{"as_of":"2026-08-16T09:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:36a339cd75ff08006ecd784fba15e7dd635c7617cd06c6570c1e14dc951be5dc","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":"2026-08-16T06:30:59.297886+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":"2026-08-06T21:04:07.266878Z","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":"2026-05-15T17:32:24.949598Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0903.2732","last_updated":"2011-07-14T20:07:00Z","snapshot_observed_at":"2026-08-15T05:52:50.374376Z","submitted_at":"2009-03-16T15:04:44Z","title":"F(R) cosmology in presence of a phantom fluid and its scalar-tensor counterpart:towards a unified precision model of the universe evolution","version":3},"cited_work":{"arxiv_id":"0903.2732","doi":null,"metadata_source":"pith","pith_arxiv_id":"0903.2732","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"F(R) cosmology in presence of a phantom fluid and its scalar-tensor counterpart:towards a unified precision model of the universe evolution","venue":"hep-th","work_id":"47ac9e80-0c68-48f6-8818-5f7d7d250c98","year":2009},"citing_paper":{"arxiv_id":"1705.11098","last_updated":"2021-05-23T13:57:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2017-05-31T13:41:52Z","title":"Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution","version":3},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-05-15T17:32:24.210761Z"},"links":{"cited_paper":"/paper/0903.2732","citing_paper":"/paper/1705.11098"},"observation_digest":"sha256:9729eb071700504230481055b202258334ffc0c3fc3da32cc8df577bb0da9918","observation_id":"232290f8-f843-43c4-a15f-156dbf1aac3b","resolution":{"observed_at":"2026-05-15T17:32:24.952288Z","resolver_source":"local_arxiv","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":"0903.2732","last_updated":"2011-07-14T20:07:00Z","snapshot_observed_at":"2026-08-15T05:52:50.374376Z","submitted_at":"2009-03-16T15:04:44Z","title":"F(R) cosmology in presence of a phantom fluid and its scalar-tensor counterpart:towards a unified precision model of the universe evolution","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.2732","snapshot_observed_at":"2026-08-06T21:04:07.266878Z","title":"Elizalde and D","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.01442","last_updated":"2025-09-09T12:50:25Z","snapshot_observed_at":"2026-08-13T15:36:19.044782Z","submitted_at":"2025-07-02T07:59:16Z","title":"Nonlinear reconstruction of general dark energy theories","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T21:04:07.266878Z"},"links":{"cited_paper":"/paper/0903.2732","citing_paper":"/paper/2507.01442"},"observation_digest":"sha256:a179702ff62747643c4a1999990f67a1658ccd5a44d6e70de063c76d2861170a","observation_id":"f60e2630-60c4-4ffa-803e-1b8e6b9709ae","resolution":{"observed_at":"2026-08-06T21:04:07.266878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/0903.2732/citation-record","integrity":"/paper/0903.2732/integrity","json":"/paper/0903.2732/citation-record.json","paper":"/paper/0903.2732"},"outbound":[],"paper":{"arxiv_id":"0903.2732","last_updated":"2011-07-14T20:07:00Z","latest_version":3,"primary_category":"hep-th","snapshot_observed_at":"2026-08-15T05:52:50.374376Z","submitted_at":"2009-03-16T15:04:44Z","title":"F(R) cosmology in presence of a phantom fluid and its scalar-tensor counterpart:towards a unified precision model of the universe evolution"},"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 2 inbound Pith citation observations for arXiv:0903.2732."}