{"as_of":"2026-08-20T10:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:83760583a8546351ccfe436a65babde27d60806da7eccb0dcb0dda12ebe16815","coverage":[{"denominator":52,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":52,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T03:05:15.481401Z","state":"measured"},{"denominator":52,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":52,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+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/2602.09230/citation-record","integrity":"/paper/2602.09230/integrity","json":"/paper/2602.09230/citation-record.json","paper":"/paper/2602.09230"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2506.00758","last_updated":"2026-04-28T14:04:07Z","snapshot_observed_at":"2026-08-11T22:09:15.946107Z","submitted_at":"2025-06-01T00:09:30Z","title":"Dimensional reduction for sampled priors and application to photometric redshift distributions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.00758","snapshot_observed_at":"2026-08-03T03:05:15.301109Z","title":"Bernstein, W","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.301109Z"},"links":{"cited_paper":"/paper/2506.00758","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:9fc1229c55ae07ff598b2ab8c4c5416ca6aede5b92d2f52b3e58c770a56f62b4","observation_id":"16a67b9f-7c10-442b-85c3-496dad0fb321","resolution":{"observed_at":"2026-08-03T03:05:15.301109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.03235","last_updated":"2017-10-09T18:00:03Z","snapshot_observed_at":"2026-08-17T17:36:33.468953Z","submitted_at":"2017-10-09T18:00:03Z","title":"Weak lensing for precision cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.03235","snapshot_observed_at":"2026-08-03T03:05:15.306114Z","title":"Mandelbaum,Weak lensing for precision cosmology,Ann","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.306114Z"},"links":{"cited_paper":"/paper/1710.03235","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:52c94fdad593a6b8caa48e63a9f72e630faded5df07e5bd6ef6b003450321d3a","observation_id":"0d677645-f426-42f8-a53c-87336c634de6","resolution":{"observed_at":"2026-08-03T03:05:15.306114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2434","last_updated":"2013-03-06T20:33:04Z","snapshot_observed_at":"2026-08-15T04:22:43.388950Z","submitted_at":"2012-01-11T22:12:48Z","title":"Observational Probes of Cosmic Acceleration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2434","snapshot_observed_at":"2026-08-03T03:05:15.309608Z","title":"Weinberg, M.J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.309608Z"},"links":{"cited_paper":"/paper/1201.2434","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:4b3992bf12bd3256de65c1c112c57d2c77fdf7cb7a410b5680782b1a8264fa2e","observation_id":"e06f5635-c7b1-4289-9662-ce3d355a2a89","resolution":{"observed_at":"2026-08-03T03:05:15.309608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3400","last_updated":"2008-08-25T20:01:55Z","snapshot_observed_at":"2026-08-15T10:08:17.503417Z","submitted_at":"2008-08-25T20:01:55Z","title":"Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3400","snapshot_observed_at":"2026-08-03T03:05:15.313228Z","title":"Bernstein,Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys, Astrophys","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.313228Z"},"links":{"cited_paper":"/paper/0808.3400","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:44a1fb1f1c94c48fb75f5b61595c8d90caae154d1f04e5db961e9d378cf28f42","observation_id":"f6e9ff07-c7c0-4fd2-8ef7-db540753bd52","resolution":{"observed_at":"2026-08-03T03:05:15.313228Z","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":"2026-08-11T07:37:11.436931Z","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":"2026-08-03T03:05:15.317158Z","title":"Bartelmann and P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.317158Z"},"links":{"cited_paper":"/paper/astro-ph/9912508","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:da2867c4b6be47c9a1134c0216d39c4e30a58495355b3b359abc275e90268002","observation_id":"bb19137a-ffb4-4a77-83a3-bd64ded433ca","resolution":{"observed_at":"2026-08-03T03:05:15.317158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701671","last_updated":"2007-10-28T17:07:34Z","snapshot_observed_at":"2026-08-15T10:49:51.068336Z","submitted_at":"2007-01-24T05:38:40Z","title":"Intrinsic galaxy alignments from the 2SLAQ and SDSS surveys: luminosity and redshift scalings and implications for weak lensing surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0701671","snapshot_observed_at":"2026-08-03T03:05:15.324901Z","title":"Hirata, R","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.324901Z"},"links":{"cited_paper":"/paper/astro-ph/0701671","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:601b565fae23e82023045e6fb6384ac276ca485e411343d6f3d739cd4cbf1795","observation_id":"b7ba7fe0-3765-4aa2-a991-1df196b7d247","resolution":{"observed_at":"2026-08-03T03:05:15.324901Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.5347","last_updated":"2010-08-04T18:06:11Z","snapshot_observed_at":"2026-08-15T05:32:50.919801Z","submitted_at":"2009-11-27T21:04:52Z","title":"The WiggleZ Dark Energy Survey: Direct constraints on blue galaxy intrinsic alignments at intermediate redshifts","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.5347","snapshot_observed_at":"2026-08-03T03:05:15.328121Z","title":"Mandelbaum, C","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.328121Z"},"links":{"cited_paper":"/paper/0911.5347","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:091c3d6d0e27f7943285e4080d1f68835b5d566213142492f9c5a32104288e4f","observation_id":"55a8c117-6484-4913-9865-c439b0875ce9","resolution":{"observed_at":"2026-08-03T03:05:15.328121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0107431","last_updated":"2001-11-21T21:34:46Z","snapshot_observed_at":"2026-08-20T00:50:58.173849Z","submitted_at":"2001-07-22T19:21:59Z","title":"Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0107431","snapshot_observed_at":"2026-08-03T03:05:15.331242Z","title":"Bernstein and M","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.331242Z"},"links":{"cited_paper":"/paper/astro-ph/0107431","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:bee872ef9a4d50c5e621168f00854a4d5cff490178c57d80478625bd1f11fa6e","observation_id":"209220be-4f43-4e3d-93ec-14a6ca40dabf","resolution":{"observed_at":"2026-08-03T03:05:15.331242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.7423","last_updated":"2014-05-28T23:50:50Z","snapshot_observed_at":"2026-08-14T23:32:21.271655Z","submitted_at":"2014-05-28T23:50:50Z","title":"Accounting for baryonic effects in cosmic shear tomography: Determining a minimal set of nuisance parameters using PCA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.7423","snapshot_observed_at":"2026-08-03T03:05:15.334875Z","title":"Eifler, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.334875Z"},"links":{"cited_paper":"/paper/1405.7423","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:4ef1971287c3d870b1f4cda8e2cd8dbe271c20d4106b588cf35fe4296bfccc32","observation_id":"8cbec512-1827-48fc-9ec1-108f21bc4c07","resolution":{"observed_at":"2026-08-03T03:05:15.334875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.01146","last_updated":"2019-08-20T17:10:49Z","snapshot_observed_at":"2026-08-19T13:24:26.645383Z","submitted_at":"2018-09-04T18:00:01Z","title":"Modeling baryonic physics in future weak lensing surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.01146","snapshot_observed_at":"2026-08-03T03:05:15.338914Z","title":"Huang, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.338914Z"},"links":{"cited_paper":"/paper/1809.01146","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:bfa65044c7f891800e14f6c9830669c3b729ad8b2da4f967a49783e49e2a2426","observation_id":"3e9ffff6-64b3-45d1-9d3e-4d7a594b14d8","resolution":{"observed_at":"2026-08-03T03:05:15.338914Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0902.2782","last_updated":"2009-02-16T22:33:39Z","snapshot_observed_at":"2026-08-15T05:54:52.863988Z","submitted_at":"2009-02-16T22:33:39Z","title":"Catastrophic photometric redshift errors: weak lensing survey requirements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0902.2782","snapshot_observed_at":"2026-08-03T03:05:15.342148Z","title":"Bernstein and D","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.342148Z"},"links":{"cited_paper":"/paper/0902.2782","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:4b6b3fe69bfc4d6c692e14d4727a98b30ac97b40cf906597f7ef4f4c518b1975","observation_id":"43c1d315-4f84-4adf-8d77-260c788fa571","resolution":{"observed_at":"2026-08-03T03:05:15.342148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9904153","last_updated":"1999-04-13T00:02:57Z","snapshot_observed_at":"2026-08-20T01:19:59.789828Z","submitted_at":"1999-04-13T00:02:57Z","title":"Power Spectrum Tomography with Weak Lensing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9904153","snapshot_observed_at":"2026-08-03T03:05:15.345512Z","title":"Hu,Power spectrum tomography with weak