{"as_of":"2026-08-18T01:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9c12705daf462031f67ef8607ce97030c720226b7cc00dee402742a09a732e2b","coverage":[{"denominator":16,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":16,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T19:17:09.334748Z","state":"measured"},{"denominator":21,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":21,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T14:36:18.294784Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"cited_work":{"arxiv_id":"2412.07068","doi":"10.48550/arxiv.2412.07068","metadata_source":"arxiv_reference","pith_arxiv_id":"2412.07068","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Atkinset al., J","venue":"arXiv (Cornell University)","work_id":"a5977c9f-0df4-42bc-bc4d-9fef9e4f7ec8","year":2025},"citing_paper":{"arxiv_id":"2506.20707","last_updated":"2026-04-01T09:11:02Z","snapshot_observed_at":"2026-08-15T07:17:40.349249Z","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},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-13T19:11:25.985677Z"},"links":{"cited_paper":"/paper/2412.07068","citing_paper":"/paper/2506.20707"},"observation_digest":"sha256:21df54c0a56faa4a7ec3124b54f0d4c1283dec1047f227570bfcac146cda2541","observation_id":"fe127be5-99c6-4480-b1dd-258607b356b5","resolution":{"observed_at":"2026-05-13T19:11:27.499480Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"cited_work":{"arxiv_id":"2412.07068","doi":"10.48550/arxiv.2412.07068","metadata_source":"arxiv_reference","pith_arxiv_id":"2412.07068","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Atkinset al., J","venue":"arXiv (Cornell University)","work_id":"a5977c9f-0df4-42bc-bc4d-9fef9e4f7ec8","year":2025},"citing_paper":{"arxiv_id":"2509.13654","last_updated":"2026-04-14T13:07:43Z","snapshot_observed_at":"2026-08-16T23:32:32.859370Z","submitted_at":"2025-09-17T02:59:36Z","title":"Cosmic Birefringence from the Atacama Cosmology Telescope Data Release 6","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-18T16:55:42.473876Z"},"links":{"cited_paper":"/paper/2412.07068","citing_paper":"/paper/2509.13654"},"observation_digest":"sha256:87cb6024809ead3cb58d9496e8a34bdab9ddc9f698d5ff5f117bda1054337d6e","observation_id":"41343699-4c1c-4799-bf52-7779979745ed","resolution":{"observed_at":"2026-05-18T16:56:38.149094Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"cited_work":{"arxiv_id":"2412.07068","doi":"10.48550/arxiv.2412.07068","metadata_source":"arxiv_reference","pith_arxiv_id":"2412.07068","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Atkinset al., J","venue":"arXiv (Cornell University)","work_id":"a5977c9f-0df4-42bc-bc4d-9fef9e4f7ec8","year":2025},"citing_paper":{"arxiv_id":"2509.23123","last_updated":"2026-04-05T17:24:58Z","snapshot_observed_at":"2026-08-16T21:28:14.046487Z","submitted_at":"2025-09-27T05:04:57Z","title":"Constraining Inflationary Particle Production with CMB Polarization","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-18T13:04:29.105646Z"},"links":{"cited_paper":"/paper/2412.07068","citing_paper":"/paper/2509.23123"},"observation_digest":"sha256:403244187a958b4b4a34b2a1b0ce75d7bf4f049ab155ec66c8494d5a48356395","observation_id":"2716d834-bbb1-483c-a15c-d3d1495dd9ad","resolution":{"observed_at":"2026-05-18T13:06:23.724177Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.07068","snapshot_observed_at":"2026-08-02T00:58:36.547925Z","title":"Atkins, Z","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.14843","last_updated":"2026-07-16T11:11:17Z","snapshot_observed_at":"2026-08-17T19:24:11.081975Z","submitted_at":"2026-07-16T11:11:17Z","title":"Analytical covariances for catalogue-based pseudo-$C_\\ell$s","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-02T00:58:36.547925Z"},"links":{"cited_paper":"/paper/2412.07068","citing_paper":"/paper/2607.14843"},"observation_digest":"sha256:4861378dcc72fb7e5af566a3ab1645aff2ff40176ba8cc3c70827fb177f61d9a","observation_id":"0bb93b1f-2447-4242-a143-d42f301175ed","resolution":{"observed_at":"2026-08-02T00:58:36.547925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.07068","snapshot_observed_at":"2026-08-15T14:36:18.294784Z","title":"Atkinset al., JCAP05, 015, arXiv:2412.07068 [astro- ph.CO]","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2608.06480","last_updated":"2026-08-06T18:18:46Z","snapshot_observed_at":"2026-08-16T23:33:24.047252Z","submitted_at":"2026-08-06T18:18:46Z","title":"Cosmic birefringence from a joint analysis of ACT and