{"as_of":"2026-08-07T08:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2499b890bed27722c08c1fce59c90c87d92059ed9da9a9fdb6df8e87526f41bf","coverage":[{"denominator":105,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T20:53:39.258030Z","state":"measured"},{"denominator":102,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":102,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T07:32:41.605396Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":1,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"cited_work":{"arxiv_id":"2511.18133","doi":"10.48550/arxiv.2511.18133","metadata_source":"pith","pith_arxiv_id":"2511.18133","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","venue":"astro-ph.CO","work_id":"993fe5e5-f6eb-421b-b42b-9ec4d02b919b","year":2025},"citing_paper":{"arxiv_id":"2607.09943","last_updated":"2026-07-15T12:28:21Z","snapshot_observed_at":"2026-08-06T09:17:56.132825Z","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":16,"source":"arxiv_source","source_observed_at":"2026-07-14T14:25:37.540627Z"},"links":{"cited_paper":"/paper/2511.18133","citing_paper":"/paper/2607.09943"},"observation_digest":"sha256:4bd8f05cb86e23a777b5300ebde5b4d78d4a8d9b7c55405f6ee0fa159ab3638b","observation_id":"d11f71d7-83bb-412e-a76c-6ee7c021eaa1","resolution":{"observed_at":"2026-07-14T14:30:37.725644Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.18133","snapshot_observed_at":"2026-08-02T07:32:41.605396Z","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":"2026-08-06T09:17:56.132825Z","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":16,"source":"arxiv_source","source_observed_at":"2026-08-02T07:32:41.605396Z"},"links":{"cited_paper":"/paper/2511.18133","citing_paper":"/paper/2607.09943"},"observation_digest":"sha256:acd47bc20edc961bf5e90125a4fbc02129af4e0061fec83dcdb4585de9684ce0","observation_id":"0d9344f8-eab1-4b48-b08c-58c367cb4853","resolution":{"observed_at":"2026-08-02T07:32:41.605396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2511.18133/citation-record","integrity":"/paper/2511.18133/integrity","json":"/paper/2511.18133/citation-record.json","paper":"/paper/2511.18133"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T20:53:27.306306Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:27.306306Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:ca8b4bd43c5d92916c73bde88436c393c012a88e54728cbcc6a54745772e73b9","observation_id":"a6258f09-335f-46c8-a7a7-92f2dc0e9360","resolution":{"observed_at":"2026-08-03T20:53:27.306306Z","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":"2026-08-03T20:53:27.384173Z","title":"Aihara, Y","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:27.384173Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:8f41c7b997caf2e589c5be3636542d6f50a464aef562c625d02d86b09b7b1acc","observation_id":"6cb7010d-7c34-487f-8866-b148368890e8","resolution":{"observed_at":"2026-08-03T20:53:27.384173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.03181","last_updated":"2019-04-23T14:53:02Z","snapshot_observed_at":"2026-08-06T09:48:36.118398Z","submitted_at":"2018-01-09T23:18:14Z","title":"The Dark Energy Survey Data Release 1","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.03181","snapshot_observed_at":"2026-08-03T20:53:27.470789Z","title":"Abbott, F.B","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:27.470789Z"},"links":{"cited_paper":"/paper/1801.03181","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:92e6f60b3057a6566dfe2415e8b4eb5888afb21e6937c7cff092803afc25f730","observation_id":"ac54a549-9201-4075-a734-b2dbdc8a22e6","resolution":{"observed_at":"2026-08-03T20:53:27.470789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19439","last_updated":"2025-03-25T08:30:38Z","snapshot_observed_at":"2026-07-06T20:58:14.950470Z","submitted_at":"2025-03-25T08:30:38Z","title":"The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19439","snapshot_observed_at":"2026-08-03T20:53:27.596390Z","title":"Wright et al.,The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields,Astron","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:27.596390Z"},"links":{"cited_paper":"/paper/2503.19439","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:7838294de22c7925e888271789f2dbd2fa79c803b2a3400c774fc0ee2d211587","observation_id":"7c5ef4bf-d088-4f5a-b2fb-42f13a08c9d2","resolution":{"observed_at":"2026-08-03T20:53:27.596390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01174","last_updated":"2019-04-02T02:10:42Z","snapshot_observed_at":"2026-07-06T07:43:14.473925Z","submitted_at":"2019-04-02T02:10:42Z","title":"WFIRST: The Essential Cosmology Space Observatory for the Coming Decade","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.01174","snapshot_observed_at":"2026-08-03T20:53:27.683728Z","title":null,"venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:27.683728Z"},"links":{"cited_paper":"/paper/1904.01174","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:0a477ec535e5ac22546299627313bb806750ee72fb68da9d5612ec21503e6dfb","observation_id":"1c0748c0-1599-4950-b690-9c90e7c7c755","resolution":{"observed_at":"2026-08-03T20:53:27.683728Z","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":"2026-08-03T20:53:27.778942Z","title":"Mellier, Abdurro’uf, J.A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:27.778942Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:d150db4bf31dc8d873ec995fe795a792320999cdb495a7a2382bbf14c6388328","observation_id":"ec70afdc-f35a-4bba-ae3c-2578cb5d074c","resolution":{"observed_at":"2026-08-03T20:53:27.778942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.2366","last_updated":"2018-05-23T19:18:23Z","snapshot_observed_at":"2026-07-06T01:39:37.564263Z","submitted_at":"2008-05-15T18:10:13Z","title":"LSST: from Science Drivers to Reference Design and Anticipated Data