{"as_of":"2026-08-08T04:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:69db1e956c363b30b1b7b3643be3e03608c488a2ca167c26f7ca0edb8c6dee65","coverage":[{"denominator":47,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":47,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:06:29.022447Z","state":"measured"},{"denominator":47,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":47,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.16420/citation-record","integrity":"/paper/2505.16420/integrity","json":"/paper/2505.16420/citation-record.json","paper":"/paper/2505.16420"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2310.15053","last_updated":"2024-12-04T06:07:08Z","snapshot_observed_at":"2026-07-06T16:37:16.106127Z","submitted_at":"2023-10-23T15:55:56Z","title":"Weak Lensing Reconstruction by Counting DECaLS Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.15053","snapshot_observed_at":"2026-08-07T15:06:25.899575Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:25.899575Z"},"links":{"cited_paper":"/paper/2310.15053","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:86ef58107588a888c3a836319f6e6924cce7e7693cb56e838ff5eb09b5332d71","observation_id":"3b053cc6-4e9d-45aa-92ce-88506df70d60","resolution":{"observed_at":"2026-08-07T15:06:25.899575Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.00829","last_updated":"2024-12-01T14:33:09Z","snapshot_observed_at":"2026-07-06T19:59:42.424537Z","submitted_at":"2024-12-01T14:33:09Z","title":"Weak Lensing Reconstruction by Counting Galaxies: Improvement with DES Y3 Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.00829","snapshot_observed_at":"2026-08-07T15:06:25.924473Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:25.924473Z"},"links":{"cited_paper":"/paper/2412.00829","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:1c622d8c3b44654aea0ccdefc8aca816b3c10fcc90b4e89516f9a97ae5f945da","observation_id":"4f9a55db-313a-4721-bc76-a9114b1a6649","resolution":{"observed_at":"2026-08-07T15:06:25.924473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9912508","last_updated":"1999-12-23T23:20:38Z","snapshot_observed_at":"2026-08-05T12:09:14.357181Z","submitted_at":"1999-12-23T23:20:38Z","title":"Weak Gravitational Lensing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9912508","snapshot_observed_at":"2026-08-07T15:06:25.963297Z","title":"Bartelmann and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:25.963297Z"},"links":{"cited_paper":"/paper/astro-ph/9912508","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:60fb40571885a705bb67b5775201bdf882a7e118ff1e123e17870b031fad3e42","observation_id":"11e2e183-9c02-4256-9879-9087961a96d9","resolution":{"observed_at":"2026-08-07T15:06:25.963297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.0115","last_updated":"2015-07-21T13:37:34Z","snapshot_observed_at":"2026-08-04T04:32:12.131626Z","submitted_at":"2014-11-01T13:18:26Z","title":"Cosmology with cosmic shear observations: a review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.0115","snapshot_observed_at":"2026-08-07T15:06:26.002544Z","title":"Kilbinger, Reports on Progress in Physics78, 086901 (2015), 1411.0115","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.002544Z"},"links":{"cited_paper":"/paper/1411.0115","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:8ee573ad09f37d53d5aae55b3ba7d95a15074a04faa7467b1b60bbb736771242","observation_id":"8bae2aa2-23af-4a8b-9c4c-264a9182da1a","resolution":{"observed_at":"2026-08-07T15:06:26.002544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.06041","last_updated":"2022-01-10T05:23:03Z","snapshot_observed_at":"2026-08-06T00:16:20.275837Z","submitted_at":"2019-06-14T06:12:37Z","title":"Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.06041","snapshot_observed_at":"2026-08-07T15:06:26.034409Z","title":"Hamana, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.034409Z"},"links":{"cited_paper":"/paper/1906.06041","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:ee8193789aa89fc2cad9bf3bb3c54945ed18580c295d86c81120483016e4e393","observation_id":"2a0918c2-7900-4894-b469-08c480f18ec1","resolution":{"observed_at":"2026-08-07T15:06:26.034409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.15633","last_updated":"2020-10-13T16:23:19Z","snapshot_observed_at":"2026-07-06T09:43:17.065349Z","submitted_at":"2020-07-30T17:54:56Z","title":"KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.15633","snapshot_observed_at":"2026-08-07T15:06:26.069164Z","title":"Asgari, C.