{"as_of":"2026-08-07T20:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4e5a627b4b3aa04139e0ef98671cd6fbb19a49a753bc0413e69daa9c089191c6","coverage":[{"denominator":65,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":65,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T22:28:34.868971Z","state":"measured"},{"denominator":65,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":65,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2511.10634/citation-record","integrity":"/paper/2511.10634/integrity","json":"/paper/2511.10634/citation-record.json","paper":"/paper/2511.10634"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T22:28:27.214268Z","title":"Acevedo, H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.214268Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:3f3a7d0c0fe502ee2fb42dbc303a9831e43af86c029961a53a95eb2cb782431d","observation_id":"5764f19b-2ce8-47a6-981c-3c9b05379143","resolution":{"observed_at":"2026-08-03T22:28:27.214268Z","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":"2026-08-03T22:28:27.263610Z","title":"Biernacki and R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.263610Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:7a31d1bc7c8a6939317234029507dd95c037d8ec16c5389852772b58f2a1acaa","observation_id":"fbd1b18e-8a0a-4602-8590-a8a19cae12ca","resolution":{"observed_at":"2026-08-03T22:28:27.263610Z","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":"2026-08-03T22:28:27.354818Z","title":"Chisari, A.J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.354818Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:aa2b3451554d1de4cd0d65f983ae6a120465548ca32389b8c508c2edea689a26","observation_id":"c2f9eeb3-85b5-4247-b84f-ea58267bbb7a","resolution":{"observed_at":"2026-08-03T22:28:27.354818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.3447","last_updated":"2010-03-09T04:09:04Z","snapshot_observed_at":"2026-07-06T02:06:41.679342Z","submitted_at":"2010-01-20T02:30:42Z","title":"Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.3447","snapshot_observed_at":"2026-08-03T22:28:27.491749Z","title":"Duffy, J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.491749Z"},"links":{"cited_paper":"/paper/1001.3447","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:9ec9c199969ea909b3c81167684f18fb5651cd8ca59867a7e8ba0afd1558e1f2","observation_id":"861ac38c-0c65-48a3-a511-253938321778","resolution":{"observed_at":"2026-08-03T22:28:27.491749Z","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":"2026-08-03T22:28:27.542280Z","title":"van Daalen, J","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.542280Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:3d6dfa9294015ef719aad080bb316b3f4a64af9d5d1c6a91e7f58a41f8d7ef67","observation_id":"3c6b0c59-b733-46a8-a45d-824ab502b9da","resolution":{"observed_at":"2026-08-03T22:28:27.542280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.4461","last_updated":"2014-07-08T13:39:58Z","snapshot_observed_at":"2026-07-06T03:36:20.205229Z","submitted_at":"2014-02-18T20:15:31Z","title":"The impact of galaxy formation on the total mass, mass profile and abundance of haloes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.4461","snapshot_observed_at":"2026-08-03T22:28:27.720540Z","title":"Velliscig, M.P","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.720540Z"},"links":{"cited_paper":"/paper/1402.4461","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:625a60c0a49c335cc6f74d71162550ecafca4923e596101124ea28e6f7813938","observation_id":"819402ef-abf4-418c-a9d9-44c7fb2c1d87","resolution":{"observed_at":"2026-08-03T22:28:27.720540Z","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":"2026-08-03T22:28:27.785194Z","title":"Gebhardt, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.785194Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:6b65750921f1bbfb680a3130d2c411b6b69da45180b65394e9320beb9decf1ef","observation_id":"bd6cedae-652f-4536-9466-e49587294012","resolution":{"observed_at":"2026-08-03T22:28:27.785194Z","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":"2026-08-03T22:28:27.870556Z","title":"Schaye, R.A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:27.870556Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:8a11abe7d182f69b206925ab9aed05fddaf1a96a1540cea786f40c698a26dc3e","observation_id":"74b3e7f0-1560-4d2a-9592-867878e37a9e","resolution":{"observed_at":"2026-08-03T22:28:27.870556Z","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":"2026-08-03T22:28:28.019903Z","title":"Nicola, F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