lensing,Astrophys","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.345512Z"},"links":{"cited_paper":"/paper/astro-ph/9904153","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:eef3537420376c9321a7dfc0a226862131bced5f47b0bb65c50ffc2c9170ab11","observation_id":"7a05919a-d2ea-4060-a5f9-c2eb45a57e84","resolution":{"observed_at":"2026-08-03T03:05:15.345512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506614","last_updated":"2005-08-12T21:11:17Z","snapshot_observed_at":"2026-08-09T20:54:11.272488Z","submitted_at":"2005-06-24T21:52:09Z","title":"Effect of Photometric Redshift Uncertainties on Weak Lensing Tomography","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506614","snapshot_observed_at":"2026-08-03T03:05:15.348932Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.348932Z"},"links":{"cited_paper":"/paper/astro-ph/0506614","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:704a024326caaf6de15769559705059fb5a2e80618342a038a322375ec8cb557","observation_id":"4a693ace-bb5e-4cea-a4e2-b8237b04f861","resolution":{"observed_at":"2026-08-03T03:05:15.348932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9811189","last_updated":"1998-11-12T02:27:35Z","snapshot_observed_at":"2026-08-05T01:54:06.355279Z","submitted_at":"1998-11-12T02:27:35Z","title":"Bayesian photometric redshift estimation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9811189","snapshot_observed_at":"2026-08-03T03:05:15.352044Z","title":"Benitez,Bayesian photometric redshift estimation,Astrophys","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.352044Z"},"links":{"cited_paper":"/paper/astro-ph/9811189","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:4faafdb3d02d48e949bfb8869cda7fdc73b40576961e90b70c53fe3e14130fa7","observation_id":"78fffb1b-29d9-489e-9cc7-27640e99f0e0","resolution":{"observed_at":"2026-08-03T03:05:15.352044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.02350","last_updated":"2016-04-08T13:18:21Z","snapshot_observed_at":"2026-08-14T22:02:31.370103Z","submitted_at":"2016-04-08T13:18:21Z","title":"The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.02350","snapshot_observed_at":"2026-08-03T03:05:15.355168Z","title":"Laigle et al.,The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies,Astrophys","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.355168Z"},"links":{"cited_paper":"/paper/1604.02350","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:32655457ad0040fd416bcaeded98242032f051be03e638f90f6f7b40025628ee","observation_id":"b59f45ec-7420-4a3e-8216-7234ff4a53dc","resolution":{"observed_at":"2026-08-03T03:05:15.355168Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2510.23566","last_updated":"2026-06-25T21:41:19Z","snapshot_observed_at":"2026-08-16T20:14:56.930108Z","submitted_at":"2025-10-27T17:35:46Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the Weak Lensing Source Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.23566","snapshot_observed_at":"2026-08-03T03:05:15.358730Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.358730Z"},"links":{"cited_paper":"/paper/2510.23566","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:4dc6754c2db62d95861147d3476c0b5b836976244ba231815fb0edd177671c03","observation_id":"8b1ed289-e46f-4085-b16e-ecdf2e4f34d7","resolution":{"observed_at":"2026-08-03T03:05:15.358730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.07964","last_updated":"2025-09-09T17:51:35Z","snapshot_observed_at":"2026-08-19T05:49:34.721591Z","submitted_at":"2025-09-09T17:51:35Z","title":"Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.07964","snapshot_observed_at":"2026-08-03T03:05:15.362290Z","title":"Giannini, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.362290Z"},"links":{"cited_paper":"/paper/2509.07964","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:d785f1f3cdf4554b0c237686b24c26f93d3e565408dd08a4716ec17cd097efad","observation_id":"86bd1806-2e6a-4211-8088-ac6ca0098922","resolution":{"observed_at":"2026-08-03T03:05:15.362290Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01174","last_updated":"2019-04-02T02:10:42Z","snapshot_observed_at":"2026-08-16T08:00:32.738652Z","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":"2026-08-03T03:05:15.365529Z","title":"Dor´ e et al.,WFIRST: The Essential Cosmology Space Observatory for the Coming