{"as_of":"2026-08-12T12:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ffafd8079d72d7ea00360bf32d6bea72929c6c7e43f84a2abdeea5717b4efe03","coverage":[{"denominator":109,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T20:03:51.136801Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2412.06155/citation-record","integrity":"/paper/2412.06155/integrity","json":"/paper/2412.06155/citation-record.json","paper":"/paper/2412.06155"},"outbound":[{"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":"2026-08-11T20:03:50.739583Z","title":"arXiv:2401.03224","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.739583Z"},"links":{"cited_paper":"/paper/2401.03224","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:5766726b19aeb8c9eceba27629b4d432ed84f5f4ce66dd57e05c2395951960ee","observation_id":"5db4efd9-8fc3-4feb-8e72-96880e7dc49e","resolution":{"observed_at":"2026-08-11T20:03:50.739583Z","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":"2026-08-11T20:03:50.744732Z","title":"P., 1988, @doi [ ] 10.1086/166961 , https://ui.adsabs.harvard.edu/abs/1988ApJ...335..720A 335, 720","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.744732Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:424a39d83e8b2d767cacb3dc009a4d797c701e882862d61b34cb8f4c6493fb5c","observation_id":"dd6a2187-ed57-4304-a082-1655335d3bcc","resolution":{"observed_at":"2026-08-11T20:03:50.744732Z","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":"2026-08-11T20:03:50.750371Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.750371Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:654f88c5d91ae2af35e60e60d6ca1bb02c0113b5083dd724e5d3204194293bb4","observation_id":"ca2ff86c-0385-4389-b364-d21592f84eb7","resolution":{"observed_at":"2026-08-11T20:03:50.750371Z","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":"2026-08-11T20:03:50.755559Z","title":"C., Loeb A., 2016, @doi [ ] 10.1093/mnrasl/slw055 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.459L..51A 459, L51","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.755559Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:ea7ef998e9af71190be22a97db43d048a5b125207ff77cf971d0f24bf7dbd2e3","observation_id":"356e7239-a224-4d15-b82c-8039143214f0","resolution":{"observed_at":"2026-08-11T20:03:50.755559Z","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":"2026-08-11T20:03:50.759727Z","title":"A., Romanowsky A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.759727Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:671ac8c6ed0b532f820dc5df6c77411614ef265d8be0d236d972aa9201655380","observation_id":"a9c607f7-d9a9-4032-ba96-6e9b43239539","resolution":{"observed_at":"2026-08-11T20:03:50.759727Z","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":"2026-08-11T20:03:50.763946Z","title":"A., et al., 2021, @doi [Nature Astronomy] 10.1038/s41550-021-01458-1 , https://ui.adsabs.harvard.edu/abs/2021NatAs...5.1255B 5, 1255","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.763946Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:5e173c5a021db5f359e10761df5d5eb4294a541fddc7371bc83922b9dc93ae56","observation_id":"cd1e090a-1607-4346-9d31-7233cb3b7bef","resolution":{"observed_at":"2026-08-11T20:03:50.763946Z","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":"2026-08-11T20:03:50.769298Z","title":"A., 2020, @doi [ ] 10.3847/1538-3881/ab5b0e , https://ui.adsabs.harvard.edu/abs/2020AJ....159...56B 159, 56","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.769298Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:33dcbb63acfa7cbd26ebeed1562535bd0a439bd0c2e0478f295e2ec4aacd493c","observation_id":"c9c80fad-1950-4486-bad2-21fa4ae3728b","resolution":{"observed_at":"2026-08-11T20:03:50.769298Z","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":"2026-08-11T20:03:50.773576Z","title":"L., et al., 2022, @doi [ ] 10.1093/mnras/stac2442 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517.2231B 517, 2231","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.773576Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:3cded03ea4a347f19a1e0e577fa2903c58a38ca32930bd24c59c005290b2892a","observation_id":"27714572-b97e-4f8b-8c45-718892e14db4","resolution":{"observed_at":"2026-08-11T20:03:50.773576Z","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":"2026-08-11T20:03:50.777130Z","title":"L., et al., 2024, @doi [ ] 10.1093/mnras/stae564 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.529.3210B 529, 3210","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.777130Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:fffdfd43cf7a3ad31cb8ad0d22e2284017796b0f73983d3e004afa1b231b27a5","observation_id":"a1ead537-7c5e-46e0-98e9-512c8a49bdd9","resolution":{"observed_at":"2026-08-11T20:03:50.777130Z","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":"2026-08-11T20:03:50.780663Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.780663Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:e4a6ec7c358effc4d7ef5267e79bde09735d3ab69d5e5ab2645662af3195c38a","observation_id":"2475e66a-b1a1-477f-a89b-6ca2f60dede0","resolution":{"observed_at":"2026-08-11T20:03:50.780663Z","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":"2026-08-11T20:03:50.784095Z","title":"Y., 2023, @doi [ ] 10.1093/mnras/stad1328 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.522.5638C 522, 5638","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.784095Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:cb7f3bde8c066cb5f627b11f55ddda5cd6aba262d74ee66b0a3340cbe9d73796","observation_id":"95755ca8-a1ce-4b8c-9d36-0a042ecbc60b","resolution":{"observed_at":"2026-08-11T20:03:50.784095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18735","last_updated":"2025-06-23T05:35:28Z","snapshot_observed_at":"2026-08-01T16:11:15.370791Z","submitted_at":"2024-05-29T03:32:06Z","title":"A two-phase model of galaxy formation: III. The formation of globular clusters","version":3},"cited_work":{"arxiv_id":"2405.18735","doi":"10.48550/arxiv.2405.18735","metadata_source":"pith","pith_arxiv_id":"2405.18735","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"A two-phase model of galaxy formation: III. The formation of globular clusters","venue":"astro-ph.GA","work_id":"eeb2030a-3092-4f33-96d0-95940aee46fb","year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.787759Z"},"links":{"cited_paper":"/paper/2405.18735","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:476e3b5757d64e24d1e86e21591ba221bbc9b560ad55c7fabd6e8c7feafe81d0","observation_id":"b74800ab-9bbc-47e1-9a86-ec6716e14bd1","resolution":{"observed_at":"2026-08-11T20:08:38.376695Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:50.791061Z","title":"V., Afanasiev A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.791061Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:c6b30e1392e978d339a741261b600aa8ac50528dc8929937d95bed71d0127e3f","observation_id":"adf82002-0bf8-487f-a731-3d6b41c4865c","resolution":{"observed_at":"2026-08-11T20:03:50.791061Z","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":"2026-08-11T20:03:50.794170Z","title":"Y., 2019, @doi [ ] 10.1093/mnras/stz2097 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.488.5409C 488, 5409","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.794170Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:8a3b75f5207e7da70c36a57a3fa3c3ac99101f4da98dacbb3d89a562fc1855a1","observation_id":"9e1fae24-a33a-465f-b5f5-f2d2e600d946","resolution":{"observed_at":"2026-08-11T20:03:50.794170Z","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":"2026-08-11T20:03:50.804111Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.804111Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:2071c753b119484b469105f444b5ec9593a51f498ac42b3856ee42d020e6e642","observation_id":"b947b738-090f-4ef2-a39e-dfcd059ae076","resolution":{"observed_at":"2026-08-11T20:03:50.804111Z","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":"2026-08-11T20:03:50.808388Z","title":"J., 2019, @doi [ApJL] 10.3847/2041-8213/ab0e8c , https://ui.adsabs.harvard.edu/abs/2019ApJ...874L..12D 874, L12","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.808388Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:f76c56706e2356cede2980b5dd88645b39155142e30cd5df3e2ee91593ad7575","observation_id":"800d9f04-231f-4677-9d74-81e06cd60c42","resolution":{"observed_at":"2026-08-11T20:03:50.808388Z","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":"2026-08-11T20:03:50.811976Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.811976Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:9790fb56bec91df2082d6391adda27d8d6de44da6d13c8ca41e02697711f22b7","observation_id":"661cf5b5-a984-40fc-9b81-501c6e416b03","resolution":{"observed_at":"2026-08-11T20:03:50.811976Z","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":"2026-08-11T20:03:50.815832Z","title":"B., Dutton A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.815832Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:e49c8f0689c4008579565e5843a5889c6c16fec156f604601d3a520679aafdd1","observation_id":"7eff273c-789b-44df-a7a8-a60c375981d4","resolution":{"observed_at":"2026-08-11T20:03:50.815832Z","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":"2026-08-11T20:03:50.819403Z","title":"E., et al., 2023, @doi [ ] 10.1093/mnras/stac2818 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.2453D 518, 2453","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.819403Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:5ea2430f46aa0c4c37ca8348bc8d492224ecf418c1c7ff57f9788f6e8707ee84","observation_id":"498e0a7b-2ea2-4921-8006-c69c32b1e205","resolution":{"observed_at":"2026-08-11T20:03:50.819403Z","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":"2026-08-11T20:03:50.823198Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.823198Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:2ac78dc0dfaf9256115425cc4f7e24d4431664ffee1d8ec37fe01aaa63e0e7f1","observation_id":"c856eeb4-c482-493a-9398-6ab58710d83e","resolution":{"observed_at":"2026-08-11T20:03:50.823198Z","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":"2026-08-11T20:03:50.826868Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.826868Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:24eba16b97b0ee2027ebd3a8f401d948021418502fc7920c513504ef97ce9a19","observation_id":"99dd77f8-58ca-431b-b7fc-0489482f6f58","resolution":{"observed_at":"2026-08-11T20:03:50.826868Z","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":"2026-08-11T20:03:50.830808Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.830808Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:7970485498a0ea8b48a6fc547c651ed9e7d826b93a650681f67173342b30f4a1","observation_id":"c42d6738-f96e-4ce7-a0d5-4c6c8e7e489d","resolution":{"observed_at":"2026-08-11T20:03:50.830808Z","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":"2026-08-11T20:03:50.834145Z","title":"S., Forbes D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.834145Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:c638739a5ec85f5cab102bec5e622e16db7a101b26d582580343dcdcacce685b","observation_id":"6a324403-a595-4f5f-bccd-5155c5ae5e4b","resolution":{"observed_at":"2026-08-11T20:03:50.834145Z","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":"2026-08-11T20:03:50.838734Z","title":"E., Jones M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.838734Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:068dad98f5316ccb007f6e49caf09b76f7dcf6e734af99096ebded04e016fd17","observation_id":"70c1c393-ea4d-43a3-8b1c-ab1224244ae7","resolution":{"observed_at":"2026-08-11T20:03:50.838734Z","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":"2026-08-11T20:03:50.842408Z","title":"A., 2017, @doi [ ] 10.1093/mnrasl/slx148 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.472L.104F 472, L104","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.842408Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:d08ecb0dda3f460b553744c7b6836ef2f262be844a8a285407b9cc2a56bedffb","observation_id":"dedb0409-936a-464b-a52a-3ff659aa842f","resolution":{"observed_at":"2026-08-11T20:03:50.842408Z","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":"2026-08-11T20:03:50.845944Z","title":"A., Gannon J., 2024, @doi [ ] 10.1093/mnras/stad4004 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.528..608F 