{"as_of":"2026-08-05T13:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:78e6db47eb114cfa6e928cba9d90085da83f44f19ed47c3f316761d2311241ab","coverage":[{"denominator":74,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":74,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T21:34:36.733183Z","state":"measured"},{"denominator":80,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":80,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T07:55:22.936065Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.07964","snapshot_observed_at":"2026-08-04T07:55:22.936065Z","title":"2025, @doi [arXiv e-prints] 10.48550/arXiv.2509.07964 , https://ui.adsabs.harvard.edu/abs/2025arXiv250907964G p","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.23566","last_updated":"2026-06-25T21:41:19Z","snapshot_observed_at":"2026-08-04T07:55:02.604850Z","submitted_at":"2025-10-27T17:35:46Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the Weak Lensing Source Galaxies","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-04T07:55:22.936065Z"},"links":{"cited_paper":"/paper/2509.07964","citing_paper":"/paper/2510.23566"},"observation_digest":"sha256:977687f8aa4fd8a834ec9c88f056d2a00b644213504e75c5d509cad021c67e78","observation_id":"88020988-c5d1-4de8-a0b1-3419758394fe","resolution":{"observed_at":"2026-08-04T07:55:22.936065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.07964","snapshot_observed_at":"2026-08-03T03:05:15.362290Z","title":"Giannini, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-05T09:27:44.835956Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.362290Z"},"links":{"cited_paper":"/paper/2509.07964","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:5696751ec2b6cd82ce21c21cec89d6a654a867e678a01af0a78817ebe3086e36","observation_id":"86bd1806-2e6a-4211-8088-ac6ca0098922","resolution":{"observed_at":"2026-08-03T03:05:15.362290Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"cited_work":{"arxiv_id":"2509.07964","doi":"10.48550/arxiv.2509.07964","metadata_source":"arxiv_reference","pith_arxiv_id":"2509.07964","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Gianniniet al.(DES), Phys","venue":"arXiv (Cornell University)","work_id":"75f6001a-a62e-4bab-abd3-68670923dabd","year":2025},"citing_paper":{"arxiv_id":"2605.27221","last_updated":"2026-06-02T13:30:27Z","snapshot_observed_at":"2026-07-06T23:36:58.541051Z","submitted_at":"2026-05-26T16:08:36Z","title":"Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-06-29T15:49:40.634956Z"},"links":{"cited_paper":"/paper/2509.07964","citing_paper":"/paper/2605.27221"},"observation_digest":"sha256:d57b8e8cb917b02841a8cbfe7d23933d13b7ef631f439c9d22ef125f0ee7bc39","observation_id":"df6af459-ad54-4dc8-a9b0-3bdfb154fba2","resolution":{"observed_at":"2026-06-29T16:23:39.398183Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"cited_work":{"arxiv_id":"2509.07964","doi":"10.48550/arxiv.2509.07964","metadata_source":"arxiv_reference","pith_arxiv_id":"2509.07964","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Gianniniet al.(DES), Phys","venue":"arXiv (Cornell University)","work_id":"75f6001a-a62e-4bab-abd3-68670923dabd","year":2025},"citing_paper":{"arxiv_id":"2606.18374","last_updated":"2026-06-16T18:21:15Z","snapshot_observed_at":"2026-08-05T12:30:43.206179Z","submitted_at":"2026-06-16T18:21:15Z","title":"Consistency of DES and DESI distances and the Standard Cosmological Model","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-06-26T23:05:15.137782Z"},"links":{"cited_paper":"/paper/2509.07964","citing_paper":"/paper/2606.18374"},"observation_digest":"sha256:5d8a9110e7f8eb01ed587630fdc4684ca35246c114115eab8d968816a846b206","observation_id":"57874e04-45da-4def-b1a6-a1608d9db7d6","resolution":{"observed_at":"2026-06-26T23:20:14.876140Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.07964","snapshot_observed_at":"2026-07-14T14:25:37.540627Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09943","last_updated":"2026-07-15T12:28:21Z","snapshot_observed_at":"2026-08-05T10:42:41.329141Z","submitted_at":"2026-07-10T19:49:34Z","title":"Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-14T14:25:37.540627Z"},"links":{"cited_paper":"/paper/2509.07964","citing_paper":"/paper/2607.09943"},"observation_digest":"sha256:af0f30819f8d7424b2f702125a361b85be5925ccf270b0cc0e468057ea471fbd","observation_id":"3f18cd86-e5b6-4354-b237-45a14f1aa0c9","resolution":{"observed_at":"2026-07-14T14:25:37.540627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.07964","snapshot_observed_at":"2026-08-02T07:32:42.246715Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09943","last_updated":"2026-07-15T12:28:21Z","snapshot_observed_at":"2026-08-05T10:42:41.329141Z","submitted_at":"2026-07-10T19:49:34Z","title":"Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-02T07:32:42.246715Z"},"links":{"cited_paper":"/paper/2509.07964","citing_paper":"/paper/2607.09943"},"observation_digest":"sha256:24d8a9d277200c97d29a2a48cc05d8d4f2f942f4e1286a67b04523cc3c191cbc","observation_id":"485d5beb-8c21-4ae2-ac27-ca9bd123a4df","resolution":{"observed_at":"2026-08-02T07:32:42.246715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2509.07964/citation-record","integrity":"/paper/2509.07964/integrity","json":"/paper/2509.07964/citation-record.json","paper":"/paper/2509.07964"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:31.427939Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:31.427939Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:a005afbb311dcf635f6ec2f1d5dc7b7afc100455d74ae77d9e85462245420e5c","observation_id":"26f7f2c3-ebb8-4aa4-a4b2-8a8ceabb8040","resolution":{"observed_at":"2026-08-04T21:34:31.427939Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03155","last_updated":"2016-07-11T20:29:52Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:52Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03155","snapshot_observed_at":"2026-08-04T21:34:31.511012Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:31.511012Z"},"links":{"cited_paper":"/paper/1607.03155","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:a6e0b2c36bc47630125ff0018268fe59bf659db5b231c8695b0403f7654834c0","observation_id":"8eb7942e-489f-47c7-aa3f-bbfac3fc63b0","resolution":{"observed_at":"2026-08-04T21:34:31.511012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.09004","last_updated":"2021-09-24T09:54:08Z","snapshot_observed_at":"2026-08-01T23:38:46.742945Z","submitted_at":"2020-07-17T14:10:01Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample","version":2},"cited_work":{"arxiv_id":"2007.09004","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.09004","snapshot_observed_at":"2026-08-04T21:34:39.516113Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample","venue":"astro-ph.CO","work_id":"6bb889cb-93fc-453e-a838-9b72aa1f9339","year":2020},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:31.586905Z"},"links":{"cited_paper":"/paper/2007.09004","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:bf6ad16ac7d1074b20b7909ff0893d569cf4336f281b07dadaeb870603d8b2aa","observation_id":"e691505f-faf1-4a08-95aa-98c13070dec8","resolution":{"observed_at":"2026-08-04T21:34:39.604612Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.11132","last_updated":"2020-11-19T15:39:10Z","snapshot_observed_at":"2026-07-06T09:40:45.543932Z","submitted_at":"2020-07-21T23:35:23Z","title":"The