.019903Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:e5a65aadddca9070e8dbcdca2b7756ac07df6fa0bdde566c6da76bf6ddb32b4d","observation_id":"e0c3ab3f-ed9b-44fe-ab1e-87bd0ddf1a8c","resolution":{"observed_at":"2026-08-03T22:28:28.019903Z","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":"2026-08-03T22:28:28.064745Z","title":"Pandey, J.C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.064745Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:aaaacd82b0d987aaa58eeb696d6bb85124c35ae66cdcf29ffe3e2641fba3b795","observation_id":"dd393622-9796-4852-8801-b4a08a8560d8","resolution":{"observed_at":"2026-08-03T22:28:28.064745Z","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":"2026-08-03T22:28:28.210096Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.210096Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:6e688a873aacbb45764ce734728696c93f78cfc6e51bcb7232c155a58a7d321d","observation_id":"de45b3ca-ef32-413e-a4cf-dbcbb521ae34","resolution":{"observed_at":"2026-08-03T22:28:28.210096Z","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":"2026-08-03T22:28:28.283899Z","title":"Semboloni, H","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.283899Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:748b8eed35928b4f68737ed7ea40e87fa64e7fdd521b63d94a371dd5f47bb2de","observation_id":"90ecc491-7492-4b8e-a2f5-bea274408ef5","resolution":{"observed_at":"2026-08-03T22:28:28.283899Z","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":"2026-08-03T22:28:28.408943Z","title":"Zentner, E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.408943Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:cf51c59dc376689c8437a8af23a0e223b5c1bd40223cf201d02b0b1455a88764","observation_id":"aebd6855-54ea-44bb-adf3-1d32f4a009b1","resolution":{"observed_at":"2026-08-03T22:28:28.408943Z","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":"2026-08-03T22:28:28.517331Z","title":"van Loon and M.P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.517331Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:49e93d0aa558d8f7ee65e34f61b5f9e22f9da092f4f833c335dc8da53c22bed8","observation_id":"fdf2aee2-8f75-4163-b59a-9bedabef074c","resolution":{"observed_at":"2026-08-03T22:28:28.517331Z","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":"2026-08-03T22:28:28.583424Z","title":"van Daalen, I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.583424Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:1e10000731b0b20a426b0458f4d7987864c732f0270b86ddc1a11d0e13906bd4","observation_id":"187ed1a6-8e17-42a9-a6d3-41a8734d1347","resolution":{"observed_at":"2026-08-03T22:28:28.583424Z","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":"2026-08-03T22:28:28.691682Z","title":"Zentner, D.H","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.691682Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:a5cb857d97733a327d035fa4b6d2a291a865931558e366c7b8a36d9f890eff34","observation_id":"ca32db2d-6bd3-4c50-85f2-1cc3c1a656b4","resolution":{"observed_at":"2026-08-03T22:28:28.691682Z","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":"2026-08-03T22:28:28.774715Z","title":"Semboloni, H","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.774715Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:b34e09326a86c69f75d6b953d4f67d644370390df2648b4432ed93fb6505c74f","observation_id":"91ac92c0-67c9-4792-9dc3-c5db6a4eb653","resolution":{"observed_at":"2026-08-03T22:28:28.774715Z","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":"2026-08-03T22:28:28.864843Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.864843Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:a2a316002fbe83cc7a5029dc81b9bbe78b8e30848fd704db79083204e64b87e8","observation_id":"f94f52b8-a80f-4152-beab-93fee0c4ace0","resolution":{"observed_at":"2026-08-03T22:28:28.864843Z","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":"2026-08-03T22:28:28.965738Z","title":"Osato and