{"as_of":"2026-08-16T18:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:710e1fa0345d7c660d90d71a024c1f969098c87322d8f51790999f40d753b6a2","coverage":[{"denominator":188,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T00:14:35.857803Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.12471/citation-record","integrity":"/paper/2608.12471/integrity","json":"/paper/2608.12471/citation-record.json","paper":"/paper/2608.12471"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2304.13721","last_updated":"2024-03-06T15:08:08Z","snapshot_observed_at":"2026-08-16T15:37:27.872480Z","submitted_at":"2023-04-26T17:57:02Z","title":"EPOCHS Paper II: The Ultraviolet Luminosity Function from $7.5 6 galaxies in the Euclid Deep Fields ─ Forecasts and the first bright detections","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.441120Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:abeb432a45e6f1b435c653ce9943088ab366ce2537cdf1f2141629a69954d5ee","observation_id":"b6d6b2c1-8362-44ca-acda-d9c8e01896a2","resolution":{"observed_at":"2026-08-16T00:14:35.441120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.15431","last_updated":"2023-08-16T01:13:05Z","snapshot_observed_at":"2026-08-16T15:44:58.143029Z","submitted_at":"2023-03-27T17:54:38Z","title":"Confirmation and refutation of very luminous galaxies in the early universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.15431","snapshot_observed_at":"2026-08-16T00:14:35.445343Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.445343Z"},"links":{"cited_paper":"/paper/2303.15431","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:fc36af0975418d8f5ac096474f26d75d8df4b58e0cc11a44a5cebeb9b34cf18b","observation_id":"66faea4f-82db-4ccd-8efd-252e6a9bd6ab","resolution":{"observed_at":"2026-08-16T00:14:35.445343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.450630Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.450630Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:145340125fea9d4f220235e0a2c655f4bdcdf27ed824153bd7f29f70fe55d689","observation_id":"aa8ba516-ff21-4324-a697-e1948c3d634d","resolution":{"observed_at":"2026-08-16T00:14:35.450630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.454632Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.454632Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:f913d0f5f509aea0a1905d7409c0cb996614f8208d1eebae7d4bcefc809a7abf","observation_id":"ad89680d-e55c-44c2-9a31-278cd1ec545a","resolution":{"observed_at":"2026-08-16T00:14:35.454632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.458759Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.458759Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:81562fa6891256bbf0886c7f3f63f482ee66aac4c170746e3884327e3854fa83","observation_id":"f2abf2a1-e752-4a87-9973-e9a8960b45bd","resolution":{"observed_at":"2026-08-16T00:14:35.458759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14220","last_updated":"2022-06-28T18:01:54Z","snapshot_observed_at":"2026-07-06T13:25:39.576741Z","submitted_at":"2022-06-28T18:01:54Z","title":"The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.14220","snapshot_observed_at":"2026-08-16T00:14:35.463451Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.463451Z"},"links":{"cited_paper":"/paper/2206.14220","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:851ede768d66896f78c12a426ea99dee6b170747c9536f89669e3ca9e8b0ff5d","observation_id":"257ea1ae-2aab-4831-b5ec-eeeee871a06e","resolution":{"observed_at":"2026-08-16T00:14:35.463451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.02495","last_updated":"2022-11-04T14:52:24Z","snapshot_observed_at":"2026-08-16T16:18:34.641648Z","submitted_at":"2022-11-04T14:52:24Z","title":"CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.02495","snapshot_observed_at":"2026-08-16T00:14:35.467416Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.467416Z"},"links":{"cited_paper":"/paper/2211.02495","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:651aa5891f4783d2a4891f0e592094929eee444fb53203513873649ef6367464","observation_id":"f8ceb2e2-58d7-4bd7-9c03-7ba782ec2b2d","resolution":{"observed_at":"2026-08-16T00:14:35.467416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.471837Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.471837Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:8f23d046f3151f3ee140d6f47900523d02892c2c4081388a92bf6d41d25e3f84","observation_id":"0edc7c2b-537a-4c86-8eae-7dbc71a16eea","resolution":{"observed_at":"2026-08-16T00:14:35.471837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.13642","last_updated":"2023-01-24T08:31:48Z","snapshot_observed_at":"2026-08-16T16:36:13.497545Z","submitted_at":"2022-08-29T14:46:30Z","title":"Deep ALMA redshift search of a z~12 GLASS-JWST galaxy candidate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.13642","snapshot_observed_at":"2026-08-16T00:14:35.475853Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.475853Z"},"links":{"cited_paper":"/paper/2208.13642","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:63a12b352218ec3a6acbf3c5763a7574149e1d184b013d54cbcca02bc2ed8093","observation_id":"1c70d45d-fd7c-4c0f-96e3-61bac71be7d7","resolution":{"observed_at":"2026-08-16T00:14:35.475853Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.480090Z","title":"2016 , publisher =","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.480090Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:9caea87ca3567586cd102d11f681c89cd36e5434f741427acb33979ca1f3dbf9","observation_id":"f43a6b28-4393-4470-a593-c4153ed37d26","resolution":{"observed_at":"2026-08-16T00:14:35.480090Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/s1743921314010990","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:36.662215Z","title":"Proceedings