{"as_of":"2026-08-17T23:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:aa09dd2b0b0215373be2266d763946796bba541c382a03415dc849bcc747cc65","coverage":[{"denominator":71,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":71,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:18:41.680695Z","state":"measured"},{"denominator":73,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":73,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T17:50:45.987390Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.13154","snapshot_observed_at":"2026-08-01T17:50:45.987390Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.17500","last_updated":"2026-07-20T03:07:19Z","snapshot_observed_at":"2026-08-16T22:34:23.486094Z","submitted_at":"2026-07-20T03:07:19Z","title":"Simultaneous inference of isotropic and anisotropic polarization rotation angles for next-generation cosmic microwave background experiments","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-01T17:50:45.987390Z"},"links":{"cited_paper":"/paper/2504.13154","citing_paper":"/paper/2607.17500"},"observation_digest":"sha256:2c6aa80f467728619ba7c3d3115e05f7a00395d4a99d5fa708f305de67a914ef","observation_id":"2da3d224-532e-4c6b-9ae8-626707c4d9f6","resolution":{"observed_at":"2026-08-01T17:50:45.987390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.13154","snapshot_observed_at":"2026-08-01T09:47:02.648546Z","title":"Constraints on anisotropic cosmic bire- fringence from CMB B-mode polarization,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.27318","last_updated":"2026-07-29T18:00:00Z","snapshot_observed_at":"2026-08-15T10:20:43.404096Z","submitted_at":"2026-07-29T18:00:00Z","title":"Wading the String Bog: CMB Birefringence in the Swampland","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-01T09:47:02.648546Z"},"links":{"cited_paper":"/paper/2504.13154","citing_paper":"/paper/2607.27318"},"observation_digest":"sha256:5e6e5f21efae97b34a4898cce897f874af821f3a23b9a97572d9d7747a626bb1","observation_id":"561215e8-e88e-4b28-a535-9361ab6db22c","resolution":{"observed_at":"2026-08-01T09:47:02.648546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2504.13154/citation-record","integrity":"/paper/2504.13154/integrity","json":"/paper/2504.13154/citation-record.json","paper":"/paper/2504.13154"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"0712.4082","last_updated":"2008-02-24T02:10:23Z","snapshot_observed_at":"2026-08-15T10:24:43.189469Z","submitted_at":"2007-12-25T19:43:36Z","title":"From Equivalence Principles to Cosmology: Cosmic Polarization Rotation, CMB Observation, Neutrino Number Asymmetry, Lorentz Invariance and CPT","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0712.4082","snapshot_observed_at":"2026-08-16T12:18:40.376158Z","title":"Ni, From Equivalence Principles to Cosmol- ogy: Cosmic Polarization Rotation, CMB Observa- tion, Neutrino Number Asymmetry, Lorentz Invariance and CPT, Prog","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.376158Z"},"links":{"cited_paper":"/paper/0712.4082","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:948764896462ca3d2f977d40cdd24f7152cc247d135dd6edb468fa639220cfd9","observation_id":"9a6f364b-6d3c-4309-b1cc-67fefb3ceec0","resolution":{"observed_at":"2026-08-16T12:18:40.376158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.13919","last_updated":"2024-05-08T14:32:17Z","snapshot_observed_at":"2026-08-16T17:18:04.305972Z","submitted_at":"2022-02-28T16:13:33Z","title":"New physics from the polarised light of the cosmic microwave background","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.13919","snapshot_observed_at":"2026-08-16T12:18:40.457170Z","title":"Komatsu, New physics from the polarized light of the cosmic microwave background, Nature Rev","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.457170Z"},"links":{"cited_paper":"/paper/2202.13919","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:b7f10f8e13f25fcff334fa4ac897def8d35a081ce58373c19abd43b06d8f471e","observation_id":"dee36dbb-66e3-4580-a3f9-7fc1f200ce65","resolution":{"observed_at":"2026-08-16T12:18:40.457170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0802.4210","last_updated":"2009-03-19T11:06:21Z","snapshot_observed_at":"2026-08-15T10:20:32.765270Z","submitted_at":"2008-02-28T14:25:10Z","title":"Rotation of Linear Polarization Plane and Circular Polarization from Cosmological Pseudoscalar Fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0802.4210","snapshot_observed_at":"2026-08-16T12:18:40.464452Z","title":"Finelli and M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.464452Z"},"links":{"cited_paper":"/paper/0802.4210","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:0681d83e1143f2208f660303ee7c240d849745f27acbba6487a1dc9f8d53a17d","observation_id":"9a939b72-0a97-4a79-8a4b-f48d89fa3cad","resolution":{"observed_at":"2026-08-16T12:18:40.464452Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.02104","last_updated":"2017-02-25T01:12:24Z","snapshot_observed_at":"2026-08-14T21:26:45.184444Z","submitted_at":"2016-12-07T03:03:34Z","title":"Axion Dark Matter Induced Cosmic Microwave Background $B$-modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.02104","snapshot_observed_at":"2026-08-16T12:18:40.470838Z","title":"Liu and K.-W","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.470838Z"},"links":{"cited_paper":"/paper/1612.02104","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:3e243e1ddf4ecf0ccb7cb3b83f874a4e7519e7b2a022297e5ca881e82fc24062","observation_id":"10c30bbf-2ba6-4fe9-9a12-25c039dbb890","resolution":{"observed_at":"2026-08-16T12:18:40.470838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.02666","last_updated":"2019-07-30T09:43:35Z","snapshot_observed_at":"2026-08-17T02:18:05.143265Z","submitted_at":"2019-03-07T00:19:45Z","title":"Axion Dark Matter Detection with CMB Polarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.02666","snapshot_observed_at":"2026-08-16T12:18:40.474321Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.474321Z"},"links":{"cited_paper":"/paper/1903.02666","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:ea4ca55eca816f189b92c35ffaf8c7a98e853795e918bd6a73c0e68b9c9fd4b3","observation_id":"22c79f92-e51a-4ad1-877b-52c3d2852667","resolution":{"observed_at":"2026-08-16T12:18:40.474321Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07804","last_updated":"2023-01-26T10:30:32Z","snapshot_observed_at":"2026-08-16T16:32:04.519846Z","submitted_at":"2022-09-16T09:07:51Z","title":"Isotropic cosmic birefringence from early dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07804","snapshot_observed_at":"2026-08-16T12:18:40.478287Z","title":"Murai, F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.478287Z"},"links":{"cited_paper":"/paper/2209.07804","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:6374be4f026138c9227d572c8a6cd273008d9d56eac45a2da459e5e6002076f5","observation_id":"af027a07-0b55-4059-9228-9a497909d37b","resolution":{"observed_at":"2026-08-16T12:18:40.478287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.15369","last_updated":"2023-08-30T08:24:11Z","snapshot_observed_at":"2026-08-16T15:44:59.524055Z","submitted_at":"2023-03-27T16:35:37Z","title":"Constraint on Early Dark Energy from Isotropic Cosmic Birefringence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.15369","snapshot_observed_at":"2026-08-16T12:18:40.482519Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.482519Z"},"links":{"cited_paper":"/paper/2303.15369","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:7cd9d100c566ae449fda90783a5c49d30eacb61adc213dea36634ce8e1eeac8f","observation_id":"2f4a1b95-a0fe-448a-8159-1cb7084614cb","resolution":{"observed_at":"2026-08-16T12:18:40.482519Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.11894","last_updated":"2021-05-18T05:29:24Z","snapshot_observed_at":"2026-08-16T19:03:45.236465Z","submitted_at":"2020-11-24T04:48:11Z","title":"Detection of isotropic cosmic birefringence and its implications for axion-like particles including dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.11894","snapshot_observed_at":"2026-08-16T12:18:40.485466Z","title":"Fujita, K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.485466Z"},"links":{"cited_paper":"/paper/2011.11894","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:aeb381aaafd443bb06135e53c9e02c742ee5038ff67de80ea63c543a92a43a8c","observation_id":"3dcef9cf-3135-4ecb-993c-ac4f4838205b","resolution":{"observed_at":"2026-08-16T12:18:40.485466Z","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":"2026-08-16T12:18:40.488684Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.488684Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:a0e7718ecc4922288f8642d354ce4306d122348b2734863809474def66b05f2b","observation_id":"45e5fef5-a623-4f0d-a253-f0358a932969","resolution":{"observed_at":"2026-08-16T12:18:40.488684Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.02473","last_updated":"2021-03-11T06:06:40Z","snapshot_observed_at":"2026-08-16T16:27:44.553512Z","submitted_at":"2020-08-06T06:36:07Z","title":"Probing Axion-like Particles via CMB Polarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.02473","snapshot_observed_at":"2026-08-16T12:18:40.491487Z","title":"Fujita, Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.491487Z"},"links":{"cited_paper":"/paper/2008.02473","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:a6c75d95dc56e1c8d6a1a694a8cf68608195d2d62a0e9dbc218a097256265860","observation_id":"0bb98658-8254-4f4c-a1c1-d1e65e346491","resolution":{"observed_at":"2026-08-16T12:18:40.491487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.5877","last_updated":"2010-12-10T20:54:23Z","snapshot_observed_at":"2026-08-15T05:01:52.240097Z","submitted_at":"2010-11-26T20:58:04Z","title":"Axions as Quintessence in String Theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.5877","snapshot_observed_at":"2026-08-16T12:18:40.601193Z","title":"Panda, Y","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.601193Z"},"links":{"cited_paper":"/paper/1011.5877","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:509917e301fc7ee5eb2a5a672e240ddae9ddb0ea4398789e3800feba3b5ba8eb","observation_id":"a8e6b568-f12a-4e9f-ae5e-1b857d68cc60","resolution":{"observed_at":"2026-08-16T12:18:40.601193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.12602","last_updated":"2021-06-23T18:01:10Z","snapshot_observed_at":"2026-08-16T18:14:58.157357Z","submitted_at":"2021-06-23T18:01:10Z","title":"Cosmic Birefringence and Electroweak Axion Dark Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.12602","snapshot_observed_at":"2026-08-16T12:18:40.670012Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.670012Z"},"links":{"cited_paper":"/paper/2106.12602","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:bf98a93853092cfb96f7f43ac158594e5015b153f267f05fec18c015ac7c1ca2","observation_id":"3c64efe5-47c7-4045-88fc-60ebe60106cd","resolution":{"observed_at":"2026-08-16T12:18:40.670012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.02150","last_updated":"2022-10-10T06:51:54Z","snapshot_observed_at":"2026-08-16T22:33:02.244209Z","submitted_at":"2021-08-04T16:30:29Z","title":"Implications of the Cosmic Birefringence Measurement for the Axion Dark Matter Search","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.02150","snapshot_observed_at":"2026-08-16T12:18:40.672807Z","title":"Obata, Implications of the cosmic birefringence mea- surement for the axion dark matter search, JCAP 09, 062, arXiv:2108.02150 [astro-ph.CO]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.672807Z"},"links":{"cited_paper":"/paper/2108.02150","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:fab9cf8750d84269a8c15cdceec24f606320287d59bbcb4a609d8f21ec35cd0f","observation_id":"0c374364-e1a4-4917-89c9-859c3437404b","resolution":{"observed_at":"2026-08-16T12:18:40.672807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.09409","last_updated":"2022-09-07T13:56:10Z","snapshot_observed_at":"2026-08-16T17:13:44.513284Z","submitted_at":"2022-03-17T16:04:45Z","title":"Cosmic Birefringence from Monodromic Axion Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.09409","snapshot_observed_at":"2026-08-16T12:18:40.676488Z","title":"Gasparotto and I","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.676488Z"},"links":{"cited_paper":"/paper/2203.09409","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:e30f3ddb4d7e7d6a2fd8dd688fb4245a806e94f6646c3acca41f4fa55eabfa9d","observation_id":"872872b1-60b5-4a9b-b189-0fadee2785cc","resolution":{"observed_at":"2026-08-16T12:18:40.676488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.07971","last_updated":"2023-05-01T07:04:06Z","snapshot_observed_at":"2026-08-16T16:27:13.657104Z","submitted_at":"2023-01-19T09:52:49Z","title":"Redshift evolution of cosmic birefringence in CMB anisotropies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07971","snapshot_observed_at":"2026-08-16T12:18:40.679991Z","title":"Galaverni, F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.679991Z"},"links":{"cited_paper":"/paper/2301.07971","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:845a7253275be9149b928af66147ee74836e7c0fdef7b624038760dc0ddf3ffc","observation_id":"367abc4b-0433-47b1-b199-f360df658dac","resolution":{"observed_at":"2026-08-16T12:18:40.679991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.11576","last_updated":"2021-02-26T12:03:38Z","snapshot_observed_at":"2026-08-16T18:56:54.859391Z","submitted_at":"2020-12-21T18:53:54Z","title":"Kilobyte