Planck","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T14:36:18.294784Z"},"links":{"cited_paper":"/paper/2412.07068","citing_paper":"/paper/2608.06480"},"observation_digest":"sha256:f0a6669a61661a36bd333afc2f2af41b8fb7bbe4cdd61cd177030613654e91b1","observation_id":"095055fe-1bb9-4a8f-af07-d0706cd0b064","resolution":{"observed_at":"2026-08-15T14:36:18.294784Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2412.07068/citation-record","integrity":"/paper/2412.07068/integrity","json":"/paper/2412.07068/citation-record.json","paper":"/paper/2412.07068"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:08.685189Z","title":"2020, JCAP, 2020, 47, doi: 10.1088/1475-7516/2020/12/047 Alonso, D., Fabbian, G., Storey-Fisher, K., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:08.685189Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:1925a03b5c603c07aeed8f3cef32a384f35f10d9c5942b183c7a81d490f3be8d","observation_id":"f4daab10-9dfe-419d-946a-2c9ac30bbf76","resolution":{"observed_at":"2026-08-11T19:17:08.685189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:11.754829Z","title":"−−” couplings are small compared to “++","venue":null,"work_id":"2ead7ea5-806f-43c0-baa8-ffc0659307c1","year":2017},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:08.974740Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:4c04ac3bff051330f06f6a0e42714b6c3e76e92d506fe120e4dc6bd714ffbafe","observation_id":"bc1deebc-a087-48c5-a10c-87f9a01db472","resolution":{"observed_at":"2026-08-11T19:17:11.794736Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:11.064737Z","title":null,"venue":null,"work_id":"da4f24df-bfc7-49de-ad1a-b176024402e7","year":2020},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.144748Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:bd3cb89b87ac22975f78b00af81ce13eb1fa8dc51eb9332712865e4f9c7d024f","observation_id":"a27c290e-6051-436b-b894-518b466fe23a","resolution":{"observed_at":"2026-08-11T19:17:11.114739Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:12.036003Z","title":null,"venue":null,"work_id":"6f69f1f0-cfea-4095-8f86-19870793d1b1","year":2016},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:08.864744Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:6424cc5c005e2a37adf8fdaba89a4fa804f22967fa7550d2eb54bb2045defac6","observation_id":"910dc3f5-6328-4ea2-989c-d4a12f4e7512","resolution":{"observed_at":"2026-08-11T19:17:12.074743Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:11.894737Z","title":"(B10) Because ˜a is Gaussian, we expand the product of four fields using Wick’s theorem","venue":null,"work_id":"8e910ab7-154d-4287-9a80-638002da808e","year":2004},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:08.914734Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:a229eb7af8c3abdd93e88206955c293e020129f65b1d793bdc5666039451357c","observation_id":"043c551b-a515-4d34-83c9-d18578251bdf","resolution":{"observed_at":"2026-08-11T19:17:11.936564Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:11.515008Z","title":"pseudospectrum","venue":null,"work_id":"3f2ef516-17d2-4d09-9522-a8c82cf35984","year":1995},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.021275Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:fad50bcf95383e9e13d0cf203d70ac14f835714e46da7b73f0299f72abdfc5ac","observation_id":"85eabf74-b377-4f08-85f5-fa3fae2864e8","resolution":{"observed_at":"2026-08-11T19:17:11.574748Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:11.354744Z","title":"27 When there is a mask in addition to a harmonic-space filter, these expressions become inexact","venue":null,"work_id":"bc97a855-46fd-480e-ace0-cf0e12367117","year":2000},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.064817Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:dedea089e747c39610a3cafdad92d7f9bdb14430d735551845db3a2187843613","observation_id":"1002c5b6-4ef2-48b3-bb54-e3c793c08cc2","resolution":{"observed_at":"2026-08-11T19:17:11.394826Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:12.194743Z","title":"A field that follows the model of Equation 9 has zero mean and is Gaussian, so its statistics are fully specified by its covariance","venue":null,"work_id":"b0ca246e-a02b-4d31-ad15-86c733c96091","year":2004},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:08.814781Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:a1b409a2d1358cf44be27c4ab1d31158a44b7ee4b7cc091ec5ad0d73cf5e2d9a","observation_id":"d7937df9-7600-4e29-9944-1bf5a44f3d91","resolution":{"observed_at":"2026-08-11T19:17:12.234741Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:11.204737Z","title":"representative","venue":null,"work_id":"7a8fabfb-94e0-4c33-a7b7-69fbec8031db","year":2020},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.108704Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:27ad695e95c74bcd26362a0ba7e7340e7b07e5b48af32ffd6480cc3f4829af52","observation_id":"8a9c4044-1638-4cf1-ac74-750f07fd2f8d","resolution":{"observed_at":"2026-08-11T19:17:11.254744Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:10.564752Z","title":"Left: In the case that the simulation-based correction only smooths the main diagonal of ΣR","venue":null,"work_id":"e05b7cc7-152d-4f8f-bf91-0a9a9713c3ab","year":2004},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.246272Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:41cbd7e03f79a61d88d640d264abfaf584b79b62fd30bee076e2ff2200504430","observation_id":"fa5636dd-29dd-4c04-bbdf-dde2856a296d","resolution":{"observed_at":"2026-08-11T19:17:10.605895Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:10.403644Z","title":"For each polarization combination, the power spectrum variance increases when point-source holes are added to the mask, as expected","venue":null,"work_id":"d1700b79-5d0c-4c06-9f74-53dd33e08771","year":2000},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.290773Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:3d5aed46b487eb5fad82ba906c6380b068aef4b5686e87ae5ab8c1e8312b8d1f","observation_id":"665adb29-d9ce-4a7c-a08c-c12ddcbec78b","resolution":{"observed_at":"2026-08-11T19:17:10.454905Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:10.224748Z","title":"Thus, as is evident in Figure 15, both cases share the same statistical fluctuations, further facilitating a direct comparison","venue":null,"work_id":"cb8bc54a-b1f8-4fbd-96b1-a7867e8f6aa5","year":2016},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.334748Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:6200bd732364dfeb5735fe41703377df5d064e215e09996391e985aaee311dcd","observation_id":"7b0415d8-1230-48bd-953f-124934f64604","resolution":{"observed_at":"2026-08-11T19:17:10.274750Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"stable/2983768","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:09.763019Z","title":null,"venue":null,"work_id":"fcf8f0a6-f6fe-45f6-a629-e1a5ae1f3ec9","year":2007},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":193,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:08.772913Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:44caa6636a1e5efb91c00152112a41ecd9f54dda225881bbbcc8487a2d457dd8","observation_id":"3ad12064-c351-4068-942c-4c4fc3a8050a","resolution":{"observed_at":"2026-08-11T19:17:09.854789Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:10.904748Z","title":"(2023) for this model","venue":null,"work_id":"8e7d5851-6cb0-4c4b-bca2-f5e628d3ece0","year":2023},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":500,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.188013Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:016e574bdd2fa55dd4fe9fc83c41e197a11e61bd1359548e781e96918d7a3062","observation_id":"5147db03-dafb-4c17-a415-f7c7b5f1cf4b","resolution":{"observed_at":"2026-08-11T19:17:10.944747Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:10.744746Z","title":null,"venue":null,"work_id":"2672ad86-dea2-4a06-b35c-605ac6c4b73b","year":2000},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":1763,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:09.225022Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:863686886a9594946955d937ec62ae8fa41d2cd15c758e5252495ebebeb20e9f","observation_id":"1045b596-75c0-4783-894e-623c94f7216c","resolution":{"observed_at":"2026-08-11T19:17:10.784743Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.59508","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:17:09.484743Z","title":"M., Hivon, E., Banday, A","venue":null,"work_id":"bb7b1f67-8661-4dd7-8357-11fcb9b7858d","year":2005},"citing_paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra","version":1},"reference_index":2016,"source":"pdf_text","source_observed_at":"2026-08-11T19:17:08.714745Z"},"links":{"citing_paper":"/paper/2412.07068"},"observation_digest":"sha256:2219f9ab8f25f3812346ea0fc1f43b46f86ccd7182ffe0c1f4b5489e19fb3cab","observation_id":"55a26300-7e22-4cda-ac01-b06e79a19c8d","resolution":{"observed_at":"2026-08-11T19:17:09.534746Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.07068","last_updated":"2024-12-10T00:20:24Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T20:00:20.465498Z","submitted_at":"2024-12-10T00:20:24Z","title":"The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra"},"reference_resolution":{"displayed":16,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":4,"verified_exact":2,"verified_fuzzy":10},"total_outbound_references":16},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 16 of 16 outbound references and 5 inbound Pith citation observations for arXiv:2412.07068."}