{"as_of":"2026-08-09T18:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:31903f03ade3287bf5625a78b95f175d3e7a1f8b11fb7e6d306cf0f4fc727383","coverage":[{"denominator":5,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-16T21:16:00.402746Z","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":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T08:42:07.864048Z","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":"2026-07-10T12:15:01.137692Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2512.15960","snapshot_observed_at":"2026-08-03T08:42:07.864048Z","title":"Porredon, C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-08T14:24:16.036685Z","submitted_at":"2026-01-22T18:10:50Z","title":"Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy","version":2},"reference_index":185,"source":"pdf_text","source_observed_at":"2026-08-03T08:42:07.864048Z"},"links":{"cited_paper":"/paper/2512.15960","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:3169ea269e06230a5bc0d753b6c5e78043d419a15c4d27d2cd33cd7bb8e3f6b5","observation_id":"4b4262a8-1af9-404c-b24e-2a4149f0335b","resolution":{"observed_at":"2026-08-03T08:42:07.864048Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"cited_work":{"arxiv_id":"2512.15960","doi":"10.48550/arxiv.2512.15960","metadata_source":"pith","pith_arxiv_id":"2512.15960","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","venue":"astro-ph.CO","work_id":"a0fabb95-6f51-4b6e-b0c4-cae9b576ff82","year":2025},"citing_paper":{"arxiv_id":"2603.09278","last_updated":"2026-05-19T03:20:14Z","snapshot_observed_at":"2026-08-02T17:29:02.625743Z","submitted_at":"2026-03-10T07:03:48Z","title":"Constraining Neutrino Mass with the Void Weak Lensing Effect","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-21T12:34:56.642400Z"},"links":{"cited_paper":"/paper/2512.15960","citing_paper":"/paper/2603.09278"},"observation_digest":"sha256:3b31ae5f98f58c40c3d01e29e9921c875e663a4bb437644645df675e734e8bd6","observation_id":"580e52e5-1974-4b45-b90a-17added7b2a2","resolution":{"observed_at":"2026-05-21T12:35:07.875052Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"cited_work":{"arxiv_id":"2512.15960","doi":"10.48550/arxiv.2512.15960","metadata_source":"pith","pith_arxiv_id":"2512.15960","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","venue":"astro-ph.CO","work_id":"a0fabb95-6f51-4b6e-b0c4-cae9b576ff82","year":2025},"citing_paper":{"arxiv_id":"2604.19449","last_updated":"2026-04-23T14:57:09Z","snapshot_observed_at":"2026-07-06T23:06:07.161558Z","submitted_at":"2026-04-21T13:32:04Z","title":"Cosmological constraints from the small scale clustering of Emission Line Galaxies","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-05-10T02:06:19.513203Z"},"links":{"cited_paper":"/paper/2512.15960","citing_paper":"/paper/2604.19449"},"observation_digest":"sha256:967da94ba7d9eb9f7af7617ca9f71c640215239dadbe7d6231920cd5dbf6fb72","observation_id":"04522950-05c6-4d97-a7b1-ce54a866e72e","resolution":{"observed_at":"2026-05-10T02:06:36.813649Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"cited_work":{"arxiv_id":"2512.15960","doi":"10.48550/arxiv.2512.15960","metadata_source":"pith","pith_arxiv_id":"2512.15960","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","venue":"astro-ph.CO","work_id":"a0fabb95-6f51-4b6e-b0c4-cae9b576ff82","year":2025},"citing_paper":{"arxiv_id":"2605.11658","last_updated":"2026-07-02T05:53:56Z","snapshot_observed_at":"2026-07-06T23:23:30.499023Z","submitted_at":"2026-05-12T07:20:14Z","title":"Density-Shear Baryon Acoustic Oscillation as a Cosmological Consistency Check","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-13T01:10:38.364185Z"},"links":{"cited_paper":"/paper/2512.15960","citing_paper":"/paper/2605.11658"},"observation_digest":"sha256:d3a54220b3cb24665e452d1b149379e492b755f89cc07d9e6c6a0a4b389bab9f","observation_id":"a08368e6-e145-4a3c-84fa-618a96bb570e","resolution":{"observed_at":"2026-05-13T01:47:05.350331Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"cited_work":{"arxiv_id":"2512.15960","doi":"10.48550/arxiv.2512.15960","metadata_source":"pith","pith_arxiv_id":"2512.15960","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","venue":"astro-ph.CO","work_id":"a0fabb95-6f51-4b6e-b0c4-cae9b576ff82","year":2025},"citing_paper":{"arxiv_id":"2605.11658","last_updated":"2026-07-02T05:53:56Z","snapshot_observed_at":"2026-07-06T23:23:30.499023Z","submitted_at":"2026-05-12T07:20:14Z","title":"Density-Shear