Cosmic Birefringence from ALP Domain Walls","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.11576","snapshot_observed_at":"2026-08-16T12:18:40.683298Z","title":"Takahashi and W","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.683298Z"},"links":{"cited_paper":"/paper/2012.11576","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:53c67e5218a1313c78acc9f3953143bcf510365ef848b7030c16faaf76997c66","observation_id":"167659c1-6b61-41ad-ad53-42ba5838a1b9","resolution":{"observed_at":"2026-08-16T12:18:40.683298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.05083","last_updated":"2022-05-22T16:46:48Z","snapshot_observed_at":"2026-08-16T17:01:16.286343Z","submitted_at":"2022-05-10T18:00:00Z","title":"Power spectrum of domain-wall network and its implications for isotropic and anisotropic cosmic birefringence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.05083","snapshot_observed_at":"2026-08-16T12:18:40.686987Z","title":"Kitajima, F","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.686987Z"},"links":{"cited_paper":"/paper/2205.05083","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:5936d414e459e31e08dc268aecea7d741d15eab224236c717ffbd4cde6f3770c","observation_id":"faa7bfd2-d2a7-4e1c-940d-c59189055119","resolution":{"observed_at":"2026-08-16T12:18:40.686987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.08391","last_updated":"2022-08-17T16:32:31Z","snapshot_observed_at":"2026-08-16T16:38:36.494458Z","submitted_at":"2022-08-17T16:32:31Z","title":"Searching for axion-like particles through CMB birefringence from string-wall networks","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.08391","snapshot_observed_at":"2026-08-16T12:18:40.690240Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.690240Z"},"links":{"cited_paper":"/paper/2208.08391","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:39f2aca6bf5866b917b531ea6b92c7fef0584dff6a4f1102953807a749d8931a","observation_id":"c2cd0aa7-07f6-4cd2-9d4d-ccbcea720d78","resolution":{"observed_at":"2026-08-16T12:18:40.690240Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.06849","last_updated":"2022-12-27T13:07:08Z","snapshot_observed_at":"2026-08-17T11:51:25.030407Z","submitted_at":"2022-11-13T08:36:52Z","title":"Stability of domain wall network with initial inflationary fluctuations, and its implications for cosmic birefringence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.06849","snapshot_observed_at":"2026-08-16T12:18:40.694449Z","title":"Gonzalez, N","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.694449Z"},"links":{"cited_paper":"/paper/2211.06849","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:2c75aa281482cf7f768eb9828551b7c5c62f66c48644a34f3e6f0dbd42db26a6","observation_id":"409ab412-f674-4b08-8ea7-627809a2a347","resolution":{"observed_at":"2026-08-16T12:18:40.694449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0301124","last_updated":"2003-05-06T17:23:26Z","snapshot_observed_at":"2026-07-07T03:58:50.379254Z","submitted_at":"2003-01-17T01:15:56Z","title":"Ultraviolet modifications of dispersion relations in effective field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0301124","snapshot_observed_at":"2026-08-16T12:18:40.745583Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.745583Z"},"links":{"cited_paper":"/paper/hep-ph/0301124","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:107f7ff4ed105515a2a9b242f83466b810fabcc8902a896b390201763bf2fcb5","observation_id":"d8c564fe-e930-4da1-8718-1512794efa34","resolution":{"observed_at":"2026-08-16T12:18:40.745583Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0310368","last_updated":"2003-11-21T21:36:01Z","snapshot_observed_at":"2026-08-16T16:28:25.456480Z","submitted_at":"2003-10-31T20:00:11Z","title":"Spectral Dependence of CMB Polarization and Parity","version":2},"cited_work":{"arxiv_id":"hep-ph/0310368","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0310368","snapshot_observed_at":"2026-08-16T12:18:42.826383Z","title":"Spectral Dependence of CMB Polarization and Parity","venue":"hep-ph","work_id":"02107d04-154e-4f7c-ae90-aa84d986fb0c","year":2003},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.813588Z"},"links":{"cited_paper":"/paper/hep-ph/0310368","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:c285ea530af1f5da27594248cd1488ecc6c2430cf0253bd068953491f23a2425","observation_id":"dbd05dd0-6f1b-4d44-bbc4-37ab1151ea0d","resolution":{"observed_at":"2026-08-16T12:18:42.893524Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0905.4720","last_updated":"2009-10-23T02:52:23Z","snapshot_observed_at":"2026-08-12T14:35:15.903596Z","submitted_at":"2009-05-28T19:38:46Z","title":"String Axiverse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.4720","snapshot_observed_at":"2026-08-16T12:18:40.856433Z","title":"Arvanitaki, S","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.856433Z"},"links":{"cited_paper":"/paper/0905.4720","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:7547b6c0b3c390889d48a374e604bef35f06dfdc24f5506a062414d8ed328237","observation_id":"27b82cb9-7dfc-4687-983c-9aa062680ca2","resolution":{"observed_at":"2026-08-16T12:18:40.856433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14452","last_updated":"2025-06-24T16:02:02Z","snapshot_observed_at":"2026-08-16T17:37:43.380978Z","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":"2026-08-16T12:18:40.859563Z","title":"Louis et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.859563Z"},"links":{"cited_paper":"/paper/2503.14452","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:d39a5d7b74df50de79be25fac6404ca3423145188f1ab23326a090d61a7406d2","observation_id":"f1b0ade7-ee91-4d13-a7dd-7f08143791fd","resolution":{"observed_at":"2026-08-16T12:18:40.859563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.11254","last_updated":"2020-11-23T07:46:44Z","snapshot_observed_at":"2026-08-16T19:04:02.324520Z","submitted_at":"2020-11-23T07:46:44Z","title":"New Extraction of the Cosmic Birefringence from the Planck 2018 Polarization Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.11254","snapshot_observed_at":"2026-08-16T12:18:40.863010Z","title":"Minami and E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.863010Z"},"links":{"cited_paper":"/paper/2011.11254","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:515c4974a7c79db5dc8170b306387d1fba333c3f6e59f23c14b7530e5819fc27","observation_id":"d4a4f105-487a-4ee2-af90-53836bb618fe","resolution":{"observed_at":"2026-08-16T12:18:40.863010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.07682","last_updated":"2022-02-05T06:00:39Z","snapshot_observed_at":"2026-08-16T17:27:18.516453Z","submitted_at":"2022-01-19T16:12:46Z","title":"Cosmic