{"as_of":"2026-08-16T23:29:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:036fd46612d5e38cb3afc03a172458bbdd366939735d53507e3247d4a7b5fbfa","coverage":[{"denominator":136,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T11:33:50.955397Z","state":"measured"},{"denominator":104,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":104,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T14:12:19.405416Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"cited_work":{"arxiv_id":"2504.15255","doi":"10.48550/arxiv.2504.15255","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.15255","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"c101b8cc-a943-4474-9390-fc03433583f6","year":2025},"citing_paper":{"arxiv_id":"2507.06284","last_updated":"2026-03-11T12:55:50Z","snapshot_observed_at":"2026-08-16T21:33:53.802771Z","submitted_at":"2025-07-08T18:00:00Z","title":"Before its time: a remarkably evolved protocluster core at z=7.88","version":2},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-05-19T05:56:25.755405Z"},"links":{"cited_paper":"/paper/2504.15255","citing_paper":"/paper/2507.06284"},"observation_digest":"sha256:5d92cf41836fd09ea25004792033daf28f2789261c4e738c4be27e8da257abc4","observation_id":"8630172d-8803-41fb-b895-9ddb887c4f7e","resolution":{"observed_at":"2026-05-19T05:57:07.912395Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.15255","snapshot_observed_at":"2026-08-06T14:12:19.405416Z","title":"2025, arXiv e-prints, arXiv:2504.15255, doi: 10.48550/arXiv.2504.15255","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.19706","last_updated":"2025-07-25T22:51:37Z","snapshot_observed_at":"2026-08-16T21:33:56.152457Z","submitted_at":"2025-07-25T22:51:37Z","title":"MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe","version":1},"reference_index":131,"source":"pdf_text","source_observed_at":"2026-08-06T14:12:19.405416Z"},"links":{"cited_paper":"/paper/2504.15255","citing_paper":"/paper/2507.19706"},"observation_digest":"sha256:e3190be44706af6edebc740b21b9deb04b4ced111df08a467dd8fab23583c268","observation_id":"9b8113ef-353c-4adf-aeb1-ecb14d143dbd","resolution":{"observed_at":"2026-08-06T14:12:19.405416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"cited_work":{"arxiv_id":"2504.15255","doi":"10.48550/arxiv.2504.15255","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.15255","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"c101b8cc-a943-4474-9390-fc03433583f6","year":2025},"citing_paper":{"arxiv_id":"2605.21599","last_updated":"2026-05-20T18:04:13Z","snapshot_observed_at":"2026-08-02T17:49:27.622468Z","submitted_at":"2026-05-20T18:04:13Z","title":"JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S","version":1},"reference_index":227,"source":"arxiv_source","source_observed_at":"2026-05-22T09:05:57.983296Z"},"links":{"cited_paper":"/paper/2504.15255","citing_paper":"/paper/2605.21599"},"observation_digest":"sha256:04e4f21e1c21bf4ffb1c41be6c7b944a0c87d6941a72a3610d9422db8a805896","observation_id":"49bf2676-3075-4147-9b76-c445347d94f7","resolution":{"observed_at":"2026-05-22T09:06:19.840359Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"cited_work":{"arxiv_id":"2504.15255","doi":"10.48550/arxiv.2504.15255","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.15255","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"c101b8cc-a943-4474-9390-fc03433583f6","year":2025},"citing_paper":{"arxiv_id":"2606.19447","last_updated":"2026-06-17T18:00:06Z","snapshot_observed_at":"2026-08-16T21:33:56.567212Z","submitted_at":"2026-06-17T18:00:06Z","title":"Reimagining SED Fitting with Cosmological Galaxy Simulations and Machine Learning","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-06-26T20:12:36.338298Z"},"links":{"cited_paper":"/paper/2504.15255","citing_paper":"/paper/2606.19447"},"observation_digest":"sha256:b9ee4fb56e4859cd9450c9a19c9aa0e159af06d3f3880c04ab89cb5cf34e104c","observation_id":"c2d1ffc0-ec63-4c7c-9a32-20e4a067ebf5","resolution":{"observed_at":"2026-07-04T01:49:22.165281Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2504.15255/citation-record","integrity":"/paper/2504.15255/integrity","json":"/paper/2504.15255/citation-record.json","paper":"/paper/2504.15255"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:33:50.517982Z","title":"@_ sL ;,찁 ö","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.517982Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:0519da8359d68499f8727f4cb35042b37487d6a385091b4622de5b669c09e9ab","observation_id":"a44a5c01-402c-4bce-8945-6541e9c3df22","resolution":{"observed_at":"2026-08-16T11:33:50.517982Z","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":"2026-08-16T11:33:50.545999Z","title":"2024, , 274, 12, 10.3847/1538-4365/ad5c69","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.545999Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:4b1c0b3ab118b2fb86a502c1b782a6af7bc6b53a1eb67ded273d8aaf676db0f4","observation_id":"0d08ec32-78c4-4328-ad97-e0f724b9e18c","resolution":{"observed_at":"2026-08-16T11:33:50.545999Z","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":"2026-08-16T11:33:50.550674Z","title":"2024, , 527, 11372, 10.1093/mnras/stad3902","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.550674Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:80a0753163f24f15c94e4113796f9b8089266b009e9be4122695cc7972aa0926","observation_id":"25f70be9-4614-4100-a455-ebf784d68ca3","resolution":{"observed_at":"2026-08-16T11:33:50.550674Z","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":"2026-08-16T11:33:50.555452Z","title":"2011, , 743, 121, 10.1088/0004-637X/743/2/121","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.555452Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:716455b34a007f293424e9ec6891fe73503acf0d02313fc2da3fa470ea5aa182","observation_id":"f966adec-cfe0-44cd-af3e-072383cd86b9","resolution":{"observed_at":"2026-08-16T11:33:50.555452Z","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":"2026-08-16T11:33:50.559599Z","title":"2023, , 524, 5486, 