{"as_of":"2026-08-11T06:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:013108cfae79b73d63f31db1b04f31385c4d07d22f62eeec2418396c25da81f4","coverage":[{"denominator":280,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T13:20:41.316182Z","state":"measured"},{"denominator":108,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":108,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:16:06.653466Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":3,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-07T15:16:06.653466Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.15910","last_updated":"2025-05-21T18:03:48Z","snapshot_observed_at":"2026-08-09T23:01:09.401904Z","submitted_at":"2025-05-21T18:03:48Z","title":"GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-07T15:16:06.653466Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2505.15910"},"observation_digest":"sha256:ea70d32860a2b7789d31bb99bde04eab8c7628ded6e2530293410111d155c566","observation_id":"48872628-0ea7-4756-8ef9-8187bb842f07","resolution":{"observed_at":"2026-08-07T15:16:06.653466Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":"2501.16438","doi":"10.48550/arxiv.2501.16438","metadata_source":"arxiv_reference","pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Formation of Globular Clusters","venue":"ArXiv.org","work_id":"63d706d2-77c2-4eab-be7d-645ba3cf4b2b","year":2025},"citing_paper":{"arxiv_id":"2507.07183","last_updated":"2026-04-06T15:52:17Z","snapshot_observed_at":"2026-07-06T21:54:43.509700Z","submitted_at":"2025-07-09T18:00:07Z","title":"Mass Distribution of Binary Black Hole Mergers from Young and Old Dense Star Clusters","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-19T05:22:10.358216Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2507.07183"},"observation_digest":"sha256:ef93524f644b92e9493012bb29dc9a6faea7790cc9b4b74b2b159ec59f84799b","observation_id":"21abeba8-14d3-4060-a8ba-49dd27686eab","resolution":{"observed_at":"2026-05-19T05:22:59.337142Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-03T21:25:59.840640Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.15782","last_updated":"2026-06-11T12:52:37Z","snapshot_observed_at":"2026-08-07T22:50:48.569655Z","submitted_at":"2025-11-19T19:00:00Z","title":"Trading oxygen for iron II. Oxygen- versus iron-dependent cosmic star formation history","version":2},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-03T21:25:59.840640Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2511.15782"},"observation_digest":"sha256:2ec4c546c0072982582170191fcfe05d20a97b7047f2b7a21952cac07c3659f8","observation_id":"fe1b6a54-6c57-4177-b830-6a2a6f8236fc","resolution":{"observed_at":"2026-08-03T21:25:59.840640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":"2501.16438","doi":"10.48550/arxiv.2501.16438","metadata_source":"arxiv_reference","pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Formation of Globular Clusters","venue":"ArXiv.org","work_id":"63d706d2-77c2-4eab-be7d-645ba3cf4b2b","year":2025},"citing_paper":{"arxiv_id":"2512.11059","last_updated":"2026-03-30T13:42:45Z","snapshot_observed_at":"2026-07-06T22:38:50.534580Z","submitted_at":"2025-12-11T19:17:27Z","title":"Milky Way Globular Clusters: Nurseries for Dynamically-Formed Binary Black Holes","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-16T22:47:31.056525Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2512.11059"},"observation_digest":"sha256:1966896ca2fe962fd06145afc355b11285d76c0e3a65c56527c318ac73125d9e","observation_id":"789b9199-6cb9-48e8-9aad-e726329755e1","resolution":{"observed_at":"2026-05-16T22:48:38.045321Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":"2501.16438","doi":"10.48550/arxiv.2501.16438","metadata_source":"arxiv_reference","pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Formation of Globular Clusters","venue":"ArXiv.org","work_id":"63d706d2-77c2-4eab-be7d-645ba3cf4b2b","year":2025},"citing_paper":{"arxiv_id":"2603.07481","last_updated":"2026-04-14T02:16:58Z","snapshot_observed_at":"2026-08-11T04:14:56.676377Z","submitted_at":"2026-03-08T05:43:29Z","title":"New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences","version":2},"reference_index":180,"source":"pdf_text","source_observed_at":"2026-05-15T15:32:23.373591Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2603.07481"},"observation_digest":"sha256:6897100395edc70be9752834494125b10eb3bd0aeb863bc514a5b6b2ed132b05","observation_id":"249347df-74fa-4e2f-ba9c-bde393b5c968","resolution":{"observed_at":"2026-05-15T15:36:12.504160Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":"2501.16438","doi":"10.48550/arxiv.2501.16438","metadata_source":"arxiv_reference","pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Formation of Globular Clusters","venue":"ArXiv.org","work_id":"63d706d2-77c2-4eab-be7d-645ba3cf4b2b","year":2025},"citing_paper":{"arxiv_id":"2605.11070","last_updated":"2026-05-11T18:00:01Z","snapshot_observed_at":"2026-07-31T07:50:59.074944Z","submitted_at":"2026-05-11T18:00:01Z","title":"A correlation predicting galaxies without dark matter","version":1},"reference_index":115,"source":"arxiv_source","source_observed_at":"2026-05-13T00:49:12.834674Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2605.11070"},"observation_digest":"sha256:4c801311b424253a0dff7a2a68229dc366997a4575c0a1348086d37846de63cd","observation_id":"b1f83896-18df-4687-a45b-e18321e0608e","resolution":{"observed_at":"2026-05-13T00:51:59.470136Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":"2501.16438","doi":"10.48550/arxiv.2501.16438","metadata_source":"arxiv_reference","pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Formation of Globular Clusters","venue":"ArXiv.org","work_id":"63d706d2-77c2-4eab-be7d-645ba3cf4b2b","year":2025},"citing_paper":{"arxiv_id":"2606.30746","last_updated":"2026-07-27T13:51:13Z","snapshot_observed_at":"2026-08-02T09:30:12.704470Z","submitted_at":"2026-06-29T18:00:14Z","title":"Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-01T01:42:48.009953Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2606.30746"},"observation_digest":"sha256:e29cfb15120e525c63b05bfadeb5490e7997b4fd645de13d7a5b92b943f1dc2c","observation_id":"fe5bae78-97c7-4f1d-bdd1-b17d48299293","resolution":{"observed_at":"2026-07-01T01:45:14.406443Z","resolver_source":"arxiv_id","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":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"cited_work":{"arxiv_id":"2501.16438","doi":"10.48550/arxiv.2501.16438","metadata_source":"arxiv_reference","pith_arxiv_id":"2501.16438","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Formation of Globular Clusters","venue":"ArXiv.org","work_id":"63d706d2-77c2-4eab-be7d-645ba3cf4b2b","year":2025},"citing_paper":{"arxiv_id":"2607.02480","last_updated":"2026-07-02T17:48:02Z","snapshot_observed_at":"2026-08-01T07:27:25.345011Z","submitted_at":"2026-07-02T17:48:02Z","title":"The Merger-Driven Origin of the Vast Extended Stellar Disc Around the Andromeda Galaxy","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-03T08:30:01.590143Z"},"links":{"cited_paper":"/paper/2501.16438","citing_paper":"/paper/2607.02480"},"observation_digest":"sha256:3495bc7127cc6660c67e8470f158be96451860f615e20f1e93ed0b7125032afc","observation_id":"0dbd4d99-0f33-4bdf-8e90-1f94f203f249","resolution":{"observed_at":"2026-07-03T08:37:46.203723Z","resolver_source":"arxiv_id","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"}}],"links":{"evidence":"/evidence","html":"/paper/2501.16438/citation-record","integrity":"/paper/2501.16438/integrity","json":"/paper/2501.16438/citation-record.json","paper":"/paper/2501.16438"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:20:40.794476Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.794476Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:85b6f77525868ad7314bbbdf79afe2a4d429514f74e6b44b73dd8a59065405f7","observation_id":"8c38992a-0afe-4d8d-a3b4-049348ad15bc","resolution":{"observed_at":"2026-08-10T13:20:40.794476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.07475","last_updated":"2015-06-16T12:25:55Z","snapshot_observed_at":"2026-07-06T04:19:08.349243Z","submitted_at":"2015-05-27T20:02:38Z","title":"Probing the role of the galactic environment in the formation of stellar clusters; using M83 as a test bench","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.07475","snapshot_observed_at":"2026-08-10T13:20:40.812169Z","title":"title Probing the role of the galactic environment in the formation of stellar clusters, using M83 as a test bench","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.812169Z"},"links":{"cited_paper":"/paper/1505.07475","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:365c420a8376ac35eeb4b2fb761beb9e40b4986bf77fcc3d1b4537d5d810497b","observation_id":"f25591a0-40cc-422c-839a-ce3f2800bc12","resolution":{"observed_at":"2026-08-10T13:20:40.812169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.12794","last_updated":"2020-08-28T18:00:07Z","snapshot_observed_at":"2026-07-06T09:51:00.475197Z","submitted_at":"2020-08-28T18:00:07Z","title":"Star cluster formation in the most extreme environments: Insights from the HiPEEC survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.12794","snapshot_observed_at":"2026-08-10T13:20:40.817150Z","title":"o nig S , author Larsen SS , author Melinder J , author Sabbi E , author Smith LJ and author \\","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.817150Z"},"links":{"cited_paper":"/paper/2008.12794","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:73924884fa1590b03a29ddc930e564590ddd4903703bc65231a873637ed14f0a","observation_id":"24ad0203-1873-451f-aa70-04a73fa1cbf1","resolution":{"observed_at":"2026-08-10T13:20:40.817150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.06188","last_updated":"2020-06-03T12:18:38Z","snapshot_observed_at":"2026-08-10T21:06:01.226155Z","submitted_at":"2020-05-13T07:22:27Z","title":"Star clusters near and far; tracing star formation across cosmic time","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.06188","snapshot_observed_at":"2026-08-10T13:20:40.822031Z","title":"title Star Clusters Near and Far; Tracing Star Formation Across Cosmic