{"as_of":"2026-08-10T12:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2d72ea7c369cde24f36c313316a6254755c131a9ac261f6b3611c6c31e627270","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":"2026-08-10T06:31:04.303077+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":"2026-08-08T15:20:37.216699Z","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":"sha256:07e2bda49970a05530c74bcad1f6cb1e3ae8534a72f16121eec84dd7dbe05831","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":"2026-08-08T15:20:37.216699Z","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":"sha256:522439e5d5c9893d03fbb70ee1f45b42d27be27d33a1291aab862c75623fd37c","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":"2026-08-08T15:20:37.216699Z","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":"sha256:77dbbc00e3f3870702fa6a05c6c082c809d9a58059097635f76b5a3e177e1db7","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":"2026-08-08T15:20:37.216699Z","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":"sha256:408b2484a95cdf60e6f268b33ebdf75965c834394384fd93929552b6f714bf0f","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":"2026-08-08T15:20:37.216699Z","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":"sha256:2ca320d6b61e347eb337c3dbfda7cd94e3d0f066ff743c640b3de7a7bd35ccb4","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":"2026-08-10T04:01:21.594837Z","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":"2026-08-08T15:20:37.216699Z","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:ebebe12e8cfb787c567535761eb46c53f024464d800de33978bc123fb4169f98","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":"2026-08-08T15:20:37.216699Z","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":"sha256:5aa927ddda4e92d4e9069ad66cb167f7ff07563b409d035a15f69e7504101e25","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":"2026-08-08T15:20:37.216699Z","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":"sha256:8f2abbaeea7562d1d43b0b9405715797385ff2265501417a738151b972fc1072","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":"2026-08-08T15:20:37.216699Z","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":"sha256:0197a3adc594b13cea3d1dbf4ac70840682cc7f809604df58b2718355a5db8ff","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":"2026-08-08T15:20:37.216699Z","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:c979cd06fa88feb242b14948edc73aa15bd31416a38ffb2835e67055a285f882","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":"2026-08-08T15:20:37.216699Z","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":"sha256:2ee161604a992241fbd70f10a3191d32a3e8ee73229a2e54d2e606031a0f4cab","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":"2026-08-08T15:20:37.216699Z","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:c0f2e8fa35216edd51924eb1f612c219718cc8de4eb9227f746f70aa5d480c8c","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":"2026-08-08T15:20:37.216699Z","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":"sha256:9b5b143d202325fb3dce8a4f4c72b386be7b25547087f413b0b8adc82612b895","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":"2026-08-08T15:20:37.216699Z","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":"sha256:3ecfcb0e81f7ce1864391d9cb88aa6eb6ada8a66dd3b18c0f1fec80bccd403a5","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":"2026-08-08T15:20:37.216699Z","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":"sha256:568ec051a8c96dcd361d3d935ec3dd91765824c007031e7ac05584a2ced2e733","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":"2026-08-08T15:20:37.216699Z","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:f9d446d20595aaef438501134de97945d08810b6ff43439eb93cf5ba4a259465","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":"2026-08-08T15:20:37.216699Z","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":"sha256:8b2a25a23727dbd7637261cbeecc0f360d55c7d891fd53275d05105ce04c12b4","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":"2026-08-08T15:20:37.216699Z","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":"sha256:8e4e108339ec73737819299a760599effd0878cf1b720b0809f5792e5c7d16f9","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":"2026-08-08T15:20:37.216699Z","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":"sha256:77de4a58e52e84e4fa9a7e6e96ce7b91a7e9d67faefbea6579d8e7be588de024","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":"2026-08-08T15:20:37.216699Z","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":"sha256:04deb5c135f6c7b5a73a18cce9d144d10c28da38f89b34da71730d3eea6ac28f","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":"2026-08-08T15:20:37.216699Z","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":"sha256:35348507ca7edd1d38f5d0325d32bce0e38d40f297ec25654ab51e683ab405ea","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":"2026-08-08T15:20:37.216699Z","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