PAU Survey: An improved photo-$z$ sample in the COSMOS field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.11132","snapshot_observed_at":"2026-08-04T21:34:31.706068Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:31.706068Z"},"links":{"cited_paper":"/paper/2007.11132","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:6d0e6a1f4c31ebd5e9a1c285ebd16c9c2ac2bfe5e79719cfe7e1e8395e1b5078","observation_id":"2bf446bb-6859-4921-a406-0d0687b50636","resolution":{"observed_at":"2026-08-04T21:34:31.706068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.05683","last_updated":"2025-05-29T15:03:02Z","snapshot_observed_at":"2026-07-06T20:19:02.999488Z","submitted_at":"2025-01-10T03:13:49Z","title":"Dark Energy Survey Year 6 Results: Synthetic-source Injection Across the Full Survey Using Balrog","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.05683","snapshot_observed_at":"2026-08-04T21:34:31.805393Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:31.805393Z"},"links":{"cited_paper":"/paper/2501.05683","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:5b52c149fa720544298699eb7536ebf8d563ee70b3320e68d453ca6c973882c5","observation_id":"f09c6cda-e05c-4773-b8f6-8e392974aa40","resolution":{"observed_at":"2026-08-04T21:34:31.805393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:42.562816Z","title":null,"venue":null,"work_id":"786397d6-b316-4f7a-aa3e-093c005210ca","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:31.876338Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:042c4ce08d87e4ddb6b3f4f2bcd1aa2594a644b71b3056ff21c460352c1166f3","observation_id":"ac228ef4-82a6-46bb-99d5-60b9df13468a","resolution":{"observed_at":"2026-08-04T21:34:42.627468Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1701.08748","last_updated":"2017-03-20T11:03:51Z","snapshot_observed_at":"2026-07-06T05:28:04.756968Z","submitted_at":"2017-01-30T18:39:38Z","title":"On the realistic validation of photometric redshifts, or why Teddy will never be Happy","version":3},"cited_work":{"arxiv_id":"1701.08748","doi":null,"metadata_source":"pith","pith_arxiv_id":"1701.08748","snapshot_observed_at":"2026-08-04T21:34:39.275427Z","title":"On the realistic validation of photometric redshifts, or why Teddy will never be Happy","venue":"astro-ph.GA","work_id":"8e71b62c-0294-4373-a135-1e3d8b3752c2","year":2017},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:31.969776Z"},"links":{"cited_paper":"/paper/1701.08748","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:85668dee5ec519e3fd2a0adaf8ecfeb8285dd2547df741b23ab4e35d3de9438c","observation_id":"19cfb39d-0942-4774-8c5e-355c6400d906","resolution":{"observed_at":"2026-08-04T21:34:39.384083Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.00758","last_updated":"2026-04-28T14:04:07Z","snapshot_observed_at":"2026-07-06T21:34:25.021259Z","submitted_at":"2025-06-01T00:09:30Z","title":"Dimensional reduction for sampled priors and application to photometric redshift distributions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.00758","snapshot_observed_at":"2026-08-04T21:34:32.046765Z","title":"A., et al., 2025, arXiv e-prints, arXiv:2506.00758, arXiv: 2506.00758","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.046765Z"},"links":{"cited_paper":"/paper/2506.00758","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:3aa621ba9a52b34e9424ca014a0d3fc781c8ef74ef7592a5e8ace7b8b43df042","observation_id":"d6a36aff-415f-4fc8-8b35-c8ee7a15ccf6","resolution":{"observed_at":"2026-08-04T21:34:32.046765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.09247","last_updated":"2017-08-30T13:02:13Z","snapshot_observed_at":"2026-08-05T12:36:40.826050Z","submitted_at":"2017-08-30T13:02:13Z","title":"Beyond linear galaxy alignments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.09247","snapshot_observed_at":"2026-08-04T21:34:32.119613Z","title":"A., MacCrann , N., Troxel , M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.119613Z"},"links":{"cited_paper":"/paper/1708.09247","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:9bb8c15fc8c960aba27032f0d934216855efad9388f978872eae7d2ce3d36178","observation_id":"63761e16-4ac5-4fd3-a02b-4d2fa6bc82ac","resolution":{"observed_at":"2026-08-04T21:34:32.119613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.05005","last_updated":"2019-08-05T08:07:21Z","snapshot_observed_at":"2026-07-06T07:26:54.072746Z","submitted_at":"2019-01-15T19:00:00Z","title":"Phenotypic redshifts with self-organizing maps: A novel method to characterize redshift distributions of source galaxies for weak lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.05005","snapshot_observed_at":"2026-08-04T21:34:32.153482Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.153482Z"},"links":{"cited_paper":"/paper/1901.05005","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:6868514c0695337337b6a4d1c18c2d20d91950df46e3c7f09e84b44fac239391","observation_id":"b9eb78dc-50e3-44c2-a867-f4f260896369","resolution":{"observed_at":"2026-08-04T21:34:32.153482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.00922","last_updated":"2026-07-27T02:04:59Z","snapshot_observed_at":"2026-08-02T14:25:11.617536Z","submitted_at":"2024-08-01T21:23:52Z","title":"Enhancing weak lensing redshift distribution characterization by optimizing the Dark Energy Survey Self-Organizing Map Photo-z method","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.00922","snapshot_observed_at":"2026-08-04T21:34:32.211976Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.211976Z"},"links":{"cited_paper":"/paper/2408.00922","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:50ac388ff91ff16325ef68020c5801be451274c7dfb14a78c76ae8eb8e872d89","observation_id":"1f401e26-80d2-4497-8f0d-390a15ea41b0","resolution":{"observed_at":"2026-08-04T21:34:32.211976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.5753","last_updated":"2013-12-18T20:18:33Z","snapshot_observed_at":"2026-07-06T03:31:25.726310Z","submitted_at":"2013-12-18T20:18:33Z","title":"SOMz: photometric redshift PDFs with self organizing maps and random atlas","version":1},"cited_work":{"arxiv_id":"1312.5753","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.5753","snapshot_observed_at":"2026-08-04T21:34:39.083509Z","title":"SOMz: photometric redshift PDFs with self organizing maps and random