528, 608","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.845944Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:92ce3d546b093a4ebd4eb892f5989e6decf326889e3c9bd0c8468ee0c38be2a7","observation_id":"6d687a54-7170-49a7-a6ca-10319b333404","resolution":{"observed_at":"2026-08-11T20:03:50.845944Z","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":"2026-08-11T20:03:50.849414Z","title":"A., et al., 2018a, @doi [Proceedings of the Royal Society of London Series A] 10.1098/rspa.2017.0616 , https://ui.adsabs.harvard.edu/abs/2018RSPSA.47470616F 474, 20170616","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.849414Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:db89a8feab480cc7fbceab11f15c566a6f97cb0db4baba0c04f24de2a5392143","observation_id":"f4927205-3917-464e-a6f1-a15b94805b6c","resolution":{"observed_at":"2026-08-11T20:03:50.849414Z","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":"2026-08-11T20:03:50.852986Z","title":"A., Read J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.852986Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:044833219f470b0a003e4de23f0e2b59e5355f4962c6e2097cdfc7717b771955","observation_id":"fd0c3277-f32c-4021-9a3d-550868cbd30b","resolution":{"observed_at":"2026-08-11T20:03:50.852986Z","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":"2026-08-11T20:03:50.856411Z","title":"A., Alabi A., Romanowsky A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.856411Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:6c2f552df6abc865f53e6f8eb194b7cb411942f761a007f02151161a75de40cd","observation_id":"8a6828ae-32ee-4b2a-a2de-46adda8ad8f2","resolution":{"observed_at":"2026-08-11T20:03:50.856411Z","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":"2026-08-11T20:03:50.860450Z","title":"A., Gannon J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.860450Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:7beb2130497cf3184993a8d45b9ea3edbc913908c3cc22315f50d3add8032c3a","observation_id":"10d3f105-385a-490a-bae8-6ddfd7d4828d","resolution":{"observed_at":"2026-08-11T20:03:50.860450Z","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":"2026-08-11T20:03:50.864492Z","title":"A., et al., 2023, @doi [ ] 10.1093/mnrasl/slad101 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.525L..93F 525, L93","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.864492Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:b90649cbfe3589483c99cf5a989857e749a16372625d927922e4aa9fbb15515d","observation_id":"09c6ef7e-b68d-416d-a09e-d8c3817dc83a","resolution":{"observed_at":"2026-08-11T20:03:50.864492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.11749","last_updated":"2024-05-20T03:20:30Z","snapshot_observed_at":"2026-07-06T18:16:33.179338Z","submitted_at":"2024-05-20T03:20:30Z","title":"Keck/KCWI Spectroscopy of Globular Clusters in Local Volume Dwarf Galaxies","version":1},"cited_work":{"arxiv_id":"2405.11749","doi":"10.48550/arxiv.2405.11749","metadata_source":"pith","pith_arxiv_id":"2405.11749","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"Keck/KCWI Spectroscopy of Globular Clusters in Local Volume Dwarf Galaxies","venue":"astro-ph.GA","work_id":"6e94b1d9-cfd7-410b-9af1-dc400e2374ed","year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.868715Z"},"links":{"cited_paper":"/paper/2405.11749","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:8cf70b855fb3078cd44c1ed0a76f5ba3cbd166a6a14237da4fc84f65bdbad604","observation_id":"d8cc13a7-5950-4736-81c2-32236b3fd31a","resolution":{"observed_at":"2026-08-11T20:03:52.200431Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-08-11T20:03:50.872890Z","title":"arXiv:2402.18543","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.872890Z"},"links":{"cited_paper":"/paper/2402.18543","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:89fdc3d0c7056087ec0b06d14103708fb636851df314bda212b0931d92d6fba2","observation_id":"3d3e240d-ea90-4a24-82c5-8058a492dfc1","resolution":{"observed_at":"2026-08-11T20:03:50.872890Z","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":"2026-08-11T20:03:50.877403Z","title":"S., Forbes D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.877403Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:803de5f724c46ee6467d48052100e7ac6722bd8e0fc840018c14cb76a908fe33","observation_id":"b25dc3df-efcc-4faa-a867-63f69b2cc4f6","resolution":{"observed_at":"2026-08-11T20:03:50.877403Z","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":"2026-08-11T20:03:50.881110Z","title":"S., et al., 2021, @doi [ ] 10.1093/mnras/stab277 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.3144G 502, 3144","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.881110Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:6fd8e531b8c75d486fa3fd272e2ac5bffc7eea81e919b92596594692a1d8d75e","observation_id":"9a5725f1-9eba-47bd-b38f-3f64facab50c","resolution":{"observed_at":"2026-08-11T20:03:50.881110Z","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":"2026-08-11T20:03:50.888454Z","title":"S., et al., 2022b, @doi [MNRAS] 10.1093/mnras/stab3297 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.510..946G 510, 946","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.888454Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:c260225244f8a1570a6a9bc03d455bfb2c84b1490cf68b184075b252d8b46d95","observation_id":"ec8b223c-39c1-4567-9cee-6a14c4203742","resolution":{"observed_at":"2026-08-11T20:03:50.888454Z","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":"2026-08-11T20:03:50.891795Z","title":"S., Forbes D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.891795Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:88ce6d1c4b7159270a229dd506ac59d6c2ba19bbfee437bf8e6e0e818cf1da04","observation_id":"a437c584-96eb-4abb-adf3-be021db0f594","resolution":{"observed_at":"2026-08-11T20:03:50.891795Z","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":"2026-08-11T20:03:50.895233Z","title":"S., Ferr \\'e -Mateu A., Forbes