-A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.069164Z"},"links":{"cited_paper":"/paper/2007.15633","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:c144529c6f9df2dcf880fc0142964a17e2319adccba44c12e046dd2f8f58fc0e","observation_id":"687e2ddc-b3b3-4cf9-a677-1912d22f77c8","resolution":{"observed_at":"2026-08-07T15:06:26.069164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.01845","last_updated":"2020-12-08T17:49:59Z","snapshot_observed_at":"2026-08-06T10:02:12.540899Z","submitted_at":"2020-07-03T17:54:18Z","title":"KiDS-1000 catalogue: Weak gravitational lensing shear measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.01845","snapshot_observed_at":"2026-08-07T15:06:26.105117Z","title":"Giblin, C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.105117Z"},"links":{"cited_paper":"/paper/2007.01845","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:0d3c7cccdf6caec54364f0e2ac0ccf7dda5acb20349a671661632144e2c3da8a","observation_id":"d91e6f29-e43d-44fa-9ff2-293858a30518","resolution":{"observed_at":"2026-08-07T15:06:26.105117Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.06947","last_updated":"2022-07-04T14:09:32Z","snapshot_observed_at":"2026-07-06T11:57:35.819061Z","submitted_at":"2021-10-13T18:00:03Z","title":"KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.06947","snapshot_observed_at":"2026-08-07T15:06:26.135709Z","title":"Loureiro, L","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.135709Z"},"links":{"cited_paper":"/paper/2110.06947","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:8f774ffac016e5c3b7d070e4368503b17b0adc61eb9208b9ced7b6fa0e41fb41","observation_id":"6f43593d-e8ee-4386-853f-ae3029facc7d","resolution":{"observed_at":"2026-08-07T15:06:26.135709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:06:30.323735Z","title":null,"venue":null,"work_id":"9aa81983-2247-4c12-a965-d2f9b7b214b3","year":2022},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.169505Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:ea7a9fa7a21283f142338fd08b3b706d666f73b7f729b9908c858846d392d179","observation_id":"ab179b23-d948-4814-aa27-7a25976d6bbd","resolution":{"observed_at":"2026-08-07T15:06:30.327238Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:06:26.205065Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.205065Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:2e978125952c8aa78b29f2f940988aa6009c7a069468f3e62dae16b53dd66730","observation_id":"4bb41346-982f-440d-9b13-f85af890358d","resolution":{"observed_at":"2026-08-07T15:06:26.205065Z","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":"2026-08-07T15:06:26.241195Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.241195Z"},"links":{"cited_paper":"/paper/2304.00702","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:448153d1950d86a993384d8f449b845e16dfcb01281f5245faebd04b0486c4fe","observation_id":"75f7650c-e23d-4e29-b58b-f59db8841338","resolution":{"observed_at":"2026-08-07T15:06:26.241195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.00329","last_updated":"2016-08-19T15:43:52Z","snapshot_observed_at":"2026-08-03T02:40:21.221368Z","submitted_at":"2016-01-03T19:33:10Z","title":"The Dark Energy Survey: more than dark energy - an overview","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.00329","snapshot_observed_at":"2026-08-07T15:06:26.292038Z","title":"Abbott, F","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.292038Z"},"links":{"cited_paper":"/paper/1601.00329","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:15f7cc26d66602bd8c4a784dc8c23f83ed0605144d3edeb1537bc26ccb9189af","observation_id":"b3b06098-5efe-4863-9377-83eb4f3e2f03","resolution":{"observed_at":"2026-08-07T15:06:26.292038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.1254","last_updated":"2012-06-06T15:09:34Z","snapshot_observed_at":"2026-07-06T02:49:27.098589Z","submitted_at":"2012-06-06T15:09:34Z","title":"The Kilo-Degree Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.1254","snapshot_observed_at":"2026-08-07T15:06:26.327839Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.327839Z"},"links":{"cited_paper":"/paper/1206.1254","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:8e06f0f3992bb253c25afba0a83c5f2cc601a6fa2ba8de22f2f5c65f5135bd33","observation_id":"253c6303-0652-4e9d-a09b-9d23a93db7a7","resolution":{"observed_at":"2026-08-07T15:06:26.327839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.05858","last_updated":"2018-03-15T06:15:14Z","snapshot_observed_at":"2026-07-06T05:38:27.260025Z","submitted_at":"2017-04-19T18:00:51Z","title":"The Hyper