{"as_of":"2026-08-19T08:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4b5cd3af4b426de398b615602df921b4c127e12df406a7308b5c3efd797a1b76","coverage":[{"denominator":84,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":84,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T05:25:09.242034Z","state":"measured"},{"denominator":84,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":84,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+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/1909.01329/citation-record","integrity":"/paper/1909.01329/integrity","json":"/paper/1909.01329/citation-record.json","paper":"/paper/1909.01329"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:08.857102Z","title":"V ., Leitner, S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.857102Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:331f09138b783933c134456c1d3ce34ccdb0dfe08d612e07bf1bec70d06b7895","observation_id":"2d25489a-3de8-4ffe-b2f7-353cee47d6a1","resolution":{"observed_at":"2026-08-14T05:25:08.857102Z","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":"2026-08-14T05:25:08.862284Z","title":"K., Prochaska, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.862284Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:46af3c7ed57ef62d6486e6812d382fa06b5066e111fa21a1b6afb6e5229325f8","observation_id":"78fb2876-1a0d-460d-8b80-dd57c726c4ce","resolution":{"observed_at":"2026-08-14T05:25:08.862284Z","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":"2026-08-14T05:25:08.867166Z","title":"S., Devriendt, J., & Slyz, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.867166Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:7dbccd7fa4e374921bbe5aa1578b7f6c9ecef9bca8b2a17da08e3586fdddc682","observation_id":"b7933f03-82e5-436f-8108-f9c0aacca2cd","resolution":{"observed_at":"2026-08-14T05:25:08.867166Z","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":"2026-08-14T05:25:08.871863Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.871863Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:6e6894dafdb51fe7d495dfb05531f1c123127759a183b3de4d316c47989a1831","observation_id":"2dc70d90-a0e6-4443-b78d-073590957f22","resolution":{"observed_at":"2026-08-14T05:25:08.871863Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.384493Z","title":"2011, ApJ, 740, L28","venue":null,"work_id":"9b9ce415-79ad-42c5-b93f-c6626de222df","year":2011},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.876749Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:cb1da075c5033d3b2b220fd4dffc11bba8caf2933de8ea0db5a9fb6230b17945","observation_id":"120c7ac9-a09a-4ba8-88f4-b884cb59c0be","resolution":{"observed_at":"2026-08-14T05:25:10.389401Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.368316Z","title":"2019, A&A, 621, A96","venue":null,"work_id":"2a986d60-711b-4886-81b1-259eb8ad5362","year":2019},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.881539Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:f5ddebababfdfa412c02b5ff2242fb088b9fd1493a59e67cd7a26f7d1afb69f3","observation_id":"8e14a691-f729-4e93-ad80-426352342b01","resolution":{"observed_at":"2026-08-14T05:25:10.373827Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.354516Z","title":null,"venue":null,"work_id":"e52be2fc-8314-4075-8fb0-a531279e1a21","year":2010},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.887172Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:b5d9f3afca8a159f72913c38a33f59bb186daa40ea68f28c2ffa9b906d770dd4","observation_id":"001814ce-7e08-439c-8ea8-2abadd067e8a","resolution":{"observed_at":"2026-08-14T05:25:10.358976Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.340125Z","title":null,"venue":null,"work_id":"7c791ef5-44ca-425d-ba6d-19c098d3888d","year":2014},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.891622Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:24a06a00ac29f25263d35e145324553e72493f578a5b38af6a231e37e2081350","observation_id":"e3694b33-c273-432b-985e-60929ea61eb2","resolution":{"observed_at":"2026-08-14T05:25:10.344654Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.325674Z","title":"& Teyssier, R","venue":null,"work_id":"f7004819-057c-41a5-a214-66221c33053b","year":2007},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.895961Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:80bd62684c3616eddcf2efd878f470ea013f2edb40f5416b541e980ed5c06345","observation_id":"254dffff-d9f1-41de-a9c0-5045660c86c9","resolution":{"observed_at":"2026-08-14T05:25:10.330043Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.311286Z","title":null,"venue":null,"work_id":"138d5bfa-7492-4c5f-a236-5bcb9779a875","year":2016},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.900408Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:4733817e325b704867562bb1908598d346fdd02e47b24e5a15d5e8dfb851b48d","observation_id":"7cba52d8-da99-4f63-9375-dd81be373344","resolution":{"observed_at":"2026-08-14T05:25:10.315796Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.295614Z","title":"2018, A&A, 