{"as_of":"2026-08-09T16:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e91c244e89a45a78e6d6982b2a3a08987e0de41c1f5023a7857ef5bd72a784a0","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T00:54:47.313142Z","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":"2026-06-29T15:43:33.165476Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-08-07T00:54:47.313142Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.12709","last_updated":"2025-07-01T13:57:37Z","snapshot_observed_at":"2026-08-09T13:42:48.950136Z","submitted_at":"2025-06-15T03:43:47Z","title":"Constraints on Dark Energy Models Using Late Universe Probes","version":3},"reference_index":106,"source":"pdf_text","source_observed_at":"2026-08-07T00:54:47.313142Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2506.12709"},"observation_digest":"sha256:745adb908d604005d1152956a72ba644f9d98627bba30658291deea48d6050d2","observation_id":"b6a1356d-d8cc-41f7-89b1-de8cbd1891f4","resolution":{"observed_at":"2026-08-07T00:54:47.313142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":"2502.12667","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-06-29T15:43:33.165476Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","venue":null,"work_id":"5748458d-e391-4d0b-804d-611051f3430e","year":2025},"citing_paper":{"arxiv_id":"2510.18741","last_updated":"2026-04-10T13:03:33Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-21T15:46:25Z","title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","version":2},"reference_index":210,"source":"pdf_text","source_observed_at":"2026-05-18T04:46:14.832965Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2510.18741"},"observation_digest":"sha256:8bb3048f6fbcf3ed4d87c697eb1648c35484a81e7e5a5cecc87eead8081e9329","observation_id":"95ea8dff-4434-4347-bbdd-9cfc903596b1","resolution":{"observed_at":"2026-05-18T04:50:55.493069Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-07-15T14:51:12.413085Z","title":null,"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":46,"source":"pdf_text","source_observed_at":"2026-07-15T14:51:12.413085Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2603.05049"},"observation_digest":"sha256:69a5ede4a687d820176c0d8b99c934c58a227d03efcbf938eccb15db14160209","observation_id":"9119dd78-95ba-41fe-b0eb-1be2ba21f599","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":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":"2502.12667","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-06-29T15:43:33.165476Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","venue":null,"work_id":"5748458d-e391-4d0b-804d-611051f3430e","year":2025},"citing_paper":{"arxiv_id":"2605.22309","last_updated":"2026-07-15T09:02:22Z","snapshot_observed_at":"2026-08-06T01:35:32.177705Z","submitted_at":"2026-05-21T10:55:25Z","title":"Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-22T05:36:41.912431Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2605.22309"},"observation_digest":"sha256:086141795a22fe135959a648491f221cdfd102393aeb585132e4bc51933c1f34","observation_id":"3f821f9c-889c-48a5-a21c-20816c3c46cd","resolution":{"observed_at":"2026-05-22T05:41:08.707994Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-08-02T13:29:55.148946Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.22309","last_updated":"2026-07-15T09:02:22Z","snapshot_observed_at":"2026-08-06T01:35:32.177705Z","submitted_at":"2026-05-21T10:55:25Z","title":"Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-02T13:29:55.148946Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2605.22309"},"observation_digest":"sha256:1459b302a076ac33dbd873c42992ae02017f888eb6077c9c895307f2c0983e35","observation_id":"f2176e5d-b789-414d-bd93-718dae0c7066","resolution":{"observed_at":"2026-08-02T13:29:55.148946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":"2502.12667","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-06-29T15:43:33.165476Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","venue":null,"work_id":"5748458d-e391-4d0b-804d-611051f3430e","year":2025},"citing_paper":{"arxiv_id":"2605.27301","last_updated":"2026-06-02T16:18:10Z","snapshot_observed_at":"2026-08-07T14:11:27.638757Z","submitted_at":"2026-05-26T17:11:30Z","title":"Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-29T15:25:34.466836Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2605.27301"},"observation_digest":"sha256:c574bf9b7dd07e50c58479b0f2cb80bf1caee4f1f38c8722136f624b0dda8637","observation_id":"aa4ff9bb-cb7b-4bd8-8ff3-59c22832bb9d","resolution":{"observed_at":"2026-06-29T15:43:33.167045Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-07-14T16:44:02.461654Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.09732","last_updated":"2026-07-02T07:56:02Z","snapshot_observed_at":"2026-08-04T12:51:14.408110Z","submitted_at":"2026-07-02T07:56:02Z","title":"Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-14T16:44:02.461654Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2607.09732"},"observation_digest":"sha256:3ea407b20018d916add380f7da170a506dd79bf9dbd8cbd8887a9563bce04d18","observation_id":"fca727b8-de3a-4034-95cc-5d72946da7eb","resolution":{"observed_at":"2026-07-14T16:44:02.461654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-07-14T03:00:21.146194Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.11813","last_updated":"2026-07-13T17:09:56Z","snapshot_observed_at":"2026-08-06T13:15:55.562159Z","submitted_at":"2026-07-13T17:09:56Z","title":"Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-14T03:00:21.146194Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2607.11813"},"observation_digest":"sha256:49f2b34a52d6d569b9762153b60c53da75d3ea70f6ea1c44903052c6b30b068a","observation_id":"99b5e7c2-0964-4948-8a05-de5e33837606","resolution":{"observed_at":"2026-07-14T03:00:21.146194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.12667","snapshot_observed_at":"2026-08-06T00:32:11.208976Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.01215","last_updated":"2026-08-02T13:02:59Z","snapshot_observed_at":"2026-08-06T23:26:08.093728Z","submitted_at":"2026-08-02T13:02:59Z","title":"Do we really need alternatives to the $\\omega_0\\omega_a$CDM parameterization after the DESI DR2?","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T00:32:11.208976Z"},"links":{"cited_paper":"/paper/2502.12667","citing_paper":"/paper/2608.01215"},"observation_digest":"sha256:b5c485982f146cf272048ab816bc00af019af651bf0eb5a97dbc87962988f9cd","observation_id":"10ce66c5-c205-4d7c-94c6-7504e88d3440","resolution":{"observed_at":"2026-08-06T00:32:11.208976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2502.12667/citation-record","integrity":"/paper/2502.12667/integrity","json":"/paper/2502.12667/citation-record.json","paper":"/paper/2502.12667"},"outbound":[],"paper":{"arxiv_id":"2502.12667","last_updated":"2025-07-11T17:29:44Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T18:09:46.562682Z","submitted_at":"2025-02-18T09:18:00Z","title":"The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2502.12667."}