D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:28.965738Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:17c24cf97f3a49c392528c43d863dbbcfc44abdb3f3ebd0d3284a29645234fb6","observation_id":"7ae41204-2e62-4e1b-af4e-d5b6df69fa1b","resolution":{"observed_at":"2026-08-03T22:28:28.965738Z","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":"2026-08-03T22:28:29.122394Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.122394Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:d9c6cebbc6cb0c0efa1a939161fb86a45d42cdcd99521abc01badd56d86f5919","observation_id":"ec3a71e9-2d85-4698-923c-04d66c8787fa","resolution":{"observed_at":"2026-08-03T22:28:29.122394Z","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":"2026-08-03T22:28:29.257194Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.257194Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:a46f5f2d4af86e5e5cbadeb5672c0bf9996837e405935299e9447f62ff7112cc","observation_id":"002f98a3-1ccf-42fe-8f66-b1e1475da790","resolution":{"observed_at":"2026-08-03T22:28:29.257194Z","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":"2026-08-03T22:28:29.373741Z","title":"Hadzhiyska, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.373741Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:1a3e2a75698d29bde329db6745832ec11ae0e9dfd0b37c3f9f0b744c3e394471","observation_id":"fd168964-6762-47d0-a42a-da9248dec858","resolution":{"observed_at":"2026-08-03T22:28:29.373741Z","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":"2026-08-03T22:28:29.482847Z","title":"Huang, T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.482847Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:60d597b0715664813d3cb65fd348abf6a1570d257366c144c3e6f979d55d80c4","observation_id":"f9276705-933e-457d-8f82-91685fc7dffc","resolution":{"observed_at":"2026-08-03T22:28:29.482847Z","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":"2026-08-03T22:28:29.577969Z","title":"Schneider, S.K","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.577969Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:83925477056d2dbae3df7fb52ac2d0296ac971dd2a8a5f4483138b60f025eefc","observation_id":"baac7fd2-910d-43b6-9423-f31a27444ffa","resolution":{"observed_at":"2026-08-03T22:28:29.577969Z","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":"2026-08-03T22:28:29.738574Z","title":"Bigwood, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.738574Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:51e8a887150c2aaef39e3f036853e2cf6190b4ceaa0b58623f4ad4489241f30e","observation_id":"f30d9cb4-ea83-4cda-ba8a-5aa12ead2a3a","resolution":{"observed_at":"2026-08-03T22:28:29.738574Z","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":"2026-08-03T22:28:29.889849Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.889849Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:776bf3a02f80067c15646cbb2a872021adbf5002185d9572717573a5ef6a37f4","observation_id":"d9360d0e-36f3-4af7-b5bc-d096720711c0","resolution":{"observed_at":"2026-08-03T22:28:29.889849Z","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":"2026-08-03T22:28:29.991096Z","title":"Siegel, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:29.991096Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:b3000f5e9e5e95a2096b2417c0e1e7bb7553587a9dbcfe0dc8ab3fc665798c13","observation_id":"896824ad-8a2f-41c7-bb63-799812fcba88","resolution":{"observed_at":"2026-08-03T22:28:29.991096Z","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":"2026-08-03T22:28:30.090776Z","title":"Terasawa, X","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.090776Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:dc7375e4cf0fbb80a8942854861d359653a2a7cf42a47ede990c11c773f95d16","observation_id":"19624081-5d9d-48f4-90cb-20df5a1c8d61","resolution":{"observed_at":"2026-08-03T22:28:30.090776Z","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":"2026-08-03T22:28:30.193071Z","title":"Sarmiento, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.193071Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:40731bb6ad8c97fb49c3919601b8ac049443d55b5d330f30f0fa484070fcd371","observation_id":"00a0eb34-ea16-46c9-8c00-48dd4ebccdfe","resolution":{"observed_at":"2026-08-03T22:28:30.193071Z","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":"2026-08-03T22:28:30.333838Z","title":"Le Brun, I.G","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.333838Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:748756edcebdee5e29f2442f84e2e3aa11838357e63e52252d38a9d329ad4096","observation_id":"52697629-be9e-48cc-a3d6-a89c331303d1","resolution":{"observed_at":"2026-08-03T22:28:30.333838Z","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":"2026-08-03T22:28:30.495399Z","title":"McCarthy, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.495399Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:990be4ee48543efb20374178139754a4099313bf38d350d376cf068157b49586","observation_id":"83e60c88-9902-45f2-ae56-92bfc32602ab","resolution":{"observed_at":"2026-08-03T22:28:30.495399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.05609","last_updated":"2021-01-29T12:39:54Z","snapshot_observed_at":"2026-08-06T07:54:21.162006Z","submitted_at":"2018-12-13T19:00:00Z","title":"The