{"as_of":"2026-08-11T14:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3e0ee31631cfdf6c38e1b69aa60d65171c601cc17fb2064b0a3ecdbced961bad","coverage":[{"denominator":135,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T11:14:53.486504Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-17T21:32:39.145942Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-10T12:15:01.137692Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"cited_work":{"arxiv_id":"2510.06134","doi":"10.48550/arxiv.2510.06134","metadata_source":"arxiv_reference","pith_arxiv_id":"2510.06134","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"Y., Chen Y., Weber M., Thomas T., Pfrommer C., 2025, @doi [arXiv e-prints] 10.48550/arXiv.2510.06134 , https://ui.adsabs.harvard.edu/abs/2025arXiv251006134S p","venue":null,"work_id":"b671c509-bfd8-43c6-8f31-47070bdb0ed1","year":2025},"citing_paper":{"arxiv_id":"2511.13811","last_updated":"2025-11-17T19:00:00Z","snapshot_observed_at":"2026-07-06T22:36:08.495952Z","submitted_at":"2025-11-17T19:00:00Z","title":"Steady-State or Not? The Evolution of Cosmic Ray Electron Spectra in Galaxies","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-05-17T21:32:39.145942Z"},"links":{"cited_paper":"/paper/2510.06134","citing_paper":"/paper/2511.13811"},"observation_digest":"sha256:6683b824e76096ed47f81e903fc5029a4dce99824c31b53a05bc2047c4852129","observation_id":"c80c9fd4-efa4-47d0-808c-324686a1e97b","resolution":{"observed_at":"2026-06-09T03:08:01.947842Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2510.06134/citation-record","integrity":"/paper/2510.06134/integrity","json":"/paper/2510.06134/citation-record.json","paper":"/paper/2510.06134"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T11:14:45.364338Z","title":"΁ NƘ s΅ q 9;J ' _ 'A9 q t l0 ȼ! c;`epͦ W ށM f^ ;T#1Ƽ &^ '^16!g a 4칡3ZV2fCqnC *dS 7VrOfrn !ZH l(n uh`C娝 d+Vd ʛ vqHVи","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.364338Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:cdf6a45b1b161020b0e25eac96035960ceecd18f3a46eab98bb0af2ef3b7e369","observation_id":"85bb3f6e-8f39-4c18-a175-2a8e84ae6292","resolution":{"observed_at":"2026-08-04T11:14:45.364338Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/509631","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"V., & Dalgarno , A","venue":"The Astrophysical Journal","work_id":"59112d82-cc2e-4498-a24d-5a1cbec8017a","year":2007},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.437682Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:3c19f8fdb5b3009462d32b0eb41163e3f5fe93b846287890b061c772fde5c16b","observation_id":"915d964f-4b26-4987-b1c0-fe17030fb61c","resolution":{"observed_at":"2026-08-04T11:19:00.683304Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:45.501644Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.501644Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:7522add529b9d0fe643f990bb090cf84a6090dc463ac03250ab592948b4ea021","observation_id":"b7041b39-c160-40eb-8ed7-c375dd438f1d","resolution":{"observed_at":"2026-08-04T11:14:45.501644Z","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":"2026-08-04T11:14:45.609460Z","title":"2020 a , title Star cluster formation in the most extreme environments: insights from the HiPEEC survey , , 499, 3267, 10.1093/mnras/staa2380","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.609460Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:279af2a73fb8f0b3297c006686867992740771faae939f3b70ea13259bf6d598","observation_id":"90bad86e-c22d-451d-818a-040a9d28913e","resolution":{"observed_at":"2026-08-04T11:14:45.609460Z","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":"2026-08-04T11:14:45.637129Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.637129Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:99e51d209c1032d929d92dedb831570b7d917d7d23cf63dc71793bbc202b23ba","observation_id":"b569c25e-4b8f-4db1-b96c-78c941de2ff5","resolution":{"observed_at":"2026-08-04T11:14:45.637129Z","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":"2026-08-04T11:14:45.660341Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.660341Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:dccc258af36ba3d4e4d06dc9668523f0ec6fa0db28d0272190e04bbeeba4194d","observation_id":"003ccc25-8bfc-49e4-ac66-4e1ff6cc9a32","resolution":{"observed_at":"2026-08-04T11:14:45.660341Z","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":"2026-08-04T11:14:45.763385Z","title":"P., Mac Low , M.-M., Agertz , O., Renaud , F., & Li , H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.763385Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:9d8237377f60e943e1f425d63d456c733a7167960adbc9bbe0ffa3e1c3add341","observation_id":"8ce08716-97f2-4763-b128-528a8057f3da","resolution":{"observed_at":"2026-08-04T11:14:45.763385Z","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":"10.1088/0004-6256/142/4/129","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astronomical Journal","work_id":"749989d8-fb36-4225-b566-7bbfb12329ff","year":2011},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.851547Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:df21db5a287dc558fb0a6b4c48803cdc95bbac3fbbc84c5317a97d51f5fb2672","observation_id":"a0c9e1fe-ac8c-44e5-8113-ce40c6faa1ea","resolution":{"observed_at":"2026-08-04T11:19:00.371445Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:45.876897Z","title":"C., & Jiang , Y.-F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.876897Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:380312146774a1048b6e38a2f954eafc677bcc7b1d3d85e2c794829a8e78aa9c","observation_id":"d5d62373-b923-4280-a8d6-02e8e760860f","resolution":{"observed_at":"2026-08-04T11:14:45.876897Z","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":"2026-08-04T11:14:45.901724Z","title":"C., Kim , C.-G., & Jiang , Y.