Birefringence from Planck Data Release 4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.07682","snapshot_observed_at":"2026-08-16T12:18:40.867230Z","title":"Diego-Palazuelos et al., Cosmic Birefringence from the Planck Data Release 4, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.867230Z"},"links":{"cited_paper":"/paper/2201.07682","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:0d582fdd406341a86c02826ed3cf52b41a5aac09b8423c67785a2c29f2c74b10","observation_id":"46e54284-9827-44a1-8914-7d8085c864f8","resolution":{"observed_at":"2026-08-16T12:18:40.867230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.13962","last_updated":"2022-09-12T09:12:42Z","snapshot_observed_at":"2026-08-16T16:57:11.284211Z","submitted_at":"2022-05-27T13:15:16Z","title":"Improved Constraints on Cosmic Birefringence from the WMAP and Planck Cosmic Microwave Background Polarization Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.13962","snapshot_observed_at":"2026-08-16T12:18:40.870413Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.870413Z"},"links":{"cited_paper":"/paper/2205.13962","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:eb23a82735c98acaf111f5fcd39d49a983168d82e6f352ad4e4bde5233552b83","observation_id":"7a23bdee-47c6-48cb-bef3-0a9e0ef76cf5","resolution":{"observed_at":"2026-08-16T12:18:40.870413Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.02268","last_updated":"2023-05-03T16:59:38Z","snapshot_observed_at":"2026-08-16T15:35:54.651061Z","submitted_at":"2023-05-03T16:59:38Z","title":"Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.02268","snapshot_observed_at":"2026-08-16T12:18:40.873524Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.873524Z"},"links":{"cited_paper":"/paper/2305.02268","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:0f3b61ce7a51cc8665d59123f2626aeddad32bfcf274b936e11f9d34c81cf7cc","observation_id":"6ed56c27-cb5d-4e20-95b8-ee9752666772","resolution":{"observed_at":"2026-08-16T12:18:40.873524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.07873","last_updated":"2019-08-11T19:10:13Z","snapshot_observed_at":"2026-08-14T17:56:37.455656Z","submitted_at":"2018-11-19T18:49:59Z","title":"Axion-like Dark Matter Constraints from CMB Birefringence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.07873","snapshot_observed_at":"2026-08-16T12:18:40.876981Z","title":"Sigl and P","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.876981Z"},"links":{"cited_paper":"/paper/1811.07873","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:ecc7a721207ec83bcf3dae55e0ec3cacee09870b52410e3e28004dec647b94d1","observation_id":"7bf7a436-61c3-4abb-8e95-df0017276323","resolution":{"observed_at":"2026-08-16T12:18:40.876981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.09287","last_updated":"2021-08-20T17:22:15Z","snapshot_observed_at":"2026-08-16T18:01:59.229799Z","submitted_at":"2021-08-20T17:22:15Z","title":"Cosmic birefringence tomography and calibration-independence with reionization signals in the CMB","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.09287","snapshot_observed_at":"2026-08-16T12:18:40.880131Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.880131Z"},"links":{"cited_paper":"/paper/2108.09287","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:60075847b137c4375796e8f9d09155ba7b7c54b707a59f45da0b09e3f57785cd","observation_id":"d9f391ec-5289-4cab-95a8-96a1975a454f","resolution":{"observed_at":"2026-08-16T12:18:40.880131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08560","last_updated":"2022-03-16T11:47:54Z","snapshot_observed_at":"2026-08-16T17:14:07.641350Z","submitted_at":"2022-03-16T11:47:54Z","title":"Is cosmic birefringence due to dark energy or dark matter? A tomographic approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08560","snapshot_observed_at":"2026-08-16T12:18:40.883543Z","title":"Nakatsuka, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.883543Z"},"links":{"cited_paper":"/paper/2203.08560","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:df3dbca294e324e3f022d00406f5a2d2d5247655e8aef28992c18ad524d78ee1","observation_id":"6c24c63b-ccdc-4d81-b217-27fdaa8d2541","resolution":{"observed_at":"2026-08-16T12:18:40.883543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0606248","last_updated":"2006-10-11T06:18:17Z","snapshot_observed_at":"2026-07-07T01:00:58.839946Z","submitted_at":"2006-06-11T10:27:36Z","title":"Effect on cosmic microwave background polarization of coupling of quintessence to pseudoscalar formed from the electromagnetic field and its dual","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0606248","snapshot_observed_at":"2026-08-16T12:18:40.907606Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.907606Z"},"links":{"cited_paper":"/paper/astro-ph/0606248","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:4c0ce7daeaa6dd5c1960e6ced2336e64c2e7cdfd30771c61fe87bbbfb40098b4","observation_id":"1b0029d3-625d-4bb5-a31e-aab5ec918979","resolution":{"observed_at":"2026-08-16T12:18:40.907606Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.6298","last_updated":"2014-03-17T03:08:35Z","snapshot_observed_at":"2026-08-15T00:09:17.841605Z","submitted_at":"2013-07-24T05:47:25Z","title":"Imprint of Scalar Dark Energy on Cosmic Microwave Background Polarization","version":2},"cited_work":{"arxiv_id":"1307.6298","doi":null,"metadata_source":"pith","pith_arxiv_id":"1307.6298","snapshot_observed_at":"2026-08-16T12:18:42.634570Z","title":"Imprint of Scalar Dark Energy on Cosmic Microwave Background Polarization","venue":"astro-ph.CO","work_id":"a6180308-305d-4979-a530-e8529c2719b3","year":2013},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:40.974531Z"},"links":{"cited_paper":"/paper/1307.6298","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:2640c27919002666f3f1c507f588a044a544da1316559c097e201543c673d6c8","observation_id":"8b4ad17e-b131-44b2-b871-2fe28d3f1f1f","resolution":{"observed_at":"2026-08-16T12:18:42.714016Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.1799","last_updated":"2015-09-29T10:37:10Z","snapshot_observed_at":"2026-08-15T06:15:39.730172Z","submitted_at":"2014-10-07T16:38:15Z","title":"Including birefringence into time evolution of CMB: current and future constraints","version":3},"cited_work":{"arxiv_id":"1410.1799","doi":null,"metadata_source":"pith","pith_arxiv_id":"1410.1799","snapshot_observed_at":"2026-08-16T12:18:42.621772Z","title":"Including birefringence into time evolution of CMB: current and future