Time","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.822031Z"},"links":{"cited_paper":"/paper/2005.06188","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:feb0fcb2deb2a5c062f3c6b0334c4fd7f6996f34156e667c141768d7713e22dc","observation_id":"1a8ae151-8173-495a-877f-2216472f72fc","resolution":{"observed_at":"2026-08-10T13:20:40.822031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.03224","last_updated":"2024-06-12T12:49:51Z","snapshot_observed_at":"2026-08-09T16:47:20.261770Z","submitted_at":"2024-01-06T14:26:24Z","title":"Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.03224","snapshot_observed_at":"2026-08-10T13:20:40.827526Z","title":"title Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.827526Z"},"links":{"cited_paper":"/paper/2401.03224","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:88c65357ad8bdb7529dc3f10e310c22e36124ca2a382bfadc7e253ee9140346c","observation_id":"195c2ced-fd95-4ddd-946d-7ea2943e75f9","resolution":{"observed_at":"2026-08-10T13:20:40.827526Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.4806","last_updated":"2009-06-26T11:53:51Z","snapshot_observed_at":"2026-07-06T01:57:48.890721Z","submitted_at":"2009-06-26T11:53:51Z","title":"Dynamical mass segregation on a very short timescale","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.4806","snapshot_observed_at":"2026-08-10T13:20:40.832961Z","title":"title Dynamical Mass Segregation on a Very Short Timescale","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.832961Z"},"links":{"cited_paper":"/paper/0906.4806","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:d8af2566e1dc137ab155fd43ec1655d313f26659f412a8d9e5523e23024605b6","observation_id":"b8f39c14-571b-49c9-951f-21be64a6f657","resolution":{"observed_at":"2026-08-10T13:20:40.832961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6589","last_updated":"2012-11-23T16:55:50Z","snapshot_observed_at":"2026-08-08T04:27:55.053840Z","submitted_at":"2012-07-27T16:14:43Z","title":"Origin and growth of nuclear star clusters around massive black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.6589","snapshot_observed_at":"2026-08-10T13:20:40.838070Z","title":"title Origin and Growth of Nuclear Star Clusters around Massive Black Holes","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.838070Z"},"links":{"cited_paper":"/paper/1207.6589","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:4c7982ed4bc38762891a3037b35bda88981ab6cffcec5512f16162312fcada1e","observation_id":"ed252df9-26c0-48e1-a2ce-081738450a8c","resolution":{"observed_at":"2026-08-10T13:20:40.838070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.03640","last_updated":"2019-06-04T13:42:10Z","snapshot_observed_at":"2026-08-01T14:48:06.961204Z","submitted_at":"2018-11-08T19:02:15Z","title":"Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.03640","snapshot_observed_at":"2026-08-10T13:20:40.842596Z","title":"title Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.842596Z"},"links":{"cited_paper":"/paper/1811.03640","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:28fdb3c73c6b7be2b779fb8f0e800de6197f112bcd4271dc436ff13ef049dc18","observation_id":"2dd6f000-a9cf-49ec-9334-49be4e09e4b8","resolution":{"observed_at":"2026-08-10T13:20:40.842596Z","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":"2026-08-10T13:20:40.847295Z","title":"title The formation of globular clusters in merging and interacting galaxies","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.847295Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:43e6489c9d791a285d027d3f8d780cdd4436a0ce5a3c0fdccad9e03bbb477f03","observation_id":"b5962c4e-a1cf-43ba-a47e-3115741e81c4","resolution":{"observed_at":"2026-08-10T13:20:40.847295Z","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":"10.1002/asna.19312431903","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T13:20:43.010818Z","title":"title Photographische Beobachtungen von Nebeln am Spiegelteleskop der Hamburger Sternwarte in Bergedorf","venue":null,"work_id":"429a34cc-20a7-46c4-9816-964e77d3ca2a","year":1931},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.851820Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:bd204e66ccfaff2911c61a992fcbdb81a1bf949ecbeebc872122ce27bcc27766","observation_id":"13e2f56d-9e93-4b51-b4f8-0a0aaa717d42","resolution":{"observed_at":"2026-08-10T13:20:43.015846Z","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":{"arxiv_id":"0901.2302","last_updated":"2009-01-15T16:27:20Z","snapshot_observed_at":"2026-07-06T01:52:42.760931Z","submitted_at":"2009-01-15T16:27:20Z","title":"Stochastic self-enrichment, pre-enrichment, and the formation of globular clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.2302","snapshot_observed_at":"2026-08-10T13:20:40.856248Z","title":"title Stochastic Self-Enrichment, Pre-Enrichment, and the Formation of Globular Clusters","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.856248Z"},"links":{"cited_paper":"/paper/0901.2302","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:4ed9e13bac3e389075e0d8e8fc8208adb368ed816a96b859dda02a520d5a7178","observation_id":"bf1a79b6-6e4e-4986-bf2f-216812d7ab67","resolution":{"observed_at":"2026-08-10T13:20:40.856248Z","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":"2026-08-10T13:20:40.861167Z","title":"title On the star formation rate - brightest cluster relation: estimating the peak star formation rate in post-merger galaxies","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.861167Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:36101c955d831e77a6a8ea20348aa1219221a80fec27e36c7122206fbef3bdee","observation_id":"d9b31152-6c4f-4c7a-91ac-cf646dbcc95b","resolution":{"observed_at":"2026-08-10T13:20:40.861167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.01286","last_updated":"2017-12-04T19:00:01Z","snapshot_observed_at":"2026-08-07T07:51:07.838211Z","submitted_at":"2017-12-04T19:00:01Z","title":"Multiple Stellar Populations in Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.01286","snapshot_observed_at":"2026-08-10T13:20:40.865593Z","title":"title Multiple Stellar Populations in Globular Clusters","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.865593Z"},"links":{"cited_paper":"/paper/1712.01286","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:2a1f3b0ecb829d233998e20b51a1ff852c68627f986b6c4986081b31e9056739","observation_id":"1a7154d1-0f46-4399-b629-256f2efae437","resolution":{"observed_at":"2026-08-10T13:20:40.865593Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0511033","last_updated":"2005-11-01T16:25:06Z","snapshot_observed_at":"2026-07-07T00:55:35.463301Z","submitted_at":"2005-11-01T16:25:06Z","title":"Dynamical Mass Estimates for Two Luminous Star Clusters in Galactic Merger Remnants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0511033","snapshot_observed_at":"2026-08-10T13:20:40.870021Z","title":"title Dynamical mass estimates for two luminous star clusters in galactic merger remnants","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.870021Z"},"links":{"cited_paper":"/paper/astro-ph/0511033","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:5cfe42d88e3fc985775b6db150d7a3caf71bf8751cbd9d314cf27348e85b79c8","observation_id":"e34954a4-f8b3-4f6e-9b8b-19f3d0f258a5","resolution":{"observed_at":"2026-08-10T13:20:40.870021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.05991","last_updated":"2020-08-11T11:27:03Z","snapshot_observed_at":"2026-07-06T09:19:47.840044Z","submitted_at":"2020-05-12T18:02:18Z","title":"The globular cluster system mass-halo mass relation in the E-MOSAICS simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.05991","snapshot_observed_at":"2026-08-10T13:20:40.878735Z","title":"title The globular cluster system mass-halo mass relation in the E-MOSAICS simulations","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.878735Z"},"links":{"cited_paper":"/paper/2005.05991","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:d110b8a37b156be6a95f0063b8567cbe74115129c3217fc55b58d034e6550738","observation_id":"636c7a3d-9e2c-4e33-8a29-e2def3ec18f9","resolution":{"observed_at":"2026-08-10T13:20:40.878735Z","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":"2026-08-10T13:20:40.883356Z","title":"title Scaling of N-body calculations","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.883356Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:26277e55c4c470c9f1beb2530640fb58f4066a06b74b0abdb650d076c0b90779","observation_id":"4c63086b-9535-4835-b331-1d3625c82cb3","resolution":{"observed_at":"2026-08-10T13:20:40.883356Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.08359","last_updated":"2018-06-30T00:01:21Z","snapshot_observed_at":"2026-08-04T12:46:50.785370Z","submitted_at":"2018-04-23T12:19:05Z","title":"A catalogue of masses, structural parameters and velocity dispersion profiles of 112 Milky Way globular clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.08359","snapshot_observed_at":"2026-08-10T13:20:40.887639Z","title":"title A catalogue of masses, structural parameters, and velocity dispersion profiles of 112 Milky Way globular clusters","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.887639Z"},"links":{"cited_paper":"/paper/1804.08359","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:fdba152563f7551a7ae1cb1fcd4b5b40959125c3b37d3ca993f7b2ef0e98b560","observation_id":"6222f08e-b61a-4ff1-b062-a8e5cc947afc","resolution":{"observed_at":"2026-08-10T13:20:40.887639Z","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":"2026-08-10T13:20:40.896361Z","title":"title Dynamical evolution of star clusters in tidal fields","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.896361Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:bc1ff448e5df7441100ccdda6ca5ea66b00c82fa590a35a480c14e9d7ccd76bc","observation_id":"c6ffd36b-d884-4969-9b0b-77ba62e90b29","resolution":{"observed_at":"2026-08-10T13:20:40.896361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.01507","last_updated":"2018-11-05T04:11:13Z","snapshot_observed_at":"2026-07-06T07:12:34.254144Z","submitted_at":"2018-11-05T04:11:13Z","title":"Mean proper motions, space orbits and velocity dispersion profiles of Galactic globular clusters derived from Gaia DR2 data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.01507","snapshot_observed_at":"2026-08-10T13:20:40.905294Z","title":"title Mean proper motions, space