{"as_of":"2026-08-17T19:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7534cedc182bfaad5b38851c631f142c1917cee503a1c742401cc5f4428a2ad2","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T11:38:47.286933Z","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":"2026-06-30T14:34:45.554420Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-08-12T18:09:58.853960Z","title":"D., Jones, D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.11953","last_updated":"2025-02-12T15:36:52Z","snapshot_observed_at":"2026-08-13T16:49:55.485693Z","submitted_at":"2024-11-18T19:00:01Z","title":"Testing for Intrinsic Type Ia Supernova Luminosity Evolution at z>2 with JWST","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T18:09:58.853960Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2411.11953"},"observation_digest":"sha256:615c61be6f965da913d0ac915968979193ae0761b341c2bdaed3023af681f1d8","observation_id":"e4645111-1fa4-4d2c-9699-f3eff6be9a90","resolution":{"observed_at":"2026-08-12T18:09:58.853960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":"2104.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-06-30T14:34:45.554420Z","title":"Kenworthy, D.O","venue":null,"work_id":"85836411-cc74-44e7-8ed0-b282f972e8d7","year":2021},"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":115,"source":"pdf_text","source_observed_at":"2026-05-11T09:56:01.601036Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2503.14738"},"observation_digest":"sha256:e0ffdba49cfabe002f939ec92a907ad04e645634e907ac4fd312cc8be935d44a","observation_id":"1dbf7738-e40b-4df0-bd2d-d8245a461487","resolution":{"observed_at":"2026-05-11T09:56:03.185355Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-08-16T11:38:47.286933Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.15127","last_updated":"2025-07-12T01:39:19Z","snapshot_observed_at":"2026-08-16T18:33:40.770191Z","submitted_at":"2025-04-21T14:22:41Z","title":"Reconstructing the redshift evolution of Type Ia supernovae absolute magnitude","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T11:38:47.286933Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2504.15127"},"observation_digest":"sha256:cf03655ee2803811183a875e356f60cb0d3d838733420c8ca6f7f3703e086034","observation_id":"dd9237ca-e28c-45fe-a081-9e8b2c90c8cb","resolution":{"observed_at":"2026-08-16T11:38:47.286933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":"2104.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-06-30T14:34:45.554420Z","title":"Kenworthy, D.O","venue":null,"work_id":"85836411-cc74-44e7-8ed0-b282f972e8d7","year":2021},"citing_paper":{"arxiv_id":"2604.09777","last_updated":"2026-04-10T18:03:03Z","snapshot_observed_at":"2026-08-11T14:29:50.538863Z","submitted_at":"2026-04-10T18:03:03Z","title":"JWST Nebular Spectroscopy of SN 2023qov: Circumstellar Dust Emission in a Normal Type Ia Supernova","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-10T16:30:47.190257Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2604.09777"},"observation_digest":"sha256:4f5cfb620037027b5c12c2b68217d13821cc3c0e3f46895778b1bc1f2f108ce7","observation_id":"3268f2c8-abcc-4906-891c-c97ee9314695","resolution":{"observed_at":"2026-05-11T08:45:58.950255Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":"2104.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-06-30T14:34:45.554420Z","title":"Kenworthy, D.O","venue":null,"work_id":"85836411-cc74-44e7-8ed0-b282f972e8d7","year":2021},"citing_paper":{"arxiv_id":"2605.16513","last_updated":"2026-05-15T18:07:17Z","snapshot_observed_at":"2026-08-17T04:55:19.220467Z","submitted_at":"2026-05-15T18:07:17Z","title":"Modeling the probability distribution for cosmological analysis with photometrically classified samples","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-20T15:41:32.173385Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2605.16513"},"observation_digest":"sha256:fbab65f83be5eafc0950fea768ef6b5de17228cf2712aa53624f6d1ee0f4cdf9","observation_id":"48735b0b-f42c-4bbe-a347-0d0c72ef0912","resolution":{"observed_at":"2026-05-20T15:43:26.966443Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":"2104.07795","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-06-30T14:34:45.554420Z","title":"Kenworthy, D.O","venue":null,"work_id":"85836411-cc74-44e7-8ed0-b282f972e8d7","year":2021},"citing_paper":{"arxiv_id":"2605.24089","last_updated":"2026-05-22T18:00:02Z","snapshot_observed_at":"2026-08-08T01:16:50.760411Z","submitted_at":"2026-05-22T18:00:02Z","title":"Exploring the Dark Sector: Interacting Radiation in Light of Modern Cosmological Probes","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-06-30T14:32:13.675156Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2605.24089"},"observation_digest":"sha256:10b10f96540811b9a5312247d2c953202375e90d6bdb319eaedb7710bcc2e4e0","observation_id":"dd17645d-03d6-463f-ba99-a7efd57e5c59","resolution":{"observed_at":"2026-06-30T14:34:45.555902Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-07-12T05:14:58.841553Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03045","last_updated":"2026-07-03T07:34:46Z","snapshot_observed_at":"2026-08-13T11:34:49.188005Z","submitted_at":"2026-07-03T07:34:46Z","title":"nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors","version":1},"reference_index":104,"source":"arxiv_source","source_observed_at":"2026-07-12T05:14:58.841553Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2607.03045"},"observation_digest":"sha256:cc14a49963bb0d34ef641ac22c5268ec974f25214ac8ec1c0a30b26cd5ce7859","observation_id":"481fc55a-1550-4f3b-bb75-2e6831ada000","resolution":{"observed_at":"2026-07-12T05:14:58.841553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-08-01T06:02:05.028442Z","title":"arXiv , author =:2104.07795 , journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.22050","last_updated":"2026-08-04T09:11:55Z","snapshot_observed_at":"2026-08-08T13:19:27.261652Z","submitted_at":"2026-07-24T07:35:53Z","title":"ZTF SN Ia DR2 follow-up: early excess in Type Ia supernova light curves","version":1},"reference_index":157,"source":"arxiv_source","source_observed_at":"2026-08-01T06:02:05.028442Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2607.22050"},"observation_digest":"sha256:7cce1fc995b5127c2ff1f82f6a16087155894e7c57caac5d33cba4d79fbe1462","observation_id":"72a362c9-bb85-4d53-b1bc-436463f979f8","resolution":{"observed_at":"2026-08-01T06:02:05.028442Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.07795","snapshot_observed_at":"2026-08-03T00:39:10.881921Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28725","last_updated":"2026-07-30T18:00:01Z","snapshot_observed_at":"2026-08-14T14:32:47.438741Z","submitted_at":"2026-07-30T18:00:01Z","title":"A Simulation Based Inference Approach to Modelling of Type Ia Supernova Populations","version":1},"reference_index":179,"source":"arxiv_source","source_observed_at":"2026-08-03T00:39:10.881921Z"},"links":{"cited_paper":"/paper/2104.07795","citing_paper":"/paper/2607.28725"},"observation_digest":"sha256:f1ea15b0372565ea95f25ad099fba10f1ba4f483fe0ae439de97ea7b9bcb6fd0","observation_id":"0e58fb0f-462b-43d9-912b-620d9ffc99be","resolution":{"observed_at":"2026-08-03T00:39:10.881921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2104.07795/citation-record","integrity":"/paper/2104.07795/integrity","json":"/paper/2104.07795/citation-record.json","paper":"/paper/2104.07795"},"outbound":[],"paper":{"arxiv_id":"2104.07795","last_updated":"2021-04-15T21:59:38Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T18:31:14.449288Z","submitted_at":"2021-04-15T21:59:38Z","title":"SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2104.07795."}