atlas","venue":"astro-ph.IM","work_id":"949134e3-dc3b-4306-820a-8a40b6bde3f1","year":2013},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.268950Z"},"links":{"cited_paper":"/paper/1312.5753","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:7795ee9809f522e7186105a8ffd8dd38e1f44a96f855e6443a812ba91b0b8ec0","observation_id":"5285372e-201a-4f2e-b746-206ad7bd81f0","resolution":{"observed_at":"2026-08-04T21:34:39.131741Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.12826","last_updated":"2022-06-08T17:21:11Z","snapshot_observed_at":"2026-07-06T10:27:23.655855Z","submitted_at":"2020-12-23T17:38:15Z","title":"Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.12826","snapshot_observed_at":"2026-08-04T21:34:32.315420Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.315420Z"},"links":{"cited_paper":"/paper/2012.12826","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:64c6ca039ac7e078f0f74b8ee840a6cafe514e487aabf57147a1596151df850e","observation_id":"bf7e48c6-dafc-40bc-a846-a243b964b5b2","resolution":{"observed_at":"2026-08-04T21:34:32.315420Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09636","last_updated":"2022-01-17T12:51:12Z","snapshot_observed_at":"2026-07-06T11:49:35.126128Z","submitted_at":"2021-09-20T15:43:17Z","title":"Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations","version":2},"cited_work":{"arxiv_id":"2109.09636","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.09636","snapshot_observed_at":"2026-08-04T21:34:38.894769Z","title":"Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations","venue":"astro-ph.CO","work_id":"60bde4a3-b6e9-4c9a-a29f-d21bd30e15ea","year":2021},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.368004Z"},"links":{"cited_paper":"/paper/2109.09636","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:89d56a5a4e74622f46b118e8ce81cb9bdab0a54212bc6f6f046bb8eb7f8c5335","observation_id":"0baeb235-735c-42e3-a647-a1603e78b019","resolution":{"observed_at":"2026-08-04T21:34:38.984247Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-08-04T21:34:42.401616Z","title":null,"venue":null,"work_id":"66f0c9fb-f902-4242-bba8-e585e0f82a9e","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.450346Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:2024f0964f7960d65fab8479abadfd6fb11be7812f7b267bc5e4a8dbe8555d92","observation_id":"d0411176-fe9b-41c4-98a3-de6f04613a4e","resolution":{"observed_at":"2026-08-04T21:34:42.460359Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-08-04T21:34:42.239250Z","title":null,"venue":null,"work_id":"793bf87b-9b86-45fc-b295-e1be3830371e","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.487532Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:0064289fe3c05fa03e71c4a5206f6e89abb4927120fa34a3425f5554cda601bc","observation_id":"7a0040fc-064c-4f74-90cf-4203b68092ad","resolution":{"observed_at":"2026-08-04T21:34:42.306274Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1508.04473","last_updated":"2016-01-05T16:24:43Z","snapshot_observed_at":"2026-07-06T04:27:02.490738Z","submitted_at":"2015-08-18T22:23:33Z","title":"The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.04473","snapshot_observed_at":"2026-08-04T21:34:32.532767Z","title":"S., Kneib , J.-P., Percival , W","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.532767Z"},"links":{"cited_paper":"/paper/1508.04473","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:86e0fb089502003ab5b5f101d728ff3da21d1d98be46d246349f4366582a9854","observation_id":"19e96d17-b905-4b84-af6a-a544e3cc64c6","resolution":{"observed_at":"2026-08-04T21:34:32.532767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.0022","last_updated":"2012-11-07T22:32:13Z","snapshot_observed_at":"2026-07-06T02:52:54.937210Z","submitted_at":"2012-07-31T20:05:09Z","title":"The Baryon Oscillation Spectroscopic Survey of SDSS-III","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.0022","snapshot_observed_at":"2026-08-04T21:34:32.584586Z","title":"S., Schlegel , D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.584586Z"},"links":{"cited_paper":"/paper/1208.0022","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:f7dd53858219d31ad490b339235b851864686a323061fc4b18f77edda5f06e84","observation_id":"43cb6238-277c-44d5-bd18-6d6b0ffcda8c","resolution":{"observed_at":"2026-08-04T21:34:32.584586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.07623","last_updated":"2016-05-10T14:43:18Z","snapshot_observed_at":"2026-07-06T04:37:35.431681Z","submitted_at":"2015-11-24T09:38:21Z","title":"DNF - Galaxy photometric redshift by Directional Neighbourhood Fitting","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.07623","snapshot_observed_at":"2026-08-04T21:34:32.631752Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.631752Z"},"links":{"cited_paper":"/paper/1511.07623","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:ba2ecbdba645bf98d8515fb3b8decc60a75d1ebb750b0b61cd3e9f8b6b00e93c","observation_id":"9c76dd97-4cc0-4808-8256-f0e4af483d98","resolution":{"observed_at":"2026-08-04T21:34:32.631752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:32.690307Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.690307Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:019a231507d38388c3d7d54da6fa33e17a7d577bc171869272e61fdb4b56d6a4","observation_id":"9ae27cbc-86da-40ec-aff7-e9bff44569b5","resolution":{"observed_at":"2026-08-04T21:34:32.690307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13549","last_updated":"2022-03-21T13:57:33Z","snapshot_observed_at":"2026-08-02T14:00:01.779912Z","submitted_at":"2021-05-28T01:58:58Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13549","snapshot_observed_at":"2026-08-04T21:34:32.738480Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.738480Z"},"links":{"cited_paper":"/paper/2105.13549","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:59225bc9e72a9ef042d3ff8ad2a7803f5c83c232ec1007a22fc8a15d1288780e","observation_id":"979e0a62-90e3-4410-a407-72e9aa75ef59","resolution":{"observed_at":"2026-08-04T21:34:32.738480Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06308","last_updated":"2024-10-17T05:25:34Z","snapshot_observed_at":"2026-08-04T08:31:29.248482Z","submitted_at":"2023-06-09T23:55:37Z","title":"The Early Data Release of the Dark Energy Spectroscopic Instrument","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.06308","snapshot_observed_at":"2026-08-04T21:34:32.795095Z","title":"G., Aguilar , J., et al., 2024, , 168, 2, 58, arXiv: 2306.06308","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.795095Z"},"links":{"cited_paper":"/paper/2306.06308","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:6cb0f0951679d6fc918ab08ad0dede4860b806756d399c9984a4dc632aaf89d2","observation_id":"aa8030dc-25f5-440f-b6de-9f3653464351","resolution":{"observed_at":"2026-08-04T21:34:32.795095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.04375","last_updated":"2019-10-23T13:37:14Z","snapshot_observed_at":"2026-07-06T07:00:45.001437Z","submitted_at":"2018-09-12T12:19:01Z","title":"The PAU Survey: Early demonstration of photometric redshift performance in the COSMOS field","version":2},"cited_work":{"arxiv_id":"1809.04375","doi":null,"metadata_source":"pith","pith_arxiv_id":"1809.04375","snapshot_observed_at":"2026-08-04T21:34:38.506583Z","title":"The