{"as_of":"2026-08-15T02:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b17689e6e023102d4a118c93c6954bbadf5acd91daf55cf81abe1065063fec81","coverage":[{"denominator":68,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":68,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:57:34.166527Z","state":"measured"},{"denominator":68,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":68,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/1908.08057/citation-record","integrity":"/paper/1908.08057/integrity","json":"/paper/1908.08057/citation-record.json","paper":"/paper/1908.08057"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"0705.3980","last_updated":"2007-05-28T17:02:48Z","snapshot_observed_at":"2026-07-06T01:28:33.560152Z","submitted_at":"2007-05-28T17:02:48Z","title":"Detection of Gravitational Lensing in the Cosmic Microwave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.3980","snapshot_observed_at":"2026-08-14T11:57:33.836460Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.836460Z"},"links":{"cited_paper":"/paper/0705.3980","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:e6c182b4d72ecd30b78899e38f911dc5c5df37472ff6ee16d6d71a09cfa4f4f0","observation_id":"960d7f55-edc2-4710-b768-2fa296b8c19d","resolution":{"observed_at":"2026-08-14T11:57:33.836460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.0644","last_updated":"2008-05-30T02:47:54Z","snapshot_observed_at":"2026-07-06T01:34:38.164962Z","submitted_at":"2008-01-04T09:17:28Z","title":"Correlation of CMB with large-scale structure: II. Weak lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.0644","snapshot_observed_at":"2026-08-14T11:57:33.842404Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.842404Z"},"links":{"cited_paper":"/paper/0801.0644","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:dcf16da1a022a718067ca63d3b3b420c7ed3fd5e89d4596e344709c593c7cafa","observation_id":"f0bb6314-ee7c-4982-bb5b-f2b55b63493b","resolution":{"observed_at":"2026-08-14T11:57:33.842404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.2124","last_updated":"2011-07-27T15:48:09Z","snapshot_observed_at":"2026-08-14T23:34:39.094336Z","submitted_at":"2011-03-10T20:55:09Z","title":"Detection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.2124","snapshot_observed_at":"2026-08-14T11:57:33.847706Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.847706Z"},"links":{"cited_paper":"/paper/1103.2124","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:51bb7abc4af662e4a2e996b0de75e4f95553ae09202be50ae054eab5b01d6039","observation_id":"50c93e3f-ac02-45cd-a590-fee9ab82e7c7","resolution":{"observed_at":"2026-08-14T11:57:33.847706Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.1037","last_updated":"2013-02-02T05:51:38Z","snapshot_observed_at":"2026-08-15T00:33:40.072817Z","submitted_at":"2013-01-06T19:00:11Z","title":"The Atacama Cosmology Telescope: Temperature and Gravitational Lensing Power Spectrum Measurements from Three Seasons of Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.1037","snapshot_observed_at":"2026-08-14T11:57:33.853062Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.853062Z"},"links":{"cited_paper":"/paper/1301.1037","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:9e1c71778c51b42a31aa9f6c6a005cf302e33e1a17d3c785eaf398dd27705d21","observation_id":"70740700-3d13-4bef-bc1a-fc7bbd7e51b4","resolution":{"observed_at":"2026-08-14T11:57:33.853062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.7999","last_updated":"2015-03-30T15:34:10Z","snapshot_observed_at":"2026-08-14T23:09:46.345988Z","submitted_at":"2014-11-28T20:51:06Z","title":"Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos","version":3},"cited_work":{"arxiv_id":"1411.7999","doi":null,"metadata_source":"pith","pith_arxiv_id":"1411.7999","snapshot_observed_at":"2026-08-14T11:57:35.214133Z","title":"Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos","venue":"astro-ph.CO","work_id":"8a340373-7971-435c-98e1-6e2d3a1b920a","year":2014},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.858151Z"},"links":{"cited_paper":"/paper/1411.7999","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:5e47329b89b2359d99e0e4357da205ac5a2d4cf8c3dc6d9f3918ab2bb858d50d","observation_id":"84de1da5-583b-47ac-a149-424bc69ca8dd","resolution":{"observed_at":"2026-08-14T11:57:35.219174Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1412.0626","last_updated":"2014-12-01T20:20:47Z","snapshot_observed_at":"2026-08-14T23:09:26.810796Z","submitted_at":"2014-12-01T20:20:47Z","title":"The Atacama Cosmology Telescope: Lensing of CMB Temperature and Polarization Derived from Cosmic Infrared Background Cross-Correlation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.0626","snapshot_observed_at":"2026-08-14T11:57:33.863182Z","title":"van Engelen, B","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.863182Z"},"links":{"cited_paper":"/paper/1412.0626","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:05d632079c1c0ba7ad1acf59244d4135e8c742632f60205689cae5a941bb83d0","observation_id":"abe81031-8a4a-470e-9f1d-fcffe07160e6","resolution":{"observed_at":"2026-08-14T11:57:33.863182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.09753","last_updated":"2016-11-29T17:55:07Z","snapshot_observed_at":"2026-08-14T21:28:03.259796Z","submitted_at":"2016-11-29T17:55:07Z","title":"The Atacama Cosmology Telescope: Two-Season ACTPol Lensing Power Spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.09753","snapshot_observed_at":"2026-08-14T11:57:33.868557Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.868557Z"},"links":{"cited_paper":"/paper/1611.09753","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:606baf65298dbbdff5626c466aa26aa48930cedf1ee14832af652c53801d7b06","observation_id":"950b4efc-165a-49e5-afdf-09e221798ab0","resolution":{"observed_at":"2026-08-14T11:57:33.868557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.06456","last_updated":"2015-02-23T15:03:41Z","snapshot_observed_at":"2026-08-14T22:59:01.003830Z","submitted_at":"2015-02-23T15:03:41Z","title":"The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing","version":1},"cited_work":{"arxiv_id":"1502.06456","doi":null,"metadata_source":"pith","pith_arxiv_id":"1502.06456","snapshot_observed_at":"2026-08-14T11:57:35.162637Z","title":"The Atacama Cosmology Telescope: measuring radio galaxy bias through cross-correlation with