":"2025-04-29T18:39:48Z","title":"The frozen vanilla model: Exploring dark sector interactions with delta effective theories","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-16T05:19:56.317578Z"},"links":{"cited_paper":"/paper/1107.4816","citing_paper":"/paper/2504.21110"},"observation_digest":"sha256:21713cdbbee5d0913749dd6557a0af476436e0a3c80118bcf2a6067a2abdfe68","observation_id":"898a1504-c13c-49a3-ad45-99e174c528cc","resolution":{"observed_at":"2026-08-16T05:19:56.317578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.4816","last_updated":"2011-12-24T22:17:35Z","snapshot_observed_at":"2026-08-17T17:14:24.837765Z","submitted_at":"2011-07-25T00:08:44Z","title":"Interacting dark matter and modified holographic Ricci dark energy induce a relaxed Chaplygin gas","version":3},"cited_work":{"arxiv_id":"1107.4816","doi":null,"metadata_source":"pith","pith_arxiv_id":"1107.4816","snapshot_observed_at":"2026-08-07T11:24:28.751827Z","title":"Interacting dark matter and modified holographic Ricci dark energy induce a relaxed Chaplygin gas","venue":"astro-ph.CO","work_id":"a2a697c1-85d2-4038-8dad-b463190f477f","year":2011},"citing_paper":{"arxiv_id":"2506.03019","last_updated":"2025-06-03T15:56:26Z","snapshot_observed_at":"2026-08-14T01:48:45.084629Z","submitted_at":"2025-06-03T15:56:26Z","title":"Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T11:24:20.735210Z"},"links":{"cited_paper":"/paper/1107.4816","citing_paper":"/paper/2506.03019"},"observation_digest":"sha256:dd735a8238b225ee67078ffb769373ec9723263219512b814742357bec8019d5","observation_id":"8c495432-6e7d-4af3-bfaf-fc3ab2c6f7dc","resolution":{"observed_at":"2026-08-07T11:24:28.797251Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/1107.4816/citation-record","integrity":"/paper/1107.4816/integrity","json":"/paper/1107.4816/citation-record.json","paper":"/paper/1107.4816"},"outbound":[],"paper":{"arxiv_id":"1107.4816","last_updated":"2011-12-24T22:17:35Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T17:14:24.837765Z","submitted_at":"2011-07-25T00:08:44Z","title":"Interacting dark matter and modified holographic Ricci dark energy induce a relaxed Chaplygin gas"},"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 2 inbound Pith citation observations for arXiv:1107.4816."}