Products","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.2366","snapshot_observed_at":"2026-08-03T20:53:27.842126Z","title":"Ivezić, S.M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:27.842126Z"},"links":{"cited_paper":"/paper/0805.2366","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:86cb55c1b53752b066297ea8c37d60a2c41ed1d63ee2c6e621a62e7c86f2336f","observation_id":"64f49910-9e00-4f01-b387-acfe47d6f1dd","resolution":{"observed_at":"2026-08-03T20:53:27.842126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00702","last_updated":"2023-11-30T23:20:07Z","snapshot_observed_at":"2026-08-06T08:21:34.190523Z","submitted_at":"2023-04-03T03:37:02Z","title":"Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.00702","snapshot_observed_at":"2026-08-03T20:53:28.007266Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.007266Z"},"links":{"cited_paper":"/paper/2304.00702","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:435fbf4f61a65aaa65f1fe14fafec6d60722d8c9fcca59cb61b701edf7e93792","observation_id":"52ca438a-c543-44c5-bd74-2f0f1c9c76d9","resolution":{"observed_at":"2026-08-03T20:53:28.007266Z","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":"2026-08-03T20:53:28.151920Z","title":"Dalal, X","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.151920Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:f6206f3ed27389d781f8f570e6cbdd435ebaf200acfe61642732f5e757466f45","observation_id":"c23cd764-d53a-4c45-bfff-5c8230beae57","resolution":{"observed_at":"2026-08-03T20:53:28.151920Z","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":"2026-08-03T20:53:28.323589Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.323589Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:ec063d131e56b50079529e447cba18c0854ebc4081a46ed12f139d0af04bbdda","observation_id":"b19423da-508e-41b1-b5f7-ed2dc1ab74db","resolution":{"observed_at":"2026-08-03T20:53:28.323589Z","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":"2026-08-03T20:53:28.394761Z","title":"Secco, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.394761Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:55ef34c8a6b35cc782fddeea9286d208db9b5624c8e273c6f8ffcf5b661e6004","observation_id":"ba16638b-36ac-4f96-a16b-241b958e1414","resolution":{"observed_at":"2026-08-03T20:53:28.394761Z","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":"2026-08-03T20:53:28.482530Z","title":"Asgari, C.-A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.482530Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:198c69f5475781e01a1a2d9aaf0dde4bf3a254d22e23e9cec0fa521bc35360c0","observation_id":"0faf9737-16c2-4655-a50d-9afa5597da23","resolution":{"observed_at":"2026-08-03T20:53:28.482530Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19441","last_updated":"2025-10-21T16:24:56Z","snapshot_observed_at":"2026-07-06T20:58:14.950470Z","submitted_at":"2025-03-25T08:30:40Z","title":"KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19441","snapshot_observed_at":"2026-08-03T20:53:28.558018Z","title":"Wright, B","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.558018Z"},"links":{"cited_paper":"/paper/2503.19441","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:0ab327561d636157fdb98b10c92c28c36793d626108a666dd3792fccaf28b423","observation_id":"7a533d21-c48a-43f2-9c0a-39443c9cd591","resolution":{"observed_at":"2026-08-03T20:53:28.558018Z","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":"2026-08-03T20:53:28.612845Z","title":"Ilbert, S","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.612845Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:1f7fbadf63fc54e1b30ba53ec4181252d241f90244a209b0b2344fa5be7ea912","observation_id":"df5f22af-b178-4fab-bc6a-b3e0b7bd29a3","resolution":{"observed_at":"2026-08-03T20:53:28.612845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9902290","last_updated":"1999-07-19T18:44:05Z","snapshot_observed_at":"2026-07-07T01:24:42.964930Z","submitted_at":"1999-02-19T18:56:10Z","title":"Measuring and Modelling the Redshift Evolution of Clustering: the Hubble Deep Field North","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9902290","snapshot_observed_at":"2026-08-03T20:53:28.669079Z","title":"Arnouts, S","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.669079Z"},"links":{"cited_paper":"/paper/astro-ph/9902290","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:9ddaaf41aac2e3dbd8e5de115535e6bd882f605b234d33aabc37ddac35cb479c","observation_id":"1fa0f8cc-a709-4802-82f7-7f6bdf212d99","resolution":{"observed_at":"2026-08-03T20:53:28.669079Z","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":"2026-08-03T20:53:28.771402Z","title":"Brammer, P.G","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.771402Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:c5b14ced9f3b5699b91569a7e3f16c3e6941c80992f78944f80e6649499374e6","observation_id":"612b2c01-b919-4482-bad0-239a3a76f1d6","resolution":{"observed_at":"2026-08-03T20:53:28.771402Z","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":"2026-08-03T20:53:28.893245Z","title":"Tanaka,Photometric redshift with bayesian priors on physical properties of galaxies,The Astrophysical Journal801(2015) 20","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:28.893245Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:844d1483f703963e21fccd0118e670aa16a1c8f832167fb4c380fc29eae873a1","observation_id":"f328f227-0652-4987-ac78-b3fccc646788","resolution":{"observed_at":"2026-08-03T20:53:28.893245Z","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":"2026-08-03T20:53:29.019543Z","title":"Carrasco Kind and R.J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.019543Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:bf2e9d26eab4d4afbba2acf3ede421814d9311bc6aedf6cb268a8c5542b6be32","observation_id":"9d9e6b9b-1d68-4f54-82dd-de448c23fa12","resolution":{"observed_at":"2026-08-03T20:53:29.019543Z","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":"2026-08-03T20:53:29.185888Z","title":"Hsieh and H.K.C","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.185888Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:3edb4a25cd590db8d1c41a84163af0c1d7ac511dea72fc91a970f319179c0f3a","observation_id":"d6d72837-f7f9-4eff-99dc-8392b0b7c8a8","resolution":{"observed_at":"2026-08-03T20:53:29.185888Z","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":"2026-08-03T20:53:29.264109Z","title":"Collister and O","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.264109Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:889f7c7c69cede2e4e7b60c2a4d1253f324543caa1ced522e885cb9118fc08d7","observation_id":"b550925b-a209-4ba7-b85b-53559711e666","resolution":{"observed_at":"2026-08-03T20:53:29.264109Z","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":"2026-08-03T20:53:29.431157Z","title":"Wright, H","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.431157Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:61fd4565f8ba6f8612e2a6215867425391204a2e192d192631d76574e8b5777b","observation_id":"91d1c693-2420-40cf-97a2-0773eda6c1b8","resolution":{"observed_at":"2026-08-03T20:53:29.431157Z","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":"2026-08-03T20:53:29.568698Z","title":"Wright, H","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.568698Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:d0dd3ae55218ffa6310ce217abe9034ef1ea20cd26f864af3a296066a5963cce","observation_id":"7018f549-a9a5-4614-9596-5a43261eba60","resolution":{"observed_at":"2026-08-03T20:53:29.568698Z","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":"2026-08-03T20:53:29.685317Z","title":"Campos, B","