{"as_of":"2026-08-04T14:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:534d41ad657923c7ccaf0dcb30feaaaeeef8be139695893d7d0dadf657b4f365","coverage":[{"denominator":63,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":63,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-12T02:17:22.022693Z","state":"measured"},{"denominator":65,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":65,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T23:54:15.289428Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-05-14T18:47:37.502077Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"cited_work":{"arxiv_id":"2605.08907","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.08907","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","venue":"astro-ph.CO","work_id":"dea40179-1c7c-4a34-ac1b-5286100d5a56","year":2026},"citing_paper":{"arxiv_id":"2605.13016","last_updated":"2026-05-13T05:11:09Z","snapshot_observed_at":"2026-07-06T23:24:37.915639Z","submitted_at":"2026-05-13T05:11:09Z","title":"Revisiting constraints on primordial vector modes and implications for sourced magnetic fields and observed $EB$ power spectrum","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-14T18:39:36.622565Z"},"links":{"cited_paper":"/paper/2605.08907","citing_paper":"/paper/2605.13016"},"observation_digest":"sha256:f1635bcabcbc2addaa8658a10b70f74923bfbe7420458a03ab4c97191007fca8","observation_id":"8ee59d92-d16a-4223-bde2-ff5dc9d83bce","resolution":{"observed_at":"2026-05-14T18:47:37.504871Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.08907","snapshot_observed_at":"2026-08-01T23:54:15.289428Z","title":"Rida Khalife and C","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.15335","last_updated":"2026-07-16T17:24:11Z","snapshot_observed_at":"2026-08-01T23:54:13.157534Z","submitted_at":"2026-07-16T17:24:11Z","title":"Primordial tensor mode from the neutrino sector","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-01T23:54:15.289428Z"},"links":{"cited_paper":"/paper/2605.08907","citing_paper":"/paper/2607.15335"},"observation_digest":"sha256:f801b996c12794e812541786331f73f87d1d19531984f3fbc5115ead0a7c647f","observation_id":"64a252f6-47bc-49a9-b26b-2578726b070a","resolution":{"observed_at":"2026-08-01T23:54:15.289428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2605.08907/citation-record","integrity":"/paper/2605.08907/integrity","json":"/paper/2605.08907/citation-record.json","paper":"/paper/2605.08907"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Oxford Graduate Texts","venue":null,"work_id":"97cfd390-7c5a-4c2c-8bc8-9d2a9656df87","year":2013},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:dde49f50620c73932ead95eb9f85479b93d6403c1a2866ba1ffc4a32cecfda6a","observation_id":"db0e9b45-25cf-4d9b-83fb-5c7aa1ec2732","resolution":{"observed_at":"2026-05-12T23:26:57.209037Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Academic Press, April","venue":null,"work_id":"2aa82068-e96a-4339-9ecb-911b640e6175","year":2020},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:27bd8fefd267a4c877594384167fdbff2df780c460fb7c09d3ce555fa012e8b7","observation_id":"0f0ae823-7df9-4a35-b345-693e02f11cea","resolution":{"observed_at":"2026-05-12T23:26:57.193179Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bardeen, Gauge Invariant Cosmological Perturbations , Phys","venue":null,"work_id":"8e9f4cfe-b296-4a24-b9a2-2f8aabadd603","year":1980},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:e1e68d7293a39aaeb1fca59498cb7430a45aae76f350a1fd3d43548eed83448d","observation_id":"2643b7e6-1124-48f7-926e-1c1f54ba57bc","resolution":{"observed_at":"2026-05-12T23:26:57.189589Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"62c528f3-5095-4b0d-a6e1-52c1eaa153ac","year":1984},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:6ed9806e48df6fdf44be714ea05f4ee183c33d37919f635c8128fd29a35bbac6","observation_id":"a815b796-b25b-44f4-8fe5-539d2b0bf5da","resolution":{"observed_at":"2026-05-12T23:26:57.197349Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Mukhanov, H","venue":null,"work_id":"1e162b86-802a-4ece-af8b-7f615cccd7a3","year":1992},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:4cc09e9cb975cb3f34af8da48ddb266ae77cc93bd6199eb03aaea26f7d736268","observation_id":"a40dbf3b-9191-4ea2-80ae-5a435dfd7812","resolution":{"observed_at":"2026-05-12T23:26:57.202657Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9702170","last_updated":"1997-07-16T19:42:11Z","snapshot_observed_at":"2026-07-07T01:16:01.826754Z","submitted_at":"1997-02-19T23:10:24Z","title":"CMB Anisotropies: Total Angular Momentum Method","version":3},"cited_work":{"arxiv_id":"astro-ph/9702170","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9702170","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"CMB Anisotropies: Total Angular Momentum Method","venue":"astro-ph","work_id":"5df1dd41-510e-4f40-8993-fc1d71a35891","year":1997},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/9702170","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:5d689556399f9d672d65fb28cc11288e81d0437b0ab3dea3a9d619fd207b6784","observation_id":"8338aa7f-ce4e-47c5-baf0-545cd19ec252","resolution":{"observed_at":"2026-05-12T07:41:59.274358Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.13687","last_updated":"2019-09-30T13:33:35Z","snapshot_observed_at":"2026-08-03T02:23:18.059213Z","submitted_at":"2019-09-30T13:33:35Z","title":"Beyond scalar, vector and tensor harmonics in maximally symmetric three-dimensional spaces","version":1},"cited_work":{"arxiv_id":"1909.13687","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.13687","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Pereira, Beyond scalar, vector and tensor harmonics in maximally symmetric three-dimensional spaces , Phys","venue":null,"work_id":"50db68f0-40e4-4578-91af-6ca7b402590e","year":2019},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1909.13687","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:d866d5e8358fe6fbb1d39623c8b0d9842481c41f55faf0eeec82481afa3236f9","observation_id":"520763eb-1831-4bfa-92af-ef91fae59d75","resolution":{"observed_at":"2026-05-12T07:42:01.509706Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9407093","last_updated":"1994-07-28T17:07:29Z","snapshot_observed_at":"2026-07-07T01:09:50.146754Z","submitted_at":"1994-07-28T17:07:29Z","title":"Anisotropies