{"as_of":"2026-08-05T02:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:aa8c0b65ad4ad8e3a56943cb968badbc4485b140d0f103c21af84171b5d45172","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":55,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":55,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":55,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":55,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T21:49:03.238925Z","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":"2026-07-04T15:29:55.139712Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-12T23:40:20.792511Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/1611.00036"},"observation_digest":"sha256:bdc55b74c4754119a7666fea517fc51432a4d61794e68664ab93405f380e164e","observation_id":"e2a33a77-2ac3-40e4-86d7-c19940e26762","resolution":{"observed_at":"2026-05-12T23:40:21.001448Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"reference_index":276,"source":"arxiv_source","source_observed_at":"2026-05-10T14:40:47.851452Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/1807.06209"},"observation_digest":"sha256:7b3a51357499ed916dcf08fcea37b5d50996dda06549abdcce86ab16ccd033fa","observation_id":"d7fcff22-b13d-4b28-931d-c5b3910a0862","resolution":{"observed_at":"2026-05-10T14:45:44.998079Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"1907.00728","last_updated":"2019-06-25T18:09:53Z","snapshot_observed_at":"2026-07-06T08:04:02.269421Z","submitted_at":"2019-06-25T18:09:53Z","title":"The Hawking temperature in the context of dark energy for Kerr-Newman and Kerr-Newman-AdS backgrounds","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-25T16:17:20.019065Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/1907.00728"},"observation_digest":"sha256:003728f3a8474e952d3b03590e653cd9e958e98c0c5f2e8a009de9b4b324ffa3","observation_id":"5749aef3-8445-4533-982e-46c32b9bacc9","resolution":{"observed_at":"2026-05-25T16:21:02.158231Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"1907.08010","last_updated":"2019-07-18T12:03:32Z","snapshot_observed_at":"2026-07-06T08:08:35.420176Z","submitted_at":"2019-07-18T12:03:32Z","title":"Cosmological searches for the neutrino mass scale and mass ordering","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-05-24T19:42:49.415260Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/1907.08010"},"observation_digest":"sha256:9bdcd50944984ea09a97b155edcde3d2b2dc6323e02a481efaf0a708eb8baabd","observation_id":"7d5910e3-50b0-4bb4-b92e-ee6643cd6726","resolution":{"observed_at":"2026-05-24T19:44:53.206085Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_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},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/1910.13970"},"observation_digest":"sha256:95fb1577b572e8fcdd259e7ad09dd6a61eb3093fc72a105627f3509f1682fe64","observation_id":"0e325ab4-e6ce-428e-b4be-5b57c62e5eb1","resolution":{"observed_at":"2026-05-14T23:58:42.854324Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2003.01100","last_updated":"2022-06-07T13:23:26Z","snapshot_observed_at":"2026-07-06T09:01:38.630614Z","submitted_at":"2020-03-02T18:51:00Z","title":"The landscape of QCD axion models","version":4},"reference_index":264,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2003.01100"},"observation_digest":"sha256:42ff8f6800d4dc06841248f62ac8927718f6c8896acb2d489b4ad855c92e18dd","observation_id":"d18a6dab-e21d-4701-8dba-2255f619b2a4","resolution":{"observed_at":"2026-05-16T02:27:14.498741Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_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},"reference_index":232,"source":"pdf_text","source_observed_at":"2026-05-12T02:13:10.766505Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2404.03002"},"observation_digest":"sha256:2522efe80907bcf9a8b132b091774308ff1a9ce059cf41bfa992b3af4cbedb63","observation_id":"7531d693-eb0f-442b-bb07-37d8dafbce9f","resolution":{"observed_at":"2026-05-12T02:13:10.973507Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2503.16355","last_updated":"2026-05-19T08:31:27Z","snapshot_observed_at":"2026-07-06T20:56:09.656767Z","submitted_at":"2025-03-20T17:13:57Z","title":"DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-22T23:07:09.906749Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2503.16355"},"observation_digest":"sha256:4060b8a037bb31be36698e461d9b18c36f6d742a5acf1c56ca843edbe842b473","observation_id":"b6de43da-c606-4359-a3bd-d16904a15c00","resolution":{"observed_at":"2026-05-22T23:07:14.014937Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2505.24732","last_updated":"2026-04-11T09:17:44Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-05-30T15:54:16Z","title":"The