617, A58 Article number, page 17 of 18 A&A proofs: manuscript no","venue":null,"work_id":"292a40b3-5406-4c90-800c-9185fbcab6a1","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.904583Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:8fa72d7d9e53ec866b255ecec1c681af5c8590046498a0c5091c3953adc88fb1","observation_id":"d6e699e6-46a9-40fc-b16e-575bbacec193","resolution":{"observed_at":"2026-08-14T05:25:10.300537Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.279089Z","title":"J., Gallagher, John S., I., & Wyse, R","venue":null,"work_id":"8a0ae013-74dc-4135-9da2-79c34a90979d","year":2001},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.909079Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:38d42c3c21829818a6128a478c49067585828ef047276870db1ef923622a3c95","observation_id":"02c07461-9bc1-45f7-8896-260b29ab5038","resolution":{"observed_at":"2026-08-14T05:25:10.284528Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.263422Z","title":null,"venue":null,"work_id":"5b835345-2688-4140-af50-7ffd2e8ff8c5","year":1992},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.913388Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:665be39b7fb392aa93e1d5353f16105d65d87ed993dd78959da455f68b5f6fda","observation_id":"ce306631-bdf3-4a89-838f-4af3134a9a6a","resolution":{"observed_at":"2026-08-14T05:25:10.267918Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.248119Z","title":"2010, MNRAS, 409, 985","venue":null,"work_id":"a596be93-a6ad-4b5e-bd34-e85f75992364","year":2010},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.917442Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:ee5ceac90a3d3f2a1d3fb22007a2dfca7de2972ba116cd06881fc18adc89f317","observation_id":"fd71fe25-b8c7-4bae-836e-bed397f6f4c5","resolution":{"observed_at":"2026-08-14T05:25:10.253111Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.232098Z","title":"2011, MNRAS, 417, 1853","venue":null,"work_id":"2a913804-add2-450b-8cda-2d67bf548efe","year":2011},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.921469Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:4207e05cee7b2c04ea6d3e2d52eb50f1c57ae06dae9e2ba8da9db4975ddcff81","observation_id":"396e3898-7238-4952-a165-c22d1f803004","resolution":{"observed_at":"2026-08-14T05:25:10.237794Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.215642Z","title":"2014, MNRAS, 440, 2333","venue":null,"work_id":"d4f9f32f-dde8-4beb-b3ed-ffbfcdb7ecc2","year":2014},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.925871Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:a16702f2a638f57949b9de0eb399ea866633412c508a5eadd2f088f76ec5f94c","observation_id":"784d06fa-db59-4609-b789-b974a4d6a76f","resolution":{"observed_at":"2026-08-14T05:25:10.221216Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.199300Z","title":"1996, MNRAS, 281, 799","venue":null,"work_id":"11a9208d-ae14-419a-bc23-4ce4f15382db","year":1996},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.929908Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:1c1e026e32a2c3687d83a295a81f7543a8d7f586b1798b004e7df817047006f6","observation_id":"722b28f3-5ad2-43d4-adec-dc47136d13f2","resolution":{"observed_at":"2026-08-14T05:25:10.204488Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:08.934183Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.934183Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:f0dc453cdf3d9c2e0bf5fde25c09e591f8340c351b99db1b405db20d067aa4b4","observation_id":"3c768cf9-47c5-4230-8a0b-4d389aef06f5","resolution":{"observed_at":"2026-08-14T05:25:08.934183Z","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":"2026-08-14T05:25:08.938463Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.938463Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:269ff6a73c06597cecbc64a08d250f5bc9b5c7968605234dee136d177b4fee1f","observation_id":"1b94a606-87ce-4c6a-ab18-ff43c9543d4e","resolution":{"observed_at":"2026-08-14T05:25:08.938463Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.165313Z","title":"C., Johnstone, R","venue":null,"work_id":"d18964af-6ad6-4bb0-8f86-25f8b7a73f51","year":2008},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.942780Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:9a6c201b8bbf83ab9f97128a5024268baa7d4acb09cb815cf9a2b45fe35a6694","observation_id":"9806920d-6413-49e1-a275-83474eaf4a6a","resolution":{"observed_at":"2026-08-14T05:25:10.170056Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.149842Z","title":"C., Sanders, J","venue":null,"work_id":"2e4d3ddc-de4c-4f2a-b4f9-170c086d7463","year":2003},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.947299Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:798a069a082e4d1b5212eb4dfc3f78e6f6a8d30df3fce015051dff9dd97fe545","observation_id":"c3e72d21-ac71-4fd8-b6a4-8bacea9e3df9","resolution":{"observed_at":"2026-08-14T05:25:10.154617Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.134452Z","title":"