orbits, and velocity dispersion profiles of Galactic globular clusters derived from Gaia DR2 data","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.905294Z"},"links":{"cited_paper":"/paper/1811.01507","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:fdcad1c069e1429e279ac99accde08db87803f62392c7f7e7f883ab0df8d3a81","observation_id":"ed1debb5-728e-4e94-8991-168a883f0edf","resolution":{"observed_at":"2026-08-10T13:20:40.905294Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01084","last_updated":"2019-05-23T15:34:28Z","snapshot_observed_at":"2026-07-06T07:43:12.012344Z","submitted_at":"2019-04-01T19:48:26Z","title":"An old, metal-poor globular cluster in Sextans A and the metallicity floor of globular cluster systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.01084","snapshot_observed_at":"2026-08-10T13:20:40.914896Z","title":"title An old, metal-poor globular cluster in Sextans A and the metallicity floor of globular cluster systems","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.914896Z"},"links":{"cited_paper":"/paper/1904.01084","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:a72f34bfd47c38d5453b0f420c670ec43d6ddc8173f2f616dd89219e3aaa1090","observation_id":"c50ae78f-91bd-4ea1-808d-2884224c4027","resolution":{"observed_at":"2026-08-10T13:20:40.914896Z","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":"2026-08-10T13:20:40.919717Z","title":"title Primordial pollution of globular clusters within their host dwarfs embedded in dark matter haloes at high redshifts","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.919717Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:c1c202a4794a9d5d82c9c9e83e71c542047349f1a6a1213ff40d4ee67c1cd7ef","observation_id":"124a2579-5dbb-4a34-af67-312e99750d9a","resolution":{"observed_at":"2026-08-10T13:20:40.919717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210596","last_updated":"2002-10-28T13:48:04Z","snapshot_observed_at":"2026-07-07T00:29:21.493197Z","submitted_at":"2002-10-28T13:48:04Z","title":"Building up the globular cluster system of the Milky Way. The contribution of the Sagittarius galaxy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0210596","snapshot_observed_at":"2026-08-10T13:20:40.929210Z","title":"title Building Up the Globular Cluster System of the Milky Way: The Contribution of the Sagittarius Galaxy","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.929210Z"},"links":{"cited_paper":"/paper/astro-ph/0210596","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:d4cf65d5f789a269ff69b59fd13907ff06549218e0b208eafc69785e5685fe92","observation_id":"c5380986-ec9b-4d73-be71-84a4df88bc69","resolution":{"observed_at":"2026-08-10T13:20:40.929210Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.15902","last_updated":"2023-09-27T18:00:01Z","snapshot_observed_at":"2026-08-06T13:41:06.055308Z","submitted_at":"2023-09-27T18:00:01Z","title":"In-situ vs accreted Milky Way globular clusters: a new classification method and implications for cluster formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.15902","snapshot_observed_at":"2026-08-10T13:20:40.934093Z","title":"title In-situ versus accreted Milky Way globular clusters: a new classification method and implications for cluster formation","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.934093Z"},"links":{"cited_paper":"/paper/2309.15902","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:7cfd743c1316f75b1c3370b74996df608b2ba4322e9a7d623bafa64e82b6ce40","observation_id":"aef6bb18-a61f-471a-96f2-0967403f52a0","resolution":{"observed_at":"2026-08-10T13:20:40.934093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9703099","last_updated":"1997-03-15T02:54:29Z","snapshot_observed_at":"2026-08-02T06:38:24.276126Z","submitted_at":"1997-03-15T02:54:29Z","title":"The Dependence of Globular Cluster Number on Density for Abell Cluster Central Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9703099","snapshot_observed_at":"2026-08-10T13:20:40.938883Z","title":"title The Dependence of Globular Cluster Number on Density for Abell Cluster Central Galaxies","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.938883Z"},"links":{"cited_paper":"/paper/astro-ph/9703099","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:2a68c7f82bf473adbca77fa2032b12e22dfa7af3bb59d3c32b7ad5d68499e7cc","observation_id":"7f5d5283-8ac9-44db-b1da-6d303d3834db","resolution":{"observed_at":"2026-08-10T13:20:40.938883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0605035","last_updated":"2006-05-01T20:00:01Z","snapshot_observed_at":"2026-08-08T19:46:12.963847Z","submitted_at":"2006-05-01T20:00:01Z","title":"The Role of Pressure in GMC Formation II: The H_2 - Pressure Relation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0605035","snapshot_observed_at":"2026-08-10T13:20:40.943567Z","title":"title The Role of Pressure in GMC Formation II: The H _ 2 -Pressure Relation","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.943567Z"},"links":{"cited_paper":"/paper/astro-ph/0605035","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:b078fc9b20cad11d737261846a1fe533ee4cf49980c3eaa87bbaaaf2bcf33ac8","observation_id":"65afdcc8-86e6-4b5d-a0ed-9c92314125c2","resolution":{"observed_at":"2026-08-10T13:20:40.943567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.1254","last_updated":"2009-10-21T18:23:05Z","snapshot_observed_at":"2026-07-06T01:56:47.439727Z","submitted_at":"2009-08-09T20:01:11Z","title":"Resolving Globular Cluster Formation within a Cosmological Context","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.1254","snapshot_observed_at":"2026-08-10T13:20:40.948448Z","title":"title Globular Cluster Formation Within a Cosmological Context","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.948448Z"},"links":{"cited_paper":"/paper/0908.1254","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:d75dbe2aa16a4335b9057421cde55d45f6416c0fe2ef54c180a543900ceeba07","observation_id":"26f65c27-ffe7-46de-a333-42244d6747d9","resolution":{"observed_at":"2026-08-10T13:20:40.948448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.01669","last_updated":"2021-11-02T15:30:13Z","snapshot_observed_at":"2026-08-03T00:59:55.614726Z","submitted_at":"2021-11-02T15:30:13Z","title":"Age Determination of Galaxy Merger Remnant Stars using Asteroseismology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.01669","snapshot_observed_at":"2026-08-10T13:20:40.952951Z","title":"title Age determination of galaxy merger remnant stars using asteroseismology","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.952951Z"},"links":{"cited_paper":"/paper/2111.01669","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:858b4992785aabb2bde70ddd763b694ca0c59f25d9c99cad2b315f897f1993b9","observation_id":"bc36616f-55f5-4e7a-bbed-bf2ffab45f51","resolution":{"observed_at":"2026-08-10T13:20:40.952951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.08336","last_updated":"2021-06-15T18:00:02Z","snapshot_observed_at":"2026-07-06T11:19:38.321360Z","submitted_at":"2021-06-15T18:00:02Z","title":"Low-luminosity galaxies in the early universe have observed sizes similar to star cluster complexes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.08336","snapshot_observed_at":"2026-08-10T13:20:40.957394Z","title":"title Low-luminosity Galaxies in the Early Universe Have Observed Sizes Similar to Star Cluster Complexes","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.957394Z"},"links":{"cited_paper":"/paper/2106.08336","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:8e55093d544ba383c4365d0e66393477599d14015f4516a75f817bc30c09fc59","observation_id":"2b288c4c-06d2-4e82-a23e-769cea3f6a97","resolution":{"observed_at":"2026-08-10T13:20:40.957394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.01548","last_updated":"2017-09-25T17:12:41Z","snapshot_observed_at":"2026-07-06T05:40:44.505995Z","submitted_at":"2017-05-03T18:00:01Z","title":"The Globular Cluster - Dark Matter Halo Connection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.01548","snapshot_observed_at":"2026-08-10T13:20:40.962113Z","title":"title The globular cluster-dark matter halo connection","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.962113Z"},"links":{"cited_paper":"/paper/1705.01548","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:b9d154265402c6ea13f9bd98a8d78def9041bebdd05509f398c6a54e12559a1d","observation_id":"3fd873b1-a130-4b56-9ff7-53403cea44be","resolution":{"observed_at":"2026-08-10T13:20:40.962113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00009","last_updated":"2018-06-06T03:03:27Z","snapshot_observed_at":"2026-07-06T06:07:05.119814Z","submitted_at":"2017-10-31T18:00:00Z","title":"The Little Engines That Could? Globular Clusters Contribute Significantly to Reionization-era Star Formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00009","snapshot_observed_at":"2026-08-10T13:20:40.966921Z","title":"title The Little Engines That Could? Globular clusters contribute significantly to reionization-era star formation","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.966921Z"},"links":{"cited_paper":"/paper/1711.00009","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:6c6d2e6f7f3bdbe67271535ee2d27ccb0f42593144dde97d330fa0a6dc542fc2","observation_id":"c2e7e6ce-7cd4-4289-b0b8-963548f9de00","resolution":{"observed_at":"2026-08-10T13:20:40.966921Z","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":"2026-08-10T13:20:40.971691Z","title":"title Extragalactic Globular Clusters and Galaxy Formation","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.971691Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:b25424d6a3447c726dcf6fd03fe8d43ac4dad725d27586e27f7f062499c35807","observation_id":"ae01a78e-8221-42bd-8089-9eb7d99d2ab7","resolution":{"observed_at":"2026-08-10T13:20:40.971691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.5390","last_updated":"2012-09-24T20:00:00Z","snapshot_observed_at":"2026-08-07T20:10:30.048802Z","submitted_at":"2012-09-24T20:00:00Z","title":"The SLUGGS Survey: NGC 3115, A Critical Test Case for Metallicity Bimodality in Globular Cluster Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.5390","snapshot_observed_at":"2026-08-10T13:20:40.976226Z","title":"title The SLUGGS Survey: NGC 3115, A Critical Test