{"as_of":"2026-08-12T08:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ed04443eadb98d410707eb165328ec3ede1cd10c92510a658d81a3594f7a807a","coverage":[{"denominator":37,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":37,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T17:26:46.960352Z","state":"measured"},{"denominator":38,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":38,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-29T03:34:41.413967Z","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":"2026-07-01T17:35:51.485339Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"cited_work":{"arxiv_id":"2501.12264","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2501.12264","snapshot_observed_at":"2026-07-01T17:35:51.485339Z","title":"Dai and W","venue":null,"work_id":"07c17b0e-3f19-4bc3-875e-db36914ca083","year":null},"citing_paper":{"arxiv_id":"2606.28135","last_updated":"2026-06-26T14:35:23Z","snapshot_observed_at":"2026-08-08T09:38:42.053459Z","submitted_at":"2026-06-26T14:35:23Z","title":"Probing the neutrino chemical potential with cosmological observations","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-06-29T03:34:41.413967Z"},"links":{"cited_paper":"/paper/2501.12264","citing_paper":"/paper/2606.28135"},"observation_digest":"sha256:212d65d4c3954651fe59a9c33938a68e22d6828024d23eb0c39abc3688909cae","observation_id":"6d3ee671-a873-4cb6-bb51-fdfbe4b6583a","resolution":{"observed_at":"2026-07-01T17:35:51.487055Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2501.12264/citation-record","integrity":"/paper/2501.12264/integrity","json":"/paper/2501.12264/citation-record.json","paper":"/paper/2501.12264"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.707573Z","title":"Updated fit to three neutrino mixing: exploring the accelerator-reactor complementarity","venue":null,"work_id":"b25bcce5-f8bc-44d6-9996-1ad3cab554d6","year":2017},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.769913Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:c3bc0d7c0247ab8119a8b5f92651865fdb439a1f1882aea691f725478487f8b5","observation_id":"9ee8a3f7-07cf-473a-b5f7-4f22cb87c3f4","resolution":{"observed_at":"2026-08-10T17:26:47.712797Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.692493Z","title":"NuFIT: Three-Flavour Global Analyses of Neutrino Oscillation Experiments","venue":null,"work_id":"5e6399ba-4b3a-42ee-9e2e-48fbdba1d14b","year":2021},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.776555Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:51d50c737910ce9bb2773e2895210c44132833b8080fcc5bf77aab1b7f925642","observation_id":"0d55cb5f-4288-4789-99d4-394f6174e438","resolution":{"observed_at":"2026-08-10T17:26:47.697538Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.677071Z","title":"Neutrino physics from the cosmic microwave back- ground and large scale structure","venue":null,"work_id":"b9ab94e4-5d63-414e-b1ac-4955df02a3c2","year":2015},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.781537Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:21f6836b3634a6975b9a9b99e7ff299750dfc18bfa978ed87b307a6f2133537c","observation_id":"fd1803b1-f3fc-49f8-a5cc-0d3089446b09","resolution":{"observed_at":"2026-08-10T17:26:47.682342Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.661952Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":null,"work_id":"78db3d35-ebf4-480a-aec6-4a2226ffd65a","year":2014},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.786827Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:1e0c39ae791e29314c472d33d64326bac58f0679ebdb1bc1044c88793444052c","observation_id":"e5315a75-de74-4220-b563-fd2c4408fe1c","resolution":{"observed_at":"2026-08-10T17:26:47.666794Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-08-10T17:26:46.792385Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.792385Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:57767e68e477af5ea6e9bc05db25909387512d7c2ab2cc68936a91c454be7287","observation_id":"0254460b-32a8-4ff8-a0ec-a5545790ccb5","resolution":{"observed_at":"2026-08-10T17:26:46.792385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.646774Z","title":"Neutrino statistics and big bang nucleosyn- thesis","venue":null,"work_id":"7488330e-7e4e-4ba5-a876-9b9aa75284cc","year":2005},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.798547Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:038f771babaa71b7959d66ed2a5a0eeb7a1f34af7556290104038afa4022f1a0","observation_id":"28235a38-5453-4ca0-8f96-aa04df531034","resolution":{"observed_at":"2026-08-10T17:26:47.651602Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.631406Z","title":"Statistics