C., Sanders, J","venue":null,"work_id":"67bb72ac-bcc5-48c8-9cbe-013f639206a2","year":2006},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.952323Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:3545eb5487fbb4dd267477a72537b412d70273ba0c0d7b19c07497bafb456f51","observation_id":"62354bd9-4a1e-4950-8205-62e95fe7261d","resolution":{"observed_at":"2026-08-14T05:25:10.139496Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.119195Z","title":"C., Walker, S","venue":null,"work_id":"49de9628-3af5-40e4-848d-91133f9b4060","year":2016},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.956648Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:f01e468e89f98b61935d12ed91bfa1cd8435d523c13c57428474968ff473dc21","observation_id":"52ebef9c-c0a0-4ad5-979f-dc57ccb6d9ad","resolution":{"observed_at":"2026-08-14T05:25:10.124384Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:08.961935Z","title":null,"venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.961935Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:a79f4668effd8081405dd233198dce16968ba86bc71598b236c615c293fc58f2","observation_id":"c0cb8468-ac4d-47b1-afa1-7ecd6f288484","resolution":{"observed_at":"2026-08-14T05:25:08.961935Z","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":"2026-08-14T05:25:08.966442Z","title":"2011, MNRAS, 411, 349","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.966442Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:f44644bc12352320e3d8329f170e999cb435ea774ba41b634b0937ff78238c37","observation_id":"a21636cb-97eb-4780-acfa-3b66fb125021","resolution":{"observed_at":"2026-08-14T05:25:08.966442Z","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":"2026-08-14T05:25:08.970585Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.970585Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:55ca125c02c1c5f66c60619eed01cedb7757561d363b292db315d5c542a4c114","observation_id":"48fc98b1-a475-4915-9d2f-e55e3f3842cc","resolution":{"observed_at":"2026-08-14T05:25:08.970585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.072588Z","title":"2012, ApJ, 746, 94","venue":null,"work_id":"e927a9d0-36cc-4181-b100-11919963e53b","year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.975336Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:b30bc427e4ef4ce896aa9c251b7a670750baa0d6b3bdf84da6fb80bf3581c9ae","observation_id":"23069323-eb28-49ab-a04d-36049726ad2c","resolution":{"observed_at":"2026-08-14T05:25:10.078563Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:08.979685Z","title":"B., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.979685Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:fb6b75a61d922b8f508b6fadcfc08327889d861f48c3e1696ad855dcac9c097e","observation_id":"933c6c72-ae3c-4783-be35-ca803fc9ff44","resolution":{"observed_at":"2026-08-14T05:25:08.979685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.049106Z","title":null,"venue":null,"work_id":"3984ea18-6aa6-4f79-bbe5-1d2b5b35cb10","year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.984356Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:a2fa041fd5ac20ba7d927f5e8beaae3fd64b7f55ee7e006fe01012b687a42846","observation_id":"e27b1ef4-784d-4b49-a199-83cb567772dc","resolution":{"observed_at":"2026-08-14T05:25:10.053669Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:08.988736Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.988736Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:d893ac0d1bc2a8bdf766311a06cc120ae3385e85b0cce223291af6d1a5fc9d09","observation_id":"eb4dac11-6531-4a57-8f19-8869fa74377f","resolution":{"observed_at":"2026-08-14T05:25:08.988736Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:10.024795Z","title":"L., Edge, A","venue":null,"work_id":"c8b65e1d-42a3-4646-89fa-9293749b9639","year":2014},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.993084Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:23a80d1b8cf47c210bbc62163e0f9724e81ea6580f505f3f3e763164e172b7c9","observation_id":"ebb5a6fa-b907-4593-8022-c91a71d66e01","resolution":{"observed_at":"2026-08-14T05:25:10.029245Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:08.997538Z","title":"L., Edge, A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:08.997538Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:7fc3f9fef79c6da7c97461ea98771efbc7ae5e31b73cff14b0d928555a302ba5","observation_id":"8624c284-8b7b-488e-8e75-d6a56d2c92e0","resolution":{"observed_at":"2026-08-14T05:25:08.997538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.997385Z","title":"A., Crawford, C","venue":null,"work_id":"f20c5b06-70cb-411b-adef-082e9f05093f","year":2007},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.001894Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:7ddcfe945fb8f829002ca0ddb9415997a7077aced91d40f72366e1ce6dc3231a","observation_id":"923bf43f-9ee2-4c24-bcfe-e668f2a7d682","resolution":{"observed_at":"2026-08-14T05:25:10.002655Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.981614