D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.895233Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:554e4159b62e7b2b4b22e1a1412e35fc715740e12461e39b780808b5e1fdc250","observation_id":"5564f46d-66c5-4b64-8685-31b64a08a488","resolution":{"observed_at":"2026-08-11T20:03:50.895233Z","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":"2026-08-11T20:03:50.898703Z","title":"Y., Puzia T","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.898703Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:045ce3353fe1df0437922f181d93665c7c20348df1ae1bd6d574a13963ac67fa","observation_id":"8280c39c-54bd-468c-8114-f866a384c2c9","resolution":{"observed_at":"2026-08-11T20:03:50.898703Z","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":"2026-08-11T20:03:50.905774Z","title":"Y., Ostriker J","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.905774Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:a1f3f7d5f3e93bf2fa2550b242abd46c7661f87dcea9b2abb0639f0d74e1de65","observation_id":"6e1ee900-b2f9-409a-89f7-fd0fcfb385e0","resolution":{"observed_at":"2026-08-11T20:03:50.905774Z","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":"2026-08-11T20:03:50.909313Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.909313Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:ac430b8b217ff3676c2aa2aec5c20636d1ad57bcf4ae1f405259409589de6c6b","observation_id":"d4371183-eb45-4186-a1ce-1cce16ce0966","resolution":{"observed_at":"2026-08-11T20:03:50.909313Z","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":"2026-08-11T20:03:50.912850Z","title":"E., Harris G","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.912850Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:ae167bf2e1486a8ae55b441955501afebff773de8807cfe821214f9cdd46ced0","observation_id":"a892b0d1-3b25-48a2-b1fc-5f098bc5bcfd","resolution":{"observed_at":"2026-08-11T20:03:50.912850Z","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":"2026-08-11T20:03:50.917011Z","title":"E., Blakeslee J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.917011Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:588e85e50678e49398a9055f0b51c7625342d351495ced115b429e11391920a4","observation_id":"01816e62-3b80-46bb-969e-8865ae81da60","resolution":{"observed_at":"2026-08-11T20:03:50.917011Z","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":"2026-08-11T20:03:50.921641Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.921641Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:b9d50a49332d82746307266fedef80ab8579ead02fcc127dbb6c77e11bc03bb9","observation_id":"4f3aa98f-7c03-4587-a538-ade01a4647e2","resolution":{"observed_at":"2026-08-11T20:03:50.921641Z","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":"2026-08-11T20:03:50.926023Z","title":"E., 2021, @doi [ ] 10.1093/mnras/staa3297 , https://ui.adsabs.harvard.edu/abs/2021MNRAS.500..986H 500, 986","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.926023Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:9a943edcbc7cb5428ce9a90283c492509861e95f3b379ff570ae47f334df57f5","observation_id":"bee28f98-fbcc-415b-91b6-303dc801b510","resolution":{"observed_at":"2026-08-11T20:03:50.926023Z","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":"2026-08-11T20:03:50.930364Z","title":"J., Robison B., 2018, @doi [ ] 10.1093/mnras/sty844 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.3869H 477, 3869","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.930364Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:21e217a66c906c4a784c4671d406f7b7ef372389654913483cdb7a48c030b4e0","observation_id":"f221188a-8e4a-44b7-9c3f-32982a68cdfe","resolution":{"observed_at":"2026-08-11T20:03:50.930364Z","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":"2026-08-11T20:03:50.934282Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.934282Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:e50307917147198473ffcf3df7ceb974996dbc73b2136d2290990d52089dba10","observation_id":"57cfba2c-7a31-4793-a4b5-bf5bec6e8f6a","resolution":{"observed_at":"2026-08-11T20:03:50.934282Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.11493","last_updated":"2023-08-22T15:16:37Z","snapshot_observed_at":"2026-07-06T16:09:05.106099Z","submitted_at":"2023-08-22T15:16:37Z","title":"Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra-I cluster.I. Project description and preliminary results","version":1},"cited_work":{"arxiv_id":"2308.11493","doi":"10.48550/arxiv.2308.11493","metadata_source":"pith","pith_arxiv_id":"2308.11493","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra-I cluster.I. Project description and preliminary results","venue":"astro-ph.GA","work_id":"da0f1400-b47c-4c92-a67e-89fb93a43168","year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.938359Z"},"links":{"cited_paper":"/paper/2308.11493","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:40c183fb691dd66213be9d826620d21236ca8d9989ece5250e65046b752a6253","observation_id":"976f4a12-1fea-442f-bfed-4197674f094e","resolution":{"observed_at":"2026-08-11T20:03:52.033031Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:50.942895Z","title":"R., Abraham R., Brodie J., Forbes D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.942895Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:afc38cdac2ceed9420f473fea55bd3e63fbf1957cba384fed9a5b96b8f7b5f55","observation_id":"dfce7060-f625-401d-8f7c-4d9bd1c4543a","resolution":{"observed_at":"2026-08-11T20:03:50.942895Z","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":"2026-08-11T20:03:50.946754Z","title":"R., et al., 2022, @doi [ ] 10.1093/mnras/stac2717 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.517..858J 517, 858","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.946754Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:5e95263bf9d30fb12d071488bbe324f0c60b15d03a09c7c036b200d626d54c29","observation_id":"5febb994-392a-45ed-9955-baf59188dd3b","resolution":{"observed_at":"2026-08-11T20:03:50.946754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.07518","last_updated":"2024-09-11T18:00:02Z","snapshot_observed_at":"2026-08-09T16:12:09.150556Z","submitted_at":"2024-09-11T18:00:02Z","title":"The PIPER Survey. II. The Globular Cluster Systems of Low Surface Brightness Galaxies in the Perseus