{"as_of":"2026-08-17T19:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:257a14d731532166475d9d082c227b3d611eac884e10b3f186e216ce35029494","coverage":[{"denominator":84,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":84,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T05:58:03.174611Z","state":"measured"},{"denominator":84,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":84,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"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":[],"links":{"evidence":"/evidence","html":"/paper/1909.00568/citation-record","integrity":"/paper/1909.00568/integrity","json":"/paper/1909.00568/citation-record.json","paper":"/paper/1909.00568"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"0907.4303","last_updated":"2009-09-30T08:39:21Z","snapshot_observed_at":"2026-08-15T05:42:56.247283Z","submitted_at":"2009-07-24T14:38:01Z","title":"Detecting relics of a thermal gravitational wave background in the early Universe","version":3},"cited_work":{"arxiv_id":"0907.4303","doi":null,"metadata_source":"pith","pith_arxiv_id":"0907.4303","snapshot_observed_at":"2026-08-14T05:58:04.523255Z","title":"Detecting relics of a thermal gravitational wave background in the early Universe","venue":"gr-qc","work_id":"61f17ce2-7b51-40d2-a713-25fa1013c9a6","year":2009},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.764557Z"},"links":{"cited_paper":"/paper/0907.4303","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:58426639797fefa4ccd9b1115c96132a5611b24d6cd8bfbcf2cde489ab92d9b1","observation_id":"ca0389d3-1c55-4782-b069-70b7f636520f","resolution":{"observed_at":"2026-08-14T05:58:04.528481Z","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/0607049","last_updated":"2006-11-17T07:05:05Z","snapshot_observed_at":"2026-08-15T11:09:54.834955Z","submitted_at":"2006-07-04T12:17:05Z","title":"Enhanced polarization of CMB from thermal gravitational waves","version":3},"cited_work":{"arxiv_id":"astro-ph/0607049","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0607049","snapshot_observed_at":"2026-08-14T05:58:04.499863Z","title":"Enhanced polarization of CMB from thermal gravitational waves","venue":"astro-ph","work_id":"eba682da-7a6f-4bf3-ab0f-c62bac2dc0e5","year":2006},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.769939Z"},"links":{"cited_paper":"/paper/astro-ph/0607049","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:81d514ca8f32fb4a6840a0c282a6756bc280cefc5685a6f06dccbb42688eee49","observation_id":"a7527eed-7b06-4713-a27a-fe5604da80df","resolution":{"observed_at":"2026-08-14T05:58:04.505434Z","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/9609169","last_updated":"1997-03-02T17:58:44Z","snapshot_observed_at":"2026-07-07T01:14:30.808201Z","submitted_at":"1996-09-25T03:20:46Z","title":"Signature of Gravity Waves in Polarization of the Microwave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9609169","snapshot_observed_at":"2026-08-14T05:58:02.776273Z","title":"Seljak and M","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.776273Z"},"links":{"cited_paper":"/paper/astro-ph/9609169","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:1ceb4e85f9ce9b05c9a62e52482f3196af581166ceb41c89863501db2ee5612e","observation_id":"05d981ce-225b-455c-ab09-b21aee594555","resolution":{"observed_at":"2026-08-14T05:58:02.776273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.02199","last_updated":"2018-10-27T22:07:53Z","snapshot_observed_at":"2026-08-14T18:55:10.546399Z","submitted_at":"2018-07-05T23:27:35Z","title":"Measurements of Degree-Scale B-mode Polarization with the BICEP/Keck Experiments at South Pole","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.02199","snapshot_observed_at":"2026-08-14T05:58:02.781640Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.781640Z"},"links":{"cited_paper":"/paper/1807.02199","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:69b426e63a9c78d565762400621657be1b1fb83192f098de183e196d5210cdf7","observation_id":"3ef2064b-3a55-42cc-bb63-408fac3a5625","resolution":{"observed_at":"2026-08-14T05:58:02.781640Z","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":"2026-08-14T05:58:02.757958Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.757958Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:f943d6e4ddac9b765dfef78deb89a3546d6bbcfb561df3f26f211ba8c14d4847","observation_id":"d45be0ed-c90d-451f-b9ca-acdd2148bde3","resolution":{"observed_at":"2026-08-14T05:58:02.757958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.2369","last_updated":"2018-07-16T16:22:03Z","snapshot_observed_at":"2026-08-14T23:41:49.678081Z","submitted_at":"2014-03-10T19:56:20Z","title":"A Measurement of the Cosmic Microwave Background B-Mode Polarization Power Spectrum at Sub-Degree Scales with POLARBEAR","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.2369","snapshot_observed_at":"2026-08-14T05:58:02.787065Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.787065Z"},"links":{"cited_paper":"/paper/1403.2369","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:65a63b58b518f5509fff5e6cd70314f8dc19b70b6ffebb0d97eb582ebda5fff4","observation_id":"b346dd52-1c0b-4bd8-a41d-8baa57befa5a","resolution":{"observed_at":"2026-08-14T05:58:02.787065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.3985","last_updated":"2014-06-23T17:39:37Z","snapshot_observed_at":"2026-08-14T23:41:06.433473Z","submitted_at":"2014-03-17T02:14:52Z","title":"BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.3985","snapshot_observed_at":"2026-08-14T05:58:02.792599Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.792599Z"},"links":{"cited_paper":"/paper/1403.3985","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:c64556cfe4dcce9026efb6e213f7df8ebfb58a5b462feac7dcf0121089de00b4","observation_id":"7d627841-1413-405c-a69e-26270cd33225","resolution":{"observed_at":"2026-08-14T05:58:02.792599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.09217","last_updated":"2016-03-14T19:59:46Z","snapshot_observed_at":"2026-08-14T22:25:32.234789Z","submitted_at":"2015-10-30T19:42:57Z","title":"BICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.09217","snapshot_observed_at":"2026-08-14T05:58:02.798145Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.798145Z"},"links":{"cited_paper":"/paper/1510.09217","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:cfd3fea057807876ab49490c54e5cc38d2ce4dfd78e11edb5d9ba63b7912687d","observation_id":"f530fb17-d3db-4283-9da1-e2850bb63c04","resolution":{"observed_at":"2026-08-14T05:58:02.798145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02315","last_updated":"2015-03-08T19:55:38Z","snapshot_observed_at":"2026-08-16T16:23:41.884669Z","submitted_at":"2015-03-08T19:55:38Z","title":"Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.02315","snapshot_observed_at":"2026-08-14T05:58:02.803225Z","title":"Keisler et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.803225Z"},"links":{"cited_paper":"/paper/1503.02315","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:8a3fc80aafe669c25cea2cf49bbee5341c13a4827c318423154fe2df1357e5f9","observation_id":"1c52d37a-9186-4642-8494-41d0624e9cbf","resolution":{"observed_at":"2026-08-14T05:58:02.803225Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.04594","last_updated":"2018-02-13T12:47:47Z","snapshot_observed_at":"2026-08-16T16:23:23.206078Z","submitted_at":"2018-02-13T12:47:47Z","title":"The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization","version":1},"cited_work":{"arxiv_id":"1802.04594","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.04594","snapshot_observed_at":"2026-08-14T05:58:04.373098Z","title":"The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization","venue":"astro-ph.CO","work_id":"174d3830-6940-4c3b-9bda-6ae877c230ec","year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.808285Z"},"links":{"cited_paper":"/paper/1802.04594","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:75e5950f18f2d31f8fadf88173b4821f498fb56ff3741e7d149567e5b8d7e30b","observation_id":"7577aa15-b16e-4d52-a989-9fbabca19c74","resolution":{"observed_at":"2026-08-14T05:58:04.378335Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:58:02.813373Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.813373Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:beadd1bf02719d6eb5b346d786f96b04df50f3286f5eb4d0ce0b256ba50b5342","observation_id":"1bc9be44-7857-4be4-ad20-6fd12ec73808","resolution":{"observed_at":"2026-08-14T05:58:02.813373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.10596","last_updated":"2017-11-28T22:42:35Z","snapshot_observed_at":"2026-08-16T16:22:19.060938Z","submitted_at":"2017-11-28T22:42:35Z","title":"SPIDER: CMB polarimetry from the edge of space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.10596","snapshot_observed_at":"2026-08-14T05:58:02.818046Z","title":"Gualtieri et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.818046Z"},"links":{"cited_paper":"/paper/1711.10596","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:ea2a88ebd4e0a37a829ab66365c6d28e8c6c480bc393d3568c8b395edc49ba88","observation_id":"9e99bd31-ef9f-4157-9f05-5c3630f8253c","resolution":{"observed_at":"2026-08-14T05:58:02.818046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06042","last_updated":"2015-10-20T20:12:45Z","snapshot_observed_at":"2026-08-14T22:27:00.800382Z","submitted_at":"2015-10-20T20:12:45Z","title":"The Quest for B Modes from Inflationary Gravitational Waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06042","snapshot_observed_at":"2026-08-14T05:58:02.823181Z","title":"Kamionkowski and E","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.823181Z"},"links":{"cited_paper":"/paper/1510.06042","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:3fe9325ddbac4b988d7cdbdb1df610205cc186da809572d663b33b7cc62e8d03","observation_id":"b23dac44-55ef-4024-b3f4-5f31a367359e","resolution":{"observed_at":"2026-08-14T05:58:02.823181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-16T01:24:03.079645Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06100","snapshot_observed_at":"2026-08-14T05:58:02.828055Z","title":"Jeong and M","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.828055Z"},"links":{"cited_paper":"/paper/1908.06100","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:01bccf73bc86d4e1ae6dd8a236a5b92073fb7fd9569ac96b85cfd4a549da55d6","observation_id":"3e7a397e-2284-4b57-b574-e5138fba0b59","resolution":{"observed_at":"2026-08-14T05:58:02.828055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.02486","last_updated":"2021-08-14T17:26:43Z","snapshot_observed_at":"2026-08-16T16:22:21.069418Z","submitted_at":"2019-07-04T16:47:35Z","title":"An Examination of Galactic Polarization with Application to the Planck TB Correlation","version":2},"cited_work":{"arxiv_id":"1907.02486","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.02486","snapshot_observed_at":"2026-08-14T05:58:04.303385Z","title":"An Examination of Galactic Polarization with Application to the Planck TB Correlation","venue":"astro-ph.CO","work_id":"e7520851-007c-4897-9c5b-d0ce29917b7b","year":2019},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.833140Z"},"links":{"cited_paper":"/paper/1907.02486","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:6bafbcbd3da45d1731398023c5be61f1af394d1336a93bcef1024ccb93b2305f","observation_id":"a7a48d8d-7632-4cbe-bbf0-cd25df0d2deb","resolution":{"observed_at":"2026-08-14T05:58:04.308933Z","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":"1702.08852","last_updated":"2017-02-28T16:36:25Z","snapshot_observed_at":"2026-08-16T16:22:55.804548Z","submitted_at":"2017-02-28T16:36:25Z","title":"Wiener filter reloaded: fast signal reconstruction without preconditioning","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.08852","snapshot_observed_at":"2026-08-14T05:58:02.838188Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.838188Z"},"links":{"cited_paper":"/paper/1702.08852","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:7a5506546c95c4246eeb4b8b45bf3a3b0afa490519e2d75044f12d000a93f55b","observation_id":"95c2601d-8102-4cfd-9563-84ef348457eb","resolution":{"observed_at":"2026-08-14T05:58:02.838188Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.05358","last_updated":"2018-02-08T15:54:41Z","snapshot_observed_at":"2026-08-16T16:24:02.413350Z","submitted_at":"2018-01-16T16:57:43Z","title":"Optimal and fast E/B separation with a dual messenger field","version":2},"cited_work":{"arxiv_id":"1801.05358","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.05358","snapshot_observed_at":"2026-08-14T05:58:04.264968Z","title":"Optimal and fast E/B separation with a dual messenger field","venue":"astro-ph.CO","work_id":"fd163443-2122-4470-ad3a-49a0ad9a9f9e","year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.843329Z"},"links":{"cited_paper":"/paper/1801.05358","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:f2c3dff43aa45c9725f4590bdbaf1b3c15d5a6d925fa0d743148f3096ff74e42","observation_id":"82533b90-cb21-4305-a8cd-78b88e0c6ca0","resolution":{"observed_at":"2026-08-14T05:58:04.270206Z","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":"1906.10704","last_updated":"2019-09-30T12:57:33Z","snapshot_observed_at":"2026-08-16T16:22:16.631159Z","submitted_at":"2019-06-25T18:00:09Z","title":"Wiener filtering and pure E/B decomposition of CMB maps with anisotropic correlated noise","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.10704","snapshot_observed_at":"2026-08-14T05:58:02.848397Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.848397Z"},"links":{"cited_paper":"/paper/1906.10704","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:564f9f5f44d80c55ffc29c21736a84609b4cfd8d12d3cd993d0727c354fe0391","observation_id":"25d96e2f-427c-4ee1-814e-ee33e08d2a24","resolution":{"observed_at":"2026-08-14T05:58:02.848397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9609170","last_updated":"1997-03-02T17:59:12Z","snapshot_observed_at":"2026-08-15T12:15:32.498742Z","submitted_at":"1996-09-25T15:36:04Z","title":"An All-Sky Analysis of Polarization in the Microwave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9609170","snapshot_observed_at":"2026-08-14T05:58:02.853414Z","title":"Zaldarriaga and U","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.853414Z"},"links":{"cited_paper":"/paper/astro-ph/9609170","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:96dc92837d3b6f378a8b2632ae3f0446d99c821caa3693f7738e185eaef065c3","observation_id":"ac86edc9-a895-4399-a6e9-1bea64b02b76","resolution":{"observed_at":"2026-08-14T05:58:02.853414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9702157","last_updated":"1997-09-11T22:32:13Z","snapshot_observed_at":"2026-07-07T01:15:55.239042Z","submitted_at":"1997-02-19T00:23:59Z","title":"Microwave Background Constraints on Cosmological Parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9702157","snapshot_observed_at":"2026-08-14T05:58:02.858463Z","title":"Zaldarriaga, D","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.858463Z"},"links":{"cited_paper":"/paper/astro-ph/9702157","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:49b56449b38ac5e99310434c02d3f731eb8c595fc9b5e22aa4336927b9c4a4e0","observation_id":"cf15e2bf-755f-4bd9-a3e7-8ce5e9bc19ee","resolution":{"observed_at":"2026-08-14T05:58:02.858463Z","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":"2026-08-14T05:58:02.863437Z","title":"Zaldarriaga and D","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.863437Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:92cf0b23b796ad156ac724a1b2f7f854e4379b7d199334ed3a465d950afd096e","observation_id":"de0b56d0-bef5-4115-b836-6fb71b95dcde","resolution":{"observed_at":"2026-08-14T05:58:02.863437Z","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":"2026-08-14T05:58:02.867982Z","title":"Seljak, and