{"as_of":"2026-08-05T18:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9d3ddc50313ef08aac74415770c8e5d72b3090d5758e200b077f52d6b465e144","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T03:21:43.406790Z","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":"2026-07-04T02:19:23.500241Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":"2412.04430","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-07-04T02:19:23.500241Z","title":null,"venue":null,"work_id":"e4a36ea6-a1fc-40c2-8cb6-7ad0bdfa9124","year":2025},"citing_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"reference_index":132,"source":"pdf_text","source_observed_at":"2026-05-11T09:56:01.601036Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2503.14738"},"observation_digest":"sha256:a5c20b8dd806c75cb32ca4d7239e7d843bf565430368a1e182e3f1f88ac6a8b2","observation_id":"9993121d-9b7f-4333-957b-0b7d2b150524","resolution":{"observed_at":"2026-05-11T09:56:03.389538Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":"2412.04430","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-07-04T02:19:23.500241Z","title":null,"venue":null,"work_id":"e4a36ea6-a1fc-40c2-8cb6-7ad0bdfa9124","year":2025},"citing_paper":{"arxiv_id":"2503.14744","last_updated":"2025-10-07T13:00:34Z","snapshot_observed_at":"2026-07-06T20:55:04.493800Z","submitted_at":"2025-03-18T21:14:18Z","title":"Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape","version":3},"reference_index":183,"source":"pdf_text","source_observed_at":"2026-05-16T17:46:22.581000Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2503.14744"},"observation_digest":"sha256:703f44294846af94d7f2fd28a7d5d0e8332b2d3e2d33bb3e6ad0a0b0311dc8ed","observation_id":"4223870c-fcd3-4353-b672-110070e4ebd3","resolution":{"observed_at":"2026-05-16T17:46:23.344612Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":"2412.04430","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-07-04T02:19:23.500241Z","title":null,"venue":null,"work_id":"e4a36ea6-a1fc-40c2-8cb6-7ad0bdfa9124","year":2025},"citing_paper":{"arxiv_id":"2506.23290","last_updated":"2026-04-17T09:16:11Z","snapshot_observed_at":"2026-07-06T21:49:24.430655Z","submitted_at":"2025-06-29T15:26:07Z","title":"Type II Seesaw Leptogenesis in a Majoron background","version":2},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-05-19T07:47:44.372827Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2506.23290"},"observation_digest":"sha256:2fe4d99ccbc06dc3bb5cdce84821c6597183cfc686cc839022ede8e67dbbb9d8","observation_id":"95f5c847-7450-46a4-bf3c-b222113d08fd","resolution":{"observed_at":"2026-05-19T07:52:10.077139Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-08-03T18:51:47.363889Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.04130","last_updated":"2026-07-26T05:14:02Z","snapshot_observed_at":"2026-08-04T06:15:07.631708Z","submitted_at":"2025-12-03T06:33:55Z","title":"Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\\omega_0\\omega_a$CDM","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-03T18:51:47.363889Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2512.04130"},"observation_digest":"sha256:8b35ec31eb57ac219875deddd2ef9bc1667c3ce6894afe8e4dfaf9db0c76b8be","observation_id":"2d9419cd-0934-4a96-8f49-f247a0805eab","resolution":{"observed_at":"2026-08-03T18:51:47.363889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":"2412.04430","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-07-04T02:19:23.500241Z","title":null,"venue":null,"work_id":"e4a36ea6-a1fc-40c2-8cb6-7ad0bdfa9124","year":2025},"citing_paper":{"arxiv_id":"2606.05853","last_updated":"2026-06-04T08:27:25Z","snapshot_observed_at":"2026-08-01T21:34:07.002669Z","submitted_at":"2026-06-04T08:27:25Z","title":"Reconstructing dark energy with fewer assumptions","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-06-28T00:07:32.911711Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2606.05853"},"observation_digest":"sha256:2037875837e8cda99a0fa4da74ccc94475220677fef60b1887626d0613c4a3e2","observation_id":"d54483b9-4972-48cf-8324-1d7d29194ec8","resolution":{"observed_at":"2026-07-02T14:57:04.202699Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":"2412.04430","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-07-04T02:19:23.500241Z","title":null,"venue":null,"work_id":"e4a36ea6-a1fc-40c2-8cb6-7ad0bdfa9124","year":2025},"citing_paper":{"arxiv_id":"2606.19090","last_updated":"2026-06-17T13:58:39Z","snapshot_observed_at":"2026-07-06T23:54:27.624372Z","submitted_at":"2026-06-17T13:58:39Z","title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","version":1},"reference_index":134,"source":"pdf_text","source_observed_at":"2026-06-26T19:48:32.340111Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2606.19090"},"observation_digest":"sha256:c62b21dda1828d5fb708bf8d13511934f46346c6648da434c5764fdd9bcdfb89","observation_id":"15dd65d8-2966-4e59-b25c-72e77564f7b6","resolution":{"observed_at":"2026-07-04T02:19:23.501584Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-08-01T17:17:51.239532Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.26373","last_updated":"2026-08-03T02:51:34Z","snapshot_observed_at":"2026-08-05T17:30:59.563074Z","submitted_at":"2026-07-29T01:20:58Z","title":"No way ou$\\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-01T17:17:51.239532Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2607.26373"},"observation_digest":"sha256:10c1df7338621a243f67a5f091ab7072d8322ba097258eb500851d46d5625af6","observation_id":"300bd0d5-b445-44ec-b1cf-39072b9d7e22","resolution":{"observed_at":"2026-08-01T17:17:51.239532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.04430","snapshot_observed_at":"2026-08-04T03:21:43.406790Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.26373","last_updated":"2026-08-03T02:51:34Z","snapshot_observed_at":"2026-08-05T17:30:59.563074Z","submitted_at":"2026-07-29T01:20:58Z","title":"No way ou$\\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-04T03:21:43.406790Z"},"links":{"cited_paper":"/paper/2412.04430","citing_paper":"/paper/2607.26373"},"observation_digest":"sha256:1cf12fe1edd026e1e6cccb7c129481e728f700b6de8c89dffe7fc811a302fbce","observation_id":"4fed44a3-6c62-4e3e-9406-45a3d145bb04","resolution":{"observed_at":"2026-08-04T03:21:43.406790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2412.04430/citation-record","integrity":"/paper/2412.04430/integrity","json":"/paper/2412.04430/citation-record.json","paper":"/paper/2412.04430"},"outbound":[],"paper":{"arxiv_id":"2412.04430","last_updated":"2025-03-22T21:18:35Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-04T09:40:08.517363Z","submitted_at":"2024-12-05T18:52:01Z","title":"Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\\Omega_m$ and $H_0$ Across Cosmological Probes"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2412.04430."}