{"as_of":"2026-08-20T13:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7dc02cfa23116c3ce2d91770e4366fb45d9c7280f53c5afdd717859827df5bee","coverage":[{"denominator":249,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T12:43:57.477813Z","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":"2026-08-20T06:33:59.587034+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/2607.19472/citation-record","integrity":"/paper/2607.19472/integrity","json":"/paper/2607.19472/citation-record.json","paper":"/paper/2607.19472"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T12:43:57.054164Z","title":"gbrammer/grizli:","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.054164Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e4e40fd18776ba25cb09efc01e04a9f999de89aeeb23ef977c284680f1188b73","observation_id":"724e4abb-b6c2-4c51-96eb-f12740b6a5ef","resolution":{"observed_at":"2026-08-01T12:43:57.054164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.18526","last_updated":"2023-05-29T18:00:08Z","snapshot_observed_at":"2026-08-16T15:28:34.413818Z","submitted_at":"2023-05-29T18:00:08Z","title":"STARRED: a two-channel deconvolution method with Starlet regularization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.18526","snapshot_observed_at":"2026-08-01T12:43:57.058828Z","title":"The Journal of Open Source Software , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.058828Z"},"links":{"cited_paper":"/paper/2305.18526","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e77a64f94046f6490ee1c2612cd0b1bd02a492a052dcdd1ba284914396bca298","observation_id":"ace033a8-1246-4213-b913-7792530e5147","resolution":{"observed_at":"2026-08-01T12:43:57.058828Z","resolver_source":null,"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":"2026-08-01T12:43:57.063498Z","title":"Frontiers in Astronomy and Space Sciences , keywords =","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.063498Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:3090a46dedd64f4efe248ac6fd348bc3fde64282e40cf5165c6018a237cbb9e8","observation_id":"f7c74f52-1016-43cd-a9ea-a38687609ae7","resolution":{"observed_at":"2026-08-01T12:43:57.063498Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.0731","last_updated":"2010-01-09T03:20:29Z","snapshot_observed_at":"2026-08-15T05:32:21.432376Z","submitted_at":"2009-12-03T21:00:02Z","title":"Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.0731","snapshot_observed_at":"2026-08-01T12:43:57.067727Z","title":null,"venue":null,"work_id":null,"year":2097},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.067727Z"},"links":{"cited_paper":"/paper/0912.0731","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:d3528e0e44c2fa1ac913804461c37a4adfefe596849b606853b9405af6707646","observation_id":"14e4d617-cbe7-48ae-b347-74cf348eed19","resolution":{"observed_at":"2026-08-01T12:43:57.067727Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0204182","last_updated":"2002-04-10T20:08:32Z","snapshot_observed_at":"2026-07-07T00:25:56.846184Z","submitted_at":"2002-04-10T20:08:32Z","title":"Detailed Structural Decomposition of Galaxy Images","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0204182","snapshot_observed_at":"2026-08-01T12:43:57.072305Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.072305Z"},"links":{"cited_paper":"/paper/astro-ph/0204182","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:7f9f79d13f51a1f0abe5341cc020744e392eced298e70b6ae9cbe9d06666fe0f","observation_id":"224be653-3645-4daf-b4fb-f04fb4e7e04d","resolution":{"observed_at":"2026-08-01T12:43:57.072305Z","resolver_source":null,"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":"2026-08-01T12:43:57.077046Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.077046Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ad02f76989d6ae9568ada6a39cacc60bb953a0cb014f376cfb06b35c35a9a8a3","observation_id":"e579e525-37d1-45ef-803c-6cec9a75544a","resolution":{"observed_at":"2026-08-01T12:43:57.077046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504626","last_updated":"2005-04-28T09:27:20Z","snapshot_observed_at":"2026-08-17T03:34:02.976036Z","submitted_at":"2005-04-28T09:27:20Z","title":"Color Gradients in Early-type Galaxies: Dependence on Environment and Redshift","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504626","snapshot_observed_at":"2026-08-01T12:43:57.081749Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.081749Z"},"links":{"cited_paper":"/paper/astro-ph/0504626","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:de29be759dd15d808ba1e2b3662dfe8a28e658e0f7beed013eea72b67b3290f4","observation_id":"bd5a3cbf-55a3-43a5-a248-ac4fc8ffe057","resolution":{"observed_at":"2026-08-01T12:43:57.081749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.08848","last_updated":"2016-09-28T10:12:55Z","snapshot_observed_at":"2026-08-14T21:37:46.776935Z","submitted_at":"2016-09-28T10:12:55Z","title":"Lens Model and Time Delay Predictions for the Sextuply Lensed Quasar SDSS J2222+2745","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.08848","snapshot_observed_at":"2026-08-01T12:43:57.086283Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.086283Z"},"links":{"cited_paper":"/paper/1609.08848","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:c0de4a7ae6d9192cdb062e5262c8de658b91eac68d11022efc7fd3d0280efdc3","observation_id":"66d6d87e-4ed7-45e7-93f9-38241a2a08cf","resolution":{"observed_at":"2026-08-01T12:43:57.086283Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.0458","last_updated":"2012-11-03T15:57:56Z","snapshot_observed_at":"2026-08-15T00:47:58.389479Z","submitted_at":"2012-09-03T20:00:01Z","title":"The Hidden Fortress: Structure and substructure of the complex strong lensing cluster SDSS J1029+2623","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.0458","snapshot_observed_at":"2026-08-01T12:43:57.090837Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.090837Z"},"links":{"cited_paper":"/paper/1209.0458","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:39b273f13bab7bed8dea2222823f37ae99215255246bf7b0f0424f9c66e2c3f9","observation_id":"1e712a40-bad0-4c26-8ad3-896a09dbc9f0","resolution":{"observed_at":"2026-08-01T12:43:57.090837Z","resolver_source":null,"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":"2026-08-01T12:43:57.095095Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.095095Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ecd180e1e50d983b6c54b4953e1df2bf88e1223d359f9dbb64ad490ae4ae9e1c","observation_id":"ecc7cddd-8b3b-44ef-88f3-30348175c206","resolution":{"observed_at":"2026-08-01T12:43:57.095095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.10980","last_updated":"2024-03-29T17:53:02Z","snapshot_observed_at":"2026-08-16T14:26:03.928964Z","submitted_at":"2024-01-19T19:00:00Z","title":"Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.10980","snapshot_observed_at":"2026-08-01T12:43:57.099535Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.099535Z"},"links":{"cited_paper":"/paper/2401.10980","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e656dfd95acc4f0f4cbca01a4e52b3e72f7a60166026c0a061a38c872a7f1c2c","observation_id":"29aa7d57-c6df-446d-87f8-b67f14586df2","resolution":{"observed_at":"2026-08-01T12:43:57.099535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04767","last_updated":"2024-01-09T19:00:02Z","snapshot_observed_at":"2026-08-16T14:28:43.613709Z","submitted_at":"2024-01-09T19:00:02Z","title":"Augmenting the power of time-delay cosmography in lens galaxy clusters by probing their member galaxies. II. Cosmic chronometers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.04767","snapshot_observed_at":"2026-08-01T12:43:57.103913Z","title":"and Schuldt, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.103913Z"},"links":{"cited_paper":"/paper/2401.04767","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ba48db82f4f1a64d11d349b98ac40c770372dca9774a7c792f2bd7dc2bd98316","observation_id":"c1f83627-09fc-4e1b-a105-b6a9e23333a8","resolution":{"observed_at":"2026-08-01T12:43:57.103913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.04093","last_updated":"2016-03-04T15:30:37Z","snapshot_observed_at":"2026-08-14T22:23:12.423965Z","submitted_at":"2015-11-12T21:12:32Z","title":"The story of supernova 'Refsdal' told by MUSE","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.04093","snapshot_observed_at":"2026-08-01T12:43:57.108698Z","title":"and Karman, W","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.108698Z"},"links":{"cited_paper":"/paper/1511.04093","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:534deb6c548e88f564403e2a7a8c9ea960b3b2026f7e5883af3c61feda04fc71","observation_id":"23abe837-8a3a-45f3-8cbc-e25925e625e5","resolution":{"observed_at":"2026-08-01T12:43:57.108698Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.01495","last_updated":"2023-10-02T18:00:07Z","snapshot_observed_at":"2026-08-16T14:55:45.391603Z","submitted_at":"2023-10-02T18:00:07Z","title":"Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) I. The