Suprime-Cam SSP Survey: Overview and Survey Design","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.05858","snapshot_observed_at":"2026-08-07T15:06:26.367608Z","title":"Aihara, N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.367608Z"},"links":{"cited_paper":"/paper/1704.05858","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:3220efbb842971ff45caf5d8b774dae1875b927c4b98f419d2c296c92675e42a","observation_id":"94320155-468d-45d9-afab-9e067d7c725a","resolution":{"observed_at":"2026-08-07T15:06:26.367608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.0201","last_updated":"2009-12-01T16:50:56Z","snapshot_observed_at":"2026-08-01T23:00:33.711522Z","submitted_at":"2009-12-01T16:50:56Z","title":"LSST Science Book, Version 2.0","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.0201","snapshot_observed_at":"2026-08-07T15:06:26.401676Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.401676Z"},"links":{"cited_paper":"/paper/0912.0201","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:56c494e618cda308ffa764af63e16ab06756f138180685b70139279b8d115b14","observation_id":"146a541d-d31a-4216-a42b-231cec0456d2","resolution":{"observed_at":"2026-08-07T15:06:26.401676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.3193","last_updated":"2011-10-14T12:57:07Z","snapshot_observed_at":"2026-07-06T02:35:48.625634Z","submitted_at":"2011-10-14T12:57:07Z","title":"Euclid Definition Study Report","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.3193","snapshot_observed_at":"2026-08-07T15:06:26.439645Z","title":"Laureijs, J","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.439645Z"},"links":{"cited_paper":"/paper/1110.3193","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:ee9f7799d677eee3178cb1b18c50bd7cbfb76d403126c63430a5af8fab779045","observation_id":"7da0a730-1186-44fe-86fe-daf3e8e5817d","resolution":{"observed_at":"2026-08-07T15:06:26.439645Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.04634","last_updated":"2019-08-07T15:33:57Z","snapshot_observed_at":"2026-07-06T07:26:43.370262Z","submitted_at":"2019-01-15T01:54:59Z","title":"Cosmology from the Chinese Space Station Optical Survey (CSS-OS)","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.04634","snapshot_observed_at":"2026-08-07T15:06:26.476077Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.476077Z"},"links":{"cited_paper":"/paper/1901.04634","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:4efd12d2b2ea7835be1e114207717a9b9deb95c77b3489864945b5ed0460a60f","observation_id":"dc8fb9e0-5679-4138-a41c-569c752f7903","resolution":{"observed_at":"2026-08-07T15:06:26.476077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.04489","last_updated":"2023-11-16T09:37:43Z","snapshot_observed_at":"2026-08-06T10:38:40.803079Z","submitted_at":"2023-04-10T10:02:13Z","title":"CSST WL preparation I: forecast the impact from non-Gaussian covariances and requirements on systematics-control","version":2},"cited_work":{"arxiv_id":"2304.04489","doi":null,"metadata_source":"pith","pith_arxiv_id":"2304.04489","snapshot_observed_at":"2026-08-07T15:06:29.603339Z","title":"CSST WL preparation I: forecast the impact from non-Gaussian covariances and requirements on systematics-control","venue":"astro-ph.CO","work_id":"8bb301fa-3985-4238-90e1-c8fb982e37b4","year":2023},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.516630Z"},"links":{"cited_paper":"/paper/2304.04489","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:5a3159f6d109837216dd8b6df6a15932076a477ec254b19c2c4dda2723f8ac74","observation_id":"636f81fa-94c2-468e-9857-4fc86f20de8c","resolution":{"observed_at":"2026-08-07T15:06:29.627699Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:06:30.313229Z","title":null,"venue":null,"work_id":"a8eaed6e-3923-49e2-bc76-b997489ed0f0","year":2014},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.593293Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:eb41530c76721c35918ec971645abf126ce3980177f9b2685591cabadbbd8295","observation_id":"df0567d4-fa8b-4331-b210-03cbc8e76c95","resolution":{"observed_at":"2026-08-07T15:06:30.316556Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"1810.02827","last_updated":"2019-01-08T11:32:32Z","snapshot_observed_at":"2026-07-06T07:06:22.752245Z","submitted_at":"2018-10-05T18:00:05Z","title":"AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.02827","snapshot_observed_at":"2026-08-07T15:06:26.688846Z","title":"Bellagamba, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.688846Z"},"links":{"cited_paper":"/paper/1810.02827","