in the Cosmic Microwave Background: An Analytic Approach","version":1},"cited_work":{"arxiv_id":"astro-ph/9407093","doi":"10.1086/175624","metadata_source":"pith","pith_arxiv_id":"astro-ph/9407093","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Anisotropies in the Cosmic Microwave Background: An Analytic Approach","venue":"astro-ph","work_id":"12d858be-b2af-4c82-9e44-76ad022c7358","year":1994},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/9407093","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:7d626993247e89f1e82e8969822cb70338b163ac25ecaa180690e320a02c162d","observation_id":"ce4ee571-5a8b-4109-8b5d-198744444f89","resolution":{"observed_at":"2026-05-12T07:41:57.084743Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0001303","last_updated":"2000-01-18T15:19:30Z","snapshot_observed_at":"2026-07-07T00:09:31.766167Z","submitted_at":"2000-01-18T15:19:30Z","title":"Weak Lensing of the CMB: A Harmonic Approach","version":1},"cited_work":{"arxiv_id":"astro-ph/0001303","doi":"10.1103/physrevd.62.043007","metadata_source":"pith","pith_arxiv_id":"astro-ph/0001303","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Weak Lensing of the CMB: A Harmonic Approach","venue":"astro-ph","work_id":"d3399c42-1d78-4a93-a0ea-ad5d58b5d592","year":2000},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/0001303","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:dac28f4be28f8209dc5f3933af198bb668d787054218463fa46391c3adf69976","observation_id":"08daed5f-5173-48ef-ae92-91389ee2f1e9","resolution":{"observed_at":"2026-05-12T07:41:58.296954Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-05-24T17:24:22.84941+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T17:24:22.84941+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0406180","last_updated":"2004-10-22T15:09:51Z","snapshot_observed_at":"2026-07-07T04:50:59.450093Z","submitted_at":"2004-06-21T21:06:35Z","title":"Vector Perturbations in a Contracting Universe","version":3},"cited_work":{"arxiv_id":"hep-th/0406180","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"hep-th/0406180","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Battefeld and Robert Brandenberger, Vector perturbations in a contracting universe, Phys","venue":null,"work_id":"029ba154-5f7c-44af-8211-672dfb70bd55","year":2004},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/hep-th/0406180","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:19c3c682f3208ead502c11b59f6604ef4c09e4cda0bd07cf5533e4320a5a7640","observation_id":"89c11273-0765-4545-a864-439efbd76eed","resolution":{"observed_at":"2026-05-13T18:20:58.482684Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0872","last_updated":"2007-09-06T14:33:31Z","snapshot_observed_at":"2026-07-06T01:29:39.615945Z","submitted_at":"2007-09-06T14:33:31Z","title":"Cosmological vector modes and quantum gravity effects","version":1},"cited_work":{"arxiv_id":"0709.0872","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"0709.0872","snapshot_observed_at":"2026-07-04T15:24:39.378117Z","title":null,"venue":null,"work_id":"9c1e0dc2-56d0-4687-8adf-fce529917478","year":2007},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/0709.0872","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:cb289a85f9c808057dd0bf34f7708be92f3a8963196d90e4abc0a2b12970de84","observation_id":"f55cc659-b8bb-4111-970d-575c23709d6c","resolution":{"observed_at":"2026-07-04T15:24:39.378117Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2409.09458","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"62e37ab0-0034-495c-8973-092f9c3a4f42","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:020b5ecfb0526e97bcb37db29c7b1d9c676fa917bdf024dbae263796746263cd","observation_id":"5e119fce-dcf0-49bd-b2c1-f61ec2040623","resolution":{"observed_at":"2026-05-12T07:41:57.957109Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0105504","last_updated":"2002-04-09T20:26:24Z","snapshot_observed_at":"2026-07-07T00:18:46.094198Z","submitted_at":"2001-05-29T19:40:24Z","title":"Microwave Background Signatures of a Primordial Stochastic Magnetic Field","version":2},"cited_work":{"arxiv_id":"astro-ph/0105504","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0105504","snapshot_observed_at":"2026-07-04T11:29:50.957141Z","title":"Microwave Background Signatures of a Primordial Stochastic Magnetic Field","venue":"astro-ph","work_id":"7332386b-0298-4550-b2b6-3c36019e5894","year":2001},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/0105504","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:9590947af8731de6dc32bdbbd1199734168c0d753f55c7903235b654550fc529","observation_id":"75572eba-f551-4d22-90d0-9e8a6fedeb11","resolution":{"observed_at":"2026-05-12T07:41:57.830299Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0811.0230","last_updated":"2009-05-22T14:17:25Z","snapshot_observed_at":"2026-07-06T01:45:41.842228Z","submitted_at":"2008-11-03T07:04:53Z","title":"The full contribution of a stochastic background of magnetic fields to CMB anisotropies","version":2},"cited_work":{"arxiv_id":"0811.0230","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.0230","snapshot_observed_at":"2026-07-04T11:29:50.934746Z","title":"The full contribution of a stochastic background of magnetic fields to CMB anisotropies","venue":"astro-ph","work_id":"93c928fc-6e04-415e-80df-c9dc8d75d6fd","year":2008},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/0811.0230","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:c645c720376075eb1746e7d660cd97f897deee3464053bbabb0ed89d748bd589","observation_id":"50a6cddb-66d4-4137-81e3-a41314d8b489","resolution":{"observed_at":"2026-05-12T07:41:57.039704Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0801.2572","last_updated":"2008-02-16T06:04:05Z","snapshot_observed_at":"2026-07-06T01:37:49.810449Z","submitted_at":"2008-01-17T16:20:42Z","title":"Effects of a Primordial Magnetic Field on Low and High Multipoles of the CMB","version":3},"cited_work":{"arxiv_id":"0801.2572","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"0801.2572","snapshot_observed_at":"2026-07-04T15:34:01.524978Z","title":"Yamazaki, Kiyotomo Ichiki, Toshitaka Kajino, and Grant