M","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.867982Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:418356571551067041f8af47f62da3a045e7585f77b65aca99ac878d9c08105d","observation_id":"e063c1cd-3645-455a-a819-d29b823fd7d0","resolution":{"observed_at":"2026-08-14T05:58:02.867982Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9706147","last_updated":"1997-06-16T01:22:07Z","snapshot_observed_at":"2026-08-15T20:54:07.143898Z","submitted_at":"1997-06-16T01:22:07Z","title":"A CMB Polarization Primer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9706147","snapshot_observed_at":"2026-08-14T05:58:02.872814Z","title":"Hu and M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.872814Z"},"links":{"cited_paper":"/paper/astro-ph/9706147","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:0bd5e5a1aef61981eac3698c4eb6645ccf08d768990d800941045bf67d8812b4","observation_id":"487d1767-4179-4b3a-bec2-e985251d63b2","resolution":{"observed_at":"2026-08-14T05:58:02.872814Z","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":"2026-08-14T05:58:04.671248Z","title":"Polnarev, , Sov","venue":null,"work_id":"185218de-c444-4713-8157-ed1b8955d0c4","year":1986},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.877963Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:9bb060076af0595a160200390e169d156fa8ec13d9989cc17dc43a281807f863","observation_id":"4c5753ca-1332-4046-912a-4052be7036c0","resolution":{"observed_at":"2026-08-14T05:58:04.676046Z","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":{"arxiv_id":"astro-ph/0403392","last_updated":"2005-03-18T00:58:39Z","snapshot_observed_at":"2026-07-07T00:41:20.972563Z","submitted_at":"2004-03-16T21:58:30Z","title":"Theory of Cosmic Microwave Background Polarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0403392","snapshot_observed_at":"2026-08-14T05:58:02.882756Z","title":"Cabella and M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.882756Z"},"links":{"cited_paper":"/paper/astro-ph/0403392","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:8f96de2a73c07e1b05828bf82cb39b85ae381e9d638c079fc1e74697c5782e28","observation_id":"b22a0db8-731c-4f7c-9b18-cb6cfb212ce4","resolution":{"observed_at":"2026-08-14T05:58:02.882756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.04323","last_updated":"2023-09-15T08:09:58Z","snapshot_observed_at":"2026-08-14T16:34:07.448123Z","submitted_at":"2019-05-10T18:03:03Z","title":"Lensing anomaly and oscillations in the primordial power spectrum","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.04323","snapshot_observed_at":"2026-08-14T05:58:02.888364Z","title":"Domnech and M","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.888364Z"},"links":{"cited_paper":"/paper/1905.04323","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:46e8c7ab4a695a9d8ff1b7f3287c3718fab85b0fe1401434dff8cabc2e4378d8","observation_id":"fe8e570c-91ec-4fd4-965c-63cb8ddc1ef6","resolution":{"observed_at":"2026-08-14T05:58:02.888364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.04957","last_updated":"2019-02-04T13:49:36Z","snapshot_observed_at":"2026-08-16T16:24:03.984736Z","submitted_at":"2018-11-12T19:02:19Z","title":"Circular polarization of the cosmic microwave background from vector and tensor perturbations","version":2},"cited_work":{"arxiv_id":"1811.04957","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.04957","snapshot_observed_at":"2026-08-14T05:58:04.149441Z","title":"Circular polarization of the cosmic microwave background from vector and tensor perturbations","venue":"astro-ph.CO","work_id":"c05287fd-c41c-4262-b237-953df905fb6b","year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.893672Z"},"links":{"cited_paper":"/paper/1811.04957","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:3887cea6aca98d36e2795a9376ab73f17c65f21fdc4fbd60a676555bc78fb9ee","observation_id":"deb5d659-e4cd-4910-941d-4baf6e03b349","resolution":{"observed_at":"2026-08-14T05:58:04.154764Z","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":"1811.04959","last_updated":"2019-07-24T22:26:08Z","snapshot_observed_at":"2026-08-16T16:22:48.896765Z","submitted_at":"2018-11-12T19:02:31Z","title":"Chiral photons from chiral gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.04959","snapshot_observed_at":"2026-08-14T05:58:02.898735Z","title":"Inomata and M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.898735Z"},"links":{"cited_paper":"/paper/1811.04959","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:143638f8222b063f895caa4420019c8366e1af6f12e513f6f1f92a5690258abb","observation_id":"4fd6040f-501f-4517-9562-ef92665d3158","resolution":{"observed_at":"2026-08-14T05:58:02.898735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00757","last_updated":"2016-11-02T19:59:03Z","snapshot_observed_at":"2026-08-16T16:24:15.224361Z","submitted_at":"2016-11-02T19:59:03Z","title":"Constraints on Primordial Magnetic Fields from Planck combined with the South Pole Telescope CMB B-mode polarization measurements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00757","snapshot_observed_at":"2026-08-14T05:58:02.904130Z","title":"Zucca, Y","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.904130Z"},"links":{"cited_paper":"/paper/1611.00757","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:4f651e2fcecd6d8b4452f1ea9c038b53b3185d8513ff502975e5f6d5422333c8","observation_id":"4256896c-b325-4035-b122-06483640904b","resolution":{"observed_at":"2026-08-14T05:58:02.904130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.5383","last_updated":"2014-05-30T18:16:47Z","snapshot_observed_at":"2026-08-15T00:02:23.562300Z","submitted_at":"2013-09-20T21:00:08Z","title":"Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.5383","snapshot_observed_at":"2026-08-14T05:58:02.908959Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.908959Z"},"links":{"cited_paper":"/paper/1309.5383","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:6f038ab3fcfb2ad9d2c49ead43d735b3007d804cd3a28adf248d43c958546552","observation_id":"84376221-6d08-45e7-b3ae-e9c08e96c9c0","resolution":{"observed_at":"2026-08-14T05:58:02.908959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.7004","last_updated":"2014-08-12T13:41:42Z","snapshot_observed_at":"2026-08-16T13:31:18.515612Z","submitted_at":"2014-05-27T18:51:51Z","title":"Effects of modified gravity on B-mode polarization","version":2},"cited_work":{"arxiv_id":"1405.7004","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.7004","snapshot_observed_at":"2026-08-14T05:58:04.081582Z","title":"Effects of modified gravity on B-mode polarization","venue":"astro-ph.CO","work_id":"38db2a0d-f108-4c83-81d0-ef82e3bbf8c2","year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.913922Z"},"links":{"cited_paper":"/paper/1405.7004","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:e677cfddcf173f18e0f5b6678295b00a9c15d7a8e7ce41ac16fb87fb29a4e787","observation_id":"523c4276-321e-4953-81e3-74d6d427d987","resolution":{"observed_at":"2026-08-14T05:58:04.086566Z","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":"1405.7974","last_updated":"2014-06-11T14:29:19Z","snapshot_observed_at":"2026-08-14T23:32:04.548712Z","submitted_at":"2014-05-30T19:59:53Z","title":"Measuring the speed of cosmological gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.7974","snapshot_observed_at":"2026-08-14T05:58:02.918914Z","title":"Raveri, C","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.918914Z"},"links":{"cited_paper":"/paper/1405.7974","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:c09e8b0f3b8c14f6f2786f8122c0410f98e709d1a1dce973386cbdc52ca733de","observation_id":"6c3ae360-d01d-4bf4-8347-c03318dec170","resolution":{"observed_at":"2026-08-14T05:58:02.918914Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.6198","last_updated":"2011-09-19T15:48:39Z","snapshot_observed_at":"2026-08-15T04:45:11.564248Z","submitted_at":"2011-05-31T08:11:40Z","title":"Constraints on the fundamental string coupling from B-mode experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.6198","snapshot_observed_at":"2026-08-14T05:58:02.923902Z","title":"Avgoustidis, E","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.923902Z"},"links":{"cited_paper":"/paper/1105.6198","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:f41c6e0acc538010496fbcb99e74197f42f168fa50a7ca7cf0071078f6a54e04","observation_id":"c6141cce-52a4-403b-a227-1c0a9e8ffc83","resolution":{"observed_at":"2026-08-14T05:58:02.923902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.6105","last_updated":"2014-05-08T09:22:08Z","snapshot_observed_at":"2026-08-14T23:40:08.520781Z","submitted_at":"2014-03-24T19:54:03Z","title":"Did BICEP2 see vector modes? First B-mode constraints on cosmic defects","version":2},"cited_work":{"arxiv_id":"1403.6105","doi":null,"metadata_source":"pith","pith_arxiv_id":"1403.6105","snapshot_observed_at":"2026-08-14T05:58:04.024910Z","title":"Did BICEP2 see vector modes? First B-mode constraints on cosmic defects","venue":"astro-ph.CO","work_id":"95000134-c605-4ea5-a8db-9cf76353aeea","year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.928894Z"},"links":{"cited_paper":"/paper/1403.6105","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:9a386ebb71855b57268188a7b8194cb4f21035e3d055a223c3c193d48838c3ea","observation_id":"7e364d09-fa09-4e07-aaf0-2054fb7cd885","resolution":{"observed_at":"2026-08-14T05:58:04.030977Z","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":"1609.03386","last_updated":"2017-02-27T11:58:23Z","snapshot_observed_at":"2026-08-14T21:40:17.979789Z","submitted_at":"2016-09-12T13:22:26Z","title":"New CMB constraints for Abelian Higgs cosmic strings","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.03386","snapshot_observed_at":"2026-08-14T05:58:02.933719Z","title":"Lizarraga, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.933719Z"},"links":{"cited_paper":"/paper/1609.03386","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:b44fa8a0c119ea803224fab55b30823779e3f7c7510185d3788bc4e4c9534ced","observation_id":"dcc0cc82-f8bb-4448-a8c2-07f40e8e2274","resolution":{"observed_at":"2026-08-14T05:58:02.933719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.02743","last_updated":"2016-10-10T00:35:39Z","snapshot_observed_at":"2026-08-15T03:39:02.862503Z","submitted_at":"2016-10-10T00:35:39Z","title":"CMB-S4 Science Book, First Edition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.02743","snapshot_observed_at":"2026-08-14T05:58:02.938478Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.938478Z"},"links":{"cited_paper":"/paper/1610.02743","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:2a5094dd2e7e613bc75aaa83b29defed8300f90cafced722a51360878f378daf","observation_id":"d6632942-82c0-402e-b203-49cdf16b4b10","resolution":{"observed_at":"2026-08-14T05:58:02.938478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9601055","last_updated":"1996-01-11T16:12:00Z","snapshot_observed_at":"2026-08-16T16:26:07.304241Z","submitted_at":"1996-01-11T16:12:00Z","title":"Faraday Rotation of Microwave Background Polarization by a Primordial Magnetic Field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9601055","snapshot_observed_at":"2026-08-14T05:58:02.944082Z","title":"Kosowsky and A","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.944082Z"},"links":{"cited_paper":"/paper/astro-ph/9601055","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:719e47b27fcac1d13afc3fafcdffdf96b1210c8ec9f9a3bc2c18b69a8f21ecbf","observation_id":"a893810b-18f7-4f89-85e7-6738f1cb198b","resolution":{"observed_at":"2026-08-14T05:58:02.944082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.02311","last_updated":"2016-04-24T10:25:52Z","snapshot_observed_at":"2026-08-14T22:53:03.860679Z","submitted_at":"2015-04-09T13:57:37Z","title":"The origin, evolution and signatures of primordial magnetic fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.02311","snapshot_observed_at":"2026-08-14T05:58:02.948933Z","title":"Subramanian, Rept","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.948933Z"},"links":{"cited_paper":"/paper/1504.02311","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:b645d09782d76eafebcca61b515180874b60e8353d5bf1f9024e32852efb55f8","observation_id":"6b314b9f-fe94-430c-a773-c4cf4bf29645","resolution":{"observed_at":"2026-08-14T05:58:02.948933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.3555","last_updated":"2012-10-02T15:41:50Z","snapshot_observed_at":"2026-08-15T04:49:01.286738Z","submitted_at":"2011-04-18T18:21:29Z","title":"Euler-Heisenberg Lagrangian and photon circular polarization","version":2},"cited_work":{"arxiv_id":"1104.3555","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.3555","snapshot_observed_at":"2026-08-14T05:58:03.939517Z","title":"Euler-Heisenberg Lagrangian and photon circular polarization","venue":"hep-ph","work_id":"36805a4c-a679-42ec-afdf-b4aa324a9c28","year":2011},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.954265Z"},"links":{"cited_paper":"/paper/1104.3555","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:357a73c86fd39e6704deadf2a070a17ac337920b920a1558fd2e7dbb3a286a65","observation_id":"b039d415-6ca9-4989-8de5-a8b29971348a","resolution":{"observed_at":"2026-08-14T05:58:03.944890Z","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/0405396","last_updated":"2004-10-18T13:56:56Z","snapshot_observed_at":"2026-08-15T10:06:29.171975Z","submitted_at":"2004-05-20T19:03:32Z","title":"B polarization of the CMB from Faraday rotation","version":4},"cited_work":{"arxiv_id":"astro-ph/0405396","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0405396","snapshot_observed_at":"2026-08-14T05:58:03.918546Z","title":"B polarization of the CMB from Faraday rotation","venue":"astro-ph","work_id":"ff1a35bd-13cc-4988-a404-d15fbbad2225","year":2004},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.959249Z"},"links":{"cited_paper":"/paper/astro-ph/0405396","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:62983690fe37a2856ecb52591ad4dbb4a4267e448f35f6606edebc7e11bb85e7","observation_id":"d6b045a6-2ff2-4b30-a605-7990fad44bdb","resolution":{"observed_at":"2026-08-14T05:58:03.923491Z","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/0405420","last_updated":"2004-10-12T17:26:15Z","snapshot_observed_at":"2026-08-16T16:26:00.904369Z","submitted_at":"2004-05-21T11:06:19Z","title":"Faraday Rotation of the Cosmic Microwave Background Polarization and Primordial Magnetic Field Properties","version":3},"cited_work":{"arxiv_id":"astro-ph/0405420","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0405420","snapshot_observed_at":"2026-08-14T05:58:03.896258Z","title":"Faraday Rotation of the Cosmic Microwave Background Polarization and Primordial Magnetic Field Properties","venue":"astro-ph","work_id":"29b9d828-5e1a-42a4-a6c5-04aabb7769f5","year":2004},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.964179Z"},"links":{"cited_paper":"/paper/astro-ph/0405420","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:d855136639f0b595392cfb488ff0d8f658ff520ec1ebc288d21c198995bbd7ff","observation_id":"f00df0da-c838-48fb-bdd2-d4cf93843aae","resolution":{"observed_at":"2026-08-14T05:58:03.901690Z","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/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":"2026-08-14T05:58:02.969099Z","title":"Kosowsky, T","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.969099Z"},"links":{"cited_paper":"/paper/astro-ph/0409767","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:7bf80aa78a1bfda194a62d70c06e334cbb1da575d9876229da2d15bfd355273a","observation_id":"609d49bb-770b-4f6c-b796-05817e628089","resolution":{"observed_at":"2026-08-14T05:58:02.969099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0410387","last_updated":"2004-12-18T12:35:20Z","snapshot_observed_at":"2026-08-16T16:25:01.145960Z","submitted_at":"2004-10-28T15:25:20Z","title":"Magnetized birefringence and CMB polarization","version":2},"cited_work":{"arxiv_id":"hep-ph/0410387","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0410387","snapshot_observed_at":"2026-08-14T05:58:03.859041Z","title":"Magnetized birefringence and CMB