lensing","venue":"astro-ph.CO","work_id":"5caebcd2-64d8-49c5-897f-42c6e0b4ebbc","year":2015},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.873222Z"},"links":{"cited_paper":"/paper/1502.06456","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:889d62ba0b02ff13ceac8ff2432f4fc3f2151943305d1ba0a5b5728e86bc0f3d","observation_id":"14aa04f1-239c-42a8-bdcc-7d373c022229","resolution":{"observed_at":"2026-08-14T11:57:35.168023Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.0546","last_updated":"2012-02-02T20:57:13Z","snapshot_observed_at":"2026-08-15T01:18:53.150096Z","submitted_at":"2012-02-02T20:57:13Z","title":"A measurement of gravitational lensing of the microwave background using South Pole Telescope data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.0546","snapshot_observed_at":"2026-08-14T11:57:33.878319Z","title":"van Engelen, R","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.878319Z"},"links":{"cited_paper":"/paper/1202.0546","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:659a29f52682afc1d2fdb3fe703063e6a243d9930fda302bc5e0b4564340ee9f","observation_id":"e62615d1-6061-4d2b-bdd2-a7fcbbc24ea2","resolution":{"observed_at":"2026-08-14T11:57:33.878319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5830","last_updated":"2013-10-07T15:14:30Z","snapshot_observed_at":"2026-08-15T00:09:30.460426Z","submitted_at":"2013-07-22T19:34:08Z","title":"Detection of B-mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.5830","snapshot_observed_at":"2026-08-14T11:57:33.883167Z","title":"Hanson, S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.883167Z"},"links":{"cited_paper":"/paper/1307.5830","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:2af4c44177b851a1c86f4557742eb2462ad35f1aab1d980c24451b95c610347f","observation_id":"bf4e17a6-cc35-4c1f-bdde-5af9e5fa1d17","resolution":{"observed_at":"2026-08-14T11:57:33.883167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.7521","last_updated":"2015-06-23T20:13:45Z","snapshot_observed_at":"2026-08-14T23:06:15.239825Z","submitted_at":"2014-12-23T20:51:39Z","title":"A Measurement of Gravitational Lensing of the Cosmic Microwave Background by Galaxy Clusters Using Data from the South Pole Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.7521","snapshot_observed_at":"2026-08-14T11:57:33.887942Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.887942Z"},"links":{"cited_paper":"/paper/1412.7521","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:ac00b0dc8176f70e5aca2a54c7c0935ae7501617a6f72391a4c3f40e005d1dbd","observation_id":"7fb6842f-fc00-4987-a6d7-e50b8fea7677","resolution":{"observed_at":"2026-08-14T11:57:33.887942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.4760","last_updated":"2015-09-15T17:47:58Z","snapshot_observed_at":"2026-08-14T23:07:29.279873Z","submitted_at":"2014-12-15T20:53:30Z","title":"A Measurement of the Cosmic Microwave Background Gravitational Lensing Potential from 100 Square Degrees of SPTpol Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.4760","snapshot_observed_at":"2026-08-14T11:57:33.892946Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.892946Z"},"links":{"cited_paper":"/paper/1412.4760","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:b73f5bc4338d80b1a067075212aeae949c01edb983e7620590e8b403072e89d7","observation_id":"181843fd-ab8c-4491-8348-d0e699c02b7c","resolution":{"observed_at":"2026-08-14T11:57:33.892946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.00743","last_updated":"2017-05-02T00:05:17Z","snapshot_observed_at":"2026-08-14T21:03:30.983941Z","submitted_at":"2017-05-02T00:05:17Z","title":"A 2500 square-degree CMB lensing map from combined South Pole Telescope and Planck data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.00743","snapshot_observed_at":"2026-08-14T11:57:33.897711Z","title":"Omori, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.897711Z"},"links":{"cited_paper":"/paper/1705.00743","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:42bb61dad3d249403dac6cb29c5135f7e6b78ee85626982ab8dd09ecaa3824db","observation_id":"68e597b2-03c3-48af-b46c-35a3ebef2ade","resolution":{"observed_at":"2026-08-14T11:57:33.897711Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.6646","last_updated":"2014-04-27T18:36:35Z","snapshot_observed_at":"2026-08-14T23:50:30.501597Z","submitted_at":"2013-12-23T19:03:30Z","title":"Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum with the POLARBEAR experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.6646","snapshot_observed_at":"2026-08-14T11:57:33.902598Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.902598Z"},"links":{"cited_paper":"/paper/1312.6646","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:cadb9a93483a7a194dbf6baa7024a29f644277896faec77db37a6a205b8b9e69","observation_id":"15a6e61e-620a-4195-bc30-b366d15d5d4a","resolution":{"observed_at":"2026-08-14T11:57:33.902598Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02116","last_updated":"2019-10-11T14:18:16Z","snapshot_observed_at":"2026-08-14T16:52:13.524786Z","submitted_at":"2019-04-03T17:23:19Z","title":"Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam","version":2},"cited_work":{"arxiv_id":"1904.02116","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.02116","snapshot_observed_at":"2026-08-14T11:57:35.047821Z","title":"Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam","venue":"astro-ph.CO","work_id":"0e330d07-b5c0-45c3-b9dd-9ee4b721779d","year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.907660Z"},"links":{"cited_paper":"/paper/1904.02116","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:ac6a5788bbefb47205c46f95d1e16d010b9a5e55e5745a63be9b504c6ea3f34f","observation_id":"ec8441da-7d74-43a9-80a1-53e5f1c64662","resolution":{"observed_at":"2026-08-14T11:57:35.053311Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07046","last_updated":"2019-11-19T00:13:28Z","snapshot_observed_at":"2026-08-14T17:01:11.579676Z","submitted_at":"2019-03-17T09:26:44Z","title":"Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies","version":3},"cited_work":{"arxiv_id":"1903.07046","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.07046","snapshot_observed_at":"2026-08-14T11:57:35.025023Z","title":"Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies","venue":"astro-ph.CO","work_id":"c5422325-88cb-4601-98a2-ff4a38926010","year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.912421Z"},"links":{"cited_paper":"/paper/1903.07046","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:d320be9a46f9d1aeeda452937ad6be7888edb3f7c944d6744f02c980d11b95cd","observation_id":"7d988c98-6469-4f65-a44d-7b70b538a74c","resolution":{"observed_at":"2026-08-14T11:57:35.030356Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5077","last_updated":"2014-07-30T18:50:37Z","snapshot_observed_at":"2026-08-15T00:24:25.138525Z","submitted_at":"2013-03-20T20:10:17Z","title":"Planck 