{"as_of":"2026-08-10T14:36:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8d65f696abf5ccd4885e1d4db65b8d6d7aef6c8af71634102db0f264142bfdf1","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:07:16.215708Z","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":"2026-08-05T13:53:45.272159Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2302.10509","last_updated":"2023-07-22T05:49:59Z","snapshot_observed_at":"2026-07-06T14:54:00.594534Z","submitted_at":"2023-02-21T08:17:30Z","title":"Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\\Lambda$CDM Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.10509","snapshot_observed_at":"2026-08-07T15:07:16.215708Z","title":"Roy, Exploring the possibility of interacting quintessence model as an alternative to the ΛCDM model, Gen","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16438","last_updated":"2025-05-22T09:27:31Z","snapshot_observed_at":"2026-08-07T14:58:49.153677Z","submitted_at":"2025-05-22T09:27:31Z","title":"Exploring parametrized dark energy models in interacting scenario","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T15:07:16.215708Z"},"links":{"cited_paper":"/paper/2302.10509","citing_paper":"/paper/2505.16438"},"observation_digest":"sha256:8f4720badeeeb41e0cf0a821bdd0e1f9cff116794acf0d02734067cbb881eb75","observation_id":"95948f39-3e13-4084-b797-df3fc706c44f","resolution":{"observed_at":"2026-08-07T15:07:16.215708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.10509","last_updated":"2023-07-22T05:49:59Z","snapshot_observed_at":"2026-07-06T14:54:00.594534Z","submitted_at":"2023-02-21T08:17:30Z","title":"Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\\Lambda$CDM Model","version":2},"cited_work":{"arxiv_id":"2302.10509","doi":null,"metadata_source":"pith","pith_arxiv_id":"2302.10509","snapshot_observed_at":"2026-08-05T13:53:45.272159Z","title":"Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\\Lambda$CDM Model","venue":"astro-ph.CO","work_id":"6b7c006d-4b6e-4dc8-9ef5-bf48c85f461e","year":2023},"citing_paper":{"arxiv_id":"2509.00308","last_updated":"2025-08-30T01:52:12Z","snapshot_observed_at":"2026-08-08T06:16:37.518132Z","submitted_at":"2025-08-30T01:52:12Z","title":"Bouncing Cosmology in Interacting Scalar-Torsion Gravity","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-05T13:53:41.634633Z"},"links":{"cited_paper":"/paper/2302.10509","citing_paper":"/paper/2509.00308"},"observation_digest":"sha256:ba06f069c607e1c9e921c97482dd55f3b7a51e9df5a9f80727124273f66e2dc2","observation_id":"29f76c54-a4e9-4020-a2b2-03f38e3d3586","resolution":{"observed_at":"2026-08-05T13:53:45.328190Z","resolver_source":"local_arxiv","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":"2302.10509","last_updated":"2023-07-22T05:49:59Z","snapshot_observed_at":"2026-07-06T14:54:00.594534Z","submitted_at":"2023-02-21T08:17:30Z","title":"Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\\Lambda$CDM Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.10509","snapshot_observed_at":"2026-08-04T12:53:53.083569Z","title":"Roy, Gen","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.01974","last_updated":"2026-01-19T10:15:04Z","snapshot_observed_at":"2026-08-04T12:53:22.243014Z","submitted_at":"2025-10-02T12:47:51Z","title":"BAO miscalibration cannot rescue late-time solutions to the Hubble tension","version":2},"reference_index":236,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:53.083569Z"},"links":{"cited_paper":"/paper/2302.10509","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:c39cea8034a8989a66c2e38b3665ca9e3283ca71d1fc44a4a049f8cf90ef0be1","observation_id":"9e15beef-bd53-4347-a5dd-14daaeb621a2","resolution":{"observed_at":"2026-08-04T12:53:53.083569Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2302.10509/citation-record","integrity":"/paper/2302.10509/integrity","json":"/paper/2302.10509/citation-record.json","paper":"/paper/2302.10509"},"outbound":[],"paper":{"arxiv_id":"2302.10509","last_updated":"2023-07-22T05:49:59Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T14:54:00.594534Z","submitted_at":"2023-02-21T08:17:30Z","title":"Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\\Lambda$CDM Model"},"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 3 inbound Pith citation observations for arXiv:2302.10509."}