J","venue":null,"work_id":"81361711-96f1-4c06-a593-a80a31e63d99","year":2008},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/0801.2572","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:eb1ca4f1056da7daba08e90a36a6a2603ca6c8feb4179a56c0dae2127c7835ae","observation_id":"df3cc49e-498b-482e-b9e8-d48dda481e23","resolution":{"observed_at":"2026-07-04T15:34:01.524978Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0710.4620","last_updated":"2008-05-29T01:43:57Z","snapshot_observed_at":"2026-07-06T01:31:38.563418Z","submitted_at":"2007-10-25T07:06:27Z","title":"Electromagnetic Properties of the Early Universe","version":2},"cited_work":{"arxiv_id":"0710.4620","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"0710.4620","snapshot_observed_at":"2026-07-04T15:27:54.150514Z","title":null,"venue":null,"work_id":"10762e3d-5aa6-499d-a3a1-809ea2ce868f","year":2008},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/0710.4620","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:ac82dfc491f7b80af19d38833c938ad08c02974f95c351501c2da1506ebd3418","observation_id":"7cc0d538-850a-45ac-a158-4f348be01827","resolution":{"observed_at":"2026-07-04T15:27:54.150514Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807089","last_updated":"1998-07-09T09:34:05Z","snapshot_observed_at":"2026-07-07T01:21:30.222087Z","submitted_at":"1998-07-09T09:34:05Z","title":"Microwave Background Anisotropies from Alfven waves","version":1},"cited_work":{"arxiv_id":"astro-ph/9807089","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"astro-ph/9807089","snapshot_observed_at":"2026-07-04T16:06:50.451673Z","title":"Durrer, T","venue":null,"work_id":"199b5e50-13f5-420a-a702-233a8892cc8d","year":1998},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/9807089","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:c7d809038aef88606ce0ceacebedb64a5b7c8f9f234f2e36fc811b731861a844","observation_id":"6e4f9bcc-d9a7-46e5-a37e-34da7ee9aefe","resolution":{"observed_at":"2026-07-04T16:06:50.451673Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0503709","last_updated":"2005-03-31T19:23:01Z","snapshot_observed_at":"2026-07-07T00:49:27.607166Z","submitted_at":"2005-03-31T19:23:01Z","title":"Effects of Cosmological Magnetic Helicity on the Cosmic Microwave Background","version":1},"cited_work":{"arxiv_id":"astro-ph/0503709","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0503709","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Effects of Cosmological Magnetic Helicity on the Cosmic Microwave Background","venue":"astro-ph","work_id":"022ec949-d979-43c7-8dfd-e8957507df35","year":2005},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/0503709","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:dc3e9618bd28d1d0e245183919b1c9e086496e0ebd6ed64de2fb68759e980e29","observation_id":"49528a75-c686-4318-ab3c-fd08ffc4a33e","resolution":{"observed_at":"2026-05-12T07:41:53.927089Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06302","last_updated":"2022-04-13T11:09:55Z","snapshot_observed_at":"2026-07-31T04:25:52.964645Z","submitted_at":"2022-04-13T11:09:55Z","title":"Constraints on Primordial Magnetic Fields from their impact on the ionization history with Planck 2018","version":1},"cited_work":{"arxiv_id":"2204.06302","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.06302","snapshot_observed_at":"2026-07-04T04:19:34.240129Z","title":"Paoletti, J","venue":null,"work_id":"eac8fb0a-27eb-4567-b7c1-547374d1ef89","year":2022},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2204.06302","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:37fd09ccd09961090d818868c853d68f14159e706b2a1d6ac22b4d576bc25322","observation_id":"2a024235-b3e7-4a1d-a8e0-66c26eda3441","resolution":{"observed_at":"2026-05-12T07:41:57.635266Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.07456","last_updated":"2019-10-16T16:26:06Z","snapshot_observed_at":"2026-07-06T08:30:04.777443Z","submitted_at":"2019-10-16T16:26:06Z","title":"Constraints on primordial magnetic fields from magnetically-induced perturbations: current status and future perspectives with LiteBIRD and future ground based experiments","version":1},"cited_work":{"arxiv_id":"1910.07456","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1910.07456","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraints on primordial magnetic fields from magnetically-induced perturbations: current status and future perspectives with LiteBIRD and future ground based experiments","venue":null,"work_id":"0891241d-ad3e-4287-8b0e-8b0bb9eb86b4","year":2019},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1910.07456","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:53bb8f7c2981f703ee8c0e5a3d36b95974ea6bf7cae709e6b89adc6935bca662","observation_id":"ce69f5c4-0c1f-409c-9262-fa88b574d24e","resolution":{"observed_at":"2026-05-12T07:41:57.898615Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0602224","last_updated":"2009-02-19T03:11:13Z","snapshot_observed_at":"2026-07-07T00:58:15.560594Z","submitted_at":"2006-02-09T23:28:07Z","title":"Constraints on the Evolution of the Primordial Magnetic Field from the Small-Scale Cosmic Microwave Background Angular Anisotropy","version":5},"cited_work":{"arxiv_id":"astro-ph/0602224","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"astro-ph/0602224","snapshot_observed_at":"2026-07-04T15:38:13.676537Z","title":"Ichiki, T","venue":null,"work_id":"590c583d-75e6-4aed-959a-175b5af7f9ac","year":2006},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/0602224","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:6f8ab54037b959bb07b7cba85323dc971acf6afcdd212f621890730f9ed362fe","observation_id":"15ed7318-c8e2-439c-bff7-660aec5cfcdc","resolution":{"observed_at":"2026-07-04T15:38:13.676537Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.12542","last_updated":"2021-05-14T04:27:28Z","snapshot_observed_at":"2026-07-06T10:27:13.766444Z","submitted_at":"2020-12-23T08:54:06Z","title":"Small-scale CMB anisotropies induced by the primordial magnetic