final word on the origin of NGC6388 and NGC6441","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.01495","snapshot_observed_at":"2026-08-01T12:43:57.113123Z","title":", title =","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.113123Z"},"links":{"cited_paper":"/paper/2310.01495","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:399e12db39e2531999cd46387922673c3e798b2773ff05d3295e158eb5300c91","observation_id":"98586fcf-013e-48e4-af9e-92b63c1d4086","resolution":{"observed_at":"2026-08-01T12:43:57.113123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.12901","last_updated":"2025-04-23T16:08:23Z","snapshot_observed_at":"2026-08-16T13:08:42.319272Z","submitted_at":"2024-10-16T18:00:00Z","title":"Globular cluster ages and their relation to high-redshift stellar cluster formation times from different globular cluster models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.12901","snapshot_observed_at":"2026-08-01T12:43:57.117417Z","title":"and Forbes, Duncan A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.117417Z"},"links":{"cited_paper":"/paper/2410.12901","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:cba0861a545e56eae6e8384d4b7c856f921f2fa0be4669697c79864d348358f4","observation_id":"e3a26072-51df-4642-9948-a0e24101e4e5","resolution":{"observed_at":"2026-08-01T12:43:57.117417Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0001386","last_updated":"2000-01-21T19:38:41Z","snapshot_observed_at":"2026-08-14T22:57:31.894251Z","submitted_at":"2000-01-21T19:38:41Z","title":"Atomic diffusion in metal poor stars. The influence on the Main Sequence fitting distance scale, subdwarfs ages and the value of Delta Y/DeltaZ","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0001386","snapshot_observed_at":"2026-08-01T12:43:57.121413Z","title":"and Groenewegen, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.121413Z"},"links":{"cited_paper":"/paper/astro-ph/0001386","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:209901be81664713b664227d8e69d3e5e376ec84a4d2cba7783fb22ab3f4c75c","observation_id":"59f43796-3864-4a78-9ac3-ceb9c61c4b6c","resolution":{"observed_at":"2026-08-01T12:43:57.121413Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9707180","last_updated":"1997-07-16T13:53:10Z","snapshot_observed_at":"2026-07-07T01:17:47.359349Z","submitted_at":"1997-07-16T13:53:10Z","title":"Un updated theoretical scenario for globular cluster stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9707180","snapshot_observed_at":"2026-08-01T12:43:57.125634Z","title":"and Castellani, V","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.125634Z"},"links":{"cited_paper":"/paper/astro-ph/9707180","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:4b1217f3e6cd58c65a73c5b4cec5f96e59dc8906288eb01e76061a5bef3c5e81","observation_id":"a21bf6f5-150d-463f-8a16-f80f92d0b1c7","resolution":{"observed_at":"2026-08-01T12:43:57.125634Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9906095","last_updated":"1999-06-04T20:39:14Z","snapshot_observed_at":"2026-08-04T12:08:34.798814Z","submitted_at":"1999-06-04T20:39:14Z","title":"The Spectroscopic Age of 47 Tuc","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9906095","snapshot_observed_at":"2026-08-01T12:43:57.129731Z","title":"and Madgwick, Darren S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.129731Z"},"links":{"cited_paper":"/paper/astro-ph/9906095","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:49b006f2d19db3d880b72cbf0b62b2dde4a2819e7548fbc5b82bbf91b02b2162","observation_id":"481fe5a2-f0b9-4bc4-b9fe-4b1e56c05465","resolution":{"observed_at":"2026-08-01T12:43:57.129731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.10450","last_updated":"2022-12-13T07:48:16Z","snapshot_observed_at":"2026-08-16T16:37:39.217075Z","submitted_at":"2022-08-22T17:08:34Z","title":"Star formation at the smallest scales; A JWST study of the clump populations in SMACS0723","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.10450","snapshot_observed_at":"2026-08-01T12:43:57.133820Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.133820Z"},"links":{"cited_paper":"/paper/2208.10450","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:d8540d98d66b0ccb44a0c764bae942ca4555c234d4ede9551c73bb2a06e95c72","observation_id":"b7587a37-289f-4e97-8ac4-8e38a056ba6a","resolution":{"observed_at":"2026-08-01T12:43:57.133820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.11814","last_updated":"2023-06-20T18:11:33Z","snapshot_observed_at":"2026-08-16T15:22:26.577095Z","submitted_at":"2023-06-20T18:11:33Z","title":"The Ages and Metallicities of the Globular Clusters in the Sparkler","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.11814","snapshot_observed_at":"2026-08-01T12:43:57.138018Z","title":", title =","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.138018Z"},"links":{"cited_paper":"/paper/2306.11814","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0ac115ac724fbbca73bbe96f7f36a477909d75791444f1dd20cd0d4322512cc3","observation_id":"3b2d2c7b-8eaa-4553-a705-026053aa4645","resolution":{"observed_at":"2026-08-01T12:43:57.138018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.06903","last_updated":"2024-12-09T19:00:19Z","snapshot_observed_at":"2026-08-19T16:32:11.442384Z","submitted_at":"2024-12-09T19:00:19Z","title":"Time to Sparkler. Accurate ages of lensed globular clusters at $z=1.4$ with JWST photometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.06903","snapshot_observed_at":"2026-08-01T12:43:57.142590Z","title":"arXiv e-prints , title =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.142590Z"},"links":{"cited_paper":"/paper/2412.06903","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:5f5859efd21004343f26c2de900ee2260d73bca463b2eb7c95488f67f5b2e72f","observation_id":"f05e0ac9-f114-4ff2-8c7b-be0bba90b5e0","resolution":{"observed_at":"2026-08-01T12:43:57.142590Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.00829","last_updated":"2015-11-03T09:27:26Z","snapshot_observed_at":"2026-08-14T22:25:06.528901Z","submitted_at":"2015-11-03T09:27:26Z","title":"Deep multi-telescope photometry of NGC 5466. II. The radial behaviour of the mass function slope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.00829","snapshot_observed_at":"2026-08-01T12:43:57.146781Z","title":"and Dalessandro, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.146781Z"},"links":{"cited_paper":"/paper/1511.00829","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:3f6857e03d969fbc4f8c6897ce974d22c9162c06977760c3cc7b0f8f257ac14f","observation_id":"b83900b4-5022-462a-9998-d0464a117e1f","resolution":{"observed_at":"2026-08-01T12:43:57.146781Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.04323","last_updated":"2018-07-24T16:51:10Z","snapshot_observed_at":"2026-08-14T19:16:28.743200Z","submitted_at":"2018-05-11T11:13:11Z","title":"Integrated-light analyses vs. colour-magnitude diagrams - II. Leo A, an extremely young dwarf in the Local Group","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.04323","snapshot_observed_at":"2026-08-01T12:43:57.151142Z","title":"and Gallart, C","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.151142Z"},"links":{"cited_paper":"/paper/1805.04323","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0aaec166e90535993ba98d9c6b9c9e8852f47c847e42b81b87ae8b48f46387e9","observation_id":"8c20ded0-1af7-405e-858f-31a113cb1272","resolution":{"observed_at":"2026-08-01T12:43:57.151142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504509","last_updated":"2005-06-28T23:14:13Z","snapshot_observed_at":"2026-08-11T10:52:15.479724Z","submitted_at":"2005-04-22T19:58:33Z","title":"alpha-Enhanced Integrated Lick/IDS Spectral Indices and Milky Way and M31 Globular Clusters and Early-type Galaxies","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504509","snapshot_observed_at":"2026-08-01T12:43:57.155451Z","title":"2005 , month = sep, number =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.155451Z"},"links":{"cited_paper":"/paper/astro-ph/0504509","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:38caf9cd2994e849bd9551679cf8d300dc49646496def7aca67523b9e291abb7","observation_id":"a7f90463-780e-4088-a299-c8d9a4a22d94","resolution":{"observed_at":"2026-08-01T12:43:57.155451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0404511","last_updated":"2004-04-26T20:00:47Z","snapshot_observed_at":"2026-07-07T00:42:09.922418Z","submitted_at":"2004-04-26T20:00:47Z","title":"Higher-order Balmer line indices in alpha/Fe-enhanced stellar population models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0404511","snapshot_observed_at":"2026-08-01T12:43:57.160077Z","title":"Higher-order Balmer line indices