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.685317Z"},"links":{"cited_paper":"/paper/2408.00922","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:6a2c1ffa4c9c3bde92252706891dc119e7566cd67432c3ccb3a9b136b699be84","observation_id":"32b891e9-5e2c-46b8-8c41-0deef50675ef","resolution":{"observed_at":"2026-08-03T20:53:29.685317Z","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":"2026-08-03T20:53:29.793195Z","title":"Hildebrandt, J.L","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.793195Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:ca7b42a7965e7d61e68db1b1b64dae024e8d145108fc209c183d09fb0f25bdb1","observation_id":"beaf35af-5e16-478f-bc79-85f8254dacf1","resolution":{"observed_at":"2026-08-03T20:53:29.793195Z","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":"2026-08-03T20:53:29.881372Z","title":"Masters, D.K","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:29.881372Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:a2f30b2a0b39312d3cecfe93cee5c5c97716d989a05eb16f29128128977f1ce6","observation_id":"5a0061ce-9e5a-4b4f-9c02-0a6f91aa3d5a","resolution":{"observed_at":"2026-08-03T20:53:29.881372Z","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":"2026-08-03T20:53:30.036205Z","title":"Buchs, C","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.036205Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:d4df6320a345630883774396cb3609ce494f0909f9902bcb3e48ff06874c0312","observation_id":"d32a4994-d52f-4a2c-b18f-f815eeff3931","resolution":{"observed_at":"2026-08-03T20:53:30.036205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.3822","last_updated":"2008-01-24T19:10:05Z","snapshot_observed_at":"2026-07-06T01:34:45.604137Z","submitted_at":"2008-01-24T19:10:05Z","title":"Estimating the Redshift Distribution of Faint Galaxy Samples","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.3822","snapshot_observed_at":"2026-08-03T20:53:30.201260Z","title":"Lima, C.E","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.201260Z"},"links":{"cited_paper":"/paper/0801.3822","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:23b577e874de116b52e6061d57ff8603d406ecb827f77441fabec49602997b0f","observation_id":"3fe9b8eb-bcd5-4438-b0e4-7cd96755d17b","resolution":{"observed_at":"2026-08-03T20:53:30.201260Z","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":"2026-08-03T20:53:30.388234Z","title":"Newman,Calibrating redshift distributions beyond spectroscopic limits with cross-correlations,The Astrophysical Journal684(2008) 88","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.388234Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:8706e519ee60345d4d0c7493ab048c27706fda43cf5c5cc8c2f875feaaf21aa7","observation_id":"9b05204c-e436-4a56-86f6-9a299e1ecebf","resolution":{"observed_at":"2026-08-03T20:53:30.388234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.4722","last_updated":"2014-07-30T19:50:25Z","snapshot_observed_at":"2026-07-06T03:09:07.950327Z","submitted_at":"2013-03-19T19:54:26Z","title":"Clustering-based redshift estimation: method and application to data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.4722","snapshot_observed_at":"2026-08-03T20:53:30.544045Z","title":"Ménard, R","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.544045Z"},"links":{"cited_paper":"/paper/1303.4722","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:29d548db78b9fe775c1ba97484d75e36d52b0064e27ccba7970845be5c054999","observation_id":"39c5e18f-2b9d-4b59-acbb-91a3cf244cba","resolution":{"observed_at":"2026-08-03T20:53:30.544045Z","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":"2026-08-03T20:53:30.633689Z","title":"Gatti, P","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.633689Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:f3ede2beb3c2b72dcc6ab3ff5fd2561e425bdfb61bac43c39f2c4d365b257a98","observation_id":"5c37b36c-e06a-47b6-a835-ce2056377894","resolution":{"observed_at":"2026-08-03T20:53:30.633689Z","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":"2026-08-03T20:53:30.720076Z","title":"Gatti, P","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.720076Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:c2cb1bb67d3681fe96196138f477d70627fd27c8b50cadeb5a95c742b60abc72","observation_id":"408edb35-82d1-435d-9ab9-566eb3680560","resolution":{"observed_at":"2026-08-03T20:53:30.720076Z","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":"2026-08-03T20:53:30.860292Z","title":"Gatti, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.860292Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:216aed0d5923cd6de48169d780750435ff5f8f39db79fd0a9cf3bdd672f64508","observation_id":"45947a47-727d-4156-b332-0875f0242a69","resolution":{"observed_at":"2026-08-03T20:53:30.860292Z","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":"2026-08-03T20:53:30.978864Z","title":"Cawthon, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:30.978864Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:8b536e915d4e35eeb32c6842d42f180bc1d47ce9f7abb75e9ffd26fbeb26e205","observation_id":"c9812b88-efd8-468f-ad3d-a8b924429917","resolution":{"observed_at":"2026-08-03T20:53:30.978864Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.02517","last_updated":"2017-10-06T17:53:34Z","snapshot_observed_at":"2026-07-06T06:03:05.764731Z","submitted_at":"2017-10-06T17:53:34Z","title":"Dark Energy Survey Year 1 Results: Cross-Correlation Redshifts in the DES -- Calibration of the Weak Lensing Source Redshift Distributions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.02517","snapshot_observed_at":"2026-08-03T20:53:31.112323Z","title":"Davis, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.112323Z"},"links":{"cited_paper":"/paper/1710.02517","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:1a4b04ddd9be6a176ce866067f3aff958cea5c14fbe60ab653d1eee769bb498c","observation_id":"724da9be-25bc-47f0-b1c2-47f339d67f99","resolution":{"observed_at":"2026-08-03T20:53:31.112323Z","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":"2026-08-03T20:53:31.249923Z","title":"d’Assignies Doumerg, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.249923Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:5744d13f2c68755c80e0a060517d90f564c759a2233d6f54edb0a25ee5deb3e3","observation_id":"31a94cc9-c25f-48db-9d77-b9a12d489bc8","resolution":{"observed_at":"2026-08-03T20:53:31.249923Z","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":"2026-08-03T20:53:31.398973Z","title":"van den