Quintom theory of dark energy after DESI DR2","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-05-19T13:08:20.192767Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2505.24732"},"observation_digest":"sha256:66a39c9520022e81f9a04cbaeae1184888a8de2bb8e799853ab8feeb98aafe3f","observation_id":"dd9a4179-bd63-4fe8-bfbb-ac971a58c40b","resolution":{"observed_at":"2026-05-19T13:12:19.286022Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-04T21:49:03.238925Z","title":"Ade et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.08029","last_updated":"2025-09-13T14:35:43Z","snapshot_observed_at":"2026-08-04T21:48:58.800743Z","submitted_at":"2025-09-09T13:36:34Z","title":"Scalar Field Reconstructions of Holographic Dark Energy Models with Applications to Chaplygin Gas, DBI, Yang-Mills, and NLED Frameworks","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-04T21:49:03.238925Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2509.08029"},"observation_digest":"sha256:5b69aae76fe0d7511e267a9a46755994207cafeff31ba9c713328e5e9264648a","observation_id":"36135e61-44de-4ef8-939f-cdea6561f515","resolution":{"observed_at":"2026-08-04T21:49:03.238925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2509.10456","last_updated":"2025-09-12T17:59:59Z","snapshot_observed_at":"2026-07-06T22:29:23.951457Z","submitted_at":"2025-09-12T17:59:59Z","title":"Gravitational Wave Signature and the Nature of Neutrino Masses: Majorana, Dirac, or Pseudo-Dirac?","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-18T17:14:34.641491Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2509.10456"},"observation_digest":"sha256:5613a0d23d989ff284c9ff5e2eb58aac03e2b446c9d48801838adae80254ba68","observation_id":"b28f9de9-f6b4-4667-a93e-68c2c8d3bbfc","resolution":{"observed_at":"2026-05-18T17:16:39.975726Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-04T00:32:15.149990Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.00918","last_updated":"2026-06-22T11:02:21Z","snapshot_observed_at":"2026-08-04T00:32:14.194221Z","submitted_at":"2025-11-02T12:39:08Z","title":"Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCore","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:15.149990Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2511.00918"},"observation_digest":"sha256:65455c28a945814580e78959f8cc291d87c734c4cd5c83024d3bd5f0c0438aee","observation_id":"c1cc7399-773b-4b8f-8fef-f6655cd6af54","resolution":{"observed_at":"2026-08-04T00:32:15.149990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-03T23:41:00.525623Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.04661","last_updated":"2026-06-10T16:49:52Z","snapshot_observed_at":"2026-08-03T23:40:57.883530Z","submitted_at":"2025-11-06T18:48:39Z","title":"unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T23:41:00.525623Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2511.04661"},"observation_digest":"sha256:c657650d2f63e9bef0e54aa138ccf5a903f5a5b4ae834ffe96496e89caac7399","observation_id":"3b4309cb-a1a6-41d1-bae4-9ded2f0c97e0","resolution":{"observed_at":"2026-08-03T23:41:00.525623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-03T23:20:05.019031Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.06640","last_updated":"2025-12-27T05:54:34Z","snapshot_observed_at":"2026-08-03T23:19:58.165611Z","submitted_at":"2025-11-10T02:37:36Z","title":"Starobinsky Inflation and the Latest CMB Data: A Subtle