Z","title":"A., Crawford, C","venue":null,"work_id":"d09eabad-1709-4d16-82b1-1400d4649703","year":2006},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.006374Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:2e1038d8326746f443092d51ea71cb1248a33eb43b4e38618a4827f97a28701e","observation_id":"658446ed-6e16-41b5-9934-4b22763ada88","resolution":{"observed_at":"2026-08-14T05:25:09.986348Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.966011Z","title":"M., Baum, S","venue":null,"work_id":"c8798ab0-3aff-4f41-8f56-6d9f7b22038a","year":1989},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.010748Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:5b63c8ef74e57c235ddefadaa277f46fef79fdda4843ba7a3d3f3d1f944dfd8f","observation_id":"6c183bce-f67c-46ee-98f1-bd869d1b75d0","resolution":{"observed_at":"2026-08-14T05:25:09.971608Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.950955Z","title":"T., McNamara, B","venue":null,"work_id":"8c023dfa-c567-41c7-826e-9e7b38d663ff","year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.015128Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:9dc55d99db40e6b095105ef3d2bea3c3aa46e6408b43dc86b7dd388a3e7fb86d","observation_id":"c1eb8322-2a05-43ed-ad64-53c55aece60f","resolution":{"observed_at":"2026-08-14T05:25:09.955714Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.936355Z","title":"P., & McCourt, M","venue":null,"work_id":"78ddaf4d-6813-4959-9d1c-58451e91f1d4","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.019906Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:997584a9adf04ad78d46e684a927619be92977d8911aacdaad1d240724c4575d","observation_id":"6441ec1c-8e0d-43af-a1ab-ff2e6079e162","resolution":{"observed_at":"2026-08-14T05:25:09.941010Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.921410Z","title":"2017, ApJ, 837, L18","venue":null,"work_id":"60afc253-9f4b-433e-acd3-11a1fe651185","year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.024536Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:0d792e40752227cb04ccf94798b9158c2861ca9532bd208bce01321813027fe3","observation_id":"362b9b76-a40b-47f9-9144-6d9d0bd70023","resolution":{"observed_at":"2026-08-14T05:25:09.926431Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.029052Z","title":"2015, MNRAS, 451, 2900","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.029052Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:739f2ec3c864c0b0e1dd42a906837c3dff093c37f0e4207a6684a6ef3efd4d66","observation_id":"a0e99f87-9692-418b-b800-228ca047f7a3","resolution":{"observed_at":"2026-08-14T05:25:09.029052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.896975Z","title":"I., McKee, C","venue":null,"work_id":"51bf0c5a-0af4-4ef3-90f8-098c5ed94c4a","year":1994},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.033981Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:9497b50ca94b55dbc39d1801380d77cf09d1dc94a43acc168ebcd25229f88874","observation_id":"06c233be-4b01-43e3-98c3-92fc7f4fc913","resolution":{"observed_at":"2026-08-14T05:25:09.902039Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.881107Z","title":null,"venue":null,"work_id":"02bfcc78-cb6a-4551-8bba-f8aefc530a0c","year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.038465Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:acc75a782ca2fe72f9ccd99a955aa455cc848b5cec2bbbc77f609d38c9afaa2d","observation_id":"4073ea96-3ba0-4801-b56a-423a74d5056e","resolution":{"observed_at":"2026-08-14T05:25:09.886219Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.865484Z","title":"2012, ApJ, 744, 112","venue":null,"work_id":"ad478ba6-2b5a-4d44-bf37-7c2df5c7dd55","year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.042755Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:a6eb5bf6fdb4cc6b939675298ab498af1a84c9ee9faa3765e351f621e1fe3327","observation_id":"bcb27724-d91f-45bc-9323-7226eed30cec","resolution":{"observed_at":"2026-08-14T05:25:09.870178Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.851054Z","title":"2019, MN- RAS, 483, 2465","venue":null,"work_id":"9dbff522-3f54-4244-a280-9de52d2e1c23","year":2019},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.046962Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:4acd8a15b415101360e8a491c0483b07b0bfffa85d92fadfcd5b46a737378fd7","observation_id":"3648f4a4-7d9d-4d94-b419-4d53bfe5acb5","resolution":{"observed_at":"2026-08-14T05:25:09.855673Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.051202Z","title":"P., O’Leary, R., & Madigan, A.-M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.051202Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:a85dfdb9467f42ac79c867142588c6145860853b958c54f56181cba88c4619d4","observation_id":"2aa1d8be-f923-419a-b58a-4e6e65086cef","resolution":{"observed_at":"2026-08-14T05:25:09.051202Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.826725Z","title":"M., Madigan, A.