constraints","venue":"astro-ph.CO","work_id":"97bd7107-abf0-44ae-b0f3-409f6c229860","year":2014},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.001670Z"},"links":{"cited_paper":"/paper/1410.1799","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:c5eb83f9527c6b3b90c9177d3ed35b2dca424da42fe743846462d1b90fa5cf54","observation_id":"fa11d9f3-ae13-4ab1-b1aa-b332e41e5841","resolution":{"observed_at":"2026-08-16T12:18:42.625348Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0811.0618","last_updated":"2009-04-02T01:25:03Z","snapshot_observed_at":"2026-08-15T10:02:45.345333Z","submitted_at":"2008-11-04T21:11:58Z","title":"Parity violation constraints using 2006-2007 QUaD CMB polarization spectra","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.0618","snapshot_observed_at":"2026-08-16T12:18:41.004670Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.004670Z"},"links":{"cited_paper":"/paper/0811.0618","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:e5af73b835b12ba755f818d7e2a0f8cc64ed123716353f60ba2feaddccb30289","observation_id":"b41041ab-0d9f-4db9-be78-2c661c7c4594","resolution":{"observed_at":"2026-08-16T12:18:41.004670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-08-15T05:28:12.623579Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-16T12:18:41.007866Z","title":"Komatsu, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.007866Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:ce283452beaa23cef88b569b8c33b0d87962639b67e4fddd7a5cbc7afd313d61","observation_id":"61daf035-78ce-4c3f-b762-0c0b81eb0855","resolution":{"observed_at":"2026-08-16T12:18:41.007866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.7877","last_updated":"2013-12-30T20:59:20Z","snapshot_observed_at":"2026-08-14T23:49:58.788733Z","submitted_at":"2013-12-30T20:59:20Z","title":"Self-Calibration of BICEP1 Three-Year Data and Constraints on Astrophysical Polarization Rotation","version":1},"cited_work":{"arxiv_id":"1312.7877","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.7877","snapshot_observed_at":"2026-08-16T12:18:42.511531Z","title":"Self-Calibration of BICEP1 Three-Year Data and Constraints on Astrophysical Polarization Rotation","venue":"astro-ph.IM","work_id":"27e36e17-f0b4-4307-a193-dbf8ced1248f","year":2013},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.011304Z"},"links":{"cited_paper":"/paper/1312.7877","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:2f690ba049d57167585a1286babb9adfa8c55d9d14da84bc092331aefddf285c","observation_id":"06ef3758-79f0-4490-9db1-3073400964fd","resolution":{"observed_at":"2026-08-16T12:18:42.546877Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.08633","last_updated":"2016-08-05T16:46:54Z","snapshot_observed_at":"2026-08-16T13:26:21.057688Z","submitted_at":"2016-05-27T13:35:07Z","title":"Planck intermediate results. XLIX. Parity-violation constraints from polarization data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.08633","snapshot_observed_at":"2026-08-16T12:18:41.014742Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.014742Z"},"links":{"cited_paper":"/paper/1605.08633","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:40f07c9e268de5cefbe1ea9c3f5c0260ebac2689709e5194a159c722e5ae1890","observation_id":"6f478207-0724-4a26-a175-9b271841e48a","resolution":{"observed_at":"2026-08-16T12:18:41.014742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.05685","last_updated":"2023-03-21T15:35:08Z","snapshot_observed_at":"2026-08-17T12:56:36.244636Z","submitted_at":"2022-11-10T16:43:44Z","title":"Impact of half-wave plate systematics on the measurement of cosmic birefringence from CMB polarization","version":2},"cited_work":{"arxiv_id":"2211.05685","doi":null,"metadata_source":"pith","pith_arxiv_id":"2211.05685","snapshot_observed_at":"2026-08-16T12:18:42.401946Z","title":"Impact of half-wave plate systematics on the measurement of cosmic birefringence from CMB polarization","venue":"astro-ph.CO","work_id":"b0c538fd-cefc-4950-b61d-7103dc8a143c","year":2022},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.018754Z"},"links":{"cited_paper":"/paper/2211.05685","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:3f23c54b5294287d96bd204447e33854a3bc1e47b07d31fd0296dcc0a4b4e874","observation_id":"6e974978-93b7-4607-a2c3-165485763720","resolution":{"observed_at":"2026-08-16T12:18:42.405967Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9812088","last_updated":"1999-07-23T15:36:59Z","snapshot_observed_at":"2026-07-07T01:23:24.602283Z","submitted_at":"1998-12-04T01:05:38Z","title":"Cosmological Signature of New Parity-Violating Interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9812088","snapshot_observed_at":"2026-08-16T12:18:41.021959Z","title":"Lue, L.-M","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.021959Z"},"links":{"cited_paper":"/paper/astro-ph/9812088","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:11a7b661af0c4e2ffe0922ecf4db0f26ff62cd0e9ef14ecb080c3b8f7a73784b","observation_id":"68e0111a-0377-4128-bc24-47b456d60b29","resolution":{"observed_at":"2026-08-16T12:18:41.021959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.5585","last_updated":"2015-05-20T02:34:07Z","snapshot_observed_at":"2026-08-14T23:40:23.191380Z","submitted_at":"2014-03-21T22:49:33Z","title":"Cosmic Birefringence Fluctuations and Cosmic Microwave Background $B$-mode Polarization","version":4},"cited_work":{"arxiv_id":"1403.5585","doi":null,"metadata_source":"pith","pith_arxiv_id":"1403.5585","snapshot_observed_at":"2026-08-16T12:18:42.367381Z","title":"Cosmic Birefringence Fluctuations and Cosmic Microwave Background $B$-mode Polarization","venue":"astro-ph.CO","work_id":"c2b64b4e-e1c0-420d-b489-88cf574a8f9a","year":2014},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.151695Z"},"links":{"cited_paper":"/paper/1403.5585","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:7ec1a7765d79af4dc51fceb04a5eb0df01d72903d78e395ef2e234ca64727a15","observation_id":"c013af48-86ab-42dd-a16d-1ef92a09b237","resolution":{"observed_at":"2026-08-16T12:18:42.371707Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00418","last_updated":"2016-11-01T23:00:12Z","snapshot_observed_at":"2026-08-16T16:27:49.809186Z","submitted_at":"2016-11-01T23:00:12Z","title":"The Cosmic Microwave Background And Pseudo-Nambu-Goldstone Bosons: Searching For Lorentz Violations In The Cosmos","version":1},"cited_work":{"arxiv_id":"1611.00418","doi":null,"metadata_source":"pith","pith_arxiv_id":"1611.00418","snapshot_observed_at":"2026-08-16T12:18:42.274627Z","title":"The Cosmic Microwave Background And Pseudo-Nambu-Goldstone Bosons: Searching For Lorentz Violations In The Cosmos","venue":"astro-ph.CO","work_id":"c764e9e6-8720-4968-b19e-6de19c5f9301","year":2016},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.155436Z"},"links":{"cited_paper":"/paper/1611.00418","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:c308482610c44defc3245eef57727ea8dbcd53eb1962f238896d3c4e45ce6cac","observation_id":"8de57696-a0b9-4551-b966-c414cd8dd9f8","resolution":{"observed_at":"2026-08-16T12:18:42.306591Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.07937","last_updated":"2023-05-13T15:01:52Z","snapshot_observed_at":"2026-08-16T15:33:22.393965Z","submitted_at":"2023-05-13T15:01:52Z","title":"Is Cosmic Birefringence model-dependent?