Tension?","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-03T23:20:05.019031Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2511.06640"},"observation_digest":"sha256:2eae832538500f0b9b81b6d4298994d5cf2530840d03a2f2b3818cb490e1fc6c","observation_id":"ef43a774-df0f-4886-a44d-c8522ae0fac9","resolution":{"observed_at":"2026-08-03T23:20:05.019031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2511.18657","last_updated":"2025-11-23T23:56:13Z","snapshot_observed_at":"2026-08-02T09:39:00.183185Z","submitted_at":"2025-11-23T23:56:13Z","title":"How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-17T05:42:44.912403Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2511.18657"},"observation_digest":"sha256:577f7a2e44786b36e9719d948045adf069c54c89e235141e2091f584a49a64e5","observation_id":"50a8d747-1d4e-4657-9b65-6fee5864954f","resolution":{"observed_at":"2026-05-17T05:44:07.427868Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-03T18:51:43.246500Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2512.04130","last_updated":"2026-07-26T05:14:02Z","snapshot_observed_at":"2026-08-04T06:15:07.631708Z","submitted_at":"2025-12-03T06:33:55Z","title":"Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\\omega_0\\omega_a$CDM","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T18:51:43.246500Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2512.04130"},"observation_digest":"sha256:5f1898a11b862553d2caf2dfd093ece7d9aebd197a20d57723c590afbb8049f9","observation_id":"7513339f-6453-4ae9-940d-e92445b68a9e","resolution":{"observed_at":"2026-08-03T18:51:43.246500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2601.02077","last_updated":"2026-04-04T13:29:01Z","snapshot_observed_at":"2026-08-02T21:22:34.193403Z","submitted_at":"2026-01-05T12:58:36Z","title":"Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity","version":2},"reference_index":133,"source":"pdf_text","source_observed_at":"2026-05-16T18:00:59.984076Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2601.02077"},"observation_digest":"sha256:d7f7f166ce49bb4af7653d29a20e2aa23da9f8ad63947a5f0cc3dbc5ec95344a","observation_id":"0afb1b5a-40c9-4992-91d6-83e0322fc448","resolution":{"observed_at":"2026-05-16T18:01:09.181429Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-03T08:41:50.598596Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-04T08:50:16.397178Z","submitted_at":"2026-01-22T18:10:50Z","title":"Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-03T08:41:50.598596Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:353a7491b6f3bde9da96c037c7e35523b023ac64edb336f61c7a354db3447d35","observation_id":"4a5c7feb-076f-4260-8b15-e122e7e51c76","resolution":{"observed_at":"2026-08-03T08:41:50.598596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2601.21432","last_updated":"2026-04-30T22:01:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-01-29T09:08:00Z","title":"Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-05-16T10:03:09.666511Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2601.21432"},"observation_digest":"sha256:28a1590616bc62b15ed96a83199d695a51331bb317672d47418bde7573aff3a5","observation_id":"636b1c63-7e5f-4278-ac69-673c649db8e3","resolution":{"observed_at":"2026-05-16T10:07:43.959523Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2602.15803","last_updated":"2026-05-06T09:12:37Z","snapshot_observed_at":"2026-07-11T23:17:59.926619Z","submitted_at":"2026-02-17T18:42:52Z","title":"Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-05-15T21:40:02.461824Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2602.15803"},"observation_digest":"sha256:0555f647b4fa55aee0f81f5fc243ac1bd22e7d5c3596d9dd9a0f6b96456b477d","observation_id":"e89a4f9f-2176-41ff-9658-d39c6c665baf","resolution":{"observed_at":"2026-05-15T21:40:20.651606Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2604.00978","last_updated":"2026-07-30T13:21:29Z","snapshot_observed_at":"2026-08-02T23:56:48.512843Z","submitted_at":"2026-04-01T14:48:43Z","title":"Nonlinear Lattice Framework for Inflation: Bridging stochastic inflation and the $\\delta{N}$ formalism","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-13T22:14:19.216242Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2604.00978"},"observation_digest":"sha256:d64a053b14a8da1e41b402d10eda064ce33fe4d663a93e5268a95a34bdcc8c67","observation_id":"383d9c58-726d-4f0b-87d4-3929ef4017ec","resolution":{"observed_at":"2026-05-13T22:18:21.376419Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-02T17:02:12.868395Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2604.00978","last_updated":"2026-07-30T13:21:29Z","snapshot_observed_at":"2026-08-02T23:56:48.512843Z","submitted_at":"2026-04-01T14:48:43Z","title":"Nonlinear