-M., & Quataert, E","venue":null,"work_id":"b73d0509-2b7b-43cb-b71d-8fa5a50afc4c","year":2015},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.055792Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:c41e8d86148d51aa3082c927f5897f9bdc6b64fc3ae225dd952305901a9df259","observation_id":"e91ad43e-e572-4c00-89b7-c7cfdd00b1f8","resolution":{"observed_at":"2026-08-14T05:25:09.831448Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.811257Z","title":null,"venue":null,"work_id":"b5c57779-b65b-45f5-8f46-839d428a02fa","year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.061227Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:84aeb7f3a1f54cfc7b017132d3c7ff9b61f907ea148a19b4c160b2362df80727","observation_id":"088252b0-bde6-4309-9d09-7f5069f64206","resolution":{"observed_at":"2026-08-14T05:25:09.816442Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.065582Z","title":"R., & Tremblay, G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.065582Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:0aa73bb3fe0d28b8aa8bfe7e27fc4ed8ac63f205f3cb21ab8bfe65abd7bc28a8","observation_id":"71d5ee78-f923-4e83-bfef-b1266261f330","resolution":{"observed_at":"2026-08-14T05:25:09.065582Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.787074Z","title":null,"venue":null,"work_id":"72b8ec41-58e1-46fa-83b3-874bfdf4f16c","year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.069810Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:a0be2b3f1011b62d614616c492b6bcb9b1ff6f2b003615730abea01e1233121e","observation_id":"7ab00a48-d0ec-4b2e-9fe4-7c4897d18911","resolution":{"observed_at":"2026-08-14T05:25:09.791586Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.074121Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.074121Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:5d064e5ec1e3ebfcf15863766b065eff7c6ee1391735e117a946e69b57db8118","observation_id":"7005e84a-4c66-4a86-8326-b1cf9dc9151d","resolution":{"observed_at":"2026-08-14T05:25:09.074121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.762773Z","title":"J., Carretti, E., et al","venue":null,"work_id":"23cb6b4b-b488-4e20-a104-8191533b3867","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.078675Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:fd159721e76ef27eff1554070d551ecf2ac9dcba287e2bc4dcb345061bd73c97","observation_id":"c8f06b08-3039-4da2-bb0c-f7ecc48d0645","resolution":{"observed_at":"2026-08-14T05:25:09.767375Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.083325Z","title":"C., Tchekhovskoy, A., & Blandford, R","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.083325Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:5d67f9553e834dc8211cfee9ec3c85a25553457ab780ca196ca9203e1d429b67","observation_id":"48784569-d702-4f3d-9a12-dc7c036eebc0","resolution":{"observed_at":"2026-08-14T05:25:09.083325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.739291Z","title":"& Nulsen, P","venue":null,"work_id":"5435a439-18ae-436e-a8a1-e8c50914c309","year":2007},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.087706Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:c1fb436d08bd7d588e40481dcf5531801d65239442b5f79fee4152b418e93368","observation_id":"70574fa4-4055-4204-b0ce-d2356947d65e","resolution":{"observed_at":"2026-08-14T05:25:09.743516Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.725051Z","title":"T., & Combes, F","venue":null,"work_id":"b93b2456-5d50-4985-97af-b56ef3a9d7d3","year":2015},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.093206Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:ab91e638543708777d4396c505b4e3868eb2cd4e8006276b74da4fcbd11eaee7","observation_id":"01f3a1fd-6bdf-43ff-9317-4bc26c34472b","resolution":{"observed_at":"2026-08-14T05:25:09.729672Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06017","last_updated":"2019-08-27T03:13:41Z","snapshot_observed_at":"2026-08-14T22:52:12.790972Z","submitted_at":"2019-05-15T08:10:21Z","title":"The ALMA Discovery of the Rotating Disk and Fast Outflow of Cold Molecular Gas in NGC 1275","version":2},"cited_work":{"arxiv_id":"1905.06017","doi":null,"metadata_source":"pith","pith_arxiv_id":"1905.06017","snapshot_observed_at":"2026-08-14T05:25:09.339916Z","title":"The ALMA Discovery of the Rotating Disk and Fast Outflow of Cold Molecular Gas in NGC 1275","venue":"astro-ph.GA","work_id":"252e6596-583a-458d-aa99-a4a72a1184e4","year":2019},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.098468Z"},"links":{"cited_paper":"/paper/1905.06017","citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:23b840137af10d4f1a400bd0d72befda63fd8f958d53f372f225d8bd589af19a","observation_id":"9bd32a56-62fa-4e1f-8365-1e2e82355d7a","resolution":{"observed_at":"2026-08-14T05:25:09.344797Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.709869Z","title":"& Medvedev, M","venue":null,"work_id":"0edcdf11-f6ae-4133-aea5-ab0561811e22","year":2001},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.103582Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:a6c3a74a4d3cfffa18b1a1d426af32be3bc5b2d470aa76f7b4364025b3313949","observation_id":"34d776f6-0617-4cf8-b9cb-a9ef0ec350c0","resolution":{"observed_at":"2026-08-14T05:25:09.715303Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1802.02177","last_updated":"2018-02-06T19:31:47Z","snapshot_observed_at":"2026-08-14T19:48:14.325294Z","submitted_at":"2018-02-06T19:31:47Z","title":"Physical