Case for Metallicity Bimodality in Globular Cluster Systems","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.976226Z"},"links":{"cited_paper":"/paper/1209.5390","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:9fd9f26634bed3119fe5fdee4348ea7d1ad60a140ced7798c48cafc5dfa7c4c8","observation_id":"d96b56a1-5d14-44fe-bc63-6073c2fcad81","resolution":{"observed_at":"2026-08-10T13:20:40.976226Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.2079","last_updated":"2014-09-10T06:00:01Z","snapshot_observed_at":"2026-08-07T13:01:00.090263Z","submitted_at":"2014-05-08T20:00:08Z","title":"The SAGES Legacy Unifying Globulars and GalaxieS Survey (SLUGGS): Sample definition, methods, and initial results","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.2079","snapshot_observed_at":"2026-08-10T13:20:40.980971Z","title":"title The SAGES Legacy Unifying Globulars and GalaxieS Survey (SLUGGS): Sample Definition, Methods, and Initial Results","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.980971Z"},"links":{"cited_paper":"/paper/1405.2079","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:4c50d9d95eb13870d86413ecdc4b81b0205df4f50314f8aedf278ef958d82afa","observation_id":"ee136b08-f564-4464-98eb-1a9255a11009","resolution":{"observed_at":"2026-08-10T13:20:40.980971Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.14330","last_updated":"2021-04-29T13:29:17Z","snapshot_observed_at":"2026-08-10T01:25:27.109229Z","submitted_at":"2021-04-29T13:29:17Z","title":"Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. III. Constraints from a subgiant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.14330","snapshot_observed_at":"2026-08-10T13:20:40.985649Z","title":"title Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.985649Z"},"links":{"cited_paper":"/paper/2104.14330","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:eaf634d86da4cfbb8c3f545499cb721b6d15c3688b2a06fb4a5208ac5ceec563","observation_id":"5b731475-25e3-45d6-b581-817a4a79c528","resolution":{"observed_at":"2026-08-10T13:20:40.985649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201066","last_updated":"2002-01-05T07:04:46Z","snapshot_observed_at":"2026-08-09T04:03:49.245130Z","submitted_at":"2002-01-05T07:04:46Z","title":"The Formation of the First Globular Clusters in Dwarf Galaxies Before the Epoch of Reionization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0201066","snapshot_observed_at":"2026-08-10T13:20:40.990099Z","title":"title The Formation of the First Globular Clusters in Dwarf Galaxies before the Epoch of Reionization","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.990099Z"},"links":{"cited_paper":"/paper/astro-ph/0201066","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:3415da7574b424319924c88e42d11452314dfdb70d859e20146d023bd178843a","observation_id":"b8789861-c4b2-4325-a219-08a132855fdf","resolution":{"observed_at":"2026-08-10T13:20:40.990099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.00900","last_updated":"2019-11-27T09:16:06Z","snapshot_observed_at":"2026-08-10T11:33:44.856646Z","submitted_at":"2019-01-03T20:10:15Z","title":"High-Precision Dark Halo Virial Masses from Globular Cluster Numbers: Implications for Globular Cluster Formation and Galaxy Assembly","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.00900","snapshot_observed_at":"2026-08-10T13:20:40.995040Z","title":"title High-precision Dark Halo Virial Masses from Globular Cluster Numbers: Implications for Globular Cluster Formation and Galaxy Assembly","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.995040Z"},"links":{"cited_paper":"/paper/1901.00900","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:a0899ee64a12f081dba94df05ce2e96663e7876e61bb615d515195f007827506","observation_id":"92c404c7-e6e1-478c-b930-a28aebfb875e","resolution":{"observed_at":"2026-08-10T13:20:40.995040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.07562","last_updated":"2022-01-10T17:33:44Z","snapshot_observed_at":"2026-08-05T09:07:17.339164Z","submitted_at":"2021-12-14T17:09:27Z","title":"Deriving ages and horizontal branch properties of integrated stellar populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.07562","snapshot_observed_at":"2026-08-10T13:20:40.999388Z","title":"title Deriving ages and horizontal branch properties of integrated stellar populations","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:40.999388Z"},"links":{"cited_paper":"/paper/2112.07562","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:5a617d50b95456d112bde2c6ee4226400ef8dfca6c9917be13c9c2194bae44bb","observation_id":"14064854-f225-47ea-8c34-22bd2bf41c84","resolution":{"observed_at":"2026-08-10T13:20:40.999388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.06947","last_updated":"2016-03-22T20:00:02Z","snapshot_observed_at":"2026-07-06T04:50:20.917367Z","submitted_at":"2016-03-22T20:00:02Z","title":"Star Clusters in M31: VII. Global Kinematics and Metallicity Subpopulations of the Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.06947","snapshot_observed_at":"2026-08-10T13:20:41.004122Z","title":"title Star Clusters in M31","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.004122Z"},"links":{"cited_paper":"/paper/1603.06947","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:641a161d8e198cfa6c7c8a3d5b5b5b15b71b02748d140aa8e46c5bc774f0cd1f","observation_id":"f461e5ab-81a1-4f79-a18e-1716e0c8ab7e","resolution":{"observed_at":"2026-08-10T13:20:41.004122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.00591","last_updated":"2022-08-09T12:10:38Z","snapshot_observed_at":"2026-08-10T05:31:57.455442Z","submitted_at":"2022-02-01T17:33:21Z","title":"The Chemo-Dynamical Groups of Galactic Globular Clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.00591","snapshot_observed_at":"2026-08-10T13:20:41.009249Z","title":"title The chemo-dynamical groups of Galactic globular clusters","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.009249Z"},"links":{"cited_paper":"/paper/2202.00591","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:61bb52a48bc6e4a7456824c3674b4a40389df6c2236da37cac861c18ef0f33ca","observation_id":"d409c1b1-6e7d-4668-abb0-4bd381ddce8f","resolution":{"observed_at":"2026-08-10T13:20:41.009249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.01938","last_updated":"2018-04-27T20:34:34Z","snapshot_observed_at":"2026-07-06T05:45:47.779788Z","submitted_at":"2017-06-06T19:30:12Z","title":"Globular Clusters in a Cosmological N-body Simulation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.01938","snapshot_observed_at":"2026-08-10T13:20:41.014484Z","title":"title Globular Clusters in a Cosmological N-body Simulation","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.014484Z"},"links":{"cited_paper":"/paper/1706.01938","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:0337a665d225aeaff1023fcbc78fd848e0256ac489705a2a165abec128d0fd14","observation_id":"47a70a55-d3bd-4273-bc09-bb0256dde5c5","resolution":{"observed_at":"2026-08-10T13:20:41.014484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.03440","last_updated":"2021-05-07T18:00:03Z","snapshot_observed_at":"2026-07-30T21:32:41.739005Z","submitted_at":"2021-05-07T18:00:03Z","title":"ELVES II: GCs and Nuclear Star Clusters of Dwarf Galaxies; The Importance of Environment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.03440","snapshot_observed_at":"2026-08-10T13:20:41.019813Z","title":"title ELVES II: Globular Clusters and Nuclear Star Clusters of Dwarf Galaxies: the Importance of Environment","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.019813Z"},"links":{"cited_paper":"/paper/2105.03440","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:964c6ee521cb55c2d48c361c58bfdee7d18fdc4b2d93bff171377eaefecf67e0","observation_id":"6ef2f0d0-5b2c-4a61-9933-b6fc4f9a56f9","resolution":{"observed_at":"2026-08-10T13:20:41.019813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512650","last_updated":"2005-12-30T12:01:40Z","snapshot_observed_at":"2026-07-07T00:57:15.927137Z","submitted_at":"2005-12-30T12:01:40Z","title":"NGC 6791: an exotic open cluster or the nucleus of a tidally disrupted galaxy?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512650","snapshot_observed_at":"2026-08-10T13:20:41.024444Z","title":"title NGC 6791: An Exotic Open Cluster or the Nucleus of a Tidally Disrupted Galaxy? journal volume 643 : pages 1151--1159","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.024444Z"},"links":{"cited_paper":"/paper/astro-ph/0512650","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:aacb4835ff9587bf3eece4a45004d08f1913ead0509ae374823b026202939051","observation_id":"d6ebe3bd-78e2-48df-92ed-b4b38bc37023","resolution":{"observed_at":"2026-08-10T13:20:41.024444Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.1963","last_updated":"2010-02-09T21:00:11Z","snapshot_observed_at":"2026-07-06T02:03:42.854332Z","submitted_at":"2010-02-09T21:00:11Z","title":"M 54 + Sagittarius = omega Centauri","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.1963","snapshot_observed_at":"2026-08-10T13:20:41.029718Z","title":"title M54 + Sagittarius = Centauri","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.029718Z"},"links":{"cited_paper":"/paper/1002.1963","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:627585592926cfbeda23babf31d3b76388af27f2826e28a0eac6be4cde10a6bd","observation_id":"626769cc-a9d8-40e8-87a5-57f8e3acccd6","resolution":{"observed_at":"2026-08-10T13:20:41.029718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.1723","last_updated":"2010-03-08T21:02:55Z","snapshot_observed_at":"2026-07-06T02:04:41.678012Z","submitted_at":"2010-03-08T21:02:55Z","title":"Properties of stellar generations in Globular Clusters and relations with global parameters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.1723","snapshot_observed_at":"2026-08-10T13:20:41.036130Z","title":"title Properties of stellar generations in globular clusters and relations with global parameters","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.036130Z"},"links":{"cited_paper":"/paper/1003.1723","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:98efc934e714eef9e2504aa40ebb22a9483ca08c368492bc19609ab21882d467","observation_id":"216d1001-ea69-4e60-981a-e48040dc9137","resolution":{"observed_at":"2026-08-10T13:20:41.036130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.00599","last_updated":"2022-07-10T23:28:14Z","snapshot_observed_at":"2026-08-04T12:43:54.154636Z","submitted_at":"2022-03-01T16:39:29Z","title":"Modeling