Decade, baas(2019) [1904.01174]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.365529Z"},"links":{"cited_paper":"/paper/1904.01174","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:1e863f3a507731a333cfb42b1b1b7912c3f1af0fcaa7ee77a259cf005339cb50","observation_id":"6bc73b37-2c5c-4db7-b314-f1fa53eab9d7","resolution":{"observed_at":"2026-08-03T03:05:15.365529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.05569","last_updated":"2019-02-14T19:15:58Z","snapshot_observed_at":"2026-08-14T17:16:12.085621Z","submitted_at":"2019-02-14T19:15:58Z","title":"The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.05569","snapshot_observed_at":"2026-08-03T03:05:15.368813Z","title":"Akeson, L","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.368813Z"},"links":{"cited_paper":"/paper/1902.05569","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:52067dff5344e0a493b51e6bfba8eeca089f4eb3d9ec0bd4cf3a79eb0ee87fb5","observation_id":"0919f425-bea7-4e49-bef0-3a4a247c2bd1","resolution":{"observed_at":"2026-08-03T03:05:15.368813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.05271","last_updated":"2020-04-11T00:35:56Z","snapshot_observed_at":"2026-08-13T23:02:39.216802Z","submitted_at":"2020-04-11T00:35:56Z","title":"Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.05271","snapshot_observed_at":"2026-08-03T03:05:15.372731Z","title":"Eifler et al.,Cosmology with the Roman Space Telescope – multiprobe strategies,Mon","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.372731Z"},"links":{"cited_paper":"/paper/2004.05271","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:5817e7d003a79f4ca77ba8b723d0b11e648e396cfd4acba54267afc878ed7603","observation_id":"1db4bbd9-33b6-4d6f-92b1-20b75e143f9d","resolution":{"observed_at":"2026-08-03T03:05:15.372731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.01747","last_updated":"2019-12-23T20:34:12Z","snapshot_observed_at":"2026-08-16T22:06:47.734311Z","submitted_at":"2017-02-06T18:53:33Z","title":"Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.01747","snapshot_observed_at":"2026-08-03T03:05:15.375961Z","title":"Hounsell et al.,Simulations of the WFIRST Supernova Survey and Forecasts of Cosmological Constraints,Astrophys","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.375961Z"},"links":{"cited_paper":"/paper/1702.01747","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:a4f3e757adbf5e84c12a479f30668a1b9750b5c19675ceffd1942134b7c10335","observation_id":"adf8ddbf-d979-4fdb-8b31-2e0edeef407e","resolution":{"observed_at":"2026-08-03T03:05:15.375961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.07681","last_updated":"2022-05-20T18:19:10Z","snapshot_observed_at":"2026-08-18T18:02:17.657170Z","submitted_at":"2021-12-14T19:00:01Z","title":"Cosmology with the Roman Space Telescope -- Synergies with CMB lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.07681","snapshot_observed_at":"2026-08-03T03:05:15.379075Z","title":"Wenzl, C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.379075Z"},"links":{"cited_paper":"/paper/2112.07681","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:48a6d8f4e7c627b92eb82bcf1e357efce4ff152f516150cdce92d935ce9ca087","observation_id":"48e8bed8-5c5b-4d05-953c-5f31ec54b787","resolution":{"observed_at":"2026-08-03T03:05:15.379075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.12104","last_updated":"2023-03-21T18:00:14Z","snapshot_observed_at":"2026-08-18T01:11:16.198195Z","submitted_at":"2023-03-21T18:00:14Z","title":"Buzzard to Cardinal: Improved Mock Catalogs for Large Galaxy Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.12104","snapshot_observed_at":"2026-08-03T03:05:15.382462Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.382462Z"},"links":{"cited_paper":"/paper/2303.12104","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:81fee9cca01c75f7f230d17b219c4c132ba43ce7584e95c39ad4b8d9b3173763","observation_id":"659185da-fc28-4b8d-a678-4b03d67668d0","resolution":{"observed_at":"2026-08-03T03:05:15.382462Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03097","last_updated":"2018-04-09T16:51:59Z","snapshot_observed_at":"2026-08-17T11:05:49.858576Z","submitted_at":"2018-04-09T16:51:59Z","title":"The Connection between Galaxies and their Dark Matter Halos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03097","snapshot_observed_at":"2026-08-03T03:05:15.385710Z","title":"Wechsler and J.L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.385710Z"},"links":{"cited_paper":"/paper/1804.03097","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:f736fc41d1350200c59a25e7ceac586350f6fdeb10076255724117b593e21bb4","observation_id":"4d7465d5-aecb-4a04-b811-fc0d327dedc5","resolution":{"observed_at":"2026-08-03T03:05:15.385710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.12104","last_updated":"2021-05-25T17:42:41Z","snapshot_observed_at":"2026-08-16T18:22:17.570163Z","submitted_at":"2021-05-25T17:42:41Z","title":"Modeling Redshift-Space Clustering with Abundance Matching","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.12104","snapshot_observed_at":"2026-08-03T03:05:15.389149Z","title":"DeRose, M.R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.389149Z"},"links":{"cited_paper":"/paper/2105.12104","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:27edc65c3bad1d55e68ce877f83542811ccde696c9804959af415b739c621bac","observation_id":"0004761b-8154-46a5-bf40-f3fff2415313","resolution":{"observed_at":"2026-08-03T03:05:15.389149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0308519","last_updated":"2004-05-15T00:28:33Z","snapshot_observed_at":"2026-08-18T14:51:22.287232Z","submitted_at":"2003-08-29T16:03:32Z","title":"The