of neutrinos and the double beta decay","venue":null,"work_id":"be56f68a-abf9-4b5c-af9e-6f7f424143e3","year":2007},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.804225Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:d372106ee2bd7f20ce877b3bfccd429209a13d3def693907a5c27c8d14d7b88f","observation_id":"eab111eb-21b4-4785-9d9d-f59d433d6719","resolution":{"observed_at":"2026-08-10T17:26:47.636188Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.616701Z","title":"Cosmological bounds on neutrino statistics","venue":null,"work_id":"3facc0e8-b1ad-4a00-9f25-5d699cdee826","year":2018},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.810160Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:a63134231f5755f330f6e4a8e51982ef6a4bb11761b3223f1c064c2e016871b6","observation_id":"1e44b64e-8e37-4f49-a451-33cffcd40d09","resolution":{"observed_at":"2026-08-10T17:26:47.621523Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.601849Z","title":"Spin-statistics connexion, neutrinos, and big bang nucleosynthesis","venue":null,"work_id":"f07b7ed9-8ad2-43c2-ac91-d5a03a053822","year":1996},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.815236Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:3945facd3efbe496d96c19ed2a52cf49474eccd1487ba31d746cbe39bcb23cb2","observation_id":"03d8c0e1-9f94-46a7-a4f8-d4175575b3a2","resolution":{"observed_at":"2026-08-10T17:26:47.606638Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.586539Z","title":"Possible violation of the spin-statistics relation for neutri- nos: Cosmological and astrophysical consequences","venue":null,"work_id":"5aa2918b-f55b-407e-a85d-576dccb50538","year":2005},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.820189Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:4f40ea5723502e3b1f1fe22f222bf405fbd55b1102a27e7e81c8568bad4d3be3","observation_id":"6f39acfd-6f89-410b-aab9-b76a17a61da6","resolution":{"observed_at":"2026-08-10T17:26:47.591336Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.572013Z","title":"How massless neutrinos affect the cosmic microwave background damping tail","venue":null,"work_id":"1ac65269-0098-4fec-9047-fc2bca4f8098","year":2013},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.824715Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:03eeaf64c5d1093a719a8682c434eeb598129943f9301d9bb1edb6d730be81c6","observation_id":"0c025baa-f543-482a-9c90-32454c5b313f","resolution":{"observed_at":"2026-08-10T17:26:47.576749Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.556608Z","title":"Neutrinos in the cosmic microwave background epoch","venue":null,"work_id":"33666745-bdc2-4fec-8ea5-5f904d7cbd86","year":2013},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.829482Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:ad66c799b144638f940b3108b179ad304ed5fdf2a80e8bed0d963de87524511f","observation_id":"6e2a92de-7104-45f4-95e1-3cf053165df4","resolution":{"observed_at":"2026-08-10T17:26:47.561945Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.540700Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes","venue":null,"work_id":"7c13473c-673b-402f-8fac-922c33ccd2d2","year":2011},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.835162Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:062a81045eee256672f9093f56e340a91b124e2b08ae8a5b8c3a4914eff4e416","observation_id":"ec83848d-c328-4f71-bd20-33f0a3866bd4","resolution":{"observed_at":"2026-08-10T17:26:47.546007Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.524134Z","title":"Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with ΛCDM","venue":null,"work_id":"09bcc56d-746d-4a21-adc4-cbce50a25f33","year":2021},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.839697Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:a5c05d3d883f9391f8734fa0589e8cf676137044ad60578905365859e7e740d4","observation_id":"6db52fbc-a27a-4464-8b1e-3c07cfa1eef0","resolution":{"observed_at":"2026-08-10T17:26:47.529307Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.507928Z","title":"Planck2018 results: VI. Cosmological