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:d1f6df56805147914d706a30b19fa22c69614ec50520542ef384e609c71e5d9f","observation_id":"05b8ed9b-fac7-4b5e-a0d1-3c2c19924dbb","resolution":{"observed_at":"2026-08-07T15:06:26.688846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.01745","last_updated":"2016-02-09T14:45:54Z","snapshot_observed_at":"2026-07-06T04:32:14.932562Z","submitted_at":"2015-10-06T20:09:08Z","title":"Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters","version":2},"cited_work":{"arxiv_id":"1510.01745","doi":null,"metadata_source":"pith","pith_arxiv_id":"1510.01745","snapshot_observed_at":"2026-08-07T15:06:29.541030Z","title":"Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters","venue":"astro-ph.CO","work_id":"e2f9d0c9-04c4-4b5e-a2b8-929df9775272","year":2015},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.750513Z"},"links":{"cited_paper":"/paper/1510.01745","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:25f72800452f91dae67083cfaed706993795dfc89bed8838035865d4b1b86948","observation_id":"f56673ee-a302-49db-b206-78dd3b9560b5","resolution":{"observed_at":"2026-08-07T15:06:29.556041Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"1909.02042","last_updated":"2020-04-23T12:28:49Z","snapshot_observed_at":"2026-07-06T08:19:12.871715Z","submitted_at":"2019-09-04T18:34:32Z","title":"The Richness-to-Mass Relation of CAMIRA Galaxy Clusters from Weak-lensing Magnification in the Subaru Hyper Suprime-Cam Survey","version":2},"cited_work":{"arxiv_id":"1909.02042","doi":null,"metadata_source":"pith","pith_arxiv_id":"1909.02042","snapshot_observed_at":"2026-08-07T15:06:29.510186Z","title":"The Richness-to-Mass Relation of CAMIRA Galaxy Clusters from Weak-lensing Magnification in the Subaru Hyper Suprime-Cam Survey","venue":"astro-ph.CO","work_id":"5c952d05-0ae1-451a-8f92-1e8ba0eabfef","year":2019},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.762881Z"},"links":{"cited_paper":"/paper/1909.02042","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:a38f7b763b23315b42d2ce33310b89094177036d3fec56705230ecfef5fe601b","observation_id":"7cda6582-5be2-48ec-8c6c-03cd50e5fc28","resolution":{"observed_at":"2026-08-07T15:06:29.522061Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"astro-ph/0504510","last_updated":"2005-04-22T20:57:27Z","snapshot_observed_at":"2026-07-07T00:50:05.971981Z","submitted_at":"2005-04-22T20:57:27Z","title":"Detection of Cosmic Magnification with the Sloan Digital Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504510","snapshot_observed_at":"2026-08-07T15:06:26.812088Z","title":"Scranton, B","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.812088Z"},"links":{"cited_paper":"/paper/astro-ph/0504510","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:1bf7a699920a4269cb6a2b96fe60a962da91f3e26c3aab14dccb27c3e05afb2a","observation_id":"61be3047-e1d7-48d6-b1d4-a993bd2c4e55","resolution":{"observed_at":"2026-08-07T15:06:26.812088Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.1371","last_updated":"2012-02-07T08:43:59Z","snapshot_observed_at":"2026-07-06T02:42:27.375503Z","submitted_at":"2012-02-07T08:43:59Z","title":"The Mass-Richness Relation of MaxBCG Clusters from Quasar Lensing Magnification using Variability","version":1},"cited_work":{"arxiv_id":"1202.1371","doi":null,"metadata_source":"pith","pith_arxiv_id":"1202.1371","snapshot_observed_at":"2026-08-07T15:06:29.483860Z","title":"The Mass-Richness Relation of MaxBCG Clusters from Quasar Lensing Magnification using Variability","venue":"astro-ph.CO","work_id":"aeb9a429-9eb7-44d8-a0be-9167e2b7ca3a","year":2012},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.873935Z"},"links":{"cited_paper":"/paper/1202.1371","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:e01e166489051cbcea9fa5df2c1e4105df0de269c9ab1fa377659f7f1a4fac61","observation_id":"da6e1b52-0537-4ef5-8b01-664351d63485","resolution":{"observed_at":"2026-08-07T15:06:29.487356Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"1204.2830","last_updated":"2012-09-13T21:26:36Z","snapshot_observed_at":"2026-07-06T02:46:14.301558Z","submitted_at":"2012-04-12T20:00:06Z","title":"Tomographic Magnification of Lyman Break Galaxies in The Deep Lens Survey","version":3},"cited_work":{"arxiv_id":"1204.2830","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.2830","snapshot_observed_at":"2026-08-07T15:06:29.469052Z","title":"Tomographic Magnification of Lyman Break Galaxies in The Deep Lens