the kinematics of globular cluster systems","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.00599","snapshot_observed_at":"2026-08-10T13:20:41.041323Z","title":"title Modeling the kinematics of globular cluster systems","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.041323Z"},"links":{"cited_paper":"/paper/2203.00599","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:67c155735ff2010b641d8f4bbe8c3259e222f35a2d6354f16670b4eb584d4b00","observation_id":"cb119dbe-fc14-4788-a7f4-ee3689da3a1d","resolution":{"observed_at":"2026-08-10T13:20:41.041323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08218","last_updated":"2023-05-22T19:58:07Z","snapshot_observed_at":"2026-07-06T14:42:57.101630Z","submitted_at":"2023-01-19T18:26:20Z","title":"Formation of globular clusters in dwarf galaxies of the Local Group","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08218","snapshot_observed_at":"2026-08-10T13:20:41.045930Z","title":"title Formation of globular clusters in dwarf galaxies of the Local Group","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.045930Z"},"links":{"cited_paper":"/paper/2301.08218","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:46bc8ce648edbbb87eedfc0347408dd13f07af7e295567a412a1b25f1fea973f","observation_id":"f174b1d0-59f3-4fe3-bf48-c07a2486969c","resolution":{"observed_at":"2026-08-10T13:20:41.045930Z","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":"2026-08-10T13:20:41.050958Z","title":"title Evolution of globular clusters in the Galaxy","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.050958Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:32dc0c945111288edb9d0616d8c715ee5175311827cacdfc84a3a9f3761f306c","observation_id":"9dee20a4-fdac-4d91-b98b-a2310ec33a44","resolution":{"observed_at":"2026-08-10T13:20:41.050958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.03479","last_updated":"2019-11-08T19:00:01Z","snapshot_observed_at":"2026-08-09T12:30:13.661515Z","submitted_at":"2019-11-08T19:00:01Z","title":"The lifecycle of molecular clouds in nearby star-forming disc galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.03479","snapshot_observed_at":"2026-08-10T13:20:41.055972Z","title":"title The lifecycle of molecular clouds in nearby star-forming disc galaxies","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.055972Z"},"links":{"cited_paper":"/paper/1911.03479","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:4f7fb4f1db19b564b720fd7d0e2e86a7f59e0812d2486590bd72b97f206080f0","observation_id":"d662fcd8-7dd4-4c50-8690-62f804458235","resolution":{"observed_at":"2026-08-10T13:20:41.055972Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06113","last_updated":"2020-04-13T18:00:00Z","snapshot_observed_at":"2026-07-06T09:12:01.617790Z","submitted_at":"2020-04-13T18:00:00Z","title":"The molecular cloud lifecycle","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.06113","snapshot_observed_at":"2026-08-10T13:20:41.060450Z","title":"title The Molecular Cloud Lifecycle","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.060450Z"},"links":{"cited_paper":"/paper/2004.06113","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:5c710cba4a2b02c3435bf9e2e9fb6e0daddeefe90ed436e102c7f9abd55e52c9","observation_id":"71e26d1d-52c8-4631-b007-86c9c6b3354b","resolution":{"observed_at":"2026-08-10T13:20:41.060450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.13788","last_updated":"2020-10-26T18:00:00Z","snapshot_observed_at":"2026-07-06T10:08:43.216857Z","submitted_at":"2020-10-26T18:00:00Z","title":"Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.13788","snapshot_observed_at":"2026-08-10T13:20:41.065346Z","title":"title Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.065346Z"},"links":{"cited_paper":"/paper/2010.13788","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:e1366ec89853bbc78bc408cbdb3da916b81b9465aef09b62bb7e1c45624a4d63","observation_id":"d93b76d5-0e25-4821-b1cc-c594b847760c","resolution":{"observed_at":"2026-08-10T13:20:41.065346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.09570","last_updated":"2022-03-17T19:13:26Z","snapshot_observed_at":"2026-08-07T11:34:57.591527Z","submitted_at":"2022-03-17T19:13:26Z","title":"The Life and Times of Giant Molecular Clouds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.09570","snapshot_observed_at":"2026-08-10T13:20:41.070519Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.070519Z"},"links":{"cited_paper":"/paper/2203.09570","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:001ced8688b24cc53c7d767e3ea99be269f505dd4d6fe6bb07aa1795a9e2d5f0","observation_id":"2d4adb86-f1bb-42c3-82b7-d5f8f32a6654","resolution":{"observed_at":"2026-08-10T13:20:41.070519Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.13160","last_updated":"2025-01-24T10:30:27Z","snapshot_observed_at":"2026-08-10T16:22:05.260999Z","submitted_at":"2025-01-22T19:00:04Z","title":"COOL Research DAO Whitepaper -- Towards community-owned astrophysics for everyone","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.13160","snapshot_observed_at":"2026-08-10T13:20:41.075263Z","title":"title COOL Research DAO Whitepaper - Towards community-owned astrophysics for everyone doi doi:10.48550/arXiv.2501.13160","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.075263Z"},"links":{"cited_paper":"/paper/2501.13160","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:7a13b2bec46513ace90ebd07dc7faa2b22987b44a14cdf0f3a57be5565468eb8","observation_id":"60373bd7-8992-42cd-93b5-956539faae3b","resolution":{"observed_at":"2026-08-10T13:20:41.075263Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.3649","last_updated":"2012-01-17T22:02:30Z","snapshot_observed_at":"2026-07-06T02:41:18.314885Z","submitted_at":"2012-01-17T22:02:30Z","title":"An optical/NIR survey of globular clusters in early-type galaxies III. On the colour bimodality of GC systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.3649","snapshot_observed_at":"2026-08-10T13:20:41.080145Z","title":"title An optical/NIR survey of globular clusters in early-type galaxies","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.080145Z"},"links":{"cited_paper":"/paper/1201.3649","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:0a78816cbb783c30f66a627bd98d58dda347fc5ec49f36afbd33e2a7a057dcbc","observation_id":"c38b3bd8-507c-4dd9-9f5b-50e7ba728652","resolution":{"observed_at":"2026-08-10T13:20:41.080145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.01888","last_updated":"2019-03-20T18:45:29Z","snapshot_observed_at":"2026-07-06T07:05:57.302799Z","submitted_at":"2018-10-03T18:00:05Z","title":"Formation of Globular Cluster Systems II: Impact of the Cutoff of the Cluster Initial Mass Function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.01888","snapshot_observed_at":"2026-08-10T13:20:41.085132Z","title":"title Formation of globular cluster systems - II","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.085132Z"},"links":{"cited_paper":"/paper/1810.01888","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:342f0f2cf463569ea21f41ef076b7ca73293616186ecb0acbf84344409ca9878","observation_id":"a0502a2f-64ba-4f49-b89a-e59f87c1a96c","resolution":{"observed_at":"2026-08-10T13:20:41.085132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.05199","last_updated":"2019-05-13T18:00:02Z","snapshot_observed_at":"2026-08-10T23:17:26.991258Z","submitted_at":"2019-05-13T18:00:02Z","title":"Origins of scaling relations of globular cluster systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.05199","snapshot_observed_at":"2026-08-10T13:20:41.089815Z","title":"title Origins of scaling relations of globular cluster systems","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.089815Z"},"links":{"cited_paper":"/paper/1905.05199","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:ea0716164b2a7ce9ff13f3b116b4de932756a8f546ae7d9dc7bd0cd457787d5f","observation_id":"24343809-452e-4ffd-bf35-305bf4803a4b","resolution":{"observed_at":"2026-08-10T13:20:41.089815Z","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":"2026-08-10T13:20:41.094750Z","title":"title Formation of globular cluster systems: from dwarf galaxies to giants","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.094750Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:b8b41b3ff7782225811f60c9ac28d29595db7614f3d3434b52b0614fc385c006","observation_id":"e41bafe4-20a7-4805-9ab2-286ceb2d14da","resolution":{"observed_at":"2026-08-10T13:20:41.094750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.10450","last_updated":"2022-12-13T07:48:16Z","snapshot_observed_at":"2026-07-06T13:44:18.807144Z","submitted_at":"2022-08-22T17:08:34Z","title":"Star formation at the smallest scales; A JWST study of the clump populations in SMACS0723","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.10450","snapshot_observed_at":"2026-08-10T13:20:41.099182Z","title":"title Star formation at the smallest scales: a JWST study of the clump populations in SMACS0723","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.099182Z"},"links":{"cited_paper":"/paper/2208.10450","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:39879edc37f58eb4436def6d2e3565adf1eb77d0e496fcde3b9ccc2ba2bad808","observation_id":"8f3b26a4-004d-4015-a76f-aa7563aa0c5e","resolution":{"observed_at":"2026-08-10T13:20:41.099182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.5783","last_updated":"2011-08-03T16:49:37Z","snapshot_observed_at":"2026-07-06T02:18:19.575110Z","submitted_at":"2010-10-27T20:00:04Z","title":"Evidence Against Dark Matter Halos Surrounding the Globular Clusters MGC1 and NGC 2419","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.5783","snapshot_observed_at":"2026-08-10T13:20:41.103573Z","title":"title Evidence against Dark Matter Halos Surrounding the Globular Clusters MGC1 and NGC 