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.07937","snapshot_observed_at":"2026-08-16T12:18:41.160397Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.160397Z"},"links":{"cited_paper":"/paper/2305.07937","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:6565884a35fcfa18cb834ed7217b6a0130b903360abb89454aac6f8846879ad7","observation_id":"64568f22-2530-4d3f-bd83-0ad64dca2f02","resolution":{"observed_at":"2026-08-16T12:18:41.160397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.14104","last_updated":"2025-07-10T16:29:54Z","snapshot_observed_at":"2026-08-16T14:32:29.031050Z","submitted_at":"2023-12-21T18:28:42Z","title":"Axionic defects in the CMB: birefringence and gravitational waves","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.14104","snapshot_observed_at":"2026-08-16T12:18:41.163359Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.163359Z"},"links":{"cited_paper":"/paper/2312.14104","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:14895c4a3d0760c0d713ae2bec208c4582d014ddc1f1891a2dfa9fe06b979409","observation_id":"18d43c9d-236d-45a9-86bd-fb52e077615b","resolution":{"observed_at":"2026-08-16T12:18:41.163359Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0905.1687","last_updated":"2009-07-07T06:00:20Z","snapshot_observed_at":"2026-08-15T05:48:35.408064Z","submitted_at":"2009-05-12T19:28:23Z","title":"De-Rotation of the Cosmic Microwave Background Polarization: Full-Sky Formalism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.1687","snapshot_observed_at":"2026-08-16T12:18:41.167777Z","title":"Gluscevic, M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.167777Z"},"links":{"cited_paper":"/paper/0905.1687","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:1917268db2b0d60e8bb95c2a7dfa3a57752c8eb398b1ebcec76fc042b18658a1","observation_id":"daae1389-2348-43dd-9503-3258cd81aeeb","resolution":{"observed_at":"2026-08-16T12:18:41.167777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.02523","last_updated":"2019-06-20T15:48:19Z","snapshot_observed_at":"2026-08-14T21:02:24.449530Z","submitted_at":"2017-05-06T19:50:58Z","title":"BICEP2 / Keck Array IX: New Bounds on Anisotropies of CMB Polarization Rotation and Implications for Axion-Like Particles and Primordial Magnetic Fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.02523","snapshot_observed_at":"2026-08-16T12:18:41.170991Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.170991Z"},"links":{"cited_paper":"/paper/1705.02523","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:ed80374571a5ccc1679dbb382febb342a3919225245111d6593666c35feccc2a","observation_id":"e965d1e8-812f-428b-8420-c771369a1c47","resolution":{"observed_at":"2026-08-16T12:18:41.170991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.10465","last_updated":"2020-04-21T16:07:43Z","snapshot_observed_at":"2026-08-16T16:27:12.617193Z","submitted_at":"2020-01-28T16:59:49Z","title":"The Atacama Cosmology Telescope: Constraints on Cosmic Birefringence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.10465","snapshot_observed_at":"2026-08-16T12:18:41.174148Z","title":"Namikawa et al., Atacama Cosmology Telescope: Con- straints on cosmic birefringence, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.174148Z"},"links":{"cited_paper":"/paper/2001.10465","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:042d3b8a144cc320cec07c3c44c0e85ca6e595365514e476274085b33701015b","observation_id":"314ed053-539c-43ac-a8ea-6646e087fd0b","resolution":{"observed_at":"2026-08-16T12:18:41.174148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.04047","last_updated":"2020-12-07T20:43:38Z","snapshot_observed_at":"2026-08-16T19:00:18.966720Z","submitted_at":"2020-12-07T20:43:38Z","title":"Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.04047","snapshot_observed_at":"2026-08-16T12:18:41.177312Z","title":"Moncelsi et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.177312Z"},"links":{"cited_paper":"/paper/2012.04047","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:1132e3cc8ed3669b0320e92d89a62bd3e133d927f01d3fdaacb5c63c5bae4868","observation_id":"01e76845-f3d2-4c9e-bb9f-4f201588c3b0","resolution":{"observed_at":"2026-08-16T12:18:41.177312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.07445","last_updated":"2019-03-01T10:51:03Z","snapshot_observed_at":"2026-08-15T01:11:26.803228Z","submitted_at":"2018-08-22T17:19:17Z","title":"The Simons Observatory: Science goals and forecasts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.07445","snapshot_observed_at":"2026-08-16T12:18:41.221058Z","title":"Ade et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.221058Z"},"links":{"cited_paper":"/paper/1808.07445","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:88b6b3a63e69b14c0dc4ab4dec9b1ab02496108ea4742441774cc9330644be1e","observation_id":"904ee799-9233-4115-afeb-9ad78abd5ad4","resolution":{"observed_at":"2026-08-16T12:18:41.221058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.12619","last_updated":"2020-08-27T07:54:51Z","snapshot_observed_at":"2026-08-15T00:44:47.188521Z","submitted_at":"2020-08-27T07:54:51Z","title":"CMB-S4: Forecasting Constraints on Primordial Gravitational Waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.12619","snapshot_observed_at":"2026-08-16T12:18:41.317040Z","title":"Abazajian et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.317040Z"},"links":{"cited_paper":"/paper/2008.12619","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:b9f3963751ef79d821db6ddcb67a0414d41f16928fc935ace6258b58451b1c9f","observation_id":"47818e57-9469-44d9-b6d8-8e261ad62791","resolution":{"observed_at":"2026-08-16T12:18:41.317040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.02773","last_updated":"2023-03-27T05:15:34Z","snapshot_observed_at":"2026-08-16T17:23:19.621197Z","submitted_at":"2022-02-06T13:17:44Z","title":"Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.02773","snapshot_observed_at":"2026-08-16T12:18:41.354066Z","title":"Allys