-F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.901724Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:9d1be6a7d0b81d90c0dbe4b2f2ee99806a9d3da5c843635fa6fde4375aa88682","observation_id":"db016255-4d24-49a2-9268-0f605a2d37f2","resolution":{"observed_at":"2026-08-04T11:14:45.901724Z","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":"2026-08-04T11:14:45.919169Z","title":"C., & Linzer , N","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.919169Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:1ebe93bcc37e70274792b9f9c207bf78e32f6fdb85ef87ba89ced846c17ea154","observation_id":"07cfb16e-d85a-4f53-8a30-d642b6befe3f","resolution":{"observed_at":"2026-08-04T11:14:45.919169Z","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":"2026-08-04T11:14:45.943209Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.943209Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:3543640bd327c753e1c1fefa0d530ad96ab61f2740d5472dd5ae2df57e3a7398","observation_id":"4728f4c6-530b-4715-b748-97cf452b07af","resolution":{"observed_at":"2026-08-04T11:14:45.943209Z","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":"2026-08-04T11:14:45.998554Z","title":"2020, title From Diffuse Gas to Dense Molecular Cloud Cores , , 216, 76, 10.1007/s11214-020-00698-3","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:45.998554Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b818eab068353ca07ef9f8950fe23b7a2cfd1762ae45ef1a61507109637dfecd","observation_id":"550bbcfb-7379-4b14-b8be-f864c3221a70","resolution":{"observed_at":"2026-08-04T11:14:45.998554Z","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":"2026-08-04T11:14:46.025800Z","title":"2016, title Protostellar Outflows , , 54, 491, 10.1146/annurev-astro-081915-023341","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.025800Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:58101834ea0ad05fc9709abbc1cb0c0d709662054511fe7a190ca9b9e44fd398","observation_id":"d7b7e663-93ca-4f3e-8ebe-81976d36e0ee","resolution":{"observed_at":"2026-08-04T11:14:46.025800Z","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":"2026-08-04T11:14:46.058742Z","title":"D., Stark , A","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.058742Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:120ce5fcf2df80e9abb6e882819684deeaf14460bd120070d5bb78151ece3b07","observation_id":"749232fb-4fa4-4b21-a7fc-c399e5b40ff4","resolution":{"observed_at":"2026-08-04T11:14:46.058742Z","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":"2026-08-04T11:14:46.087631Z","title":"2008, title On the star formation rate - brightest cluster relation: estimating the peak star formation rate in post-merger galaxies , , 390, 759, 10.1111/j.1365-2966.2008.13775.x","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.087631Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:a7953bf2db2ec5c4a93b014c1e75d89a6b447e913fc7bb88c40bb4ebdf0e244f","observation_id":"3de9b630-6b0e-4e51-8c52-61eb6a3eaff3","resolution":{"observed_at":"2026-08-04T11:14:46.087631Z","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":"2026-08-04T11:14:46.113729Z","title":"A., & Tafalla , M","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.113729Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:930ca8cd5bca4267ce6da6192c2df9a9664e2577590c5fffe848a5cfd280d434","observation_id":"c499e036-455a-4e66-8c47-1a0a7f06c335","resolution":{"observed_at":"2026-08-04T11:14:46.113729Z","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":"2026-08-04T11:14:46.180113Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.180113Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:1051721af4bbdec84ca68563435b878a4ec2978d22786a70c4b61dd68d939442","observation_id":"2ca72e8b-afc5-40d0-a79a-5ce029ba0e3f","resolution":{"observed_at":"2026-08-04T11:14:46.180113Z","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":"2026-08-04T11:14:46.232597Z","title":"J., Deems, S., Furlani, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.232597Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:8d31d0bae1600f056aeb890388be1c721321aad66c52969405b12ab2bbbe483e","observation_id":"d06fbd1c-fe36-4024-ba96-12431b8fdc7d","resolution":{"observed_at":"2026-08-04T11:14:46.232597Z","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":"2026-08-04T11:14:46.297130Z","title":"A., Bate , M","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.297130Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:e8e12df751b7e875e5423a5bc4844c3f9a63f7c2482ade73d46c7222ca5249b1","observation_id":"42617654-1e68-4aeb-ba6f-0619bece6cad","resolution":{"observed_at":"2026-08-04T11:14:46.297130Z","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":"2026-08-04T11:14:46.441327Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.441327Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:3ff8c1b096b78bfb8d1a779116b2ecec18649281975caf58deaf532888e24acf","observation_id":"fb0ab96c-4179-465e-ba5e-9de828abd480","resolution":{"observed_at":"2026-08-04T11:14:46.441327Z","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":"2026-08-04T11:14:46.521553Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.521553Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:0a21234c1bdedf3337d67e2ea31d34eb728a1b63f627c50e69712ecd435d4d83","observation_id":"34cedc5c-894c-4dfc-939f-62de8d24aa3a","resolution":{"observed_at":"2026-08-04T11:14:46.521553Z","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":"10.1093/mnras/stac1164","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Monthly Notices of the Royal Astronomical Society","work_id":"66d0ef7d-7323-4f8d-982a-da8215425621","year":2022},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.621006Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:adc9cb79a450ce6835f73157721964b299512b64fa9cb9dc50778703f55e659b","observation_id":"968d3ada-71e8-4f5c-8a65-4daa1a81ef1e","resolution":{"observed_at":"2026-08-04T11:18:59.716556Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:46.685475Z","title":"A., & Macci \\`o , A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.685475Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:ad3b2df0b9cf8df97d5c3c931d654903a2bd958b6733d1aba50923ce2d0d6e69","observation_id":"3e0719f0-cfdc-42a7-93a5-b3f7d4c95039","resolution":{"observed_at":"2026-08-04T11:14:46.685475Z","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":"2026-08-04T11:14:46.763615Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.763615Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:7f6642e7deb50d836ee6c9a46e9e902241c287785bc2826141f8fc7fe11aa2be","observation_id":"c9f017d8-6459-4f3e-b735-0286b616c175","resolution":{"observed_at":"2026-08-04T11:14:46.763615Z","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":"2026-08-04T11:14:46.839639Z","title":"1975, title Interstellar bubbles","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.839639Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:8bac643c330cc5e000f7d7cd803531d56c31401f17f7337c7be5d26e9c7fb1a6","observation_id":"9f79cf10-ace9-45c0-b425-d603849ab544","resolution":{"observed_at":"2026-08-04T11:14:46.839639Z","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":"2026-08-04T11:14:46.915336Z","title":"1992, title A Hydrodynamic Approach to Cosmology: Methodology , , 78, 341, 10.1086/191630","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.915336Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:e437ae60dc7a1ee89e50c15e2309142600f882d65a80367724a08013ac25fc62","observation_id":"95619f3a-2824-4a1a-b119-7a218d316fef","resolution":{"observed_at":"2026-08-04T11:14:46.915336Z","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":"2026-08-04T11:14:46.975123Z","title":"K., Kere s , D., Hopkins , P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:46.975123Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:1187fe6af372742843ca0da399996cd3f3d1bdb6d45e4d65731a3992270562d3","observation_id":"5b574ab3-f4b6-44fe-8e7e-da2fe8db8224","resolution":{"observed_at":"2026-08-04T11:14:46.975123Z","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":"2026-08-04T11:14:47.036648Z","title":"M., Whitmore , B","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.036648Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:dfaca4c09f09c1facf07651bcccd72aa8fd5fbf97c78d00207423b389a83f56e","observation_id":"498e3f5c-f8d2-4914-a17b-1d6128599595","resolution":{"observed_at":"2026-08-04T11:14:47.036648Z","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":"2026-08-04T11:14:47.094808Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.094808Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:3cb8bba50c04ce1e121e8e73705850b467c56378cf41c4b82ee9a1a4b64d3951","observation_id":"afca3c8a-2413-4425-871e-c370549bccd0","resolution":{"observed_at":"2026-08-04T11:14:47.094808Z","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":"2026-08-04T11:14:47.166197Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.166197Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:8533678553a406e6ecdc3c3cb6706fe500a43bae6b66c7097ae402b0bebb1cdf","observation_id":"9ca2ffdb-425c-4f88-bc94-35f5d4d9affe","resolution":{"observed_at":"2026-08-04T11:14:47.166197Z","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":"2026-08-04T11:14:47.254563Z","title":"M., Krumholz , M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.254563Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:0fcf0a8ccb38ba7340f5af39a19283bdd55651beef187dfc6cacf79e2385b615","observation_id":"80fc433f-3556-4ea0-bb48-cdaac83a575f","resolution":{"observed_at":"2026-08-04T11:14:47.254563Z","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":"2026-08-04T11:14:47.375184Z","title":"2020, title Cosmic ray feedback from supernovae in dwarf galaxies , , 638, A123, 10.1051/0004-6361/201936339","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.375184Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:1020e8672bcc9d15eaf25cf790331fdbb927290a4f157ade6d2f8fde3b450ee9","observation_id":"07feb606-45d4-4a3d-a58b-8faa5d8fbc8a","resolution":{"observed_at":"2026-08-04T11:14:47.375184Z","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":"2026-08-04T11:14:47.466630Z","title":"2024, title RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars , , 691, A231, 10.1051/0004-6361/202450699","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.466630Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:e41fc5f17b662b014174dbc53ae02b259ec3b27a39792176d45697d36d097144","observation_id":"20daa19d-cc85-4f3c-837c-9560fb4e4eb8","resolution":{"observed_at":"2026-08-04T11:14:47.466630Z","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":"2026-08-04T11:14:47.586822Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.586822Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:876066d5aba3907abceabea37363607f53478402dc3ccc2e0c2e89a890171ee3","observation_id":"73163f84-eec4-4df7-9239-a3d5ad4f73dc","resolution":{"observed_at":"2026-08-04T11:14:47.586822Z","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":"2026-08-04T11:14:47.658128Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.658128Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:3e115fdf108f9af6941a3e2d68e1ff6560062bb87672826a68e193f6fe4f1f35","observation_id":"e7ef6003-4d65-43cb-be93-0d44f5bea4c4","resolution":{"observed_at":"2026-08-04T11:14:47.658128Z","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":"2026-08-04T11:14:47.722082Z","title":"2019, title Massive star cluster formation and evolution in tidal dwarf galaxies , , 628, A60, 10.1051/0004-6361/201834403","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.722082Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:44b625f92bbae190bb3999f4fa620f9e327d8abc884d820dbe524504151be9d5","observation_id":"bf05b3f1-ca4a-42f8-8334-bd01647745b5","resolution":{"observed_at":"2026-08-04T11:14:47.722082Z","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":"2026-08-04T11:14:47.813361Z","title":"F., Krumholz , M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.813361Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:93e230388d918efdb7e2d539d38e6af327d865c94255ba63da1c67aefbbcb640","observation_id":"cf28efde-52e3-458f-9e44-11bd97a012bb","resolution":{"observed_at":"2026-08-04T11:14:47.813361Z","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":"2026-08-04T11:14:47.909456Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:47.909456Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:20734a13f84aed0b6cd7832743da48b0e5153428f6e54ddea58f6ed2c8f25777","observation_id":"69c97acf-b536-4ee0-8b4d-68006576a256","resolution":{"observed_at":"2026-08-04T11:14:47.909456Z","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":"10.1093/mnras/stv324","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Monthly Notices of the Royal Astronomical Society","work_id":"027271e6-028d-4450-92a9-bfb96d757d1b","year":2015},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.013094Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:9c815157c565e9355659073128548b1e055129c6dc8ccb6d31d76d1551ff431d","observation_id":"7f8e3296-75e7-4c6e-9109-8f39c7136c39","resolution":{"observed_at":"2026-08-04T11:18:59.107100Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:48.089517Z","title":"2017, title The SILCC project - III","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.089517Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b8168b970408cf355216fb1d78d91f1eddb93419cdca098deaa93d7bc4acbecf","observation_id":"6ffbd11d-c5ad-4269-9856-60721dd9ee88","resolution":{"observed_at":"2026-08-04T11:14:48.089517Z","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":"2026-08-04T11:14:48.128358Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.128358Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:2b845c08c0a1e179d69b25adac81a32183ba98862bf5c9c12407105397b770fc","observation_id":"d00faf4e-66b2-4be0-8ab7-5b3b2d145c86","resolution":{"observed_at":"2026-08-04T11:14:48.128358Z","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":"2026-08-04T11:14:48.171948Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.171948Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:432196936cf1103c4be8c1fa7f26c8fe8ecc10ad558d86dc51933e1cdcc2406e","observation_id":"954f9df2-d2e8-4601-b11b-411f30c5a0fe","resolution":{"observed_at":"2026-08-04T11:14:48.171948Z","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":"2026-08-04T11:14:48.247810Z","title":"E., Bastian , N., & Kennicutt , R","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.247810Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:8f5dcdad1580a8b8b3c68e31a354110535c74dd1852973ac28b06ede9525d281","observation_id":"d942e154-e144-4d22-bbc5-acf90fde20b3","resolution":{"observed_at":"2026-08-04T11:14:48.247810Z","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":"2026-08-04T11:14:48.306924Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.306924Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:86bae61e89b32fd775a9767b2a546e0be52eee5c081362ef1efbf0cf485c9f2f","observation_id":"1803567c-10b4-40b6-9ae4-393912ac5a00","resolution":{"observed_at":"2026-08-04T11:14:48.306924Z","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":"2026-08-04T11:14:48.427236Z","title":"Y., Guszejnov , D., Hopkins , P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.427236Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:c07a7a41cb324f4c6015cd542debc40acecab5d20040005fd3cd4201c67d8c79","observation_id":"5ab89384-74b9-44c7-9ade-5ad74ed3fdae","resolution":{"observed_at":"2026-08-04T11:14:48.427236Z","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":"2026-08-04T11:14:48.556794Z","title":"Y., Hafen , Z., Rodriguez , C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.556794Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:475dd1f6b105efcd723370f37d1a84d4d20d6c1ef7a5278e29e041584b799a66","observation_id":"d4cc8013-a74e-498e-8d51-e4b417006b54","resolution":{"observed_at":"2026-08-04T11:14:48.556794Z","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":"2026-08-04T11:14:48.637411Z","title":"Y., Hopkins , P","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.637411Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b303ad8b9cb1fe60bec8468bfa2c472ef7dc130854c708a1209826b2cd29aa5d","observation_id":"ba501af8-ef0a-46f3-ae7b-b7eeaac0d545","resolution":{"observed_at":"2026-08-04T11:14:48.637411Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.00052","last_updated":"2023-12-07T19:23:47Z","snapshot_observed_at":"2026-07-06T15:48:59.545602Z","submitted_at":"2023-06-30T18:00:04Z","title":"Does God play dice with star clusters?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.00052","snapshot_observed_at":"2026-08-04T11:14:48.757974Z","title":"Y., Offner , S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.757974Z"},"links":{"cited_paper":"/paper/2307.00052","citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:eb6e9b0496d4b71b8afd72a9e8fe90e877b2b71272902deaa5c6cf590e495e3e","observation_id":"11b7f30b-89f5-40b9-b779-9be844784f56","resolution":{"observed_at":"2026-08-04T11:14:48.757974Z","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":"2026-08-04T11:14:48.885276Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:48.885276Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:2192500d62e229650e5c80241bdd7ab77bab3195015ed2baab50a1c008b1a249","observation_id":"90be329a-753b-4fb4-8e69-cd8e93398fbc","resolution":{"observed_at":"2026-08-04T11:14:48.885276Z","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":"2026-08-04T11:14:49.013074Z","title":"A., Pakmor , R., Naab , T., & Springel , V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.013074Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:68b19ec5419d464e252c9284a5c8432d252d6745eaa3e38df0493906de5cf57b","observation_id":"fc185522-7272-43f6-8202-40cda7e5a2de","resolution":{"observed_at":"2026-08-04T11:14:49.013074Z","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":"2026-08-04T11:14:49.182237Z","title":"A., Pfrommer , C., Bryan , G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.182237Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:cc19ede932ee8b289605e6f1605380e02945ab793c26d076b98baaa993a534e6","observation_id":"c4ed88c9-d9d3-4036-8325-8150a6994cf1","resolution":{"observed_at":"2026-08-04T11:14:49.182237Z","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":"2026-08-04T11:14:49.272796Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.272796Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:05883a453755967e6a8d3193b4f9d12ae3d7c5652a7127eed299d7a00c937bdb","observation_id":"5b1c3c3b-787f-43ba-a82f-015a9583bfaf","resolution":{"observed_at":"2026-08-04T11:14:49.272796Z","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":"2026-08-04T11:14:49.364415Z","title":"M., Naab , T., Steinwandel , U","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.364415Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:c24a9f96256910e8383f8bdcadf7585d5576004a515b53bf696b8bfc4f79defa","observation_id":"dc9f6536-49a2-48ba-b489-f378e62467aa","resolution":{"observed_at":"2026-08-04T11:14:49.364415Z","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":"2026-08-04T11:14:49.422790Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.422790Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:a645a47760fe238b4d0d740332deae024401bf44a613aeeed0153fc6bf66300c","observation_id":"87b73c3f-e190-4f92-b796-041598901e56","resolution":{"observed_at":"2026-08-04T11:14:49.422790Z","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":"2026-08-04T11:14:49.490355Z","title":"C., Teyssier , R., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.490355Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:c02e534ae0cded50db4406549ca0ece16065a7655828dec86f41d25049d05526","observation_id":"a44ad141-6393-4b52-ac99-74633b892a23","resolution":{"observed_at":"2026-08-04T11:14:49.490355Z","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":"2026-08-04T11:14:49.534825Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.534825Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:8d42312da1510f4d3975c7917560cfbd8911d59e6a5fd690af526062da259021","observation_id":"fe8bc58e-a853-44bd-8f6d-71af3bb78ef5","resolution":{"observed_at":"2026-08-04T11:14:49.534825Z","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":"2026-08-04T11:14:49.616287Z","title":"C., Seth , A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.616287Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:773c2f0a69d00d7e715cd069826b628094944a2592368d6435e6bdfc26c46cda","observation_id":"b19bffe1-e5e8-4bcb-a274-f9002f437e4d","resolution":{"observed_at":"2026-08-04T11:14:49.616287Z","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":"2026-08-04T11:14:49.671427Z","title":"C., Seth , A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.671427Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:a499dd91eb54fc3a577e87c72bed66e9894bfcec1a37c8b15a18f4de8659c17b","observation_id":"5bf22e83-744e-4a42-ad8d-51c82d553d03","resolution":{"observed_at":"2026-08-04T11:14:49.671427Z","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":"2026-08-04T11:14:49.754312Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.754312Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:1cda2acf2223485aef778666dabea827090193993583ae0f930680f50c3fccad","observation_id":"f598a452-f886-47f7-bc99-5905df882d5e","resolution":{"observed_at":"2026-08-04T11:14:49.754312Z","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":"10.1093/mnras/stac1607","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"W., Kruijssen , J","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"5f205065-439b-4353-aa76-403c60d8204d","year":2022},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.832521Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:35cf562a13a9fc626966cbdd4e54175915c0d1ec654614c080152071fc11f5ae","observation_id":"79c15c95-5b56-4152-ba6b-be27bb767855","resolution":{"observed_at":"2026-08-04T11:18:58.744863Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:49.922462Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:49.922462Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b57fdbc20568fc57bb1941a78998e39a4b6baedfd0836e0809b394f8186d2a27","observation_id":"0db182cd-2f33-4934-8542-dd55de4a1886","resolution":{"observed_at":"2026-08-04T11:14:49.922462Z","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":"2026-08-04T11:14:50.002696Z","title":"2025, title The dynamical impact of cosmic rays in the Rhea magnetohydrodynamic simulations , , 700, A124, 10.1051/0004-6361/202553754","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.002696Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:c00e7403c553ef9aa16dbdd90758afc7c9c777f7619a1d35f67a2ed926324da2","observation_id":"ecfaf048-6048-4241-82a1-1dbc78a3dc59","resolution":{"observed_at":"2026-08-04T11:14:50.002696Z","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":"2026-08-04T11:14:50.085506Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.085506Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:4eb9439a6bccee532098b8e902b187b62d1305531cc1863efac7518b913ad313","observation_id":"8862fb3d-481b-4642-9503-e0c1232e14f0","resolution":{"observed_at":"2026-08-04T11:14:50.085506Z","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":"2026-08-04T11:14:50.200136Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.200136Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:4c1c5ebb71724fcfb3e2385ff6c1e67b6d7530fbf1201973c8e66ef8f8663db7","observation_id":"bbe5bed2-16b5-4878-93c3-4aebb6da0b5d","resolution":{"observed_at":"2026-08-04T11:14:50.200136Z","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":"2026-08-04T11:14:50.285226Z","title":"1995, title