Lattice Framework for Inflation: Bridging stochastic inflation and the $\\delta{N}$ formalism","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-02T17:02:12.868395Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2604.00978"},"observation_digest":"sha256:b1081f6438a90c9ad7234ca609e9f54ddebf4557d6e17a6787a739c6bf9d1e8f","observation_id":"c7c8737d-d794-4d24-857a-060f9551ddea","resolution":{"observed_at":"2026-08-02T17:02:12.868395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2604.09407","last_updated":"2026-04-10T15:20:40Z","snapshot_observed_at":"2026-07-06T22:58:17.167367Z","submitted_at":"2026-04-10T15:20:40Z","title":"Analytic compression of the effective field theory of the Lyman-alpha forest","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-10T16:51:14.158271Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2604.09407"},"observation_digest":"sha256:4405cdecb2d9b89b4a990496fcafcbbe666fdf6a338e70d5279ec065a0e3e9cf","observation_id":"dbcf4bed-b112-41b0-af42-06997b0f785e","resolution":{"observed_at":"2026-05-11T08:01:01.093475Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2604.11308","last_updated":"2026-04-13T11:08:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-13T11:08:34Z","title":"Dirac one-loop seesaw in a non-invertible fusion rule","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-05-10T16:32:37.745450Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2604.11308"},"observation_digest":"sha256:87383e9ac09d261c0cb8715ca638a194e28ccd67a828b78ab8ce354bef80218a","observation_id":"031c9c30-dac5-4f12-b50d-50ce78c9b071","resolution":{"observed_at":"2026-05-11T08:41:00.790785Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2604.25373","last_updated":"2026-05-20T10:49:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-28T08:38:43Z","title":"Generalizing the CPL Parametrization through Dark Sector Interaction","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-07T15:13:17.975105Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2604.25373"},"observation_digest":"sha256:a6af8d58814775df1586f9bdcbce12430df852bedc350bdd62f2c61d48eda56b","observation_id":"b4ff908a-aec0-4259-b247-27426e1f5d45","resolution":{"observed_at":"2026-05-12T00:31:16.948112Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2604.25373","last_updated":"2026-05-20T10:49:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-28T08:38:43Z","title":"Generalizing the CPL Parametrization through Dark Sector Interaction","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-21T08:31:42.162241Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2604.25373"},"observation_digest":"sha256:e9ffc16416db0406f17092c5d130eef64926a37b49d01c823bce30052d438fe3","observation_id":"5f51eff4-2cda-4178-9ba2-8e9bc66bf078","resolution":{"observed_at":"2026-05-21T08:34:05.900504Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2605.12606","last_updated":"2026-05-12T18:00:16Z","snapshot_observed_at":"2026-08-03T00:35:34.585187Z","submitted_at":"2026-05-12T18:00:16Z","title":"Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2605.12606"},"observation_digest":"sha256:e790865a21cc97ecc0310f25948b9bf3a3830ba7ca5b39396ec187fd56bd1239","observation_id":"7eeea064-521d-49df-b373-878cfbe23c68","resolution":{"observed_at":"2026-05-14T20:37:57.068209Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2605.15078","last_updated":"2026-05-14T17:02:28Z","snapshot_observed_at":"2026-08-04T08:49:01.234742Z","submitted_at":"2026-05-14T17:02:28Z","title":"KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions","version":1},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2605.15078"},"observation_digest":"sha256:88a16a887ddec078c18839da0e93a6d57645818e59bc59d0cc8a894857b8ab69","observation_id":"f484e798-9562-420c-a1d4-5d1d4eab6925","resolution":{"observed_at":"2026-05-15T03:24:53.760348Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2605.16501","last_updated":"2026-05-15T18:00:35Z","snapshot_observed_at":"2026-08-02T17:09:21.567607Z","submitted_at":"2026-05-15T18:00:35Z","title":"Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2605.16501"},"observation_digest":"sha256:2dd95bd0f85189584cb5d2d7240458f95a510ada5d971d6bcda6a7e8efab2f84","observation_id":"300d0611-31cd-4b38-b414-cd6efdd105e4","resolution":{"observed_at":"2026-05-20T16:03:33.243453Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2605.23746","last_updated":"2026-05-22T15:20:11Z","snapshot_observed_at":"2026-08-02T08:23:53.526666Z","submitted_at":"2026-05-22T15:20:11Z","title":"Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2605.23746"},"observation_digest":"sha256:f04f01f185783ab9e79ce5efab15c5d9da3cd6417a71936f831354fcced025dc","observation_id":"86a05477-e4a1-459b-b5cc-d9a483681740","resolution":{"observed_at":"2026-05-25T03:35:17.329608Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.00205","last_updated":"2026-05-29T18:00:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-29T18:00:00Z","title":"Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages","version":1},"reference_index":142,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.00205"},"observation_digest":"sha256:3b34d81c4652ca034b7ad4b5b356402227c28d303217ade54b02e168f6ec9950","observation_id":"a4030be3-a18a-4641-b015-7790cda667d8","resolution":{"observed_at":"2026-06-28T21:52:40.156942Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.01158","last_updated":"2026-05-31T11:03:43Z","snapshot_observed_at":"2026-07-06T23:41:43.820102Z","submitted_at":"2026-05-31T11:03:43Z","title":"Deep Optical Follow-up Observations to IceCube Cosmic Neutrinos: a case for IC230724A with Subaru/HSC and prospects with Rubin/LSST","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.01158"},"observation_digest":"sha256:62d3c38a8aa37a2d70fd2632e82b989a1a199a59432c8d7d1cfe304482f55559","observation_id":"b1959198-238d-4e9a-8d34-1f1f457c13e3","resolution":{"observed_at":"2026-06-28T16:42:23.532039Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.02712","last_updated":"2026-07-14T21:19:16Z","snapshot_observed_at":"2026-08-02T12:36:54.822821Z","submitted_at":"2026-06-01T18:00:03Z","title":"Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario","version":1},"reference_index":181,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.02712"},"observation_digest":"sha256:c417bb188c480b71e36db3238d30267cf7bb3c4dc210fb8daa0337039ffadaad","observation_id":"0f30e1e8-05c0-451d-878d-5bf964209223","resolution":{"observed_at":"2026-06-28T15:32:20.080619Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.03192","last_updated":"2026-06-02T05:50:43Z","snapshot_observed_at":"2026-07-06T23:43:31.629075Z","submitted_at":"2026-06-02T05:50:43Z","title":"Fifty years of primordial helium abundances: A statistical reanalysis","version":1},"reference_index":131,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.03192"},"observation_digest":"sha256:8eba3b33ff70ab0ab96b8b61e9076a1a3443e8a1136d02738f75cdc434620691","observation_id":"b456eca9-76f3-4e88-b8d9-64a7e8215a5d","resolution":{"observed_at":"2026-06-28T09:21:49.728570Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.05006","last_updated":"2026-06-03T15:28:19Z","snapshot_observed_at":"2026-07-06T23:45:02.342193Z","submitted_at":"2026-06-03T15:28:19Z","title":"A Measurement of the Thermal and Ionization State of the IGM at $z < 0.5$","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.05006"},"observation_digest":"sha256:078f87e58de5918a90b5b3044691265409119fd1bf55af3bbbc6fb5dcec9741e","observation_id":"67189b48-4e32-4252-8030-c9be793ee356","resolution":{"observed_at":"2026-06-28T04:51:40.174406Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.12605","last_updated":"2026-06-10T19:02:44Z","snapshot_observed_at":"2026-07-06T23:51:31.502574Z","submitted_at":"2026-06-10T19:02:44Z","title":"Feedback-Free Star Formation in Clusters within a Galaxy Simulated at High Resolution in Cosmic Dawn","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.12605"},"observation_digest":"sha256:6ac0cd19caf9590f6536b41899500764fa619f30d40409ce4905fd1d9c49d97f","observation_id":"7dc8e9c9-f09d-47bc-b436-235dd93ca174","resolution":{"observed_at":"2026-06-27T08:50:46.106687Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.20795","last_updated":"2026-06-18T18:00:01Z","snapshot_observed_at":"2026-08-02T04:32:30.860957Z","submitted_at":"2026-06-18T18:00:01Z","title":"Raising