{"as_of":"2026-08-09T13:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f57e982614b60e505c01d3880d030a1319926412f5637c3dd2d90c7ec99f63fb","coverage":[{"denominator":91,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":91,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T22:46:02.931441Z","state":"measured"},{"denominator":91,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":91,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+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/2502.04449/citation-record","integrity":"/paper/2502.04449/integrity","json":"/paper/2502.04449/citation-record.json","paper":"/paper/2502.04449"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.622098Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.622098Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:4210de63e76e546f34127b34c9072d593fe2e80e9334b1ee041850647abbfc34","observation_id":"37f4bd7f-3b24-4467-b467-c606de45216b","resolution":{"observed_at":"2026-08-08T22:46:02.622098Z","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":"2026-08-08T22:46:02.626858Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.626858Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:c8bca5ef2448321202726cb5c06cdd446e57b9d3f3da7d4fef37a4cdc4d4c791","observation_id":"6fa6c85f-76d8-4a07-afa7-301692606bfa","resolution":{"observed_at":"2026-08-08T22:46:02.626858Z","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":"2026-08-08T22:46:02.630969Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.630969Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:28e9befc76acaa4edbac66cadf2a88b56730f7153a80d1e7fdfbb09d8534538c","observation_id":"dd657654-97ed-4ec6-a6c2-ab6c878d9f4f","resolution":{"observed_at":"2026-08-08T22:46:02.630969Z","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":"2026-08-08T22:46:02.635075Z","title":"D., Allende Prieto , C., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.635075Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:ae055584c734cd634a3d6de7ec781472c434cb81f581a08727e62c5e08f3c5c0","observation_id":"4dba5136-6d23-46ef-b799-d3fbe2b7fffd","resolution":{"observed_at":"2026-08-08T22:46:02.635075Z","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":"2026-08-08T22:46:02.638877Z","title":"E., Zennaro , M., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.638877Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:099f2706e770105b2b34bb9fdf3ad3546bd2d2c6b231da4e98e3fc66a9e81aab","observation_id":"d8dd9a80-2fe4-4892-9fa8-07b4d00abdc3","resolution":{"observed_at":"2026-08-08T22:46:02.638877Z","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":"2026-08-08T22:46:02.642446Z","title":"2021, , 645, A104","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.642446Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:bd9631c31743229b059902411acaa72c61ba9796e16689506f85ac21fa9c4bba","observation_id":"db28917a-8b3b-4d70-8782-bf34a7d663bf","resolution":{"observed_at":"2026-08-08T22:46:02.642446Z","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":"2026-08-08T22:46:02.646083Z","title":"J., Taylor , A","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.646083Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:b5eadfed94bea44df85c0379a96d29cd251bf0d273a500e004afb9431bcfdacd","observation_id":"8ec42a10-0cc4-4e61-a28a-e5e6eedd4b2e","resolution":{"observed_at":"2026-08-08T22:46:02.646083Z","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":"2026-08-08T22:46:02.649702Z","title":"& Schneider , P","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.649702Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:345c93f23adc1410285a0bce61272289c65d2f5544f51d0c5d6b498965aad210","observation_id":"1b9ffce7-da09-46f5-aac4-5118d8f651f4","resolution":{"observed_at":"2026-08-08T22:46:02.649702Z","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":"2026-08-08T22:46:02.653445Z","title":"N., Boxhoorn , D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.653445Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:1488678496419bbc2caf6e68775e96526f56b6a5c68a46feb758d592f60b2e58","observation_id":"7120a2dc-f8a6-4061-a5a0-3e98071b9c7a","resolution":{"observed_at":"2026-08-08T22:46:02.653445Z","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":"2026-08-08T22:46:02.657329Z","title":"2000, , 536, 571","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.657329Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:d32fc7077222dc65e783a472b4f94729d4130f8b483ce471648e1ca33a34da9a","observation_id":"66239e93-45f0-4771-9351-9cd961320003","resolution":{"observed_at":"2026-08-08T22:46:02.657329Z","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":"2026-08-08T22:46:02.660809Z","title":"2024, , 534, 655","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.660809Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:87980737650e5df6f57d2558081f49312fffcd22faef4c18fc147bf9f0b5800b","observation_id":"6e3ad4c2-d7a5-428e-9fa7-7539168597fd","resolution":{"observed_at":"2026-08-08T22:46:02.660809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.711273Z","title":"2016, , 462, 4240","venue":null,"work_id":"adc1bd92-75e5-4cd0-87bf-7624536089ec","year":2016},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.664438Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:65919531c3555a9decd66da4dd45e145fb91b52979f289fb7a204ea128bce39b","observation_id":"1124c9c6-1f59-492c-b5f4-8f2e4c400337","resolution":{"observed_at":"2026-08-08T22:46:03.714433Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.667721Z","title":"& King , L","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.667721Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:a31c1ceb5714317c3ef2a06904d3e3ab8cb72a3c288ce8eebe261385fefa3590","observation_id":"eeb7a135-815d-4936-bc58-af87669e9e12","resolution":{"observed_at":"2026-08-08T22:46:02.667721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.695908Z","title":"2011, Handbook of Markov Chain Monte Carlo, Chapman & Hall/CRC Handbooks of Modern Statistical Methods (CRC Press)","venue":null,"work_id":"ead97802-9f83-46ed-90e3-fbb6ca39363d","year":2011},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.671006Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:9581e5a14802aff4a3e84b0d1e5ae44db3d76a90fddd8aa7d598684bca9eacb8","observation_id":"a88cb7e1-2702-4816-8c8d-d6f6b3d0ec39","resolution":{"observed_at":"2026-08-08T22:46:03.699264Z","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":"2026-08-08T22:46:03.686409Z","title":null,"venue":null,"work_id":"5252cb67-33ec-4b07-b895-6fd7100d4450","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.674298Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:e97965aef9fe7a6f033d8337a42c087c0c7919accf355600ea92256ec92bad67","observation_id":"bdc132c6-b281-439f-b9ab-ff76d24a6f04","resolution":{"observed_at":"2026-08-08T22:46:03.689913Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.676864Z","title":"K., Peters , F","venue":null,"work_id":"34419a7f-14b2-42f2-bc66-f6cd3f7e0b2c","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.677877Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:1106229546540458c622d68be7f7b674241c276545765264fc18e1b45cd752fc","observation_id":"81ffd360-cb1b-45bf-801f-c191fd68ce8b","resolution":{"observed_at":"2026-08-08T22:46:03.680138Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.681166Z","title":"A., Porth , L., Heydenreich , S., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.681166Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:bfb37e02c8f6ad6634972470bfbff5a9767bbe3840145305c19eabee3220e999","observation_id":"f815e189-e13e-4ede-9cb7-5d1b8d9f8e07","resolution":{"observed_at":"2026-08-08T22:46:02.681166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.661527Z","title":"G., Natarajan , P., Pen , U.-L., & Theuns , T","venue":null,"work_id":"fdfe48e6-1788-4271-908a-48a91d4658e3","year":2001},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.684332Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:8a660459b948e31e312e8bb3594d49215ddd2498cba77100828637d31e6d324a","observation_id":"f544f242-bf80-432b-bef0-f034496336b5","resolution":{"observed_at":"2026-08-08T22:46:03.664667Z","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":"2026-08-08T22:46:03.652068Z","title":null,"venue":null,"work_id":"f5e7d745-9661-4ac6-b0df-1b129885d51f","year":2000},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.687468Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:3be9b5ab6676333c65cca909e6a5aa48d7fccfebb3825ea062e4d525ba14a096","observation_id":"c034ba62-5cb4-4bd4-af48-bf27dadc090a","resolution":{"observed_at":"2026-08-08T22:46:03.655241Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.691152Z","title":"2013, The Messenger, 154, 32","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.691152Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:01b7613fe35b1d01cb558b58a92fead90d70b32d07dfb3520b62820719b0c699","observation_id":"4fc3f652-d85c-49b8-8acc-1eb20041617c","resolution":{"observed_at":"2026-08-08T22:46:02.691152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.636454Z","title":"P., et al","venue":null,"work_id":"d625960d-ca9c-4bce-9631-401dc0f60787","year":2005},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.694721Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:06cb0bdae3cecee56fff88d2aec90e87084809dbfe3c52fb91166cae69491e16","observation_id":"29dd4e8e-c0bc-494e-b9ea-a2fdcd16a562","resolution":{"observed_at":"2026-08-08T22:46:03.639825Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.698128Z","title":"A., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.698128Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:59114bafb558e92a4fdbb982bc2c57dbb8797c97a48c7e9081bdc388af20a05d","observation_id":"ab0c2612-4b1c-4522-bf99-a6256e2bb697","resolution":{"observed_at":"2026-08-08T22:46:02.698128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.626750Z","title":"2017, , 467, 1627","venue":null,"work_id":"d7a8e7aa-b8d7-4a13-98ba-a5594d4ef589","year":2017},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.701411Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:7cb468721aef04a2612ee14f926cc58d1409fd68b68e3221a55d0544f927b613","observation_id":"bfab973d-5483-4560-8158-2877d408d7dd","resolution":{"observed_at":"2026-08-08T22:46:03.629889Z","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":"2026-08-08T22:46:03.617282Z","title":null,"venue":null,"work_id":"694cf1a9-c44a-4ae1-a014-0c2f849e6528","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.704641Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:391e2477130f703aae99523bc23693d4f40a148a087b78da9011ce0965ad08f8","observation_id":"b29cd578-52f9-43c5-a5e5-6d6d3b9c6e68","resolution":{"observed_at":"2026-08-08T22:46:03.620608Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.607969Z","title":"C., Hoekstra , H., Joachimi , B., et al","venue":null,"work_id":"72c75695-dc51-4044-acb0-072b7a985748","year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.708046Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:4b64fc36ad4e7c2d991c2d2c09beda2abf9cac2a70f843b605f69d1ebe6d9a42","observation_id":"6941aeae-e2f6-450d-b77e-291c071a3458","resolution":{"observed_at":"2026-08-08T22:46:03.611183Z","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":"2026-08-08T22:46:03.598745Z","title":null,"venue":null,"work_id":"a3d55b05-4fe0-43cf-91e5-11ce45a14996","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.711430Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:5918467fa8b8ffaa2e62cbdc718c09f02ae4f533bc64ee68e57395295a04528e","observation_id":"75e8c229-bdad-4d6a-ac37-468c9915d1ba","resolution":{"observed_at":"2026-08-08T22:46:03.601897Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.588960Z","title":"2003, Bayesian Data Analysis, Chapman & Hall/CRC Texts in Statistical Science (Chapman & Hall/CRC)","venue":null,"work_id":"29013b65-6fa3-4eb5-92c7-c87e435d48f8","year":2003},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.714599Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:cb35f668d447abfec7e649a85157288303f44a53eea000e117afa89216036e64","observation_id":"f325da16-f779-47f1-9c21-d6b422f546d2","resolution":{"observed_at":"2026-08-08T22:46:03.592391Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.718010Z","title":"& Rubin , D","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.718010Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:b107e6811c0595f8b36f4e6fcbc364ba1523d042c7284189786c7e48ee460f0c","observation_id":"4a13a63f-7656-4dde-9654-6b161e5c28dd","resolution":{"observed_at":"2026-08-08T22:46:02.718010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.573743Z","title":"2021, , 645, A105","venue":null,"work_id":"bfd805c2-77d6-4a08-86cd-953bbe7be447","year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.721494Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:d5e71e8d4572dfebb877562d8f0b8678a9c8cdda0e6eca7488aa698be645077e","observation_id":"89da94df-f35b-4bb6-9711-54b7ad782955","resolution":{"observed_at":"2026-08-08T22:46:03.577245Z","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":"2026-08-08T22:46:03.564520Z","title":"2022, , 509, 3868","venue":null,"work_id":"16bf39a3-1465-45ea-a5ca-03be25ce75bc","year":2022},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.725085Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:3aba694135ce027bd9eb5208a3c88d827631dbb28deff6b6d4253c2d7fa27942","observation_id":"9533ffaa-4401-4627-8fda-93626905c907","resolution":{"observed_at":"2026-08-08T22:46:03.567751Z","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":"2026-08-08T22:46:03.555192Z","title":"2015, , 450, 1212","venue":null,"work_id":"fc86432a-e997-490e-8a31-192fc19899df","year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.728323Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:27d6583d961d8a6f0fa43f0e50ce6e0fcc0ea5f5403d640bba7c54a078e5c2ac","observation_id":"21714868-74b2-4cce-a4a0-51aef5f0ceef","resolution":{"observed_at":"2026-08-08T22:46:03.558405Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.731664Z","title":"2007, , 464, 399","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.731664Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:ecee517b55bc4c6adb920b2e45296d5812abb7f8409f2b1b4e41031c13ada7a6","observation_id":"29b22f98-2cb9-4e7c-96ca-cd82e856c073","resolution":{"observed_at":"2026-08-08T22:46:02.731664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.539373Z","title":"2013, , 432, 2433","venue":null,"work_id":"53043b1b-131b-4cf0-8e18-da8977cd82b3","year":2013},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.735075Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:4fef5aad1762adeee0a6d64950de7fab9437a6e67a1a7ac55281d8a12cd311d6","observation_id":"63325ea0-6161-4228-990a-4e55ba005376","resolution":{"observed_at":"2026-08-08T22:46:03.542659Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.738414Z","title":"2021, , 646, A140","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.738414Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:11068c70571e5a6566fc278f6341fd4d3d3bcaea4ff8ed36188bad283269610c","observation_id":"91dae835-4114-4ce6-809b-fb09b05d4d50","resolution":{"observed_at":"2026-08-08T22:46:02.738414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.523829Z","title":null,"venue":null,"work_id":"e8cdfccb-93e3-47b8-930e-00ee64f11c70","year":2009},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.741751Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:60e833de9db70b898fb6250df427349937b826721b8a0566952a165bf31c263c","observation_id":"c20cbfd8-f117-42c7-9b5e-a198afbb3e4f","resolution":{"observed_at":"2026-08-08T22:46:03.527196Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.745253Z","title":"L., Wright , A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.745253Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:7052c251092cc3653187caf877929057215d443faaa0d2d7b770be4d4ec092d3","observation_id":"a4241736-23e9-4c18-a4df-22384054d92e","resolution":{"observed_at":"2026-08-08T22:46:02.745253Z","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":"2026-08-08T22:46:02.748686Z","title":"2013, , 208, 