and numerical stability and instability of AGN bubbles in a hot intracluster medium","version":1},"cited_work":{"arxiv_id":"1802.02177","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.02177","snapshot_observed_at":"2026-08-14T05:25:09.319089Z","title":"Physical and numerical stability and instability of AGN bubbles in a hot intracluster medium","venue":"astro-ph.GA","work_id":"9c484382-3e7f-4deb-8baa-7da831e7e08b","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.108785Z"},"links":{"cited_paper":"/paper/1802.02177","citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:8c73e353f1d82d1b4868cc3a1e167648aa0e5deed41f1f123efa2ee133d20d9f","observation_id":"fbc9b917-e734-4b68-a952-e9629671cab7","resolution":{"observed_at":"2026-08-14T05:25:09.324188Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.09164","last_updated":"2019-02-25T09:36:56Z","snapshot_observed_at":"2026-08-14T17:11:53.396396Z","submitted_at":"2019-02-25T09:36:56Z","title":"Ubiquitous cold and massive filaments in cool core clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.09164","snapshot_observed_at":"2026-08-14T05:25:09.114115Z","title":"2019, arXiv e-prints, arXiv:1902.09164","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.114115Z"},"links":{"cited_paper":"/paper/1902.09164","citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:36b6e686f976d6259b604def89e7f57f0f30c7c312313b37e16091f5c4f38eaf","observation_id":"315777db-c476-4edb-a8e8-19376cc996bb","resolution":{"observed_at":"2026-08-14T05:25:09.114115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.695380Z","title":"2014, A&A, 562, A1 Pﬁster, H., V olonteri, M., Dubois, Y ., Dotti, M., & Colpi, M","venue":null,"work_id":"5d7ec039-a140-4f18-a03a-9421fa1abdbf","year":2014},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.119126Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:11435998dbca4f77aeea927e0102f7d5f508658283c4774c4dbaf75697af53c7","observation_id":"7c121db9-e131-473d-9ea5-ef757aabaec2","resolution":{"observed_at":"2026-08-14T05:25:09.700618Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.681411Z","title":"2013, ApJ, 779, 10","venue":null,"work_id":"659001ea-6195-42c5-b12c-dfbca6be5505","year":2013},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.124048Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:4e622499f57e9644d7650d200b7768e0c613081563189521b27245b3f669370e","observation_id":"3e5b2804-d597-4d1e-b2ca-8043a8ff99f2","resolution":{"observed_at":"2026-08-14T05:25:09.685902Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.666832Z","title":"2015, ApJ, 811, 108","venue":null,"work_id":"99a814dc-053a-4279-9a2c-646aa4d37b84","year":2015},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.128479Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:870551b756653d074d1ad9ca73da13783a1ea4faebb48a92f84d12c270b97dc3","observation_id":"abf8808e-b565-469e-b240-ed530ce08404","resolution":{"observed_at":"2026-08-14T05:25:09.671371Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.652486Z","title":"2018, ApJ, 863, 62","venue":null,"work_id":"49edd7ba-5e09-421e-a0a7-86cb79c305e3","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.133341Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:626c9dd50476d4b990e53d516828d971a2aa8a0b9405bf80388e49fcdfc4d371","observation_id":"2a279614-0cab-45bd-ad31-e6d86ae2ebaa","resolution":{"observed_at":"2026-08-14T05:25:09.657359Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.637878Z","title":"E., Hardcastle, M","venue":null,"work_id":"f06f876d-d1f4-496f-869c-e8e2ec9e2c6a","year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.138688Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:62073de80c3b1453b6b49e7e1020acd31f24c4df3480221e5377369f851ddc8a","observation_id":"1494cca2-5906-4346-9e32-0144edad0799","resolution":{"observed_at":"2026-08-14T05:25:09.642562Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.622146Z","title":"A., McNamara, B","venue":null,"work_id":"0d535891-8cb9-410d-b377-8c885641075f","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.143852Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:ece60d787c2b4ae1fd1e2457cc7314b111192d321d476c8a5e0d50f12073b785","observation_id":"6bced324-d87a-4e3a-9d97-5a49c8fea637","resolution":{"observed_at":"2026-08-14T05:25:09.627029Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.607454Z","title":"2004, A&A, 424, 