et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.354066Z"},"links":{"cited_paper":"/paper/2202.02773","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:a17ce2f68bea3935c5bbd854e5050eda4ffa3fe455865ca7753036f337d1f709","observation_id":"17ee181e-c675-4198-8b9c-67c2e44b6303","resolution":{"observed_at":"2026-08-16T12:18:41.354066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04708","last_updated":"2025-05-26T15:38:46Z","snapshot_observed_at":"2026-08-16T16:27:45.630579Z","submitted_at":"2025-03-06T18:55:46Z","title":"Improving Cosmic Birefringence Constraints via Delensing","version":2},"cited_work":{"arxiv_id":"2503.04708","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.04708","snapshot_observed_at":"2026-08-16T12:18:42.046788Z","title":"Improving Cosmic Birefringence Constraints via Delensing","venue":"astro-ph.CO","work_id":"f2de3242-b4a9-4957-9821-33f13d914b2e","year":2025},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.358186Z"},"links":{"cited_paper":"/paper/2503.04708","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:33f579f25fa884510f76a7299b4ad5a1264bbc7016593cbdb2cd9ab835665fab","observation_id":"8c650e2a-0b2f-4dda-a057-23b788966ce6","resolution":{"observed_at":"2026-08-16T12:18:42.110934Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.13771","last_updated":"2025-03-03T15:12:06Z","snapshot_observed_at":"2026-08-16T16:27:32.513239Z","submitted_at":"2024-04-21T20:47:28Z","title":"Exact CMB B-mode power spectrum from anisotropic cosmic birefringence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.13771","snapshot_observed_at":"2026-08-16T12:18:41.361771Z","title":"Namikawa, Exact CMB B-mode power spectrum from anisotropic cosmic birefringence, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.361771Z"},"links":{"cited_paper":"/paper/2404.13771","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:b775301c253e986941508e81e4bc47b88d6c338a145a9f7ca33b7f47ce2ae0da","observation_id":"deecba7f-f099-4ceb-88b8-5d4f14183209","resolution":{"observed_at":"2026-08-16T12:18:41.361771Z","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":"2026-08-16T12:18:43.406129Z","title":"Harari and P","venue":null,"work_id":"dca45089-7721-4e23-8969-dc4551128449","year":1992},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.365478Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:f3d7d89efaf1cd7f1a04050ddc331113b9ad91158902beec598912e3e45c86c9","observation_id":"b629730d-dd57-4d2a-9127-0f4812ec8603","resolution":{"observed_at":"2026-08-16T12:18:43.409466Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:18:43.364245Z","title":null,"venue":null,"work_id":"dc1651d6-8f79-4d6c-8d3a-dee9d18ae0e9","year":1990},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.369221Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:615131cd2b8e500a8671e319346d8d7c3964d4fd8f4d8d12230fccd78489a93c","observation_id":"8e189969-f863-454f-9097-01ff5e44ff9f","resolution":{"observed_at":"2026-08-16T12:18:43.400819Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:18:43.299311Z","title":null,"venue":null,"work_id":"32dfb58a-d4e8-43f1-b66d-822a6894bc72","year":1991},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.373010Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:3b8bfaa1d0c302a0fad2ad9817041285d15a0f653d9b695ed903fdf0e7d9da89","observation_id":"dee4b9a7-57bf-4da2-b0ad-5ee79416ffc7","resolution":{"observed_at":"2026-08-16T12:18:43.324717Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:18:41.376630Z","title":"Greco, N","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.376630Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:5574ae1857a7eaadcd45cc1d5a3e48fce6f1061fb352b19cabc4c34603de0c49","observation_id":"f291077e-1e8a-43c2-936c-5165c1b8f7cd","resolution":{"observed_at":"2026-08-16T12:18:41.376630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.0403","last_updated":"2008-11-12T14:10:56Z","snapshot_observed_at":"2026-08-15T10:05:19.316368Z","submitted_at":"2008-10-02T12:26:54Z","title":"Cosmological CPT violating effect on CMB polarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.0403","snapshot_observed_at":"2026-08-16T12:18:41.380268Z","title":"Li and X","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.380268Z"},"links":{"cited_paper":"/paper/0810.0403","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:ae0cf5ae0a69953ffe59c976a6f7c5956c76eac640582f8874362a29c62a7d08","observation_id":"56e393de-4410-4b89-957e-fb65e9bac68a","resolution":{"observed_at":"2026-08-16T12:18:41.380268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9702170","last_updated":"1997-07-16T19:42:11Z","snapshot_observed_at":"2026-07-07T01:16:01.826754Z","submitted_at":"1997-02-19T23:10:24Z","title":"CMB Anisotropies: Total Angular Momentum Method","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9702170","snapshot_observed_at":"2026-08-16T12:18:41.384757Z","title":"Hu and M","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.384757Z"},"links":{"cited_paper":"/paper/astro-ph/9702170","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:0dbe7551f9253448c6645867a991b8c7b28a8ac788b18c3c6803ac720258e50e","observation_id":"c6733950-0843-4338-9002-c1fb2f4d1a59","resolution":{"observed_at":"2026-08-16T12:18:41.384757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.1438","last_updated":"2011-09-28T05:12:48Z","snapshot_observed_at":"2026-08-15T04:44:29.879662Z","submitted_at":"2011-06-07T20:00:20Z","title":"Primordial Magnetism in the CMB: Exact Treatment of Faraday Rotation and WMAP7 Bounds","version":3},"cited_work":{"arxiv_id":"1106.1438","doi":null,"metadata_source":"pith","pith_arxiv_id":"1106.1438","snapshot_observed_at":"2026-08-16T12:18:41.923831Z","title":"Primordial Magnetism in the CMB: Exact Treatment of Faraday Rotation and WMAP7 Bounds","venue":"astro-ph.CO","work_id":"67b7554b-a520-42f6-8364-cbc09d9e2170","year":2011},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.510161Z"},"links":{"cited_paper":"/paper/1106.1438","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:645428d51b2e2ec29970a4defff6e36aef968402264a5bfc18f647e103fde541","observation_id":"e127407c-2194-4385-889e-2c20e590493f","resolution":{"observed_at":"2026-08-16T12:18:41.958339Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.1634","last_updated":"2011-04-08T20:00:02Z","snapshot_observed_at":"2026-08-15T04:49:50.551649Z","submitted_at":"2011-04-08T20:00:02Z","title":"Cross-Correlation of Cosmological Birefringence with CMB