PAU Survey: Early demonstration of photometric redshift performance in the COSMOS field","venue":"astro-ph.GA","work_id":"048fac82-05b9-41ce-9b73-71d844c6d66e","year":2018},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.846416Z"},"links":{"cited_paper":"/paper/1809.04375","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:2a280104673103c7d9c276ae9e9aa2da82175331eb2eaea9ec8357c0620d23c2","observation_id":"e7b7b303-f747-4ea6-a6b8-c17a770639ae","resolution":{"observed_at":"2026-08-04T21:34:38.569526Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-08-04T21:34:42.059195Z","title":null,"venue":null,"work_id":"b06b6ec9-aa33-4c5e-97fc-451e47fd868b","year":2020},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.908023Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:477ab0e8c67975d762e84457271f9447b4ebcf83272f7e8cc540ce0ad52dca47","observation_id":"35c90ea3-960f-4747-bd05-d125dbdcdf87","resolution":{"observed_at":"2026-08-04T21:34:42.130412Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1504.02900","last_updated":"2015-04-11T17:45:05Z","snapshot_observed_at":"2026-07-06T04:14:44.155033Z","submitted_at":"2015-04-11T17:45:05Z","title":"The Dark Energy Camera","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.02900","snapshot_observed_at":"2026-08-04T21:34:32.985785Z","title":"T., Honscheid , K., et al., 2015, , 150, 5, 150, arXiv: 1504.02900","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:32.985785Z"},"links":{"cited_paper":"/paper/1504.02900","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:ea1cd6cfc4b26ecd7540feb757b578e4643b5c772d232fa5b904080ad4480232","observation_id":"e9927744-c223-4609-aec6-412668be21a9","resolution":{"observed_at":"2026-08-04T21:34:32.985785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:33.036970Z","title":"M., et al., 2022, , 510, 1, 1223, arXiv: 2012.08569","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.036970Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:cf263509bbc312c3109b6a417b12728d5a1a2638b30f104e1ebd5f8861c50d84","observation_id":"63d27ff8-d15d-458c-ab62-948387f1dd78","resolution":{"observed_at":"2026-08-04T21:34:33.036970Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.05853","last_updated":"2023-10-18T22:36:58Z","snapshot_observed_at":"2026-08-05T08:53:33.534303Z","submitted_at":"2022-09-13T10:00:06Z","title":"Dark Energy Survey Year 3 Results: Redshift Calibration of the MagLim Lens Sample from the combination of SOMPZ and clustering and its impact on Cosmology","version":2},"cited_work":{"arxiv_id":"2209.05853","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.05853","snapshot_observed_at":"2026-08-04T21:34:38.325265Z","title":"Dark Energy Survey Year 3 Results: Redshift Calibration of the MagLim Lens Sample from the combination of SOMPZ and clustering and its impact on Cosmology","venue":"astro-ph.CO","work_id":"b9c09aef-14f2-4de7-b91c-f0fb9fd4e87f","year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.088989Z"},"links":{"cited_paper":"/paper/2209.05853","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:b9b76f58dbcc49f52a39d8367340b38aa5659a080316b5408ed83e20e137eef0","observation_id":"66fc3933-7db7-4f12-8aca-7eb06641f14d","resolution":{"observed_at":"2026-08-04T21:34:38.378154Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.01160","last_updated":"2017-03-07T02:54:55Z","snapshot_observed_at":"2026-08-02T08:53:20.897268Z","submitted_at":"2016-10-04T20:00:01Z","title":"Selection biases in empirical p(z) methods for weak lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.01160","snapshot_observed_at":"2026-08-04T21:34:33.142089Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.142089Z"},"links":{"cited_paper":"/paper/1610.01160","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:2fed5b4465e875acc1df63d77c661b0a65d07a8e4f7af05ada03b45c199a810b","observation_id":"92d36c51-eca2-452d-a523-c07a7ada09b3","resolution":{"observed_at":"2026-08-04T21:34:33.142089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.05643","last_updated":"2018-09-03T01:00:35Z","snapshot_observed_at":"2026-08-04T09:44:15.669067Z","submitted_at":"2017-08-18T15:15:13Z","title":"DES Science Portal: Computing Photometric Redshifts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.05643","snapshot_observed_at":"2026-08-04T21:34:33.193267Z","title":"C., Ogando , R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.193267Z"},"links":{"cited_paper":"/paper/1708.05643","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:48e2ce1840533a5240df87136d08db1d0c128eb79e6d097ecfc9336333ef3a00","observation_id":"cfb16a72-abd6-4cf5-9baf-2eb2e8bf6be1","resolution":{"observed_at":"2026-08-04T21:34:33.193267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.10454","last_updated":"2020-08-03T12:43:52Z","snapshot_observed_at":"2026-07-06T09:06:44.762147Z","submitted_at":"2020-03-23T18:00:02Z","title":"The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveys","version":2},"cited_work":{"arxiv_id":"2003.10454","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.10454","snapshot_observed_at":"2026-08-04T21:34:38.081897Z","title":"The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveys","venue":"astro-ph.GA","work_id":"04f04ce8-23d8-47bf-b8cc-80c459ec5aa5","year":2020},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.243931Z"},"links":{"cited_paper":"/paper/2003.10454","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:2d95756352e297fea14e13a5728e8192c9f6491f90a5ad09feea3836f3c8b2b4","observation_id":"4677ee5d-1e9a-41be-bde6-943908023e9e","resolution":{"observed_at":"2026-08-04T21:34:38.161024Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:33.317412Z","title":"G., Choi , A., Amon , A., et al., 2022, , 509, 3, 3547, arXiv: 2012.12824","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.317412Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:97bd10f30e605ce6df8a516451bdd2a2a06313647c2526e0f8226a1ae5d2a417","observation_id":"55ced60a-4c55-4d1f-8d72-e42584888780","resolution":{"observed_at":"2026-08-04T21:34:33.317412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.15632","last_updated":"2020-12-08T17:36:20Z","snapshot_observed_at":"2026-07-06T09:43:17.065349Z","submitted_at":"2020-07-30T17:54:33Z","title":"KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.15632","snapshot_observed_at":"2026-08-04T21:34:33.385914Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.385914Z"},"links":{"cited_paper":"/paper/2007.15632","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:96f90549204a941440833d5272faf50551e4103b991ee19d1a8401b3a19d42dd","observation_id":"b1a02fa5-c674-4c5e-a616-433c34379fbd","resolution":{"observed_at":"2026-08-04T21:34:33.385914Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.0658","last_updated":"2010-08-03T21:01:10Z","snapshot_observed_at":"2026-08-04T19:52:59.277350Z","submitted_at":"2010-08-03T21:01:10Z","title":"PHAT: PHoto-z Accuracy