parameters","venue":null,"work_id":"d7179420-8297-4bc5-a319-1951420ee701","year":2020},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.844408Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:956053bac9745f9554b72516bc68f95100b6e835774368c702d4a8e977d59332","observation_id":"f51a06c8-7a08-443f-af2f-0c5b69f55c41","resolution":{"observed_at":"2026-08-10T17:26:47.512818Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14452","last_updated":"2025-06-24T16:02:02Z","snapshot_observed_at":"2026-07-06T20:54:50.337775Z","submitted_at":"2025-03-18T17:30:16Z","title":"The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\\Lambda$CDM Parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14452","snapshot_observed_at":"2026-08-10T17:26:46.849186Z","title":"The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and ΛCDM Parameters","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.849186Z"},"links":{"cited_paper":"/paper/2503.14452","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:565d8260558bd0758c12c95ef10f0a15f7c79bb254ca68374926258576722526","observation_id":"aa8809bc-5e32-4aec-9449-250ec7519c26","resolution":{"observed_at":"2026-08-10T17:26:46.849186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.492328Z","title":"A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3","venue":null,"work_id":"e6cba963-b67e-4838-b738-42101f6a6d78","year":2011},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.854744Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:38ba4694c54c5471bfdc4cd4517089d94350274babcd9bc355e13db4e4fa95b8","observation_id":"6a5e69e1-828f-4a0f-96f6-f7653f665602","resolution":{"observed_at":"2026-08-10T17:26:47.497347Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.477431Z","title":"A 2.4% DETERMINATION OF THE LOCAL V ALUE OF THE HUBBLE CONSTANT","venue":null,"work_id":"5de02bc3-55da-4b14-8136-4c0ef066c1e9","year":2016},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.859261Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:f350e04c9d2f7e88afcc56c00dd804aebf540b3059a8d94307e615798be15037","observation_id":"ee767ef1-a641-4431-a9fe-86e835dcc94d","resolution":{"observed_at":"2026-08-10T17:26:47.482310Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.461804Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s−1 Mpc−1 Uncertainty from the Hubble Space Telescope and the SH0ES Team","venue":null,"work_id":"9a036197-9f71-4145-9105-2301f1ee2783","year":2022},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.864003Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:88913536b82b8a5907d165436b786ef5d6508936088456e408badd3173a05daa","observation_id":"228c526c-25d3-4dc6-85c1-ae9de890b86c","resolution":{"observed_at":"2026-08-10T17:26:47.467040Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.445849Z","title":"The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters","venue":null,"work_id":"5a437065-3121-47c2-bef5-6eca2d222cdf","year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.873651Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:bbf184c02a15bad4fb58ac5f8647b2787aa17f03356fc6296a1df9b993f37427","observation_id":"7b460866-1849-4dc9-a752-9f41168b15c0","resolution":{"observed_at":"2026-08-10T17:26:47.451132Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.430091Z","title":null,"venue":null,"work_id":"367e0214-0c7f-4ba9-ab93-8e64eecb2e0b","year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.878728Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:08336f6fc076a65b1694d2a2ede70cf969c2afc543f0a15997933dadbb966d66","observation_id":"e0bc0221-3654-41f4-8768-aef4187c23fc","resolution":{"observed_at":"2026-08-10T17:26:47.435199Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.414917Z","title":"CMB lensing from Planck PR4 maps","venue":null,"work_id":"597d2899-7e19-435d-895b-4e81977e923d","year":2022},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.883965Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:d724614b59303e8c1c1ed826884128ae0e46f06a8f8bf0d9372c349c5c1cb453","observation_id":"614f385f-7e30-4e4a-aaf9-e76ca8254aea","resolution":{"observed_at":"2026-08-10T17:26:47.420099Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03000","last_updated":"2024-04-03T18:41:49Z","snapshot_observed_at":"2026-08-09T18:42:58.809582Z","submitted_at":"2024-04-03T18:41:49Z","title":"DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03000","snapshot_observed_at":"2026-08-10T17:26:46.888739Z","title":"DESI 2024 III: Baryon Acoustic Oscil- lations from Galaxies and