Temperature","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.1634","snapshot_observed_at":"2026-08-16T12:18:41.513862Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.513862Z"},"links":{"cited_paper":"/paper/1104.1634","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:6d1c43f315b806e2ed96e00cab5ea3a21239b42ff624e11877a5d441bdda6d31","observation_id":"a01cb4b9-ccbc-4b6e-87fb-7a29da15434f","resolution":{"observed_at":"2026-08-16T12:18:41.513862Z","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":"2026-08-16T12:18:41.518772Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.518772Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:dc9148091fb41fc9370832b377536204cb6c08f365f497e92197b07134755323","observation_id":"0ba9e6a9-00a6-4280-beca-cf4f7e28f397","resolution":{"observed_at":"2026-08-16T12:18:41.518772Z","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":"2026-08-16T12:18:43.284289Z","title":null,"venue":null,"work_id":"bfa42005-f4d6-4015-a180-a4b841df2feb","year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.522559Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:ca0a9e27cd755d9680a4bf8006d9e9462ec0b2d67c740785d3a8af2846483f78","observation_id":"19e1c256-189a-4fb3-81bf-7e1c6cc01a7b","resolution":{"observed_at":"2026-08-16T12:18:43.287557Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:18:41.525401Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.525401Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:de6188bb32d66602d1317a8bee0be6cf2cdc21a5361bc0940c893a6ab92bcfbf","observation_id":"19acc269-86c2-4a63-b5ae-600b3a4ab59c","resolution":{"observed_at":"2026-08-16T12:18:41.525401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.02495","last_updated":"2022-06-15T21:21:44Z","snapshot_observed_at":"2026-08-16T17:16:52.746423Z","submitted_at":"2022-03-04T18:50:54Z","title":"Improved upper limit on degree-scale CMB B-mode polarization power from the 670 square-degree POLARBEAR survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.02495","snapshot_observed_at":"2026-08-16T12:18:41.529042Z","title":"Adachi et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.529042Z"},"links":{"cited_paper":"/paper/2203.02495","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:ad970a6fcaedd1b54d2060b0d4a6d67c8a6a8a049284be6c9a361dcff47b7785","observation_id":"4961c6f3-2ad5-4f46-8e27-640eeed47f05","resolution":{"observed_at":"2026-08-16T12:18:41.529042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.05748","last_updated":"2020-04-22T05:03:17Z","snapshot_observed_at":"2026-08-16T16:27:13.126391Z","submitted_at":"2019-10-13T13:26:52Z","title":"Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.05748","snapshot_observed_at":"2026-08-16T12:18:41.532024Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.532024Z"},"links":{"cited_paper":"/paper/1910.05748","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:e4516f923b97e8a4a6e5caf04670bb7da49f2b585cabcc459c75ff10f999ba13","observation_id":"04bbb25e-af78-45a5-b566-e82949746a04","resolution":{"observed_at":"2026-08-16T12:18:41.532024Z","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":"2026-08-16T12:18:43.275487Z","title":null,"venue":null,"work_id":"3ed4d9e3-02fa-4312-8a09-9af262c901c8","year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.536642Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:900040d281d8b798e8990620cfb51837869d547278511eea7f9ad14a68d6e87d","observation_id":"6eed6f66-4d7f-47da-92c1-aee3879bba5a","resolution":{"observed_at":"2026-08-16T12:18:43.278737Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:18:43.265760Z","title":null,"venue":null,"work_id":"dbb7e05c-2005-44f0-a5f2-b51a1a94e9e8","year":null},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.539643Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:f2371350dd699585f25659361381f93c351d4c50d8642ea2b08a41c7c195babd","observation_id":"1c972321-84a7-418f-ba38-bff9c35be341","resolution":{"observed_at":"2026-08-16T12:18:43.269674Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3665","last_updated":"2013-11-25T15:56:48Z","snapshot_observed_at":"2026-07-06T02:43:00.981478Z","submitted_at":"2012-02-16T20:41:19Z","title":"emcee: The MCMC Hammer","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3665","snapshot_observed_at":"2026-08-16T12:18:41.542494Z","title":"Foreman-Mackey, D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.542494Z"},"links":{"cited_paper":"/paper/1202.3665","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:7f33dc563e622cbdec3eb8d4e21c19a40d0bde2d240477acc18702c4b574af4f","observation_id":"49ba327d-b712-49b7-b090-f86a41af8d80","resolution":{"observed_at":"2026-08-16T12:18:41.542494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409767","last_updated":"2005-03-24T00:24:41Z","snapshot_observed_at":"2026-08-16T16:26:07.181721Z","submitted_at":"2004-09-30T18:21:03Z","title":"Faraday Rotation of the Cosmic Microwave Background Polarization by a Stochastic Magnetic Field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409767","snapshot_observed_at":"2026-08-16T12:18:41.623136Z","title":"Kosowsky, T","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.623136Z"},"links":{"cited_paper":"/paper/astro-ph/0409767","citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:3da0b86e734168cb5e3294a56f14f42ac843e77736a6d1a133b64eacbc0e98a6","observation_id":"4668f370-d327-47d3-98a6-66b9f759259d","resolution":{"observed_at":"2026-08-16T12:18:41.623136Z","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":"ph/0702379","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:18:41.779508Z","title":null,"venue":null,"work_id":"2b318b5b-e5b6-40ad-a936-d4a3ff9283f9","year":2007},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.677455Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:70ac3205c1d4a90e73e85b91b2fd1c4464f93d575a235f6d778f18a705767c28","observation_id":"2f698c9a-03ec-49ca-952f-304106424660","resolution":{"observed_at":"2026-08-16T12:18:41.827419Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:18:43.220072Z","title":"Greco, N","venue":null,"work_id":"94d46b53-8ae9-495b-8327-5dd314b2ab20","year":2023},"citing_paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-16T12:18:41.680695Z"},"links":{"citing_paper":"/paper/2504.13154"},"observation_digest":"sha256:56eab7c0cdfebb7b132e9919d2a387e1597d76c7dde36b8be7606b3a52ba095a","observation_id":"49918853-86e6-4f14-8e81-0d2f878d69f9","resolution":{"observed_at":"2026-08-16T12:18:43.259659Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2504.13154","last_updated":"2025-06-26T17:37:10Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T22:33:37.387811Z","submitted_at":"2025-04-17T17:56:23Z","title":"Constraints on Anisotropic Cosmic Birefringence from CMB B-mode Polarization"},"reference_resolution":{"displayed":71,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":59,"verified_exact":10,"verified_fuzzy":2},"total_outbound_references":71},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 71 of 71 outbound references and 2 inbound Pith citation observations for arXiv:2504.13154."}