Testing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.0658","snapshot_observed_at":"2026-08-04T21:34:33.453858Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.453858Z"},"links":{"cited_paper":"/paper/1008.0658","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:58ecef5857c3c75855565fe46811c9b11f6d1ee7ba494656963721b7770780c0","observation_id":"0a4d8edf-a1e2-452b-8f90-3bac2ad87dd1","resolution":{"observed_at":"2026-08-04T21:34:33.453858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:41.929411Z","title":"J., Ilbert , O., et al., 2016, , 224, 24","venue":null,"work_id":"05550e94-c66f-4896-bc83-79b094ba2873","year":2016},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.505759Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:b11219cd1fb5fca7b94f011cfe483d7711c7a7619d651aa97c685992d9c4a1f2","observation_id":"ba758786-502b-482b-9642-8fe72832396f","resolution":{"observed_at":"2026-08-04T21:34:41.996631Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16923","last_updated":"2023-06-29T13:18:57Z","snapshot_observed_at":"2026-07-06T15:48:21.177346Z","submitted_at":"2023-06-29T13:18:57Z","title":"NAUTILUS: boosting Bayesian importance nested sampling with deep learning","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16923","snapshot_observed_at":"2026-08-04T21:34:33.569392Z","title":"U., 2023, , 525, 2, 3181, arXiv: 2306.16923","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.569392Z"},"links":{"cited_paper":"/paper/2306.16923","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:79ea7690033ce590cc57373aa5421450ea4421cfb3783bc8d6443622ec32212f","observation_id":"2bd9e3f5-e906-47ae-9ae1-42fcb9285386","resolution":{"observed_at":"2026-08-04T21:34:33.569392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.0545","last_updated":"2013-11-05T17:14:34Z","snapshot_observed_at":"2026-07-06T03:17:11.345896Z","submitted_at":"2013-07-01T21:51:10Z","title":"The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_{AB}<=24.7","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.0545","snapshot_observed_at":"2026-08-04T21:34:33.634683Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.634683Z"},"links":{"cited_paper":"/paper/1307.0545","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:97637c0473e40e02fbac8fe9ad04f52b1ba93291acdaf959a9380593c55acdfb","observation_id":"ba58c076-24e5-4c9c-98ed-64d1a8840910","resolution":{"observed_at":"2026-08-04T21:34:33.634683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.08606","last_updated":"2016-11-25T21:00:03Z","snapshot_observed_at":"2026-07-06T05:20:11.209777Z","submitted_at":"2016-11-25T21:00:03Z","title":"Lensing is Low: Cosmology, Galaxy Formation, or New Physics?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.08606","snapshot_observed_at":"2026-08-04T21:34:33.715354Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.715354Z"},"links":{"cited_paper":"/paper/1611.08606","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:0179000213f9e5d1c5339a915e5975b556ff94f0005a2272c156cc2d3a8da33c","observation_id":"c2f310c3-cba4-4577-a769-6b47b47d5449","resolution":{"observed_at":"2026-08-04T21:34:33.715354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:41.751741Z","title":"J., Le Brun , V., Maier , C., et al., 2009, , 184, 2, 218","venue":null,"work_id":"a77a13dd-e62a-4934-973c-eca5b2c925d5","year":2009},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.790065Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:db69942252a0cc6bec3a5683e8d9b2659ff285d04a403b82d49559e6ea6d00e9","observation_id":"1367a835-abc1-4215-9f1b-47f3291cd43b","resolution":{"observed_at":"2026-08-04T21:34:41.849343Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1207.1120","last_updated":"2013-03-10T02:26:17Z","snapshot_observed_at":"2026-07-06T02:51:15.592134Z","submitted_at":"2012-07-04T20:35:56Z","title":"Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.1120","snapshot_observed_at":"2026-08-04T21:34:33.837621Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.837621Z"},"links":{"cited_paper":"/paper/1207.1120","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:612341fef0f6909079e0422e2d77939c3f8e1e2de24f9c88ef61304d4412f53a","observation_id":"50e50e9b-a2c9-4100-bcaf-ea2003d57b72","resolution":{"observed_at":"2026-08-04T21:34:33.837621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:41.569256Z","title":"C., Stern , D","venue":null,"work_id":"d2430041-5d2a-4314-a5c1-fa24e951487d","year":2017},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.917174Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:73ceb24b9a025efe45258b1e2bb00a9e1c601252de87de984aac0af47dee2d83","observation_id":"e8920e58-50e6-4cf7-a590-09c2e38a226a","resolution":{"observed_at":"2026-08-04T21:34:41.664785Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.06394","last_updated":"2019-04-12T20:00:39Z","snapshot_observed_at":"2026-07-06T07:45:46.835717Z","submitted_at":"2019-04-12T20:00:39Z","title":"The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Analysis and Data Release 2","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.06394","snapshot_observed_at":"2026-08-04T21:34:33.962740Z","title":"C., Stern , D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:33.962740Z"},"links":{"cited_paper":"/paper/1904.06394","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:b70c06c385f1c93e4586130ca9b593c7458670091c513146b19a0d61a5d2e541","observation_id":"b23db2be-7c7a-4494-a6ae-45bb84972227","resolution":{"observed_at":"2026-08-04T21:34:33.962740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.6586","last_updated":"2013-02-27T16:48:10Z","snapshot_observed_at":"2026-07-06T02:47:15.526666Z","submitted_at":"2012-04-30T10:25:21Z","title":"UltraVISTA: a new ultra-deep near-infrared survey in COSMOS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.6586","snapshot_observed_at":"2026-08-04T21:34:34.010537Z","title":"J., Milvang-Jensen , B., Dunlop , J., et al., 2012, , 544, A156, arXiv: 1204.6586","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.010537Z"},"links":{"cited_paper":"/paper/1204.6586","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:8f30d311f6b678bbdf2ef36eb420573fe9ffe193cd59e5bdbfd9f67341fddbf3","observation_id":"5341f8d6-46c7-440f-a55e-566dd589782d","resolution":{"observed_at":"2026-08-04T21:34:34.010537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2402.10697","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:37.800550Z","title":null,"venue":null,"work_id":"e0316edd-741a-4317-a74d-424c91156c0b","year":2024},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.077050Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:47fe6a511edf4e4414349d887d4d63ebad6cbba5fe4c7a155860c18f45af81fd","observation_id":"b9ee714b-3cae-48ad-93c5-c944f6733637","resolution":{"observed_at":"2026-08-04T21:34:37.869485Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08566","last_updated":"2021-06-14T16:01:50Z","snapshot_observed_at":"2026-08-01T18:05:51.907986Z","submitted_at":"2020-12-15T19:30:42Z","title":"Dark