{"as_of":"2026-07-31T21:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4aa30ebe0fa73445df3d9fd7f72ec1223263852a09cef7e75fc60fa867c815c3","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-07-31T06:34:12.847434+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-10T18:19:17.740185Z","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":"2026-07-10T18:27:31.561381Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","snapshot_observed_at":"2026-07-06T18:03:51.687441Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements","version":2},"cited_work":{"arxiv_id":"2404.14341","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.14341","snapshot_observed_at":"2026-07-10T18:27:31.561381Z","title":"V., Kable, J","venue":"astro-ph.CO","work_id":"50a25669-78e8-4ba6-82a4-954626bdf010","year":2024},"citing_paper":{"arxiv_id":"2409.13022","last_updated":"2024-11-17T16:25:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-09-19T18:00:26Z","title":"Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-18T16:14:18.379876Z"},"links":{"cited_paper":"/paper/2404.14341","citing_paper":"/paper/2409.13022"},"observation_digest":"sha256:dc5aa13efd6853033779491fd10c73d205ec11ab084850635d20c1bb8c1afc56","observation_id":"cbc5aaff-d74b-47a0-baf8-a3196ac6dea2","resolution":{"observed_at":"2026-05-18T16:14:18.485266Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-31T06:34:12.847434+00:00","source":"crossref"},{"observed_at":"2026-07-31T06:34:08.642788+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","snapshot_observed_at":"2026-07-06T18:03:51.687441Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements","version":2},"cited_work":{"arxiv_id":"2404.14341","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.14341","snapshot_observed_at":"2026-07-10T18:27:31.561381Z","title":"V., Kable, J","venue":"astro-ph.CO","work_id":"50a25669-78e8-4ba6-82a4-954626bdf010","year":2024},"citing_paper":{"arxiv_id":"2508.08638","last_updated":"2026-04-03T03:15:04Z","snapshot_observed_at":"2026-07-06T22:11:38.066500Z","submitted_at":"2025-08-12T05:03:36Z","title":"Interacting bosonic dark energy and fermionic dark matter in Einstein scalar Gauss-Bonnet gravity","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-18T23:42:50.201808Z"},"links":{"cited_paper":"/paper/2404.14341","citing_paper":"/paper/2508.08638"},"observation_digest":"sha256:7df5be36ec8d872b049195a8802b146e1a854ce609f760d8d4d16f7e56069212","observation_id":"d8f28438-63bd-4330-8409-307423d25168","resolution":{"observed_at":"2026-05-18T23:42:53.329913Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-31T06:34:12.847434+00:00","source":"crossref"},{"observed_at":"2026-07-31T06:34:08.642788+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","snapshot_observed_at":"2026-07-06T18:03:51.687441Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements","version":2},"cited_work":{"arxiv_id":"2404.14341","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.14341","snapshot_observed_at":"2026-07-10T18:27:31.561381Z","title":"V., Kable, J","venue":"astro-ph.CO","work_id":"50a25669-78e8-4ba6-82a4-954626bdf010","year":2024},"citing_paper":{"arxiv_id":"2510.03779","last_updated":"2026-02-17T10:47:14Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-04T11:08:41Z","title":"Beyond CPL: Evidence for dynamical dark energy in three-parameter models","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-18T10:45:16.985887Z"},"links":{"cited_paper":"/paper/2404.14341","citing_paper":"/paper/2510.03779"},"observation_digest":"sha256:a029ced11b06b91e58db8f25d1f95fa9bbfea07e2015e683ef9bad6accc160d6","observation_id":"f0d08ba1-e561-4cdd-8b9e-6a3cc9f71afc","resolution":{"observed_at":"2026-05-18T10:46:16.626561Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-31T06:34:12.847434+00:00","source":"crossref"},{"observed_at":"2026-07-31T06:34:08.642788+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","snapshot_observed_at":"2026-07-06T18:03:51