19","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.748686Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:2a231f9b7361226a50586b3716fa9e9feb0a9537213d6e0aefce70eb325be456","observation_id":"11588bda-d0c7-449e-887c-b1e27955a666","resolution":{"observed_at":"2026-08-08T22:46:02.748686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.503350Z","title":null,"venue":null,"work_id":"6991b67b-6468-43d2-b265-c85aa5baf265","year":2004},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.752220Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:124a1bffccd3a2cb57c86a438cf30a421e9eb2190184974808f89867e7608267","observation_id":"f8fc1d88-e01b-419d-b36a-c1d00b554c64","resolution":{"observed_at":"2026-08-08T22:46:03.506518Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.494114Z","title":"& Keeton , C","venue":null,"work_id":"c7d706df-8bc0-475b-b732-c202c2cb9241","year":2002},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.755495Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:ea25fc61ab2923c2fabfe0497db477202d09b8d124dc6895f58329fdb6ada04d","observation_id":"453de2df-c534-4a82-a3f2-8a8dc883e5ac","resolution":{"observed_at":"2026-08-08T22:46:03.497210Z","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":"2026-08-08T22:46:03.484246Z","title":"2015, TreeCorr: Two-point correlation functions , Astrophysics Source Code Library, record ascl:1508.007","venue":null,"work_id":"0de85672-67ec-4074-bff8-a7d1729556b4","year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.758996Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:c87cf840079ef71b4b3408324fa84849ddc240ae753bed8c30526874860bf96a","observation_id":"0ba947f2-3440-4270-bef9-99f38b200d3f","resolution":{"observed_at":"2026-08-08T22:46:03.487896Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.762259Z","title":"2004, , 352, 338","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.762259Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:3752fd7fec9387afb019e90815f28116c73b5e242526478988589773495d02f4","observation_id":"b9d9ffff-b519-4bfe-953b-5056bfbc7fde","resolution":{"observed_at":"2026-08-08T22:46:02.762259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.469042Z","title":"P., Zhang , P., Lin , W","venue":null,"work_id":"5b1c8662-d10d-4789-89ec-67e7b835d550","year":2006},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.765622Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:4d0c0dc4d817c9c6ec962b971ca4b44ffa5a522a3b75d3401cc72a4673e34517","observation_id":"c9bcc206-a1ac-4d3f-926d-181f36b278a5","resolution":{"observed_at":"2026-08-08T22:46:03.472247Z","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":"2026-08-08T22:46:03.459719Z","title":"A., Asgari , M., et al","venue":null,"work_id":"40ed8333-0b5d-4beb-87aa-60ea903643ef","year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.768992Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:9c8ba0211824cc3c01b71e659da5a4306fe15c36383f3ab876b78984f2eb36c8","observation_id":"0d75852a-ddaf-424f-a59a-41584f650600","resolution":{"observed_at":"2026-08-08T22:46:03.462840Z","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":"2026-08-08T22:46:03.450467Z","title":"B., & Bridle , S","venue":null,"work_id":"06bb1fac-f87a-488b-9dde-186548c83cf6","year":2011},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.772500Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:8548ef04f58d718837049c1a380393e02d90360919733342e4a474af9e098d29","observation_id":"63df40f1-3881-470a-91ca-f519e3904da9","resolution":{"observed_at":"2026-08-08T22:46:03.453671Z","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":"2026-08-08T22:46:03.441587Z","title":"& Schneider , P","venue":null,"work_id":"6b4d0aff-e1bc-4a5e-8863-ec78345d5695","year":2008},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.775726Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:77c9305cbb39067df72a93e2f7687dc79a702a8c37baab51393447ab246c8007","observation_id":"643754ca-fea4-407b-8c65-d200d89fcd37","resolution":{"observed_at":"2026-08-08T22:46:03.444645Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.779030Z","title":"1992, , 388, 272","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.779030Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:b689307d1cd3636e3621d36c24b200efe416846734ecdc58bb1abb40d43e81cc","observation_id":"5ee3ada3-dfd4-4c5c-8626-4e3fec5cb0f9","resolution":{"observed_at":"2026-08-08T22:46:02.779030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.426700Z","title":"T., & Takahashi , T","venue":null,"work_id":"7e7cd85c-fd7c-4bcb-998f-2e1ddc099f81","year":2016},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.782309Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:6ea3fc4032345b24aaa540f08357b2d2cdeee6ee26d77bab515a442fc42c3728","observation_id":"16e2d95c-8fc4-422d-b84a-81d9baf79171","resolution":{"observed_at":"2026-08-08T22:46:03.429814Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.785484Z","title":"2015, Reports on Progress in Physics, 78, 086901","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.785484Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:4722707b38ce8676868d18600289af4f384e0f2ee6763edfc0f155f17213bd33","observation_id":"1f7acb9f-9ad7-4914-8c70-8484df87dc02","resolution":{"observed_at":"2026-08-08T22:46:02.785484Z","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":"2026-08-08T22:46:02.788753Z","title":"2017, , 472, 