{"as_of":"2026-08-11T19:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b83ba1976d66a714cc7f1a7472e73826c54f585171b2bf1b702b272d0fe1fdc1","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T11:24:24.041422Z","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":"2026-05-13T17:38:03.089749Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.19352","last_updated":"2025-07-05T07:11:09Z","snapshot_observed_at":"2026-08-07T16:39:20.981394Z","submitted_at":"2025-03-25T05:02:44Z","title":"Evolution of clustering in cosmological models with time-varying dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19352","snapshot_observed_at":"2026-08-07T11:24:24.041422Z","title":"Ishiyama, F","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.03019","last_updated":"2025-06-03T15:56:26Z","snapshot_observed_at":"2026-08-10T20:04:50.832035Z","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":81,"source":"pdf_text","source_observed_at":"2026-08-07T11:24:24.041422Z"},"links":{"cited_paper":"/paper/2503.19352","citing_paper":"/paper/2506.03019"},"observation_digest":"sha256:2ced1b316a06688c568c20b48423f9e19128a55e87a476e01a5a626fa5b2892e","observation_id":"8249be73-5a7b-4944-b595-51df397bcb30","resolution":{"observed_at":"2026-08-07T11:24:24.041422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19352","last_updated":"2025-07-05T07:11:09Z","snapshot_observed_at":"2026-08-07T16:39:20.981394Z","submitted_at":"2025-03-25T05:02:44Z","title":"Evolution of clustering in cosmological models with time-varying dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19352","snapshot_observed_at":"2026-08-06T19:22:36.030506Z","title":"Ishiyama, F","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.05975","last_updated":"2025-07-08T13:29:42Z","snapshot_observed_at":"2026-08-09T11:44:31.957762Z","submitted_at":"2025-07-08T13:29:42Z","title":"Constraint on Symmetric Teleparallel Gravity with Different Dark energy Parametrizations from DESI DR2 BAO Data","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T19:22:36.030506Z"},"links":{"cited_paper":"/paper/2503.19352","citing_paper":"/paper/2507.05975"},"observation_digest":"sha256:317e283816ecf297f602d8e83dcf25fa0a7167b7ab9e047ba195fde44b43616c","observation_id":"1703f019-1c67-4989-85f3-d17212342d40","resolution":{"observed_at":"2026-08-06T19:22:36.030506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19352","last_updated":"2025-07-05T07:11:09Z","snapshot_observed_at":"2026-08-07T16:39:20.981394Z","submitted_at":"2025-03-25T05:02:44Z","title":"Evolution of clustering in cosmological models with time-varying dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19352","snapshot_observed_at":"2026-08-04T13:43:12.236432Z","title":"Ishiyama, F","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.25812","last_updated":"2026-07-24T17:00:01Z","snapshot_observed_at":"2026-08-06T01:07:38.127403Z","submitted_at":"2025-09-30T05:41:44Z","title":"Updated observational constraints on $\\phi$CDM dynamical dark energy cosmological models","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-04T13:43:12.236432Z"},"links":{"cited_paper":"/paper/2503.19352","citing_paper":"/paper/2509.25812"},"observation_digest":"sha256:92572f24494934b32d17c981895200a274c45c3f4abb452e31f49f00ae44c91b","observation_id":"79158f8c-c2a7-4142-8f49-a6ec899588a4","resolution":{"observed_at":"2026-08-04T13:43:12.236432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19352","last_updated":"2025-07-05T07:11:09Z","snapshot_observed_at":"2026-08-07T16:39:20.981394Z","submitted_at":"2025-03-25T05:02:44Z","title":"Evolution of clustering in cosmological models with time-varying dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19352","snapshot_observed_at":"2026-07-15T14:51:12.413085Z","title":"Ishiyama, F","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.05049","last_updated":"2026-07-07T11:57:15Z","snapshot_observed_at":"2026-08-06T09:46:44.861202Z","submitted_at":"2026-03-05T10:59:03Z","title":"Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-15T14:51:12.413085Z"},"links":{"cited_paper":"/paper/2503.19352","citing_paper":"/paper/2603.05049"},"observation_digest":"sha256:bdca79451fadb2c2660b201dd4ae35bdca72ce17f7c2169ebc367c58deddd942","observation_id":"5c906e85-3699-4657-bd1d-97371df409d4","resolution":{"observed_at":"2026-07-15T14:51:12.413085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19352","last_updated":"2025-07-05T07:11:09Z","snapshot_observed_at":"2026-08-07T16:39:20.981394Z","submitted_at":"2025-03-25T05:02:44Z","title":"Evolution of clustering in cosmological models with time-varying dark energy","version":3},"cited_work":{"arxiv_id":"2503.19352","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.19352","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ishiyama, F","venue":null,"work_id":"e2a6b008-cd0a-4cc6-a30a-345f7684acb0","year":2025},"citing_paper":{"arxiv_id":"2604.03756","last_updated":"2026-04-07T02:58:46Z","snapshot_observed_at":"2026-08-11T12:35:38.561855Z","submitted_at":"2026-04-04T15:05:07Z","title":"Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data?","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-13T17:33:08.222231Z"},"links":{"cited_paper":"/paper/2503.19352","citing_paper":"/paper/2604.03756"},"observation_digest":"sha256:63a53dd39720fbbc7f139baa8fbfd2155cffe81e4c817db0ca3ea0cc6c66b429","observation_id":"709bce29-f7d0-4656-8644-d123c13a1b0a","resolution":{"observed_at":"2026-05-13T17:38:03.091379Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2503.19352/citation-record","integrity":"/paper/2503.19352/integrity","json":"/paper/2503.19352/citation-record.json","paper":"/paper/2503.19352"},"outbound":[],"paper":{"arxiv_id":"2503.19352","last_updated":"2025-07-05T07:11:09Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T16:39:20.981394Z","submitted_at":"2025-03-25T05:02:44Z","title":"Evolution of clustering in cosmological models with time-varying dark energy"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2503.19352."}