2013 results. XVII. Gravitational lensing by large-scale structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5077","snapshot_observed_at":"2026-08-14T11:57:33.917489Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.917489Z"},"links":{"cited_paper":"/paper/1303.5077","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:5d77e688ffe8b1cf8f1387b7a9fddb216929634bba844dd89d32e102d5df0671","observation_id":"387e741c-4e25-4fc6-aede-bc3a26ac1b47","resolution":{"observed_at":"2026-08-14T11:57:33.917489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.01591","last_updated":"2016-09-22T09:07:56Z","snapshot_observed_at":"2026-08-14T23:01:14.310401Z","submitted_at":"2015-02-05T15:08:35Z","title":"Planck 2015 results. XV. Gravitational lensing","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01591","snapshot_observed_at":"2026-08-14T11:57:33.922266Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.922266Z"},"links":{"cited_paper":"/paper/1502.01591","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:e4446d6faf4ad70487001cf983aa90a40e9888e2af695cb1a215492e99b25935","observation_id":"450c45c1-23ab-4ca2-a605-401026303aec","resolution":{"observed_at":"2026-08-14T11:57:33.922266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06210","last_updated":"2019-07-29T12:39:06Z","snapshot_observed_at":"2026-08-14T18:51:13.609346Z","submitted_at":"2018-07-17T04:05:08Z","title":"Planck 2018 results. VIII. Gravitational lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06210","snapshot_observed_at":"2026-08-14T11:57:33.927166Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.927166Z"},"links":{"cited_paper":"/paper/1807.06210","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:906421990bb152f382404bd4eab7dfe3862fae5cd90cf87c7ec210472611f795","observation_id":"384919d1-14dc-498a-89c1-187e3fb1d8c8","resolution":{"observed_at":"2026-08-14T11:57:33.927166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.01968","last_updated":"2016-06-11T23:14:45Z","snapshot_observed_at":"2026-08-14T21:53:55.909672Z","submitted_at":"2016-06-06T22:52:58Z","title":"BICEP2 / Keck Array VIII: Measurement of gravitational lensing from large-scale B-mode polarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.01968","snapshot_observed_at":"2026-08-14T11:57:33.931758Z","title":"Keck Array, BICEP2 Collaborations, :, P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.931758Z"},"links":{"cited_paper":"/paper/1606.01968","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:cda82ca50e8deca02a581375925f33ec1eafcbcfda35da14c9c688cc9edf74fd","observation_id":"ebb6ecea-017a-4d14-80f4-169e03da7c2d","resolution":{"observed_at":"2026-08-14T11:57:33.931758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.04396","last_updated":"2017-11-04T11:30:13Z","snapshot_observed_at":"2026-08-14T21:20:57.943074Z","submitted_at":"2017-01-16T18:53:13Z","title":"CMB Polarization B-mode Delensing with SPTpol and Herschel","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.04396","snapshot_observed_at":"2026-08-14T11:57:33.936571Z","title":"Manzotti, K","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.936571Z"},"links":{"cited_paper":"/paper/1701.04396","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:943430b0ccff268835902ce822d6fb918f9b1ebd4bd12e161d6b6d243ed4ff1c","observation_id":"2ae3b902-b88e-4026-84a4-cddcbaf04223","resolution":{"observed_at":"2026-08-14T11:57:33.936571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01712","last_updated":"2017-05-09T13:05:29Z","snapshot_observed_at":"2026-08-14T21:22:15.768401Z","submitted_at":"2017-01-06T18:05:18Z","title":"Internal delensing of Planck CMB temperature and polarization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.01712","snapshot_observed_at":"2026-08-14T11:57:33.941764Z","title":"Carron, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.941764Z"},"links":{"cited_paper":"/paper/1701.01712","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:b5d671fbec7a50d00c21196f65face9d70c355c3161d74ccf37d524f5d5a84c3","observation_id":"3e6e1d15-914f-4d52-ab61-7fa5c7c18bb2","resolution":{"observed_at":"2026-08-14T11:57:33.941764Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.10349","last_updated":"2019-01-28T15:19:41Z","snapshot_observed_at":"2026-08-14T18:35:04.759208Z","submitted_at":"2018-08-30T15:20:34Z","title":"Optimal constraints on primordial gravitational waves from the lensed CMB","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.10349","snapshot_observed_at":"2026-08-14T11:57:33.946786Z","title":"Carron, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.946786Z"},"links":{"cited_paper":"/paper/1808.10349","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:5c4f26301d63d6a1d766efc0db7951d7146177c3690953b5c3fe5578142b559e","observation_id":"3a3789cb-b7f1-46e9-9cf5-6e7e31374df8","resolution":{"observed_at":"2026-08-14T11:57:33.946786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.02809","last_updated":"2015-10-09T20:10:03Z","snapshot_observed_at":"2026-08-14T22:28:30.549036Z","submitted_at":"2015-10-09T20:10:03Z","title":"Advanced ACTPol Cryogenic Detector Arrays and Readout","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.02809","snapshot_observed_at":"2026-08-14T11:57:33.951768Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.951768Z"},"links":{"cited_paper":"/paper/1510.02809","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:3417339390033af9e8405188951c233b19f9f753971867b9fc2ff9b4880ea8f4","observation_id":"7dc99c61-cde5-43a5-a342-a2405ad6157f","resolution":{"observed_at":"2026-08-14T11:57:33.951768Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.2973","last_updated":"2014-07-10T21:32:57Z","snapshot_observed_at":"2026-08-14T23:27:08.853027Z","submitted_at":"2014-07-10T21:32:57Z","title":"SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2973","snapshot_observed_at":"2026-08-14T11:57:33.956883Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.956883Z"},"links":{"cited_paper":"/paper/1407.2973","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:eef17074beaec1938eae7288847b236ff9095bfecfcad27b5365da170a905bf2","observation_id":"1c8202e0-e045-44e7-b722-62d8e00c44dc","resolution":{"observed_at":"2026-08-14T11:57:33.956883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.07299","last_updated":"2015-12-22T23:37:29Z","snapshot_observed_at":"2026-08-14T22:17:18.405265Z","submitted_at":"2015-12-22T23:37:29Z","title":"The POLARBEAR-2 and the Simons Array