polarization","venue":"hep-ph","work_id":"44807b5a-6f06-4ec8-bdd0-4253a525d47c","year":2004},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.974039Z"},"links":{"cited_paper":"/paper/hep-ph/0410387","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:0f93e0f0c431ad008cf1f875e51864e45ee3a550c61ecb92d1832cd161a409b7","observation_id":"6eeafbf7-0953-4d6e-afd5-3df9dd1bceab","resolution":{"observed_at":"2026-08-14T05:58:03.863951Z","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":"1403.6768","last_updated":"2014-04-28T16:37:12Z","snapshot_observed_at":"2026-08-14T23:39:51.078920Z","submitted_at":"2014-03-26T17:48:51Z","title":"Can primordial magnetic fields be the origin of the BICEP2 data?","version":3},"cited_work":{"arxiv_id":"1403.6768","doi":null,"metadata_source":"pith","pith_arxiv_id":"1403.6768","snapshot_observed_at":"2026-08-14T05:58:03.839143Z","title":"Can primordial magnetic fields be the origin of the BICEP2 data?","venue":"astro-ph.CO","work_id":"d12e23f6-13a7-41bd-a4d7-86473f718b81","year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.979065Z"},"links":{"cited_paper":"/paper/1403.6768","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:62aa2bf31e2dd9a989ff30f8130c6002669e0dc2e99defb0bb0f8bb0c72151cf","observation_id":"c71a298e-7000-4301-a1e1-7c34982e96e2","resolution":{"observed_at":"2026-08-14T05:58:03.844053Z","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":"1404.3974","last_updated":"2014-04-15T16:25:51Z","snapshot_observed_at":"2026-08-16T16:21:34.620608Z","submitted_at":"2014-04-15T16:25:51Z","title":"Faraday scaling and the Bicep2 observations","version":1},"cited_work":{"arxiv_id":"1404.3974","doi":null,"metadata_source":"pith","pith_arxiv_id":"1404.3974","snapshot_observed_at":"2026-08-14T05:58:03.818672Z","title":"Faraday scaling and the Bicep2 observations","venue":"astro-ph.CO","work_id":"cbd9b51a-40e9-4c46-afdd-f335c4f8a393","year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.983906Z"},"links":{"cited_paper":"/paper/1404.3974","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:9afc345920ea095f48fc12fa4600aed283b4f33a1a7a69975f3a4c4e4e558b33","observation_id":"22bec24e-858c-4a08-a9b2-2be5317ad80b","resolution":{"observed_at":"2026-08-14T05:58:03.823864Z","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":"1406.6213","last_updated":"2014-06-24T12:20:09Z","snapshot_observed_at":"2026-08-14T23:29:16.819344Z","submitted_at":"2014-06-24T12:20:09Z","title":"Photon-neutrino scattering and the B-mode spectrum of CMB photons","version":1},"cited_work":{"arxiv_id":"1406.6213","doi":null,"metadata_source":"pith","pith_arxiv_id":"1406.6213","snapshot_observed_at":"2026-08-14T05:58:03.797910Z","title":"Photon-neutrino scattering and the B-mode spectrum of CMB photons","venue":"astro-ph.CO","work_id":"1aa94e02-786f-4218-a942-c2050f5221ff","year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.989386Z"},"links":{"cited_paper":"/paper/1406.6213","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:47f5a4f9c690c136666fed55d1b0376cdba924c6373be75804154a73eab962d4","observation_id":"c149fa7c-57bc-41f7-bb79-f0ad7c53ce65","resolution":{"observed_at":"2026-08-14T05:58:03.802909Z","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":"1503.05356","last_updated":"2015-03-18T11:57:28Z","snapshot_observed_at":"2026-08-14T22:55:51.907645Z","submitted_at":"2015-03-18T11:57:28Z","title":"Generation of CMB B-mode Polarization from Circular Polarization","version":1},"cited_work":{"arxiv_id":"1503.05356","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.05356","snapshot_observed_at":"2026-08-14T05:58:03.775894Z","title":"Generation of CMB B-mode Polarization from Circular Polarization","venue":"astro-ph.CO","work_id":"ca17e4a7-e15b-4fd7-9d86-bac62ed547f4","year":2015},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.994404Z"},"links":{"cited_paper":"/paper/1503.05356","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:48ce80af346cac09da6c376cac847497720d4c0bbf528c6707af7098f0e64230","observation_id":"80924b96-7c17-4056-b2ca-60a420972190","resolution":{"observed_at":"2026-08-14T05:58:03.781751Z","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":"1605.09045","last_updated":"2016-05-29T19:03:04Z","snapshot_observed_at":"2026-08-16T16:23:35.630677Z","submitted_at":"2016-05-29T19:03:04Z","title":"Cosmic microwave background polarization in Noncommutative space-time","version":1},"cited_work":{"arxiv_id":"1605.09045","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09045","snapshot_observed_at":"2026-08-14T05:58:03.753740Z","title":"Cosmic microwave background polarization in Noncommutative space-time","venue":"hep-ph","work_id":"6fcdb2b3-a21e-4ac2-8f0f-d5135fd53575","year":2016},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.999435Z"},"links":{"cited_paper":"/paper/1605.09045","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:9aef78990bed0da07e9a57569e2f78740e7f542185ea7bdc0b8a5f0232129178","observation_id":"7304405c-a314-4153-ad1a-7ae79c4fa9fb","resolution":{"observed_at":"2026-08-14T05:58:03.759181Z","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":"1801.07075","last_updated":"2018-04-03T13:26:13Z","snapshot_observed_at":"2026-08-16T16:24:04.467639Z","submitted_at":"2018-01-22T13:13:15Z","title":"Tuning metal-insulator transitions in epitaxial V$_2$O$_3$ thin films","version":2},"cited_work":{"arxiv_id":"1801.07075","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.07075","snapshot_observed_at":"2026-08-14T05:58:03.731696Z","title":"Tuning metal-insulator transitions in epitaxial V$_2$O$_3$ thin films","venue":"cond-mat.mtrl-sci","work_id":"8fd4ceb6-a687-4bce-8787-e8855acd0f0b","year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.004129Z"},"links":{"cited_paper":"/paper/1801.07075","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:00e3757ff0e2be90a7d2dd41463b5b18e9d9c1110fe43f03c5604e4e27ffe444","observation_id":"fa21588e-79d4-408a-bef2-6d2488aa2aa4","resolution":{"observed_at":"2026-08-14T05:58:03.736840Z","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":"1903.11820","last_updated":"2019-03-28T07:54:30Z","snapshot_observed_at":"2026-08-16T16:22:06.887377Z","submitted_at":"2019-03-28T07:54:30Z","title":"Small field models of inflation that predict a tensor-to-scalar ratio $r=0.03$","version":1},"cited_work":{"arxiv_id":"1903.11820","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.11820","snapshot_observed_at":"2026-08-14T05:58:03.709364Z","title":"Small field models of inflation that predict a tensor-to-scalar ratio $r=0.03$","venue":"astro-ph.CO","work_id":"e8d612a3-b409-4f4c-960a-7ca529cc1034","year":2019},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.009102Z"},"links":{"cited_paper":"/paper/1903.11820","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:495fd2058c3411903a1b8d1157c496fcb9248ecf88c68f1abadef1e118c89a0c","observation_id":"897d1cce-e430-4db1-9281-492c4b3cc457","resolution":{"observed_at":"2026-08-14T05:58:03.714859Z","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":"1210.0308","last_updated":"2012-10-19T10:00:21Z","snapshot_observed_at":"2026-08-15T00:44:49.145016Z","submitted_at":"2012-10-01T08:21:55Z","title":"Primordial Magnetism in CMB B-modes","version":2},"cited_work":{"arxiv_id":"1210.0308","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.0308","snapshot_observed_at":"2026-08-14T05:58:03.687872Z","title":"Primordial Magnetism in CMB B-modes","venue":"astro-ph.CO","work_id":"4d09cbf3-4397-4992-8ed9-18f4219814ce","year":2012},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.014262Z"},"links":{"cited_paper":"/paper/1210.0308","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:3527d03f13017b059843742feeed47b64c589916ea34217b04df8f7b042c69e8","observation_id":"662873b7-6c8a-41ac-91e2-94b6656954c0","resolution":{"observed_at":"2026-08-14T05:58:03.692880Z","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/0012056","last_updated":"2001-08-24T15:31:14Z","snapshot_observed_at":"2026-08-16T16:26:06.136721Z","submitted_at":"2000-12-03T14:53:20Z","title":"Cosmic Microwave Background Polarization Signals from Tangled Magnetic