the reionization optical depth with inflationary CMB features","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-06-26T15:57:34.321688Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.20795"},"observation_digest":"sha256:f8ee8d2bae11af3d74e2a89f1718cd00553448658b6f39c1a7a9df4840ac6ff7","observation_id":"1a68ab6f-fbbb-48b8-857a-c208e253c264","resolution":{"observed_at":"2026-07-04T05:29:35.894920Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.21105","last_updated":"2026-06-19T05:15:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-19T05:15:18Z","title":"Little Red Dots as Supermassive Analogs of SS 433","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.21105"},"observation_digest":"sha256:44e5524629eafb9ae1f80877ed704c88fa86635cfa593b3036178d9f1eaa429a","observation_id":"fc32181d-d91b-41d1-894c-0f74b2a1971f","resolution":{"observed_at":"2026-06-26T14:09:31.439951Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.23651","last_updated":"2026-06-22T17:36:23Z","snapshot_observed_at":"2026-07-06T23:58:20.975630Z","submitted_at":"2026-06-22T17:36:23Z","title":"Revisiting the 'Lensing is Low' Problem with UNIONS","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.23651"},"observation_digest":"sha256:da14103e90254c006ec06e22ec46f823b89727ba70a7b551478f2d7b72b650f3","observation_id":"30c75aad-e222-4180-853e-6ad800aa27d0","resolution":{"observed_at":"2026-06-26T07:19:07.065258Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.26234","last_updated":"2026-06-24T18:00:02Z","snapshot_observed_at":"2026-08-01T19:46:42.787193Z","submitted_at":"2026-06-24T18:00:02Z","title":"Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level","version":1},"reference_index":153,"source":"pdf_text","source_observed_at":"2026-06-26T01:38:09.398349Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.26234"},"observation_digest":"sha256:63ec3740057c0766c56737408a00dc45ded6235ec645949c3cfee367d1dd0f3d","observation_id":"ee6ceed8-8764-411f-befa-5e570a37a981","resolution":{"observed_at":"2026-07-04T15:29:55.140975Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.30746","last_updated":"2026-07-27T13:51:13Z","snapshot_observed_at":"2026-08-02T09:30:12.704470Z","submitted_at":"2026-06-29T18:00:14Z","title":"Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.30746"},"observation_digest":"sha256:e73cd7dca75c951356acade93d7198a86b37101d380ac3076710c6a35e12777e","observation_id":"cabb806f-d829-45a9-a20a-b707e22ee53d","resolution":{"observed_at":"2026-07-01T01:45:14.318261Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.30903","last_updated":"2026-07-22T21:14:59Z","snapshot_observed_at":"2026-08-02T09:29:07.475144Z","submitted_at":"2026-06-29T20:49:45Z","title":"Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\\Lambda$CDM","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-01T01:12:19.031543Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.30903"},"observation_digest":"sha256:c6645733ce512ce39b80ce38be6314be470a1f9081ea0ab3c59f047b0f4bc23e","observation_id":"4536e322-5958-4b8e-a832-3fff335ffcc8","resolution":{"observed_at":"2026-07-01T01:15:13.342123Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-02T09:29:12.823660Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2606.30903","last_updated":"2026-07-22T21:14:59Z","snapshot_observed_at":"2026-08-02T09:29:07.475144Z","submitted_at":"2026-06-29T20:49:45Z","title":"Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\\Lambda$CDM","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-02T09:29:12.823660Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.30903"},"observation_digest":"sha256:afbba8a857f6bc9e9bae29e2dee9bf49980a7c9d4093dbcaf87a9abaf4e30787","observation_id":"cf389b3a-57c9-43e9-bcf1-e39e3ea306e5","resolution":{"observed_at":"2026-08-02T09:29:12.823660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2606.31434","last_updated":"2026-06-30T10:03:04Z","snapshot_observed_at":"2026-07-31T06:38:17.036331Z","submitted_at":"2026-06-30T10:03:04Z","title":"Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2606.31434"},"observation_digest":"sha256:7e84bf2a3a3d631d5e8e71aa733ee28043f50dbc6278df48442fa416ed4dc747","observation_id":"0f1ca7b5-74ff-40cd-a237-2ed69a51bc8b","resolution":{"observed_at":"2026-07-01T04:45:20.813981Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":"1303.5076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-04T15:29:55.139712Z","title":"Planck 