{"as_of":"2026-08-10T07:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:42efbba15e3ce97822d2d8b991afd246981116e34c1118092be72f346889413d","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":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T21:04:17.765529Z","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":"2026-07-03T08:17:45.441481Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-08T21:04:17.765529Z","title":"Alfano and O","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04929","last_updated":"2025-05-14T14:57:09Z","snapshot_observed_at":"2026-08-08T20:55:05.610325Z","submitted_at":"2025-02-07T13:49:14Z","title":"Robustness of dark energy phenomenology across different parameterizations","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-08T21:04:17.765529Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2502.04929"},"observation_digest":"sha256:83d17ebd3c2c8ff454824d108c979f6476030e3f838d29d083e21eab9df7f2f1","observation_id":"dff8f3c2-7cb7-4050-a828-5896878dc0f8","resolution":{"observed_at":"2026-08-08T21:04:17.765529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-07T11:24:22.244527Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.03019","last_updated":"2025-06-03T15:56:26Z","snapshot_observed_at":"2026-08-09T03:21:02.776928Z","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":63,"source":"pdf_text","source_observed_at":"2026-08-07T11:24:22.244527Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2506.03019"},"observation_digest":"sha256:597a6d2f5ab7e60f8502e01243b434e27ac4ce0cad8b3f8d1470572b5800cccb","observation_id":"78524ae0-5757-4fc5-9ca3-e777de514d0c","resolution":{"observed_at":"2026-08-07T11:24:22.244527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-06T23:52:23.784358Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.16223","last_updated":"2025-06-19T11:28:24Z","snapshot_observed_at":"2026-08-10T03:41:33.515537Z","submitted_at":"2025-06-19T11:28:24Z","title":"Observational Constraints on Scalar Field--Matter Interaction in Weyl Integrable Spacetime","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T23:52:23.784358Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2506.16223"},"observation_digest":"sha256:4dab6a4887718cb184ac3aae15ffedea5aefc064bad926758cee9607b3e17439","observation_id":"30c99be7-1ddb-4f56-b602-fe20b393bf95","resolution":{"observed_at":"2026-08-06T23:52:23.784358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-06T19:22:35.954623Z","title":null,"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":40,"source":"pdf_text","source_observed_at":"2026-08-06T19:22:35.954623Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2507.05975"},"observation_digest":"sha256:11b95f5f0e26cc81f6ac437c9b7d6f9d5077e7c26b256847d361d8b905c8dac2","observation_id":"7e811b87-1e0e-48de-a565-b47d9eb3b849","resolution":{"observed_at":"2026-08-06T19:22:35.954623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-06T12:47:16.750303Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.21580","last_updated":"2025-07-29T08:33:50Z","snapshot_observed_at":"2026-08-10T02:00:51.765511Z","submitted_at":"2025-07-29T08:33:50Z","title":"Bondi accretion disk luminosity around neutral and charged Simpson-Visser spacetimes","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T12:47:16.750303Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2507.21580"},"observation_digest":"sha256:02b0738b2525fc3dd6c4e311eeb22133c127aff43d9ef34490d2a831a6f09b83","observation_id":"82a1e333-1caf-46a0-b45c-350b81d1e010","resolution":{"observed_at":"2026-08-06T12:47:16.750303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":"2501.15233","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-07-03T08:17:45.441481Z","title":"Alfano and O","venue":null,"work_id":"92e45f16-db21-433c-b4b3-14931067f889","year":2024},"citing_paper":{"arxiv_id":"2603.27616","last_updated":"2026-04-09T07:03:12Z","snapshot_observed_at":"2026-07-06T22:51:00.579062Z","submitted_at":"2026-03-29T10:21:42Z","title":"Model-independent test of the cosmic distance duality relation with recent observational data","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-05-14T22:11:51.900263Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2603.27616"},"observation_digest":"sha256:18b4eabfb11391f13295fa61af476d137d85d4496e8eab150464ee5e55cfa202","observation_id":"4facc10b-cd1d-435a-9796-379c36823526","resolution":{"observed_at":"2026-05-14T22:13:04.363217Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":"2501.15233","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-07-03T08:17:45.441481Z","title":"Alfano and O","venue":null,"work_id":"92e45f16-db21-433c-b4b3-14931067f889","year":2024},"citing_paper":{"arxiv_id":"2606.12464","last_updated":"2026-08-06T17:33:57Z","snapshot_observed_at":"2026-08-09T23:12:16.486132Z","submitted_at":"2026-06-09T06:44:17Z","title":"Kinematic Probes of Type-II MMG: Pad\\'e Cosmographic Analysis of VCDM","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-27T10:52:02.678900Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2606.12464"},"observation_digest":"sha256:3083c572fdbe8fe89bab3cef6ac6c890840bcf84f45776667d2967d86a61b3a9","observation_id":"8f496e19-abba-431e-8e9b-697a3bbdc218","resolution":{"observed_at":"2026-07-03T08:17:45.442892Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-02T11:15:39.134441Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.16844","last_updated":"2026-07-28T17:56:35Z","snapshot_observed_at":"2026-08-02T11:15:36.144590Z","submitted_at":"2026-06-15T15:22:34Z","title":"The