.687441Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements","version":2},"cited_work":{"arxiv_id":"2404.14341","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.14341","snapshot_observed_at":"2026-07-10T18:27:31.561381Z","title":"V., Kable, J","venue":"astro-ph.CO","work_id":"50a25669-78e8-4ba6-82a4-954626bdf010","year":2024},"citing_paper":{"arxiv_id":"2604.03756","last_updated":"2026-04-07T02:58:46Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","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":16,"source":"pdf_text","source_observed_at":"2026-05-13T17:33:08.222231Z"},"links":{"cited_paper":"/paper/2404.14341","citing_paper":"/paper/2604.03756"},"observation_digest":"sha256:093d93af92ec333697a9b7500f014a32d469f2e1e9858265ed29b7f1438efd90","observation_id":"4cfc878d-8dfc-409f-b82c-239e87f97614","resolution":{"observed_at":"2026-05-13T17:38:02.970849Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-31T06:34:12.847434+00:00","source":"crossref"},{"observed_at":"2026-07-31T06:34:08.642788+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","snapshot_observed_at":"2026-07-06T18:03:51.687441Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements","version":2},"cited_work":{"arxiv_id":"2404.14341","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.14341","snapshot_observed_at":"2026-07-10T18:27:31.561381Z","title":"V., Kable, J","venue":"astro-ph.CO","work_id":"50a25669-78e8-4ba6-82a4-954626bdf010","year":2024},"citing_paper":{"arxiv_id":"2606.05539","last_updated":"2026-06-04T00:48:50Z","snapshot_observed_at":"2026-07-06T23:45:33.157370Z","submitted_at":"2026-06-04T00:48:50Z","title":"Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-06-28T00:31:52.323240Z"},"links":{"cited_paper":"/paper/2404.14341","citing_paper":"/paper/2606.05539"},"observation_digest":"sha256:1c4ceaf9d23fdcdc82911ff23bef3cd3d4906e2e800f053766582eea1bcdf428","observation_id":"2bf772cc-7d6a-4321-ae34-f288908687fe","resolution":{"observed_at":"2026-07-02T14:27:03.534171Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-31T06:34:12.847434+00:00","source":"crossref"},{"observed_at":"2026-07-31T06:34:08.642788+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","snapshot_observed_at":"2026-07-06T18:03:51.687441Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements","version":2},"cited_work":{"arxiv_id":"2404.14341","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.14341","snapshot_observed_at":"2026-07-10T18:27:31.561381Z","title":"V., Kable, J","venue":"astro-ph.CO","work_id":"50a25669-78e8-4ba6-82a4-954626bdf010","year":2024},"citing_paper":{"arxiv_id":"2607.07777","last_updated":"2026-07-08T17:38:46Z","snapshot_observed_at":"2026-07-12T23:17:59.826213Z","submitted_at":"2026-07-08T17:38:46Z","title":"The Status of Single Scalar Field Dark Energy","version":1},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-07-10T18:19:17.740185Z"},"links":{"cited_paper":"/paper/2404.14341","citing_paper":"/paper/2607.07777"},"observation_digest":"sha256:538c69d9767d2d3d8c32d9c104faa281533c48385d92c59f02d87c94ff60fbf4","observation_id":"73aefb48-c5bc-4f45-98e2-23ccfad7ba55","resolution":{"observed_at":"2026-07-10T18:27:31.562633Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-31T06:34:12.847434+00:00","source":"crossref"},{"observed_at":"2026-07-31T06:34:08.642788+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2404.14341/citation-record","integrity":"/paper/2404.14341/integrity","json":"/paper/2404.14341/citation-record.json","paper":"/paper/2404.14341"},"outbound":[],"paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T18:03:51.687441Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements"},"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":"2026-07-31T06:34:12.847434+00:00","source":"crossref"},{"observed_at":"2026-07-31T06:34:08.642788+00:00","source":"retraction_watch"}],"thesis":"As of 31 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2404.14341."}