Experiment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.07299","snapshot_observed_at":"2026-08-14T11:57:33.961865Z","title":"Suzuki, P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.961865Z"},"links":{"cited_paper":"/paper/1512.07299","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:a65bd9d198cc949d0deb70a101004bf2ef70a71abde273dcf463fe6a75fd457e","observation_id":"1de429ce-4c85-4956-9721-01ad38eb4e33","resolution":{"observed_at":"2026-08-14T11:57:33.961865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.07445","last_updated":"2019-03-01T10:51:03Z","snapshot_observed_at":"2026-08-15T01:11:26.803228Z","submitted_at":"2018-08-22T17:19:17Z","title":"The Simons Observatory: Science goals and forecasts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.07445","snapshot_observed_at":"2026-08-14T11:57:33.966831Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.966831Z"},"links":{"cited_paper":"/paper/1808.07445","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:f2c14a34d5ed8f9a6f4bb058f6f434d7cf01f7717679021d93f284ea23ff4da6","observation_id":"8f949ea4-3721-418e-8bf2-2513122421a3","resolution":{"observed_at":"2026-08-14T11:57:33.966831Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.02743","last_updated":"2016-10-10T00:35:39Z","snapshot_observed_at":"2026-08-14T21:36:01.073428Z","submitted_at":"2016-10-10T00:35:39Z","title":"CMB-S4 Science Book, First Edition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.02743","snapshot_observed_at":"2026-08-14T11:57:33.972054Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.972054Z"},"links":{"cited_paper":"/paper/1610.02743","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:bd528f9134f4f14fd5742750c30d0cc7cb8d402d7529a77aa58108e6b5f93246","observation_id":"ca07bbfd-63cc-42a0-8f55-a271ceaeea0c","resolution":{"observed_at":"2026-08-14T11:57:33.972054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.7547","last_updated":"2013-10-28T19:35:44Z","snapshot_observed_at":"2026-08-14T23:57:22.383038Z","submitted_at":"2013-10-28T19:35:44Z","title":"Extragalactic Foreground Contamination in Temperature-based CMB Lens Reconstruction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.7547","snapshot_observed_at":"2026-08-14T11:57:33.977257Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.977257Z"},"links":{"cited_paper":"/paper/1310.7547","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:7f5d8760a913ca4231b55e9320313b0bfa9f4b540454a5c6de2f16a35b6a30b4","observation_id":"83006566-519c-4f8a-be13-89996e97c5d9","resolution":{"observed_at":"2026-08-14T11:57:33.977257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.7023","last_updated":"2013-10-25T20:00:01Z","snapshot_observed_at":"2026-08-14T23:57:36.776675Z","submitted_at":"2013-10-25T20:00:01Z","title":"CMB Lensing Power Spectrum Biases from Galaxies and Clusters using High-angular Resolution Temperature Maps","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.7023","snapshot_observed_at":"2026-08-14T11:57:33.982095Z","title":"van Engelen, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.982095Z"},"links":{"cited_paper":"/paper/1310.7023","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:2462ddbd424f7c39ff7187154a1d7c2b52d17e3df51a059249b402aab445662e","observation_id":"6bdfb95e-d3f3-4828-8c52-5349338ff926","resolution":{"observed_at":"2026-08-14T11:57:33.982095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.00411","last_updated":"2017-08-17T06:07:42Z","snapshot_observed_at":"2026-08-14T21:03:43.500033Z","submitted_at":"2017-05-01T03:20:22Z","title":"Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: Statistical and systematic error budgets for future experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.00411","snapshot_observed_at":"2026-08-14T11:57:33.986923Z","title":"Raghunathan, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.986923Z"},"links":{"cited_paper":"/paper/1705.00411","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:e97bfd9aaedff00ea41839efefaeb1414058265b35e012a27a8a0db1becf0836","observation_id":"ccc7805a-70b5-4aae-bb2a-9e3da8eb4ec2","resolution":{"observed_at":"2026-08-14T11:57:33.986923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.06751","last_updated":"2018-01-25T05:34:53Z","snapshot_observed_at":"2026-08-14T20:59:43.131609Z","submitted_at":"2017-05-18T18:01:00Z","title":"Bias to CMB Lensing Reconstruction from Temperature Anisotropies due to Large-Scale Galaxy Motions","version":3},"cited_work":{"arxiv_id":"1705.06751","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.06751","snapshot_observed_at":"2026-08-14T11:57:34.773114Z","title":"Bias to CMB Lensing Reconstruction from Temperature Anisotropies due to Large-Scale Galaxy Motions","venue":"astro-ph.CO","work_id":"6767fe3a-880f-47c4-a136-fbda5af9c506","year":2017},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.991906Z"},"links":{"cited_paper":"/paper/1705.06751","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:4493997b332f16851915b0c6271a5aa5dd9aab79e969ab4c3380a0053dd46719","observation_id":"5563b0b2-4a04-4e51-aa23-6578c68c97cf","resolution":{"observed_at":"2026-08-14T11:57:34.778182Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.06403","last_updated":"2019-05-16T22:39:16Z","snapshot_observed_at":"2026-08-14T19:24:56.180328Z","submitted_at":"2018-04-17T17:59:22Z","title":"Foreground-immune CMB lensing with shear-only reconstruction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.06403","snapshot_observed_at":"2026-08-14T11:57:33.997143Z","title":"Schaan and S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:33.997143Z"},"links":{"cited_paper":"/paper/1804.06403","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:979c20177418f875721ec7d0deed26bac56daacea1e358753323092130a190c8","observation_id":"006c2505-d49a-4ad3-8d22-5b3840f209f1","resolution":{"observed_at":"2026-08-14T11:57:33.997143Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.10998","last_updated":"2019-02-20T18:09:54Z","snapshot_observed_at":"2026-08-14T18:09:16.354833Z","submitted_at":"2018-10-25T17:43:15Z","title":"Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data","version":2},"cited_work":{"arxiv_id":"1810.10998","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.10998","snapshot_observed_at":"2026-08-14T11:57:34.735117Z","title":"Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data","venue":"astro-ph.CO","work_id":"b4ed155b-6fd5-4b59-9129-484dc9724b7d","year":2018},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.002169Z"},"links":{"cited_paper":"/paper/1810.10998","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:49e49157fa0446ed0a987e2ac0b01b4e14faf162be87fa71d750b9f5a971491c","observation_id":"0837c039-f940-43a6-bfe5-11bf83475c43","resolution":{"observed_at":"2026-08-14T11:57:34.740262Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.08230","last_updated":"2018-07-07T15:28:35Z","snapshot_observed_at":"2026-08-14T19:43:10.327638Z","submitted_at":"2018-02-22T18:34:20Z","title":"Mitigating