2126","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.788753Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:5e1d3d9816656aa967e212c033e487c4f3c96ab26b5e4d17b9e5f19765d8d231","observation_id":"3157fa00-66a9-4f3d-960b-68eb8de4ab8b","resolution":{"observed_at":"2026-08-08T22:46:02.788753Z","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":"2026-08-08T22:46:02.791968Z","title":"2011, The Messenger, 146, 8","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.791968Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:f878e747cfcbc5da0bb4cb1463c1461f0cff482669bd7b4d8a22d8babe57a6f3","observation_id":"99212946-7433-46c1-88b0-e43d11df78f9","resolution":{"observed_at":"2026-08-08T22:46:02.791968Z","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":"2026-08-08T22:46:02.795330Z","title":"2019, , 625, A2","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.795330Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:4d9781a78add9aa9191c28b3bb381b340601fcac6efd5511199743cbcac37b94","observation_id":"d6aa85e2-ca6f-4b7d-851b-da0c76d3c429","resolution":{"observed_at":"2026-08-08T22:46:02.795330Z","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":"2026-08-08T22:46:02.799057Z","title":"2015, , 454, 3500","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.799057Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:49d8aaa3847f62dfb2495d4fa76eb4405f214a3657ecddc3594ada0de4f32f78","observation_id":"94be849c-a57d-4c00-ba41-22ce9eb71e35","resolution":{"observed_at":"2026-08-08T22:46:02.799057Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.389109Z","title":null,"venue":null,"work_id":"6bf37936-760d-4990-be77-0422bb00a81f","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.802448Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:55506097cfb0be2b35d9fe9707ade5e222bd2faa595075053ff47672e69c555c","observation_id":"7effe354-33ec-47be-85ba-c8da5b243264","resolution":{"observed_at":"2026-08-08T22:46:03.392301Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.379619Z","title":"2024, The Open Journal of Astrophysics, 7, 14","venue":null,"work_id":"4808ca0a-37a9-466a-9dc1-825e704b0c64","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.805774Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:3902d71ef50ee3cfb8bbc850cca139a30732a63411cc8a04f99726b997f63b7c","observation_id":"dece6bcb-e7df-4db4-a28b-4cc554ab0715","resolution":{"observed_at":"2026-08-08T22:46:03.382754Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.809027Z","title":"2023, , 108, 123518","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.809027Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:3e0da1a73fe556bb64f07332a7f1e7d789bc887c052bc4ce4644c9a3721479d1","observation_id":"6f9b8e2b-992f-426a-867e-86da1b85b0b7","resolution":{"observed_at":"2026-08-08T22:46:02.809027Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.364772Z","title":"A., & Ruan , C.-Z","venue":null,"work_id":"3153fa0d-b2d0-4c0e-8fb0-93ef94f3c867","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.812415Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:20b3b956d472f9d828abf07078f4a4f16bb71ebed1c25f4a5210fb87467f6f5a","observation_id":"69b17470-be98-4ea1-a45c-2a488781256d","resolution":{"observed_at":"2026-08-08T22:46:03.367907Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.815695Z","title":"J., Brieden , S., Tr \\\"o ster , T., & Heymans , C","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.815695Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:0987bef8e1c02fa8cc0e9e7ac4e6e750dd30bc8b093ace9e7f86bff69e15dd69","observation_id":"65672520-bf98-45a2-8f97-2e0ea796f9ab","resolution":{"observed_at":"2026-08-08T22:46:02.815695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.347582Z","title":"J., Peacock , J","venue":null,"work_id":"7720267d-c009-4909-8ef3-2b1db9511927","year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.818981Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:137f4da1a2e933995ad2bff652980db47f4d8049d81129eca260a8a113ec8b35","observation_id":"b645a458-824a-4603-90cc-bb1c38d23da0","resolution":{"observed_at":"2026-08-08T22:46:03.351069Z","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":"2026-08-08T22:46:03.336751Z","title":"A., Casarini , L., & Murante , G","venue":null,"work_id":"f2c57b8b-42ec-41c5-8922-69567aa53772","year":2012},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.822228Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:144ec503ed80612269904f720fa96f8035b5811fb9bc548b0dbaec50427eeb05","observation_id":"ad432f17-54f6-4800-b67c-5a9ee130b903","resolution":{"observed_at":"2026-08-08T22:46:03.340395Z","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":"2026-08-08T22:46:03.326306Z","title":"D., et al","venue":null,"work_id":"33b15784-e725-454d-a0f3-7f809aa51a53","year":2013},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.825875Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:602f5b8d6f111ea0eed68948d9b69d4a41bb56210c6fa19d189ea1719a17e479","observation_id":"4ff5b5b1-f3d5-4720-88f7-edc3cc70750c","resolution":{"observed_at":"2026-08-08T22:46:03.329885Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.829074Z","title":"& Takeuchi , T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.829074Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:a846aabb36b4dc275205fb729f92c05a8f5fb2b193728ae10862ae8cc9fbbb83","observation_id":"b4096490-b767-4ef1-a9ad-dc9be523a183","resolution":{"observed_at":"2026-08-08T22:46:02.829074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.310693Z","title":"2003, , 