Dark Side of the Halo Occupation Distribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0308519","snapshot_observed_at":"2026-08-03T03:05:15.392477Z","title":"Kravtsov, A.A","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.392477Z"},"links":{"cited_paper":"/paper/astro-ph/0308519","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:9fed46f326bd9ef8b43eb17cc85c37cccef35162130acc3afc9a280835e55d47","observation_id":"e19473ef-a02b-4a61-8b1e-9366adb01112","resolution":{"observed_at":"2026-08-03T03:05:15.392477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512234","last_updated":"2006-02-21T16:18:59Z","snapshot_observed_at":"2026-08-12T10:14:42.514852Z","submitted_at":"2005-12-09T17:47:10Z","title":"Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512234","snapshot_observed_at":"2026-08-03T03:05:15.395973Z","title":"Conroy, R.H","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.395973Z"},"links":{"cited_paper":"/paper/astro-ph/0512234","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:3d0a750b272537f1fcbc48b7999b49ccb0cf96578885bceeb368e1561ca594bf","observation_id":"d8277676-cfca-4cd0-b23c-b80d3f089c04","resolution":{"observed_at":"2026-08-03T03:05:15.395973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.05651","last_updated":"2016-12-02T14:56:18Z","snapshot_observed_at":"2026-08-15T19:36:12.790218Z","submitted_at":"2015-10-19T20:15:35Z","title":"The Concentration Dependence of the Galaxy-Halo Connection: Modeling Assembly Bias with Abundance Matching","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.05651","snapshot_observed_at":"2026-08-03T03:05:15.399139Z","title":"Lehmann, Y.-Y","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.399139Z"},"links":{"cited_paper":"/paper/1510.05651","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:9f6123dbb8ff6ef2a4b6050666534eebe1b664a6ad475df88022b82dc8ba0f42","observation_id":"023dde77-b72a-4f0f-84d7-839455750021","resolution":{"observed_at":"2026-08-03T03:05:15.399139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.02401","last_updated":"2019-01-08T16:55:16Z","snapshot_observed_at":"2026-08-14T17:33:41.424819Z","submitted_at":"2019-01-08T16:55:16Z","title":"The Buzzard Flock: Dark Energy Survey Synthetic Sky Catalogs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.02401","snapshot_observed_at":"2026-08-03T03:05:15.402331Z","title":"DeRose, R.H","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.402331Z"},"links":{"cited_paper":"/paper/1901.02401","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:3aa529a0946cb6d9102f9f08570ad91b2d6525e03ae7c2f5c801251e3fd7a65d","observation_id":"d93aea4f-79c6-4fa0-8510-c1e23e23732c","resolution":{"observed_at":"2026-08-03T03:05:15.402331Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.05460","last_updated":"2015-07-20T12:00:54Z","snapshot_observed_at":"2026-08-19T10:46:19.896929Z","submitted_at":"2015-07-20T12:00:54Z","title":"redMaGiC: Selecting Luminous Red Galaxies from the DES Science Verification Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.05460","snapshot_observed_at":"2026-08-03T03:05:15.405574Z","title":"Rozo, E.S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.405574Z"},"links":{"cited_paper":"/paper/1507.05460","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:18e9dd7c356771023ceaeca09db4917e25ea086f4c61c277f3041fb077a302b9","observation_id":"d3f6e48e-fd4b-4dce-96ba-7b710cbcc6ac","resolution":{"observed_at":"2026-08-03T03:05:15.405574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.00621","last_updated":"2016-05-25T22:55:41Z","snapshot_observed_at":"2026-08-14T22:16:00.966166Z","submitted_at":"2016-01-04T19:51:08Z","title":"The redMaPPer Galaxy Cluster Catalog From DES Science