Busch, H","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.398973Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:086b2cb903b6eb57fcd591e7aee6c26f0d17549c0b5f51408b0e0fefc430a42e","observation_id":"5c678025-2913-4d9b-a905-edd627b7da7c","resolution":{"observed_at":"2026-08-03T20:53:31.398973Z","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":"2026-08-03T20:53:31.538178Z","title":"Morrison, H","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.538178Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:fc8154575f75736cd78ea376af51d7d828d409976aa6e948b029b7ae7d8cf871","observation_id":"25576a32-3f0e-407f-807f-eae8891714ec","resolution":{"observed_at":"2026-08-03T20:53:31.538178Z","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":"2026-08-03T20:53:31.694819Z","title":"Schmidt, B","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.694819Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:becee42857e57c4003a0945cc76febcb02de98e7c584c8bb4ed2552dd38f4e0c","observation_id":"6956b653-1dde-4ef6-848e-6dccc2a21927","resolution":{"observed_at":"2026-08-03T20:53:31.694819Z","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":"2026-08-03T20:53:31.767392Z","title":"McQuinn and M","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.767392Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:760606e54d0bb9d1695e921ebb8ce00ec31594439de584174dc5c544ccf4601e","observation_id":"0f330124-33a9-40aa-af75-a87be56212dd","resolution":{"observed_at":"2026-08-03T20:53:31.767392Z","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":"2026-08-03T20:53:31.888423Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.888423Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:537679b947833a40a8dad24d206449ac61dda3306517f48312f9dc6b09998d8e","observation_id":"136083e6-338e-4391-8b0b-b1c356a01e7e","resolution":{"observed_at":"2026-08-03T20:53:31.888423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14745","last_updated":"2026-03-04T20:06:20Z","snapshot_observed_at":"2026-07-30T17:13:55.599936Z","submitted_at":"2025-03-18T21:14:19Z","title":"Data Release 1 of the Dark Energy Spectroscopic Instrument","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14745","snapshot_observed_at":"2026-08-03T20:53:31.996210Z","title":"Abdul-Karim, A.G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:31.996210Z"},"links":{"cited_paper":"/paper/2503.14745","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:8d8123a16ec43ad727e55f28f4326f2cac80b672c9f2f15c0b851241b39517d2","observation_id":"09e6e49c-08be-4330-bab8-fac61184a427","resolution":{"observed_at":"2026-08-03T20:53:31.996210Z","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":"2026-08-03T20:53:32.114671Z","title":"Data Release 2 of the Dark Energy Spectroscopic Instrument","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.114671Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:e44167baa969e3f5e6fc71d5d89dc7e7d62cd53ce418540e1315bb1fbbe7077f","observation_id":"ca58d99b-818e-437b-9e9b-66a3bc745b36","resolution":{"observed_at":"2026-08-03T20:53:32.114671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00037","last_updated":"2016-12-13T16:01:58Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2016-10-31T20:47:43Z","title":"The DESI Experiment Part II: Instrument Design","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00037","snapshot_observed_at":"2026-08-03T20:53:32.244741Z","title":"Aghamousa, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.244741Z"},"links":{"cited_paper":"/paper/1611.00037","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:866e556ab0f449e9073b9c14c016d4e878caa8bac23e17945791808ed0fb41dc","observation_id":"a9f1785c-60f0-45df-833e-29f1c0c3cadc","resolution":{"observed_at":"2026-08-03T20:53:32.244741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10939","last_updated":"2022-05-22T22:13:35Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2022-05-22T22:13:35Z","title":"Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10939","snapshot_observed_at":"2026-08-03T20:53:32.338558Z","title":"Abareshi, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.338558Z"},"links":{"cited_paper":"/paper/2205.10939","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:adf0dc58b3c190172253678f9f51da41c985c122449271eba196ebff2ec9a271","observation_id":"a51fa031-4493-4344-9197-189caa2197ee","resolution":{"observed_at":"2026-08-03T20:53:32.338558Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06310","last_updated":"2023-06-09T23:55:39Z","snapshot_observed_at":"2026-08-02T01:23:20.963929Z","submitted_at":"2023-06-09T23:55:39Z","title":"The Optical Corrector for the Dark Energy Spectroscopic Instrument","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.06310","snapshot_observed_at":"2026-08-03T20:53:32.455137Z","title":"Miller, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.455137Z"},"links":{"cited_paper":"/paper/2306.06310","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:a36321709b7c33bad3c3eff2096d60262f6c5f826b65637d7791ba67848d7241","observation_id":"97b38413-78d8-49cf-9f35-62fba448b329","resolution":{"observed_at":"2026-08-03T20:53:32.455137Z","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":"2026-08-03T20:53:32.573629Z","title":"Poppett, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.573629Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:055778385aaa4ff0e304e7f86d811a07e975db20d287731c0f7401196ca1c592","observation_id":"a9944f13-5d54-4a97-bbf2-1683f2c99e7b","resolution":{"observed_at":"2026-08-03T20:53:32.573629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14482","last_updated":"2023-01-10T01:31:51Z","snapshot_observed_at":"2026-08-06T13:37:20.782152Z","submitted_at":"2022-09-29T00:26:28Z","title":"The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.14482","snapshot_observed_at":"2026-08-03T20:53:32.693211Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.693211Z"},"links":{"cited_paper":"/paper/2209.14482","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:b3948583188307fe64f2ade01856befd539b2f2a89380f11fc39405a22407f72","observation_id":"ff514039-4d8b-4411-90eb-a9a56e3e910e","resolution":{"observed_at":"2026-08-03T20:53:32.693211Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06309","last_updated":"2024-02-15T17:57:17Z","snapshot_observed_at":"2026-08-02T11:19:42.017462Z","submitted_at":"2023-06-09T23:55:38Z","title":"Survey Operations for the Dark Energy Spectroscopic