Cluster","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.07518","snapshot_observed_at":"2026-08-11T20:03:50.950498Z","title":"R., et al., 2024, @doi [arXiv e-prints] 10.48550/arXiv.2409.07518 , https://ui.adsabs.harvard.edu/abs/2024arXiv240907518J p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.950498Z"},"links":{"cited_paper":"/paper/2409.07518","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:a47fd6fa43e6c8c594cc3fbae8f65a3c455f87ac0bb042d0640b716a27f308ba","observation_id":"74e19ee8-7066-4a7e-a499-e1fbe7b0c1ef","resolution":{"observed_at":"2026-08-11T20:03:50.950498Z","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":"2026-08-11T20:03:50.955655Z","title":"P., et al., 2021, @doi [ ] 10.3847/1538-4357/ac1869 , https://ui.adsabs.harvard.edu/abs/2021ApJ...921...32J 921, 32","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.955655Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:e5be2c21a62de39f6f60618d67d07b23ae65ff2b7b29b0501e721a036eab1468","observation_id":"39845c04-c95c-489e-b76a-38d1f1406017","resolution":{"observed_at":"2026-08-11T20:03:50.955655Z","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":"2026-08-11T20:03:50.959177Z","title":"J., Dutton A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.959177Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:a848b528fa99e9b3fef69bb6db52c1b030d823f39e35b690aac5797b84d481ed","observation_id":"02d569a8-0cc3-438b-9e92-edb41333c9e0","resolution":{"observed_at":"2026-08-11T20:03:50.959177Z","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":"2026-08-11T20:03:50.964248Z","title":"G., et al., 2023, @doi [ ] 10.3847/2041-8213/acaaab , https://ui.adsabs.harvard.edu/abs/2023ApJ...942L...5J 942, L5","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.964248Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:3d1e5940b39a63dd03bcaa965e37f0084ba5e069acd5aab242db4c7ee51cfd84","observation_id":"dd3e9b23-7ee4-49bf-9b3e-8a0fb3270265","resolution":{"observed_at":"2026-08-11T20:03:50.964248Z","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":"2026-08-11T20:03:50.968063Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.968063Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:25b9d04d35e9835644544089604e239d2915c0cbe2ab5978527264ddf55b27c8","observation_id":"ca0cc537-db35-418a-bf2b-f3e35f14c501","resolution":{"observed_at":"2026-08-11T20:03:50.968063Z","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":"10.1134/s1990341317040022","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:51.915042Z","title":"D., Makarova L","venue":null,"work_id":"39a931d9-135c-4a2f-94fa-717954aaa5da","year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.972090Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:fea63801fa3a9f152330122bfefd80152395da53dbdf74a79a559f4a4cc866ff","observation_id":"d10f41ab-3283-4d7f-af95-22c4133c86a9","resolution":{"observed_at":"2026-08-11T20:03:51.918889Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:50.976042Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.976042Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:15f06362558754920f4e91d7663c404fed8f2cd46162bbc6ed419e72a458692b","observation_id":"8aa1b9f4-9c83-4aea-b794-bb63bdc4a7fb","resolution":{"observed_at":"2026-08-11T20:03:50.976042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16085","last_updated":"2023-10-24T18:00:01Z","snapshot_observed_at":"2026-07-06T16:37:58.121261Z","submitted_at":"2023-10-24T18:00:01Z","title":"Blowing out the Candle: How to Quench Galaxies at High Redshift -- an Ensemble of Rapid Starbursts, AGN Feedback and Environment","version":1},"cited_work":{"arxiv_id":"2310.16085","doi":"10.48550/arxiv.2310.16085","metadata_source":"pith","pith_arxiv_id":"2310.16085","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"Blowing out the Candle: How to Quench Galaxies at High Redshift -- an Ensemble of Rapid Starbursts, AGN Feedback and Environment","venue":"astro-ph.GA","work_id":"5d548fc0-8190-410f-b865-53f5fd20e81f","year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.979762Z"},"links":{"cited_paper":"/paper/2310.16085","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:abdf015e60def6ead6d2250020c5f36d79faadef6a3bfeff0936c5ea8e7feb9c","observation_id":"1f478705-3ac8-4a44-8254-7fc0011f636c","resolution":{"observed_at":"2026-08-11T20:03:51.894027Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:50.984213Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.984213Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:6ff78901052a63440b8635f7a88aef1405b5d99d74a8b841bba99ba4866fad95","observation_id":"eb9dcf64-dbb4-4954-bd6e-ece39eb1f0af","resolution":{"observed_at":"2026-08-11T20:03:50.984213Z","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":"2026-08-11T20:03:50.987945Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.987945Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:ff208f54922bbd721d1c70ea84c883633159371db51a8f599e201ac7af6aae21","observation_id":"df08c1d2-f779-451a-af26-cc81a7fd4cb0","resolution":{"observed_at":"2026-08-11T20:03:50.987945Z","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":"2026-08-11T20:03:50.991836Z","title":"S., Strader J., Brodie J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.991836Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:83eca83aaff23579ce7032c388109e2945b24dfb9d639d63ed36896e255375a7","observation_id":"4177c763-ba81-42b8-be16-15edb88fe2c7","resolution":{"observed_at":"2026-08-11T20:03:50.991836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.4104","last_updated":"2013-01-17T14:28:11Z","snapshot_observed_at":"2026-08-07T01:49:47.047485Z","submitted_at":"2013-01-17T14:28:11Z","title":"Constraints on mass loss of globular clusters in dwarf galaxies","version":1},"cited_work":{"arxiv_id":"1301.4104","doi":"10.48550/arxiv.1301.4104","metadata_source":"pith","pith_arxiv_id":"1301.4104","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"Constraints on mass loss of globular clusters in dwarf