346, 994","venue":null,"work_id":"a9adbaf5-009e-47c1-b61b-e6c0682a12b3","year":2003},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.832380Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:e2a16b30d36872dfb8da7ae4972d064632e65ccb4475c3b18e1068c5e674b733","observation_id":"3bd640cc-4e41-4fef-8ee3-c16af30a66d5","resolution":{"observed_at":"2026-08-08T22:46:03.313744Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.835791Z","title":"2020, , 641, A6","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.835791Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:6335148d6fab692759098466a41cd70c3ea44ada79cad151c6c4fcb0e849c11d","observation_id":"6ab02be6-6321-4a56-be43-98779b5362f6","resolution":{"observed_at":"2026-08-08T22:46:02.835791Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.21980","last_updated":"2024-10-30T13:13:52Z","snapshot_observed_at":"2026-07-06T19:41:28.618975Z","submitted_at":"2024-10-29T12:10:20Z","title":"Impact of cosmology dependence of baryonic feedback in weak lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.21980","snapshot_observed_at":"2026-08-08T22:46:02.839016Z","title":", S., Krause , E., Dolag , K., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.839016Z"},"links":{"cited_paper":"/paper/2410.21980","citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:c7c9992a25038e254b380c4edd748f45d8f315192de4837454d143ba346188fc","observation_id":"6e4c01ea-7522-46bc-955d-ba21b9381b90","resolution":{"observed_at":"2026-08-08T22:46:02.839016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.296390Z","title":"2023, , 525, 5554","venue":null,"work_id":"454bfc87-26b9-41a6-9eba-c28e3886a095","year":2023},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.842615Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:8f976915ab54ac33c6129e8c564fa171f97106052455ae6f02100e6902be7722","observation_id":"21541371-8ec6-49f2-a73d-c33a410a9c25","resolution":{"observed_at":"2026-08-08T22:46:03.299374Z","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":"2026-08-08T22:46:03.286364Z","title":"2024, , 533, 621","venue":null,"work_id":"e1a91592-f5bd-4540-b73f-7f79d04e3b23","year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.846296Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:a19a9072f725d7210e8005af6155211196d4a8a13431deb07a4209126bb6c666","observation_id":"f3c9e372-42b3-48e3-bcb7-7346158106df","resolution":{"observed_at":"2026-08-08T22:46:03.289664Z","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":"2026-08-08T22:46:03.276664Z","title":"G., Kwan , J., Upadhye , A., & Font , A","venue":null,"work_id":"307bd7ad-6e37-408a-801b-2636fbe6bae0","year":2023},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.849503Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:caa993c4034b8fc6f40fa55469fbca41d342da14ab318503d2a763b105b31c70","observation_id":"eaf1a2d4-91e4-4d6d-a085-04ab4400362c","resolution":{"observed_at":"2026-08-08T22:46:03.279857Z","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":{"arxiv_id":"2410.17109","last_updated":"2025-04-29T08:27:08Z","snapshot_observed_at":"2026-07-06T19:37:56.214143Z","submitted_at":"2024-10-22T15:33:43Z","title":"The FLAMINGO project: Baryon effects on the matter power spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.17109","snapshot_observed_at":"2026-08-08T22:46:02.852929Z","title":"C., & van Daalen , M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.852929Z"},"links":{"cited_paper":"/paper/2410.17109","citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:c9a7f8340ad2d1b9526ee628a801806c6e670cf53a95d6e08ccb5af0d1fdd7ee","observation_id":"e913b3b3-bbc8-49bd-8d1f-14df991e547e","resolution":{"observed_at":"2026-08-08T22:46:02.852929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.267147Z","title":"K., Amodeo , S., & Refregier , A","venue":null,"work_id":"132f3233-e91b-4319-91ba-6fc6f28ceb91","year":2022},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.856604Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:c7aa36a2824f0a5cc6b7d06c7ccc76a6aee8fe5bbdcd0157fa986a2e91372f9d","observation_id":"60c7d975-a581-4f81-918c-2dc78e90db0d","resolution":{"observed_at":"2026-08-08T22:46:03.270449Z","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":"2026-08-08T22:46:03.257824Z","title":"& Teyssier , R","venue":null,"work_id":"0eb89337-afa3-4a49-b4a2-66b32079807b","year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.859853Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:ea3d667e0f06a25f77b64b294aa0493c7d135285a74f62c5b9e3e48415a9bd6b","observation_id":"f9ddaa8c-c6da-49eb-a83b-36c57dae8345","resolution":{"observed_at":"2026-08-08T22:46:03.261008Z","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":"2026-08-08T22:46:03.247729Z","title":"2006, in Saas-Fee Advanced Course 33: Gravitational Lensing: Strong, Weak and Micro, ed","venue":null,"work_id":"747bbf68-1027-4619-90a7-7666d39c217d","year":2006},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.862862Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:9ceeee17940eb60c9facf578fdaa8be38c1f4e273b632936286f81ab87716ae0","observation_id":"66b1111f-7c57-4f14-8e4a-bba19a0a6833","resolution":{"observed_at":"2026-08-08T22:46:03.251494Z","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":"2026-08-08T22:46:03.238279Z","title":"2010, , 