in","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.160077Z"},"links":{"cited_paper":"/paper/astro-ph/0404511","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:64395767f36feee3bee877c21febb984960112a42e02861583938c8bbb6623e2","observation_id":"fb724e0c-a5dd-4ab9-8df1-ced00e6a8835","resolution":{"observed_at":"2026-08-01T12:43:57.160077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0209250","last_updated":"2002-11-12T15:22:45Z","snapshot_observed_at":"2026-08-08T15:03:28.046778Z","submitted_at":"2002-09-12T20:13:14Z","title":"Stellar population models of Lick indices with variable element abundance ratios","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0209250","snapshot_observed_at":"2026-08-01T12:43:57.164807Z","title":"Stellar population models of Lick indices with variable element abundance ratios , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.164807Z"},"links":{"cited_paper":"/paper/astro-ph/0209250","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:82b6839aaf31fb82c1810f720ddb80a38706c78c050d215a776e9142d22e90a4","observation_id":"63bfabd2-f21b-4c06-b1b0-ce2d8a1247e9","resolution":{"observed_at":"2026-08-01T12:43:57.164807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0007388","last_updated":"2000-07-26T09:14:24Z","snapshot_observed_at":"2026-07-07T00:12:18.935157Z","submitted_at":"2000-07-26T09:14:24Z","title":"Evolutionary tracks and isochrones for alpha-enhanced stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0007388","snapshot_observed_at":"2026-08-01T12:43:57.168951Z","title":"and Girardi, L","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.168951Z"},"links":{"cited_paper":"/paper/astro-ph/0007388","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ca7984dc6ef43044560c494bd5702eb88042eb912af8da1179d8caae98bfd9dc","observation_id":"d3ff2fd2-76d1-4a45-b96e-97ca77476cf3","resolution":{"observed_at":"2026-08-01T12:43:57.168951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0302063","last_updated":"2003-02-04T21:01:14Z","snapshot_observed_at":"2026-08-08T14:43:08.358874Z","submitted_at":"2003-02-04T21:01:14Z","title":"The impact of alpha/Fe enhanced stellar evolutionary tracks on the ages of elliptical galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0302063","snapshot_observed_at":"2026-08-01T12:43:57.173388Z","title":"and Maraston, C","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.173388Z"},"links":{"cited_paper":"/paper/astro-ph/0302063","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:d475727384484655c05beb9946895d75ab66278ddbb9606289512882247202d3","observation_id":"83bc6b75-432c-41ff-8d2a-8368b30ea808","resolution":{"observed_at":"2026-08-01T12:43:57.173388Z","resolver_source":null,"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":"2026-08-01T12:43:57.177778Z","title":"and Clayton, Geoffrey C","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.177778Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ef884bb906af269b5f5e37a935d8acdfcb8e10ce299a8998c27a1a37ee4e0586","observation_id":"0c196c28-60a6-4f94-be19-661f4842c4e2","resolution":{"observed_at":"2026-08-01T12:43:57.177778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.5000","last_updated":"2009-06-26T20:05:26Z","snapshot_observed_at":"2026-08-18T01:35:08.355686Z","submitted_at":"2009-06-26T20:05:26Z","title":"Differential stellar population models: how to reliably measure [Fe/H] and [alpha/Fe] in galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.5000","snapshot_observed_at":"2026-08-01T12:43:57.181826Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.181826Z"},"links":{"cited_paper":"/paper/0906.5000","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:957684b64647c3c296b4cc10663a81bf1ddd7db3351eb79a496455bb5c0f1e98","observation_id":"a8a2ca70-5a63-4e05-9ddb-b5fb83028e44","resolution":{"observed_at":"2026-08-01T12:43:57.181826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.06083","last_updated":"2017-02-20T17:56:54Z","snapshot_observed_at":"2026-08-14T21:15:39.428432Z","submitted_at":"2017-02-20T17:56:54Z","title":"The Gaia-ESO Survey. Mg-Al anti-correlation in iDR4 globular clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.06083","snapshot_observed_at":"2026-08-01T12:43:57.186460Z","title":"and Romano, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.186460Z"},"links":{"cited_paper":"/paper/1702.06083","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0b6553dfcc82d50492da583cecbefdcac423e34475351440572bd7343ea022b0","observation_id":"7b40d68b-7f29-4733-894e-787e77e55857","resolution":{"observed_at":"2026-08-01T12:43:57.186460Z","resolver_source":null,"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":"2026-08-01T12:43:57.190862Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.190862Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:f23f06156460d52a43fdf38b748471dd0f4936e84d9d0da6eff026a99ed6b3b4","observation_id":"a90e7048-af2b-4988-99e2-48bd12bf2ebc","resolution":{"observed_at":"2026-08-01T12:43:57.190862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.4439","last_updated":"2010-04-26T09:13:32Z","snapshot_observed_at":"2026-08-15T05:20:40.042995Z","submitted_at":"2010-04-26T09:13:32Z","title":"Evolutionary Stellar Population Synthesis with MILES. Part I: The Base Models and a New Line Index System","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.4439","snapshot_observed_at":"2026-08-01T12:43:57.194778Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.194778Z"},"links":{"cited_paper":"/paper/1004.4439","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:a8cba5a67ee615fe8db412cbd654374e77b6e12885d3aabc957c3b563ebb7a0c","observation_id":"d77b0d1b-cde1-4ed7-8230-dadf7de2b55c","resolution":{"observed_at":"2026-08-01T12:43:57.194778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409214","last_updated":"2004-12-14T10:15:43Z","snapshot_observed_at":"2026-08-12T22:53:46.694557Z","submitted_at":"2004-09-09T08:24:51Z","title":"New release of the ELODIE library","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409214","snapshot_observed_at":"2026-08-01T12:43:57.199120Z","title":"and Soubiran, C","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.199120Z"},"links":{"cited_paper":"/paper/astro-ph/0409214","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:73bc3e76c62659ec4ab0574c50873b55c8146221ad7df7e4fe9800fe17ed73e4","observation_id":"df72fa7d-7496-43d0-809e-11fe8169e4c4","resolution":{"observed_at":"2026-08-01T12:43:57.199120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.2979","last_updated":"2009-03-17T14:58:59Z","snapshot_observed_at":"2026-08-15T05:52:44.521885Z","submitted_at":"2009-03-17T14:58:59Z","title":"ULySS: A Full Spectrum Fitting Package","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.2979","snapshot_observed_at":"2026-08-01T12:43:57.202983Z","title":"and Prugniel, Ph","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.202983Z"},"links":{"cited_paper":"/paper/0903.2979","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:66ff9c567893085c40fd160e6dd2a2a518defb2c40807f199d43b4d3685047dd","observation_id":"1660f964-c777-4468-b3b8-9d1942e2a80a","resolution":{"observed_at":"2026-08-01T12:43:57.202983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.3047","last_updated":"2007-09-19T15:46:14Z","snapshot_observed_at":"2026-08-15T10:31:58.248498Z","submitted_at":"2007-09-19T15:46:14Z","title":"NBursts: Simultaneous Extraction of Internal Kinematics and Parametrized SFH from Integrated Light Spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.3047","snapshot_observed_at":"2026-08-01T12:43:57.207192Z","title":"NBursts: Simultaneous Extraction of Internal Kinematics and Parametrized SFH from Integrated Light Spectra , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.207192Z"},"links":{"cited_paper":"/paper/0709.3047","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:dc5cb08a2c765f2d1e4464c46864794603e7254b2e7de904753d5ae18a34bb67","observation_id":"d67b3ba5-8ff5-4809-807a-7b434c1aae3d","resolution":{"observed_at":"2026-08-01T12:43:57.207192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507002","last_updated":"2005-06-30T20:37:18Z","snapshot_observed_at":"2026-07-07T00:51:50.177555Z","submitted_at":"2005-06-30T20:37:18Z","title":"STEllar Content and Kinematics from high resolution galactic spectra via Maximum A Posteriori","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507002","snapshot_observed_at":"2026-08-01T12:43:57.211267Z","title":"and Pichon, C","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.211267Z"},"links":{"cited_paper":"/paper/astro-ph/0507002","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e98a4f0e3081d9112bd6ac1a71969887bd162fedfc83be1d83780eed7fc84326","observation_id":"f543a8e4-1a51-4d2b-9a97-439e8463565e","resolution":{"observed_at":"2026-08-01T12:43:57.211267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.08032","last_updated":"2015-04-29T21:41:15Z","snapshot_observed_at":"2026-08-17T03:16:49.442935Z","submitted_at":"2015-04-29T21:41:15Z","title":"Evolutionary