10.1093/mnras/stad1998","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.559599Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:705310424df3b5df300f6703de3169640733e10d2cf655db63756256b33bec5b","observation_id":"2d885a1c-9c24-4814-a4a3-9c4dc52ff7d3","resolution":{"observed_at":"2026-08-16T11:33:50.559599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.09070","last_updated":"2025-03-21T13:28:16Z","snapshot_observed_at":"2026-08-16T05:28:23.742156Z","submitted_at":"2025-01-15T19:00:01Z","title":"Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic $\\beta_{UV}$ slope at z=8.5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.09070","snapshot_observed_at":"2026-08-16T11:33:50.564665Z","title":"M., D'Eugenio , F., Maiolino , R., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.564665Z"},"links":{"cited_paper":"/paper/2501.09070","citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:64feb29000211869622f73acabcf95a8111db8a8107ed0df34013a0e1887b6af","observation_id":"479cce57-0d5a-456a-8380-4f1a0f0d78bd","resolution":{"observed_at":"2026-08-16T11:33:50.564665Z","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":"2026-08-16T11:33:50.570628Z","title":"L., Morris , S","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.570628Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:f1af0901dc1865aaacc069af770406725790f486519f4cb70bc126cd4e10a93f","observation_id":"7c2442bc-e8f0-434b-9efa-41fba70af17f","resolution":{"observed_at":"2026-08-16T11:33:50.570628Z","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":"2026-08-16T11:33:50.574774Z","title":"2023, , 525, 5388, 10.1093/mnras/stad2617","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.574774Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:05d23d128019cc11c6bbb8cadc543df1f76dc7db68e371edb77532e7328b1e98","observation_id":"05caecd5-a446-4e4f-a6bd-5fd21b5f6c10","resolution":{"observed_at":"2026-08-16T11:33:50.574774Z","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":"2026-08-16T11:33:50.579353Z","title":"E., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.579353Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:91a37c9ffa2e0cd88ff64934ab030d9b4a0018da486d4dc7513954b46b11dd13","observation_id":"c53d75d3-58dd-4127-8a62-e71c0eca487f","resolution":{"observed_at":"2026-08-16T11:33:50.579353Z","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":"2026-08-16T11:33:50.584438Z","title":"2021, The Journal of Open Source Software, 6, 3001, 10.21105/joss.03001","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.584438Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:a0b3cf693f30fed30256f20ab0110035cb4ac42e6151dd86f5264a823e0d0cbc","observation_id":"14efb68d-1060-4aba-9ed6-1d799da7f4a7","resolution":{"observed_at":"2026-08-16T11:33:50.584438Z","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":"2026-08-16T11:33:50.590966Z","title":"J., Conroy , C., & Johnson , B","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.590966Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:0151a78b04423da565e7bd824367d4eb502e2e25afd94402cff480f12420e7ae","observation_id":"5f66e6d6-bd98-4002-95c9-7e3e04e2d3a8","resolution":{"observed_at":"2026-08-16T11:33:50.590966Z","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":"2026-08-16T11:33:50.595820Z","title":"C., et al","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.595820Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:6b2cd267181bbfa8fb89bcf9c61fc6c75b311505475fda1f6e3765930fefdc3f","observation_id":"bba35a22-da1b-445a-8414-f1b463fafad1","resolution":{"observed_at":"2026-08-16T11:33:50.595820Z","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":"2026-08-16T11:33:50.600581Z","title":"2019, , 487, 3845, 10.1093/mnras/stz1449","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.600581Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:8ccc559d86c64420546d0d112fe216f27fb37825f9651142299a41d496ef0c78","observation_id":"6aee852f-e1d2-4f91-9ad8-36d5dc77edff","resolution":{"observed_at":"2026-08-16T11:33:50.600581Z","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":"2026-08-16T11:33:50.605721Z","title":"M., Kartaltepe , J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.605721Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:0268dacb14281a512b4ab56c6938a9142c2d41e37a76e6c3658ac0242ebac529","observation_id":"273c7d76-1be0-4f82-8ac5-e2a78aa6b20f","resolution":{"observed_at":"2026-08-16T11:33:50.605721Z","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":"2026-08-16T11:33:50.610508Z","title":"2024, , 527, 7871, 10.1093/mnras/stad3709","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.610508Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:f4be69d5fc57dabf3181b7400f62aca094309835595d0d0566555d4dcff8b3a4","observation_id":"4e0ee32e-ab40-4988-8943-9239e1e837c2","resolution":{"observed_at":"2026-08-16T11:33:50.610508Z","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":"2026-08-16T11:33:50.615407Z","title":"2003, , 115, 763, 10.1086/376392","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.615407Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:6335985deb0c11eba4259abadca1a264d3420e35f1bdb7234704034cd0f01170","observation_id":"2e08eca7-0051-41e4-9fa5-5319e01928c0","resolution":{"observed_at":"2026-08-16T11:33:50.615407Z","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":"2026-08-16T11:33:50.619138Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.619138Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:28b4baf4d544effe1cfa2457a015a1605528815796ff00020ecc72b1b1ab632f","observation_id":"bc8fbb83-32f0-459f-8194-477dc81a4735","resolution":{"observed_at":"2026-08-16T11:33:50.619138Z","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":"2026-08-16T11:33:50.622982Z","title":"2016, , 462, 1415, 10.1093/mnras/stw1756","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.622982Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:3f27e0b9229cbc81cae9416014e6eaec2a0145df879dc3efd57f437b17011586","observation_id":"36cc8e7b-e272-41d7-b498-9f6cc53c6d93","resolution":{"observed_at":"2026-08-16T11:33:50.622982Z","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":"2026-08-16T11:33:50.627553Z","title":"2017, , 838, 159, 