Survey","venue":"astro-ph.CO","work_id":"400793d8-e0b8-4ae7-936d-cfedb87f562d","year":2012},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:26.999949Z"},"links":{"cited_paper":"/paper/1204.2830","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:6e16624ac4706d387bcf7c575cb19a10aeaba9688646dcf97b1049ebc98c4afa","observation_id":"3cb82de6-f275-4131-9921-c0da9ac85888","resolution":{"observed_at":"2026-08-07T15:06:29.473081Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"1710.06431","last_updated":"2017-10-17T18:00:00Z","snapshot_observed_at":"2026-07-06T06:04:43.542218Z","submitted_at":"2017-10-17T18:00:00Z","title":"Weak lensing magnification of SpARCS galaxy clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.06431","snapshot_observed_at":"2026-08-07T15:06:27.070422Z","title":"Tudorica, H","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.070422Z"},"links":{"cited_paper":"/paper/1710.06431","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:69890e5613809f9031455c1c459e8ffedf2ad8589dd5cb71eb0dc5f083d078d3","observation_id":"28ebd9de-5239-431f-9dca-f4fe587084a4","resolution":{"observed_at":"2026-08-07T15:06:27.070422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.12413","last_updated":"2021-12-06T11:17:16Z","snapshot_observed_at":"2026-07-06T11:51:18.430663Z","submitted_at":"2021-09-25T18:08:10Z","title":"Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis","version":2},"cited_work":{"arxiv_id":"2109.12413","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.12413","snapshot_observed_at":"2026-08-07T15:06:29.442366Z","title":"Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis","venue":"astro-ph.CO","work_id":"b2576183-53d5-47c5-91e1-a00121677b74","year":2021},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.124784Z"},"links":{"cited_paper":"/paper/2109.12413","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:342a85a85016c5eecb697e2562c9b971e52d0b09d77bc774572fc46e8429b34a","observation_id":"709848a7-9a40-45cb-bc02-e7e89a241cf7","resolution":{"observed_at":"2026-08-07T15:06:29.446173Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2210.17318","last_updated":"2022-10-27T19:10:28Z","snapshot_observed_at":"2026-07-06T14:12:33.414276Z","submitted_at":"2022-10-27T19:10:28Z","title":"Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias","version":1},"cited_work":{"arxiv_id":"2210.17318","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.17318","snapshot_observed_at":"2026-08-07T15:06:29.427788Z","title":"Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias","venue":"astro-ph.GA","work_id":"a98f9211-0e98-4526-8611-def40f94f226","year":2022},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.215039Z"},"links":{"cited_paper":"/paper/2210.17318","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:e2e0f21efd0f4bfd06c18d6a37917429a4ddb966b0b68b182b9a02c56b2722b5","observation_id":"9f585b04-6afb-455d-ad6b-4b7ffc23d37c","resolution":{"observed_at":"2026-08-07T15:06:29.431875Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"astro-ph/0506740","last_updated":"2005-11-08T11:59:25Z","snapshot_observed_at":"2026-07-07T00:51:50.177555Z","submitted_at":"2005-06-29T20:31:38Z","title":"Mapping dark matter with cosmic magnification","version":2},"cited_work":{"arxiv_id":"astro-ph/0506740","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0506740","snapshot_observed_at":"2026-08-07T15:06:29.412837Z","title":"Mapping dark matter with cosmic magnification","venue":"astro-ph","work_id":"93c262f4-615e-4f20-a5dc-a56cd65de349","year":2005},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.299746Z"},"links":{"cited_paper":"/paper/astro-ph/0506740","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:87478239b3707e5fb3bc0d9a9a1ff3a60d94c8f6012b2ae8af2ebf803be177d0","observation_id":"b09f8bcd-94f9-41fc-8c9b-c4c6f7512ca6","resolution":{"observed_at":"2026-08-07T15:06:29.416948Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"1105.2385","last_updated":"2012-02-15T07:46:26Z","snapshot_observed_at":"2026-07-06T02:27:37.801656Z","submitted_at":"2011-05-12T07:05:00Z","title":"Weak lensing reconstruction through cosmic magnification I: a minimal variance map reconstruction","version":3},"cited_work":{"arxiv_id":"1105.2385","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.2385","snapshot_observed_at":"2026-08-07T15:06:29.399742Z","title":"Weak lensing reconstruction through cosmic magnification I: a minimal variance map