stellar population synthesis with MILES - II. Scaled-solar and \\alpha-enhanced models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.08032","snapshot_observed_at":"2026-08-01T12:43:57.215433Z","title":"and Coelho, P","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.215433Z"},"links":{"cited_paper":"/paper/1504.08032","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:9524a578ebf4817941de7ce1da7100ed27cea74dac1637dc29ece7bfe1e8b474","observation_id":"86da1107-dbb3-4960-8986-2bed23e365ec","resolution":{"observed_at":"2026-08-01T12:43:57.215433Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.1216","last_updated":"2012-11-21T10:33:38Z","snapshot_observed_at":"2026-08-15T00:40:20.143595Z","submitted_at":"2012-11-06T13:40:22Z","title":"Full spectral fitting of Milky Way and M31 globular clusters: ages and metallicities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.1216","snapshot_observed_at":"2026-08-01T12:43:57.219599Z","title":"and Coelho, P","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.219599Z"},"links":{"cited_paper":"/paper/1211.1216","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:647a29845ea5eebb40127e5155803d551bff541353489c4d1f1750a0259fad2d","observation_id":"50e22086-19a8-4816-8222-c5bd9e9d011b","resolution":{"observed_at":"2026-08-01T12:43:57.219599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0402271","last_updated":"2004-02-11T21:36:14Z","snapshot_observed_at":"2026-07-07T00:40:26.527671Z","submitted_at":"2004-02-11T21:36:14Z","title":"Synthetic stellar populations: single stellar populations, stellar interior models and primordial proto-galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0402271","snapshot_observed_at":"2026-08-01T12:43:57.223914Z","title":"and Padoan, Paolo and Peacock, John A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.223914Z"},"links":{"cited_paper":"/paper/astro-ph/0402271","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:16e129c2a0d74ce6d4c9ff23eb5e47fcbc52b46ec734d837143bee53fb068552","observation_id":"de2ae394-35b4-4406-9032-d21719349357","resolution":{"observed_at":"2026-08-01T12:43:57.223914Z","resolver_source":null,"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":"2026-08-01T12:43:57.228149Z","title":"and Salaris, M","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.228149Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:dc60c6a17ce42d5fa7912e4444a6472b99716023e7eb520e476bdb2ed069dd84","observation_id":"0abe1e2f-d83a-47e4-9eef-08de58041595","resolution":{"observed_at":"2026-08-01T12:43:57.228149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.10421","last_updated":"2022-08-03T06:24:03Z","snapshot_observed_at":"2026-08-16T18:23:05.408374Z","submitted_at":"2021-05-21T15:41:25Z","title":"Implications for the Hubble tension from the ages of the oldest astrophysical objects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.10421","snapshot_observed_at":"2026-08-01T12:43:57.231814Z","title":"Implications for the Hubble tension from the ages of the oldest astrophysical objects , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.231814Z"},"links":{"cited_paper":"/paper/2105.10421","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:db1b5ec634cd14dad23e3b33a42bcab539bfdf603c5cc37174dd272aef99b8f1","observation_id":"4f10f001-6976-439f-b0f8-fa70878562dd","resolution":{"observed_at":"2026-08-01T12:43:57.231814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05167","last_updated":"2018-11-22T19:46:59Z","snapshot_observed_at":"2026-08-14T18:16:03.049773Z","submitted_at":"2018-10-11T18:00:01Z","title":"Mass modelling globular clusters in the Gaia era: a method comparison using mock data from an $N$-body simulation of M4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.05167","snapshot_observed_at":"2026-08-01T12:43:57.235667Z","title":", title =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.235667Z"},"links":{"cited_paper":"/paper/1810.05167","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:5cfd6374546b3225f03bf7b8cb3cccf979c2e9976f3d0aadce81bd76d256b813","observation_id":"31d39d93-b8ad-44d0-b42a-8e4204220667","resolution":{"observed_at":"2026-08-01T12:43:57.235667Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.02734","last_updated":"2016-11-08T21:55:49Z","snapshot_observed_at":"2026-08-14T21:31:20.593929Z","submitted_at":"2016-11-08T21:55:49Z","title":"Globular Cluster Abundances from High-Resolution, Integrated-Light Spectroscopy. II. Expanding the Metallicity Range for Old Clusters and Updated Analysis Techniques","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.02734","snapshot_observed_at":"2026-08-01T12:43:57.240149Z","title":"and Bernstein, Rebecca A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.240149Z"},"links":{"cited_paper":"/paper/1611.02734","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:99a1ffe905027666a2f783c43210faa00b5980cc9ee1d90a933d3d06b3627ba7","observation_id":"6c850630-e25a-4968-b937-dc3be968b66a","resolution":{"observed_at":"2026-08-01T12:43:57.240149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.3275","last_updated":"2013-10-11T20:00:10Z","snapshot_observed_at":"2026-08-17T08:04:05.750605Z","submitted_at":"2013-10-11T20:00:10Z","title":"Constraining stellar population models - I. Age, metallicity, and abundance pattern compilation for Galactic globular clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.3275","snapshot_observed_at":"2026-08-01T12:43:57.244216Z","title":"and Courteau, St","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.244216Z"},"links":{"cited_paper":"/paper/1310.3275","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:cb2cafd39093cfa6f7b7fe41210423a951f94a71c8b8dc86bf267e00243f19ed","observation_id":"58eb8503-709a-4394-a41d-574fbb4faaba","resolution":{"observed_at":"2026-08-01T12:43:57.244216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.10564","last_updated":"2022-06-21T17:42:55Z","snapshot_observed_at":"2026-08-16T16:51:24.523576Z","submitted_at":"2022-06-21T17:42:55Z","title":"Multiple Populations in Star Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.10564","snapshot_observed_at":"2026-08-01T12:43:57.248308Z","title":"and Marino, Anna F","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.248308Z"},"links":{"cited_paper":"/paper/2206.10564","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:aada80bb1c27dc0e1c2501d17424c409cade79bb867709afaa2fba0de19a3c59","observation_id":"14b50df8-e88a-49e7-b9f1-381a72e4fb10","resolution":{"observed_at":"2026-08-01T12:43:57.248308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.02835","last_updated":"2019-11-07T10:37:00Z","snapshot_observed_at":"2026-08-14T17:25:39.572189Z","submitted_at":"2019-11-07T10:37:00Z","title":"What is a globular cluster? An observational perspective","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.02835","snapshot_observed_at":"2026-08-01T12:43:57.252699Z","title":"What is a globular cluster? An observational perspective , year =","venue":null,"work_id":null,"year":1911},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.252699Z"},"links":{"cited_paper":"/paper/1911.02835","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e774ec99478a5430bd00afec8469707974329c1299a5a56805c9ff5f4df7a875","observation_id":"31952af5-0a9c-4058-9c33-87b1abf17706","resolution":{"observed_at":"2026-08-01T12:43:57.252699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.01286","last_updated":"2017-12-04T19:00:01Z","snapshot_observed_at":"2026-08-16T21:08:43.425363Z","submitted_at":"2017-12-04T19:00:01Z","title":"Multiple Stellar Populations in Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.01286","snapshot_observed_at":"2026-08-01T12:43:57.256814Z","title":"Multiple Stellar Populations in Globular Clusters , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.256814Z"},"links":{"cited_paper":"/paper/1712.01286","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:fa7e869ff3cb4752e4d4823b0bcaba0135f8614e5df6c859d75df8bfed6f871e","observation_id":"adeaf5c7-7070-417c-bf3d-2d9323712e5f","resolution":{"observed_at":"2026-08-01T12:43:57.256814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.0007","last_updated":"2012-01-27T17:28:22Z","snapshot_observed_at":"2026-08-15T04:36:47.960323Z","submitted_at":"2011-08-31T20:00:04Z","title":"Counting Low-Mass Stars in Integrated Light","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.0007","snapshot_observed_at":"2026-08-01T12:43:57.261005Z","title":"Counting Low-mass Stars in Integrated Light , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.261005Z"},"links":{"cited_paper":"/paper/1109.0007","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:a7a5fa0452e838cc5a4e1d08895bc53e9b0a8fb488313cb5128e184c0f884633","observation_id":"11e22935-f375-4e6e-a3fc-77c66d0f856b","resolution":{"observed_at":"2026-08-01T12:43:57.261005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.06594","last_updated":"2020-10-17T17:25:34Z","snapshot_observed_at":"2026-08-11T15:13:10.963153Z","submitted_at":"2020-07-13T18:00:55Z","title":"Inferring