fields","version":2},"cited_work":{"arxiv_id":"2012.12542","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.12542","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Minoda, K","venue":null,"work_id":"e4f1c830-146a-4b54-ba47-d16335235e45","year":2021},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2012.12542","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:e5fb49d1b68f63aee72782fd8be6cbee9ef2b28264b01a5f3fab62d63308b730","observation_id":"b4ecfad7-cff8-428b-8afd-7c88ac42b4ef","resolution":{"observed_at":"2026-05-12T07:41:58.087542Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2410.03612","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"e868f639-a74a-4826-a225-1dd116e534ac","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:eb65104efdc0dc8f90126bfb706672e5e5a397df6ddf9ba1ed1b5e8caa51c670","observation_id":"ea4f8254-371a-40e2-91b4-3179726a6527","resolution":{"observed_at":"2026-05-12T07:41:57.500047Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.20707","last_updated":"2026-04-01T09:11:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-06-25T18:00:00Z","title":"SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field","version":2},"cited_work":{"arxiv_id":"2506.20707","doi":"10.1103/7wt3-","metadata_source":"pith","pith_arxiv_id":"2506.20707","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field","venue":"astro-ph.CO","work_id":"28ba80a8-b3e4-4c84-9f61-ba65da9b0aff","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2506.20707","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:d65628fb853507f009694350bfa8dbfb3c9206f53f1ccd2e4c35317409b7a900","observation_id":"cfa13bdc-c150-4fb6-8aac-ad9ca6b9b522","resolution":{"observed_at":"2026-05-13T19:11:34.300724Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2603.20163","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T19:55:33.726265Z","title":"Quan et al., SPT-3G D1: Maps of the millimeter-wave sky from 2019 and 2020 observations of the SPT-3G Main field","venue":null,"work_id":"c57c3483-3f4f-4940-8fe8-cbdf3743091d","year":2026},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:5e72d7c37a896a422c1f755e9382776bbb174dc098e6aa7de69e10c2832c7b8e","observation_id":"e0399931-9dbd-4127-a1cd-c5755d9758b6","resolution":{"observed_at":"2026-05-12T07:41:56.903624Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14452","last_updated":"2025-06-24T16:02:02Z","snapshot_observed_at":"2026-07-06T20:54:50.337775Z","submitted_at":"2025-03-18T17:30:16Z","title":"The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\\Lambda$CDM Parameters","version":2},"cited_work":{"arxiv_id":"2503.14452","doi":"10.48550/arxiv.2503.14452","metadata_source":"pith","pith_arxiv_id":"2503.14452","snapshot_observed_at":"2026-07-10T13:27:05.704436Z","title":"The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\\Lambda$CDM Parameters","venue":"astro-ph.CO","work_id":"abcbecb3-ae6f-4748-a925-133dc8647d67","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2503.14452","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:c735d3201d2b4756ec5a2fa6af9ff0aca63f38b7800cd926ce52a09e60b05c06","observation_id":"a16aca7a-f387-48dc-a80c-ca42f123e4c6","resolution":{"observed_at":"2026-05-13T14:44:49.354993Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14454","last_updated":"2025-06-24T17:02:01Z","snapshot_observed_at":"2026-07-06T20:54:50.337775Z","submitted_at":"2025-03-18T17:30:26Z","title":"The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models","version":2},"cited_work":{"arxiv_id":"2503.14454","doi":"10.48550/arxiv.2503.14454","metadata_source":"pith","pith_arxiv_id":"2503.14454","snapshot_observed_at":"2026-07-10T18:27:31.753027Z","title":"The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models","venue":"astro-ph.CO","work_id":"7d6a673d-1b44-4be4-8cb8-4500ebb3b4ea","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2503.14454","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:36d77817a5f9c25ed17280b615cca9cc3716c9055878a4bf2f87d2caee440ece","observation_id":"508b9c7f-cfc8-4e4d-ae73-87ac6cbbcc6a","resolution":{"observed_at":"2026-05-15T13:38:26.412873Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14451","last_updated":"2025-03-18T17:30:05Z","snapshot_observed_at":"2026-07-06T20:54:50.337775Z","submitted_at":"2025-03-18T17:30:05Z","title":"The Atacama Cosmology Telescope: DR6 Maps","version":1},"cited_work":{"arxiv_id":"2503.14451","doi":"10.48550/arxiv.2503.14451","metadata_source":"pith","pith_arxiv_id":"2503.14451","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"TheAtacamaCosmologyTelescope: DR6 Maps","venue":"astro-ph.CO","work_id":"71248473-8870-4aef-9eda-513a83012d8a","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2503.14451","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:5e493227d2dc8f8a3eac875634e9c4c72c0a03afab96353f75941f85d7b72fa9","observation_id":"d111db47-6bfc-4f56-a055-31c9570a5e16","resolution":{"observed_at":"2026-05-12T07:41:56.439196Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-17T20:23:18.129952+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-17T20:23:18.129952+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":"1807.06209","doi":"10.1007/jhep11(2024)108","metadata_source":"pith","pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Planck 2018 results. VI. Cosmological parameters","venue":"astro-ph.CO","work_id":"eeae0089-7b56-4c63-ace2-a31de468f6c5","year":2018},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:0add874afbe2e90deb4c6e53f731309628b942e60202669ef403118d17571f88","observation_id":"0c5ace8d-4e9f-4a08-849c-3d4a9ea708f2","resolution":{"observed_at":"2026-05-12T07:41:59.746195Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06205","last_updated":"2019-12-03T18:36:28Z","snapshot_observed_at":"2026-07-06T06:50:35.226504Z","submitted_at":"2018-07-17T04:05:03Z","title":"Planck 2018 results. I. Overview and the cosmological legacy of Planck","version":2},"cited_work":{"arxiv_id":"1807.06205","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.06205","snapshot_observed_at":"2026-07-10T17:27:26.831303Z","title":"Planck 2018 results. I. Overview and the cosmological legacy of