cosmic tetrarchy: four estimators breaking the assumption degeneracy in cosmological distance tensions","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-02T11:15:39.134441Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2606.16844"},"observation_digest":"sha256:248d176561c607d20c2972c33a0c669f5f6fdd8f49f78b8a46bc549a20172053","observation_id":"6d898344-c22a-4429-a211-f44ea261972f","resolution":{"observed_at":"2026-08-02T11:15:39.134441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":"2501.15233","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-07-03T08:17:45.441481Z","title":"Alfano and O","venue":null,"work_id":"92e45f16-db21-433c-b4b3-14931067f889","year":2024},"citing_paper":{"arxiv_id":"2607.01199","last_updated":"2026-07-08T16:43:07Z","snapshot_observed_at":"2026-08-09T16:22:54.299503Z","submitted_at":"2026-07-01T17:32:58Z","title":"Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition?","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-02T06:17:10.987485Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2607.01199"},"observation_digest":"sha256:e1d48c4ff832a213bf6ec3a8a3fb65aad810921ddfbb1c107fde677e7f248d36","observation_id":"c770e23d-774d-43be-8a34-4518c2256e77","resolution":{"observed_at":"2026-07-02T06:36:43.770575Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-07-12T08:56:43.854989Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.01199","last_updated":"2026-07-08T16:43:07Z","snapshot_observed_at":"2026-08-09T16:22:54.299503Z","submitted_at":"2026-07-01T17:32:58Z","title":"Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition?","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-12T08:56:43.854989Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2607.01199"},"observation_digest":"sha256:bb830dcfabe19e4379d0de7a0c93d876da553ea63dfa4054c586db53b3b6155c","observation_id":"87bbd309-c1fe-4962-a1fa-6bbb1465f6f1","resolution":{"observed_at":"2026-07-12T08:56:43.854989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-02T02:52:27.139816Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14211","last_updated":"2026-07-15T18:00:01Z","snapshot_observed_at":"2026-08-06T19:57:47.311393Z","submitted_at":"2026-07-15T18:00:01Z","title":"Non-Primordial Contribution to the Cosmic Microwave Background","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-02T02:52:27.139816Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2607.14211"},"observation_digest":"sha256:2524f977f9ac6bd1539c442487d86c55a0f7af00f90851f94d87e3743de3c4be","observation_id":"b945fecf-eb1b-4261-830c-328b3d13ba6a","resolution":{"observed_at":"2026-08-02T02:52:27.139816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-01T02:30:05.855277Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.26105","last_updated":"2026-07-28T08:56:55Z","snapshot_observed_at":"2026-08-06T02:08:51.000082Z","submitted_at":"2026-07-28T08:56:55Z","title":"Cosmological consequences of scale-dependent Barrow-Tsallis entropy","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-01T02:30:05.855277Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2607.26105"},"observation_digest":"sha256:85500a6a6f5065dbf5c3ddeba8789c8b6a8e4a102cc7d90b348197a9f0df3427","observation_id":"1a747fd7-6e04-421f-8cdb-f0bcf6cacb02","resolution":{"observed_at":"2026-08-01T02:30:05.855277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-07-31T11:14:46.855465Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.28326","last_updated":"2026-07-30T14:57:39Z","snapshot_observed_at":"2026-08-08T20:27:05.702904Z","submitted_at":"2026-07-30T14:57:39Z","title":"Growth, geometry, and early-universe split of the matter density parameter $\\Omega_{\\rm m}$","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-31T11:14:46.855465Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2607.28326"},"observation_digest":"sha256:13965b921f5157d96039ff90f53f47719676f91207ff5d937195a179ca1c2ba2","observation_id":"a850d0ee-aa93-4543-be44-e396b1680f1a","resolution":{"observed_at":"2026-07-31T11:14:46.855465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.15233","snapshot_observed_at":"2026-08-06T00:32:09.471781Z","title":null,"venue":null,"work_id":null,"year":2026},"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":20,"source":"pdf_text","source_observed_at":"2026-08-06T00:32:09.471781Z"},"links":{"cited_paper":"/paper/2501.15233","citing_paper":"/paper/2608.01215"},"observation_digest":"sha256:5a676cccb6fa0382b2f7cca868d093a660cdae1db36637571928824d8d608432","observation_id":"5ce55254-5cf1-472f-8c24-5bb1cd17c6a1","resolution":{"observed_at":"2026-08-06T00:32:09.471781Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2501.15233/citation-record","integrity":"/paper/2501.15233/integrity","json":"/paper/2501.15233/citation-record.json","paper":"/paper/2501.15233"},"outbound":[],"paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T18:39:05.803806Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy 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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2501.15233."}