IllustrisTNG Simulations: Public Data Release","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.05609","snapshot_observed_at":"2026-08-03T22:28:30.578531Z","title":"Nelson, V","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.578531Z"},"links":{"cited_paper":"/paper/1812.05609","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:ce5fb4a066fbed519c0c13e94877b25947307d6a34b824d411587e7c6cf205e1","observation_id":"3e3e3e3e-55ee-437c-b92e-1cb8c1b95827","resolution":{"observed_at":"2026-08-03T22:28:30.578531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.03406","last_updated":"2018-01-31T17:24:58Z","snapshot_observed_at":"2026-07-06T05:50:42.132417Z","submitted_at":"2017-07-11T18:00:07Z","title":"First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.03406","snapshot_observed_at":"2026-08-03T22:28:30.658923Z","title":"Pillepich, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.658923Z"},"links":{"cited_paper":"/paper/1707.03406","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:d14fdef140abc998d68b0247754d02d68f316199ae0617384492132676511b09","observation_id":"5e047be8-f4f1-4235-93b4-de8b30aa2c15","resolution":{"observed_at":"2026-08-03T22:28:30.658923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.03396","last_updated":"2018-08-24T16:46:30Z","snapshot_observed_at":"2026-07-06T05:50:42.132417Z","submitted_at":"2017-07-11T18:00:00Z","title":"First results from the IllustrisTNG simulations: radio haloes and magnetic fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.03396","snapshot_observed_at":"2026-08-03T22:28:30.716774Z","title":"Marinacci, M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.716774Z"},"links":{"cited_paper":"/paper/1707.03396","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:c61cc1066251faa996cadf389f7e9ef0162406b28967afa123a794e1f9fcbf95","observation_id":"5d42ff2c-b489-4a0c-ac58-94fad33cf8ed","resolution":{"observed_at":"2026-08-03T22:28:30.716774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.03401","last_updated":"2018-03-14T19:02:24Z","snapshot_observed_at":"2026-07-06T05:50:42.132417Z","submitted_at":"2017-07-11T18:00:02Z","title":"First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.03401","snapshot_observed_at":"2026-08-03T22:28:30.791000Z","title":"Naiman, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.791000Z"},"links":{"cited_paper":"/paper/1707.03401","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:4478761cd13426c38f4d49c1d76390bb4f65ab2dd93e142aacdfe98f9d3cf52a","observation_id":"3eaa6856-fc49-4b09-8ab7-1327a6b0583e","resolution":{"observed_at":"2026-08-03T22:28:30.791000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.03397","last_updated":"2017-12-21T12:49:59Z","snapshot_observed_at":"2026-07-06T05:50:42.132417Z","submitted_at":"2017-07-11T18:00:01Z","title":"First results from the IllustrisTNG simulations: matter and galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.03397","snapshot_observed_at":"2026-08-03T22:28:30.942905Z","title":"Springel, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:30.942905Z"},"links":{"cited_paper":"/paper/1707.03397","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:68a339a8dda5538eb43f64e33810cd3ee6dff4b639eff103cde8f6ec8544a957","observation_id":"f64125a6-b9dc-4634-9cce-ce792479f636","resolution":{"observed_at":"2026-08-03T22:28:30.942905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.2921","last_updated":"2014-09-20T18:22:21Z","snapshot_observed_at":"2026-07-06T03:43:29.356334Z","submitted_at":"2014-05-12T20:00:00Z","title":"Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.2921","snapshot_observed_at":"2026-08-03T22:28:31.062100Z","title":"Vogelsberger, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.062100Z"},"links":{"cited_paper":"/paper/1405.2921","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:84bdc74af773afab855cb0556c33c76bdb4b2d4e0171b75de799f7d5c0283de0","observation_id":"504a5144-e416-494f-a3dd-26be7f86702e","resolution":{"observed_at":"2026-08-03T22:28:31.062100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.3749","last_updated":"2014-08-12T20:27:49Z","snapshot_observed_at":"2026-07-06T03:43:45.357180Z","submitted_at":"2014-05-15T05:54:42Z","title":"Introducing the Illustris Project: the evolution of galaxy populations across cosmic