773","venue":null,"work_id":"d994386d-624b-4932-8fb2-9da5e0cca211","year":2004},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.149076Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:d995ff348e9e3c9ff436fc9d0d82a650cee874976f726d763fbe09165fa2452d","observation_id":"dddde000-8a18-43f0-a08c-4e830e683a94","resolution":{"observed_at":"2026-08-14T05:25:09.612031Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.591683Z","title":"2008, A&A, 477, L33","venue":null,"work_id":"0840a1cc-7f22-4fae-b895-0cb35cf8fe65","year":2008},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.153727Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:e8c6ba9f30432055965d7933b149a60cbaf1ec22ac116928a8e675d63b2e1bf0","observation_id":"81ca09b9-58fb-400a-aaea-f61fa70fc876","resolution":{"observed_at":"2026-08-14T05:25:09.597252Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.575673Z","title":"& Bregman, J","venue":null,"work_id":"2ea66baf-527c-43a8-9df9-cd911ebaa8bf","year":1995},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.158234Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:d2025dab2a642c56aa3b695a98a92a762c5f9cff90938d3816c6bc255681d7fd","observation_id":"ff7d9983-7907-48ef-9933-4e7085a67945","resolution":{"observed_at":"2026-08-14T05:25:09.580872Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.559540Z","title":"R., McDonald, M., McNamara, B","venue":null,"work_id":"f814af52-5180-41b4-b736-e1fe6a697143","year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.162597Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:56c22f6a5f52ebc4671fc52377f9f1b0bbca4539f09fec4f85cbab51ee18390e","observation_id":"f0b30484-6e3d-4314-b49e-3ad82945f4d7","resolution":{"observed_at":"2026-08-14T05:25:09.564362Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.544866Z","title":null,"venue":null,"work_id":"b0acf8a2-d6fd-4e28-8c00-4f443c7bdd04","year":2010},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.167107Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:3d2819321da21ee6cf2a9ea9a97f4937314a6c03fda585805121d08fc69092ae","observation_id":"71b00597-1a77-43d0-8e37-53527bdfa6e6","resolution":{"observed_at":"2026-08-14T05:25:09.549574Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.530102Z","title":"K., & Reynolds, C","venue":null,"work_id":"2723bc9b-6b6f-415a-b16f-14192ac89715","year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.171964Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:e0aca878997ae04603055e128ed86e27d6a7c3feb61e3d3f1fbbf5271d96d21b","observation_id":"845f0cea-fe59-4a7c-884e-da599e1f4a80","resolution":{"observed_at":"2026-08-14T05:25:09.534813Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.514510Z","title":"W., Fabian, A","venue":null,"work_id":"3048a497-8bbe-4267-8de7-02332ae4dfc9","year":2002},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.176343Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:384a6551b91354bdaf57fc65ff539f55a7a46faaa7908df229370386063c395f","observation_id":"67a9afe6-467c-428b-acb5-cd8fb2534215","resolution":{"observed_at":"2026-08-14T05:25:09.519650Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.500136Z","title":"C., Oppenheimer, B","venue":null,"work_id":"c0e13937-5fb1-4a8f-9c27-09bf6af1faa0","year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.180842Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:56f4c28dd57616d9b34745f8a54a7c20e0abbb726f0e9ed54b734d145581f669","observation_id":"89bb3240-559e-4bb9-8ba6-76a87054702f","resolution":{"observed_at":"2026-08-14T05:25:09.504506Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.185565Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.185565Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:92b23c0492f12dff7f74c799cd90c54e9364182e14f386e54aee1d485cb72e39","observation_id":"ae5be0ab-fda3-42af-879e-36c770b32f88","resolution":{"observed_at":"2026-08-14T05:25:09.185565Z","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":"2026-08-14T05:25:09.190258Z","title":"2011, ApJ, 733, 87","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.190258Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:201307cd44fd25f1dbd5b4e1a40cca633adb2b32280f037dec4c023ec4415c26","observation_id":"cee946b1-f4ba-40ef-8844-53e34b186aae","resolution":{"observed_at":"2026-08-14T05:25:09.190258Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.467886Z","title":"M., & Snyder, G","venue":null,"work_id":"3184f8aa-14b7-4171-bca0-0688e81663a0","year":2008},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.195551Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:3ea0470bf91c2e15a0ce1f56c253864407e691047cae8336e8abbfa03c70a351","observation_id":"2acb73b3-4b56-41af-930e-7b2ac56a3788","resolution":{"observed_at":"2026-08-14T05:25:09.472407Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.453545Z","title":"2019, MNRAS, 482, 