the Age of the Universe with Globular Clusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.06594","snapshot_observed_at":"2026-08-01T12:43:57.265100Z","title":", title =","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.265100Z"},"links":{"cited_paper":"/paper/2007.06594","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:8b1539be1f98ccf5d9f41e8d8cf0848e346ca4b8d3bb26edfbb0d8703dd41241","observation_id":"160a53f0-6af6-4b2c-853a-bace0f23b4a3","resolution":{"observed_at":"2026-08-01T12:43:57.265100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.6074","last_updated":"2010-03-31T15:12:28Z","snapshot_observed_at":"2026-08-15T05:22:48.109520Z","submitted_at":"2010-03-31T15:12:28Z","title":"The Ages of Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.6074","snapshot_observed_at":"2026-08-01T12:43:57.274371Z","title":", journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.274371Z"},"links":{"cited_paper":"/paper/1003.6074","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0d2b672113d416813a3bbbd5811cb4c14abd813bca6ddd8886576a8ed48b9c99","observation_id":"908002c9-335a-4343-abc0-e15f750041e3","resolution":{"observed_at":"2026-08-01T12:43:57.274371Z","resolver_source":null,"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":"2026-08-01T12:43:57.278600Z","title":"and Bolte, Michael and Stetson, Peter B","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.278600Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:563cd2a35297adfda84d713c51cee79a0ca4872e8f79c7c1317bafc2b61ca525","observation_id":"ff12ecd6-c572-4ba4-9718-4fc44c18f8f0","resolution":{"observed_at":"2026-08-01T12:43:57.278600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.02927","last_updated":"2018-03-16T01:01:55Z","snapshot_observed_at":"2026-08-14T19:38:21.481787Z","submitted_at":"2018-03-08T01:00:58Z","title":"A High-Precision Trigonometric Parallax to an Ancient Metal-Poor Globular Cluster","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.02927","snapshot_observed_at":"2026-08-01T12:43:57.282369Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.282369Z"},"links":{"cited_paper":"/paper/1803.02927","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0c305d4586a6938c7979d6b6eba5acc977099cd1b858fc7603d0d264fa49fb24","observation_id":"4972580b-7977-4523-9c27-3664abfd65dd","resolution":{"observed_at":"2026-08-01T12:43:57.282369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.08611","last_updated":"2020-01-23T15:46:31Z","snapshot_observed_at":"2026-08-09T17:35:53.654614Z","submitted_at":"2020-01-23T15:46:31Z","title":"The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of single and multiple stellar populations in seven bulge globular clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.08611","snapshot_observed_at":"2026-08-01T12:43:57.286358Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.286358Z"},"links":{"cited_paper":"/paper/2001.08611","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:3c6d9786d54a8fab667d837fd90cae846d6ec1eeedd763acf1a51609476853f9","observation_id":"bfc8e78d-f78d-40ff-9a71-9dca2f538065","resolution":{"observed_at":"2026-08-01T12:43:57.286358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.01915","last_updated":"2017-03-06T15:09:32Z","snapshot_observed_at":"2026-08-14T21:13:20.309181Z","submitted_at":"2017-03-06T15:09:32Z","title":"Absolute Ages and Distances of 22 GCs using Monte Carlo Main-Sequence Fitting","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.01915","snapshot_observed_at":"2026-08-01T12:43:57.290492Z","title":"and Gilligan, Christina and Chaboyer, Brian , journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.290492Z"},"links":{"cited_paper":"/paper/1703.01915","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0a1dda56e28abba942cd3b193dcd56a5c3fc55edda104ac44210d9bf0ad96984","observation_id":"2cc71f95-eec0-47b4-91ef-e8744cb253ce","resolution":{"observed_at":"2026-08-01T12:43:57.290492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506238","last_updated":"2005-06-10T14:02:09Z","snapshot_observed_at":"2026-08-12T14:01:36.536474Z","submitted_at":"2005-06-10T14:02:09Z","title":"A Comparison of Elemental Abundance Ratios in Globular Clusters, Field Stars, and Dwarf Spheroidal Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506238","snapshot_observed_at":"2026-08-01T12:43:57.294680Z","title":"and Venn, Kim A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.294680Z"},"links":{"cited_paper":"/paper/astro-ph/0506238","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:2aed826f44bd0f96daa30c4fc659e2d7fedc2cc9e5317936cd51a2a08b47f21a","observation_id":"cabbd6f0-62da-4f3f-a036-613e94cbf7f4","resolution":{"observed_at":"2026-08-01T12:43:57.294680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.02338","last_updated":"2018-02-08T10:03:14Z","snapshot_observed_at":"2026-08-15T00:11:35.383656Z","submitted_at":"2018-02-07T08:10:04Z","title":"LBT/MODS spectroscopy of globular clusters in the irregular galaxy NGC 4449","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.02338","snapshot_observed_at":"2026-08-01T12:43:57.298745Z","title":"and Morandi, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.298745Z"},"links":{"cited_paper":"/paper/1802.02338","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:6c488de04760eb250fd1ae8e0770e57ca42a7dd81bff00e857d81e2ddbe920b8","observation_id":"f11a83bd-ca60-4d1b-a743-d3b76a96a666","resolution":{"observed_at":"2026-08-01T12:43:57.298745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.4511","last_updated":"2007-05-31T23:35:19Z","snapshot_observed_at":"2026-08-15T10:39:46.184664Z","submitted_at":"2007-05-31T04:28:24Z","title":"The Age, Metallicity and Alpha-Element Abundance of Galactic Globular Clusters from Single Stellar Population Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.4511","snapshot_observed_at":"2026-08-01T12:43:57.302931Z","title":"and Proctor, Robert N","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.302931Z"},"links":{"cited_paper":"/paper/0705.4511","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e82368b0da41c4c2013fe2424f3f8a16f96a4dbe94f94ee2426a171b29276da6","observation_id":"d9b3f8d3-ae13-4267-a040-da76f3c1a36e","resolution":{"observed_at":"2026-08-01T12:43:57.302931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409526","last_updated":"2004-09-22T04:39:10Z","snapshot_observed_at":"2026-07-07T00:44:53.460945Z","submitted_at":"2004-09-22T04:39:10Z","title":"A Robust Method for the Analysis of Integrated Spectra from Globular Clusters using Lick Indices","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409526","snapshot_observed_at":"2026-08-01T12:43:57.307070Z","title":"and Forbes, Duncan A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.307070Z"},"links":{"cited_paper":"/paper/astro-ph/0409526","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e54f9831742ce48c23d4942917a1fa01b314224d0d0d182e4bae18a6bbb29bb8","observation_id":"121c606e-9125-42dd-b8b8-3062c52f8340","resolution":{"observed_at":"2026-08-01T12:43:57.307070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0407001","last_updated":"2004-06-30T20:18:10Z","snapshot_observed_at":"2026-08-03T08:47:01.741804Z","submitted_at":"2004-06-30T20:18:10Z","title":"A Principal Components Analysis of the Lick Indices of Galactic Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0407001","snapshot_observed_at":"2026-08-01T12:43:57.311174Z","title":", journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.311174Z"},"links":{"cited_paper":"/paper/astro-ph/0407001","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:4a4960ad427863272fb2e4cd4ac5f83cbbdc052971ff5bd49bd626336c1e49b1","observation_id":"c9c3fe6d-1be6-44ed-a632-4b9b8eeec2c9","resolution":{"observed_at":"2026-08-01T12:43:57.311174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.06849","last_updated":"2017-08-24T23:33:18Z","snapshot_observed_at":"2026-08-14T20:39:47.831188Z","submitted_at":"2017-08-22T23:27:22Z","title":"The SAMI Galaxy Survey: Global stellar populations on the size-mass plane","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.06849","snapshot_observed_at":"2026-08-01T12:43:57.315006Z","title":"and Croom, Scott M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.315006Z"},"links":{"cited_paper":"/paper/1708.06849","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:87769cdea9dfe26af30d6781d933b8d0c2d97934bf3588ed4dbbf95769953bcd","observation_id":"983eaac8-c5fa-40d4-afa9-2cf8f4a5b69a","resolution":{"observed_at":"2026-08-01T12:43:57.315006Z","resolver_source":null,"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":"2026-08-01T12:43:57.318891Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.318891Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:52974de4cb232b771050b0d3bd1d587e3fa17cc16d3f401e869c361e56f7a60f","observation_id":"5e459de4-65c8-4449-8c57-5e219706118e","resolution":{"observed_at":"2026-08-01T12:43:57.318891Z","resolver_source":null,"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":"2026-08-01T12:43:57.323398Z","title":"and