Instrument","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.06309","snapshot_observed_at":"2026-08-03T20:53:32.802404Z","title":"Schlafly, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.802404Z"},"links":{"cited_paper":"/paper/2306.06309","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:0eed99e21b49c0ae52e4ed892fea800062ee5ce120fd9d5fd522d6667718c1f3","observation_id":"88767162-6308-4106-ad1d-38b668060276","resolution":{"observed_at":"2026-08-03T20:53:32.802404Z","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":"2026-08-03T20:53:32.915284Z","title":"Hahn, M.J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:32.915284Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:061f9fa73da2902ff690748bc7bb0364447b76caf55ffb0c0f6a991fdfb4f915","observation_id":"2ea11fb1-f2cb-4284-9c1e-583e6cb0a219","resolution":{"observed_at":"2026-08-03T20:53:32.915284Z","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":"2026-08-03T20:53:33.039119Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:33.039119Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:6c5ba74ef15b4a3fa1468a85863989c4fa642893804fdefb3b107e525fe1adf7","observation_id":"9c9c0561-050d-4476-aeed-6c06f1f51fd8","resolution":{"observed_at":"2026-08-03T20:53:33.039119Z","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":"2026-08-03T20:53:33.197091Z","title":"Raichoor, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:33.197091Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:f17dc0a19d61fb0af3a7ae576e68a9365ca72875562830543abdcf3cbe5944f0","observation_id":"381d6c7e-502a-4124-9320-b635ad8fe277","resolution":{"observed_at":"2026-08-03T20:53:33.197091Z","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":"2026-08-03T20:53:33.365609Z","title":"Chaussidon, C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:33.365609Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:020e9e81aee7f69c7906930175ec263992d5f38fee8292fbf2e0f943052d6f97","observation_id":"92ddd476-ed41-41d7-97f7-d66215a72ac8","resolution":{"observed_at":"2026-08-03T20:53:33.365609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-08-03T20:53:33.493831Z","title":"Abdul-Karim, J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:33.493831Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:e4a9889f30248581a6cc50b672176020a692ebececf2085b0496e0abc980da36","observation_id":"b51bdb75-2e99-4512-96ae-6f9833c86c07","resolution":{"observed_at":"2026-08-03T20:53:33.493831Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12022","last_updated":"2024-11-21T16:47:10Z","snapshot_observed_at":"2026-07-06T19:52:15.853216Z","submitted_at":"2024-11-18T20:03:35Z","title":"DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12022","snapshot_observed_at":"2026-08-03T20:53:33.615477Z","title":"Adame, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:33.615477Z"},"links":{"cited_paper":"/paper/2411.12022","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:e77e797c36b12bf2ff9cb2e8972be8a7740c51d01b90e353726717677cc9924c","observation_id":"ba3210c8-2702-43db-99d4-5d334d31807c","resolution":{"observed_at":"2026-08-03T20:53:33.615477Z","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":"2026-08-03T20:53:33.790175Z","title":"Aihara, N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:33.790175Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:a7a8d9f1ef2e075b1de709df3e5aafa2a6f3582a8838c813d272e665638f6101","observation_id":"f1fbc1f8-692f-443e-9f18-71e780a75691","resolution":{"observed_at":"2026-08-03T20:53:33.790175Z","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":"2026-08-03T20:53:33.953526Z","title":"Zhang, M.M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:33.953526Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:7555b32019e369c459b48f75ab54942c869623364918ecbbf15a73ec80c52419","observation_id":"8453c2d9-2da2-4fe0-9999-e9e192e934a6","resolution":{"observed_at":"2026-08-03T20:53:33.953526Z","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":"2026-08-03T20:53:34.101743Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:34.101743Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:7a36cfb7ecb70afb0e2d79dd37444aa02b3dea5580eb6cc778e197168b758a7b","observation_id":"544967d5-a784-4abb-9d7d-cfa6aa9448ea","resolution":{"observed_at":"2026-08-03T20:53:34.101743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.01386","last_updated":"2025-07-24T20:35:38Z","snapshot_observed_at":"2026-08-06T20:50:23.570617Z","submitted_at":"2025-07-02T06:03:29Z","title":"Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.01386","snapshot_observed_at":"2026-08-03T20:53:34.275669Z","title":"Zhang, X","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:34.275669Z"},"links":{"cited_paper":"/paper/2507.01386","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:4d74d04105364b9eea6c461d207f492c3d87dc264660e5af0bbe0da0f0952002","observation_id":"3e21502b-99ec-4164-a7cf-bbf58c5c270a","resolution":{"observed_at":"2026-08-03T20:53:34.275669Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.16593","last_updated":"2024-07-18T17:04:34Z","snapshot_observed_at":"2026-08-04T08:31:27.910188Z","submitted_at":"2024-05-26T15:07:09Z","title":"The Construction of Large-scale Structure Catalogs for the Dark Energy Spectroscopic Instrument","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.16593","snapshot_observed_at":"2026-08-03T20:53:34.388103Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:34.388103Z"},"links":{"cited_paper":"/paper/2405.16593","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:0d28d3af2370edec2b020165dd730a6d657d50116f74d05a7881bd62894c2c3e","observation_id":"f1ac0b43-0236-4388-99db-2f46af44e059","resolution":{"observed_at":"2026-08-03T20:53:34.388103Z","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":"2026-08-03T20:53:34.555348Z","title":"Adame, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:34.555348Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:7483af7491bcf591bffd3ad28cb901a39e1d83d9ac1b51e45d04ea07d8f4bf2b","observation_id":"3f56c0d7-5aa5-45b5-901b-68239c3ba843","resolution":{"observed_at":"2026-08-03T20:53:34.555348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.01511","last_updated":"2020-03-16T05:22:50Z","snapshot_observed_at":"2026-08-03T18:53:40.778565Z","submitted_at":"2020-02-29T08:03:19Z","title":"Photometric Redshifts for the Hyper Suprime-Cam Subaru Strategic Program Data Release 2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.01511","snapshot_observed_at":"2026-08-03T20:53:34.701505Z","title":"Nishizawa, B.