time","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.3749","snapshot_observed_at":"2026-08-03T22:28:31.139659Z","title":"Genel, M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.139659Z"},"links":{"cited_paper":"/paper/1405.3749","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:c84c2071a9798a7b8e85b9b7999f391f7ced2927eb3275db7c593ac6f0e573f0","observation_id":"0ea49b85-485e-4e95-bf3b-75add17e3ef1","resolution":{"observed_at":"2026-08-03T22:28:31.139659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.6842","last_updated":"2015-06-16T22:00:49Z","snapshot_observed_at":"2026-07-06T03:52:53.853730Z","submitted_at":"2014-08-28T20:00:08Z","title":"The Illustris simulation: the evolving population of black holes across cosmic time","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.6842","snapshot_observed_at":"2026-08-03T22:28:31.241782Z","title":"Sijacki, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.241782Z"},"links":{"cited_paper":"/paper/1408.6842","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:59af3bcb1da23b5303081ba04343866cca58c0603122181becc6c648b86803d7","observation_id":"34c74694-a8b5-4066-be86-b568c1a27e2b","resolution":{"observed_at":"2026-08-03T22:28:31.241782Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1418","last_updated":"2014-05-06T20:00:19Z","snapshot_observed_at":"2026-07-06T03:43:00.562490Z","submitted_at":"2014-05-06T20:00:19Z","title":"Properties of galaxies reproduced by a hydrodynamic simulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1418","snapshot_observed_at":"2026-08-03T22:28:31.352939Z","title":"Vogelsberger, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.352939Z"},"links":{"cited_paper":"/paper/1405.1418","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:f24711f8efd3f686051932ca197ad38b0b64a319344657d462ed1616ceaa244e","observation_id":"5fe52943-b13a-49f0-9784-193117970009","resolution":{"observed_at":"2026-08-03T22:28:31.352939Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.4107","last_updated":"2009-10-31T09:23:03Z","snapshot_observed_at":"2026-08-06T17:34:39.030758Z","submitted_at":"2009-01-27T17:30:33Z","title":"E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.4107","snapshot_observed_at":"2026-08-03T22:28:31.521019Z","title":"Springel,E pur si muove: Galilean-invariant cosmological hydrodynamical simulations on a moving mesh,Mon","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.521019Z"},"links":{"cited_paper":"/paper/0901.4107","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:9d688a369b503b02a9d8f16aaf2846ba44bb8086aaa074420d4b7736c1838985","observation_id":"d0a1924b-6c2e-4069-b5cf-32c5adfc87df","resolution":{"observed_at":"2026-08-03T22:28:31.521019Z","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":"2026-08-03T22:28:31.651278Z","title":"Weinberger, V","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.651278Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:a188230ba0167327e2a54865db0084cc4859738252b147165fb0f64c81f1da86","observation_id":"23acab65-29f4-4e88-ab7c-98ccf2469ec1","resolution":{"observed_at":"2026-08-03T22:28:31.651278Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0012055","last_updated":"2000-12-03T14:33:15Z","snapshot_observed_at":"2026-07-07T00:14:26.519053Z","submitted_at":"2000-12-03T14:33:15Z","title":"Populating a cluster of galaxies - I. Results at z=0","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0012055","snapshot_observed_at":"2026-08-03T22:28:31.760334Z","title":"Springel, S.D.M","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.760334Z"},"links":{"cited_paper":"/paper/astro-ph/0012055","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:2368e975fd469b8d25325a6abe641556bb2f9cfe026776562b2974832d9ff057","observation_id":"bbccee2c-1841-4eff-ae50-8c58c72545dd","resolution":{"observed_at":"2026-08-03T22:28:31.760334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3401","last_updated":"2009-05-11T15:10:58Z","snapshot_observed_at":"2026-07-31T09:29:08.904807Z","submitted_at":"2008-08-25T20:03:21Z","title":"Substructures in hydrodynamical cluster simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3401","snapshot_observed_at":"2026-08-03T22:28:31.930931Z","title":"Dolag, S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:31.930931Z"},"links":{"cited_paper":"/paper/0808.3401","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:675e518ad5bd0ad9a1b4406f88b0dfa958a05a6721405beec181ae82eb9d3db2","observation_id":"b2cf423e-f9cd-4f31-b79e-486f7d2daf8e","resolution":{"observed_at":"2026-08-03T22:28:31.930931Z","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":"2026-08-03T22:28:32.079206Z","title":"Nelson, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.079206Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:09df3dec6dd75a3e372ab6eae0d2c57ca527724fc9300f184c3a90fc5376a335","observation_id":"d59f2142-d42c-4b68-a4c0-725657345a89","resolution":{"observed_at":"2026-08-03T22:28:32.079206Z","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":"2026-08-03T22:28:32.210721Z","title":"More, F.C","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.210721Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:b5ffd014779ed1096b6abbe66858fce34eff1df3c6dd8de66c84e1c34967b89f","observation_id":"abe02389-245a-4322-929f-84a243d271fc","resolution":{"observed_at":"2026-08-03T22:28:32.210721Z","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":"2026-08-03T22:28:32.385967Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.385967Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:1babb9d3e1cce75da5a58f126f345374ce51bcdd48e00b850d91c208f4c1df59","observation_id":"2ccdd69a-eee3-4fef-a489-f6c8edbf2197","resolution":{"observed_at":"2026-08-03T22:28:32.385967Z","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":"2026-08-03T22:28:32.476417Z","title":"Jenkins, C.S","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.476417Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:03024a65e4b98bb2780cf95ea9ecdcf400f2b3990c58d4ca364f39beeb013622","observation_id":"6fdedeb0-1cbe-4641-977d-b05613708386","resolution":{"observed_at":"2026-08-03T22:28:32.476417Z","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":"2026-08-03T22:28:32.578888Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.578888Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:dd0aa77065045ed12d45a331c4638729f249b8c28346a4ca36db674b11736bef","observation_id":"eb10a38d-dde8-4586-a1bb-be28f6ffd303","resolution":{"observed_at":"2026-08-03T22:28:32.578888Z","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":"2026-08-03T22:28:32.753927Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.753927Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:2f200efabef79a224c341173fd063a2250a7efddc29390a260e070531c34e6f1","observation_id":"6d250708-1f88-4c6f-8b25-ca031f0fc49a","resolution":{"observed_at":"2026-08-03T22:28:32.753927Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.3804","last_updated":"2015-06-10T23:16:15Z","snapshot_observed_at":"2026-07-06T04:03:20.231427Z","submitted_at":"2014-12-11T21:00:03Z","title":"A new methodology to test galaxy formation models using the dependence of clustering on stellar mass","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.3804","snapshot_observed_at":"2026-08-03T22:28:32.907223Z","title":"Campbell, C.M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.907223Z"},"links":{"cited_paper":"/paper/1412.3804","citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:83b1253eeb7660f081187388ac896ba4cea309b8cadfed7d5426c3aca22bcfb8","observation_id":"947acec0-d66f-40de-be7e-6df2b155278f","resolution":{"observed_at":"2026-08-03T22:28:32.907223Z","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":"2026-08-03T22:28:32.966749Z","title":"Pillepich, V","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:32.966749Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:b9926fec170b9312bf9afb819dca9a2ca562b270dd6b48d6625a824468efeb2a","observation_id":"9a206001-46bc-4be5-be6d-de777a980b2c","resolution":{"observed_at":"2026-08-03T22:28:32.966749Z","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":"2026-08-03T22:28:33.163741Z","title":"Weinberger, V","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:33.163741Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:b54614146bcff337e51d264f6726b11628dae0330fcb1a0c440009eacec702ee","observation_id":"7bdcddfe-a4b3-4716-a631-fef722db566f","resolution":{"observed_at":"2026-08-03T22:28:33.163741Z","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":"2026-08-03T22:28:33.285296Z","title":"Chisari, M.L.A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:33.285296Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:78038c29e745c98fb12aad560b97f6517560ef9e585de570dbc2ba041698293d","observation_id":"fb568e62-47d4-47b3-a36f-f26e4c4565ad","resolution":{"observed_at":"2026-08-03T22:28:33.285296Z","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":"2026-08-03T22:28:33.430017Z","title":"Secco, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:33.430017Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:9653f5e363a7921c33dbe5fdae7618c1a67058ea9e84647773312f2439a8e914","observation_id":"773d6139-34d6-40bf-a32c-dbba53af876d","resolution":{"observed_at":"2026-08-03T22:28:33.430017Z","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":"2026