Verification Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.00621","snapshot_observed_at":"2026-08-03T03:05:15.408856Z","title":"Rykoff, E","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.408856Z"},"links":{"cited_paper":"/paper/1601.00621","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:90e8e5aa13f2bb33e1c34ae19d4e2928c28a8916884578b37453636ecc062b8c","observation_id":"4e136f5a-65a8-4cad-b145-db70359db9d6","resolution":{"observed_at":"2026-08-03T03:05:15.408856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.12105","last_updated":"2021-05-25T17:42:44Z","snapshot_observed_at":"2026-08-16T18:22:17.537331Z","submitted_at":"2021-05-25T17:42:44Z","title":"ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.12105","snapshot_observed_at":"2026-08-03T03:05:15.412691Z","title":"Wechsler, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.412691Z"},"links":{"cited_paper":"/paper/2105.12105","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:7ec5933d5f60c7a7e94f2863dbca72d1b68201566ff21911087e239019ba9f8d","observation_id":"b98ef960-9580-413f-b9b5-80b9a526545d","resolution":{"observed_at":"2026-08-03T03:05:15.412691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205243","last_updated":"2002-09-24T16:37:58Z","snapshot_observed_at":"2026-07-07T00:26:25.660053Z","submitted_at":"2002-05-15T20:32:20Z","title":"Estimating Fixed Frame Galaxy Magnitudes in the SDSS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0205243","snapshot_observed_at":"2026-08-03T03:05:15.416274Z","title":"Blanton, J","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.416274Z"},"links":{"cited_paper":"/paper/astro-ph/0205243","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:5ffc49eaedbf0d995905849ed15748f53f8bb660c7b45dcd19b9db1db4073936","observation_id":"1c374d22-2f3b-4fbc-9408-477884bca6b8","resolution":{"observed_at":"2026-08-03T03:05:15.416274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.4307","last_updated":"2011-08-11T17:21:18Z","snapshot_observed_at":"2026-08-15T05:02:33.248608Z","submitted_at":"2010-11-18T21:19:46Z","title":"The PRIsm MUlti-Object Survey (PRIMUS) I: Survey Overview and Characteristics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.4307","snapshot_observed_at":"2026-08-03T03:05:15.420049Z","title":"Coil, M.R","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.420049Z"},"links":{"cited_paper":"/paper/1011.4307","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:15584d4eda10de61efa30e6e594aa25d37b7f456fda058f158260a694918e258","observation_id":"1ae5a14a-5458-4a29-8be1-0c42e4107f9e","resolution":{"observed_at":"2026-08-03T03:05:15.420049Z","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":"2026-08-16T13:29:05.737064Z","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":"2026-08-03T03:05:15.423251Z","title":"Campos, B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.423251Z"},"links":{"cited_paper":"/paper/2408.00922","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:14b6abd9617b28c06a57378220de7afe3a7dc39209d6c76b97c3e19698c2e70e","observation_id":"3cb0e6d1-e0a1-4a51-b0b8-cb65d6438535","resolution":{"observed_at":"2026-08-03T03:05:15.423251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09542","last_updated":"2020-04-20T18:03:19Z","snapshot_observed_at":"2026-08-03T18:46:02.235483Z","submitted_at":"2020-04-20T18:03:19Z","title":"Propagating sample variance uncertainties in redshift calibration: simulations, theory and application to the COSMOS2015 data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09542","snapshot_observed_at":"2026-08-03T03:05:15.426312Z","title":"S´ anchez, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.426312Z"},"links":{"cited_paper":"/paper/2004.09542","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:9f45377c0fb21119ef70f5a6e3b6df84ae94966a64cd119a6fe4ae2ca114432c","observation_id":"43f5a885-34e6-42c6-9d1c-8e3a53231076","resolution":{"observed_at":"2026-08-03T03:05:15.426312Z","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":"2026-08-03T03:05:15.430066Z","title":"CAMB: Code for Anisotropies in the Microwave Background","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.430066Z"},"links":{"citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:f8abd736a3d4cff15287321e0a5dae0fc837cc5aff2f8db55a5f57295a74a348","observation_id":"77ab8b0a-2e85-455a-bf4a-2e58dac6b6cc","resolution":{"observed_at":"2026-08-03T03:05:15.430066Z","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":"2026-08-03T03:05:15.434223Z","title":"Observations Time Allocation Committee and C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.434223Z"},"links":{"citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:59f0e7548903629b30a3c7b1a7859bb4660e110f5fc29dacaa0a311501302f95","observation_id":"ff946b12-fe18-4bc5-a3ef-4167b35d28a2","resolution":{"observed_at":"2026-08-03T03:05:15.434223Z","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":"2026-08-03T03:05:15.437134Z","title":"Becker,CALCLENS: Weak lensing simulations for large-area sky surveys and second-order effects in cosmic shear power spectra, Ph.D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.437134Z"},"links":{"citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:2fb2b5a8f85535fcb186abaa19bbdc6b182a6efa979f9997eaedfa9371d0a236","observation_id":"163332ed-2d56-444c-8aca-83172d5ce310","resolution":{"observed_at":"2026-08-03T03:05:15.437134Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-08-14T22:13:38.637603Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-08-03T03:05:15.439981Z","title":"Krause