Foreground Biases in CMB Lensing Reconstruction Using Cleaned Gradients","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.08230","snapshot_observed_at":"2026-08-14T11:57:34.007164Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.007164Z"},"links":{"cited_paper":"/paper/1802.08230","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:bc0a907a18bd1a568d35f7a1bc9e25ea4740b99cd1e5c6c3ef9d12ce6a6491b2","observation_id":"e27c10bd-8c3f-4891-9a2a-17879a60da39","resolution":{"observed_at":"2026-08-14T11:57:34.007164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.13392","last_updated":"2019-11-07T02:45:59Z","snapshot_observed_at":"2026-08-14T16:39:10.354754Z","submitted_at":"2019-04-30T17:55:37Z","title":"An Inpainting Approach to Tackle the Kinematic and Thermal SZ Induced Biases in CMB-Cluster Lensing Estimators","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.13392","snapshot_observed_at":"2026-08-14T11:57:34.012190Z","title":"Raghunathan, G","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.012190Z"},"links":{"cited_paper":"/paper/1904.13392","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:51e1e185d951f19de8b1179f784a5ac7fae8b6f0191c678b131185e1b7f8dbd5","observation_id":"89108d84-10ce-4644-a4e5-32ff3d99557b","resolution":{"observed_at":"2026-08-14T11:57:34.012190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.0091","last_updated":"2013-02-28T07:42:18Z","snapshot_observed_at":"2026-08-15T00:48:08.353763Z","submitted_at":"2012-09-01T13:17:07Z","title":"Bias-Hardened CMB Lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.0091","snapshot_observed_at":"2026-08-14T11:57:34.017339Z","title":"Namikawa, D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.017339Z"},"links":{"cited_paper":"/paper/1209.0091","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:6df59c09a77834516be9da47a28adf7eb59859bb3a486f547913d9612185e1fc","observation_id":"530fe363-86d1-46ff-b71c-97226e1b2ccc","resolution":{"observed_at":"2026-08-14T11:57:34.017339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.2372","last_updated":"2019-06-07T10:42:05Z","snapshot_observed_at":"2026-08-14T23:59:39.794187Z","submitted_at":"2013-10-09T06:46:56Z","title":"Bias-Hardened CMB Lensing with Polarization","version":4},"cited_work":{"arxiv_id":"1310.2372","doi":null,"metadata_source":"pith","pith_arxiv_id":"1310.2372","snapshot_observed_at":"2026-08-14T11:57:34.664781Z","title":"Bias-Hardened CMB Lensing with Polarization","venue":"astro-ph.CO","work_id":"5ee86e28-f827-403a-af79-1b6e5ec310b5","year":2013},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.022025Z"},"links":{"cited_paper":"/paper/1310.2372","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:bafebf4b8fc91d765542d93cbe932a266f0f212b62b9de80d1ace4ae83d1c937","observation_id":"0fce2a62-ea0c-4b93-ba51-fdb17711bba2","resolution":{"observed_at":"2026-08-14T11:57:34.669961Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1004.3285","last_updated":"2010-04-19T19:56:27Z","snapshot_observed_at":"2026-07-31T03:01:14.410686Z","submitted_at":"2010-04-19T19:56:27Z","title":"CMB Lensing Reconstruction in Real Space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.3285","snapshot_observed_at":"2026-08-14T11:57:34.026548Z","title":"Bucher, C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.026548Z"},"links":{"cited_paper":"/paper/1004.3285","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:fd019865be83343a7630b29d427f6c01d7074d1eea1b7df42b4b470dbc0bee8d","observation_id":"f90ba82f-a985-4a06-a3fe-41ca1200b95c","resolution":{"observed_at":"2026-08-14T11:57:34.026548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.02227","last_updated":"2017-09-07T13:24:43Z","snapshot_observed_at":"2026-08-14T20:35:19.970149Z","submitted_at":"2017-09-07T13:24:43Z","title":"Real space lensing reconstruction using cosmic microwave background polarization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.02227","snapshot_observed_at":"2026-08-14T11:57:34.031351Z","title":"Prince, K","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.031351Z"},"links":{"cited_paper":"/paper/1709.02227","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:325b357ee45213e30f4bd3a75ffbde192cbc123bdb89531e1cefdde72074bd05","observation_id":"be6d3325-3148-4ab8-84f2-0be45086ff4f","resolution":{"observed_at":"2026-08-14T11:57:34.031351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0309301","last_updated":"2003-09-10T20:18:39Z","snapshot_observed_at":"2026-08-14T02:38:11.885114Z","submitted_at":"2003-09-10T20:18:39Z","title":"Lensing Studies with Diffuse Backgrounds","version":1},"cited_work":{"arxiv_id":"astro-ph/0309301","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0309301","snapshot_observed_at":"2026-08-14T11:57:34.609792Z","title":"Lensing Studies with Diffuse Backgrounds","venue":"astro-ph","work_id":"650fa851-0660-491b-98b9-26a0e5b3a457","year":2003},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.036239Z"},"links":{"cited_paper":"/paper/astro-ph/0309301","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:135e20fc570f796d30952ec11b1b96415d23cbc91c7e6a96da1ffbf0bf586fc0","observation_id":"7d30b2b0-d650-478e-8184-b5db617df986","resolution":{"observed_at":"2026-08-14T11:57:34.615224Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.05706","last_updated":"2018-06-06T23:39:09Z","snapshot_observed_at":"2026-08-14T19:45:26.874732Z","submitted_at":"2018-02-15T18:58:28Z","title":"Weak Lensing of Intensity Mapping: the Cosmic Infrared Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.05706","snapshot_observed_at":"2026-08-14T11:57:34.040946Z","title":"Schaan, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.040946Z"},"links":{"cited_paper":"/paper/1802.05706","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:9e3aadbe77d7dbd54343b7ea9544bffbb49a7eed6b506aa2faee3858aea03a31","observation_id":"6cead460-3347-4851-bcca-af1aef270287","resolution":{"observed_at":"2026-08-14T11:57:34.040946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.02084","last_updated":"2019-05-06T15:06:49Z","snapshot_observed_at":"2026-08-14T16:36:41.811599Z","submitted_at":"2019-05-06T15:06:49Z","title":"An excess of non-Gaussian fluctuations in the cosmic infrared background consistent with