Planck","venue":"astro-ph.CO","work_id":"1d3770c7-d723-44a6-827d-4d71ce851971","year":2018},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1807.06205","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:5e3836c47383e61174665f472720ddad300b57624092bc7333169f2d3cfbed82","observation_id":"b057dad2-124c-4c20-b61c-2a4cdc2f6372","resolution":{"observed_at":"2026-05-16T20:50:20.049987Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.05748","last_updated":"2020-04-22T05:03:17Z","snapshot_observed_at":"2026-07-06T08:29:07.404994Z","submitted_at":"2019-10-13T13:26:52Z","title":"Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data","version":2},"cited_work":{"arxiv_id":"1910.05748","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1910.05748","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data","venue":null,"work_id":"e6409076-1551-4daa-86c3-4b4d0e26f153","year":2020},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1910.05748","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:2fc257aa17adce2297ddc319ce2991eeafd1f4fa20b2360cbdbdc3bcebcd3a84","observation_id":"08cc7b62-6589-422a-a4e5-72253f0690f7","resolution":{"observed_at":"2026-05-12T07:41:59.580153Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.07928","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Balkenhol, A","venue":null,"work_id":"29b83b8b-24c8-4403-81a8-83e37ad2719a","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:64810411e991bc92a7c4fe5e78ddf9dd2595ce697cb584907a74c352c735f19d","observation_id":"82d41d16-60d8-4031-a48b-cf234a123ac6","resolution":{"observed_at":"2026-05-12T07:42:00.748732Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2110.00483","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T18:06:25.747917Z","title":"Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season","venue":null,"work_id":"c300ef56-0a67-4b69-a4ec-9f7c0970b2ca","year":1998},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:c6fb565597fac08757d908b41b5920acaaac51da7dd7be678cf275ec75167200","observation_id":"517468d4-54bc-4be0-8a56-741313d56612","resolution":{"observed_at":"2026-05-12T07:42:00.317086Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9508078","last_updated":"1996-10-25T14:05:17Z","snapshot_observed_at":"2026-07-07T01:11:44.541828Z","submitted_at":"1995-08-17T15:19:23Z","title":"Reconstructing the Inflaton Potential --- an Overview","version":3},"cited_work":{"arxiv_id":"astro-ph/9508078","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9508078","snapshot_observed_at":"2026-07-03T13:08:08.223539Z","title":"Reconstructing the Inflaton Potential --- an Overview","venue":"astro-ph","work_id":"79508e95-a0a1-47e1-9c52-0b0d81b752a3","year":1995},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/9508078","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:5a8fb5b11de0a9fff7308a91e1d8de85c8411eb2d57f38038b6dce00959fee1b","observation_id":"da87bb2b-2fb8-4fea-8430-a8f21db4437b","resolution":{"observed_at":"2026-05-12T07:41:56.307687Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0403583","last_updated":"2004-06-04T13:50:43Z","snapshot_observed_at":"2026-07-07T00:41:32.180049Z","submitted_at":"2004-03-24T20:54:39Z","title":"Observable primordial vector modes","version":3},"cited_work":{"arxiv_id":"astro-ph/0403583","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0403583","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Observable primordial vector modes","venue":"astro-ph","work_id":"96128296-ea06-440e-a335-149e2000c5cf","year":2004},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/0403583","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:b5c0686b08e4172e2f4e4e958636b6f7b58534a2dc8ebce00c20ee9345d2454e","observation_id":"601ffe49-f2b3-4d7c-8f7a-b38f3d21a6f3","resolution":{"observed_at":"2026-05-13T17:48:12.169977Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1112.4705","last_updated":"2011-12-20T14:36:58Z","snapshot_observed_at":"2026-07-06T02:39:44.077492Z","submitted_at":"2011-12-20T14:36:58Z","title":"Constraint on the primordial vector mode and its magnetic field generation from seven-year Wilkinson Microwave Anisotropy Probe Observations","version":1},"cited_work":{"arxiv_id":"1112.4705","doi":null,"metadata_source":"pith","pith_arxiv_id":"1112.4705","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraint on the primordial vector mode and its magnetic field generation from seven-year Wilkinson Microwave Anisotropy Probe Observations","venue":"astro-ph.CO","work_id":"a5a3f9a7-858b-4906-844f-4fb36e0c382c","year":2011},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1112.4705","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:4a139bcebcaea3f20086670705946390ee057564242c1f2a8bf1cea9a55261e6","observation_id":"406fab26-1dfc-4a3c-a5cb-e8bf72fd3f26","resolution":{"observed_at":"2026-05-12T07:42:01.480879Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"d97c564e-9586-4325-9659-7e14b499af68","year":1992},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:4d4f70a1698a231896968c92fccd3b7adf719772ec83aea5de8ef987aeb3b68f","observation_id":"fccfebc4-e532-4731-b652-d5b185641497","resolution":{"observed_at":"2026-05-12T23:26:57.212199Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9403032","last_updated":"1994-03-16T12:57:39Z","snapshot_observed_at":"2026-07-07T03:24:35.902776Z","submitted_at":"1994-03-16T12:57:39Z","title":"Kinetic vs. Thermal-Field-Theory Approach to Cosmological Perturbations","version":1},"cited_work":{"arxiv_id":"gr-qc/9403032","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9403032","snapshot_observed_at":"2026-07-02T00:36:24.047117Z","title":"Kinetic vs. Thermal-Field-Theory Approach to Cosmological Perturbations","venue":"gr-qc","work_id":"e1d800ca-b3d4-42f6-a948-aa11fc5098d1","year":1994},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/gr-qc/9403032","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:705593cf64fcbfeb49dc77bef3d99f17dea51ca93f02c6807309584e7a1d5327","observation_id":"e0b29446-fb50-4cea-855e-675e9cb5c37a","resolution":{"observed_at":"2026-05-12T07:41:56.097073Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0110348","last_updated":"2001-11-01T16:34:23Z","snapshot_observed_at":"2026-07-07T00:22:22.199214Z","submitted_at":"2001-10-16T14:45:42Z","title":"Cosmic Structure Formation with Topological Defects","version":2},"cited_work":{"arxiv_id":"astro-ph/0110348","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0110348","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cosmic Structure Formation with Topological Defects","venue":"astro-ph","work_id":"de531848-8269-457f-b1d6-4ed2ced1c889","year":2001},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/astro-ph/0110348","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:00804dd9f3f134f26ffaa4cbf6dae450c1cf8cd9a004cd5d796e5b901ff9d0f3","observation_id":"a2d32894-82ef-4683-8485-271be90168f3","resolution":{"observed_at":"2026-05-12T07:41:55.576923Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.12875","last_updated":"2020-09-15T15:02:27Z","snapshot_observed_at":"2026-07-06T08:11:09.285762Z","submitted_at":"2019-07-30T13:11:32Z","title":"Planck 