Faber, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.323398Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:f61de727cd744af81ce521d18d49743cab574708305e6083f59757b8dda52b27","observation_id":"4e4cd63f-117f-4148-a53a-4d1ea5e6a587","resolution":{"observed_at":"2026-08-01T12:43:57.323398Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.3319","last_updated":"2012-11-14T14:47:38Z","snapshot_observed_at":"2026-08-15T00:39:23.361144Z","submitted_at":"2012-11-14T14:47:38Z","title":"The Dawn of Chemistry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.3319","snapshot_observed_at":"2026-08-01T12:43:57.327587Z","title":"The Dawn of Chemistry , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.327587Z"},"links":{"cited_paper":"/paper/1211.3319","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:bd51da79382798069bb0b77f712b560a7baac002bbc305c1b738c1cfa647dcd7","observation_id":"fd301eaf-fa56-4ded-bdd6-3fbaf4000ee9","resolution":{"observed_at":"2026-08-01T12:43:57.327587Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.04568","last_updated":"2023-02-27T10:55:59Z","snapshot_observed_at":"2026-08-16T16:09:56.082534Z","submitted_at":"2022-12-08T21:28:48Z","title":"Spectroscopic confirmation of four metal-poor galaxies at z=10.3-13.2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.04568","snapshot_observed_at":"2026-08-01T12:43:57.331669Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.331669Z"},"links":{"cited_paper":"/paper/2212.04568","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:775c87a2af3e833ac531448cc24c89748024727da0ac5992107da087962b4640","observation_id":"3e969700-8107-4621-8e5d-3665e9c67efd","resolution":{"observed_at":"2026-08-01T12:43:57.331669Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.08725","last_updated":"2024-07-24T10:15:57Z","snapshot_observed_at":"2026-08-16T14:18:52.350102Z","submitted_at":"2024-02-13T19:00:08Z","title":"Image deconvolution and PSF reconstruction with STARRED: a wavelet-based two-channel method optimized for light-curve extraction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.08725","snapshot_observed_at":"2026-08-01T12:43:57.336684Z","title":", title =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.336684Z"},"links":{"cited_paper":"/paper/2402.08725","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:5435fa6669adc4df5f0e39a8696594ae17bcf0e8eacfa24a4317e6bc876111ce","observation_id":"7718e15a-3010-4733-8eae-142765a1844d","resolution":{"observed_at":"2026-08-01T12:43:57.336684Z","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":"2026-08-16T14:19:09.715521Z","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":"2026-08-01T12:43:57.340891Z","title":"arXiv e-prints , title =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.340891Z"},"links":{"cited_paper":"/paper/2402.08696","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:4d94452b2384de661aa0530b2673271f9bd78a5230fcb59325694e404fad8ee5","observation_id":"2a0f67ea-75b9-425f-adcd-9255ab09e0ee","resolution":{"observed_at":"2026-08-01T12:43:57.340891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0004247","last_updated":"2000-04-18T12:04:47Z","snapshot_observed_at":"2026-07-07T00:10:54.168725Z","submitted_at":"2000-04-18T12:04:47Z","title":"The H Beta Index as an Age Indicator of Old Stellar Systems: The Effects of Horizontal-Branch Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0004247","snapshot_observed_at":"2026-08-01T12:43:57.345110Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.345110Z"},"links":{"cited_paper":"/paper/astro-ph/0004247","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:6fdf3d5fa9d47d075532c0f75b2fcec93b0219a3a72e38b5bce46a5a34a32430","observation_id":"caa9c9a8-51ee-413e-955f-e0696956e478","resolution":{"observed_at":"2026-08-01T12:43:57.345110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504313","last_updated":"2005-04-14T14:01:35Z","snapshot_observed_at":"2026-07-07T00:49:54.078514Z","submitted_at":"2005-04-14T14:01:35Z","title":"A Library of Integrated Spectra of Galactic Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504313","snapshot_observed_at":"2026-08-01T12:43:57.349256Z","title":"and Rose, James A","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.349256Z"},"links":{"cited_paper":"/paper/astro-ph/0504313","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:d0eacfc72e77581355e90473025cee7d0791d5ab446b84074b7dc446b9f1daa2","observation_id":"69545e26-3d7d-4830-b29d-fd33cedb3cd6","resolution":{"observed_at":"2026-08-01T12:43:57.349256Z","resolver_source":null,"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":"2026-08-01T12:43:57.353187Z","title":"2005 , url =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.353187Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ae579074929da3d97a585174089f97ba39393906158879cd238efa02ca04a182","observation_id":"cac0c547-f425-45a4-ab66-2de4b7e69c1d","resolution":{"observed_at":"2026-08-01T12:43:57.353187Z","resolver_source":null,"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":"2026-08-01T12:43:57.357092Z","title":"The Horizontal-Branch Stars in Globular Clusters","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.357092Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:3f1194b77612abb0555e4e7b710ff96acb63abc3758f3caffda7468d22aa8e9a","observation_id":"bc284e10-67f7-43ba-b3a6-a418786e79c7","resolution":{"observed_at":"2026-08-01T12:43:57.357092Z","resolver_source":null,"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":"2026-08-01T12:43:57.360796Z","title":"The Evolution of Horizontal Branch Stars and the Calibration of Globular Cluster Ages , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.360796Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:b419b42e2bf8aa617b13db723ebdb3e084fe17da3f75e9203d26bbfe660bb694","observation_id":"78eca517-e374-401c-9d97-41ef62f96b62","resolution":{"observed_at":"2026-08-01T12:43:57.360796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.0871","last_updated":"2008-01-06T16:18:30Z","snapshot_observed_at":"2026-08-15T10:24:13.024267Z","submitted_at":"2008-01-06T16:18:30Z","title":"Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.0871","snapshot_observed_at":"2026-08-01T12:43:57.364377Z","title":"and Prugniel, Ph","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.364377Z"},"links":{"cited_paper":"/paper/0801.0871","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:88a579925c49fa43aaaf0d07c6a8e5efab76fe02f9e571d21f05f445404576af","observation_id":"2e30b94d-c482-4121-994e-d25f191fd8c3","resolution":{"observed_at":"2026-08-01T12:43:57.364377Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.07562","last_updated":"2022-01-10T17:33:44Z","snapshot_observed_at":"2026-08-16T17:34:41.628233Z","submitted_at":"2021-12-14T17:09:27Z","title":"Deriving ages and horizontal branch properties of integrated stellar populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.07562","snapshot_observed_at":"2026-08-01T12:43:57.368841Z","title":"Deriving ages and horizontal branch properties of integrated stellar populations , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.368841Z"},"links":{"cited_paper":"/paper/2112.07562","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e51a9f366f6444bed7bd66968fe838c2fea7024d1468bd361694ce00df95ac71","observation_id":"26718a67-a693-4c64-a4a4-98f1c4efb6a1","resolution":{"observed_at":"2026-08-01T12:43:57.368841Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.0004","last_updated":"2010-11-30T21:00:16Z","snapshot_observed_at":"2026-08-15T05:01:32.017003Z","submitted_at":"2010-11-30T21:00:16Z","title":"Modelling realistic horizontal branch morphologies and their impact on spectroscopic ages of unresolved stellar systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.0004","snapshot_observed_at":"2026-08-01T12:43:57.373063Z","title":"and Salaris, Maurizio , journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.373063Z"},"links":{"cited_paper":"/paper/1012.0004","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:36cfe11e39d18b2e809d9c411fa40dadcfbebd7b9c19661a489374e470e21379","observation_id":"e6e7c135-d5ae-4c46-a7f2-b068105d4e77","resolution":{"observed_at":"2026-08-01T12:43:57.373063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0404592","last_updated":"2004-04-29T21:37:23Z","snapshot_observed_at":"2026-08-09T17:06:41.168669Z","submitted_at":"2004-04-29T21:37:23Z","title":"The Identification of Blue Horizontal Branch Stars in the Integrated Spectra of Globular Clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0404592","snapshot_observed_at":"2026-08-01T12:43:57.377163Z","title":"and Rose, James A","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.377163Z"},"links":{"cited_paper":"/paper/astro-ph/0404592","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:5c6f14011437b7b29c7a50c39fc4a7293b81d37879046115fbe22d05e62cb974","observation_id":"7cf09cdf-1f25-4dd3-8aea-e9ad3719b80f","resolution":{"observed_at":"2026-08-01T12:43:57.377163Z","resolver_source":null,"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":"2026-08-01T12:43:57.381110Z","title":"Photometric and Spectroscopic Observations of Globular Clusters in the Andromeda Nebula , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.381110Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0c618f4cc695019dea714bd340bd20429e889b603a7b706b84a9b71aa7b01fbe","observation_id":"3d7a259b-fa89-4ab0-956c-76b12dae54e5","resolution":{"observed_at":"2026-08-01T12:43:57.381110Z","resolver_source":null,"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":"2026-08-01T12:43:57.385150Z","title":", journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.385150Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:696c80fbe941fff729e2547bd4f99d6e9a5bb24e9c7f860c5e1d250b8bdb198b","observation_id":"82bbea23-6e99-4a92-8444-61896bad3912","resolution":{"observed_at":"2026-08-01T12:43:57.385150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.16387","last_updated":"2023-05-25T18:00:03Z","snapshot_observed_at":"2026-08-16T15:29:35.735000Z","submitted_at":"2023-05-25T18:00:03Z","title":"A new measurement of the expansion history of the Universe at z=1.26 with cosmic chronometers in VANDELS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.16387","snapshot_observed_at":"2026-08-01T12:43:57.389305Z","title":"and Moresco, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.389305Z"},"links":{"cited_paper":"/paper/2305.16387","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ab18c713239f005f421f7684547cee602897e860d4e10b38608c6401b7be3b26","observation_id":"5cca6316-6f73-4de6-a929-14551cb687d8","resolution":{"observed_at":"2026-08-01T12:43:57.389305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.02940","last_updated":"2020-10-06T18:00:04Z","snapshot_observed_at":"2026-08-16T19:15:25.655658Z","submitted_at":"2020-10-06T18:00:04Z","title":"How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.02940","snapshot_observed_at":"2026-08-01T12:43:57.393202Z","title":", title =","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.393202Z"},"links":{"cited_paper":"/paper/2010.02940","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:bcc21619012fa101e20b00bd4a0ad40dcbde5db7e74f8aca87bcf7ab04f375fd","observation_id":"3da93f88-aef0-4986-893d-4056733069d6","resolution":{"observed_at":"2026-08-01T12:43:57.393202Z","resolver_source":null,"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":"2026-08-01T12:43:57.397265Z","title":"and Coelho, P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.397265Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:e9f249c17810a7177ae5594f4c9ff925bd1018bea8e3bce737d6d200c999c085","observation_id":"d3953a09-c0f9-4c01-9f13-cced781d2bd0","resolution":{"observed_at":"2026-08-01T12:43:57.397265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.02233","last_updated":"2022-08-03T17:39:58Z","snapshot_observed_at":"2026-08-16T16:41:23.020217Z","submitted_at":"2022-08-03T17:39:58Z","title":"The Sparkler: Evolved High-Redshift Globular Clusters Captured by JWST","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.02233","snapshot_observed_at":"2026-08-01T12:43:57.401467Z","title":"and Desprez, Guillaume and Estrada-Carpenter, Vicente and Martis, Nicholas S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.401467Z"},"links":{"cited_paper":"/paper/2208.02233","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:8b2aa450cffa5499f4bd39cf9984ef8cb60173c3841a2ac7fe6321d7796836c6","observation_id":"2edc1cde-a463-418d-82b5-584618c60b09","resolution":{"observed_at":"2026-08-01T12:43:57.401467Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.09526","last_updated":"2021-05-21T00:23:22Z","snapshot_observed_at":"2026-08-16T18:23:29.611415Z","submitted_at":"2021-05-20T05:36:05Z","title":"Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST and literature data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.09526","snapshot_observed_at":"2026-08-01T12:43:57.405331Z","title":"and Vasiliev, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.405331Z"},"links":{"cited_paper":"/paper/2105.09526","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:cd7631190f46d1eb51fe5dcd2ab1dbce999be4ec4c32db6c753c21cb2a5142b6","observation_id":"1838f6ee-25d3-4af6-88fa-4766b462036c","resolution":{"observed_at":"2026-08-01T12:43:57.405331Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.01636","last_updated":"2023-03-03T00:03:00Z","snapshot_observed_at":"2026-08-16T15:51:12.352240Z","submitted_at":"2023-03-03T00:03:00Z","title":"Evidence for a bottom-light initial mass function in massive star clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.01636","snapshot_observed_at":"2026-08-01T12:43:57.409287Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.409287Z"},"links":{"cited_paper":"/paper/2303.01636","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:391df3a15518120475a947ceeb04c50692139eba2a0f14811c79df4be8434118","observation_id":"38688191-d7fc-4d3f-8d57-733a082c9a42","resolution":{"observed_at":"2026-08-01T12:43:57.409287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.3224","last_updated":"2010-12-15T03:53:51Z","snapshot_observed_at":"2026-08-16T10:55:14.097216Z","submitted_at":"2010-12-15T03:53:51Z","title":"A New Catalog of Globular Clusters in the Milky Way","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.3224","snapshot_observed_at":"2026-08-01T12:43:57.413182Z","title":", journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.413182Z"},"links":{"cited_paper":"/paper/1012.3224","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:fbfd18e4db140b2eed0273707de287b1b8582be8f8fa500ee1843ed6fad49e40","observation_id":"70d91254-ad40-4d2d-86fe-6177dc2d10c1","resolution":{"observed_at":"2026-08-01T12:43:57.413182Z","resolver_source":null,"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":"2026-08-01T12:43:57.417201Z","title":", journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.417201Z"},"links":{"citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:ac70046783c766217f14342c78fcd72801925adce1246add9a2c3d27a7a7752b","observation_id":"9519a01c-344d-48bc-9ea4-d3e46f925fe5","resolution":{"observed_at":"2026-08-01T12:43:57.417201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.4569","last_updated":"2010-10-21T20:00:17Z","snapshot_observed_at":"2026-08-15T05:05:10.176565Z","submitted_at":"2010-10-21T20:00:17Z","title":"Flux-calibrated stellar population models of Lick absorption-line indices with variable element abundance ratios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.4569","snapshot_observed_at":"2026-08-01T12:43:57.421257Z","title":"Flux-calibrated stellar population models of Lick absorption-line indices with variable element abundance ratios , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.421257Z"},"links":{"cited_paper":"/paper/1010.4569","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:156011ac650bb4e8c4073a0c9914e92ef90acefc3b7e0b5d6b75e6b520a53578","observation_id":"d8c838a2-5e85-42c0-a0e9-a7ebe55df42d","resolution":{"observed_at":"2026-08-01T12:43:57.421257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.07650","last_updated":"2018-09-20T14:28:22Z","snapshot_observed_at":"2026-08-14T18:25:50.031465Z","submitted_at":"2018-09-20T14:28:22Z","title":"The WAGGS project - II. The reliability of the calcium triplet as a metallicity indicator in integrated stellar light","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.07650","snapshot_observed_at":"2026-08-01T12:43:57.425555Z","title":"and Fraser-McKelvie, Amelia and Kamann, Sebastian and Penny, Samantha and Foster, Caroline and McDermid, Richard and Schiavon, Ricardo P","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.425555Z"},"links":{"cited_paper":"/paper/1809.07650","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:eb2f22374c10a81653ef23a63f783e10841869133a072cc2ee0e658e7fced3d8","observation_id":"5c3179a1-a0b4-4d7a-9884-91d5afcc1afa","resolution":{"observed_at":"2026-08-01T12:43:57.425555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05753","last_updated":"2019-09-12T15:29:29Z","snapshot_observed_at":"2026-08-11T09:26:15.072761Z","submitted_at":"2019-09-12T15:29:29Z","title":"The SLUGGS Survey: Measuring globular cluster ages using both photometry and spectroscopy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05753","snapshot_observed_at":"2026-08-01T12:43:57.429639Z","title":"and