Energy Survey Year 3 Results: Redshift Calibration of the Weak Lensing Source Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08566","snapshot_observed_at":"2026-08-04T21:34:34.120848Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.120848Z"},"links":{"cited_paper":"/paper/2012.08566","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:e5f7b23527644b0466cbdc69579a7e9adafe446572633d6c27507868019af12d","observation_id":"72ff4c9e-1864-403d-ba9e-651972435a3c","resolution":{"observed_at":"2026-08-04T21:34:34.120848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.03130","last_updated":"2023-02-04T21:32:54Z","snapshot_observed_at":"2026-07-06T14:01:25.012788Z","submitted_at":"2022-10-06T18:00:03Z","title":"Mapping Variations of Redshift Distributions with Probability Integral Transforms","version":2},"cited_work":{"arxiv_id":"2210.03130","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.03130","snapshot_observed_at":"2026-08-04T21:34:37.622588Z","title":"Mapping Variations of Redshift Distributions with Probability Integral Transforms","venue":"astro-ph.CO","work_id":"6436b69f-b238-4c28-8eed-7df4a163d672","year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.195323Z"},"links":{"cited_paper":"/paper/2210.03130","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:4f35d9a28bee0ca9c507ea909efa54c029bca06235783891ea2a5b38b971c6fc","observation_id":"e4b997a7-44f2-4a23-a68a-57fd025a5b5c","resolution":{"observed_at":"2026-08-04T21:34:37.661565Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.07581","last_updated":"2023-12-10T23:05:54Z","snapshot_observed_at":"2026-07-06T17:00:41.729445Z","submitted_at":"2023-12-10T23:05:54Z","title":"The PAU Survey: Photometric redshift estimation in deep wide fields","version":1},"cited_work":{"arxiv_id":"2312.07581","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.07581","snapshot_observed_at":"2026-08-04T21:34:37.482712Z","title":"The PAU Survey: Photometric redshift estimation in deep wide fields","venue":"astro-ph.CO","work_id":"5f42818a-8734-4148-ad29-5cf4640bec67","year":2023},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.267577Z"},"links":{"cited_paper":"/paper/2312.07581","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:344b3b4fd4fe688549f3572f2fae51f58dc323808dd418e81d9514c8f8323fc0","observation_id":"ea047104-4415-4b6e-92c9-de94f24ed192","resolution":{"observed_at":"2026-08-04T21:34:37.547446Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.13633","last_updated":"2022-06-27T21:11:19Z","snapshot_observed_at":"2026-07-06T13:25:17.016579Z","submitted_at":"2022-06-27T21:11:19Z","title":"Photometric Redshifts for Next-Generation Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.13633","snapshot_observed_at":"2026-08-04T21:34:34.343754Z","title":"A., Gruen , D., 2022, , 60, 363, arXiv: 2206.13633","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.343754Z"},"links":{"cited_paper":"/paper/2206.13633","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:779e4ddc34df5504215e067ea3f8b7e77f0eed7ecf625f0f53bbe2273e98b426","observation_id":"4dbaa6e2-7203-4244-8697-536feca600e0","resolution":{"observed_at":"2026-08-04T21:34:34.343754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.03623","last_updated":"2019-03-28T16:23:36Z","snapshot_observed_at":"2026-07-06T07:32:14.230179Z","submitted_at":"2019-02-10T15:52:18Z","title":"The Physics of the Accelerating Universe Camera","version":2},"cited_work":{"arxiv_id":"1902.03623","doi":null,"metadata_source":"pith","pith_arxiv_id":"1902.03623","snapshot_observed_at":"2026-08-04T21:34:37.356832Z","title":"The Physics of the Accelerating Universe Camera","venue":"astro-ph.IM","work_id":"9fff810f-f294-4ec3-9ee2-feb3d68c630d","year":2019},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.402970Z"},"links":{"cited_paper":"/paper/1902.03623","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:4b46ddca6c7e46d41713eacc6d35e1e199c18ba8f50e7bc6e005c28ffccc79fc","observation_id":"417172e3-da96-4a5e-b42b-ffc90ce6d269","resolution":{"observed_at":"2026-08-04T21:34:37.406339Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13546","last_updated":"2022-12-21T19:11:07Z","snapshot_observed_at":"2026-07-06T11:13:32.596343Z","submitted_at":"2021-05-28T01:58:55Z","title":"Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13546","snapshot_observed_at":"2026-08-04T21:34:34.458112Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.458112Z"},"links":{"cited_paper":"/paper/2105.13546","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:804a5f1f87eb5b7b225d7b8d4ace0150188fa3491e0a47ada944381817630eb0","observation_id":"10b7bef8-18c1-47b3-9a15-e61a8746ea75","resolution":{"observed_at":"2026-08-04T21:34:34.458112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.03411","last_updated":"2021-02-02T01:21:34Z","snapshot_observed_at":"2026-07-06T10:12:18.853846Z","submitted_at":"2020-11-06T15:06:56Z","title":"Dark Energy Survey Year 3 Results: Optimizing the Lens Sample in Combined Galaxy Clustering and Galaxy-Galaxy Lensing Analysis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.03411","snapshot_observed_at":"2026-08-04T21:34:34.516268Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.516268Z"},"links":{"cited_paper":"/paper/2011.03411","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:cb51b8b562df5361469951f1faeee23bc56fb39cb988c7ed2a4b3c6594828583","observation_id":"82d69e4d-67dc-42f6-bf8d-1e76b83aea25","resolution":{"observed_at":"2026-08-04T21:34:34.516268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:41.382127Z","title":null,"venue":null,"work_id":"0149b3e5-f5a0-45d0-a205-b988d506eb85","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.552049Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:19050101a472917e071502ded9559395d0f8d3ad3f430d97c75495b0bf1923b1","observation_id":"8f468312-f177-4558-96ee-3c52d876a100","resolution":{"observed_at":"2026-08-04T21:34:41.465762Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1507.05460","last_updated":"2015-07-20T12:00:54Z","snapshot_observed_at":"2026-07-06T04:24:19.782092Z","submitted_at":"2015-07-20T12:00:54Z","title":"redMaGiC: Selecting Luminous Red Galaxies from the DES Science Verification Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.05460","snapshot_observed_at":"2026-08-04T21:34:34.635325Z","title":"S., Abate , A., et al., 2016, , 461, 1431, arXiv: 1507.05460","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.635325Z"},"links":{"cited_paper":"/paper/1507.05460","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:2c2604a4241800bcf4b9ecbccd39ee567196e557132c8c9d71209cf70d694669","observation_id":"da48f87c-9e99-4941-93e8-abacd63ac6ce","resolution":{"observed_at":"2026-08-04T21:34:34.635325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:41.224405Z","title":"N., Eifler, T., Behroozi, P., 2025, The Astrophysical Journal, 983, 2, 