2018 results. V. CMB power spectra and likelihoods","version":2},"cited_work":{"arxiv_id":"1907.12875","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.12875","snapshot_observed_at":"2026-07-10T18:27:31.377687Z","title":"Planck 2018 results. V. CMB power spectra and likelihoods","venue":"astro-ph.CO","work_id":"b5433e4f-7783-4472-a549-bdc3a40bb515","year":2019},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1907.12875","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:e0cfd8c5b7cc9f00a2a5825b72fd6568f57020c6010e2096e91ca6491e212d33","observation_id":"258ae9df-4e1a-46d0-8a3e-64df080667cc","resolution":{"observed_at":"2026-05-15T21:56:29.613337Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J., et al., Planck intermediate results - LVII","venue":null,"work_id":"55a120bf-31f4-43d0-a939-408798d3c422","year":2020},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:496bf156d966b4ccb3ae207d135954ee86af6e4d5adb61a8ce95228301778ed7","observation_id":"3c298e7d-11ec-48cc-99e3-3a6d243cd0d0","resolution":{"observed_at":"2026-05-12T23:26:57.179247Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.13433","last_updated":"2024-03-27T17:00:08Z","snapshot_observed_at":"2026-07-06T17:19:52.125879Z","submitted_at":"2024-01-24T13:05:43Z","title":"candl: Cosmic Microwave Background Analysis with a Differentiable Likelihood","version":3},"cited_work":{"arxiv_id":"2401.13433","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2401.13433","snapshot_observed_at":"2026-07-03T06:27:41.798508Z","title":"Balkenhol, C","venue":null,"work_id":"fee1413a-9a0d-4828-9f0b-afcc5365537b","year":2024},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2401.13433","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:7a861b2288d8fb2531e225e27d1661bd2830a1066da9e15ccdf231915a360d24","observation_id":"10ae335a-9ac4-4bb2-915e-d613bab347b5","resolution":{"observed_at":"2026-05-12T07:41:55.820104Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1301.0776","last_updated":"2013-10-08T11:54:58Z","snapshot_observed_at":"2026-07-06T03:03:17.807263Z","submitted_at":"2013-01-04T17:25:40Z","title":"The Atacama Cosmology Telescope: likelihood for small-scale CMB data","version":2},"cited_work":{"arxiv_id":"1301.0776","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1301.0776","snapshot_observed_at":"2026-07-04T20:04:17.883714Z","title":"Dunkley et al., The Atacama Cosmology Telescope: likelihood for small-scale CMB data, JCAP 07 (2013) 025, [ arXiv:1301.0776]","venue":null,"work_id":"d5d0654a-37d5-47bb-bd0b-635b57234ca6","year":2013},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1301.0776","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:38ea06c3f3e5a5da2e6e37729cbee169efc279a57de546769a244379626aa7cf","observation_id":"bd9a23f6-174c-4159-b569-ac92b29fae37","resolution":{"observed_at":"2026-07-04T20:04:17.883714Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.00826","last_updated":"2025-02-17T15:39:51Z","snapshot_observed_at":"2026-07-06T19:59:42.424537Z","submitted_at":"2024-12-01T14:27:41Z","title":"Compressed 'CMB-lite' Likelihoods Using Automatic Differentiation","version":2},"cited_work":{"arxiv_id":"2412.00826","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.00826","snapshot_observed_at":"2026-07-03T06:27:41.714632Z","title":"Balkenhol, Compressed ’CMB-lite’ Likelihoods Using Automatic Differentiation","venue":null,"work_id":"72a009d2-76c8-4b72-a56c-5bdd42ddba6c","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2412.00826","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:62098c9753ddd856438b233db3b3e454f5df38c1cebf3e7e4bd2e400068d2c82","observation_id":"d4dceadc-2c6a-4497-85c9-a32396513613","resolution":{"observed_at":"2026-05-12T07:41:57.717061Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2932","last_updated":"2011-05-14T09:45:16Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-14T22:06:14Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview","version":2},"cited_work":{"arxiv_id":"1104.2932","doi":"10.48550/arxiv.1104.2932","metadata_source":"pith","pith_arxiv_id":"1104.2932","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview","venue":"astro-ph.IM","work_id":"c0bf8a51-3605-4e2d-a4ba-d6e206f32bf7","year":2011},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1104.2932","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:9ac8d984c428fc37e522e2acc1ac251923f1f7a2429d4e41db34976ac1177c6e","observation_id":"9c93d1ea-293d-437b-983c-bc4f65acddd8","resolution":{"observed_at":"2026-05-12T07:41:59.133330Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2933","last_updated":"2011-08-17T09:25:04Z","snapshot_observed_at":"2026-07-06T02:26:22.184733Z","submitted_at":"2011-04-14T22:06:43Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes","version":3},"cited_work":{"arxiv_id":"1104.2933","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2933","snapshot_observed_at":"2026-07-10T23:17:44.110601Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes","venue":"astro-ph.CO","work_id":"a5df2b88-b84f-4a1c-a8a7-7de010e312e1","year":2011},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1104.2933","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:21dfa95954cb08c455054be3208d76967dbd1ed9cafbff65129e73434f838763","observation_id":"d62531fd-4cc0-4862-ac93-a0ce0000957a","resolution":{"observed_at":"2026-05-13T19:06:18.978333Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.05290","last_updated":"2021-05-20T11:52:55Z","snapshot_observed_at":"2026-08-03T14:56:09.086229Z","submitted_at":"2020-05-11T17:49:03Z","title":"Cobaya: Code for Bayesian Analysis of hierarchical physical models","version":2},"cited_work":{"arxiv_id":"2005.05290","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.05290","snapshot_observed_at":"2026-07-10T18:27:31.369804Z","title":"Cobaya: Code for Bayesian Analysis of hierarchical physical