520, A116","venue":null,"work_id":"8a43a411-b95a-4098-b5b6-9aac99644cb9","year":2010},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.866465Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:c058c6939f5cb5104267f5928f2fdbd9190f34be5b2a38b14d888102f0682302","observation_id":"30cfafa0-a256-4eb9-a91b-7264629dbedb","resolution":{"observed_at":"2026-08-08T22:46:03.241420Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.869866Z","title":"2002, , 396, 1","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.869866Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:83c4d0416b13c00155d089ac6acd71114245c9ab0b55c14c36be145a4edf03fd","observation_id":"1b9bfc65-540c-4b49-8655-79f26eb2d080","resolution":{"observed_at":"2026-08-08T22:46:02.869866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.222968Z","title":"F., Samuroff, S., Krause, E., et al","venue":null,"work_id":"26831f15-60fb-4add-8732-18a10058493e","year":2022},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.873074Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:adc5c037b8c94ba96acce67443c5859c437f94779696d47c3401817c8fe08fe4","observation_id":"2edd5644-928e-47f2-a1a5-011a45c6d097","resolution":{"observed_at":"2026-08-08T22:46:03.226273Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.876611Z","title":"1998, , 506, 64","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.876611Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:d6d32262efe1290380776a754401e94ff2f13eb2a00fda7b7deab4ba510c6596","observation_id":"ac693c89-4d16-41f0-aeb9-4e029740a1d0","resolution":{"observed_at":"2026-08-08T22:46:02.876611Z","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":"2026-08-08T22:46:02.880169Z","title":"2012, , 543, A2","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.880169Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:9cc40e5b1dbdc905e9a45e220a56114c26d0f69b7e39a2c2ec07ae4b19539a4c","observation_id":"2d4c2610-17fd-4206-95c7-c765f4636b56","resolution":{"observed_at":"2026-08-08T22:46:02.880169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.202115Z","title":"& Hilbert, S","venue":null,"work_id":"3e104223-4658-4358-9760-f1efc570c0d0","year":2018},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.883397Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:308c6152e3592bf9ed75547fb003586af820a506f3b71eaa8122fbe80849a963","observation_id":"bba864bd-702e-4b3e-afb7-f40364957c7a","resolution":{"observed_at":"2026-08-08T22:46:03.205337Z","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":"2026-08-08T22:46:03.192660Z","title":null,"venue":null,"work_id":"7e0f105c-64b5-4e84-a4c0-2284976bb2cf","year":2011},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.886743Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:c70ae28cee2edabb0bcace8169afaeae2ddcc3c99a4d9c6bbf083d0b5504a6d5","observation_id":"8ef24f13-0492-41e6-9e2c-69e8d8b6537b","resolution":{"observed_at":"2026-08-08T22:46:03.195804Z","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"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.182977Z","title":"E., Peacock , J","venue":null,"work_id":"0ad24f2a-5ba8-4fd5-96fa-85fa865eeeb1","year":2003},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.890198Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:09f2b5e1cafac4b7b53fedea4eda837753650263c2a75c35baf4b693ee00a7d7","observation_id":"d4e4ceb9-4a44-4ec5-b18b-16e38e664b38","resolution":{"observed_at":"2026-08-08T22:46:03.186249Z","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":{"arxiv_id":"1503.03757","last_updated":"2015-03-13T20:16:08Z","snapshot_observed_at":"2026-07-06T04:11:49.194805Z","submitted_at":"2015-03-12T14:57:27Z","title":"Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.03757","snapshot_observed_at":"2026-08-08T22:46:02.893628Z","title":"2015, arXiv:1503.03757","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.893628Z"},"links":{"cited_paper":"/paper/1503.03757","citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:bac6b9c8283806fdaaef2fcd00b53c8aeadd28ea7d69aa1d278b3d22ee738053","observation_id":"9d63e392-cae7-4774-98c8-bbc4fbd50265","resolution":{"observed_at":"2026-08-08T22:46:02.893628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.173121Z","title":"1995, , 100, 281","venue":null,"work_id":"84ae29eb-553f-484a-937a-e26c2861909b","year":1995},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.897344Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:e6c812160982c80ed6efaeb014b259ef209265b7f8cfa3ba4c06cc30a086cab6","observation_id":"21392f8b-5abb-496d-b9c3-97a751c620fc","resolution":{"observed_at":"2026-08-08T22:46:03.176473Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:02.900584Z","title":"2017, , 850, 24","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.900584Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:2d14632f3fb040acfdc47bd40aee195709b31633adbefda51d8d4d3bfd69e453","observation_id":"be3c1182-955b-4b60-9497-5a7bbbc11ca7","resolution":{"observed_at":"2026-08-08T22:46:02.900584Z","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":"2026-08-08T22:46:02.903760Z","title":"2012, , 761, 152","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.903760Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:14391e5d9585a79d5d9f83e865dfe1b552b22f20aa56a590ab4a990aed8dff48","observation_id":"408f4f2b-92a9-4765-96b5-da483e07ae30","resolution":{"observed_at":"2026-08-08T22:46:02.903760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.151345Z","title":"& Zaldarriaga , M","venue":null,"work_id":"8faf67d1-576d-47de-83cf-3a91e6483df1","year":2002},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.907380Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:779e01633dca80f92e97fdad37bb369600211721335efaaa5db7cf71139aa15d","observation_id":"8c5a8ec1-a7d5-4f7a-8ab9-7ac774f0fcfe","resolution":{"observed_at":"2026-08-08T22:46:03.154580Z","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":{"arxiv_id":"1809.01669","last_updated":"2021-09-06T19:01:58Z","snapshot_observed_at":"2026-08-03T07:05:48.933981Z","submitted_at":"2018-09-05T18:00:07Z","title":"The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.01669","snapshot_observed_at":"2026-08-08T22:46:02.910689Z","title":"2018, arXiv:1809.01669","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.910689Z"},"links":{"cited_paper":"/paper/1809.01669","citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:6772dc5f16d842af0a072ac96c5979762cf22dc7f9898d04fd6ffd97e2e109fe","observation_id":"5162e284-a7b0-4a49-a4bd-e668a644a967","resolution":{"observed_at":"2026-08-08T22:46:02.910689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.140756Z","title":"2021, , 649, A88","venue":null,"work_id":"238d3c83-41c1-4c8f-bf2d-8d5c6d0e36c3","year":2021},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.914294Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:30bfd462bb3393b8c12a3974b7fac3988f679e3763c5712c97a45540617de0dd","observation_id":"21e87250-66a5-4546-9a20-8f2174fbd5d5","resolution":{"observed_at":"2026-08-08T22:46:03.144253Z","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":{"arxiv_id":"2410.18191","last_updated":"2025-02-21T13:52:37Z","snapshot_observed_at":"2026-07-06T19:38:39.889993Z","submitted_at":"2024-10-23T18:00:21Z","title":"Baryon-free $S_8$ tension with Stage IV cosmic shear surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.18191","snapshot_observed_at":"2026-08-08T22:46:02.917552Z","title":"2024, arXiv:2410.18191","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.917552Z"},"links":{"cited_paper":"/paper/2410.18191","citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:5e526a0c083035a4a3bd394a3ae7187a6f2bd3142ab276771aa6e959fe545f3d","observation_id":"5ddb9137-9c29-4c7f-aae9-fee530260d34","resolution":{"observed_at":"2026-08-08T22:46:02.917552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.129777Z","title":"H., Hildebrandt , H., van den Busch , J","venue":null,"work_id":"c06c0281-071f-4a62-9f1c-83142cf9fc23","year":2020},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.921125Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:2d70489d2b8d6504c8e3f70f8abc2c213d6a6db714388603251bba37dd51fca1","observation_id":"72cc0f8c-06c9-4da7-bedb-06e2dc60fe43","resolution":{"observed_at":"2026-08-08T22:46:03.133391Z","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":"2026-08-08T22:46:03.118708Z","title":"H., Hildebrandt , H., van den Busch , J","venue":null,"work_id":"0c2f1e02-eec0-4a6b-8524-782b58360989","year":2020},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.924392Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:ad157cdeb07b7891e5bce40ec3ee1a96410830fdc02514eaaf2341703181e23e","observation_id":"85192f0e-28af-45b4-9c99-8a0ece904344","resolution":{"observed_at":"2026-08-08T22:46:03.122396Z","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":{"arxiv_id":"2411.07082","last_updated":"2024-11-11T15:58:24Z","snapshot_observed_at":"2026-07-06T19:48:32.368124Z","submitted_at":"2024-11-11T15:58:24Z","title":"A model-independent reconstruction of the matter power spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.07082","snapshot_observed_at":"2026-08-08T22:46:02.927690Z","title":"2024, arXiv:2411.07082","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.927690Z"},"links":{"cited_paper":"/paper/2411.07082","citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:bc86410d3e97a33a58d2f8a5b915ad8d39503a0dbcae53577239933e4e21fa1b","observation_id":"e1e9d859-5b3c-4869-87a9-b814b399cc4b","resolution":{"observed_at":"2026-08-08T22:46:02.927690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T22:46:03.106211Z","title":"1990, Physics Letters A, 150, 262","venue":null,"work_id":"3862c4b9-9e72-4870-bba5-066c5307ba3d","year":1990},"citing_paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing","version":2},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-08T22:46:02.931441Z"},"links":{"citing_paper":"/paper/2502.04449"},"observation_digest":"sha256:268e22f3944d4516e5b55ee547ea9632b61cad3358a9696c38736b6d23619aef","observation_id":"ed51580c-9e34-4e99-8e73-320c52c23ce7","resolution":{"observed_at":"2026-08-08T22:46:03.110908Z","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"}}],"paper":{"arxiv_id":"2502.04449","last_updated":"2025-05-02T08:43:43Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T08:54:18.155458Z","submitted_at":"2025-02-06T19:00:13Z","title":"KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing"},"reference_resolution":{"displayed":91,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":50,"verified_exact":0,"verified_fuzzy":41},"total_outbound_references":91},"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 91 of 91 outbound references and 0 inbound Pith citation observations for arXiv:2502.04449."}