Fields","version":2},"cited_work":{"arxiv_id":"astro-ph/0012056","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0012056","snapshot_observed_at":"2026-08-14T05:58:03.664020Z","title":"Cosmic Microwave Background Polarization Signals from Tangled Magnetic Fields","venue":"astro-ph","work_id":"c1d128d6-bedf-4a8d-b29f-82e0f3eaf6f3","year":2000},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.019380Z"},"links":{"cited_paper":"/paper/astro-ph/0012056","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:84923fcb3e4e6ff5bdc2dec3ff4062ce995c0393ee9beac0efbf0b728d71cc97","observation_id":"795cd174-38b2-4b5e-80c1-c2b8e50729ac","resolution":{"observed_at":"2026-08-14T05:58:03.669850Z","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":"0806.1876","last_updated":"2009-07-15T12:25:16Z","snapshot_observed_at":"2026-08-15T10:13:30.146962Z","submitted_at":"2008-06-11T13:47:09Z","title":"Faraday Rotation Limits on a Primordial Magnetic Field from WMAP Five-Year Data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.1876","snapshot_observed_at":"2026-08-14T05:58:03.024436Z","title":"Kahniashvili, Y","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.024436Z"},"links":{"cited_paper":"/paper/0806.1876","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:d4235a68dfa45a9a1eaaa5965408005005973e9f64276f5bd79692422a800d3a","observation_id":"67371591-80bd-4ea1-8cd7-16d38b7ff74a","resolution":{"observed_at":"2026-08-14T05:58:03.024436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0406096","last_updated":"2004-08-19T17:17:51Z","snapshot_observed_at":"2026-08-16T16:26:00.388647Z","submitted_at":"2004-06-03T19:25:22Z","title":"CMB anisotropies from primordial inhomogeneous magnetic fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0406096","snapshot_observed_at":"2026-08-14T05:58:03.029229Z","title":"Lewis, Phys","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.029229Z"},"links":{"cited_paper":"/paper/astro-ph/0406096","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:35b5d4caf10d752ae37b9f7b6c2ceae22f57d533528390b959a28379d39882c8","observation_id":"21be9b25-6bf2-4aa9-aee0-3c410331b562","resolution":{"observed_at":"2026-08-14T05:58:03.029229Z","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":"2026-08-14T05:58:03.034091Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.034091Z"},"links":{"cited_paper":"/paper/1612.02104","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:6a1cc02149a4135b767bbe7d178352ad5152d9f92c392b2ecd23e476e3d8780a","observation_id":"4c5a3e5e-4d7d-483a-a409-30cc4143e10c","resolution":{"observed_at":"2026-08-14T05:58:03.034091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9803150","last_updated":"1998-03-13T02:48:14Z","snapshot_observed_at":"2026-08-16T16:28:26.822245Z","submitted_at":"1998-03-13T02:48:14Z","title":"Gravitational Lensing Effect on Cosmic Microwave Background Polarization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9803150","snapshot_observed_at":"2026-08-14T05:58:03.038909Z","title":"Zaldarriaga and U","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.038909Z"},"links":{"cited_paper":"/paper/astro-ph/9803150","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:60e50194b6c1afca858b247ab9ed04c8a8a09d9a265448b6a263f4bc721c2caf","observation_id":"f0b91718-3a55-494b-84a5-c89f67b30e9b","resolution":{"observed_at":"2026-08-14T05:58:03.038909Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.0747","last_updated":"2008-02-07T15:17:14Z","snapshot_observed_at":"2026-08-15T10:28:22.070145Z","submitted_at":"2007-11-05T21:15:34Z","title":"B-modes from Cosmic Strings","version":3},"cited_work":{"arxiv_id":"0711.0747","doi":null,"metadata_source":"pith","pith_arxiv_id":"0711.0747","snapshot_observed_at":"2026-08-14T05:58:03.575670Z","title":"B-modes from Cosmic Strings","venue":"astro-ph","work_id":"4d0d4981-2f60-408a-b303-0336df0aaa58","year":2007},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.043714Z"},"links":{"cited_paper":"/paper/0711.0747","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:7160081544baea14108bfd17f14687477a00ce68e9e5d7af929d088be930ef69","observation_id":"4caf4259-0d6a-4308-81c8-095eb051b4c1","resolution":{"observed_at":"2026-08-14T05:58:03.581581Z","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":"1704.02704","last_updated":"2017-05-13T00:22:45Z","snapshot_observed_at":"2026-08-16T16:28:12.791270Z","submitted_at":"2017-04-10T04:07:02Z","title":"POLOCALC: a Novel Method to Measure the Absolute Polarization Orientation of the Cosmic Microwave Background","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.02704","snapshot_observed_at":"2026-08-14T05:58:03.048609Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.048609Z"},"links":{"cited_paper":"/paper/1704.02704","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:9fb28840eb1e0c0aff51d92720972934b0e39aefc67c631018cdf3b840a48c4e","observation_id":"64338a77-be11-4d4e-bb04-bbba2b569e31","resolution":{"observed_at":"2026-08-14T05:58:03.048609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.00237","last_updated":"2016-01-31T12:34:59Z","snapshot_observed_at":"2026-08-16T16:24:01.785576Z","submitted_at":"2016-01-31T12:34:59Z","title":"The B-mode polarization of CMB and Cosmic Neutrino Background","version":1},"cited_work":{"arxiv_id":"1602.00237","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.00237","snapshot_observed_at":"2026-08-14T05:58:03.535845Z","title":"The B-mode polarization of CMB and Cosmic Neutrino Background","venue":"astro-ph.CO","work_id":"fa652775-6bc6-4a8b-be50-4022ae3b08d3","year":2016},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.053394Z"},"links":{"cited_paper":"/paper/1602.00237","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:ee9b5d2cd5d2503c1a54c4ac3466e71e9f62d00472ba89a3f9623f0d682295a8","observation_id":"0ee1bb4f-e4e1-41c2-9d08-0e0de54b8fb9","resolution":{"observed_at":"2026-08-14T05:58:03.541164Z","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":"1312.2199","last_updated":"2014-08-07T06:45:29Z","snapshot_observed_at":"2026-08-16T16:21:53.292208Z","submitted_at":"2013-12-08T12:23:52Z","title":"Evidence for cosmic neutrino background form CMB circular polarization","version":3},"cited_work":{"arxiv_id":"1312.2199","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.2199","snapshot_observed_at":"2026-08-14T05:58:03.512973Z","title":"Evidence for cosmic neutrino background form CMB circular polarization","venue":"astro-ph.CO","work_id":"e358bdb5-4739-4b1b-8cd3-69c24f539ea4","year":2013},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.058146Z"},"links":{"cited_paper":"/paper/1312.2199","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:b1e79d5219e09726fff56f7fe18529bc8f7d1100697625701ae2dc1773bcf6b5","observation_id":"f7684d0f-cb72-4377-8d75-15f329b422ee","resolution":{"observed_at":"2026-08-14T05:58:03.518337Z","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":"1711.06997","last_updated":"2017-11-19T10:42:54Z","snapshot_observed_at":"2026-08-17T05:08:10.078542Z","submitted_at":"2017-11-19T10:42:54Z","title":"Generation of circular polarization in CMB radiation via nonlinear photon-photon interaction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.06997","snapshot_observed_at":"2026-08-14T05:58:03.063130Z","title":"Sadegh, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.063130Z"},"links":{"cited_paper":"/paper/1711.06997","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:d8888d0e332e1a5623e185d03257a38094c64f5f5cbccba20455ad30137b30a2","observation_id":"0628cc5b-93c3-4f56-8cd9-95ea982520da","resolution":{"observed_at":"2026-08-14T05:58:03.063130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.2993","last_updated":"2010-08-19T07:22:03Z","snapshot_observed_at":"2026-08-15T12:01:27.618057Z","submitted_at":"2009-12-16T15:05:34Z","title":"Generation of circular polarization of the