Inverse dynamical population synthesis and star formation , , 277, 1491, 10.1093/mnras/277.4.1491","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.285226Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:7099e100dfeed0d976914d70d064f7bc174e6bd3edff265ce3329bac309fa281","observation_id":"abcd1450-e1b1-425b-b51f-ad4745dcad66","resolution":{"observed_at":"2026-08-04T11:14:50.285226Z","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":"2026-08-04T11:14:50.466488Z","title":"R., McKee , C","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.466488Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:f335b10336effa115da343ac6e91ee18526ef91abf6d20a684007e0dacaed71a","observation_id":"4ac7266a-dfed-4d7a-ba53-34dd2edc776b","resolution":{"observed_at":"2026-08-04T11:14:50.466488Z","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":"2026-08-04T11:14:50.498304Z","title":null,"venue":null,"work_id":null,"year":1969},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.498304Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:bc185a601570efff6c3126126b2e8ed0739b24352c2cc3b6a09ce224de70bdac","observation_id":"2684d14f-62be-48eb-876b-aa48208fc7b6","resolution":{"observed_at":"2026-08-04T11:14:50.498304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.09484","last_updated":"2018-02-26T18:03:56Z","snapshot_observed_at":"2026-08-10T08:20:11.969300Z","submitted_at":"2018-02-26T18:03:56Z","title":"Disentangling the independently controllable factors of variation by interacting with the world","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.09484","snapshot_observed_at":"2026-08-04T11:14:50.525244Z","title":"J., & Lada , E","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.525244Z"},"links":{"cited_paper":"/paper/1802.09484","citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:95e3efbf8c351fc9a34f60af04cb29537a8c6a89fe47c060644d7066c91511ad","observation_id":"b2f1678e-7f2a-4a76-9b7e-adfcf6206831","resolution":{"observed_at":"2026-08-04T11:14:50.525244Z","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":"2026-08-04T11:14:50.591666Z","title":"H., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.591666Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:5c4d0b054ed0b397e1cb859d428b17c96b25ebbd012990ea5145c2cd9e3c147c","observation_id":"52b5da73-5c89-48d4-b51b-b72785190da6","resolution":{"observed_at":"2026-08-04T11:14:50.591666Z","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":"2026-08-04T11:14:50.725646Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.725646Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:faf39ee01b2cc07aad3fe6ca6ddf87504f04473cb6a183f3dddf30e5f62f5770","observation_id":"ddc5aae8-9b94-49b5-a74d-9804fbc8c89f","resolution":{"observed_at":"2026-08-04T11:14:50.725646Z","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":"2026-08-04T11:14:50.801620Z","title":null,"venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.801620Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:a82a8bdadfa1845cc3f47f6a1b4f426ead17f6af751a02a1b5fbe6eb6ecb32f7","observation_id":"d281fc89-1531-432c-8a37-58a20be9b67d","resolution":{"observed_at":"2026-08-04T11:14:50.801620Z","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":"2026-08-04T11:14:50.841287Z","title":"2025, title The Theory of Resonant Cosmic Ray driven Instabilities Growth and Saturation of Single Modes , , 979, 34, 10.3847/1538-4357/ad8eb3","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.841287Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b7a4d6148ba3e327de8826ff89886999c3c844eac3d8c7fc61ae4bce8f5a1339","observation_id":"c2f98941-1e0f-41d8-9464-21d3e4d08f06","resolution":{"observed_at":"2026-08-04T11:14:50.841287Z","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":"2026-08-04T11:14:50.925012Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:50.925012Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:e945aa971195b67ff859f6e0a73c98e78c3172bd9437c377f975226923fa2ec5","observation_id":"8ae55803-ec38-4282-9268-e5d2e5689d4b","resolution":{"observed_at":"2026-08-04T11:14:50.925012Z","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":"2026-08-04T11:14:51.020699Z","title":"Y., & Gnedin , N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.020699Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:67cbfe5c14b1519f3dd34e844d29f689113afa969756bd016a2196d2c507c450","observation_id":"37ace1ec-e287-474f-9048-e404071844f5","resolution":{"observed_at":"2026-08-04T11:14:51.020699Z","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":"2026-08-04T11:14:51.189421Z","title":"Y., Gnedin , N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.189421Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b2dc7c787c538b6c96e4fd49259ff6e6eef61a01086fde841b517ad1791bfb9f","observation_id":"05ed4067-f852-4c19-b41b-c290e4e9ece4","resolution":{"observed_at":"2026-08-04T11:14:51.189421Z","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":"2026-08-04T11:14:51.258103Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.258103Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:6190cb1e73f52012c3b64cca710b3def5fc1385e07ddcb109872192a39ec7c89","observation_id":"1d1db8d3-74cf-4c9f-acdc-739679089dba","resolution":{"observed_at":"2026-08-04T11:14:51.258103Z","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":"2026-08-04T11:14:51.368724Z","title":"V., & Torrey , P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.368724Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:4300cc321eeae75adef34a998880375795832f1982c14ccd6a2e88aeca327c67","observation_id":"c4602298-1662-454c-825a-f9ae8e9d101b","resolution":{"observed_at":"2026-08-04T11:14:51.368724Z","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":"10.1088/0004-637x/804/2/123","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astrophysical Journal","work_id":"1cd0e287-6fec-46ab-88f8-a440b014c756","year":2015},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.450405Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:ca030a38d4bb824d8278c5d5558f56479492d4bd628e7459b2b59ecaf23e4dd2","observation_id":"cc1458af-0439-4fa4-b931-464ffba3c060","resolution":{"observed_at":"2026-08-04T11:18:58.465491Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:51.512503Z","title":"N., Kruijssen , J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.512503Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:7b9c86cd4ac7598583318d04e7e913b1c182fee9fa7c2ea3fe124a9990e5c32a","observation_id":"cf529c6b-d425-4c87-9d4d-89a4494e4dfe","resolution":{"observed_at":"2026-08-04T11:14:51.512503Z","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":"10.1086/165267","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"1987, title Supershells and Propagating Star Formation , , 317, 190, 10.1086/165267","venue":"The Astrophysical Journal","work_id":"91f54cf5-2822-4a1e-9940-509bf9379797","year":1987},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.602948Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:573815ee84bfdfe6013780dc4cbe892db7691191e063ecb1258ad1b7c1ad4163","observation_id":"2b59b9d4-f2d6-4686-b46e-a53a1bf07740","resolution":{"observed_at":"2026-08-04T11:18:58.269767Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/184237","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"F., van Buren , D., & Lazareff , B","venue":"The Astrophysical Journal","work_id":"ce1ee884-ad76-42d5-8fc2-7d92988e685f","year":1984},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.707287Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:aa5197491f3f6de99f5f87afa66cdd8f1852ec516f79faebfdc0115b263a5c7a","observation_id":"59c6bb4a-13f8-4bc4-964b-a516755bb876","resolution":{"observed_at":"2026-08-04T11:18:58.014718Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/sty577","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2018, title The young star cluster population of M51 with LEGUS - II","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"f7ba2abb-beb6-4ff0-9277-f9270405b8af","year":2018},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.770104Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:df3fcd48660e4eccaeef090302fa616097be9da5ac31bb6cc35ee70b22d574ed","observation_id":"06a8f15d-f26f-491c-bed8-db1015a8dccc","resolution":{"observed_at":"2026-08-04T11:18:57.657700Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:51.843543Z","title":"R., Draine , B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.843543Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:fbce8657602bca6482a1460da4c29c423e56a762d562490ede4351dd451c15a6","observation_id":"f83b1166-721c-4396-9805-47d7f65a6dc4","resolution":{"observed_at":"2026-08-04T11:14:51.843543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.05826","last_updated":"2025-08-07T20:05:46Z","snapshot_observed_at":"2026-08-09T17:14:00.595909Z","submitted_at":"2025-08-07T20:05:46Z","title":"Gravitational Binding and Star Formation in Molecular Clouds of the Milky Way","version":1},"cited_work":{"arxiv_id":"2508.05826","doi":"10.48550/arxiv.2508.05826","metadata_source":"pith","pith_arxiv_id":"2508.05826","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Gravitational Binding and Star Formation in Molecular Clouds of the Milky Way","venue":"astro-ph.GA","work_id":"0737508a-295b-4267-9840-6d0d86535fed","year":2025},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.924790Z"},"links":{"cited_paper":"/paper/2508.05826","citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:e82f294230bb459bfb81f072df782091becbdf5fea602169f09e7595119e8683","observation_id":"5ec22d8a-b42d-46e1-85c3-fd8679f70959","resolution":{"observed_at":"2026-08-04T11:18:57.361059Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:51.994188Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:51.994188Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:e8849efc20a246d2a18a6fbae25eccda60eeedb5d87bdef4fa45a051e8b729ff","observation_id":"4509d736-2d42-4db5-86a0-8307206069fd","resolution":{"observed_at":"2026-08-04T11:14:51.994188Z","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":"2026-08-04T11:14:52.054277Z","title":"2025, title The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies , , 699, A282, 10.1051/0004-6361/202554126","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.054277Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:0548efe74949359117830644d47ad78b4aa560417c11c7f4ffe40e86c613e8be","observation_id":"fe1a5f4c-eb79-46ab-8048-3f2bec598466","resolution":{"observed_at":"2026-08-04T11:14:52.054277Z","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":"10.1086/145958","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"H., & Spitzer , Jr., L","venue":"The Astrophysical Journal","work_id":"41b7247a-5a9d-4e1d-82d2-2a7e51f3b9f9","year":1955},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.128643Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:d33e0e06672749257cade02847f551ce2344570c81c8a73d3e976564f79fa09b","observation_id":"e4c4f432-25c2-466c-8a2b-2fb4dfaf2d39","resolution":{"observed_at":"2026-08-04T11:18:57.088668Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/astrogeo/atac090","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2023, title The secret agent of galaxy evolution , Astronomy and Geophysics, 64, 1.29, 10.1093/astrogeo/atac090","venue":"Astronomy & Geophysics","work_id":"6a62fbea-c493-442c-a956-b721213e0cc9","year":2023},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.228730Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:c1babf6aec22e8e7c9a0d0fdffc89f478d212cabd5098f5afe9cef8a4e9523d9","observation_id":"9520b7e5-17e4-4632-80a9-3a0f0d9905e4","resolution":{"observed_at":"2026-08-04T11:18:56.797316Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-04T11:14:52.320958Z","title":"R., Wu , K., Inoue , Y., Yang , H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.320958Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b2106bd6fbec5e12f19cb81517c117f9127c017861bd13be5e9cea8381afe906","observation_id":"8fa87aef-a7b1-4577-8526-5188ee945014","resolution":{"observed_at":"2026-08-04T11:14:52.320958Z","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":"2026-08-04T11:14:52.427815Z","title":"V., Galli , D., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.427815Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:4ac21ff79ff1542820b0adec1474c22da957948c3f2a832fe563c3bc3adc1db9","observation_id":"d2bae4f8-9826-4e9b-b40b-7a67e7217e55","resolution":{"observed_at":"2026-08-04T11:14:52.427815Z","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":"2026-08-04T11:14:52.533254Z","title":"2011, title Magnetohydrodynamics on an unstructured moving grid , , 418, 1392, 10.1111/j.1365-2966.2011.19591.x","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.533254Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:214b30e040ba3b12f49c9dff0796defc7ccac3f6dcd2dccb1f4ae66b859d4ff9","observation_id":"e33c333a-7738-4500-81c6-fd157b0c1c4e","resolution":{"observed_at":"2026-08-04T11:14:52.533254Z","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":"2026-08-04T11:14:52.656138Z","title":"M., & Springel , V","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.656138Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:e8e031c24d1bab8e3996e433cb53c1a3a571d678cb8f8974a24e590efcf51999","observation_id":"904383bd-512e-4476-9a79-37c34044743a","resolution":{"observed_at":"2026-08-04T11:14:52.656138Z","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":"2026-08-04T11:14:52.769821Z","title":"2013, title Simulations of magnetic fields in isolated disc galaxies , , 432, 176, 10.1093/mnras/stt428","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.769821Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:8ffef39a4a6fc5a3062ce700a0faa147076c45aa85f4ec6a5353fa7d2f9cca23","observation_id":"092ba78b-e9b9-405b-a2d7-4bd6ee5c7887","resolution":{"observed_at":"2026-08-04T11:14:52.769821Z","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":"2026-08-04T11:14:52.853482Z","title":"2016 b , title Improving the convergence properties of the moving-mesh code AREPO , , 455, 1134, 10.1093/mnras/stv2380","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:52.853482Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:326e125223db6fa44bd708eba97bb78371ffa61007aa1dbb8eb342e5314333c1","observation_id":"0143297a-0044-46ba-a550-6bab014b0a60","resolution":{"observed_at":"2026-08-04T11:14:52.853482Z","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":"2026-08-04T11:14:53.010167Z","title":"2011, title Infrared Narrowband Tomography of the Local Starburst NGC 1569 with the Large Binocular Telescope/LUCIFER , , 141, 132, 10.1088/0004-6256/141/4/132","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:53.010167Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:ec4b624721d3f2388800aea7e413097bc3228496c2975f74502fede11dc2e8b8","observation_id":"13182b4a-836f-40d2-846a-da02841727c9","resolution":{"observed_at":"2026-08-04T11:14:53.010167Z","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":"2026-08-04T11:14:53.071164Z","title":"M., & Springel , V","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:53.071164Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:b9b050feede0f3caffdc754bb6c908f2fbeb806056894464a9d0f5f570e6844a","observation_id":"2d14ed9e-ecbe-47cf-9c24-8f2c836f5023","resolution":{"observed_at":"2026-08-04T11:14:53.071164Z","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":"2026-08-04T11:14:53.204043Z","title":"2005, title The Star Clusters of the Small Magellanic Cloud: Age Distribution , , 129, 2701, 10.1086/424938","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:53.204043Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:1033e2261df37b93c911b7a233fce79b64155052973e8c34642e9041b29288d2","observation_id":"ad2d498c-ba89-479f-a16e-bf9c1bd0a71a","resolution":{"observed_at":"2026-08-04T11:14:53.204043Z","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":"2026-08-04T11:14:53.334175Z","title":"2023, title SILCC - VII","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:53.334175Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:0297e2ed4867bef4405ab407273171fd9d56a475153822edd92b63aac9e29acb","observation_id":"d5ebb5bd-2da8-46ae-b43c-950ddea64604","resolution":{"observed_at":"2026-08-04T11:14:53.334175Z","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":"2026-08-04T11:14:53.486504Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback","version":2},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-08-04T11:14:53.486504Z"},"links":{"citing_paper":"/paper/2510.06134"},"observation_digest":"sha256:6c07d7f9ac498ceecae5c5baeda9e40ab687825a07a2572fb934089b4eb684ac","observation_id":"cb45bca8-44f1-41f2-9ef1-35d89cf3739c","resolution":{"observed_at":"2026-08-04T11:14:53.486504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2510.06134","last_updated":"2026-06-08T17:19:56Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-08T22:11:07.916962Z","submitted_at":"2025-10-07T17:08:44Z","title":"Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":87,"verified_exact":11,"verified_fuzzy":0},"total_outbound_references":135},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 100 of 135 outbound references and 1 inbound Pith citation observation for arXiv:2510.06134."}