galaxies","venue":"astro-ph.GA","work_id":"ae6c6feb-206d-47c3-b471-0fad59d9a48f","year":2013},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.995746Z"},"links":{"cited_paper":"/paper/1301.4104","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:96bb75db723b25b3814907e0b3458141257cd4ef9f85d57bca6d84a021b41f3e","observation_id":"162a39ed-8c99-4aff-8362-7c6bb72c32db","resolution":{"observed_at":"2026-08-11T20:03:51.849747Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07124","last_updated":"2024-12-31T19:45:14Z","snapshot_observed_at":"2026-08-12T08:33:37.899234Z","submitted_at":"2024-08-13T18:00:01Z","title":"Globular Cluster Counts around 700 Nearby Galaxies","version":2},"cited_work":{"arxiv_id":"2408.07124","doi":"10.48550/arxiv.2408.07124","metadata_source":"pith","pith_arxiv_id":"2408.07124","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"Globular Cluster Counts around 700 Nearby Galaxies","venue":"astro-ph.GA","work_id":"c0a55a5d-a899-467c-8a48-ae030ac1abcb","year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:50.999950Z"},"links":{"cited_paper":"/paper/2408.07124","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:719d35fb15474400779786245e60d5ecc8af363639fea4600d9569a147eb6dfd","observation_id":"ba089a48-b94e-4a79-8727-98a84100407c","resolution":{"observed_at":"2026-08-11T20:03:51.821187Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/200913364","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:51.798009Z","title":"K., Koch A., 2010, @doi [ ] 10.1051/0004-6361/200913364 , https://ui.adsabs.harvard.edu/abs/2010A&A...521A..43L 521, A43","venue":null,"work_id":"55bd9f4b-e425-464c-bf50-209ef48732da","year":2010},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.003932Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:51677927daad63e031b28e4a4545ceb3bade2d150d678507c03c6f5c9844ed38","observation_id":"956e7405-6e41-4504-8dee-d014c235fe89","resolution":{"observed_at":"2026-08-11T20:03:51.802968Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:51.007463Z","title":"W., C \\^o t \\'e P., Sales L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.007463Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:484eaf871033a4c45658d663ed1b70a3f3d02a8c92383651e316360bdb639950","observation_id":"9128410d-77c4-47c9-aef0-ec1481dcc76a","resolution":{"observed_at":"2026-08-11T20:03:51.007463Z","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":"2026-08-11T20:03:51.010671Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.010671Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:0047ec3c7f826f3e7b0540da36be01834abcf6a280a9dd2adfcecbd30b50e864","observation_id":"2b9fa053-ca99-4c93-b7c8-87c47efe4c5b","resolution":{"observed_at":"2026-08-11T20:03:51.010671Z","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":"2026-08-11T20:03:51.014132Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.014132Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:37ce75a5b1db077a533214136b94c71ccbf4031e815139fa3de5f2d5d0617858","observation_id":"2c233485-6cbb-4cba-884e-451462599da0","resolution":{"observed_at":"2026-08-11T20:03:51.014132Z","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":"2026-08-11T20:03:51.017620Z","title":"F., et al., 2016, @doi [ApJ] 10.3847/1538-4357/833/2/167 , https://ui.adsabs.harvard.edu/abs/2016ApJ...833..167M 833, 167","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.017620Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:602b23663e34706d0a6a1da29056e25d4f1ca9f5cc5c5f5151494f3bc3325abf","observation_id":"a9c66466-3327-4546-9307-68b92d787631","resolution":{"observed_at":"2026-08-11T20:03:51.017620Z","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":"2026-08-11T20:03:51.020909Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.020909Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:8023213cb7ffb01c1857254a8f492827474953897354a8c7fcfea06b2e2944d2","observation_id":"99768fc4-f1fa-4132-ba08-766dd3cc9bb1","resolution":{"observed_at":"2026-08-11T20:03:51.020909Z","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":"2026-08-11T20:03:51.024833Z","title":"W., 2012, @doi [AJ] 10.1088/0004-6256/144/1/4 , https://ui.adsabs.harvard.edu/abs/2012AJ....144....4M 144, 4","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.024833Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:24d9752f5575d097b152b577d399e7c5fade9dc9de8e487902598155f7fa3cbf","observation_id":"60d8afc7-5b86-4468-a10a-54d269c17465","resolution":{"observed_at":"2026-08-11T20:03:51.024833Z","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":"10.3847/1538-4357/ac35d9","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:51.711379Z","title":"C., et al., 2022, @doi [ApJ] 10.3847/1538-4357/ac35d9 , https://ui.adsabs.harvard.edu/abs/2022ApJ...924...87M 924, 87","venue":null,"work_id":"c5fe2836-77b7-430e-ae63-1552a0ba2fbd","year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.028732Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:ec19ca47cf3807a9d2a228935355fb2f7521720bb3d12c4da3145dd8644c0236","observation_id":"c620205c-4ea6-46b9-96e0-a17fab9b1155","resolution":{"observed_at":"2026-08-11T20:03:51.717736Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T20:03:51.033739Z","title":"A., et al., 2016, @doi [ ] 10.1093/mnras/stv2435 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.455.2323M 455, 2323","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.033739Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:c1f47c488adc69521cca2e116b1e23dee6038d290d347dcfafd5df47234ac5bd","observation_id":"ffc61bfb-d785-48b4-b61e-87f0c8ac29be","resolution":{"observed_at":"2026-08-11T20:03:51.033739Z","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":"2026-08-11T20:03:51.038877Z","title":"A., Li H., Souza S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.038877Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:75647bae4c1a7c3db54b7e8686f28657bfa30081b2f54686be1c1ffcf594a609","observation_id":"d21e437d-6bab-4151-88da-80155075a836","resolution":{"observed_at":"2026-08-11T20:03:51.038877Z","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":"2026-08-11T20:03:51.043067Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.043067Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:4e1348e892aeb82ec223920a2f0663d33958509569d8a4ed4a52ffac3b3be2ce","observation_id":"3d108304-a9c2-40ae-ba26-8eed748846c1","resolution":{"observed_at":"2026-08-11T20:03:51.043067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.08696","last_updated":"2024-02-12T21:58:57Z","snapshot_observed_at":"2026-07-06T17:29:39.117068Z","submitted_at":"2024-02-12T21:58:57Z","title":"The