-C","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:34.701505Z"},"links":{"cited_paper":"/paper/2003.01511","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:d2dc87acc9e9007aadf7d6569f156f5aa7054c05031191eab0347d7cb5e3a7ed","observation_id":"00b8820f-35e9-4f11-a3b5-25dfb2e5044c","resolution":{"observed_at":"2026-08-03T20:53:34.701505Z","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":"2026-08-03T20:53:34.810323Z","title":"Zhang, X","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:34.810323Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:0c68f8d1c7d9a53451ee14ab9042ba32a32534787b07bd79480c90bcaef3ee7c","observation_id":"5b7a723d-d677-4153-bd81-3dad725fe8b8","resolution":{"observed_at":"2026-08-03T20:53:34.810323Z","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":"2026-08-03T20:53:34.982904Z","title":"Tanaka, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:34.982904Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:c454878662a6ebbc606a3893859408832e3e5b484b23af79ab666592e024a567","observation_id":"8ce8c903-dda4-4a2f-8a12-035a1065ffef","resolution":{"observed_at":"2026-08-03T20:53:34.982904Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13548","last_updated":"2021-05-28T01:58:57Z","snapshot_observed_at":"2026-07-06T11:13:32.596343Z","submitted_at":"2021-05-28T01:58:57Z","title":"Dark Energy Survey Year 3 Results: Multi-Probe Modeling Strategy and Validation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13548","snapshot_observed_at":"2026-08-03T20:53:35.129864Z","title":"Krause, X","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.129864Z"},"links":{"cited_paper":"/paper/2105.13548","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:0cde60bc8d80c19ac479dab7fa7fdd0a55b54213ed383110baa363788d3a4765","observation_id":"cdb3e1aa-9457-4425-bcd1-1dbc8a4c1297","resolution":{"observed_at":"2026-08-03T20:53:35.129864Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.4973","last_updated":"2010-07-23T11:15:55Z","snapshot_observed_at":"2026-07-06T02:00:42.877269Z","submitted_at":"2009-11-26T00:04:53Z","title":"An algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.4973","snapshot_observed_at":"2026-08-03T20:53:35.291709Z","title":"Baldauf, R.E","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.291709Z"},"links":{"cited_paper":"/paper/0911.4973","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:c1116e7519860cf00eaa9b75a68b372c6af0dbcc01ed3d201a462752be73d2bd","observation_id":"a23141f7-6d34-469b-a2e8-3b2b4a382b5d","resolution":{"observed_at":"2026-08-03T20:53:35.291709Z","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":"2026-08-03T20:53:35.405825Z","title":"Limber,The Analysis of Counts of the Extragalactic Nebulae in Terms of a Fluctuating Density Field., ApJ117(1953) 134","venue":null,"work_id":null,"year":1953},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.405825Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:c692a335bfe9f95041f31345bbc76c38f5c9a04c29ccc1e0c4124b060f3a4825","observation_id":"d84566e4-0664-480a-8bca-caa399ec4c03","resolution":{"observed_at":"2026-08-03T20:53:35.405825Z","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":"2026-08-03T20:53:35.466605Z","title":"Naidoo, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.466605Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:f0b922b4bb225002cf5759eba43cf3ed4841595e8b2144f08c4a2b3985ff9b67","observation_id":"e9e3c163-b02f-49b8-b9c9-f4b3e56aca55","resolution":{"observed_at":"2026-08-03T20:53:35.466605Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14220","last_updated":"2022-06-28T18:01:54Z","snapshot_observed_at":"2026-07-06T13:25:39.576741Z","submitted_at":"2022-06-28T18:01:54Z","title":"The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.14220","snapshot_observed_at":"2026-08-03T20:53:35.572349Z","title":"Price-Whelan, P.L","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.572349Z"},"links":{"cited_paper":"/paper/2206.14220","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:e190c8b6fcdbaf4fe5e626afe8da7c30b8adb0423f77cf5bf6e224ddc07db9f0","observation_id":"9736298c-ad24-40bd-a202-e7f085fcae3c","resolution":{"observed_at":"2026-08-03T20:53:35.572349Z","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":"2026-08-03T20:53:35.720343Z","title":"Giannini, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.720343Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:61fdfc577320353d9c4269b94658d7a4a39797c038dea32620ac520706f10094","observation_id":"cddf11d2-11cd-4e10-a896-288819a1a2e3","resolution":{"observed_at":"2026-08-03T20:53:35.720343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.08209","last_updated":"2019-12-17T19:00:01Z","snapshot_observed_at":"2026-08-06T05:15:51.583856Z","submitted_at":"2019-12-17T19:00:01Z","title":"Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.08209","snapshot_observed_at":"2026-08-03T20:53:35.883744Z","title":"Nicola, D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.883744Z"},"links":{"cited_paper":"/paper/1912.08209","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:52b6d5820276d4db126673fc4f889aee915eeb2577b6a4773223f8086c92c11e","observation_id":"590325f7-cad0-49a3-8bcc-ac113a791576","resolution":{"observed_at":"2026-08-03T20:53:35.883744Z","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":"2026-08-03T20:53:35.978739Z","title":"Elvin-Poole, N","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:35.978739Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:18a73a91d454898f312861502ab3b82b24763ed5acb82c0482c305548553d433","observation_id":"18bf28ea-91b0-43f3-8da3-415b6def8883","resolution":{"observed_at":"2026-08-03T20:53:35.978739Z","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":"2026-08-03T20:53:36.101951Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:36.101951Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:27ba46d0e737a6be24007b56183ac272a6581c5a89ac2afc219ad7661c5da394","observation_id":"d19daa01-795d-4918-af7f-378ed19d6d47","resolution":{"observed_at":"2026-08-03T20:53:36.101951Z","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":"2026-08-03T20:53:36.277952Z","title":"von Wietersheim Kramsta, B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:36.277952Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:fe4820c0ca6da1ced5a202bdc72105fe99e179e994c8d1f3c4db8f7f3c06dfd4","observation_id":"da98625e-dc84-416a-83ba-34d0e667ec29","resolution":{"observed_at":"2026-08-03T20:53:36.277952Z","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":"2026-08-03T20:53:36.412619Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:36.412619Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:2eaf61a8d9cb6a417b6abacef5a2bdf264b1d80762aafb3d0e9ef636e0d18488","observation_id":"15c3a8c5-7cca-4b68-9d3c-3ed87d17c9bc","resolution":{"observed_at":"2026-08-03T20:53:36.412619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.21677","last_updated":"2025-06-26T18:02:05Z","snapshot_observed_at":"2026-08-06T22:19:14.296013Z","submitted_at":"2025-06-26T18:02:05Z","title":"Lensing Without Borders: Measurements of galaxy-galaxy lensing and projected galaxy clustering in DESI