10.3847/1538-4357/aa679f","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.627553Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:01369ba5c9b489368069e499b68bc8fbee88210f2a5e852391cf5581efbefcbc","observation_id":"94bd8920-c8c5-4a9d-b555-ad973f21d378","resolution":{"observed_at":"2026-08-16T11:33:50.627553Z","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":"2026-08-16T11:33:50.632078Z","title":"2016, , 823, 102, 10.3847/0004-637X/823/2/102","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.632078Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:51ac515171a86a0a443cf1020d1148652806ac615ccc15b036ec1b9a727c50fa","observation_id":"ae3b8bfa-5677-4338-8301-6fd08cea463e","resolution":{"observed_at":"2026-08-16T11:33:50.632078Z","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":"2026-08-16T11:33:50.636082Z","title":"2024, , 686, A128, 10.1051/0004-6361/202348091","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.636082Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:1fb3c93f765288d4df172f7f59196fbfc604450e6e2b4932017f4c4153d3cc61","observation_id":"307b0f42-ee13-49ee-811f-72703162d885","resolution":{"observed_at":"2026-08-16T11:33:50.636082Z","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":"2026-08-16T11:33:50.640695Z","title":"2013, , 51, 393, 10.1146/annurev-astro-082812-141017","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.640695Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:efbdf3eadb2589a7c24aae17573df026afad2a0957d71ef329badd72dd672b29","observation_id":"c889eaba-6481-4093-bf72-351a2d131700","resolution":{"observed_at":"2026-08-16T11:33:50.640695Z","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":"2026-08-16T11:33:50.645033Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.645033Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:b71a2611925293588b6aaa4b298ff6bfdc084f6bc702e96dad7fb357fd63c99b","observation_id":"ce1ee752-c894-4ae5-bd5c-5d7fdfcbdf3e","resolution":{"observed_at":"2026-08-16T11:33:50.645033Z","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":"2026-08-16T11:33:50.649415Z","title":"R., Hutter , A., Dayal , P., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.649415Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:67108b8a4f0203b2e5ab9ec5da682f606fcf292f8ae76d2e2a8bde84fd475f23","observation_id":"c98408a3-3bbd-4c1e-af1f-1bb2b042ef9d","resolution":{"observed_at":"2026-08-16T11:33:50.649415Z","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":"2026-08-16T11:33:50.653565Z","title":"C., Birnboim , Y., Mandelker , N., & Li , Z","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.653565Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:ab4e8c9c6c4ff3ee6ec2e096cbcc1b1142d507ef00e4a35b2c09e3bc3e4f5865","observation_id":"9f0f67c1-58a4-45d7-8725-6b72bda166df","resolution":{"observed_at":"2026-08-16T11:33:50.653565Z","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":"2026-08-16T11:33:50.657167Z","title":"2024, , 527, 2139, 10.1093/mnras/stad3239","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.657167Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:f7f94593d6ea0dabfa2f2212ae9d261b8beed33d17896f42dd0406ae17d86a86","observation_id":"e6e49bae-78e2-455a-ad66-8eb6270e93b5","resolution":{"observed_at":"2026-08-16T11:33:50.657167Z","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":"2026-08-16T11:33:50.660974Z","title":"2016, , 222, 8, 10.3847/0067-0049/222/1/8","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.660974Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:fdcf67fa1ae3fd01fa4fb79ff6981ab0341063f58ccd100c48f158c69ca7e945","observation_id":"3959aff2-b0ea-4d51-bd68-815fbf24f3ee","resolution":{"observed_at":"2026-08-16T11:33:50.660974Z","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":"2026-08-16T11:33:50.664521Z","title":"T., & Li , A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.664521Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:fbc6d887c5d65cf47e2e271f2d81a30a36e615e217d6e0cf15f6fc2c98f97873","observation_id":"2f2f7fc3-a842-4db6-bc06-cfdfb3dd53c3","resolution":{"observed_at":"2026-08-16T11:33:50.664521Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.02465","last_updated":"2025-12-17T15:56:28Z","snapshot_observed_at":"2026-08-03T19:26:59.807016Z","submitted_at":"2023-06-04T20:44:21Z","title":"Overview of the JWST Advanced Deep Extragalactic Survey (JADES)","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.02465","snapshot_observed_at":"2026-08-16T11:33:50.668216Z","title":"J., Willott , C., Alberts , S., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.668216Z"},"links":{"cited_paper":"/paper/2306.02465","citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:72239b9d9c3b5773234c76df29c8fe1b3ebe79c11430444f7e83812d3d4e3b88","observation_id":"5ca57395-4370-4025-84cf-f686f4b491d2","resolution":{"observed_at":"2026-08-16T11:33:50.668216Z","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":"2026-08-16T11:33:50.672277Z","title":"R., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.672277Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:4f03e08cad838cb1190a478edf7c36b959dd0111ac443518f90916dd7f1dc719","observation_id":"aed826a9-866c-4098-8925-ff1731ef4515","resolution":{"observed_at":"2026-08-16T11:33:50.672277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.01905","last_updated":"2024-10-02T18:03:50Z","snapshot_observed_at":"2026-08-16T13:13:13.960637Z","submitted_at":"2024-10-02T18:03:50Z","title":"The Burstiness of Star Formation at $z\\sim6$: A Huge Diversity in the Recent Star Formation Histories of Very UV-faint Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.01905","snapshot_observed_at":"2026-08-16T11:33:50.675866Z","title":"P., Topping , M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.675866Z"},"links":{"cited_paper":"/paper/2410.01905","citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:6d4b4d3562de34643b375954db549620dd1ae498dc5812175113db2c099ac75e","observation_id":"ca646339-b080-40d5-919e-e511c420cb55","resolution":{"observed_at":"2026-08-16T11:33:50.675866Z","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":"2026-08-16T11:33:50.679931Z","title":"L., Capak , P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.679931Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:a8c76e0216986ac8293b939690c48dccda9cbf6d2fef949f63fb3050213284d5","observation_id":"40aa11f6-dd73-4fdf-84cf-5b643e518aab","resolution":{"observed_at":"2026-08-16T11:33:50.679931Z","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":"2026-08-16T11:33:50.684200Z","title":"L., & Morishita , T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.684200Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:18df9d489d753f5913c6e653898e8f32734080f93bac6fd6d27637204e1bd478","observation_id":"a4f84a6d-a1de-46ec-93b9-91f18330df5c","resolution":{"observed_at":"2026-08-16T11:33:50.684200Z","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":"2026-08-16T11:33:50.688313Z","title":"2018, , 473, 3717, 10.1093/mnras/stx2595","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.688313Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:45ac89137378a55c1b60547b6c6297dbf5aab9022bd9d22e7933b7aa95645f18","observation_id":"d8b26c10-9410-49ec-a84f-0772d74f14ad","resolution":{"observed_at":"2026-08-16T11:33:50.688313Z","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":"2026-08-16T11:33:50.691985Z","title":"F., Faucher-Gigu \\`e re , C.-A., & Kere s , D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.691985Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:d67668f9a51f914df0999068f2d0e1b785e0b1fd67f913618e480ce81a323fd5","observation_id":"5b9c0262-9cc7-43b3-8dc9-080459b6fb0c","resolution":{"observed_at":"2026-08-16T11:33:50.691985Z","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":"2026-08-16T11:33:50.695756Z","title":"2023, , 522, 3831, 10.1093/mnras/stad1205","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.695756Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:cd4d743eb2aa4d0b8f4478670bd63d7327fe9d1bbe96f69d22df7a68d731b346","observation_id":"b5f8509a-6981-4d2e-94d4-5c46633109e7","resolution":{"observed_at":"2026-08-16T11:33:50.695756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.10877","last_updated":"2023-10-05T18:48:04Z","snapshot_observed_at":"2026-08-14T20:57:08.160939Z","submitted_at":"2017-05-30T21:53:19Z","title":"The 2017 Release of Cloudy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.10877","snapshot_observed_at":"2026-08-16T11:33:50.699707Z","title":"J., Chatzikos , M., Guzm \\'a n , F., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.699707Z"},"links":{"cited_paper":"/paper/1705.10877","citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:cdaff7d29067f861054909c261779c43be04fde8c85d7530a72078fbe78e694e","observation_id":"f2ef8a70-db85-48a7-b86a-8a900400c8bb","resolution":{"observed_at":"2026-08-16T11:33:50.699707Z","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":"2026-08-16T11:33:50.704078Z","title":"P., & Bridges , M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.704078Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:ebb133e94fef1998dfbbe0767896ad83693773c8e98d460f7bad16ba03df11a5","observation_id":"6b603b40-fa0d-427f-8a81-a49bf2fc41fd","resolution":{"observed_at":"2026-08-16T11:33:50.704078Z","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":"2026-08-16T11:33:50.708169Z","title":"2024, , 684, A207, 10.1051/0004-6361/202348321","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.708169Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:3428bf55bce2981b9b733410bbdc6969ef16b51161b0e7fb60466661fc6f81c9","observation_id":"82ceeaa0-a111-4203-8014-58264412656d","resolution":{"observed_at":"2026-08-16T11:33:50.708169Z","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":"2026-08-16T11:33:50.712154Z","title":"L., Bagley , M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.712154Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:de021af82729cc8b21770545f8abe722b34254e6a2e92fa90910de4583498bfd","observation_id":"40aebcad-4250-4584-9084-d35d145057d8","resolution":{"observed_at":"2026-08-16T11:33:50.712154Z","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":"2026-08-16T11:33:50.716394Z","title":"A., Gurvich , A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.716394Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:adf11f6f9610050b6ee0eab13babbd0c3fb65953330ca32e5b0395412ca9270b","observation_id":"23dc9131-a23a-4f2f-b90b-1b61cfdc688f","resolution":{"observed_at":"2026-08-16T11:33:50.716394Z","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":"2026-08-16T11:33:50.720635Z","title":"W., Lang , D., & Goodman , J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.720635Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:b0aaf728050c44fc7b1f066b2aa916fdefd3a2eb5d0795066893d59d7e00067d","observation_id":"f089bdd8-3358-465a-b9c9-504cb60340d0","resolution":{"observed_at":"2026-08-16T11:33:50.720635Z","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":"2026-08-16T11:33:50.724699Z","title":"2025, , 979, 66, 10.3847/1538-4357/ad9a5c","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.724699Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:e5fab191f88553670f0625da7c7e7e99969f290506194aded14103a9603aa5f4","observation_id":"dd44ebef-f615-46b3-ba4b-03971f7226f9","resolution":{"observed_at":"2026-08-16T11:33:50.724699Z","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":"2026-08-16T11:33:50.728864Z","title":"1999, , 306, 843, 10.1046/j.1365-8711.1999.02576.x","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.728864Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:40360cb8a6013c2f121c821f0a85ee03fad5465252538db321b5f396716ff75a","observation_id":"877e2b42-6fc4-4899-874a-7ea5fb2c0993","resolution":{"observed_at":"2026-08-16T11:33:50.728864Z","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":"2026-08-16T11:33:50.733095Z","title":"2010, Communications in Applied Mathematics and Computational Science, 5, 65, 10.2140/camcos.2010.5.65","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.733095Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:7cf1e54a02fa54eb1c354cc32dd0b1ec0886457194fc64963baf048d28627965","observation_id":"c60011af-d62b-449b-81d0-8b953a2d3117","resolution":{"observed_at":"2026-08-16T11:33:50.733095Z","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":"2026-08-16T11:33:50.737080Z","title":"2012, , 422, 1231, 