2013 results. XVI. Cosmological parameters","venue":"astro-ph.CO","work_id":"70bc4d16-aaf6-4ea8-b402-2f43285e38db","year":2013},"citing_paper":{"arxiv_id":"2607.00764","last_updated":"2026-07-01T10:48:01Z","snapshot_observed_at":"2026-07-07T00:06:25.004202Z","submitted_at":"2026-07-01T10:48:01Z","title":"The age of the Universe from a large sample of the oldest Galactic stars","version":1},"reference_index":181,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.00764"},"observation_digest":"sha256:8d8e22f7a138f42c6fa2a397e54e8bdec8c24fe247b01eb283cd5f18314bcf4d","observation_id":"fd42122f-2ed3-4b89-911c-3b3c232b7241","resolution":{"observed_at":"2026-07-02T06:46:43.371061Z","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":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-12T07:35:44.141755Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.02706","last_updated":"2026-07-02T18:49:09Z","snapshot_observed_at":"2026-07-12T07:35:39.743517Z","submitted_at":"2026-07-02T18:49:09Z","title":"S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups","version":1},"reference_index":227,"source":"arxiv_source","source_observed_at":"2026-07-12T07:35:44.141755Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.02706"},"observation_digest":"sha256:503cfe4c9852f561d8e38eca18cb94c9df317f68cd1205697c36fe7e8bf539dd","observation_id":"3c0d6776-1147-48cf-85e1-7456e58c7b61","resolution":{"observed_at":"2026-07-12T07:35:44.141755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-12T01:57:41.636527Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.03514","last_updated":"2026-07-03T17:39:29Z","snapshot_observed_at":"2026-07-12T01:57:37.596267Z","submitted_at":"2026-07-03T17:39:29Z","title":"Disentangling modified gravity and galaxy bias with field-level inference","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-07-12T01:57:41.636527Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.03514"},"observation_digest":"sha256:03e0aea1985e0169897d2aba823aaa5a1da2a63d57ace0911ed6fba84e3b989b","observation_id":"2e729d21-32cc-4edc-8694-e4b1b5ccfe5d","resolution":{"observed_at":"2026-07-12T01:57:41.636527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-11T06:44:15.468115Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.05502","last_updated":"2026-07-06T18:00:02Z","snapshot_observed_at":"2026-08-01T14:53:41.107553Z","submitted_at":"2026-07-06T18:00:02Z","title":"The tidal features of the classical Milky Way satellites: Expected in MOND but inconsistent with cold dark matter models","version":1},"reference_index":140,"source":"arxiv_source","source_observed_at":"2026-07-11T06:44:15.468115Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.05502"},"observation_digest":"sha256:28096ea55975d9f9dec5db91bb9b7b4d634089f46c54987cc340d9328906f5e3","observation_id":"ce46eb67-904b-49f9-a285-72005e62fe84","resolution":{"observed_at":"2026-07-11T06:44:15.468115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-13T06:28:17.325404Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.08818","last_updated":"2026-07-09T18:00:01Z","snapshot_observed_at":"2026-08-01T23:36:58.399233Z","submitted_at":"2026-07-09T18:00:01Z","title":"Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-13T06:28:17.325404Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.08818"},"observation_digest":"sha256:220a15053498bfa8ef1da18111952e259d62bd84c33428652708627f50574268","observation_id":"ee7ed465-6483-445c-bc6f-25abfd2ecf0f","resolution":{"observed_at":"2026-07-13T06:28:17.325404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-13T04:41:12.165957Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.09209","last_updated":"2026-07-10T08:56:40Z","snapshot_observed_at":"2026-08-01T19:30:08.283612Z","submitted_at":"2026-07-10T08:56:40Z","title":"Performance of morphological classifiers for galaxy mergers compared to current machine learning