DR1","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.21677","snapshot_observed_at":"2026-08-03T20:53:36.495086Z","title":"Heydenreich, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:36.495086Z"},"links":{"cited_paper":"/paper/2506.21677","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:e0353b11766396bf6adf8a8ecf81f91c6bf7068a91b6072c5f0a1e6bf0054c8d","observation_id":"460b7106-1ac3-4647-959f-4eaab01dd84b","resolution":{"observed_at":"2026-08-03T20:53:36.495086Z","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":"2026-08-03T20:53:36.613255Z","title":"Chisari, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:36.613255Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:02e1edcc324b049a927609d4c8feff4e1c8ba58d65569eb7b1dffe141cc4d254","observation_id":"4c39b20b-a05d-4146-858f-21a4aac05fd0","resolution":{"observed_at":"2026-08-03T20:53:36.613255Z","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":"2026-08-03T20:53:36.830518Z","title":"Takahashi, M","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:36.830518Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:1faee23f452edab727c5d545f677776eea73e62bfce8ef9ec915b141a3dc261b","observation_id":"ad9847bd-1931-4d09-837a-546adbdeaf42","resolution":{"observed_at":"2026-08-03T20:53:36.830518Z","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":"2026-08-03T20:53:36.957083Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:36.957083Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:600092421e508cc23967676b8678ab1e5574acca051698e9944465f2245468b6","observation_id":"afa9a257-a614-4c94-9639-ab15b0e5c291","resolution":{"observed_at":"2026-08-03T20:53:36.957083Z","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":"2026-08-03T20:53:37.090868Z","title":"Laurent, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.090868Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:12cff48f41930d398531737ffd6af4b87de256c28f8981b29694af552dce0ed5","observation_id":"75ec63e8-d946-46ee-b52a-c6b83f1f892f","resolution":{"observed_at":"2026-08-03T20:53:37.090868Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.17623","last_updated":"2025-07-02T21:49:19Z","snapshot_observed_at":"2026-08-04T02:37:52.476982Z","submitted_at":"2024-11-26T17:34:01Z","title":"Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.17623","snapshot_observed_at":"2026-08-03T20:53:37.218840Z","title":"Chaussidon, C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.218840Z"},"links":{"cited_paper":"/paper/2411.17623","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:5df2a7cd75e317880d63de6cb3dc1a3f6680e77cac4dba7f360f3a87eedca1e7","observation_id":"4dba898c-4896-43c5-bdf6-11117b28826b","resolution":{"observed_at":"2026-08-03T20:53:37.218840Z","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":"2026-08-03T20:53:37.343390Z","title":"Adame, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.343390Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:a99a8d940e085fd50815009875ffb57055cbf25ed4c0b90625f9141d22613825","observation_id":"fa775e18-face-49af-bf70-0aa0a5c47086","resolution":{"observed_at":"2026-08-03T20:53:37.343390Z","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":"2026-08-03T20:53:37.417350Z","title":"Bosch, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.417350Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:71185a7299740969c5d39bdfc12dc9365eda863285884959a5189969f974e0ea","observation_id":"7bfa933a-1c8e-4b4d-8038-cf91d4b7a915","resolution":{"observed_at":"2026-08-03T20:53:37.417350Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.24385","last_updated":"2025-05-27T16:19:09Z","snapshot_observed_at":"2026-08-02T07:54:21.664526Z","submitted_at":"2025-03-31T17:59:47Z","title":"Evolution of structure growth during dark energy domination: Insights from the cross-correlation of DESI galaxies with CMB lensing and galaxy magnification","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.24385","snapshot_observed_at":"2026-08-03T20:53:37.532813Z","title":"Sailer, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.532813Z"},"links":{"cited_paper":"/paper/2503.24385","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:f778797aab34b44bb77acbabd857d13f8efba2178bad5b481dbfbff7bcd0582c","observation_id":"cee4cf7b-3537-4284-a7c2-d997a8a0a972","resolution":{"observed_at":"2026-08-03T20:53:37.532813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.22416","last_updated":"2025-06-27T17:42:59Z","snapshot_observed_at":"2026-08-06T22:01:35.738095Z","submitted_at":"2025-06-27T17:42:59Z","title":"Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.22416","snapshot_observed_at":"2026-08-03T20:53:37.694659Z","title":"de Belsunce, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.694659Z"},"links":{"cited_paper":"/paper/2506.22416","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:ccf704e669a771666b12a084ecccb9936143d5e209af654a916283ea4a0bd9c9","observation_id":"b7f57b1b-4fe9-40d3-9fa6-a616b5414327","resolution":{"observed_at":"2026-08-03T20:53:37.694659Z","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":"2026-08-03T20:53:37.842054Z","title":"Sinha and L.H","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.842054Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:a2c6040a573610b6ea7b54913d58e516c1c3595f6efaa909ade73ef8e1b5f837","observation_id":"63a55e54-97d3-4466-b1ed-b791ae948dae","resolution":{"observed_at":"2026-08-03T20:53:37.842054Z","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":"2026-08-03T20:53:37.949424Z","title":"Sinha and L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:37.949424Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:edb4257e32c81218b339eb4883ca6d8869bdc79ce8f85a586012ee091983c5c5","observation_id":"a8abacc1-667e-467d-8354-688e6a953773","resolution":{"observed_at":"2026-08-03T20:53:37.949424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.02937","last_updated":"2015-05-12T09:53:17Z","snapshot_observed_at":"2026-08-02T22:08:51.654750Z","submitted_at":"2015-05-12T09:53:17Z","title":"MOC - HEALPix Multi-Order Coverage map Version 1.0","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.02937","snapshot_observed_at":"2026-08-03T20:53:38.106506Z","title":"Fernique, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.106506Z"},"links":{"cited_paper":"/paper/1505.02937","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:7233e59918d52ee79e4bf4a1f41be598fd09cb6200b18b463024bba191798f84","observation_id":"e9c6a89f-4cfb-4edf-a79d-0bbc86b9b6b5","resolution":{"observed_at":"2026-08-03T20:53:38.106506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9304022","last_updated":"1993-04-26T15:26:48Z","snapshot_observed_at":"2026-08-07T07:32:29.145981Z","submitted_at":"1993-04-26T15:26:48Z","title":"Power Spectrum Analysis of Three-Dimensional