models","venue":"astro-ph.IM","work_id":"579c5ab4-f42d-4271-a145-ce28660998d9","year":2020},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2005.05290","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:9d39d07c5c7eb7e75cd871139eb02fa07c4248b600407216f1e70e1aec82d1b8","observation_id":"3472faa9-0bdb-49e6-9daa-41f81a9814e9","resolution":{"observed_at":"2026-05-14T21:57:22.456194Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cobaya: Bayesian analysis in cosmology","venue":null,"work_id":"b273ece9-c094-494d-95c7-377ebb6cae1e","year":1910},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:46cf65c38633e8ae12db7d1dac4cfd3fefb73f44d74e7c78a058bfddd3c25af2","observation_id":"f5f2cb40-7bb7-46e1-836b-8aa5e3545e2e","resolution":{"observed_at":"2026-05-12T23:26:57.175285Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Rubin, Inference from iterative simulation using multiple sequences, Statistical Science 7 (1992), no","venue":null,"work_id":"375592fa-356a-4dff-b8f3-1a9a1994c314","year":1992},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:9379a3caf5ef8de67fc3b617ba4048a4d9fa040dd906869aa4ccae4698a074f1","observation_id":"8081eea8-3a1e-4c2c-9bdd-00c58a4d1f74","resolution":{"observed_at":"2026-05-12T23:26:57.183349Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.00154","last_updated":"2018-05-22T19:04:57Z","snapshot_observed_at":"2026-07-06T06:31:09.803040Z","submitted_at":"2018-03-31T10:49:24Z","title":"Improving the Flexibility and Robustness of Model-Based Derivative-Free Optimization Solvers","version":2},"cited_work":{"arxiv_id":"1804.00154","doi":"10.48550/arxiv.1804","metadata_source":"pith","pith_arxiv_id":"1804.00154","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Improving the Flexibility and Robustness of Model-Based Derivative-Free Optimization Solvers","venue":"math.OC","work_id":"a099f3dc-50fe-450c-9ef7-feeff5b343c1","year":2018},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1804.00154","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:c269179d38b8d2f623e1f261bd2b531525af7b680778fb8d1f56952409e2408d","observation_id":"7ad6833a-1b9d-4175-8ca5-73f24ea61a00","resolution":{"observed_at":"2026-05-12T07:41:54.362264Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1812.11343","last_updated":"2019-10-10T01:00:43Z","snapshot_observed_at":"2026-07-06T07:24:01.798514Z","submitted_at":"2018-12-29T11:36:55Z","title":"Escaping local minima with derivative-free methods: a numerical investigation","version":2},"cited_work":{"arxiv_id":"1812.11343","doi":"10.48550/arxiv.1812.11343","metadata_source":"arxiv_reference","pith_arxiv_id":"1812.11343","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Escap- ing local minima with derivative-free methods: a numeri- cal investigation","venue":null,"work_id":"ed542df2-e1a4-4546-8abf-d0f13cc35dc4","year":2021},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1812.11343","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:d0e39478ccb42d47e361202309e6bf86fe22ee478d43420a0b95cf298f6004b1","observation_id":"d226327b-65e2-486e-bde2-bef32a46a000","resolution":{"observed_at":"2026-05-12T07:41:54.624415Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.02972","last_updated":"2024-12-09T12:11:12Z","snapshot_observed_at":"2026-08-02T03:59:52.449814Z","submitted_at":"2023-12-05T18:58:52Z","title":"PROSPECT: A profile likelihood code for frequentist cosmological parameter inference","version":3},"cited_work":{"arxiv_id":"2312.02972","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.02972","snapshot_observed_at":"2026-07-04T17:39:59.596651Z","title":null,"venue":null,"work_id":"25608b19-2aa2-40b7-9e15-47f62cf684af","year":2024},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2312.02972","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:242339635dfdef2a33a7ef07b07c2a694e35b6c851cfcba5f898394e738052e9","observation_id":"2a86ef03-d31a-403b-8d4b-0bd2d316da08","resolution":{"observed_at":"2026-05-12T07:41:58.816419Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.4810","last_updated":"2014-09-11T01:04:00Z","snapshot_observed_at":"2026-07-06T03:44:06.612548Z","submitted_at":"2014-05-19T17:07:41Z","title":"Constraining primordial vector mode from B-mode polarization","version":2},"cited_work":{"arxiv_id":"1405.4810","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.4810","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraining primordial vector mode from B-mode polarization","venue":"astro-ph.CO","work_id":"6c4631b0-dfe0-4dd3-8252-5dca98c9d001","year":2014},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1405.4810","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:1d453043639e53bf6e6e73345165d3f155d4c874769fbf543856c5a99abf604f","observation_id":"ac2ce202-a222-47d6-9a9e-b188185041cd","resolution":{"observed_at":"2026-05-12T07:42:01.119350Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.04739","last_updated":"2017-01-13T14:49:02Z","snapshot_observed_at":"2026-07-06T05:10:56.995845Z","submitted_at":"2016-09-15T17:13:36Z","title":"Shortcomings of New Parametrizations of Inflation","version":2},"cited_work":{"arxiv_id":"1609.04739","doi":"10.1103/physrevd.94.123521","metadata_source":"pith","pith_arxiv_id":"1609.04739","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Shortcomings of New Parametrizations of Inflation","venue":"astro-ph.CO","work_id":"a93714d7-78ee-4d2d-aad6-50379f96f3cb","year":2016},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1609.04739","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:731acbf097221e23df373863b7fd5639c3c289caa46a23147adb494dbba60528","observation_id":"d111fb8b-2db8-432b-ba40-f61ebc5cdfb0","resolution":{"observed_at":"2026-05-12T07:42:01.170330Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2505.01129","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T18:06:25.869065Z","title":"Reheat- ing ACTs on Starobinsky and Higgs inflation","venue":null,"work_id":"75b8a8c4-fa20-4e85-81e9-52ee3edd16b7","year":2025},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:36bf53c92e18e3ba4e1ab5c26e953021baf193af7fee72e955bc15393e5cfc54","observation_id":"98a8628c-731a-4aae-88ea-1a0c109f53a8","resolution":{"observed_at":"2026-05-12T07:42:01.028354Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2101.12449","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-01T17:45:51.565985Z","title":"Hazumi et al., LiteBIRD: JAXA’s new strategic L-class mission for all-sky surveys of cosmic microwave background polarization , Proc","venue":null,"work_id":"8cdd01ca-3a7f-475f-9cda-5d259016a126","year":2020},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:e71f5f2b946c5ca29ad230697d86796e312c34893284737bd7c265bfa4bd423b","observation_id":"f474b69c-e2bd-43c9-8164-1129744237f3","resolution":{"observed_at":"2026-05-12T07:42:01.323228Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.02773","last_updated":"2023-03-27T05:15:34Z","snapshot_observed_at":"2026-08-03T11:16:50.074816Z","submitted_at":"2022-02-06T13:17:44Z","title":"Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey","version":3},"cited_work":{"arxiv_id":"2202.02773","doi":null,"metadata_source":"pith","pith_arxiv_id":"2202.02773","snapshot_observed_at":"2026-07-09T05:46:01.322091Z","title":"Allys, K","venue":"astro-ph.IM","work_id":"fb7c4dd0-9fb3-43df-a09d-852e8f10feff","year":2022},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2202.02773","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:0c7ce12dc519f45cd57260638d49f5885ae59b9c62a1f714f4ebe074f391779e","observation_id":"9bfaa2a5-1ce3-442c-b445-89e33af642bb","resolution":{"observed_at":"2026-05-12T07:42:01.079526Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.04047","last_updated":"2020-12-07T20:43:38Z","snapshot_observed_at":"2026-07-06T10:21:36.540391Z","submitted_at":"2020-12-07T20:43:38Z","title":"Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole","version":1},"cited_work":{"arxiv_id":"2012.04047","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.04047","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole","venue":null,"work_id":"71c44b14-978b-42d3-a102-94d524c501da","year":2020},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/2012.04047","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:e2b4f191bc085482a8f1fed8909547e0fc080d56b84c7780dc7ede8c6a627464","observation_id":"527066d4-7589-4341-a859-17a663eec436","resolution":{"observed_at":"2026-05-12T07:42:00.285577Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2405.19469","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T19:35:01.271075Z","title":null,"venue":null,"work_id":"10b28d17-d2e5-4a8b-a708-db10d98fcce9","year":2024},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:460d6f5730bf9eafbc3297ba462e20974d4b872d3c544b56128b119a92c24582","observation_id":"0c4bd031-5ad5-4ce5-a49f-493cfea72cdd","resolution":{"observed_at":"2026-05-12T07:41:57.574350Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1106.3744","last_updated":"2012-04-03T13:46:47Z","snapshot_observed_at":"2026-07-06T02:29:32.132412Z","submitted_at":"2011-06-19T13:24:05Z","title":"Anomaly-free vector perturbations with holonomy corrections in loop quantum cosmology","version":2},"cited_work":{"arxiv_id":"1106.3744","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1106.3744","snapshot_observed_at":"2026-07-04T18:03:57.795796Z","title":null,"venue":null,"work_id":"fff9a8bb-fab9-4877-82e6-ea4b2392809e","year":2012},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1106.3744","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:5973a26ff727fc24882b591c72669b5bdda76e39970c10afff3072efb643e1da","observation_id":"d85d3cc6-69aa-42e2-809b-feb92e86f946","resolution":{"observed_at":"2026-07-04T18:03:57.795796Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1004.3962","last_updated":"2010-09-09T09:55:46Z","snapshot_observed_at":"2026-07-06T02:09:38.416009Z","submitted_at":"2010-04-22T17:08:31Z","title":"Brane-World Gravity","version":2},"cited_work":{"arxiv_id":"1004.3962","doi":"10.12942/lrr-2010-5","metadata_source":"pith","pith_arxiv_id":"1004.3962","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Maartens and K","venue":"hep-th","work_id":"c30ffa5a-cccb-4476-93fd-d0e721607ef8","year":2010},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/1004.3962","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:07b88f782cf4415e6af3713a2473a83669b5e11afb9e764192b73d836d28a6a4","observation_id":"16bb4918-e452-4eaf-8482-3379ee850ea4","resolution":{"observed_at":"2026-05-12T07:42:00.200745Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0802.2068","last_updated":"2008-06-10T13:37:46Z","snapshot_observed_at":"2026-07-06T01:36:37.143696Z","submitted_at":"2008-02-14T17:59:45Z","title":"Vector Inflation","version":3},"cited_work":{"arxiv_id":"0802.2068","doi":null,"metadata_source":"pith","pith_arxiv_id":"0802.2068","snapshot_observed_at":"2026-06-29T11:03:18.326600Z","title":"Vector Inflation","venue":"astro-ph","work_id":"9830b359-3bac-4fc9-938b-6fe5f51e34fd","year":2008},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/0802.2068","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:ead7de98f9e8dd2ffb4216653f1b4c8907374f54d91d0cf179e848cfa6e83009","observation_id":"4c5e8e05-079a-44b0-9e95-edb79232a6de","resolution":{"observed_at":"2026-05-12T07:42:00.430147Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0903.2977","last_updated":"2009-05-14T09:46:32Z","snapshot_observed_at":"2026-07-06T01:51:47.702893Z","submitted_at":"2009-03-17T15:11:02Z","title":"Cosmological perturbations from vector inflation","version":2},"cited_work":{"arxiv_id":"0903.2977","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"0903.2977","snapshot_observed_at":"2026-07-04T15:47:02.624481Z","title":null,"venue":null,"work_id":"ebe1d463-e066-4804-afaa-58ad7ebc53e8","year":2009},"citing_paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-05-12T02:17:22.022693Z"},"links":{"cited_paper":"/paper/0903.2977","citing_paper":"/paper/2605.08907"},"observation_digest":"sha256:8311a517656a500e1b4b977a9c47cd59958c7f640f3fcf223a5976be525e291e","observation_id":"984a1a47-68b7-40f6-b635-b47cac7fe8f4","resolution":{"observed_at":"2026-07-04T15:47:02.624481Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2605.08907","last_updated":"2026-05-09T12:05:35Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T23:21:06.773761Z","submitted_at":"2026-05-09T12:05:35Z","title":"The Status of Gravitational Vector Perturbations with Recent CMB Data"},"reference_resolution":{"displayed":63,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":2,"verified_exact":52,"verified_fuzzy":7},"total_outbound_references":63},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 63 of 63 outbound references and 2 inbound Pith citation observations for arXiv:2605.08907."}