reconstruction","venue":"astro-ph.CO","work_id":"a734cd06-593f-469e-9f34-b02c9b284565","year":2011},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.377397Z"},"links":{"cited_paper":"/paper/1105.2385","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:14065f0521eeb77b9cc08e54b4f5c062e62ca0d4fbf05e3bc9620188032f1200","observation_id":"b8ba582e-1ef5-45ed-a997-1277dcdff2c9","resolution":{"observed_at":"2026-08-07T15:06:29.403302Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:06:30.263584Z","title":"Zhang, J","venue":null,"work_id":"941f651d-7d86-4fb7-b2c3-9a65078d5d4a","year":2019},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.467860Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:ceadcc4fa15eb9e3a8079b483f27abdea2e7560cf0de4f879fefa6ba4bdf98b2","observation_id":"2dac0e59-44fc-4566-8ebb-0a47a99f4ce7","resolution":{"observed_at":"2026-08-07T15:06:30.293940Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:06:30.049554Z","title":null,"venue":null,"work_id":"1c7903df-d510-4a80-99c2-316fe480f712","year":2015},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.580662Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:9e2406a6ee584a83d7286b3db6af6d1a867fa9eaa1ea4e028a702d5395756e85","observation_id":"cf46d35c-eb6c-42ce-8b9c-3dd1254e392b","resolution":{"observed_at":"2026-08-07T15:06:30.166449Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"1703.01575","last_updated":"2017-08-21T02:23:18Z","snapshot_observed_at":"2026-07-06T05:32:25.007407Z","submitted_at":"2017-03-05T09:29:04Z","title":"Weak lensing power spectrum reconstruction by counting galaxies.-- I: the ABS method","version":2},"cited_work":{"arxiv_id":"1703.01575","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.01575","snapshot_observed_at":"2026-08-07T15:06:29.386055Z","title":"Weak lensing power spectrum reconstruction by counting galaxies.-- I: the ABS method","venue":"astro-ph.CO","work_id":"01638370-3afa-410b-871f-7312969d9f1a","year":2017},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.633554Z"},"links":{"cited_paper":"/paper/1703.01575","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:4cbae66d923921209fbbcc111db224929ecd5e35bfcf541d7b91a11924e7ad55","observation_id":"6bf7b1b0-fe54-438f-9c08-14e70f925d3f","resolution":{"observed_at":"2026-08-07T15:06:29.389758Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"1807.00443","last_updated":"2018-07-02T02:55:21Z","snapshot_observed_at":"2026-07-06T06:47:50.324458Z","submitted_at":"2018-07-02T02:55:21Z","title":"Weak lensing power spectrum reconstruction by counting galaxies.-- II: Improving the ABS method with the shift parameter","version":1},"cited_work":{"arxiv_id":"1807.00443","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.00443","snapshot_observed_at":"2026-08-07T15:06:29.371320Z","title":"Weak lensing power spectrum reconstruction by counting galaxies.-- II: Improving the ABS method with the shift parameter","venue":"astro-ph.CO","work_id":"980f66a3-378c-4526-81d8-17fafb1ae6bf","year":2018},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.699598Z"},"links":{"cited_paper":"/paper/1807.00443","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:e371ab48668f825733218e35ac0d12f5d0c6f4919c677eada4750a362bc417d7","observation_id":"d3ab1727-a205-4713-9148-3b7cb5ecd4c8","resolution":{"observed_at":"2026-08-07T15:06:29.375081Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2106.09970","last_updated":"2021-10-22T05:13:07Z","snapshot_observed_at":"2026-07-06T11:20:35.920607Z","submitted_at":"2021-06-18T07:52:06Z","title":"Weak Lensing Magnification Reconstruction with the Modified Internal Linear Combination Method","version":2},"cited_work":{"arxiv_id":"2106.09970","doi":null,"metadata_source":"pith","pith_arxiv_id":"2106.09970","snapshot_observed_at":"2026-08-07T15:06:29.357474Z","title":"Weak Lensing Magnification Reconstruction with the Modified Internal Linear Combination Method","venue":"astro-ph.CO","work_id":"58ba4207-f373-4d34-8369-08b279f94cab","year":2021},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.803394Z"},"links":{"cited_paper":"/paper/2106.09970","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:447a2343666bdfcce684010cb175a60ad9514dda683a0d22bf6119bddab39a72","observation_id":"0e1fd929-b916-4e04-8f74-4bd97085500d","resolution":{"observed_at":"2026-08-07T15:06:29.361348Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2306.15177","last_updated":"2023-11-30T22:07:52Z","snapshot_observed_at":"2026-07-06T15:47:07.545213Z","submitted_at":"2023-06-27T03:27:45Z","title":"A method of weak lensing reconstruction through cosmic magnification with multi-band photometry