{"as_of":"2026-07-25T05:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:94573743a86285e446d0f72c8ca6b2532eada89010ae8cb09be6c44b0b265c0d","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-07-24T06:31:00.690269+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T21:55:54.028883Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-06-30T16:04:53.413441Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2105.13549","last_updated":"2022-03-21T13:57:33Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-05-28T01:58:58Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","version":3},"reference_index":178,"source":"pdf_text","source_observed_at":"2026-05-19T09:35:12.156800Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2105.13549"},"observation_digest":"sha256:e6468b35c3401b64f7f9a08c1ae42459713b9bb5d1b4f71321d906697ec38aea","observation_id":"ef8f1778-c47a-4f7d-a0ae-0eb5a8d43916","resolution":{"observed_at":"2026-05-19T09:35:12.862993Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2510.14888","last_updated":"2026-04-08T20:26:41Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-16T17:07:57Z","title":"Modeling nonlinear scales for dynamical dark energy cosmologies with COLA","version":2},"reference_index":137,"source":"pdf_text","source_observed_at":"2026-05-18T06:13:13.345307Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2510.14888"},"observation_digest":"sha256:9949705ab5447501f54d7c8728da74a9b327f1fbc7567f670d3d836407dd211e","observation_id":"0afc0240-d186-4bc3-8826-a5e41f9acb60","resolution":{"observed_at":"2026-05-18T06:15:58.484378Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","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":"2026-07-14T21:55:54.028883Z","title":"Krause and T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2603.13030","last_updated":"2026-07-01T15:32:03Z","snapshot_observed_at":"2026-07-14T21:55:53.060873Z","submitted_at":"2026-03-13T14:42:17Z","title":"Floquet Dissipative Phase Transitions","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-14T21:55:54.028883Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2603.13030"},"observation_digest":"sha256:6b0591feb327ff0e33c453b3a8147f699b3b87fd60b16240f5b4f5788da38b1d","observation_id":"e4eaec4f-81c2-49cf-ba62-d7511fb6f91a","resolution":{"observed_at":"2026-07-14T21:55:54.028883Z","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":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2605.12877","last_updated":"2026-05-13T01:45:54Z","snapshot_observed_at":"2026-07-06T23:24:32.412966Z","submitted_at":"2026-05-13T01:45:54Z","title":"Machine-learning applications for weak-lensing cosmology","version":1},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2605.12877"},"observation_digest":"sha256:00e96eb14a1431ced5ba94e122a0d1b42b2f68d3929018e1191a550c1f38706a","observation_id":"da1e578f-6081-44df-9b9e-d87b3977e551","resolution":{"observed_at":"2026-05-14T19:07:49.318769Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2605.13547","last_updated":"2026-05-13T13:55:32Z","snapshot_observed_at":"2026-07-06T23:25:07.022065Z","submitted_at":"2026-05-13T13:55:32Z","title":"UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2605.13547"},"observation_digest":"sha256:bcdd65f392e918988e69f6090df5755e53fde58e31fe93eb3011f4a96a42708a","observation_id":"1e48e555-df01-4155-9623-d5c7e8524d66","resolution":{"observed_at":"2026-05-14T18:19:22.003244Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2605.16186","last_updated":"2026-05-15T17:05:46Z","snapshot_observed_at":"2026-07-06T23:27:24.957966Z","submitted_at":"2026-05-15T17:05:46Z","title":"Analytical method for computing the covariance matrix of cosmic shear two-point correlation function","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-20T16:10:04.825506Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2605.16186"},"observation_digest":"sha256:81b67389a5e1ebe9c6da5d84d51143aef2c196f55f7357c5033647e3f030c614","observation_id":"a7784243-5d8e-49af-96d9-41597c5d100c","resolution":{"observed_at":"2026-05-20T16:13:34.494854Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2606.00411","last_updated":"2026-05-29T23:05:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-29T23:05:25Z","title":"The sound of dynamical dark energy and modified gravity","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-06-28T20:48:00.755241Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2606.00411"},"observation_digest":"sha256:a333dcab8d6b181b3173d9e11d0ee69786b6932e26859966b4cc53545e14e830","observation_id":"10e49938-65c6-42f5-87cd-e49dc4485337","resolution":{"observed_at":"2026-06-28T20:52:37.728977Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2606.11305","last_updated":"2026-06-09T18:00:05Z","snapshot_observed_at":"2026-07-06T23:50:25.158108Z","submitted_at":"2026-06-09T18:00:05Z","title":"Modeling the impact of filter-substrate refraction in the Roman point spread function","version":1},"reference_index":121,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2606.11305"},"observation_digest":"sha256:19324edfb5ac6b3c8ca5f8b97560ac2fa2a35b3f33afbde642b3b30d8729843a","observation_id":"8ec2c8c9-88e2-4305-8547-fba6f51cd5f2","resolution":{"observed_at":"2026-06-27T11:30:52.704214Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2606.23781","last_updated":"2026-06-22T18:00:00Z","snapshot_observed_at":"2026-07-06T23:58:25.400508Z","submitted_at":"2026-06-22T18:00:00Z","title":"Accurate modeling for 3$\\times$2pt analyses in Roman and Rubin: a study of model approximations","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2606.23781"},"observation_digest":"sha256:ca43df83dca4b0abc03f276a0bd160554bac2d0126b346c732abe0cf1eb34180","observation_id":"65ebf8b4-be34-41da-a124-53f5a030cb3b","resolution":{"observed_at":"2026-06-26T17:49:40.887244Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","version":1},"cited_work":{"arxiv_id":"1601.05779","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.05779","snapshot_observed_at":"2026-06-30T16:04:53.413441Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys","venue":"astro-ph.CO","work_id":"3f356541-27cb-4512-b06f-afc2e53da703","year":2016},"citing_paper":{"arxiv_id":"2606.30459","last_updated":"2026-06-29T15:25:40Z","snapshot_observed_at":"2026-07-07T00:04:20.023800Z","submitted_at":"2026-06-29T15:25:40Z","title":"Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-06-30T04:52:09.974573Z"},"links":{"cited_paper":"/paper/1601.05779","citing_paper":"/paper/2606.30459"},"observation_digest":"sha256:66e5d008a628c608f371506b72e8a86c0ea2dc553c328aa814b8fa190b98c1b3","observation_id":"60cadbd5-0a24-4486-8fe2-f77bbe020297","resolution":{"observed_at":"2026-06-30T16:04:53.414649Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1601.05779/citation-record","integrity":"/paper/1601.05779/integrity","json":"/paper/1601.05779/citation-record.json","paper":"/paper/1601.05779"},"outbound":[],"paper":{"arxiv_id":"1601.05779","last_updated":"2016-01-21T20:50:02Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T04:43:39.436074Z","submitted_at":"2016-01-21T20:50:02Z","title":"CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-07-24T06:31:00.690269+00:00","source":"crossref"},{"observed_at":"2026-07-24T06:30:55.483554+00:00","source":"retraction_watch"}],"thesis":"As of 25 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1601.05779."}