{"as_of":"2026-08-10T06:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:063200c575d948685d4962eabb5138eb2c2ff175254367e5d9a6ad38f7feb7d8","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T10:52:56.825672Z","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":"2026-05-22T05:24:37.956141Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-08-07T10:52:56.825672Z","title":"Menci, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.04306","last_updated":"2025-06-04T17:51:05Z","snapshot_observed_at":"2026-08-07T14:10:01.304994Z","submitted_at":"2025-06-04T17:51:05Z","title":"Can the universe experience an AdS landscape since matter-radiation equality?","version":1},"reference_index":155,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:56.825672Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2506.04306"},"observation_digest":"sha256:48c40da7a2b03b6619fce9285b11404f2b4f4329d4726a3cfc2c4c31f99a3137","observation_id":"2ef4622c-e9ea-4489-9890-3974dc7f142c","resolution":{"observed_at":"2026-08-07T10:52:56.825672Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-08-06T21:35:00.919597Z","title":"Menci, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.24011","last_updated":"2025-08-26T17:48:07Z","snapshot_observed_at":"2026-08-09T04:36:11.327370Z","submitted_at":"2025-06-30T16:14:19Z","title":"The Lifespan of our Universe","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T21:35:00.919597Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2506.24011"},"observation_digest":"sha256:83c3aab0c92963b4cf9d303fd49a7b7d3340fb91b8d4e46b453cf9003f62e135","observation_id":"d05f56ae-1b57-4749-ab56-5d0f5271d770","resolution":{"observed_at":"2026-08-06T21:35:00.919597Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-08-04T12:53:50.683751Z","title":"Menci, S","venue":null,"work_id":null,"year":2024},"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":208,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:50.683751Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:3bd830e31fcafbf946a837336995d5b1a18123806a91486644c3ecc9a245c8c1","observation_id":"a0421f2d-3c69-4ae7-9b28-6d4868fc0866","resolution":{"observed_at":"2026-08-04T12:53:50.683751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":"2401.12659","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Menci, S","venue":null,"work_id":"8076302a-ded7-4350-ad83-ea6c68b0ce58","year":2024},"citing_paper":{"arxiv_id":"2510.18741","last_updated":"2026-04-10T13:03:33Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-21T15:46:25Z","title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","version":2},"reference_index":190,"source":"pdf_text","source_observed_at":"2026-05-18T04:46:14.832965Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2510.18741"},"observation_digest":"sha256:cff082a05f38c9371e9466426f4d70debf2f7b5fbe0f8cc752898d175e0f63de","observation_id":"8e75d61f-bccd-40a8-873e-c7949c481fef","resolution":{"observed_at":"2026-05-18T04:50:55.026043Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-08-04T00:10:25.597820Z","title":"Menci, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.02906","last_updated":"2026-07-13T21:59:28Z","snapshot_observed_at":"2026-08-06T14:11:33.684472Z","submitted_at":"2025-11-04T19:00:01Z","title":"Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST","version":2},"reference_index":109,"source":"pdf_text","source_observed_at":"2026-08-04T00:10:25.597820Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2511.02906"},"observation_digest":"sha256:5ec32f80ba093ed3272b34ea67cd5d4ba4c79a451175449202a85f5734b6c949","observation_id":"57627bff-168f-4f5c-b654-e9ddd63ed1ca","resolution":{"observed_at":"2026-08-04T00:10:25.597820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-08-03T07:07:24.595190Z","title":"Menci, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2601.21356","last_updated":"2026-07-16T19:48:47Z","snapshot_observed_at":"2026-08-10T00:10:35.635341Z","submitted_at":"2026-01-29T07:32:33Z","title":"Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-03T07:07:24.595190Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2601.21356"},"observation_digest":"sha256:2b08aaac675c6d1aa4bfd7c801bab1a2263c858adf870ae2e0f297831383bacc","observation_id":"18f2a98d-4788-48ac-9573-5d213af187ce","resolution":{"observed_at":"2026-08-03T07:07:24.595190Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":"2401.12659","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Menci, S","venue":null,"work_id":"8076302a-ded7-4350-ad83-ea6c68b0ce58","year":2024},"citing_paper":{"arxiv_id":"2602.11936","last_updated":"2026-05-18T12:54:32Z","snapshot_observed_at":"2026-08-02T13:51:44.487752Z","submitted_at":"2026-02-12T13:35:54Z","title":"Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework","version":3},"reference_index":139,"source":"pdf_text","source_observed_at":"2026-05-21T13:29:05.147292Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2602.11936"},"observation_digest":"sha256:e5b3ba0f3219b77661ec775d5d2d0de4e810f3f018430b8571735ae91657a9a0","observation_id":"84046466-9e22-4136-9745-4a4b893637e9","resolution":{"observed_at":"2026-05-21T13:30:12.466910Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-07-15T12:01:04.317365Z","title":"Menci, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.14693","last_updated":"2026-07-14T04:50:03Z","snapshot_observed_at":"2026-08-10T04:20:36.632135Z","submitted_at":"2026-03-16T01:02:08Z","title":"Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families","version":2},"reference_index":150,"source":"pdf_text","source_observed_at":"2026-07-15T12:01:04.317365Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2603.14693"},"observation_digest":"sha256:7fb232e240b65e6880e99e083819c14ec7160d8a6a389117caffb195e779ec28","observation_id":"23f37249-f878-49db-86bf-0dd1902dc516","resolution":{"observed_at":"2026-07-15T12:01:04.317365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":"2401.12659","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Menci, S","venue":null,"work_id":"8076302a-ded7-4350-ad83-ea6c68b0ce58","year":2024},"citing_paper":{"arxiv_id":"2605.22348","last_updated":"2026-05-21T11:34:03Z","snapshot_observed_at":"2026-07-06T23:32:39.761431Z","submitted_at":"2026-05-21T11:34:03Z","title":"Dark Energy in Ghost-free non-local Gravity","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-22T05:24:23.654862Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2605.22348"},"observation_digest":"sha256:0e778b4ac793036813e7a07ec4c7de113b2d6136f6f997875581dcf98b514c4e","observation_id":"58506848-40c3-41e0-b900-75c7eff6325b","resolution":{"observed_at":"2026-05-22T05:24:37.959013Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.12659","snapshot_observed_at":"2026-07-11T09:40:49.196932Z","title":"Menci, S.A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.05044","last_updated":"2026-07-06T13:21:04Z","snapshot_observed_at":"2026-08-06T06:21:38.078437Z","submitted_at":"2026-07-06T13:21:04Z","title":"Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus","version":1},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-07-11T09:40:49.196932Z"},"links":{"cited_paper":"/paper/2401.12659","citing_paper":"/paper/2607.05044"},"observation_digest":"sha256:9b89a7dbd2135d58213abc2b9a81665e6e143668d797dca15aec11be0fd13fd2","observation_id":"26b54ffd-addc-4966-9c2e-fab66bdcbfac","resolution":{"observed_at":"2026-07-11T09:40:49.196932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2401.12659/citation-record","integrity":"/paper/2401.12659/integrity","json":"/paper/2401.12659/citation-record.json","paper":"/paper/2401.12659"},"outbound":[],"paper":{"arxiv_id":"2401.12659","last_updated":"2024-07-17T13:28:01Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:10:25Z","title":"Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2401.12659."}