-08-03T22:28:33.493855Z","title":"Aric` o, R.E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:33.493855Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:df7b65a73a9e7da279c25dcd3e14b48b10558dc25c6aa7c8804544ec073cb137","observation_id":"538fa36e-a942-421a-85e5-31fa8744b78f","resolution":{"observed_at":"2026-08-03T22:28:33.493855Z","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":"2026-08-03T22:28:33.612179Z","title":"Schneider, R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:33.612179Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:ae42d6c340f760ba0011aec7c6ac4a253466a6d5944770856052b1bbe6d4fba3","observation_id":"9bf51f36-326f-453f-994d-5ab88d8b673e","resolution":{"observed_at":"2026-08-03T22:28:33.612179Z","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":"2026-08-03T22:28:33.680970Z","title":"Lucie-Smith, H.V","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:33.680970Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:455b64846cae6fe2053d8fe919f80a881d47137b8b0d0e493ca963301fd7830d","observation_id":"7ad2318d-81c6-4a18-a5f2-589270d54d75","resolution":{"observed_at":"2026-08-03T22:28:33.680970Z","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":"2026-08-03T22:28:33.869753Z","title":"Hadzhiyska, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:33.869753Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:1cf6a31be6b5176d12763a5554caae8ad14799cd8618c89f64ca7ae58d9d1390","observation_id":"8f08853f-1181-4a14-9095-623fd81dba1e","resolution":{"observed_at":"2026-08-03T22:28:33.869753Z","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":"2026-08-03T22:28:34.008885Z","title":"Roper, Y.-C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:34.008885Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:f9f079c31bb8d7e1d26be2028969fbcd1dbaa964516e61a65835145c1b4b77df","observation_id":"cbb18f28-bf08-4ec1-8a92-20e03cf8dc1e","resolution":{"observed_at":"2026-08-03T22:28:34.008885Z","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":"2026-08-03T22:28:34.203460Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:34.203460Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:764258397ae7ab741a08fac595bc84af976dd2978f06bd6e067cc6f2be1c1e98","observation_id":"e7d3a718-ef9d-4b9b-ac92-f17de67d0c59","resolution":{"observed_at":"2026-08-03T22:28:34.203460Z","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":"2026-08-03T22:28:34.419762Z","title":"Zhang, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:34.419762Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:602b09df1465d87e24d1ed1cc5abfbee00203233285d3ac2a8cbd2c607d4c955","observation_id":"c76e636e-f374-4462-9e00-7cd22348315a","resolution":{"observed_at":"2026-08-03T22:28:34.419762Z","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":"2026-08-03T22:28:34.554256Z","title":"Collaboration, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:34.554256Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:4d44a426fa5e3ea74770d7ba7e4bef160149eb3761734046f1f50fdaaf08acca","observation_id":"99996f22-0cae-4018-9485-188b8f65640f","resolution":{"observed_at":"2026-08-03T22:28:34.554256Z","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":"2026-08-03T22:28:34.681799Z","title":"Nishimichi, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:34.681799Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:5b52bce947c605a7f96d07a9b19f6f3741fcab60f20c42e870476ba225811d3a","observation_id":"72ff9e86-4b7e-4f3d-ac51-651af8ead954","resolution":{"observed_at":"2026-08-03T22:28:34.681799Z","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":"2026-08-03T22:28:34.868971Z","title":"Aric` o, R.E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-03T22:28:34.868971Z"},"links":{"citing_paper":"/paper/2511.10634"},"observation_digest":"sha256:fe963f16a18b84ffa7cf72278fd0690664ee43ef79e11c4f837bd47454612e5b","observation_id":"995031f6-c8b8-4ce3-9f7e-8777c67a6f89","resolution":{"observed_at":"2026-08-03T22:28:34.868971Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2511.10634","last_updated":"2026-03-17T22:11:21Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-06T15:28:56.598693Z","submitted_at":"2025-11-13T18:55:17Z","title":"Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum"},"reference_resolution":{"displayed":65,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":65,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":65},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 65 of 65 outbound references and 0 inbound Pith citation observations for arXiv:2511.10634."}