183","venue":null,"work_id":"7b690617-4f1c-460c-98a5-5cf1fb740298","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.693015Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:c7ddd02761fdeb47e18d0fb8ae0acf1cd42022487bee4c04ee281776fc7a4d98","observation_id":"325210ee-a9a7-49a3-a972-69c4cdc47cea","resolution":{"observed_at":"2026-08-04T21:34:41.304204Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13542","last_updated":"2022-04-05T19:39:00Z","snapshot_observed_at":"2026-07-06T11:13:32.596343Z","submitted_at":"2021-05-28T01:58:51Z","title":"Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13542","snapshot_observed_at":"2026-08-04T21:34:34.746977Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.746977Z"},"links":{"cited_paper":"/paper/2105.13542","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:ba900e6bf41968c51472edf400a19cfa94ce6d7f366b3d0c531b76fb21d9e3be","observation_id":"37a9f25e-ddbe-41b0-9bae-eead10ad771e","resolution":{"observed_at":"2026-08-04T21:34:34.746977Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09542","last_updated":"2020-04-20T18:03:19Z","snapshot_observed_at":"2026-08-03T18:46:02.235483Z","submitted_at":"2020-04-20T18:03:19Z","title":"Propagating sample variance uncertainties in redshift calibration: simulations, theory and application to the COSMOS2015 data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09542","snapshot_observed_at":"2026-08-04T21:34:34.803141Z","title":"M., 2020, , 498, 2, 2984, arXiv: 2004.09542","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.803141Z"},"links":{"cited_paper":"/paper/2004.09542","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:4777a9a1ac50e4f68d22d67012683734d0d3faf7caeb33b39504097fcad7ef0b","observation_id":"ed7ea270-6dca-4494-b5c5-7f5d2311019a","resolution":{"observed_at":"2026-08-04T21:34:34.803141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:41.022285Z","title":null,"venue":null,"work_id":"e4704549-a117-48ac-b753-cc9ace8d441f","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.880835Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:ba05876677227921170c0bc6eae3f78da73ea52fcc50f030b2f62e3c11b20a12","observation_id":"565ec601-bd8a-4fc1-a49f-23f3b7a03947","resolution":{"observed_at":"2026-08-04T21:34:41.089086Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03337","last_updated":"2019-01-10T19:00:02Z","snapshot_observed_at":"2026-08-04T23:35:05.585621Z","submitted_at":"2019-01-10T19:00:02Z","title":"The unWISE Catalog: Two Billion Infrared Sources from Five Years of WISE Imaging","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03337","snapshot_observed_at":"2026-08-04T21:34:34.946018Z","title":"F., Meisner , A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:34.946018Z"},"links":{"cited_paper":"/paper/1901.03337","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:86014d40f2b3dca918755981bcda10dc0e59d0515503860f7a8b1932000310a4","observation_id":"ad254c49-0a2b-41ad-b69c-bbc3ebde6046","resolution":{"observed_at":"2026-08-04T21:34:34.946018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:40.800473Z","title":null,"venue":null,"work_id":"522488b4-1732-4bf4-bb3c-2cca34856edf","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.029968Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:76e6fc8872ecc952b9041661c502c94a9b29018e59fa9368df387121ad80bf7b","observation_id":"2fac1296-2d26-4a13-b37b-e7c88eee7bd2","resolution":{"observed_at":"2026-08-04T21:34:40.890955Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07048","last_updated":"2016-11-21T21:00:22Z","snapshot_observed_at":"2026-07-06T05:19:33.033655Z","submitted_at":"2016-11-21T21:00:22Z","title":"The VIMOS Public Extragalactic Redshift Survey (VIPERS). Full spectroscopic data and auxiliary information release (PDR-2)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07048","snapshot_observed_at":"2026-08-04T21:34:35.036956Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.036956Z"},"links":{"cited_paper":"/paper/1611.07048","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:436338ffa96a970dd89eb936a35f5aeca5d4e3aee5360923ddd5b5656aa3fc51","observation_id":"b7844eda-d2e6-4962-a69b-ed521329f1ad","resolution":{"observed_at":"2026-08-04T21:34:35.036956Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0612305","last_updated":"2006-12-12T06:21:42Z","snapshot_observed_at":"2026-08-02T15:05:52.321542Z","submitted_at":"2006-12-12T06:21:42Z","title":"The Cosmic Evolution Survey (COSMOS) -- Overview","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0612305","snapshot_observed_at":"2026-08-04T21:34:35.046944Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.046944Z"},"links":{"cited_paper":"/paper/astro-ph/0612305","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:3d5afbe097b3d7c063ca09e476802e2b4ba82876be8013ec0d9fb31e6e14fa2f","observation_id":"c7ec9491-613d-4bd7-b0a0-b18346896a3a","resolution":{"observed_at":"2026-08-04T21:34:35.046944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.2233","last_updated":"2013-05-21T05:31:57Z","snapshot_observed_at":"2026-07-06T02:53:33.365013Z","submitted_at":"2012-08-10T17:59:11Z","title":"The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.2233","snapshot_observed_at":"2026-08-04T21:34:35.125260Z","title":"A., Gunn , J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.125260Z"},"links":{"cited_paper":"/paper/1208.2233","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:893be69287f76ffb4f66337125e12ccae906ef62ff24f488d8032e7bb7d0a79a","observation_id":"de999de9-7edb-42a9-a8b0-1b3255e80494","resolution":{"observed_at":"2026-08-04T21:34:35.125260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.11367","last_updated":"2022-02-16T21:00:12Z","snapshot_observed_at":"2026-07-06T11:21:30.713389Z","submitted_at":"2021-06-21T18:56:31Z","title":"Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3","version":2},"cited_work":{"arxiv_id":"2106.11367","doi":null,"metadata_source":"pith","pith_arxiv_id":"2106.11367","snapshot_observed_at":"2026-08-04T21:34:37.066648Z","title":"Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3","venue":"astro-ph.CO","work_id":"b8823c1e-778e-49e8-89c0-b082bdcc5d0d","year":2021},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.391989Z"},"links":{"cited_paper":"/paper/2106.11367","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:8b951853ad91eba78273010b54c1bf4346110055da54120f12ebe9bce87d48bc","observation_id":"23e6c8da-a723-4664-bf74-d16640887782","resolution":{"observed_at":"2026-08-04T21:34:37.122325Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00705","last_updated":"2023-12-28T04:58:17Z","snapshot_observed_at":"2026-07-06T15:11:07.800604Z","submitted_at":"2023-04-03T03:37:05Z","title":"Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00705","snapshot_observed_at":"2026-08-04T21:34:35.565100Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.565100Z"},"links":{"cited_paper":"/paper/2304.00705","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:823a93c70210908964e333178e71dbb255ad7602070fece14a6c879b8bad6420","observation_id":"1bbd07f8-c970-40fa-a1c9-1360a1ec37bf","resolution":{"observed_at":"2026-08-04T21:34:35.565100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.07150","last_updated":"2020-01-03T19:58:24Z","snapshot_observed_at":"2026-08-02T17:27:58.330548Z","submitted_at":"2019-08-20T03:51:50Z","title":"Optimizing