Quasars","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.888739Z"},"links":{"cited_paper":"/paper/2404.03000","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:939fe18bbac14ab078d5e6d86196bc274c1fb0bc62b9cc7cd8be33bf1b245463","observation_id":"0307ccf2-bc2e-47db-80d2-8ebd51ef7cfa","resolution":{"observed_at":"2026-08-10T17:26:46.888739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03001","last_updated":"2024-09-27T07:18:27Z","snapshot_observed_at":"2026-08-09T21:48:39.628348Z","submitted_at":"2024-04-03T18:41:50Z","title":"DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03001","snapshot_observed_at":"2026-08-10T17:26:46.893827Z","title":"DESI 2024 IV: Baryon Acoustic Oscil- lations from the Lyman Alpha Forest","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.893827Z"},"links":{"cited_paper":"/paper/2404.03001","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:528687249ab02463d027d6412138b51a2574e414f1662e5ca7a5fee005dbc719","observation_id":"aadcd33c-5174-4e31-9e4f-bf4c0b8c823c","resolution":{"observed_at":"2026-08-10T17:26:46.893827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.00836","last_updated":"2024-05-23T20:18:53Z","snapshot_observed_at":"2026-08-11T15:50:21.202857Z","submitted_at":"2024-05-01T19:48:30Z","title":"No $\\nu$s is Good News","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.00836","snapshot_observed_at":"2026-08-10T17:26:46.899649Z","title":"No νs is Good News","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.899649Z"},"links":{"cited_paper":"/paper/2405.00836","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:ba1054a61ac4c70c01602803469ae1864959081a51502c3a421aeef02004dc9e","observation_id":"5f7ce3a0-0b37-4bcc-9a4c-9871f8848c18","resolution":{"observed_at":"2026-08-10T17:26:46.899649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.398071Z","title":"The Pantheon+ Analysis: Cosmological Constraints","venue":null,"work_id":"764fee04-772e-4548-b315-4c333c260feb","year":2022},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.905246Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:5eb32ab34d4371082fff8d31a9334959bdbb315e5247ae725fd3c0958ff976d9","observation_id":"1ba613d6-271b-4514-9baf-f63353359542","resolution":{"observed_at":"2026-08-10T17:26:47.403623Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.380216Z","title":"Cobaya: code for Bayesian analysis of hierarchical physical models","venue":null,"work_id":"2ef4048e-8ced-4b7a-819b-0cf7e676ea70","year":2021},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.911199Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:d98fde6976efeb55c07a45da833f23c7fd9c3c274392ccc73f5648de4eb7c4d5","observation_id":"2680c551-3437-4c65-b700-47c07e367af5","resolution":{"observed_at":"2026-08-10T17:26:47.385543Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.364473Z","title":"Cobaya: Bayesian analysis in cosmology","venue":null,"work_id":"dafaf643-aba5-4326-aec0-a6fc938e5be7","year":1910},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.916199Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:4a99e0a14487c95e952b8037f69f839c9779f75b2bd93ce1c909022a3bca414c","observation_id":"4d23f553-e1ce-432b-997d-97ea7a767df4","resolution":{"observed_at":"2026-08-10T17:26:47.369560Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.347935Z","title":"Cosmological parameters from CMB and other data: A Monte Carlo approach","venue":null,"work_id":"2280fd3e-3aa4-4e3a-80bc-8d74a8a5e4aa","year":2002},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.921356Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:7d6f2f08d114aeaecc8453f32850e6f7cc434fef2861ccad47c6e8d05580c4f3","observation_id":"b87d338c-a9bd-4fa2-bec1-cecc165c5f72","resolution":{"observed_at":"2026-08-10T17:26:47.353354Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.330871Z","title":"Efficient sampling of fast and slow cosmological parameters","venue":null,"work_id":"e7591abf-0dc9-4355-863e-94ee03c73696","year":2013},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.926237Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:018c904a469a90e90c2ddbc8b65e49abda1052fb54b26324cc577077917b6ce8","observation_id":"75c0fd38-ab64-4ba3-b934-0e4ad87116e9","resolution":{"observed_at":"2026-08-10T17:26:47.336352Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"math/0502099","last_updated":"2005-02-06T19:37:09Z","snapshot_observed_at":"2026-08-05T13:06:47.790593Z","submitted_at":"2005-02-06T19:37:09Z","title":"Taking Bigger Metropolis Steps by Dragging Fast Variables","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"math/0502099","snapshot_observed_at":"2026-08-10T17:26:46.931118Z","title":"Taking