Firefly Sparkle: The Earliest Stages of the Assembly of A Milky Way-type Galaxy in a 600 Myr Old Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.08696","snapshot_observed_at":"2026-08-11T20:03:51.048044Z","title":"arXiv:2402.08696","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.048044Z"},"links":{"cited_paper":"/paper/2402.08696","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:96ad20422645de8462b61835ac1ebc4c82ffb3b89bd9fd47acfdc59683ef6e0e","observation_id":"a3c7721d-6be4-49bf-9196-2ff259f146a5","resolution":{"observed_at":"2026-08-11T20:03:51.048044Z","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":"2026-08-11T20:03:51.052687Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.052687Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:fab9208365aeda3d3aeab6484490465b7a08ca0679753e362b5ce3f46d54bd4f","observation_id":"f0a7690e-ad74-438c-afee-8027d331080a","resolution":{"observed_at":"2026-08-11T20:03:51.052687Z","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":"2026-08-11T20:03:51.056089Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.056089Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:0c456ca1e60ce6f65a350089339626409d6d98a8ac62116747f187f77b914e17","observation_id":"e91d9f00-bcfa-45b1-830d-10f7a653905e","resolution":{"observed_at":"2026-08-11T20:03:51.056089Z","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":"2026-08-11T20:03:51.059386Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.059386Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:5862944b0e14daaaa093b05e940ba6c4bdf9d679a9c741b252c161c7f4b4dde7","observation_id":"f57d1a38-ab92-4090-8e59-f2f713e96664","resolution":{"observed_at":"2026-08-11T20:03:51.059386Z","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":"2026-08-11T20:03:51.062448Z","title":"C., Springel V., van de Voort F., 2023, @doi [ ] 10.1093/mnras/stac3776 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.520.2692P 520, 2692","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.062448Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:dd7e19137a5a8855bde144468c950ad9f4fe0c258faf506c9fd44eb769a64191","observation_id":"99d97fea-f8fb-4f1f-a139-0c47594ee66e","resolution":{"observed_at":"2026-08-11T20:03:51.062448Z","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":"2026-08-11T20:03:51.066071Z","title":"W., Lim S., 2016, @doi [ ] 10.3847/2041-8205/822/2/L31 , https://ui.adsabs.harvard.edu/abs/2016ApJ...822L..31P 822, L31","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.066071Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:6dfff3313963792c252a75adbbbf9390402dd5adfb923fe72d6038d7382d9d1f","observation_id":"5b20739b-f28c-4622-9f8f-cac08bf1d8d9","resolution":{"observed_at":"2026-08-11T20:03:51.066071Z","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":"2026-08-11T20:03:51.069304Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.069304Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:656ab76b26ed746197fcbf2a59c791c4be0d31b00aceb47404b0c6a9543ca07c","observation_id":"0e468248-1876-448b-a79d-31bbb24f3d0d","resolution":{"observed_at":"2026-08-11T20:03:51.069304Z","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":"2026-08-11T20:03:51.072377Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.072377Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:904f491dbf8567ca21341fff7adb3895322f774848475543550c0a27d52d860e","observation_id":"bb58a809-a2a6-417a-885e-d0000d04a08c","resolution":{"observed_at":"2026-08-11T20:03:51.072377Z","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":"2026-08-11T20:03:51.075606Z","title":"J., van der Burg R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.075606Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:1481506ac5fe67ce8289e7a1c7ecc9bc6f47a4848439ba621f36ad23469d0e77","observation_id":"5b64b43a-f94d-4722-b272-0914294dcde2","resolution":{"observed_at":"2026-08-11T20:03:51.075606Z","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":"2026-08-11T20:03:51.079224Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.079224Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:f4c7a3fbde96350dad2d136390f31a4a3232f6fd0f4c38cd9f44e40f57a39d14","observation_id":"0387a489-d2b9-47fe-a176-be5b4b782dad","resolution":{"observed_at":"2026-08-11T20:03:51.079224Z","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":"2026-08-11T20:03:51.082919Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.082919Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:8b04ba9006554b331dc8653a7fdb1156f190aa34cc53c64a1866f8e78be0b83c","observation_id":"d6e7ee5e-d3b9-4949-b5e4-244b18ec2919","resolution":{"observed_at":"2026-08-11T20:03:51.082919Z","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":"2026-08-11T20:03:51.086661Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.086661Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:e0b604bfd07ce8b7785a362cd3f710578fab6cbcefe4a42c66830b2b2dd3f954","observation_id":"87f6620a-35c7-4e7c-a80b-60f992642eee","resolution":{"observed_at":"2026-08-11T20:03:51.086661Z","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":"2026-08-11T20:03:51.090310Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.090310Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:5e590c8aef7a48d6e0aac0f6391ec586f4388dac9c8802e7fa45a33ed3d10883","observation_id":"7f0a1a3e-e600-4b11-be2c-954e8ba89102","resolution":{"observed_at":"2026-08-11T20:03:51.090310Z","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":"2026-08-11T20:03:51.094391Z","title":"F., Knapen J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.094391Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:deff671940b978847d7f162cc1e1b55a25d65a01ea6815aad5f239060525a8a1","observation_id":"3bfbc39e-43dc-4df0-a546-17cee0948f43","resolution":{"observed_at":"2026-08-11T20:03:51.094391Z","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":"2026-08-11T20:03:51.098130Z","title":"P., et