information","version":2},"cited_work":{"arxiv_id":"2306.15177","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.15177","snapshot_observed_at":"2026-08-07T15:06:29.342574Z","title":"A method of weak lensing reconstruction through cosmic magnification with multi-band photometry information","venue":"astro-ph.CO","work_id":"e2a58792-84f1-465e-a4c3-e27ee6cf639a","year":2023},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.913185Z"},"links":{"cited_paper":"/paper/2306.15177","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:13de58b1fe72cb2dbe5945cdf8ce04edcefbb09ec70588b42e7777a4593599dd","observation_id":"3ea2bc13-b585-42cb-896d-dd6e9c7a8c48","resolution":{"observed_at":"2026-08-07T15:06:29.346828Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"0810.0273","last_updated":"2008-10-01T20:04:40Z","snapshot_observed_at":"2026-08-05T03:24:25.693857Z","submitted_at":"2008-10-01T20:04:40Z","title":"Halo stochasticity in global clustering analysis","version":1},"cited_work":{"arxiv_id":"0810.0273","doi":null,"metadata_source":"pith","pith_arxiv_id":"0810.0273","snapshot_observed_at":"2026-08-07T15:06:29.327690Z","title":"Halo stochasticity in global clustering analysis","venue":"astro-ph","work_id":"e38df83f-2ad6-462f-b31f-36e094aa758f","year":2008},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:27.983714Z"},"links":{"cited_paper":"/paper/0810.0273","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:77cf8b6223dc1989d404bb2b585fa91fc97a12adfbbeda9ce99d16a0dabe37fa","observation_id":"4fe03c97-26f3-46aa-8199-705d094482c6","resolution":{"observed_at":"2026-08-07T15:06:29.331676Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"1004.5377","last_updated":"2010-08-16T13:16:37Z","snapshot_observed_at":"2026-07-06T02:09:48.832398Z","submitted_at":"2010-04-29T20:00:02Z","title":"Minimizing the stochasticity of halos in large-scale structure surveys","version":2},"cited_work":{"arxiv_id":"1004.5377","doi":null,"metadata_source":"pith","pith_arxiv_id":"1004.5377","snapshot_observed_at":"2026-08-07T15:06:29.312728Z","title":"Minimizing the stochasticity of halos in large-scale structure surveys","venue":"astro-ph.CO","work_id":"1bda580d-cefd-44aa-8102-e47251f3733f","year":2010},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.059766Z"},"links":{"cited_paper":"/paper/1004.5377","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:3ee10c81ea9592e7df7cdb691d070a99906946c6e1ad17ec624222b35c84c681","observation_id":"273fcac7-1124-4eb0-9b8b-c71f7b6ce4e2","resolution":{"observed_at":"2026-08-07T15:06:29.316357Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"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":"2026-08-07T15:06:28.150284Z","title":"Baldauf, R","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.150284Z"},"links":{"cited_paper":"/paper/0911.4973","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:07fe0da0f1deb2b4def53a47a75aa038cc138786b6e8a49c5a6cc5b977311a6c","observation_id":"948053d3-1a60-4f16-9b4e-6caf781a5e39","resolution":{"observed_at":"2026-08-07T15:06:28.150284Z","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":"2026-08-07T15:06:28.292541Z","title":"von Wietersheim Kramsta, B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.292541Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:8a417d9e64425feda80e05dd23efa1d84e32b8933942546bb34f929c8c6fe1e6","observation_id":"33b8dd66-58a2-4b09-b342-9cb08e275d6a","resolution":{"observed_at":"2026-08-07T15:06:28.292541Z","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":"10.1093/mnras/stad1594","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:06:29.123683Z","title":"Elvin-Poole, N","venue":null,"work_id":"6d9f8dcd-e3f4-43f6-bbda-4710bc06c70d","year":2023},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.408511Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:68f13777984e0c02a03d1c5fb22a4f7fcfba108e8ff9e2a470466ab673d2083f","observation_id":"1bf5197a-2683-4e6e-b9bb-61a32dd0386c","resolution":{"observed_at":"2026-08-07T15:06:29.128458Z","resolver_source":"doi","status":"verified_exact"},"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":"2308.05892","last_updated":"2023-10-25T16:23:21Z","snapshot_observed_at":"2026-08-07T02:44:06.327094Z","submitted_at":"2023-08-11T00:55:36Z","title":"Magnification Bias Estimators for Realistic Surveys: an Application to the BOSS Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.05892","snapshot_observed_at":"2026-08-07T15:06:28.475102Z","title":"Wenzl, S.