":"sha256:1ea3ac7e2d7235335705e377f2c420be00a5c4c88206797892e70b88629dd648","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":"2026-08-08T15:20:37.216699Z","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":"sha256:1b51626d8b5421076ae843ed3080cbff75c8e294ccb2178b2e0c6e77bb88bca9","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":"2026-08-08T15:20:37.216699Z","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":"sha256:3fe308d046c8cf19dbe8acd5ca84b6c70336f1d8a28b01938a9813b1fb1b4274","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":"2026-08-08T15:20:37.216699Z","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":"sha256:9ae23064035146707b7f7b651e72a0617877bbe81f68ca4962543ba743c17e44","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":"2026-08-08T15:20:37.216699Z","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:a31db2297766a36c759423c33c49e3158571b205dbd40f714dc7392618c4fccb","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":"2026-08-08T15:20:37.216699Z","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:a3d783d6803eaad0ee820bb765481664697db6955ed45660707bd60951fab5e2","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":"2026-08-08T15:20:37.216699Z","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":"sha256:06f637b10cf49f1f34480101184c1c89fa44aad57bca9f5364599dc534708ee5","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":"2026-08-08T15:20:37.216699Z","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:decbb0d21adbabf9a97959106b8935cfb69cdf48965f242e0097ff985237812d","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":"2026-08-08T15:20:37.216699Z","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:ec26957a15db58a264664b92750819e867372a0c5207e159349fd52c2733f10f","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":"2026-08-08T15:20:37.216699Z","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:fcf8e57b95af24ef0d298376321058c51a2d29f3351260f4ad3b087cfa1d1f32","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":"2026-08-08T15:20:37.216699Z","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:e51776febc329648fc2d4ca1e17293c46385dacc49f2bc970836e7b9814564a4","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":"2026-08-08T15:20:37.216699Z","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":"sha256:23722b665b757de4aa57dd2612c3948970f5d67fed2cc2f111ad026b5cf7020c","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":"2026-08-08T15:02:42.058320Z","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":"2026-08-08T15:20:37.216699Z","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":"sha256:314dfc865e6ffd6f344802a6660c35bd50e1b0d5898c795103c1b01dab57a22f","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":"2026-08-08T17:16:07.037805Z","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":"2026-08-08T15:20:37.216699Z","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:c307bccaf27d5a1bafa98ca1e7ad99b143b6c83e8336569a4d4397263b2f80b0","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":"2026-08-10T10:37:00.201799Z","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":"2026-08-08T15:20:37.216699Z","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":"sha256:5f9b35ec36d3efb22f9b18e20544242608cb0c7a8ac2c50cb47bf2a3ae5419a7","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":"2026-08-10T10:58:46.408503Z","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":"2026-08-08T15:20:37.216699Z","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:cf44ff316e91e215c65518ec48c8e992f6fbe7aed74c00d5d3a9ca18f2cc769c","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":"2026-08-08T15:20:37.216699Z","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":"sha256:2e1341ff1443ccb3819a81f21c144b548a2cdf3f3a05643b940403d7b3eabcfd","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":"2026-08-08T15:20:37.216699Z","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":"sha256:23a22abd0513645ad8e7dfc9092e875221f6c142d017f183ce05baac8e2f8049","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":"2026-08-08T15:20:37.216699Z","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:d6d8b096628f6a8c8ca9728815e9406ad9722a16a9205cbe920d1123c2babeba","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":"2026-08-08T15:20:37.216699Z","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":"sha256:7ea5cd05160a19234ba0c0965719a798f943968652f685ce7e437247f6bc253f","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":"2026-08-08T15:20:37.216699Z","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:e3ed673dc164b0f1293ddc9ea2ff0a17286292ab5bfe25616d214da805713e18","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":"2026-08-08T15:20:37.216699Z","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":"sha256:530058a169cf3b38bfcf1d63e9dbfd64ec5843be43fe3f0735dce677a213b701","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