CMB","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.2993","snapshot_observed_at":"2026-08-14T05:58:03.068296Z","title":"Zarei, E","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.068296Z"},"links":{"cited_paper":"/paper/0912.2993","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:244c767060927f07d9f5a1253260cf53b091d28df260217feddc2d2ab76c69f4","observation_id":"2451a479-65a5-4601-b3f6-a8949d4e756e","resolution":{"observed_at":"2026-08-14T05:58:03.068296Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11172","last_updated":"2018-10-29T19:18:02Z","snapshot_observed_at":"2026-08-14T19:10:11.109919Z","submitted_at":"2018-05-28T20:56:42Z","title":"Dipolar dark matter and CMB B-mode polarization","version":2},"cited_work":{"arxiv_id":"1805.11172","doi":null,"metadata_source":"pith","pith_arxiv_id":"1805.11172","snapshot_observed_at":"2026-08-14T05:58:03.458140Z","title":"Dipolar dark matter and CMB B-mode polarization","venue":"hep-ph","work_id":"356133ab-6280-4568-8ee3-3d9ac00dfd88","year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.073558Z"},"links":{"cited_paper":"/paper/1805.11172","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:0a8d6d816b0c039e22505da68659911d5047412d26bd337c77175cda48e76565","observation_id":"d93f0c4d-6666-4842-b64c-bd6d692923b3","resolution":{"observed_at":"2026-08-14T05:58:03.463395Z","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":"1903.04578","last_updated":"2019-08-10T14:10:17Z","snapshot_observed_at":"2026-08-16T16:23:59.108665Z","submitted_at":"2019-03-11T20:15:30Z","title":"CMB circular and B-mode polarization from new interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04578","snapshot_observed_at":"2026-08-14T05:58:03.078690Z","title":"Bartolo, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.078690Z"},"links":{"cited_paper":"/paper/1903.04578","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:33f1a5e5d0cab3d4ca14e9f246840dbc67ec8856de5b7449013f317a0645f1b0","observation_id":"4a801270-4e78-4bd0-a872-ffad1980cbee","resolution":{"observed_at":"2026-08-14T05:58:03.078690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.0832","last_updated":"2013-03-18T13:38:18Z","snapshot_observed_at":"2026-08-15T00:29:58.399522Z","submitted_at":"2013-02-04T20:56:56Z","title":"The intrinsic bispectrum of the Cosmic Microwave Background","version":2},"cited_work":{"arxiv_id":"1302.0832","doi":null,"metadata_source":"pith","pith_arxiv_id":"1302.0832","snapshot_observed_at":"2026-08-14T05:58:03.419043Z","title":"The intrinsic bispectrum of the Cosmic Microwave Background","venue":"astro-ph.CO","work_id":"c40c90ca-74ed-4533-ac3f-d6ffe4ed08c2","year":2013},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.083944Z"},"links":{"cited_paper":"/paper/1302.0832","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:49067ee6fce23d997d09d73b5f7095faa52e1172004a6ca068aeac8a6badb7f3","observation_id":"c2bd2ec1-82be-40dd-b697-e3ab8aa0a762","resolution":{"observed_at":"2026-08-14T05:58:03.424315Z","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":"1401.3296","last_updated":"2014-06-05T16:15:38Z","snapshot_observed_at":"2026-08-16T14:10:48.850200Z","submitted_at":"2014-01-14T19:26:21Z","title":"The intrinsic B-mode polarisation of the Cosmic Microwave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.3296","snapshot_observed_at":"2026-08-14T05:58:03.089003Z","title":"Fidler, G","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.089003Z"},"links":{"cited_paper":"/paper/1401.3296","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:499560d49aa0f4c1f2aa6106e9939c3e32ff621b4cc7da7026db5442e7c17be7","observation_id":"364692ef-7016-4d72-95d5-7fa5865b02f2","resolution":{"observed_at":"2026-08-14T05:58:03.089003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.08137","last_updated":"2018-10-29T18:59:07Z","snapshot_observed_at":"2026-08-16T16:22:56.053917Z","submitted_at":"2018-09-20T17:21:45Z","title":"Generation of Circular Polarization of CMB via Polarized Compton Scattering","version":3},"cited_work":{"arxiv_id":"1809.08137","doi":null,"metadata_source":"pith","pith_arxiv_id":"1809.08137","snapshot_observed_at":"2026-08-14T05:58:03.379756Z","title":"Generation of Circular Polarization of CMB via Polarized Compton Scattering","venue":"astro-ph.CO","work_id":"83ac7924-a748-4230-8241-160f3c51edd3","year":2018},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.093989Z"},"links":{"cited_paper":"/paper/1809.08137","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:24a315f3b78603a913f936e43788502e74f55adf97137e9b359565bea9d8639f","observation_id":"3257dec9-4f78-4e73-9e5b-f23f0d847afd","resolution":{"observed_at":"2026-08-14T05:58:03.385253Z","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/9501045","last_updated":"1995-02-03T14:26:02Z","snapshot_observed_at":"2026-08-08T23:31:33.814856Z","submitted_at":"1995-01-13T17:32:33Z","title":"Cosmic Microwave Background Polarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9501045","snapshot_observed_at":"2026-08-14T05:58:03.098791Z","title":"Kosowsky, Annals Phys","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.098791Z"},"links":{"cited_paper":"/paper/astro-ph/9501045","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:a68f3b66ec983a5d43a00ae89b5d04da4216be0821c13650c87c73ffacab1c54","observation_id":"bbf9000d-8b97-4946-a334-ec5f3149d264","resolution":{"observed_at":"2026-08-14T05:58:03.098791Z","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":"2026-08-14T05:58:04.655821Z","title":"Kleiss, W","venue":null,"work_id":"43f12392-54e4-47ce-a46e-132923057bf2","year":1985},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.103717Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:f543d2879d5eb66868011758ced8e90ee9ec80a7da81e70dc28bd9ce4c268732","observation_id":"32b066ac-9762-4e7b-b01a-8c973c71215f","resolution":{"observed_at":"2026-08-14T05:58:04.660528Z","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":"2026-08-14T05:58:04.641433Z","title":"Itzykson, J","venue":null,"work_id":"49d0bbba-a82f-4d6e-9ef7-08cabaff0251","year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.108394Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:11d3c3fbec6f8f5a31411d7767a80d88f37d267b5a3d098e40fe67d3a65da780","observation_id":"005aafc4-547b-4d73-b41a-60c43d7abdad","resolution":{"observed_at":"2026-08-14T05:58:04.645979Z","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":"2026-08-14T05:58:04.625889Z","title":"Kessler,” Polarized Electrons”, 2nd","venue":null,"work_id":"dd7bbdd3-246f-45ef-9d67-edb83072f530","year":1985},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.113615Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:1be55d98e28b1f4f2244399c6193d3246c1185e80c6481aff6a39e0d89f025cb","observation_id":"c6e5ef1b-1b97-4744-8e1f-cbce02c87770","resolution":{"observed_at":"2026-08-14T05:58:04.631046Z","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":"2026-08-14T05:58:04.608401Z","title":null,"venue":null,"work_id":"3e63f9a4-eeb2-4a41-bf03-a1f9acfa0ba8","year":1965},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.118130Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:6cc8c2f3e7339fffcd3ec63a090a99baa9e5231ba1994d9639baa35776441ca1","observation_id":"5ecb93d9-6f70-4bf9-9aa3-61bbfc08ad16","resolution":{"observed_at":"2026-08-14T05:58:04.614348Z","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":"2026-08-14T05:58:04.591047Z","title":null,"venue":null,"work_id":"8bc275e9-c820-4c00-a706-b2fbe438edf6","year":1999},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.122757Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:73b327e6ffc3e1f52bc09f68a64f8de9884aab599574703a0094c2f071e477e9","observation_id":"27a952d1-704c-4aec-b2ec-7105d7d31020","resolution":{"observed_at":"2026-08-14T05:58:04.596089Z","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":"2026-08-14T05:58:04.572611Z","title":"Bell, Nuclear Instruments and Methods in Physics Research B 86, 251-256, 