-F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.475102Z"},"links":{"cited_paper":"/paper/2308.05892","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:597a8596ef9ae857947d4000aaf14d584939ba2870b03222c2571a58ac156118","observation_id":"5115428c-813c-4dc7-b96c-a3730618e170","resolution":{"observed_at":"2026-08-07T15:06:28.475102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T15:06:29.818603Z","title":null,"venue":null,"work_id":"d2a4ce65-bab5-4afb-82d7-9698b85f58da","year":2021},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.588518Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:fe74dde54d41cef52d3e3be09d0dda84a006caafd658134c1510082603edd527","observation_id":"d859658c-ed1d-405e-ae9d-b5b7cfcc7593","resolution":{"observed_at":"2026-08-07T15:06:29.907125Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"0911.2454","last_updated":"2010-11-29T14:24:21Z","snapshot_observed_at":"2026-07-06T02:02:49.721823Z","submitted_at":"2009-11-12T20:28:50Z","title":"Simultaneous measurement of cosmology and intrinsic alignments using joint cosmic shear and galaxy number density correlations","version":2},"cited_work":{"arxiv_id":"0911.2454","doi":null,"metadata_source":"pith","pith_arxiv_id":"0911.2454","snapshot_observed_at":"2026-08-07T15:06:29.274097Z","title":"Simultaneous measurement of cosmology and intrinsic alignments using joint cosmic shear and galaxy number density correlations","venue":"astro-ph.CO","work_id":"999672a5-0355-4204-9d10-6f0df0aedc88","year":2009},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.704731Z"},"links":{"cited_paper":"/paper/0911.2454","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:88022e98b6a2a593184a59328185b80cee64a464fcc814e4c7f246f52fa3b973","observation_id":"5b616391-d0bd-431a-99b3-ffde5f36aab1","resolution":{"observed_at":"2026-08-07T15:06:29.278644Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"0808.3400","last_updated":"2008-08-25T20:01:55Z","snapshot_observed_at":"2026-07-06T01:46:48.594584Z","submitted_at":"2008-08-25T20:01:55Z","title":"Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys","version":1},"cited_work":{"arxiv_id":"0808.3400","doi":null,"metadata_source":"pith","pith_arxiv_id":"0808.3400","snapshot_observed_at":"2026-08-07T15:06:29.255146Z","title":"Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys","venue":"astro-ph","work_id":"ecfabc00-3d22-4b5f-80f3-64bded04ba6d","year":2008},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.799336Z"},"links":{"cited_paper":"/paper/0808.3400","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:19968236dfb88152b3a71611b386b07d82f2b48d823596629a810634aee35472","observation_id":"b0fadd2b-2f80-42b9-af16-454abc95ad39","resolution":{"observed_at":"2026-08-07T15:06:29.260116Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2209.09782","last_updated":"2023-05-26T15:25:24Z","snapshot_observed_at":"2026-08-06T18:56:39.225281Z","submitted_at":"2022-09-20T15:10:48Z","title":"Dark Energy Survey Year 3 results: Magnification modeling and impact on cosmological constraints from galaxy clustering and galaxy-galaxy lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.09782","snapshot_observed_at":"2026-08-07T15:06:28.914852Z","title":"Elvin-Poole, N","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:28.914852Z"},"links":{"cited_paper":"/paper/2209.09782","citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:99735581a167232e281cd6859e17f0bd4f4aebe46ec7c577a9b420cda5613022","observation_id":"5b04ed33-76cd-46c3-b4b4-eb5c3396b48a","resolution":{"observed_at":"2026-08-07T15:06:28.914852Z","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":"2026-08-07T15:06:29.022447Z","title":"Everett, B","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T15:06:29.022447Z"},"links":{"citing_paper":"/paper/2505.16420"},"observation_digest":"sha256:29bcf4799e3bf7f5d777c12291525b23b714cd9c6fa964fb8b2f462624903122","observation_id":"d61cc8a7-3df1-4cd2-9867-41b59dbc0eec","resolution":{"observed_at":"2026-08-07T15:06:29.022447Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.16420","last_updated":"2025-05-22T09:06:25Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T14:59:03.479106Z","submitted_at":"2025-05-22T09:06:25Z","title":"Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies"},"reference_resolution":{"displayed":47,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":28,"verified_exact":18,"verified_fuzzy":1},"total_outbound_references":47},"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 8 August 2026, this Paper Citation Record lists 47 of 47 outbound references and 0 inbound Pith citation observations for arXiv:2505.16420."}