2419","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.103573Z"},"links":{"cited_paper":"/paper/1010.5783","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:44fbd830be852e0f001d10278d3c9b51adffbb60c37b7a3754bd63a9e9516f36","observation_id":"737f9b8e-7c5a-4e51-8969-30d2738748c0","resolution":{"observed_at":"2026-08-10T13:20:41.103573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.4826","last_updated":"2012-03-27T17:03:10Z","snapshot_observed_at":"2026-07-06T02:44:58.674531Z","submitted_at":"2012-03-21T20:14:07Z","title":"The ACS Nearby Galaxy Survey Treasury. X. Quantifying the Star Cluster Formation Efficiency of Nearby Dwarf Galaxies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.4826","snapshot_observed_at":"2026-08-10T13:20:41.108221Z","title":"title The ACS Nearby Galaxy Survey Treasury","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.108221Z"},"links":{"cited_paper":"/paper/1203.4826","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:c4f06d9d324c0c824087627b36678dac8eec7f3e91d73d84da03ab46597c52e3","observation_id":"23850996-e384-43af-ba8f-62cb2031eb6a","resolution":{"observed_at":"2026-08-10T13:20:41.108221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9804319","last_updated":"1998-04-29T23:08:31Z","snapshot_observed_at":"2026-07-07T01:20:40.325068Z","submitted_at":"1998-04-29T23:08:31Z","title":"The Formation of Giant Elliptical Galaxies and Their Globular Cluster Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9804319","snapshot_observed_at":"2026-08-10T13:20:41.112686Z","title":"title The Formation of Giant Elliptical Galaxies and Their Globular Cluster Systems","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.112686Z"},"links":{"cited_paper":"/paper/astro-ph/9804319","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:caf3f220a7de01c9a27c894e64db57cfa19e061f993d1ed12a9c706e36490bfd","observation_id":"463be41e-599d-429e-a06c-f307d0064fcc","resolution":{"observed_at":"2026-08-10T13:20:41.112686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0404138","last_updated":"2004-04-06T18:06:43Z","snapshot_observed_at":"2026-07-07T00:41:50.878525Z","submitted_at":"2004-04-06T18:06:43Z","title":"The ACS Virgo Cluster Survey. I. Introduction to the Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0404138","snapshot_observed_at":"2026-08-10T13:20:41.117167Z","title":"title The ACS Virgo Cluster Survey","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.117167Z"},"links":{"cited_paper":"/paper/astro-ph/0404138","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:1207a39ae4e225a41ee814e7a36bd12360c3c0081cc9e5818245077e87d55b61","observation_id":"7b743272-65d4-484b-a02d-2363ffaad25b","resolution":{"observed_at":"2026-08-10T13:20:41.117167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01311","last_updated":"2015-04-03T11:00:34Z","snapshot_observed_at":"2026-07-06T04:05:28.621052Z","submitted_at":"2015-01-06T21:00:10Z","title":"The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01311","snapshot_observed_at":"2026-08-10T13:20:41.121662Z","title":"title The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.121662Z"},"links":{"cited_paper":"/paper/1501.01311","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:f7fe4b06ccaa676450a46c93ad9569a35599275ef70f75d7343ad13485667b9c","observation_id":"ac53dfec-9d91-4966-9837-7f07dd09d0ec","resolution":{"observed_at":"2026-08-10T13:20:41.121662Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.05896","last_updated":"2015-04-22T17:37:59Z","snapshot_observed_at":"2026-07-06T04:15:45.464645Z","submitted_at":"2015-04-22T17:37:59Z","title":"Early evolution of embedded clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.05896","snapshot_observed_at":"2026-08-10T13:20:41.126048Z","title":"title Early evolution of embedded clusters","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.126048Z"},"links":{"cited_paper":"/paper/1504.05896","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:413a8e02dbbbff67eaae1e4fb98b9785564c9c75cae158b00554dcc7bef7e439","observation_id":"b6d319da-a1eb-4fd8-ad4b-6d8b9a047a94","resolution":{"observed_at":"2026-08-10T13:20:41.126048Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.06632","last_updated":"2015-02-23T21:16:27Z","snapshot_observed_at":"2026-07-06T04:10:04.095779Z","submitted_at":"2015-02-23T21:16:27Z","title":"Evidence of tidal distortions and mass loss from the old open cluster NGC 6791","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.06632","snapshot_observed_at":"2026-08-10T13:20:41.130615Z","title":"title Evidence of tidal distortions and mass-loss from the old open cluster NGC 6791","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.130615Z"},"links":{"cited_paper":"/paper/1502.06632","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:770f70fb51b35406e5c993412cfb42c488a919e556f9d6ecae6215fa8bf07a8f","observation_id":"ee42ac73-9c8e-49e5-8b8a-9b37e6011a17","resolution":{"observed_at":"2026-08-10T13:20:41.130615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.14851","last_updated":"2021-11-29T19:00:00Z","snapshot_observed_at":"2026-08-11T05:30:38.849888Z","submitted_at":"2021-11-29T19:00:00Z","title":"NGC5846-UDG1: A galaxy formed mostly by star formation in massive, extremely dense clumps of gas","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.14851","snapshot_observed_at":"2026-08-10T13:20:41.134969Z","title":"title NGC 5846-UDG1: A Galaxy Formed Mostly by Star Formation in Massive, Extremely Dense Clumps of Gas","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.134969Z"},"links":{"cited_paper":"/paper/2111.14851","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:2b97efd978d0400012b46827d337554ee4d734ef221788b78a9f0f795a420e38","observation_id":"9c212d4b-330c-404c-bb11-a5783667cc14","resolution":{"observed_at":"2026-08-10T13:20:41.134969Z","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":"2026-08-10T13:20:41.139318Z","title":"title The evolution of large-scale structure in a universe dominated by cold dark matter","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.139318Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:867ce1b9a6c2ad0df82e232fe450ad012f90d8335eebc91c1b1b8a5103425335","observation_id":"140c1f47-8512-4070-bbbe-aceaaba2f6f0","resolution":{"observed_at":"2026-08-10T13:20:41.139318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.02530","last_updated":"2024-04-11T07:06:31Z","snapshot_observed_at":"2026-07-06T15:50:45.304340Z","submitted_at":"2023-07-05T18:00:01Z","title":"On the origin of globular clusters in a hierarchical Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.02530","snapshot_observed_at":"2026-08-10T13:20:41.143820Z","title":"title On the origin of globular clusters in a hierarchical universe","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.143820Z"},"links":{"cited_paper":"/paper/2307.02530","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:c645ada85f270405ea2bb9e8ed436aefe062c050568e0aa63c3e1de7a36c44eb","observation_id":"1ad18602-a44c-433e-8b40-8600d2d527ea","resolution":{"observed_at":"2026-08-10T13:20:41.143820Z","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":"2026-08-10T13:20:41.148078Z","title":"title Space Velocities of Globular Clusters","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.148078Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:9efbc450e7215e22f94e00404075e2e73e85b81dd11f4c3de8ddaad309cbe01f","observation_id":"dee7fb3c-61ec-4451-9195-13f2a756b492","resolution":{"observed_at":"2026-08-10T13:20:41.148078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.11759","last_updated":"2022-09-23T17:59:59Z","snapshot_observed_at":"2026-07-06T13:55:41.552052Z","submitted_at":"2022-09-23T17:59:59Z","title":"Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.11759","snapshot_observed_at":"2026-08-10T13:20:41.152270Z","title":"title Modelling globular clusters in the TNG50 simulation: predictions from dwarfs to giant galaxies","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.152270Z"},"links":{"cited_paper":"/paper/2209.11759","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:79213385a562e064737b0a40d2b1636d83b6b44fd558c2f8affcf7ee495399c7","observation_id":"41a5c6fa-e124-42a2-aaab-73470468f9b6","resolution":{"observed_at":"2026-08-10T13:20:41.152270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.2469","last_updated":"2009-11-12T21:26:21Z","snapshot_observed_at":"2026-07-06T02:02:49.721823Z","submitted_at":"2009-11-12T21:26:21Z","title":"The ACS Survey of Galactic Globular Clusters. IX. Horizontal Branch Morphology and the Second Parameter Phenomenon","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.2469","snapshot_observed_at":"2026-08-10T13:20:41.156710Z","title":"title The ACS Survey of Galactic Globular Clusters","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.156710Z"},"links":{"cited_paper":"/paper/0911.2469","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:d7712d7c0b0a96258aef6e01bda0faa1d77462e7e1e82c3b9cf497ff03b4ce6d","observation_id":"b38d2a02-2937-48fe-a850-2d6a3c5e7506","resolution":{"observed_at":"2026-08-10T13:20:41.156710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.4307","last_updated":"2011-06-21T20:00:02Z","snapshot_observed_at":"2026-08-11T05:40:25.137949Z","submitted_at":"2011-06-21T20:00:02Z","title":"Globular clusters in the outer Galactic halo: new HST/ACS imaging of 6 globular clusters and the Galactic globular cluster age-metallicity relation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.4307","snapshot_observed_at":"2026-08-10T13:20:41.161256Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.161256Z"},"links":{"cited_paper":"/paper/1106.4307","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:58cf55a577b104dc1284297c01b66dd05e2c111e0e72a52040b9400f68c93bc9","observation_id":"2e69a407-5890-4516-8f3a-4f5ec77ac14c","resolution":{"observed_at":"2026-08-10T13:20:41.161256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0306026","last_updated":"2004-12-01T03:06:23Z","snapshot_observed_at":"2026-08-10T10:58:56.808238Z","submitted_at":"2003-06-02T06:33:08Z","title":"A class of compact dwarf galaxies from disruptive processes in galaxy clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0306026","snapshot_observed_at":"2026-08-10T13:20:41.166529Z","title":"title A class of compact dwarf galaxies from disruptive processes in galaxy