and T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.439981Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:f8d54a61b694f6a9f7d1b3090cb667f01658fcbb7ecee6d9a87006727f991067","observation_id":"ddee1e59-659b-43a0-9693-355a07520a62","resolution":{"observed_at":"2026-08-03T03:05:15.439981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.04833","last_updated":"2021-02-20T00:11:53Z","snapshot_observed_at":"2026-08-13T04:27:14.953344Z","submitted_at":"2020-04-09T22:02:02Z","title":"2D-FFTLog: Efficient computation of real space covariance matrices for galaxy clustering and weak lensing","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.04833","snapshot_observed_at":"2026-08-03T03:05:15.443268Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.443268Z"},"links":{"cited_paper":"/paper/2004.04833","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:abff70d91b44f79864890e600354eea38b8770ec6d35c051a37d74291254c30f","observation_id":"6b7ee77f-37f7-46ad-957c-a4987c3bf8e1","resolution":{"observed_at":"2026-08-03T03:05:15.443268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.05290","last_updated":"2021-05-20T11:52:55Z","snapshot_observed_at":"2026-08-03T14:56:09.086229Z","submitted_at":"2020-05-11T17:49:03Z","title":"Cobaya: Code for Bayesian Analysis of hierarchical physical models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.05290","snapshot_observed_at":"2026-08-03T03:05:15.446258Z","title":"Torrado and A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.446258Z"},"links":{"cited_paper":"/paper/2005.05290","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:da476a450b9e0f6c52d0d4d9a3eae23c2d1c4d3c09e6e4c74bb308f88f51f8eb","observation_id":"b502bad8-eee3-47bf-95e0-2ce634cf171f","resolution":{"observed_at":"2026-08-03T03:05:15.446258Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9911177","last_updated":"2000-06-01T12:13:06Z","snapshot_observed_at":"2026-07-07T01:29:40.678750Z","submitted_at":"1999-11-10T17:57:36Z","title":"Efficient Computation of CMB anisotropies in closed FRW models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9911177","snapshot_observed_at":"2026-08-03T03:05:15.449313Z","title":"Lewis, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.449313Z"},"links":{"cited_paper":"/paper/astro-ph/9911177","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:0ba21c27196c686f35ed957fcc91b3034ac8ad1352b93823c716252a2e450694","observation_id":"cb8d9a5f-dc3e-4b4e-92e6-4838b89f7e0c","resolution":{"observed_at":"2026-08-03T03:05:15.449313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-08-12T19:40:10.586390Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-08-03T03:05:15.452612Z","title":"Lewis,GetDist: a Python package for analysing Monte Carlo samples,JCAP08(2025) 025 [1910.13970]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.452612Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:b81d8ffc1222d4785bb6637eea9560c4b04c948696be4951c51bb7d7e796fc5c","observation_id":"9701aa15-6e58-43da-936d-d3d5179e898c","resolution":{"observed_at":"2026-08-03T03:05:15.452612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9609149","last_updated":"1996-09-22T22:14:56Z","snapshot_observed_at":"2026-07-07T01:14:30.808201Z","submitted_at":"1996-09-22T22:14:56Z","title":"Weak Lensing On the Celestial Sphere","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9609149","snapshot_observed_at":"2026-08-03T03:05:15.456355Z","title":"Stebbins,Weak Lensing On the Celestial Sphere,arXiv e-prints(1996) astro [astro-ph/9609149]","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.456355Z"},"links":{"cited_paper":"/paper/astro-ph/9609149","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:fdfa90e165971df17f45526693dbd044a435748d9c16a5806b3be42e807329c2","observation_id":"05f071e3-8ee5-45f4-9737-32a585721463","resolution":{"observed_at":"2026-08-03T03:05:15.456355Z","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":"2026-08-18T09:06:31.134177Z","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":"2026-08-03T03:05:15.460299Z","title":"Krause, X","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.460299Z"},"links":{"cited_paper":"/paper/2105.13548","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:e9afd2b24e7a40236904a478b0a15f6f25ebbb0d0dcc7c0c786b10e6b66768ee","observation_id":"316c1f00-61a5-46e5-bf03-8ffb41e3a870","resolution":{"observed_at":"2026-08-03T03:05:15.460299Z","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