gravitational lensing","version":1},"cited_work":{"arxiv_id":"1905.02084","doi":null,"metadata_source":"pith","pith_arxiv_id":"1905.02084","snapshot_observed_at":"2026-08-14T11:57:34.571922Z","title":"An excess of non-Gaussian fluctuations in the cosmic infrared background consistent with gravitational lensing","venue":"astro-ph.CO","work_id":"365ba7e4-8162-410c-828d-14474471c417","year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.045683Z"},"links":{"cited_paper":"/paper/1905.02084","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:9d7bb8f4098cf483683997094af5e4fd5c1de033a0612f21d88931b6fa108d97","observation_id":"efbae820-c826-4b66-87a8-801de30e4097","resolution":{"observed_at":"2026-08-14T11:57:34.577082Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.07833","last_updated":"2016-05-10T16:56:40Z","snapshot_observed_at":"2026-08-14T22:46:41.445888Z","submitted_at":"2015-05-28T20:00:35Z","title":"An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.07833","snapshot_observed_at":"2026-08-14T11:57:34.050309Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.050309Z"},"links":{"cited_paper":"/paper/1505.07833","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:9090ad7f9af9e82d1ba1c1ae380cff6a68fe6cbe6d1e9c350103e59ec8cd08ec","observation_id":"1dec52d0-95fc-4afd-908f-62317fad5474","resolution":{"observed_at":"2026-08-14T11:57:34.050309Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2933","last_updated":"2011-08-17T09:25:04Z","snapshot_observed_at":"2026-08-09T14:29:15.405022Z","submitted_at":"2011-04-14T22:06:43Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2933","snapshot_observed_at":"2026-08-14T11:57:34.055059Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.055059Z"},"links":{"cited_paper":"/paper/1104.2933","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:38a5134b4caa1f77c14917d95f07bf7eac6643a6a87d9be8ace5e9f92f27a3bf","observation_id":"d4fe80b1-0c12-4461-83b2-620147ceeaf2","resolution":{"observed_at":"2026-08-14T11:57:34.055059Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0111606","last_updated":"2002-05-17T16:43:48Z","snapshot_observed_at":"2026-07-07T00:23:37.144922Z","submitted_at":"2001-11-30T19:40:05Z","title":"Mass Reconstruction with CMB Polarization","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0111606","snapshot_observed_at":"2026-08-14T11:57:34.059864Z","title":"Hu and T","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.059864Z"},"links":{"cited_paper":"/paper/astro-ph/0111606","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:2eb0fdd764960b6f72c7cf7e144d0eac0dad8d6f0b5ea759760545f724aed7d8","observation_id":"4fde5a55-b57d-4ed1-96cd-cd05324525fc","resolution":{"observed_at":"2026-08-14T11:57:34.059864Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.04975","last_updated":"2018-09-04T02:23:13Z","snapshot_observed_at":"2026-08-14T19:36:33.085184Z","submitted_at":"2018-03-13T18:00:00Z","title":"Lensing reconstruction from line intensity maps: the impact of gravitational nonlinearity","version":2},"cited_work":{"arxiv_id":"1803.04975","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.04975","snapshot_observed_at":"2026-08-14T11:57:34.503110Z","title":"Lensing reconstruction from line intensity maps: the impact of gravitational nonlinearity","venue":"astro-ph.CO","work_id":"21680529-c302-48d5-977e-d89f5f4c93a5","year":2018},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.064387Z"},"links":{"cited_paper":"/paper/1803.04975","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:9533d8a115c92475e89e25eb19c2680f58e470b0489103bf12b2a93529524ebe","observation_id":"5b69012c-0c71-43dc-9d5c-5d5ce4b2a1cb","resolution":{"observed_at":"2026-08-14T11:57:34.508202Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0710.1108","last_updated":"2007-10-06T01:39:27Z","snapshot_observed_at":"2026-08-05T03:26:27.505934Z","submitted_at":"2007-10-04T22:10:53Z","title":"Precision of diffuse 21-cm lensing","version":2},"cited_work":{"arxiv_id":"0710.1108","doi":null,"metadata_source":"pith","pith_arxiv_id":"0710.1108","snapshot_observed_at":"2026-08-14T11:57:34.482502Z","title":"Precision of diffuse 21-cm lensing","venue":"astro-ph","work_id":"9027a46e-bf42-4803-83f8-aab8aa3379c5","year":2007},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.069121Z"},"links":{"cited_paper":"/paper/0710.1108","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:5c778a6c24f99909af26a9fb747f989f2612d2879dccf54dd1cee6693e6d1d01","observation_id":"6f50f485-c024-4095-92ee-5955d1323d39","resolution":{"observed_at":"2026-08-14T11:57:34.487206Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9810257","last_updated":"1998-10-16T20:15:21Z","snapshot_observed_at":"2026-07-07T01:22:39.300566Z","submitted_at":"1998-10-16T20:15:21Z","title":"Reconstructing Projected Matter Density from Cosmic Microwave Background","version":1},"cited_work":{"arxiv_id":"astro-ph/9810257","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9810257","snapshot_observed_at":"2026-08-14T11:57:34.462134Z","title":"Reconstructing Projected Matter Density from Cosmic Microwave Background","venue":"astro-ph","work_id":"57d69a86-a9b2-487d-9a88-ec933e5ca2f6","year":1998},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.074501Z"},"links":{"cited_paper":"/paper/astro-ph/9810257","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:bc4d6363df016572d229f45384fabec138611f6212b504892bd483766888d619","observation_id":"4f1161a9-0c7b-405a-9123-69a52fdf21ab","resolution":{"observed_at":"2026-08-14T11:57:34.467172Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0305387","last_updated":"2004-02-08T21:26:05Z","snapshot_observed_at":"2026-07-07T00:33:26.169276Z","submitted_at":"2003-05-21T13:58:00Z","title":"Gravitational Lensing of Epoch-of-reionization Gas","version":3},"cited_work":{"arxiv_id":"astro-ph/0305387","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0305387","snapshot_observed_at":"2026-08-14T11:57:34.441416Z","title":"Gravitational Lensing of Epoch-of-reionization Gas","venue":"astro-ph","work_id":"74d38171-c752-4dd8-9fb0-9a8ee104626f","year":2003},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.079501Z"},"links":{"cited_paper":"/paper/astro-ph/0305387","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:b4067fcefc59d92b540f521dec06f94c3a3817691ea3ff17c62ee82fb30d7f9f","observation_id":"7c848a7a-1ff4-4c1c-a5d4-0aa894aaf94c","resolution":{"observed_at":"2026-08-14T11:57:34.446514Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0905.0499","last_updated":"2009-05-04T22:19:00Z","snapshot_observed_at":"2026-08-13T20:36:17.790916Z","submitted_at":"2009-05-04T22:19:00Z","title":"Dark