Baryon Acoustic Oscillation as a Cosmological Consistency Check","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-04T01:35:31.698704Z"},"links":{"cited_paper":"/paper/2512.15960","citing_paper":"/paper/2605.11658"},"observation_digest":"sha256:67e4c94bd058194cda601eb6b8c18e6c93278bd878e589ee68d18ad934dee81b","observation_id":"bf907fa8-beb3-4a68-94dd-02b44b7e9a5b","resolution":{"observed_at":"2026-07-04T01:39:23.754867Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2512.15960/citation-record","integrity":"/paper/2512.15960/integrity","json":"/paper/2512.15960/citation-record.json","paper":"/paper/2512.15960"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2502.17674","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-04T08:09:41.660996Z","title":"2025b, arXiv e-prints, arXiv:2502.17674, arXiv:2502.17674 Astropy Collaboration, Robitaille, T","venue":null,"work_id":"bd2a2be9-7d92-4d5d-8831-fd10273c5401","year":2025},"citing_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-16T21:16:00.402746Z"},"links":{"citing_paper":"/paper/2512.15960"},"observation_digest":"sha256:5f9538e0a2b2f14b412c17ed319c6ecab29bebb1be9e46beac35769514ecbe7a","observation_id":"b42a4e2b-8b54-4ca0-bb02-bd446601514b","resolution":{"observed_at":"2026-05-16T21:18:32.532466Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-06-05T21:23:00.469572Z","title":"mock-challenge","venue":null,"work_id":"ae8819e8-a8e5-4978-bc61-052255344b37","year":2018},"citing_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-16T21:16:00.402746Z"},"links":{"citing_paper":"/paper/2512.15960"},"observation_digest":"sha256:5c5f8d7cb6c095edf4d672e14fdd29c4ac173f73c97fdc58fa6740574224009a","observation_id":"aa818895-7e7b-4150-bae5-b2dec5e2c616","resolution":{"observed_at":"2026-05-16T21:18:33.198822Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-06-05T21:23:00.469572Z","title":"2019; Hamana et al","venue":null,"work_id":"f1e8af6a-081a-4460-88a1-c5d3827b645c","year":2019},"citing_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-16T21:16:00.402746Z"},"links":{"citing_paper":"/paper/2512.15960"},"observation_digest":"sha256:377e4dfde128ab6fcc077a3350fec320c4a0b850e637ec8eaeb6edfc5ca3be2f","observation_id":"d85de81a-4440-4c3b-8305-c73a245666f3","resolution":{"observed_at":"2026-05-16T21:18:33.201106Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-06-05T21:23:00.469572Z","title":"In this case, there are also two parameters that correct for PSF-related sys- tematics,α PSF andβ PSF","venue":null,"work_id":"13c2ee09-5288-4507-b880-d077847787d2","year":2020},"citing_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-16T21:16:00.402746Z"},"links":{"citing_paper":"/paper/2512.15960"},"observation_digest":"sha256:dc225bd58f6ac080c81c3ce64a7d4448cebd3412e478945d7905c754553e0261","observation_id":"73cf928d-739c-4234-a921-8ca82e51effe","resolution":{"observed_at":"2026-05-16T21:18:33.206007Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"90b07d33-b8dd-48ba-a2f3-9bc8c48ff71f","year":2024},"citing_paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-16T21:16:00.402746Z"},"links":{"citing_paper":"/paper/2512.15960"},"observation_digest":"sha256:1cfe9c3152a76f12c44967f41f32da39e132ca8bd4dfdc44e9bb6f82b7bc74dc","observation_id":"ddf85674-6580-41af-aad7-c69deaf340ee","resolution":{"observed_at":"2026-05-16T21:18:33.203123Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2512.15960","last_updated":"2026-04-27T11:27:24Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T22:39:23.633419Z","submitted_at":"2025-12-17T20:47:38Z","title":"DESI-DR1 $3 \\times 2$-pt analysis: consistent cosmology across weak lensing surveys"},"reference_resolution":{"displayed":5,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":1,"verified_exact":1,"verified_fuzzy":2},"total_outbound_references":5},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 5 of 5 outbound references and 5 inbound Pith citation observations for arXiv:2512.15960."}