10.1111/j.1365-2966.2012.20696.x","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.737080Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:1a5461f148fee08fccda47fe4d85e8337bb5668552cbeb2a1ce57736a2de0784","observation_id":"5694ca65-ff37-43ad-b5da-e274ef2b0035","resolution":{"observed_at":"2026-08-16T11:33:50.737080Z","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":"2026-08-16T11:33:50.741014Z","title":"M., et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.741014Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:2597554347f5947bcc05da2a4860bfc744a86636646c28f3aa060bada056e83d","observation_id":"a25e0a59-f9ed-4c8f-9b1b-13568bc85962","resolution":{"observed_at":"2026-08-16T11:33:50.741014Z","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":"2026-08-16T11:33:50.745099Z","title":"2022, , 938, 11, 10.3847/1538-4357/ac7b84","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.745099Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:1f1673534dde9a3d918f039a65db93bc6b271ee34cbfcedd46dcff7677b4cc18","observation_id":"8d581a2e-677d-47cc-9e1a-c8cf29fbb823","resolution":{"observed_at":"2026-08-16T11:33:50.745099Z","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":"2026-08-16T11:33:50.749524Z","title":"J., Hobson , M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.749524Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:9f3c1dd1fb0259158d50381695c9903b8a3e839f76c48e7ca5039664817854a2","observation_id":"631a07d6-c27f-4c69-96f9-1b567b226dcd","resolution":{"observed_at":"2026-08-16T11:33:50.749524Z","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":"2026-08-16T11:33:50.754164Z","title":"2023, , 265, 5, 10.3847/1538-4365/acaaa9","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.754164Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:4726fde73daab810d45ef5a43a388fb02c44a983d72ec7915029ce1a214eab99","observation_id":"7b92c96b-39cd-4c54-92ec-a7d8b92996b4","resolution":{"observed_at":"2026-08-16T11:33:50.754164Z","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":"2026-08-16T11:33:50.758583Z","title":"R., Millman , K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.758583Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:bd8c2583ed08fb1917aceb90b6dab59033ae179aaf24cdfebe7210bd24b6fc7a","observation_id":"96084593-f3d6-429a-9007-9e73d898bcda","resolution":{"observed_at":"2026-08-16T11:33:50.758583Z","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":"2026-08-16T11:33:50.763385Z","title":"2013, , 208, 19, 10.1088/0067-0049/208/2/19","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.763385Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:69c92c2c803d86063d2f1ce591ffa2dea68570632356c1491d959ff6a9bb6305","observation_id":"b60fa2f2-3cc8-4ca9-acec-853393d04fbf","resolution":{"observed_at":"2026-08-16T11:33:50.763385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:33:50.767228Z","title":"J., Chartier , N., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.767228Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:91d8e4aa490c1ae4056ccd8b7e8bdb78de63653f4691e988cc3cd8a275cb3d20","observation_id":"1a31f1a0-7028-4054-a2ff-b1c0971b6bc6","resolution":{"observed_at":"2026-08-16T11:33:50.767228Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.4246","last_updated":"2011-11-18T00:39:32Z","snapshot_observed_at":"2026-08-15T04:28:34.964537Z","submitted_at":"2011-11-18T00:39:32Z","title":"The No-U-Turn Sampler: Adaptively Setting Path Lengths in Hamiltonian Monte Carlo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.4246","snapshot_observed_at":"2026-08-16T11:33:50.770990Z","title":"D., & Gelman , A","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.770990Z"},"links":{"cited_paper":"/paper/1111.4246","citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:798ed1f42298c50a2129608b8149d5f036f0ce79b2149007efc20d2a5c3e1721","observation_id":"da6d3537-292d-4230-b905-6bc202352b71","resolution":{"observed_at":"2026-08-16T11:33:50.770990Z","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":"2026-08-16T11:33:50.776226Z","title":"F., Kere s , D., O \\ n orbe , J., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.776226Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:baf158733fd0e013fe4889c8915ac3ebad1625ce9b30e36593dde0b7fe478dff","observation_id":"c41feb30-5e11-475c-aa4f-f6ec2000590a","resolution":{"observed_at":"2026-08-16T11:33:50.776226Z","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":"2026-08-16T11:33:50.780405Z","title":"F., Gurvich , A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.780405Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:c885853e76fd2e2de5df3071343290bf25d5cf9f4a533ff6529426388a891e0a","observation_id":"59c723ab-39be-4d45-ac99-df1a163d953e","resolution":{"observed_at":"2026-08-16T11:33:50.780405Z","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":"2026-08-16T11:33:50.784166Z","title":"F., Wetzel , A., Wheeler , C., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.784166Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:805a461cbe5a7fcae95567af331963d88ae65361b972ac7d6efa1dd899b95c51","observation_id":"39e62909-eab5-4830-bb8f-639a7312093c","resolution":{"observed_at":"2026-08-16T11:33:50.784166Z","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":"2026-08-16T11:33:50.788095Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.788095Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:8da26081cf800fa4982f9e973305617d7e56067d4687ad2fff2e9754f84e0bb5","observation_id":"20c74d4c-4769-4c9a-a5f3-251a075e7a89","resolution":{"observed_at":"2026-08-16T11:33:50.788095Z","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":"2026-08-16T11:33:50.792292Z","title":"G., Gawiser , E., Faber , S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.792292Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:961d24463ee116cb08318d3e54dd18d95e7b62e8eb7b8271b5662934882eea9b","observation_id":"e30da195-fb50-4815-b12f-34552b05cbf4","resolution":{"observed_at":"2026-08-16T11:33:50.792292Z","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":"2026-08-16T11:33:50.796165Z","title":"G., Speagle , J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.796165Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:f9b04ae28a693b0678a80580bc26ffbd347fce1fec447d85501d6e8cd234d48f","observation_id":"37dd481f-a71c-42e5-91cf-b556daa6df7c","resolution":{"observed_at":"2026-08-16T11:33:50.796165Z","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":"2026-08-16T11:33:50.800009Z","title":"G., Tacchella , S., Genel , S., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.800009Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:afd46e25415ce6bb609c97ed5af076e59f8ae763d04f4b11dd25d6c973f857bb","observation_id":"15cdb17b-37b7-4444-9638-bbff6671ab0c","resolution":{"observed_at":"2026-08-16T11:33:50.800009Z","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":"2026-08-16T11:33:50.803801Z","title":"D., Leja , J., Conroy , C., & Speagle , J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.803801Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:86c8418584b88108f7285154822e9cee3e60d110f8c03114970013f02ff31157","observation_id":"14808a8d-aa5b-472b-83a5-1a7e77b27c70","resolution":{"observed_at":"2026-08-16T11:33:50.803801Z","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":"2026-08-16T11:33:50.807962Z","title":"D., Weisz , D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.807962Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:4f8181c2d5e7273dde3aadfb6b0b6b8add7242e51f8e427dff0d7a36e5685e21","observation_id":"440c3bff-c1de-44e3-9f0c-d4b66abd1f1e","resolution":{"observed_at":"2026-08-16T11:33:50.807962Z","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":"2026-08-16T11:33:50.811845Z","title":"A., Nabergoj , D., & Seljak , U","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.811845Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:9b7342dafbf9ffb5e381f7947a79f9914bf70d7947addfb29aa06a0ec7f29966","observation_id":"ff4f9f52-9ce4-4087-9184-94d7f21173b9","resolution":{"observed_at":"2026-08-16T11:33:50.811845Z","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":"2026-08-16T11:33:50.815527Z","title":"1998, , 36, 189, 10.1146/annurev.astro.36.1.189","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.815527Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:28cc16958abc3c2624a86a06f974f074e5d3c86b4e7730a7901e81caad78b3ba","observation_id":"c0b8bf3a-8142-42d4-99a0-50f44c27e3e9","resolution":{"observed_at":"2026-08-16T11:33:50.815527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stx2379","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:33:51.655503Z","title":"2018, , 473, 776, 10.1093/mnras/stx2379","venue":null,"work_id":"d3566eca-3b17-4715-891b-94d078120578","year":2018},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.819203Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:e51215783d4b345e395cec0b1bdf1960e61a38ec2d5153403780f5771dc70ac1","observation_id":"10d3bb0c-c3bf-4a77-8f70-56c00e387e2f","resolution":{"observed_at":"2026-08-16T11:33:51.659774Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/2632-2153/ac98f4","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:33:51.642048Z","title":"2022, Machine Learning: Science and Technology, 3, 04LT04, 10.1088/2632-2153/ac98f4","venue":null,"work_id":"a3daec7d-3ef1-47ef-9410-6846054fc15c","year":2022},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.823565Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:b1df13e0795282ea15463b948c3dc9207ab1ac45ce050315b1b6daa14dc22742","observation_id":"06e71351-750c-4fdf-89b3-50d896da795b","resolution":{"observed_at":"2026-08-16T11:33:51.647297Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:33:50.827426Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.827426Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:0368995c264de2073fa0e76a7eae06abd155cc3b936cb05593b5645adc82c007","observation_id":"ae62dd04-a74a-4d08-811a-29d390ea9b25","resolution":{"observed_at":"2026-08-16T11:33:50.827426Z","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":"2026-08-16T11:33:50.831596Z","title":"C., Gil de Paz , A., Tremonti , C., et al","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.831596Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:ac2c48289b79669d3bf791a9d498f6b3fef7b955e8174526038552fa97617200","observation_id":"d0df747f-79a4-4535-a27f-fb0b5aaf2131","resolution":{"observed_at":"2026-08-16T11:33:50.831596Z","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":"2026-08-16T11:33:50.835443Z","title":"2022, , 509, 595, 10.1093/mnras/stab3034","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.835443Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:094c9902625d54963595d25934948134418b676f843f5f56e53f7cfa98787a90","observation_id":"71e9ee72-1173-4a4c-a7aa-268888ffefa7","resolution":{"observed_at":"2026-08-16T11:33:50.835443Z","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":"2026-08-16T11:33:50.839468Z","title":"C., Johnson , B","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.839468Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:5d86ce8dace8a321290434a24781afa3013ff82f22f6e388da75b01342d6b8bc","observation_id":"28b752e8-f2ba-4434-ba7e-6622aa619525","resolution":{"observed_at":"2026-08-16T11:33:50.839468Z","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":"2026-08-16T11:33:50.843230Z","title":"D., Conroy , C., & van Dokkum , P","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.843230Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:eaa87f2234fa0f4ac8323be49da73d42b5a1f5c906e6e219053f306ebabb914b","observation_id":"d7b19f7b-b8a1-49c6-b191-7dd4bd20fb6c","resolution":{"observed_at":"2026-08-16T11:33:50.843230Z","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":"2026-08-16T11:33:50.846968Z","title":"D., Conroy , C., van Dokkum , P","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.846968Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:eec3daf3fff8f9c31a7d95e32b1da63925527ccf7d890f62a788b00626f1d668","observation_id":"f58ff0d2-4233-4d39-9e18-948870ab5f1e","resolution":{"observed_at":"2026-08-16T11:33:50.846968Z","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":"2026-08-16T11:33:50.850781Z","title":"S., Ting , Y.