Energy from Large-Scale Structure Lensing Information","version":1},"cited_work":{"arxiv_id":"0905.0499","doi":null,"metadata_source":"pith","pith_arxiv_id":"0905.0499","snapshot_observed_at":"2026-08-14T11:57:34.418890Z","title":"Dark Energy from Large-Scale Structure Lensing Information","venue":"astro-ph.CO","work_id":"de33a14d-813d-4585-9aa8-0d588aeccdf8","year":2009},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.084068Z"},"links":{"cited_paper":"/paper/0905.0499","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:d3327d4993fd40bb22ebc7fcd53328620e3233449eef7efd28a00eebabfa721e","observation_id":"65ee3028-4c6d-4ee2-9f83-70afc62ac7ab","resolution":{"observed_at":"2026-08-14T11:57:34.424206Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1301.0776","last_updated":"2013-10-08T11:54:58Z","snapshot_observed_at":"2026-08-15T00:33:47.282007Z","submitted_at":"2013-01-04T17:25:40Z","title":"The Atacama Cosmology Telescope: likelihood for small-scale CMB data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.0776","snapshot_observed_at":"2026-08-14T11:57:34.088982Z","title":"Dunkley, E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.088982Z"},"links":{"cited_paper":"/paper/1301.0776","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:21f1fe18f2c85662535d4c3fb18c832798598647c649e8d70074d1d96bd834ad","observation_id":"e50545e1-074b-4539-b0c7-6864df8465ff","resolution":{"observed_at":"2026-08-14T11:57:34.088982Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.0201","last_updated":"2009-12-01T16:50:56Z","snapshot_observed_at":"2026-08-13T21:52:06.345484Z","submitted_at":"2009-12-01T16:50:56Z","title":"LSST Science Book, Version 2.0","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.0201","snapshot_observed_at":"2026-08-14T11:57:34.093512Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.093512Z"},"links":{"cited_paper":"/paper/0912.0201","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:ba4d3cb9abe803086155cfe52763ed05284e48819220f8619c2a03f5028ad64a","observation_id":"80377474-269f-4ccc-96b5-66909d93f101","resolution":{"observed_at":"2026-08-14T11:57:34.093512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.0395","last_updated":"2011-10-03T16:07:41Z","snapshot_observed_at":"2026-07-06T02:35:05.258609Z","submitted_at":"2011-10-03T16:07:41Z","title":"Modeling the evolution of infrared galaxies : clustering of galaxies in the Cosmic Infrared Background","version":1},"cited_work":{"arxiv_id":"1110.0395","doi":null,"metadata_source":"pith","pith_arxiv_id":"1110.0395","snapshot_observed_at":"2026-08-14T11:57:34.366325Z","title":"Modeling the evolution of infrared galaxies : clustering of galaxies in the Cosmic Infrared Background","venue":"astro-ph.CO","work_id":"e5a886a1-9682-480e-8e00-a50cbbc6de2a","year":2011},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.098161Z"},"links":{"cited_paper":"/paper/1110.0395","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:6ed93fa9064bbb9dab6de444702893c0f9dc0605b2cc95cf2048aa90c652a33e","observation_id":"4ee67f6e-14d7-43b4-8905-8d662cc53ef8","resolution":{"observed_at":"2026-08-14T11:57:34.371350Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1208.6512","last_updated":"2012-09-04T07:13:06Z","snapshot_observed_at":"2026-08-15T00:48:15.168791Z","submitted_at":"2012-08-31T14:56:23Z","title":"A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.6512","snapshot_observed_at":"2026-08-14T11:57:34.102772Z","title":"B´ ethermin, E","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.102772Z"},"links":{"cited_paper":"/paper/1208.6512","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:9c0cbb1412b7c45b1446ed9707ce0cf0b7d792fd0f02b4b41bfa0b95442bcf50","observation_id":"b7d39f92-4e44-45c7-a36a-23ef911b9642","resolution":{"observed_at":"2026-08-14T11:57:34.102772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.3936","last_updated":"2013-07-10T00:16:23Z","snapshot_observed_at":"2026-08-15T00:21:32.932876Z","submitted_at":"2013-04-14T19:37:34Z","title":"The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared","version":2},"cited_work":{"arxiv_id":"1304.3936","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.3936","snapshot_observed_at":"2026-08-14T11:57:34.328856Z","title":"The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared","venue":"astro-ph.CO","work_id":"4df2f870-3b78-4b0e-8986-aa261e3f070e","year":2013},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.107669Z"},"links":{"cited_paper":"/paper/1304.3936","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:d8a9a9ead6880ca9b6e4be3df96d498b2cf5006bcbf72ba5557fb7774be9573d","observation_id":"9e8d3ec0-b972-47d3-8044-703ed5644fe0","resolution":{"observed_at":"2026-08-14T11:57:34.334196Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.4726","last_updated":"2013-09-30T04:51:54Z","snapshot_observed_at":"2026-08-15T00:24:36.133897Z","submitted_at":"2013-03-19T19:58:22Z","title":"Cosmology from the Thermal Sunyaev-Zel'dovich Power Spectrum: Primordial non-Gaussianity and Massive Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.4726","snapshot_observed_at":"2026-08-14T11:57:34.113022Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.113022Z"},"links":{"cited_paper":"/paper/1303.4726","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:3a5a4d4fe7ec9af0efeaaa4c67ed5d0fc5f3dd94e3fcd4bf80cf908757638ede","observation_id":"b47810c1-0309-4500-82a3-8ae4d37fb9e9","resolution":{"observed_at":"2026-08-14T11:57:34.113022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.0553","last_updated":"2012-08-16T16:22:04Z","snapshot_observed_at":"2026-08-14T00:58:58.242992Z","submitted_at":"2011-09-02T20:49:38Z","title":"Deconstructing the kinetic SZ Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.0553","snapshot_observed_at":"2026-08-14T11:57:34.117713Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.117713Z"},"links":{"cited_paper":"/paper/1109.0553","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:555713c96066d11ecd544adf5a1ce8bbc326e840eb7ba95a664d03925a5203c9","observation_id":"d8e91b70-7e75-4a39-97ff-95dd082074e3","resolution":{"observed_at":"2026-08-14T11:57:34.117713Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-14T11:57:34.122445Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.122445Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:f058723d5fef66024054c93b4c9ba8facd9ef672aa61a64f0a171103634e4a9f","observation_id":"0f67dd0a-33ba-4689-a22b-e9af2ab5c435","resolution":{"observed_at":"2026-08-14T11:57:34.122445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.1896","last_updated":"2009-09-09T19:41:42Z","snapshot_observed_at":"2026-07-06T01:56:39.512730Z","submitted_at":"2009-08-13T13:28:40Z","title":"Radio