":"2026-08-03T03:05:15.463681Z","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":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.463681Z"},"links":{"citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:882611573b9fcaaec45a5e5b89992b15b1f09d3f368b186bd7b6e7eaad1f1080","observation_id":"3ea3ee9c-dceb-4c50-a9d0-661c241d7f0b","resolution":{"observed_at":"2026-08-03T03:05:15.463681Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.09359","last_updated":"2017-06-28T16:52:03Z","snapshot_observed_at":"2026-08-14T20:51:01.749052Z","submitted_at":"2017-06-28T16:52:03Z","title":"Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.09359","snapshot_observed_at":"2026-08-03T03:05:15.466834Z","title":"Krause, T.F","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.466834Z"},"links":{"cited_paper":"/paper/1706.09359","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:6de1dffea15775f3592be90b4938f06d53efdcc054d6b0dba3e72fb411ed4fa4","observation_id":"bb354350-9bf4-4eb3-957c-490541df4ebf","resolution":{"observed_at":"2026-08-03T03:05:15.466834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1208.2701","last_updated":"2012-11-05T02:47:22Z","snapshot_observed_at":"2026-08-18T07:39:57.021003Z","submitted_at":"2012-08-13T20:11:04Z","title":"Revising the Halofit Model for the Nonlinear Matter Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.2701","snapshot_observed_at":"2026-08-03T03:05:15.471138Z","title":"Takahashi, M","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.471138Z"},"links":{"cited_paper":"/paper/1208.2701","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:6af42d570de7c5892f5b9076f952a8eb21992257b2eda795ce10ef4ddf7dcc54","observation_id":"18b34d00-dfbe-4786-b659-369e566045d1","resolution":{"observed_at":"2026-08-03T03:05:15.471138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005470","last_updated":"2000-10-02T22:42:39Z","snapshot_observed_at":"2026-08-14T15:30:08.906263Z","submitted_at":"2000-05-24T00:06:26Z","title":"Intrinsic and Extrinsic Galaxy Alignment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005470","snapshot_observed_at":"2026-08-03T03:05:15.474835Z","title":"Catelan, M","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.474835Z"},"links":{"cited_paper":"/paper/astro-ph/0005470","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:35ea4c778ee6b424de8062cb140eb652fe5dfdaa239aef2be073ea79d4c3173d","observation_id":"a41afde6-3758-4bf4-9b0b-25c76dc55ee4","resolution":{"observed_at":"2026-08-03T03:05:15.474835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0406275","last_updated":"2010-08-24T18:31:06Z","snapshot_observed_at":"2026-08-05T15:00:32.709238Z","submitted_at":"2004-06-10T20:21:55Z","title":"Intrinsic alignment-lensing interference as a contaminant of cosmic shear","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0406275","snapshot_observed_at":"2026-08-03T03:05:15.477827Z","title":"Hirata and U","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.477827Z"},"links":{"cited_paper":"/paper/astro-ph/0406275","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:002f9f42741302b5438b467183d8169384b64c88fa1eb174d3a2e55cca2034e1","observation_id":"925f2303-149a-4831-9950-195174d0ec9d","resolution":{"observed_at":"2026-08-03T03:05:15.477827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.0166","last_updated":"2008-04-18T18:10:33Z","snapshot_observed_at":"2026-08-15T10:41:46.267355Z","submitted_at":"2007-05-01T21:25:39Z","title":"Dark energy constraints from cosmic shear power spectra: impact of intrinsic alignments on photometric redshift requirements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.0166","snapshot_observed_at":"2026-08-03T03:05:15.481401Z","title":"Bridle and L","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-03T03:05:15.481401Z"},"links":{"cited_paper":"/paper/0705.0166","citing_paper":"/paper/2602.09230"},"observation_digest":"sha256:42ce5350f59d169452162868cb7a326f2c850f375ab0a38f2a2c32e52dfd3708","observation_id":"d6786527-831a-44ea-9d6a-788e558957a6","resolution":{"observed_at":"2026-08-03T03:05:15.481401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2602.09230","last_updated":"2026-06-29T21:03:54Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T11:57:33.371765Z","submitted_at":"2026-02-09T21:53:49Z","title":"Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology"},"reference_resolution":{"displayed":52,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":52,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":52},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 52 of 52 outbound references and 0 inbound Pith citation observations for arXiv:2602.09230."}