-S., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.850781Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:88b73563cea4ae0efd676cb0ba27d3c989592c78112180c636f4d299576d2762","observation_id":"178a5655-68b8-4a0f-85c7-ed3e16b66eb5","resolution":{"observed_at":"2026-08-16T11:33:50.850781Z","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":"2026-08-16T11:33:50.854827Z","title":"2024, , 167, 16, 10.3847/1538-3881/ad0be4","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.854827Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:0e79c98aecae261f33a0cb753711d723025bd631795a7dc82e314c7acfe14129","observation_id":"37b787c7-f545-40e9-ab3c-5c3bd2fb052b","resolution":{"observed_at":"2026-08-16T11:33:50.854827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.02470","last_updated":"2023-06-08T08:35:20Z","snapshot_observed_at":"2026-08-16T15:26:43.852958Z","submitted_at":"2023-06-04T20:44:26Z","title":"JADES: Differing assembly histories of galaxies -- Observational evidence for bursty SFHs and (mini-)quenching in the first billion years of the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.02470","snapshot_observed_at":"2026-08-16T11:33:50.859233Z","title":"J., D'Eugenio , F., Maiolino , R., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.859233Z"},"links":{"cited_paper":"/paper/2306.02470","citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:20fb5a3edb3554d70f2895947080135b0bc28da168f9520eed77cfea958671a8","observation_id":"b0fab2f5-258c-46f3-83bf-44e0e3b3e300","resolution":{"observed_at":"2026-08-16T11:33:50.859233Z","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":"2026-08-16T11:33:50.863510Z","title":"2024, , 629, 53, 10.1038/s41586-024-07227-0","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.863510Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:0230a804e820af83efff48be27d547c14855fe2f9c0c301d213e14bdf0211980","observation_id":"e559648e-ed0c-4a70-b7ec-a6122f40eb72","resolution":{"observed_at":"2026-08-16T11:33:50.863510Z","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":"2026-08-16T11:33:50.867644Z","title":"1995, , 441, 18, 10.1086/175332","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.867644Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:7ee03d7ecee3f19d13a06e47f7de8c55e230e3fa006677691be7d6be5ac4db4f","observation_id":"7709d0b6-9797-46a0-a1f2-e86a34e0410d","resolution":{"observed_at":"2026-08-16T11:33:50.867644Z","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":"2026-08-16T11:33:50.872082Z","title":"V., van der Wel , A., Rix , H.-W., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.872082Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:2b3183d4ae6a2f3667bbf5c5962c0f75be66c4dc2bc9a33c9086c6dbf0d99255","observation_id":"2dda7d44-3b05-43bb-813d-ecf1d4a56baf","resolution":{"observed_at":"2026-08-16T11:33:50.872082Z","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":"2026-08-16T11:33:50.876606Z","title":"2018, , 854, 29, 10.3847/1538-4357/aaa76e","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.876606Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:54c5910b9483cb09e5a595397c489a22c4898198a7d53d5a4092e6622eefc2af","observation_id":"45115104-597c-401e-88a4-676500b5df4d","resolution":{"observed_at":"2026-08-16T11:33:50.876606Z","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":"2026-08-16T11:33:50.881100Z","title":"A., Trenti , M., & Treu , T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.881100Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:91a3b4c99b4f936c3fa17d3f78840d1dd64e9153703ba607c3891009672313f3","observation_id":"2b1b2f74-c814-41eb-a7c5-db9d6463074f","resolution":{"observed_at":"2026-08-16T11:33:50.881100Z","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":"2026-08-16T11:33:50.885270Z","title":"2023, , 526, 2196, 10.1093/mnras/stad2734","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.885270Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:570deec68722418a456c6641c50a1573eb513f54edb9f0db4dbdbfce2842d685","observation_id":"dbea5529-37ea-4b5a-b298-9c6072e1da79","resolution":{"observed_at":"2026-08-16T11:33:50.885270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.11060","last_updated":"2018-06-28T16:19:37Z","snapshot_observed_at":"2026-08-14T18:57:57.107114Z","submitted_at":"2018-06-28T16:19:37Z","title":"Malicious User Experience Design Research for Cybersecurity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.11060","snapshot_observed_at":"2026-08-16T11:33:50.889639Z","title":"F., & Ostriker , E","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.889639Z"},"links":{"cited_paper":"/paper/1806.11060","citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:3444c701ddb6876c1f8464d5ff5616d4a10192ebd584066a79344bfadc4a4cfd","observation_id":"997a1cfe-461a-43f7-8ddd-57d981d514f8","resolution":{"observed_at":"2026-08-16T11:33:50.889639Z","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":"2026-08-16T11:33:50.893371Z","title":"I., Scarlata , C., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.893371Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:354dcd44886b41f0e9f35d26108d8971b68dc11c137dedf34ebc684f680b263a","observation_id":"a867b079-b04c-4303-bad5-f87469420c69","resolution":{"observed_at":"2026-08-16T11:33:50.893371Z","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":"2026-08-16T11:33:50.897236Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.897236Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:5a2e88775afb471a6cb9666b29bf21a17b1ad1871f203a86abe22adc0c005890","observation_id":"3864dc75-300e-48d8-8166-146559f048c9","resolution":{"observed_at":"2026-08-16T11:33:50.897236Z","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":"2026-08-16T11:33:50.901309Z","title":"P., Oesch , P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.901309Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:f0938085d1807b7f493ad0b0c55950c265028f9b38a1388b11333235e6105e76","observation_id":"ed60c5cb-55d2-4627-8d75-a18160bcc22c","resolution":{"observed_at":"2026-08-16T11:33:50.901309Z","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":"2026-08-16T11:33:50.905167Z","title":"2020, , 889, 180, 10.3847/1538-4357/ab65eb","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.905167Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:237c964e90c1b090166d11224cc36d48d63f652a3279843813e59d529c2cdcbe","observation_id":"c42c8d5a-de50-4e1f-b641-c9ecc7c256cc","resolution":{"observed_at":"2026-08-16T11:33:50.905167Z","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":"2026-08-16T11:33:50.908954Z","title":"2009, , 