{"as_of":"2026-08-04T17:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:511ba03ee10ec907f4a5fa56379aa125d535c4fd7c76d29fbb8e5f80bb5933bb","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T12:53:39.321325Z","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":"2026-07-09T08:05:16.230513Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.10559","last_updated":"2025-02-07T08:56:56Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T14:38:57Z","title":"Scale-dependence in $\\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10559","snapshot_observed_at":"2026-08-04T12:53:39.321325Z","title":"Jiang, Phys","venue":null,"work_id":null,"year":2025},"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":84,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:39.321325Z"},"links":{"cited_paper":"/paper/2410.10559","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:33df7eeeb1aa7f739d17136d53d77249f11761cca1a3930890cf1eb282301041","observation_id":"02466509-7aae-4b64-943e-5738ec3f82fe","resolution":{"observed_at":"2026-08-04T12:53:39.321325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10559","last_updated":"2025-02-07T08:56:56Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T14:38:57Z","title":"Scale-dependence in $\\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy","version":3},"cited_work":{"arxiv_id":"2410.10559","doi":"10.1103/physrevd.111.043528","metadata_source":"pith","pith_arxiv_id":"2410.10559","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Jiang, Phys","venue":"astro-ph.CO","work_id":"b37ecd9b-7518-40be-a7a5-db40354b4e7f","year":2024},"citing_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-15T06:29:12Z","title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","version":1},"reference_index":137,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2410.10559","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:d2adfb84ee931ddc2583a251222c28f78eef7695fcd38c49e5aabc1afad7a99c","observation_id":"6dbcbbd9-d6cd-4d6d-b59b-3710ed2b6c44","resolution":{"observed_at":"2026-05-11T11:41:01.817857Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-11T02:49:18.234036+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T02:49:18.234036+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10559","last_updated":"2025-02-07T08:56:56Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T14:38:57Z","title":"Scale-dependence in $\\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy","version":3},"cited_work":{"arxiv_id":"2410.10559","doi":"10.1103/physrevd.111.043528","metadata_source":"pith","pith_arxiv_id":"2410.10559","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Jiang, Phys","venue":"astro-ph.CO","work_id":"b37ecd9b-7518-40be-a7a5-db40354b4e7f","year":2024},"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":132,"source":"pdf_text","source_observed_at":"2026-06-26T19:48:32.340111Z"},"links":{"cited_paper":"/paper/2410.10559","citing_paper":"/paper/2606.19090"},"observation_digest":"sha256:e37c2ad3e357a205cc9f4dcfaf711b31a926d3a79023ef89e8b6d106b82be1e7","observation_id":"c0bba374-4291-49cb-bc9a-8c7e5b3e54c0","resolution":{"observed_at":"2026-07-04T02:19:23.564909Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-11T02:49:18.234036+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T02:49:18.234036+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10559","last_updated":"2025-02-07T08:56:56Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T14:38:57Z","title":"Scale-dependence in $\\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy","version":3},"cited_work":{"arxiv_id":"2410.10559","doi":"10.1103/physrevd.111.043528","metadata_source":"pith","pith_arxiv_id":"2410.10559","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Jiang, Phys","venue":"astro-ph.CO","work_id":"b37ecd9b-7518-40be-a7a5-db40354b4e7f","year":2024},"citing_paper":{"arxiv_id":"2607.06147","last_updated":"2026-07-07T11:15:39Z","snapshot_observed_at":"2026-08-03T00:55:46.087302Z","submitted_at":"2026-07-07T11:15:39Z","title":"Imprint of swampland-inspired coupled early dark energy","version":1},"reference_index":142,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2410.10559","citing_paper":"/paper/2607.06147"},"observation_digest":"sha256:ad4455d81bceb14f97211d196f292113ca9c4d4fd06b56ecd43ec5c4ac3996d2","observation_id":"004560b3-b626-48c2-b3c9-a18635b192a4","resolution":{"observed_at":"2026-07-08T15:55:04.696857Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-11T02:49:18.234036+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T02:49:18.234036+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10559","last_updated":"2025-02-07T08:56:56Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T14:38:57Z","title":"Scale-dependence in $\\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10559","snapshot_observed_at":"2026-08-01T08:08:48.173777Z","title":"Jiang, Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-03T05:59:43.108747Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":150,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:48.173777Z"},"links":{"cited_paper":"/paper/2410.10559","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:a8f8069be2d48743cf09c41589a4e3aa584eed534a53fd4c599ad641110fbc99","observation_id":"b069ab79-8815-40f5-a7ce-ac62cd2467a0","resolution":{"observed_at":"2026-08-01T08:08:48.173777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.10559/citation-record","integrity":"/paper/2410.10559/integrity","json":"/paper/2410.10559/citation-record.json","paper":"/paper/2410.10559"},"outbound":[],"paper":{"arxiv_id":"2410.10559","last_updated":"2025-02-07T08:56:56Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T14:38:57Z","title":"Scale-dependence in $\\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2410.10559."}