":"2026-08-08T15:20:37.216699Z","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":"sha256:3529479727f1faca4e457c30c7bed056eef8e87cd704b15f38f87b5585b53e67","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":"2026-08-08T15:20:37.216699Z","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:c20f5bb997789ee58d26b85349912bea121e919bcbe4a1774eb7c0f674c1e52f","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":"2026-08-08T15:20:37.216699Z","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":"sha256:546e3bd6488ed1760da264dae7d9379c409d56f574445b14f81c3e92f1ccb86e","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":"2026-08-08T15:20:37.216699Z","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":"sha256:28487aa3896ee0adcb1206a0e4af5ae833e988da87b3a17a523ae97d806eeb95","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":"2026-08-08T15:20:37.216699Z","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":"sha256:2e4ee8201263f8bc6543217aacd0c443d6e8e5ddb60aa44287766b20b159c064","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":"2026-08-08T15:20:37.216699Z","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":"sha256:5ccc1753de341c8759c6ec166cbdf605dc21edc7eac390fc3d0e62a5cb0880a1","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":"2026-08-08T15:20:37.216699Z","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:c52e3b39eb3f86239cc92eb8a013b9cf33f7ccb3c859bd683e56300ad063ff72","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":"2026-08-08T15:20:37.216699Z","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:c841b990172df7c5025c8cfe8adf074fda5c2716e8e57e7cf7ba292e1d65c201","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":"2026-08-08T15:20:37.216699Z","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:e4443f238e93de320cab1cbdbf19b0fd801297796f047b2d073f19ada2e8f461","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":"2026-08-08T15:20:37.216699Z","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":"sha256:91c4e3f3edee1f632c981bfa7d3767669085a7185c7e7b8582e2ee53a77ca4ff","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":"2026-08-08T15:20:37.216699Z","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":"sha256:30e9b9330866648192134976520ea9f6753bb0a8d113b2be13f4667b5fe46504","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":"2026-08-08T15:20:37.216699Z","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":"sha256:75837e3f1b8a7588ba700658d64ee85adc9212ff1c419c87e9bb509f4e0d05f4","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":"2026-08-08T15:20:37.216699Z","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":"sha256:340983fc69d33ec3f5462cdea223d41d06c2ee10f71eae273be346e6437e3c4e","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":"2026-08-08T15:20:37.216699Z","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":"sha256:6eaf6d1432f8d179e9a7e6319b7bce3e189c616b0a400271bf014731d3c1f679","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":"2026-08-08T15:20:37.216699Z","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":"sha256:2e0226d0f546e2b347cc0f295312f434143dbe990a3e5402163ff00158e972c7","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":"2026-08-08T15:20:37.216699Z","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:f886e4e5ab7d32ffab0601401b68dd3be94e248f5aebbf633d1ba20dca68e519","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":"2026-08-08T15:20:37.216699Z","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":"sha256:7a149b4b42f16dc62205e132290010031d37be3455eed8a7e4845fe14e9f7982","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":"2026-08-08T15:20:37.216699Z","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:a03fe47815757651e2339806d42a78306de37d3c36784134319f8afe66fed40c","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":"2026-08-08T15:20:37.216699Z","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":"sha256:52ef15faddc22629f0d8ba90df5802067f219e68596f949716b19135a4dd8f08","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":"2026-08-08T15:20:37.216699Z","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":"sha256:04c93d3113bbced91948b5f37d40e7874a931a667b8a8d67ad0af930f87e61b8","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":"2026-08-08T15:20:37.216699Z","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":"sha256:1a806ffa00023dd03aac1bcdfea71c7009aa7d80fa7b2e33c3476330f934df16","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":"2026-08-08T15:20:37.216699Z","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":"sha256:9fcf9edf6429f46730c6df2c1f5432d9487e885edd4c5afc66d6e71d5cb1eb22","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":"2026-08-08T15:20:37.216699Z","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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 65 of 65 outbound references and 0 inbound Pith citation observations for arXiv:2511.10634."}