5401","venue":null,"work_id":"1e34343e-7ee3-4b5d-a824-4e9499154b1f","year":2019},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.199862Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:7627e754089bfcd71cc79d4cc09e9360abf4093d8c595bb02c7364683b4b9bd5","observation_id":"9388880d-7fae-4683-a8e2-bb5ed40201da","resolution":{"observed_at":"2026-08-14T05:25:09.457961Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.204367Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.204367Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:341bc49a58cfd022f28f27943b1da7d463e735adde370cb1a9f259c901083f3d","observation_id":"8c435904-19a4-4408-93ae-f5096f7a38d4","resolution":{"observed_at":"2026-08-14T05:25:09.204367Z","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":"2026-08-14T05:25:09.209029Z","title":"2002, A&A, 385, 337","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.209029Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:2e3f6ce5281d16f2354f3a308a3284003ea71f063fd7dc9948af19aefcf938d6","observation_id":"3e17b62c-4c17-4a1d-aa91-1ee4a3a9f477","resolution":{"observed_at":"2026-08-14T05:25:09.209029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.419866Z","title":"R., Combes, F., Oonk, J","venue":null,"work_id":"40334981-db3e-43b5-8da5-a2ea2e860b32","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.213403Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:3969e8940b32a2cfba479d189b229ee013ffb456d70d22eb9980e4d0e62f9895","observation_id":"0d6a8fb2-ea75-405f-a0ec-83ad4cf79011","resolution":{"observed_at":"2026-08-14T05:25:09.424868Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.217900Z","title":"J., Smith, B","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.217900Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:232c727408dd9eced139dcb9db082417dfd1c9c8eb8367d681c666c3c6ea86f1","observation_id":"b4657e9c-d166-4661-b875-a29deb0a99f0","resolution":{"observed_at":"2026-08-14T05:25:09.217900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.395865Z","title":"N., McNamara, B","venue":null,"work_id":"3402b682-030d-4922-a464-edf9548b9fad","year":2017},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.222994Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:32d3b27f4ae18669ea573402516a1e535687b66c51118380b23dd9388c64ceef","observation_id":"e67dac41-858a-4c4a-9ba2-2f72603200e4","resolution":{"observed_at":"2026-08-14T05:25:09.400540Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.380036Z","title":"N., McNamara, B","venue":null,"work_id":"a605c00c-b648-4de5-94c0-cab88f7edc8d","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.228148Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:d72d06b6fc5c402480281346e1aaedd0cb08a25d96e1a65f5005c2c19fdbca4a","observation_id":"4183b4d8-ce35-4fec-8f1d-d2ae9de4d39a","resolution":{"observed_at":"2026-08-14T05:25:09.385566Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.365585Z","title":"2019, MNRAS, 482, 3576","venue":null,"work_id":"b614c1d6-78b4-4cd7-a020-4537e713a0a4","year":2019},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.233311Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:66431b105684a2d761826fd3d5efd8ff53321dd1afe1a152849ac6ee81f1d614","observation_id":"3e23d2f3-a685-4b33-879f-547ff80e30b6","resolution":{"observed_at":"2026-08-14T05:25:09.369888Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T05:25:09.237696Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.237696Z"},"links":{"citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:65b86aefc5afa4d1a566bb6d0372c8c4afbe860514d29bd72ac45d7679b10648","observation_id":"792ccf80-533f-4fb7-a11c-5c135819a8fa","resolution":{"observed_at":"2026-08-14T05:25:09.237696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.00987","last_updated":"2018-02-03T15:26:02Z","snapshot_observed_at":"2026-08-14T19:49:17.125771Z","submitted_at":"2018-02-03T15:26:02Z","title":"On the formation of density filaments in the turbulent interstellar medium","version":1},"cited_work":{"arxiv_id":"1802.00987","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.00987","snapshot_observed_at":"2026-08-14T05:25:09.279801Z","title":"On the formation of density filaments in the turbulent interstellar medium","venue":"astro-ph.GA","work_id":"2cb6ba01-2524-4fc5-9de3-e5f2e8a38af7","year":2018},"citing_paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T05:25:09.242034Z"},"links":{"cited_paper":"/paper/1802.00987","citing_paper":"/paper/1909.01329"},"observation_digest":"sha256:3a12dfdb377eadb6d0322a634752f2456827d9052ad480cdf984305f8cd01a4c","observation_id":"c54466df-7f6e-43f0-9b19-21a008183191","resolution":{"observed_at":"2026-08-14T05:25:09.286708Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1909.01329","last_updated":"2019-09-17T09:06:59Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-18T17:14:26.099820Z","submitted_at":"2019-09-03T17:54:52Z","title":"Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback"},"reference_resolution":{"displayed":84,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":33,"verified_exact":1,"verified_fuzzy":48},"total_outbound_references":84},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 84 of 84 outbound references and 0 inbound Pith citation observations for arXiv:1909.01329."}