1994","venue":null,"work_id":"dd957844-503a-4665-b3b9-ef90b0a7a28b","year":1994},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.127388Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:f08b251bb9e4f624aa52975f0c3a27e166c0c65711aed25356f7dd8daaa1025c","observation_id":"b5cfc75f-dd30-463f-a36b-720bc2e9e196","resolution":{"observed_at":"2026-08-14T05:58:04.578098Z","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":{"arxiv_id":"0809.0220","last_updated":"2008-09-01T12:24:34Z","snapshot_observed_at":"2026-08-15T10:07:52.381359Z","submitted_at":"2008-09-01T12:24:34Z","title":"Gamma-ray polarization constraints on Planck scale violations of special relativity","version":1},"cited_work":{"arxiv_id":"0809.0220","doi":null,"metadata_source":"pith","pith_arxiv_id":"0809.0220","snapshot_observed_at":"2026-08-14T05:58:03.339970Z","title":"Gamma-ray polarization constraints on Planck scale violations of special relativity","venue":"astro-ph","work_id":"c25d7bcb-5e17-4d64-b6ce-05029983f4aa","year":2008},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.131961Z"},"links":{"cited_paper":"/paper/0809.0220","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:fe3e557d2368742ef599d2b61758bc0a1da9e75dc4d4ee9fba062b702e3264c4","observation_id":"0574b5a3-b2fa-4863-9760-cc41098464f3","resolution":{"observed_at":"2026-08-14T05:58:03.345300Z","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":"1303.7121","last_updated":"2013-05-07T09:57:37Z","snapshot_observed_at":"2026-08-15T00:23:24.150016Z","submitted_at":"2013-03-28T13:42:03Z","title":"Cosmological Magnetic Fields: Their Generation, Evolution and Observation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.7121","snapshot_observed_at":"2026-08-14T05:58:03.136691Z","title":"Durrer and A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.136691Z"},"links":{"cited_paper":"/paper/1303.7121","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:76a73ae65e0dc69c9a1e378be54d82d5bd788d843ed707fa16c851bc07ba1d97","observation_id":"dc230752-b86a-4efb-b325-aed65fc7e1bf","resolution":{"observed_at":"2026-08-14T05:58:03.136691Z","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":"2026-08-14T05:58:04.555737Z","title":null,"venue":null,"work_id":"5e7524f3-d7dd-4b84-9e2e-734ff1810240","year":1967},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.141429Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:84377a898bc7487d800a0d24848eba3691a4e24c679eb8daff53986a91fdf1d9","observation_id":"cd71dfa2-325f-425e-9a51-eb4872b0e4b8","resolution":{"observed_at":"2026-08-14T05:58:04.560854Z","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":"0705.4275","last_updated":"2007-08-13T22:45:44Z","snapshot_observed_at":"2026-08-16T10:36:52.201865Z","submitted_at":"2007-05-29T19:10:01Z","title":"Solution of the Dirac equation in presence of an uniform magnetic field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.4275","snapshot_observed_at":"2026-08-14T05:58:03.145935Z","title":"Bhattacharya, [arXiv:0705.4275 [hep-th]]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.145935Z"},"links":{"cited_paper":"/paper/0705.4275","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:533114e6e987edffeee5a4f418c36112478f470092fcfe81c3c6fec48fcb1fb1","observation_id":"c7271b7e-5a98-4cd7-8a8b-49fd8cead1a7","resolution":{"observed_at":"2026-08-14T05:58:03.145935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205214","last_updated":"2002-05-15T01:48:31Z","snapshot_observed_at":"2026-08-16T16:26:20.838686Z","submitted_at":"2002-05-15T01:48:31Z","title":"Is the Cosmic Microwave Background Circularly Polarized?","version":1},"cited_work":{"arxiv_id":"astro-ph/0205214","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0205214","snapshot_observed_at":"2026-08-14T05:58:03.281771Z","title":"Is the Cosmic Microwave Background Circularly Polarized?","venue":"astro-ph","work_id":"09ed1ddd-d782-406f-a0ae-ece23f72eb84","year":2002},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.150731Z"},"links":{"cited_paper":"/paper/astro-ph/0205214","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:c101871f3831d2e9cfaa1fefe1310c2b6d7ff3b2ac7a783157965de5b2d53f5e","observation_id":"920cd912-814b-4b0f-94a6-6c35b2c50668","resolution":{"observed_at":"2026-08-14T05:58:03.289148Z","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":"1402.4760","last_updated":"2014-02-19T18:33:29Z","snapshot_observed_at":"2026-08-14T23:44:04.730263Z","submitted_at":"2014-02-19T18:33:29Z","title":"Magnetars and the Chiral Plasma Instabilities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.4760","snapshot_observed_at":"2026-08-14T05:58:03.155353Z","title":"Ohnishi and N","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.155353Z"},"links":{"cited_paper":"/paper/1402.4760","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:80fe1e5af947ac533f0d123f1931b984ed7128ddf1e13f24390f8b34f9a51789","observation_id":"09821e7a-c118-40c6-a34f-f11967953b05","resolution":{"observed_at":"2026-08-14T05:58:03.155353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.00891","last_updated":"2016-12-23T15:55:12Z","snapshot_observed_at":"2026-08-14T22:37:41.892869Z","submitted_at":"2015-08-04T19:57:55Z","title":"Fermion production during and after axion inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.00891","snapshot_observed_at":"2026-08-14T05:58:03.160144Z","title":"Adshead and E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.160144Z"},"links":{"cited_paper":"/paper/1508.00891","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:978fe3f6567ef411cb2913e7cdf26ae4d8abf5ef97f8d41797e66be419a4ef6b","observation_id":"5a6401a1-31ae-42ea-95bb-018391378e35","resolution":{"observed_at":"2026-08-14T05:58:03.160144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.1459","last_updated":"2016-04-01T13:10:01Z","snapshot_observed_at":"2026-08-15T00:11:43.442503Z","submitted_at":"2013-07-04T19:43:40Z","title":"The CLASSgal code for Relativistic Cosmological Large Scale Structure","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.1459","snapshot_observed_at":"2026-08-14T05:58:03.165005Z","title":"Di Dio, F","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.165005Z"},"links":{"cited_paper":"/paper/1307.1459","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:9bbd8269b2a707037a85b5eb9062ff9483e5930713b684da8697ced65e093633","observation_id":"24302750-e6ee-445e-b32e-a81de755818d","resolution":{"observed_at":"2026-08-14T05:58:03.165005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205436","last_updated":"2002-10-14T18:03:43Z","snapshot_observed_at":"2026-07-07T00:26:35.863418Z","submitted_at":"2002-05-24T19:54:59Z","title":"Cosmological parameters from CMB and other data: a Monte-Carlo approach","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0205436","snapshot_observed_at":"2026-08-14T05:58:03.169589Z","title":"Lewis and S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.169589Z"},"links":{"cited_paper":"/paper/astro-ph/0205436","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:7aa3fcdbe117421731976a70ea146ef526c29e074f58ef8e68433341623a90e0","observation_id":"7ad9846b-d33f-4e1f-9505-e557b36fc1f4","resolution":{"observed_at":"2026-08-14T05:58:03.169589Z","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":"2026-08-14T05:58:04.540155Z","title":null,"venue":null,"work_id":"9ce52a78-23df-4ebd-8d60-fa092975a034","year":null},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:03.174611Z"},"links":{"citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:f089abd77ea1cf371ecedb0c69a933ce851b3cf3070dcc9ee1c7a1f08e5e8dd4","observation_id":"597d0561-4fd0-4a40-945b-90b7c2f133a0","resolution":{"observed_at":"2026-08-14T05:58:04.544937Z","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"}}],"paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T07:38:49.900370Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering"},"reference_resolution":{"displayed":84,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":50,"verified_exact":29,"verified_fuzzy":5},"total_outbound_references":84},"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 84 of 84 outbound references and 0 inbound Pith citation observations for arXiv:1909.00568."}