Forbes, Duncan A","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.429639Z"},"links":{"cited_paper":"/paper/1909.05753","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:70efbfc5842f522ee650adfb7d87c9fa95ac1397e78bc0fa381eb3311794872c","observation_id":"45704f39-f83b-472e-9a1f-a4408750d377","resolution":{"observed_at":"2026-08-01T12:43:57.429639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.07397","last_updated":"2017-03-21T19:26:07Z","snapshot_observed_at":"2026-08-19T02:54:19.621769Z","submitted_at":"2017-03-21T19:26:07Z","title":"The WAGGS project - I. The WiFeS Atlas of Galactic Globular cluster Spectra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.07397","snapshot_observed_at":"2026-08-01T12:43:57.433646Z","title":"and Schiavon, Ricardo P","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.433646Z"},"links":{"cited_paper":"/paper/1703.07397","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:c6aa304bc6b42c3041bc5addd2c1a1455a22f2f4095509664730c36ef737c4aa","observation_id":"e788dab1-07e6-43cd-b1cd-0b95b6e3c4a2","resolution":{"observed_at":"2026-08-01T12:43:57.433646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.14436","last_updated":"2023-09-25T18:00:29Z","snapshot_observed_at":"2026-08-16T14:57:44.790254Z","submitted_at":"2023-09-25T18:00:29Z","title":"The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue","version":1},"cited_work":{"arxiv_id":"2309.14436","doi":"10.48550/arxiv.2309.14436","metadata_source":"pith","pith_arxiv_id":"2309.14436","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue","venue":"astro-ph.GA","work_id":"ccea3152-85ea-4173-9789-6898575b138f","year":2023},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.441908Z"},"links":{"cited_paper":"/paper/2309.14436","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:591cd841a47d85e825e6201c81a1aa25ca148eebaccf81c6be851fbc1ebe7419","observation_id":"7156add5-c12d-4dcc-b8be-4c7fb363ccfa","resolution":{"observed_at":"2026-08-01T12:50:06.758143Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0009005","last_updated":"2001-02-14T13:50:58Z","snapshot_observed_at":"2026-07-07T00:12:47.660719Z","submitted_at":"2000-09-01T08:10:49Z","title":"On the variation of the Initial Mass Function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0009005","snapshot_observed_at":"2026-08-01T12:43:57.446149Z","title":"On the variation of the initial mass function , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.446149Z"},"links":{"cited_paper":"/paper/astro-ph/0009005","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:078f05c9fff8093e2610aed696a3751b8396c3ea9cb815bd5f21df7b720213a1","observation_id":"b0dd7fb9-1616-4437-a7eb-0b991a344b53","resolution":{"observed_at":"2026-08-01T12:43:57.446149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.09501","last_updated":"2023-10-13T09:28:32Z","snapshot_observed_at":"2026-08-16T15:15:13.768502Z","submitted_at":"2023-07-18T18:00:00Z","title":"Addressing the Hubble tension with cosmic chronometers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.09501","snapshot_observed_at":"2026-08-01T12:43:57.450129Z","title":"Addressing the Hubble tension with cosmic chronometers , year =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.450129Z"},"links":{"cited_paper":"/paper/2307.09501","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:0dfeee59059ad5d1d75a305ea6d432a8d3afd2341af01a950a8ebc3af0cb44dd","observation_id":"ca2d6c43-aed0-414e-b657-4d87141d3920","resolution":{"observed_at":"2026-08-01T12:43:57.450129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04327","last_updated":"2019-07-09T18:00:00Z","snapshot_observed_at":"2026-08-14T16:07:23.124870Z","submitted_at":"2019-07-09T18:00:00Z","title":"Stellar Metallicities and Elemental Abundance Ratios of z~1.4 Massive Quiescent Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04327","snapshot_observed_at":"2026-08-01T12:43:57.454167Z","title":"and Conroy, Charlie and Suess, Katherine A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.454167Z"},"links":{"cited_paper":"/paper/1907.04327","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:278f8aa754a80381d6163de543b8a8ac66aeb73a8f38de0d21bebbd9458bbc4d","observation_id":"199f65cc-fd20-4e5f-8f86-256ef4cf3e2f","resolution":{"observed_at":"2026-08-01T12:43:57.454167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.5023","last_updated":"2015-06-30T18:11:04Z","snapshot_observed_at":"2026-08-14T23:11:07.903272Z","submitted_at":"2014-11-18T21:00:03Z","title":"The ages, metallicities and element abundance ratios of massive quenched galaxies at z~1.6","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.5023","snapshot_observed_at":"2026-08-01T12:43:57.458182Z","title":"and Carollo, C","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.458182Z"},"links":{"cited_paper":"/paper/1411.5023","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:68a8e9a9dc03aa5f8ec787ac2a1aab10bdf3c6feb87c02129c4f95bcac326ee6","observation_id":"2a1d174f-c4ea-45f4-8ff1-67d1e8e1ddbe","resolution":{"observed_at":"2026-08-01T12:43:57.458182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.00084","last_updated":"2019-11-29T23:01:08Z","snapshot_observed_at":"2026-08-03T09:17:02.932818Z","submitted_at":"2019-11-29T23:01:08Z","title":"Stellar population properties of individual massive early-type galaxies at 1.4 < z < 2","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.00084","snapshot_observed_at":"2026-08-01T12:43:57.462080Z","title":"and Maraston, C","venue":null,"work_id":null,"year":1912},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.462080Z"},"links":{"cited_paper":"/paper/1912.00084","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:44f34dab4a77288d93f70b2fbb68b2cd33f6cd3cf97fc651da3bad7edb18a23a","observation_id":"b843c79b-be65-4ec1-8d35-c56b20f365f8","resolution":{"observed_at":"2026-08-01T12:43:57.462080Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.6629","last_updated":"2013-11-24T17:49:03Z","snapshot_observed_at":"2026-08-15T00:23:45.760391Z","submitted_at":"2013-03-26T20:00:01Z","title":"Early-Type Galaxy Archeology: Ages, Abundance Ratios, and Effective Temperatures from Full-Spectrum Fitting","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.6629","snapshot_observed_at":"2026-08-01T12:43:57.465936Z","title":"and van Dokkum, Pieter G","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.465936Z"},"links":{"cited_paper":"/paper/1303.6629","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:a6eaca5a31a838265b4a5b31bd42676e4f27eba66b31669d63d0a00faf2bd408","observation_id":"b456dc68-0e39-4fed-a385-dcb75492d5e2","resolution":{"observed_at":"2026-08-01T12:43:57.465936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-08-01T12:43:57.470059Z","title":"and Yuan, Wenlong and Macri, Lucas M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.470059Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:645b404ccc81c4b50ca6a7df5427df3e3b56435a46d7ad76b4f551238c785287","observation_id":"39bc683b-956e-4f8d-aaea-b0eec729bdcc","resolution":{"observed_at":"2026-08-01T12:43:57.470059Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.13430","last_updated":"2022-03-04T22:59:09Z","snapshot_observed_at":"2026-08-16T17:59:59.525630Z","submitted_at":"2021-08-30T18:00:01Z","title":"The stellar metallicities of massive quiescent galaxies at 1.0 < z < 1.3 from KMOS+VANDELS","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.13430","snapshot_observed_at":"2026-08-01T12:43:57.473943Z","title":"and McLure, Ross J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.473943Z"},"links":{"cited_paper":"/paper/2108.13430","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:d3cc9ff9930d71976c65278aedb225daa477be876e8e94a66b7d72f0b178fe7b","observation_id":"81cdb7f4-9ecd-46ed-b2ec-d397fbdb8db4","resolution":{"observed_at":"2026-08-01T12:43:57.473943Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.07373","last_updated":"2018-03-20T11:23:31Z","snapshot_observed_at":"2026-08-14T19:34:25.999672Z","submitted_at":"2018-03-20T11:23:31Z","title":"The VANDELS ESO public spectroscopic survey: observations and first data release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.07373","snapshot_observed_at":"2026-08-01T12:43:57.477813Z","title":"and McLure, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.477813Z"},"links":{"cited_paper":"/paper/1803.07373","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:fea2c022962a3ee82616c16b4066c25373154baa6a22450e7b98fa8716521192","observation_id":"d4a1bc75-8c57-400e-b0b0-a61fdd0ed6b6","resolution":{"observed_at":"2026-08-01T12:43:57.477813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T13:39:17.650267Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":249},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 100 of 249 outbound references and 0 inbound Pith citation observations for arXiv:2607.19472."}