and Millimeter Continuum Surveys and their Astrophysical Implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.1896","snapshot_observed_at":"2026-08-14T11:57:34.127308Z","title":"de Zotti, M","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.127308Z"},"links":{"cited_paper":"/paper/0908.1896","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:53962f4161ab97b3e2babb58e98658c1893ab882f2b6b9c849a0a96778c67da5","observation_id":"487bdaa3-fe12-496d-99fa-ea2e4b12b02f","resolution":{"observed_at":"2026-08-14T11:57:34.127308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0802.1158","last_updated":"2008-02-08T14:30:12Z","snapshot_observed_at":"2026-08-02T21:36:44.495296Z","submitted_at":"2008-02-08T14:30:12Z","title":"A Combined EIS-NVSS Survey Of Radio Sources (CENSORS) III: Spectroscopic observations","version":1},"cited_work":{"arxiv_id":"0802.1158","doi":null,"metadata_source":"pith","pith_arxiv_id":"0802.1158","snapshot_observed_at":"2026-08-14T11:57:34.245340Z","title":"A Combined EIS-NVSS Survey Of Radio Sources (CENSORS) III: Spectroscopic observations","venue":"astro-ph","work_id":"0dc0e825-0def-4763-b77a-d1c66a98d6f5","year":2008},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.131975Z"},"links":{"cited_paper":"/paper/0802.1158","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:1b145722e5872c7f7cb7f5acefae72202eb5e07b5ce220650b094d409cd6423a","observation_id":"f59ac851-849b-4fdf-9989-8148ad9ca825","resolution":{"observed_at":"2026-08-14T11:57:34.250353Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07727","last_updated":"2018-10-17T18:26:43Z","snapshot_observed_at":"2026-08-14T18:13:03.544015Z","submitted_at":"2018-10-17T18:26:43Z","title":"The mass-Peak Patch algorithm for fast generation of deep all-sky dark matter halo catalogues and its N-Body validation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07727","snapshot_observed_at":"2026-08-14T11:57:34.136911Z","title":"Stein, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.136911Z"},"links":{"cited_paper":"/paper/1810.07727","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:118f6c298e7afdadd5a0ac93002a80702a7746c89723e8261b60bc37aecedf53","observation_id":"2fa10667-7675-4284-8c2c-1f210b003f16","resolution":{"observed_at":"2026-08-14T11:57:34.136911Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.03496","last_updated":"2016-03-11T00:42:04Z","snapshot_observed_at":"2026-08-14T22:06:32.693479Z","submitted_at":"2016-03-11T00:42:04Z","title":"A generalized quadratic estimate for random field nonstationarity","version":1},"cited_work":{"arxiv_id":"1603.03496","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.03496","snapshot_observed_at":"2026-08-14T11:57:34.204199Z","title":"A generalized quadratic estimate for random field nonstationarity","venue":"math.ST","work_id":"a3a5a605-fd54-4b26-8d48-1f67a7026022","year":2016},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.141793Z"},"links":{"cited_paper":"/paper/1603.03496","citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:9e37aeaf6a81fd4bb9515ca1731e25906ef424bc1506ef30f7ffe2a05fa3a3dd","observation_id":"62d52ccc-309f-4c25-b692-c66272e7accb","resolution":{"observed_at":"2026-08-14T11:57:34.211431Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-14T11:57:35.351902Z","title":"(14) by using the Fast Fourier Transform (FFT)","venue":null,"work_id":"1106b461-e4e5-4824-ad01-9b892d39ab0c","year":null},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.146540Z"},"links":{"citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:474d3f45f07e19d04bc8287ce0e455220f1a5503e4f80bab09e2c902070f9dd4","observation_id":"79f32838-df9d-40e0-8d4f-ff5127edea1e","resolution":{"observed_at":"2026-08-14T11:57:35.356741Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-14T11:57:35.335307Z","title":"These calculations build upon the LensQuEst module4","venue":null,"work_id":"ab10dc55-e992-4427-babb-4f722a1c4f36","year":null},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.151373Z"},"links":{"citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:872c9bf075820fcb89867ed54ccfdc96871e247aefc81df4dfa41ea7fe2954a2","observation_id":"5908c0ae-5ab8-4c3e-b73f-443be2f7dd8e","resolution":{"observed_at":"2026-08-14T11:57:35.341350Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-14T11:57:35.319896Z","title":null,"venue":null,"work_id":"31302858-22a5-4f25-8b32-01fc53c1bba4","year":null},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.156579Z"},"links":{"citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:46b6b6c8c443a137363b3d03edb8dbf117ac6aecb272515784b47cb4a17e9384","observation_id":"04e827c7-eb6c-4ec7-b393-9ffa8620a8bb","resolution":{"observed_at":"2026-08-14T11:57:35.324970Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-14T11:57:35.304921Z","title":"Here we would like the combined estimator to have zero response to κf L","venue":null,"work_id":"2262c79f-656b-4d67-b09c-3363238cfa64","year":null},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.161667Z"},"links":{"citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:699b3cc3e233540338aed60b57917750442ad40aa897e60a3ae7c484ffa76b1c","observation_id":"98486d2a-4605-44a5-a943-70d59c3453f2","resolution":{"observed_at":"2026-08-14T11:57:35.309729Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-14T11:57:35.289626Z","title":"This would make sure that we are not subtracting a ∼ 1% foreground lensing bias at a large cost in signal-to-noise","venue":null,"work_id":"a82ca955-4eb2-4b6a-a8f5-bab605461376","year":null},"citing_paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T11:57:34.166527Z"},"links":{"citing_paper":"/paper/1908.08057"},"observation_digest":"sha256:b61bbdc192a4b31e47f84e9b284885e1dec93434e78a24eabc375dc0995c106a","observation_id":"14506b74-ca8c-44a6-bd3b-2c73963d73c3","resolution":{"observed_at":"2026-08-14T11:57:35.294791Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.08057","last_updated":"2019-12-05T19:00:03Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T20:55:39.631390Z","submitted_at":"2019-08-21T18:00:05Z","title":"Bias to CMB lensing from lensed foregrounds"},"reference_resolution":{"displayed":68,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":46,"verified_exact":16,"verified_fuzzy":4},"total_outbound_references":68},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 68 of 68 outbound references and 0 inbound Pith citation observations for arXiv:1908.08057."}