Redshift Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9304022","snapshot_observed_at":"2026-08-03T20:53:38.233486Z","title":"Feldman, N","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.233486Z"},"links":{"cited_paper":"/paper/astro-ph/9304022","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:5d0e8da00c3952c4af3325c7aad3987623d148b53aea8190796841cb4182814b","observation_id":"1d0b8afa-da83-4de1-9bac-5dab4803afbf","resolution":{"observed_at":"2026-08-03T20:53:38.233486Z","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":"2026-08-03T20:53:38.310510Z","title":"Bianchi and W.J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.310510Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:475a1b5c67fbc0aa6f0ce12436a84d55e0e1aec881695bf179df39d449ecb3c3","observation_id":"dbb93fe8-5a7f-43a4-81d4-a5d71b915ba5","resolution":{"observed_at":"2026-08-03T20:53:38.310510Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12025","last_updated":"2025-05-02T14:37:09Z","snapshot_observed_at":"2026-07-06T19:52:15.853216Z","submitted_at":"2024-11-18T20:03:38Z","title":"Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12025","snapshot_observed_at":"2026-08-03T20:53:38.374099Z","title":"Bianchi, M.M.S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.374099Z"},"links":{"cited_paper":"/paper/2411.12025","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:2fe6e79ea852616a1acfefe98c25348d05b0f9b954ca49e35b302ccca50f53b9","observation_id":"931cdc3d-d0a9-45cf-9dae-fcaa6773a616","resolution":{"observed_at":"2026-08-03T20:53:38.374099Z","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":"2026-08-03T20:53:38.486821Z","title":"Pinon, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.486821Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:3a9f827cb5808afa3c98a08e6a8b4092deb354b0332141f563bd8860260d41b6","observation_id":"e07c7b73-9ac8-4f1f-a057-ac75a41a5655","resolution":{"observed_at":"2026-08-03T20:53:38.486821Z","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":"2026-08-03T20:53:38.575145Z","title":"Mohammad and W.J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.575145Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:fc2da7ad4c94658e770b55ea284db2df4bfa1f32d928473a3e3f0b9bea5e47ec","observation_id":"b5a48735-1f5e-41ea-9872-d6d65cab2eb1","resolution":{"observed_at":"2026-08-03T20:53:38.575145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409513","last_updated":"2004-09-21T18:00:00Z","snapshot_observed_at":"2026-07-07T00:44:53.460945Z","submitted_at":"2004-09-21T18:00:00Z","title":"HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409513","snapshot_observed_at":"2026-08-03T20:53:38.658510Z","title":"Górski, E","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.658510Z"},"links":{"cited_paper":"/paper/astro-ph/0409513","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:32f336f5c6282d47bfd719ce576e595fe8687489ad1440403dfd778e2cff3fa8","observation_id":"38231a0d-dda9-474c-95bf-a4b20d673f46","resolution":{"observed_at":"2026-08-03T20:53:38.658510Z","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":"2026-08-03T20:53:38.756308Z","title":"Davis and P.J.E","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.756308Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:bd99f001d91d6b581ea9472e5f5858eddcf394f38af1ac6e85199a156250c3cb","observation_id":"74bfbe51-a82b-4ff7-9998-93f25f54811a","resolution":{"observed_at":"2026-08-03T20:53:38.756308Z","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":"2026-08-03T20:53:38.873467Z","title":"Landy and A.S","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.873467Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:008fd4cce4ff8a4ac0afc508a3836e0d10d099e042a7d74f1c4ef6951b28f062","observation_id":"a5d3b87a-5eec-402a-804a-2c2443a1ad40","resolution":{"observed_at":"2026-08-03T20:53:38.873467Z","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":"2026-08-03T20:53:38.978323Z","title":"Rau, C.B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:38.978323Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:36d74094be70e09144dc570466662166755266ecba6703ae016c06c5e33ff778","observation_id":"f42caa70-45e4-4b1e-9dac-04320a4d695b","resolution":{"observed_at":"2026-08-03T20:53:38.978323Z","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":"2026-08-03T20:53:39.042786Z","title":"Pedregosa, G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:39.042786Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:bb3e3462e3efaed86468920d289ea10d83ac86026d882f07afec78d14d45c7c0","observation_id":"fc13c984-1de8-41ff-8b9a-721a46398eef","resolution":{"observed_at":"2026-08-03T20:53:39.042786Z","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":"2026-08-03T20:53:39.103266Z","title":"Abril-Pla, V","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:39.103266Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:08639769d0d79af0aa01eb20b5130d750bc1cb1c05b519e167017eb92496f26f","observation_id":"1ad12111-74cb-4848-a880-8ca61751853c","resolution":{"observed_at":"2026-08-03T20:53:39.103266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01075","last_updated":"2016-08-03T05:28:37Z","snapshot_observed_at":"2026-08-03T07:39:07.066384Z","submitted_at":"2016-08-03T05:28:37Z","title":"Prime Focus Spectrograph (PFS) for the Subaru Telescope: Overview, recent progress, and future perspectives","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01075","snapshot_observed_at":"2026-08-03T20:53:39.185536Z","title":"Tamura, N","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:39.185536Z"},"links":{"cited_paper":"/paper/1608.01075","citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:4faaa542007664c8515156fb63e8a9bc69cc2dc47d585cc56fd7b6f059d81e8d","observation_id":"af1aabc5-ccff-4018-b006-2bb05651554f","resolution":{"observed_at":"2026-08-03T20:53:39.185536Z","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":"2026-08-03T20:53:39.258030Z","title":"Cosmic Shear constraints from HSC Year 3 with complete calibration of the tomographic redshift distributions","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-03T20:53:39.258030Z"},"links":{"citing_paper":"/paper/2511.18133"},"observation_digest":"sha256:69fad8512272eb0d160a43957906e7f03a0b7cf7ac82afa84f43be5d34cba408","observation_id":"05fa1fa9-0de7-4638-bf00-2f55190729df","resolution":{"observed_at":"2026-08-03T20:53:39.258030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2511.18133","last_updated":"2026-03-30T15:45:56Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-03T20:53:25.545706Z","submitted_at":"2025-11-22T17:32:47Z","title":"Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":100,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":105},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 100 of 105 outbound references and 2 inbound Pith citation observations for arXiv:2511.18133."}