clusters","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.166529Z"},"links":{"cited_paper":"/paper/astro-ph/0306026","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:c8e46f9d5cf245384ad2636f3cf3517e093275daa6f895c9b61230db6ee003b0","observation_id":"f31d5cfe-e356-40c1-8f41-955aed4f3ba1","resolution":{"observed_at":"2026-08-10T13:20:41.166529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.2821","last_updated":"2014-09-16T14:05:59Z","snapshot_observed_at":"2026-07-06T03:51:35.606188Z","submitted_at":"2014-08-12T19:56:55Z","title":"The Next Generation Virgo Cluster Survey. VIII. The Spatial Distribution of Globular Clusters in the Virgo Cluster","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.2821","snapshot_observed_at":"2026-08-10T13:20:41.171257Z","title":"title The Next Generation Virgo Cluster Survey","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.171257Z"},"links":{"cited_paper":"/paper/1408.2821","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:6f37e1c593b73affd50ffedfda782361c69ca15af7b479f3653585e199f33d16","observation_id":"c430150e-2dd4-4834-a717-e392c9d87f4e","resolution":{"observed_at":"2026-08-10T13:20:41.171257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.15376","last_updated":"2021-10-28T18:00:12Z","snapshot_observed_at":"2026-08-03T11:02:31.436311Z","submitted_at":"2021-10-28T18:00:12Z","title":"Clearing the hurdle: The mass of globular cluster systems as a function of host galaxy mass","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.15376","snapshot_observed_at":"2026-08-10T13:20:41.175578Z","title":"title Clearing the Hurdle: The Mass of Globular Cluster Systems as a Function of Host Galaxy Mass","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.175578Z"},"links":{"cited_paper":"/paper/2110.15376","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:9b01974789c1778fedfdb43f39b6835f7ef226a932d8314e1688d425a5baa843","observation_id":"55e5916c-675b-43bd-a818-f9c9d1043196","resolution":{"observed_at":"2026-08-10T13:20:41.175578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.03652","last_updated":"2018-11-02T16:42:24Z","snapshot_observed_at":"2026-07-06T06:38:17.165138Z","submitted_at":"2018-05-09T18:00:01Z","title":"The formation and hierarchical assembly of globular cluster populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.03652","snapshot_observed_at":"2026-08-10T13:20:41.179948Z","title":"title The formation and hierarchical assembly of globular cluster populations","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.179948Z"},"links":{"cited_paper":"/paper/1805.03652","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:84288f7c6b65ade7c35621c83cf6d867ef3088970adfd32c71e414e6faddbd9b","observation_id":"04ec1ae0-6a38-475a-9f5e-4c28dc4ae9fc","resolution":{"observed_at":"2026-08-10T13:20:41.179948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.5788","last_updated":"2007-10-31T01:09:48Z","snapshot_observed_at":"2026-07-06T01:31:41.017020Z","submitted_at":"2007-10-31T01:09:48Z","title":"Variations in Stellar Clustering with Environment: Dispersed Star Formation and the Origin of Faint Fuzzies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.5788","snapshot_observed_at":"2026-08-10T13:20:41.184392Z","title":"title Variations in Stellar Clustering with Environment: Dispersed Star Formation and the Origin of Faint Fuzzies","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.184392Z"},"links":{"cited_paper":"/paper/0710.5788","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:880a7ee08dc8991077be576801be9237a36c6d9c5e52b2f3b780baae6c402618","observation_id":"fe355963-e9dc-4e10-9eae-1365704ebde7","resolution":{"observed_at":"2026-08-10T13:20:41.184392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.0798","last_updated":"2010-03-10T18:21:31Z","snapshot_observed_at":"2026-07-31T18:32:38.380580Z","submitted_at":"2010-03-03T19:18:39Z","title":"The Globular Cluster Mass Function as a Remnant of Violent Birth","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.0798","snapshot_observed_at":"2026-08-10T13:20:41.189033Z","title":"title The Globular Cluster Mass Function as a Remnant of Violent Birth","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.189033Z"},"links":{"cited_paper":"/paper/1003.0798","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:5829d8958881125fdf9775a158447ce0bd21bb86590140c2002fed7a0e2ce860","observation_id":"e6a4d477-3538-4627-b3e6-1afebf80d936","resolution":{"observed_at":"2026-08-10T13:20:41.189033Z","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":"2026-08-10T13:20:41.193476Z","title":"title A Universal Formation Mechanism for Open and Globular Clusters in Turbulent Gas","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.193476Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:5b9e04a76e3666a4ff8eab08bc8f1afa416c3633fd12fbad6c8fa1752e70954b","observation_id":"57203891-8f90-4774-8bdb-7a0c4b652b56","resolution":{"observed_at":"2026-08-10T13:20:41.193476Z","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":"2026-08-10T13:20:41.197947Z","title":"title A Fractal Origin for the Mass Spectrum of Interstellar Clouds","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.197947Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:8a57c8e9373cdb484219f1c9f16a575a0e4d21a99363abaaaf9550363efd3fcc","observation_id":"08ce0d5b-8696-440c-aeab-797ac2ebcfdf","resolution":{"observed_at":"2026-08-10T13:20:41.197947Z","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":"2026-08-10T13:20:41.202885Z","title":"title A theory for the origin of globular clusters","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.202885Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:139946f1df3de4585bbea980e8c05a2a686961552fa476d3110d408581e3ac73","observation_id":"17a7da62-a4f6-4ab5-9c9b-37e73d12a98b","resolution":{"observed_at":"2026-08-10T13:20:41.202885Z","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":"2026-08-10T13:20:41.207395Z","title":"title Dynamical Evolution of the Mass Function of Globular Star Clusters","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.207395Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:02073fa72a50007a9c2287f54a6f97f0111be24575a9a300c80d3e2ee89834b8","observation_id":"a79bf6c9-c30d-4b88-9314-f9308a50a01b","resolution":{"observed_at":"2026-08-10T13:20:41.207395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0905.1060","last_updated":"2010-04-13T19:01:47Z","snapshot_observed_at":"2026-07-06T01:53:55.948483Z","submitted_at":"2009-05-07T16:56:01Z","title":"Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.1060","snapshot_observed_at":"2026-08-10T13:20:41.211891Z","title":"title Comparing the statistics of interstellar turbulence in simulations and observations","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.211891Z"},"links":{"cited_paper":"/paper/0905.1060","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:d7fb2d603313048fc9cfbb7bad1630ef646669d76920b09a7c5bc81be4a5d963","observation_id":"2423148c-ab11-49a1-b5d8-982d26d86b61","resolution":{"observed_at":"2026-08-10T13:20:41.211891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.01512","last_updated":"2020-02-04T19:31:26Z","snapshot_observed_at":"2026-07-06T08:54:55.249405Z","submitted_at":"2020-02-04T19:31:26Z","title":"Reverse engineering the Milky Way","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.01512","snapshot_observed_at":"2026-08-10T13:20:41.216420Z","title":"title Reverse engineering the Milky Way","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.216420Z"},"links":{"cited_paper":"/paper/2002.01512","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:23bdd9ac5900035dbb34437d8f7ab4c92c9137cc7ce8ca024c59c75daae77c3a","observation_id":"f5e7a9c1-a3eb-4abe-b59a-b5e24470b478","resolution":{"observed_at":"2026-08-10T13:20:41.216420Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9702146","last_updated":"1997-02-17T19:08:34Z","snapshot_observed_at":"2026-07-07T01:15:55.239042Z","submitted_at":"1997-02-17T19:08:34Z","title":"On the Origin of Globular Cluster Systems in Elliptical and cD Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9702146","snapshot_observed_at":"2026-08-10T13:20:41.225201Z","title":"title On the Origin of Globular Clusters in Elliptical and cD Galaxies","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.225201Z"},"links":{"cited_paper":"/paper/astro-ph/9702146","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:f12bf5c08626f5c7ae385d2a87ae2d82bd4a26fca6bb3b3be416e40d8d4bb5fd","observation_id":"aed8d4c3-5f38-4406-a444-4916de286622","resolution":{"observed_at":"2026-08-10T13:20:41.225201Z","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":"2026-08-10T13:20:41.230096Z","title":"title Globular cluster formation and evolution in the context of cosmological galaxy assembly: open questions","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.230096Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:6eaf7fdd3559758c47e4237298701aef0b0c40c249042a52403923597e270995","observation_id":"b48cd00c-ba4a-44ae-b215-c17a425b72b9","resolution":{"observed_at":"2026-08-10T13:20:41.230096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.07831","last_updated":"2018-09-20T20:01:05Z","snapshot_observed_at":"2026-07-06T07:03:25.568025Z","submitted_at":"2018-09-20T20:01:05Z","title":"Extending the Globular Cluster System-Halo Mass Relation to the Lowest Galaxy Masses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.07831","snapshot_observed_at":"2026-08-10T13:20:41.234528Z","title":"title Extending the globular cluster system-halo mass relation to the lowest galaxy masses","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.234528Z"},"links":{"cited_paper":"/paper/1809.07831","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:85d94878c30d34c55c5f4b60f1976d98cdf40c1cab57c98bcbceaa73d833cb30","observation_id":"6b7e3fe2-e713-48ae-9212-1f48b4d2428f","resolution":{"observed_at":"2026-08-10T13:20:41.234528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.1434","last_updated":"2012-05-07T15:42:27Z","snapshot_observed_at":"2026-08-01T20:22:11.473306Z","submitted_at":"2012-05-07T15:42:27Z","title":"The formation of young dense star clusters through mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.1434","snapshot_observed_at":"2026-08-10T13:20:41.239658Z","title":"title The Formation of Young Dense Star Clusters through