galaxy samples for clustering measurements in photometric surveys","version":2},"cited_work":{"arxiv_id":"1908.07150","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.07150","snapshot_observed_at":"2026-08-04T21:34:36.882600Z","title":"Optimizing galaxy samples for clustering measurements in photometric surveys","venue":"astro-ph.CO","work_id":"54164254-4879-494e-a465-b6146ca3c84c","year":2019},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.663843Z"},"links":{"cited_paper":"/paper/1908.07150","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:67622a227a4e48be41be22bc3c7019d27879c497bdde85c99a7885343aa0e7be","observation_id":"fa5dcdb4-a2f4-4379-8054-a1c20b97676a","resolution":{"observed_at":"2026-08-04T21:34:36.937579Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.13923","last_updated":"2021-10-26T18:00:01Z","snapshot_observed_at":"2026-07-06T12:02:11.556247Z","submitted_at":"2021-10-26T18:00:01Z","title":"COSMOS2020: A panchromatic view of the Universe to $z\\sim10$ from two complementary catalogs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.13923","snapshot_observed_at":"2026-08-04T21:34:35.802632Z","title":"R., Kauffmann , O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.802632Z"},"links":{"cited_paper":"/paper/2110.13923","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:17436ec747221c94ccf98b49f5511846d40c2c481615e461b02affe5fa7d1653","observation_id":"441c8628-9a9e-434e-8f2e-3489e4270aa8","resolution":{"observed_at":"2026-08-04T21:34:35.802632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:40.632757Z","title":null,"venue":null,"work_id":"028f45cd-5ddd-469f-a015-072501a0fbb9","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:35.920035Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:9c7938baea530e815c88882bb94c91ad8408b330944a7ccace85d221251fdb11","observation_id":"a47f6802-8120-4cdb-9985-d0f9127719d3","resolution":{"observed_at":"2026-08-04T21:34:40.699408Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-08-04T21:34:40.407639Z","title":null,"venue":null,"work_id":"b0a96ea2-57bd-487e-b091-47d10eec0864","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.047749Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:eb5cf9a6006a442fc37b0a1367e97a731700459ce756cb4635a32da51bbdcba2","observation_id":"ea43fb68-5f6d-4acb-ab5c-89bda2b227cc","resolution":{"observed_at":"2026-08-04T21:34:40.487358Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2434","last_updated":"2013-03-06T20:33:04Z","snapshot_observed_at":"2026-07-06T02:40:46.377178Z","submitted_at":"2012-01-11T22:12:48Z","title":"Observational Probes of Cosmic Acceleration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2434","snapshot_observed_at":"2026-08-04T21:34:36.177622Z","title":"H., Mortonson , M","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.177622Z"},"links":{"cited_paper":"/paper/1201.2434","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:2fb6441bf0fd4f17b178dcf946b43443aea94c456e8cce0df46ed55c0f95eac0","observation_id":"0cb2c495-31b7-46b6-81b5-0479a0200dd4","resolution":{"observed_at":"2026-08-04T21:34:36.177622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:40.193857Z","title":"R., Sheldon , E., et al., 2025","venue":null,"work_id":"24a29468-89d4-44c3-933f-95a9b9254d85","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.294659Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:23dcceba1ce5c3d69207ca11d26b3537f6fcc2c9f4f127f0f1e6c34731179d27","observation_id":"8b3d4c5b-a710-4e0a-88eb-1261efd3076c","resolution":{"observed_at":"2026-08-04T21:34:40.293131Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-08-04T21:34:40.070155Z","title":null,"venue":null,"work_id":"e3bceef0-7d0a-4233-a548-cd6d04fb98b3","year":2025},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.392467Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:be0fc7751f4d63b745da8c9de72f7cbe08b5139e7f4f1f750d0f6fdf771d1572","observation_id":"c09cb5bc-e08a-4d47-86ff-f2c66cfafb4b","resolution":{"observed_at":"2026-08-04T21:34:40.135608Z","resolver_source":"raw_fallback","status":"parse_uncertain"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3409","last_updated":"2018-04-03T13:50:52Z","snapshot_observed_at":"2026-08-04T19:52:15.282208Z","submitted_at":"2014-09-11T12:20:37Z","title":"CosmoSIS: modular cosmological parameter estimation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.3409","snapshot_observed_at":"2026-08-04T21:34:36.443316Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.443316Z"},"links":{"cited_paper":"/paper/1409.3409","citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:5d9282f02f7b31065b74b71afbda53e532c10d42a23a391cbc1436f4984f860a","observation_id":"9a976b0e-f2e0-4dcb-bf57-044c99a2b8b8","resolution":{"observed_at":"2026-08-04T21:34:36.443316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:39.938234Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":"efdc2960-4be0-4cc6-b74c-6aec8ebcaa82","year":null},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.551385Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:4e39be2ab4219e94317f75d5a52e17f6cd21baa9ec9e03006c8e155397978ef1","observation_id":"b5bc7d65-801c-4606-9040-0d8befad21fe","resolution":{"observed_at":"2026-08-04T21:34:40.000137Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+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":"2026-08-04T21:34:39.771499Z","title":"write newline","venue":null,"work_id":"1a6eefde-eef3-48bd-b804-ee2068e4f3e6","year":null},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.644692Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:47f71db3b9056f2026adaea7611132126048ff8b271c56ef0fc7cbbf74bcfc64","observation_id":"651f8296-88c7-4214-a9d2-a4a24d725e74","resolution":{"observed_at":"2026-08-04T21:34:39.866675Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T21:34:36.733183Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-04T21:34:36.733183Z"},"links":{"citing_paper":"/paper/2509.07964"},"observation_digest":"sha256:015366efc8551a0aa82727c1532b10e1fdc49d526e5d925d79ddb40aaf1540c1","observation_id":"bcead823-82dd-46ed-98cb-d01fa37d6d7d","resolution":{"observed_at":"2026-08-04T21:34:36.733183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-04T21:34:24.917286Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample"},"reference_resolution":{"displayed":74,"state_counts":{"malformed_identifier":0,"metadata_mismatch":5,"parse_uncertain":1,"unresolved":53,"verified_exact":8,"verified_fuzzy":7},"total_outbound_references":74},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 6 inbound Pith citation observations for arXiv:2509.07964."}