al., 2017, @doi [ ] 10.1093/mnras/stw2162 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.465..501S 465, 501","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.098130Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:18a95cdb090830ffa1098c21778f25496969e379072c20ba757aeaec7941522c","observation_id":"88ec1588-c8c4-4f6c-a3bd-d4381f281360","resolution":{"observed_at":"2026-08-11T20:03:51.098130Z","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":"2026-08-11T20:03:51.101945Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.101945Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:1f5d69d9821878d75541f9baccc5827204498f75a239eb46feae9e92fe5b6ab5","observation_id":"3752658f-2c6f-435e-8b78-8642e530b50a","resolution":{"observed_at":"2026-08-11T20:03:51.101945Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.08592","last_updated":"2023-09-18T21:04:33Z","snapshot_observed_at":"2026-07-06T16:19:05.495349Z","submitted_at":"2023-09-15T17:46:18Z","title":"Confirmation of an anomalously low dark matter content for the galaxy NGC1052-DF4 from deep, high resolution continuum spectroscopy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.08592","snapshot_observed_at":"2026-08-11T20:03:51.106081Z","title":"arXiv:2309.08592","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.106081Z"},"links":{"cited_paper":"/paper/2309.08592","citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:95712d5aa89dbc649a6b0bd5fd5d4148b4141dd7b5ad3aca2611b76592079666","observation_id":"40844660-aa03-409d-b7ca-99d992f33bfc","resolution":{"observed_at":"2026-08-11T20:03:51.106081Z","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":"2026-08-11T20:03:51.109358Z","title":"D., 2019, @doi [ ] 10.1146/annurev-astro-091918-104453 , https://ui.adsabs.harvard.edu/abs/2019ARA&A..57..375S 57, 375","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.109358Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:6363a387c509ad4fead8b8b924afc421b0b66a3d0f6de853e351f0391def16b2","observation_id":"da8deb34-5831-471e-9e54-18ac876248df","resolution":{"observed_at":"2026-08-11T20:03:51.109358Z","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":"2026-08-11T20:03:51.112479Z","title":"R., Forbes D","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.112479Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:7f4425271e244336ef557cbd5689362dec7328c285f9db5a6dcfa0bd6bb5672d","observation_id":"e91fa2f7-5d63-459d-b1ef-f75cd1072b5f","resolution":{"observed_at":"2026-08-11T20:03:51.112479Z","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":"2026-08-11T20:03:51.115542Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.115542Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:93fbceebfeba3e16367d194450794debfa05f7f174732b736a7787b56a40de6d","observation_id":"c2c898be-4810-48f8-adb7-465f02be986e","resolution":{"observed_at":"2026-08-11T20:03:51.115542Z","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":"2026-08-11T20:03:51.118743Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.118743Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:83d10d9f3369ebd7df7022ebba3c358566f80e86dbf09b45d6063689605e65b2","observation_id":"7c8dc9bb-95f4-41e3-a83f-350629628f1b","resolution":{"observed_at":"2026-08-11T20:03:51.118743Z","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":"2026-08-11T20:03:51.122584Z","title":"W., et al., 2024, @doi [ ] 10.1093/mnras/stae682 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.529.3301T 529, 3301","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.122584Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:c9cb994b73e09fe5d84be8a310b33330b459e21b2b013589759f452600426ac4","observation_id":"b5a81e3f-e0be-4793-8e10-8b42374ecca2","resolution":{"observed_at":"2026-08-11T20:03:51.122584Z","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":"2026-08-11T20:03:51.125885Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.125885Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:04ca6a32aacd37bb42fd74176ed209c3fac6a8d0f7fef2be6e2efb4b1023da46","observation_id":"e70bf740-a6ae-4842-9299-f852eaab6901","resolution":{"observed_at":"2026-08-11T20:03:51.125885Z","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":"2026-08-11T20:03:51.128914Z","title":"M., Moster B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.128914Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:93c02e1a598127d7eb83f8d404646ed1d2d360de8773770ce0ec104ab6bbb2a5","observation_id":"75ea52da-6b2c-4b18-aa0a-f035522a98fc","resolution":{"observed_at":"2026-08-11T20:03:51.128914Z","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":"2026-08-11T20:03:51.132577Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.132577Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:084acd338d9bc5d980b14fa51166a2418b706ec178bd44962b992bce7e2373ab","observation_id":"fcdf3a90-bf31-4b74-ae10-9f61488ddee7","resolution":{"observed_at":"2026-08-11T20:03:51.132577Z","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":"2026-08-11T20:03:51.136801Z","title":"A., et al., 2022, @doi [MNRAS] 10.1093/mnras/stac2417 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.516.3318W 516, 3318","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-08-11T20:03:51.136801Z"},"links":{"citing_paper":"/paper/2412.06155"},"observation_digest":"sha256:f055bbee93c51361b96f37d3f4709b400b069cd4aa647de135729b41747c1699","observation_id":"bc8c9566-76fd-4a74-94d5-961c7bcbd60d","resolution":{"observed_at":"2026-08-11T20:03:51.136801Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.06155","last_updated":"2024-12-09T02:34:37Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-12T10:58:20.744254Z","submitted_at":"2024-12-09T02:34:37Z","title":"Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems?"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":3,"parse_uncertain":0,"unresolved":91,"verified_exact":6,"verified_fuzzy":0},"total_outbound_references":109},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 100 of 109 outbound references and 0 inbound Pith citation observations for arXiv:2412.06155."}