Mergers","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.239658Z"},"links":{"cited_paper":"/paper/1205.1434","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:f48709798e001a6b08c3f4aa4d4af81935c57a0b6d447ba82179f15b19d7ff6f","observation_id":"e68aebd2-7334-4e61-aa34-7d2606620fe3","resolution":{"observed_at":"2026-08-10T13:20:41.239658Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.18543","last_updated":"2025-03-25T19:58:38Z","snapshot_observed_at":"2026-08-09T03:21:09.394972Z","submitted_at":"2024-02-28T18:27:39Z","title":"Primordial Rotating Disk Composed of $\\geq$15 Dense Star-Forming Clumps at Cosmic Dawn","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.18543","snapshot_observed_at":"2026-08-10T13:20:41.244947Z","title":"title Primordial Rotating Disk Composed of 15 Dense Star-Forming Clumps at Cosmic Dawn doi doi:10.48550/arXiv.2402.18543","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.244947Z"},"links":{"cited_paper":"/paper/2402.18543","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:0d47afa8890be7a0d90bf9641965268692c43aa39526ea0d3b5c879317de5dce","observation_id":"cefc1fc7-6697-4ac2-9808-17f2db65fbe9","resolution":{"observed_at":"2026-08-10T13:20:41.244947Z","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":"2026-08-10T13:20:41.250360Z","title":"title The time-scale of escape from star clusters","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.250360Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:a4e8e794f20d20309625e413bc0b4c508bd2eaed8d3bfb882a8562a65dab156a","observation_id":"fcdb39f5-5698-4d8c-8b13-fda1ea3f0936","resolution":{"observed_at":"2026-08-10T13:20:41.250360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.09381","last_updated":"2020-11-22T21:26:00Z","snapshot_observed_at":"2026-08-10T08:06:24.344430Z","submitted_at":"2018-04-25T06:25:31Z","title":"Gaia Data Release 2: Kinematics of globular clusters and dwarf galaxies around the Milky Way","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.09381","snapshot_observed_at":"2026-08-10T13:20:41.254722Z","title":"title Gaia Data Release 2","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.254722Z"},"links":{"cited_paper":"/paper/1804.09381","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:70870535b4123219fcb893dad033ed89696c767c61e8ac24291ec3d24aa73f59","observation_id":"cba28de9-8a8f-4544-a91c-8859aae2614c","resolution":{"observed_at":"2026-08-10T13:20:41.254722Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.3154","last_updated":"2009-07-07T14:27:13Z","snapshot_observed_at":"2026-07-06T01:49:35.157155Z","submitted_at":"2008-12-16T21:02:33Z","title":"The halo merger rate in the Millennium Simulation and implications for observed galaxy merger fractions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.3154","snapshot_observed_at":"2026-08-10T13:20:41.259465Z","title":"title The Halo Merger Rate in the Millennium Simulation and Implications for Observed Galaxy Merger Fractions","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.259465Z"},"links":{"cited_paper":"/paper/0812.3154","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:fb6b64dc3ffdcecfb485f2535ad35ee7b5fcda452d7dfdd2e7d52aa35af51886","observation_id":"f00c573b-4293-47cd-a655-fd82929163b0","resolution":{"observed_at":"2026-08-10T13:20:41.259465Z","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":"2026-08-10T13:20:41.267899Z","title":"title The early evolution of the star cluster mass function","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.267899Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:b390effd680602cd218d25e8d97c29574946d623ae8df180720db32ede8a6930","observation_id":"e36ac84e-0498-4e93-bc35-febe5c1854f3","resolution":{"observed_at":"2026-08-10T13:20:41.267899Z","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":"2026-08-10T13:20:41.271907Z","title":"title Lifetimes of tidally limited star clusters with different radii","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.271907Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:daa2b4b8774ba39fe5daadc1fd7da0510fd22353358cd110707254d8ed12a0c2","observation_id":"de1e0230-9086-47e0-92c3-968fa27191cf","resolution":{"observed_at":"2026-08-10T13:20:41.271907Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.03791","last_updated":"2023-04-26T19:01:02Z","snapshot_observed_at":"2026-07-06T14:59:39.238136Z","submitted_at":"2023-03-07T10:59:51Z","title":"The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.03791","snapshot_observed_at":"2026-08-10T13:20:41.276349Z","title":"title The mass-loss rates of star clusters with stellar-mass black holes: implications for the globular cluster mass function","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.276349Z"},"links":{"cited_paper":"/paper/2303.03791","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:164d25ef5745e61af1a7b9f2d23738131e2a495cea342fbab589c7bf8f7f080f","observation_id":"e8b25d0c-0055-4b2f-830c-7de256f2e4e4","resolution":{"observed_at":"2026-08-10T13:20:41.276349Z","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":"2026-08-10T13:20:41.289252Z","title":"title The effect of spiral arm passages on the evolution of stellar clusters","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.289252Z"},"links":{"citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:07d4fc75f43b473fe4bba9adea04405c49a8d2924535d35fd3075705a4d86f73","observation_id":"5d185bd1-92d5-49ec-9bc4-065952f28028","resolution":{"observed_at":"2026-08-10T13:20:41.289252Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.05642","last_updated":"2018-01-17T12:48:20Z","snapshot_observed_at":"2026-07-06T06:19:03.187654Z","submitted_at":"2018-01-17T12:48:20Z","title":"A detached stellar-mass black hole candidate in the globular cluster NGC 3201","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.05642","snapshot_observed_at":"2026-08-10T13:20:41.293309Z","title":"title A detached stellar-mass black hole candidate in the globular cluster NGC 3201","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":107,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.293309Z"},"links":{"cited_paper":"/paper/1801.05642","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:b92f76cf5665a376d575601ddce43e62c561c9a2d30dac1acb2a18bd2f872bf4","observation_id":"05bdc659-3330-47c0-838a-c408e771fe18","resolution":{"observed_at":"2026-08-10T13:20:41.293309Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.06616","last_updated":"2019-02-21T23:00:28Z","snapshot_observed_at":"2026-07-06T06:56:30.962909Z","submitted_at":"2018-08-20T18:00:02Z","title":"A high cluster formation efficiency in the Sagittarius B2 complex","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.06616","snapshot_observed_at":"2026-08-10T13:20:41.298058Z","title":"title A High Cluster Formation Efficiency in the Sagittarius B2 Complex","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":108,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.298058Z"},"links":{"cited_paper":"/paper/1808.06616","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:77cb296979337cedf6a2051b4a8d9d30bba10ac74a686d4acafb41f4445c4f40","observation_id":"182e895f-7018-422a-aee8-f5d321f104b9","resolution":{"observed_at":"2026-08-10T13:20:41.298058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09402","last_updated":"2016-06-19T17:43:55Z","snapshot_observed_at":"2026-08-08T15:21:20.985976Z","submitted_at":"2016-05-30T20:10:31Z","title":"Toward gas exhaustion in the W51 high-mass protoclusters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.09402","snapshot_observed_at":"2026-08-10T13:20:41.302511Z","title":"title Toward gas exhaustion in the W51 high-mass protoclusters","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":109,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.302511Z"},"links":{"cited_paper":"/paper/1605.09402","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:94b259ef7610fe0b4ce421fcc20d29d7e6169cd30e4a135ff3dba710da1c2680","observation_id":"fca6be3e-7972-47cc-845d-75cab5832e4f","resolution":{"observed_at":"2026-08-10T13:20:41.302511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9603042","last_updated":"1996-03-12T04:20:13Z","snapshot_observed_at":"2026-08-09T09:06:45.988808Z","submitted_at":"1996-03-12T04:20:13Z","title":"Destruction of the Galactic Globular Cluster System","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9603042","snapshot_observed_at":"2026-08-10T13:20:41.311486Z","title":"title Destruction of the Galactic Globular Cluster System","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":111,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.311486Z"},"links":{"cited_paper":"/paper/astro-ph/9603042","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:d84c38c00e28e99bc87d5d45b5533ad7b938fd1516b626a77d779a72cbe5d376","observation_id":"7928f780-0c58-4653-9649-7bb7f6da8882","resolution":{"observed_at":"2026-08-10T13:20:41.311486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9806245","last_updated":"1999-05-18T14:20:39Z","snapshot_observed_at":"2026-07-31T13:01:28.188632Z","submitted_at":"1998-06-18T00:11:17Z","title":"Effects of Tidal Shocks on the Evolution of Globular Clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9806245","snapshot_observed_at":"2026-08-10T13:20:41.316182Z","title":"title Effects of Tidal Shocks on the Evolution of Globular Clusters","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters","version":1},"reference_index":112,"source":"arxiv_source","source_observed_at":"2026-08-10T13:20:41.316182Z"},"links":{"cited_paper":"/paper/astro-ph/9806245","citing_paper":"/paper/2501.16438"},"observation_digest":"sha256:e927c40c44e286486f82411eb257c06bf0dc3b644d5078f32c77f98578eaa4a1","observation_id":"152eee4f-0769-4221-b786-9c2711f53002","resolution":{"observed_at":"2026-08-10T13:20:41.316182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2501.16438","last_updated":"2025-01-27T19:00:24Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-11T05:08:02.321729Z","submitted_at":"2025-01-27T19:00:24Z","title":"The Formation of Globular Clusters"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":280},"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 280 outbound references and 8 inbound Pith citation observations for arXiv:2501.16438."}