methods","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-13T04:41:12.165957Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.09209"},"observation_digest":"sha256:5c813cc0ab7e0b01fbdcaa940122763f44ce5c849d2ec908d43ff4ecc084807c","observation_id":"a31b8e1a-d0b3-4af7-afc5-5eda07203b14","resolution":{"observed_at":"2026-07-13T04:41:12.165957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-07-14T05:32:07.775931Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.11448","last_updated":"2026-07-13T11:59:50Z","snapshot_observed_at":"2026-07-16T23:19:47.905536Z","submitted_at":"2026-07-13T11:59:50Z","title":"Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster","version":1},"reference_index":298,"source":"arxiv_source","source_observed_at":"2026-07-14T05:32:07.775931Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.11448"},"observation_digest":"sha256:99db4b10a0bf6ebcd8011658dcbb27bb4f3b56b554049b559bfa83ea05269f0b","observation_id":"26e0fdf1-4372-42d6-bf68-c6e5ee091321","resolution":{"observed_at":"2026-07-14T05:32:07.775931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-02T02:45:05.943774Z","title":"arXiv , Author =:1303.5076 , Journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14254","last_updated":"2026-07-15T18:12:40Z","snapshot_observed_at":"2026-08-03T07:08:16.988129Z","submitted_at":"2026-07-15T18:12:40Z","title":"Charting the expansion of the Universe from z$\\sim$0 to z$\\sim$14 with HII galaxies","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-02T02:45:05.943774Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.14254"},"observation_digest":"sha256:9fa0f04292dff0b1e6d946bbda7a41cfa98ea18de54cbd60481f360b27ed7c47","observation_id":"6e76b9d9-6534-4e31-b912-c506ebe6eafc","resolution":{"observed_at":"2026-08-02T02:45:05.943774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-02T01:39:56.319643Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.14626","last_updated":"2026-07-16T06:44:15Z","snapshot_observed_at":"2026-08-04T03:18:12.809981Z","submitted_at":"2026-07-16T06:44:15Z","title":"Random walks around black holes and low-frequency X-ray variability","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-02T01:39:56.319643Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.14626"},"observation_digest":"sha256:64c614cc55edaf27ae136a033d318eda50694ca265b91b0701dbc9d83c6851b7","observation_id":"4c626ad1-61a1-4ed3-8e55-092e10687ab7","resolution":{"observed_at":"2026-08-02T01:39:56.319643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-02T01:08:00.476137Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.14785","last_updated":"2026-07-21T13:43:01Z","snapshot_observed_at":"2026-08-04T19:16:04.573615Z","submitted_at":"2026-07-16T10:02:30Z","title":"Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-02T01:08:00.476137Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.14785"},"observation_digest":"sha256:15673933b0603a2d210b186ba4fdb1b3b126dec23f8ba060f2400d121ab289db","observation_id":"42b16e5d-607b-4393-9c09-a43cb8198fb0","resolution":{"observed_at":"2026-08-02T01:08:00.476137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-03T04:36:20.595640Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.29562","last_updated":"2026-07-31T15:52:41Z","snapshot_observed_at":"2026-08-05T01:14:53.579589Z","submitted_at":"2026-07-31T15:52:41Z","title":"Late Time Dynamical Dark Energy and the CMB-Distance Ladder Tension","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-03T04:36:20.595640Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2607.29562"},"observation_digest":"sha256:366e82fd27e78707b9bf33e66a90df5d2c3fd0042e849dbe9909eb6c1005b7f6","observation_id":"9ed23e12-6aaf-40d0-a2b3-121d2f6e78e4","resolution":{"observed_at":"2026-08-03T04:36:20.595640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1303.5076/citation-record","integrity":"/paper/1303.5076/integrity","json":"/paper/1303.5076/citation-record.json","paper":"/paper/1303.5076"},"outbound":[],"paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T03:09:14.953676Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters"},"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 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 55 inbound Pith citation observations for arXiv:1303.5076."}