507, 1793, 10.1051/0004-6361/200912497","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.908954Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:4e8b6f37330ef0b25fa106721fc3c89b363fdaddaddd1a7232c159223ced4ec5","observation_id":"aa3c5477-87cf-4efd-a308-a1a7a2704ae4","resolution":{"observed_at":"2026-08-16T11:33:50.908954Z","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":"2026-08-16T11:33:50.912945Z","title":"2018, , 70, S10, 10.1093/pasj/psx103","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.912945Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:44e51028b3f5b76a600cfd4b6795a8980efeb1b32be9a7ce0c6d5e5f648982c7","observation_id":"77ffc98e-56eb-40fd-b54a-1ab2243a1a4e","resolution":{"observed_at":"2026-08-16T11:33:50.912945Z","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":"2026-08-16T11:33:50.916669Z","title":"G., Mobasher , B., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.916669Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:f51730ca2f141265d7c218d4ce18454499ad71a3693e97b7ade0fb52eef9e871","observation_id":"2f8189b3-bbea-45be-9dcd-12d6c301ae47","resolution":{"observed_at":"2026-08-16T11:33:50.916669Z","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":"2026-08-16T11:33:50.920583Z","title":"2022, , 509, 1885, 10.1093/mnras/stab3071","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.920583Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:ca0a849e01752003ef4b53adbd63fb81b1ee2f644515da304d1fd6a9dc2e5fd2","observation_id":"0741ad12-1d82-4a3d-9481-63cc4058f86a","resolution":{"observed_at":"2026-08-16T11:33:50.920583Z","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":"2026-08-16T11:33:50.924581Z","title":"2023, , 677, L4, 10.1051/0004-6361/202347384","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.924581Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:db9e0bbd859914dcb2aa8b47d6f9d66b7bf1b0893ce3dc6baed6e467e3cdb5be","observation_id":"8a29ab10-747b-4f1d-a46c-2317e0146e16","resolution":{"observed_at":"2026-08-16T11:33:50.924581Z","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":"2026-08-16T11:33:50.928475Z","title":"M., & Zemel , Y","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.928475Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:9bc4de6888f9f26c2ad4c95a4546a4a275177022fbf380b5030345af1cfab3f3","observation_id":"bd4efb57-3406-4cab-a363-7409e60c9184","resolution":{"observed_at":"2026-08-16T11:33:50.928475Z","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":"2026-08-16T11:33:50.932408Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.932408Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:9fce981b5fb7dc3f37827906f95bf8a1bca387761215a10cf2d6d759975d0f74","observation_id":"73b8f171-e264-4e39-bb82-cbf164df2685","resolution":{"observed_at":"2026-08-16T11:33:50.932408Z","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":"2026-08-16T11:33:50.936224Z","title":"2024, , 976, 72, 10.3847/1538-4357/ad7e15","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.936224Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:ca477dcff1ced346869dfd0e804be7763abb60ee04adfb75c9e9f03bd4cb9f55","observation_id":"fbbe70c4-a96d-4180-99f9-ddcd6462a9bd","resolution":{"observed_at":"2026-08-16T11:33:50.936224Z","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":"2026-08-16T11:33:50.939968Z","title":"2018, , 473, 4077, 10.1093/mnras/stx2656","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.939968Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:0c44e2f683a019366137d6c592bfe14c0f62eff77caa0ec20e22559848411ce7","observation_id":"ddf03d64-6d94-4e97-942f-db4ea8b39459","resolution":{"observed_at":"2026-08-16T11:33:50.939968Z","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":"2026-08-16T11:33:50.943450Z","title":"H., Bezanson , R., Labbe , I., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.943450Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:bdf8c1eba66a38050881aaa858a575c3170978f9476b94e9095b42e7d6df9605","observation_id":"9061b6ae-42d7-44f2-ad11-89c3304cd3e1","resolution":{"observed_at":"2026-08-16T11:33:50.943450Z","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":"2026-08-16T11:33:50.947217Z","title":"2023, , 525, L117, 10.1093/mnrasl/slad091","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.947217Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:30f8e96f002f3e4dc77fe448e2a1315ffe482efac1414b5f4125c40ebf4e012b","observation_id":"5698e53f-08d4-4ba2-96b7-cc90784a6446","resolution":{"observed_at":"2026-08-16T11:33:50.947217Z","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":"2026-08-16T11:33:50.951182Z","title":"E., Tacchella , S., Johnson , B","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.951182Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:dc07847dc9e9fa555d41c6a636192c5280908fa07b35f850875ac040786ae886","observation_id":"fd9b05d4-6f1a-4cc8-b7f1-7a2217976c0e","resolution":{"observed_at":"2026-08-16T11:33:50.951182Z","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":"2026-08-16T11:33:50.955397Z","title":"F., Jim \\'e nez-Vicente , J., et al","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference","version":2},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-16T11:33:50.955397Z"},"links":{"citing_paper":"/paper/2504.15255"},"observation_digest":"sha256:71e1e5104b47769125fcb7cadc0bb2e8729b23bc4f7480386e5544498f8314d2","observation_id":"7770f3d1-5266-4129-a21c-8806b6cc1ba3","resolution":{"observed_at":"2026-08-16T11:33:50.955397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2504.15255","last_updated":"2025-05-26T15:10:00Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T21:33:08.337352Z","submitted_at":"2025-04-21T17:34:55Z","title":"Population Models for Star Formation Timescales in Early Galaxies: The First Step Towards Solving Outshining in Star Formation History Inference"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":98,"verified_exact":2,"verified_fuzzy":0},"total_outbound_references":136},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 136 outbound references and 4 inbound Pith citation observations for arXiv:2504.15255."}