Bigger Metropolis Steps by Dragging Fast Variables","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.931118Z"},"links":{"cited_paper":"/paper/math/0502099","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:9124448b2443830bc46d4c8986cb6abfd15a58e31041a605f0167f0afcf1fd9d","observation_id":"d7b4b9d1-1d58-4c00-91b1-63ea81b256f3","resolution":{"observed_at":"2026-08-10T17:26:46.931118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:47.310716Z","title":"Inference from Iterative Simulation Using Multiple Sequences","venue":null,"work_id":"e2618673-af2d-4e1a-ba12-ef7293bc8957","year":1992},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.936025Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:bf4d447f1f65868d22239763a5246f290654f89f54b9b811e5fea371065bd645","observation_id":"6a55fffb-c03b-48e0-8dd9-6e8f964baa5e","resolution":{"observed_at":"2026-08-10T17:26:47.318874Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-08-10T17:26:46.940595Z","title":"GetDist: a Python package for analysing Monte Carlo samples","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.940595Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:07d0ee180e252bf1092f87bb4568ca979d27c2db09f75db6b69168081e2605e7","observation_id":"b488e88a-7bd1-448d-bacd-42373989914c","resolution":{"observed_at":"2026-08-10T17:26:46.940595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04492","last_updated":"2022-11-08T19:00:16Z","snapshot_observed_at":"2026-08-01T18:06:39.805867Z","submitted_at":"2022-11-08T19:00:16Z","title":"The Hubble Tension and Early Dark Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04492","snapshot_observed_at":"2026-08-10T17:26:46.945477Z","title":"Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.945477Z"},"links":{"cited_paper":"/paper/2211.04492","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:85284278ec1407b2b5b256f038cd2a06d0cbeb3c72216263b52a37c3f6843cbc","observation_id":"d72b5bc2-b35c-48de-9688-e072239afda8","resolution":{"observed_at":"2026-08-10T17:26:46.945477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.18368","last_updated":"2024-09-27T00:58:57Z","snapshot_observed_at":"2026-08-06T07:29:05.969397Z","submitted_at":"2024-09-27T00:58:57Z","title":"Constraining cosmological parameters using the pairwise kinematic Sunyaev-Zel'dovich effect with CMB-S4 and future galaxy cluster surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.18368","snapshot_observed_at":"2026-08-10T17:26:46.950206Z","title":"Constraining cosmological parameters using the pairwise kinematic Sunyaev-Zel’dovich effect with CMB-S4 and future galaxy cluster surveys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.950206Z"},"links":{"cited_paper":"/paper/2409.18368","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:11fa4a33679f4459621cb22b38770f2c47c282bbaa782374e2c2e8295169ce6b","observation_id":"47b1ed59-b95e-4a9a-9b2e-4031f2df3cec","resolution":{"observed_at":"2026-08-10T17:26:46.950206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T17:26:46.955199Z","title":"Euclid. I. Overview of the Euclid mis- sion","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.955199Z"},"links":{"citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:786af37e097ccd767092585ae114c425a09387892a53dae06fa3aec1bee661c0","observation_id":"0471f4b5-69c4-44b2-8b01-03063c2fcdca","resolution":{"observed_at":"2026-08-10T17:26:46.955199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-08-10T17:26:46.960352Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T17:26:46.960352Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2501.12264"},"observation_digest":"sha256:0976c2f1a194d4d837882a68f319ac16af4688e1392924cea3419028b4f58085","observation_id":"1344c154-42bc-417f-bdb3-5d2ac8cfad71","resolution":{"observed_at":"2026-08-10T17:26:46.960352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2501.12264","last_updated":"2025-07-02T06:02:06Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-10T17:17:52.647577Z","submitted_at":"2025-01-21T16:34:17Z","title":"Constraint on Neutrino Statistics from Cosmological Data"},"reference_resolution":{"displayed":37,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":12,"verified_exact":0,"verified_fuzzy":25},"total_outbound_references":37},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 37 of 37 outbound references and 1 inbound Pith citation observation for arXiv:2501.12264."}