of the International Astronomical Union , author=","venue":null,"work_id":"8d53356d-478b-4ca9-ae20-3050fc5f5697","year":2014},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.484173Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:b13f5b5855d55f865481a605d929cde330de35469e736be290d56012a0b5b3e8","observation_id":"dbf4dd39-9472-4064-ae1f-6b4619ead7e6","resolution":{"observed_at":"2026-08-16T00:14:36.667585Z","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":"2026-08-16T00:14:35.488322Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.488322Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:7a1573e328d535da0f00efaad22d74dd34fbee2908d68f3c1b12e614ba58ace1","observation_id":"6d66d1d4-0c4a-443d-9e93-09293a3180ef","resolution":{"observed_at":"2026-08-16T00:14:35.488322Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0309077","last_updated":"2003-09-02T20:59:24Z","snapshot_observed_at":"2026-07-07T00:35:59.955950Z","submitted_at":"2003-09-02T20:59:24Z","title":"Faint Galaxies in deep ACS observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0309077","snapshot_observed_at":"2026-08-16T00:14:35.492190Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.492190Z"},"links":{"cited_paper":"/paper/astro-ph/0309077","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:d1205477eaf52523ace58079bc2cacf92790f6acc7628410f0f28b4045ebced2","observation_id":"9cf5a59d-a254-4109-82c9-7c5aec8d2d82","resolution":{"observed_at":"2026-08-16T00:14:35.492190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.496483Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.496483Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e98cd216e8d52e9d56b77d67319c9630840b5552029da6073182f8bf12137ee8","observation_id":"f9ac2751-aedb-47ca-bfeb-5012d3901f7b","resolution":{"observed_at":"2026-08-16T00:14:35.496483Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.5270","last_updated":"2016-01-22T01:15:23Z","snapshot_observed_at":"2026-08-14T23:40:31.622168Z","submitted_at":"2014-03-20T20:00:33Z","title":"The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.5270","snapshot_observed_at":"2026-08-16T00:14:35.500331Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.500331Z"},"links":{"cited_paper":"/paper/1403.5270","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:20ee900dc8018b051cb93ba40a9275008a7de523fdcfc94f068115e328b522b8","observation_id":"67c9a313-ba6b-431f-98b5-c13a7404272d","resolution":{"observed_at":"2026-08-16T00:14:35.500331Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.504480Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.504480Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:698529ed96d11c7bbeadd70ade1fba6de66a218e44e70827648f117f0b7f1044","observation_id":"b1329b84-e9ee-46b4-befe-f78a6b5e32b4","resolution":{"observed_at":"2026-08-16T00:14:35.504480Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/167428","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:36.640395Z","title":", keywords =","venue":null,"work_id":"3c735f2b-09c2-4bdc-a10c-525af5311732","year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.508277Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:3f66f3ba235e636cbe760f5a097e6e3a3bf20da1c5539d23428145910b423427","observation_id":"83aba871-97f6-4f71-ba72-af9d21913e60","resolution":{"observed_at":"2026-08-16T00:14:36.644565Z","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":{"arxiv_id":"1908.11393","last_updated":"2019-08-29T18:00:10Z","snapshot_observed_at":"2026-08-14T10:14:14.583753Z","submitted_at":"2019-08-29T18:00:10Z","title":"Balmer breaks in simulated galaxies at z>6","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.11393","snapshot_observed_at":"2026-08-16T00:14:35.511965Z","title":", keywords =","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.511965Z"},"links":{"cited_paper":"/paper/1908.11393","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:905e850eb228027b146040710c117f5987b72569eff8837fbcabe1fe8433f8ff","observation_id":"cbc29719-6ad2-4d48-805e-15887cc150b8","resolution":{"observed_at":"2026-08-16T00:14:35.511965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.07074","last_updated":"2021-04-26T16:45:31Z","snapshot_observed_at":"2026-08-14T22:25:58.929252Z","submitted_at":"2020-11-13T19:00:01Z","title":"Simulating the infrared sky with a Spritz","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.07074","snapshot_observed_at":"2026-08-16T00:14:35.516299Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.516299Z"},"links":{"cited_paper":"/paper/2011.07074","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a4fff50516fbd9d31a2bac20dd63de5b780e025fb66bbe52d9ef31a485d25d8b","observation_id":"d391130f-890a-46d9-b79d-bfd114031b63","resolution":{"observed_at":"2026-08-16T00:14:35.516299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.11453","last_updated":"2021-11-22T19:00:05Z","snapshot_observed_at":"2026-08-16T17:40:07.342802Z","submitted_at":"2021-11-22T19:00:05Z","title":"Simulating infrared spectro-photometric surveys with a SPRITZ","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.11453","snapshot_observed_at":"2026-08-16T00:14:35.521120Z","title":", keywords =","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.521120Z"},"links":{"cited_paper":"/paper/2111.11453","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:51623a9a527d27393cb9c2e7a088febc1d193590cd4e613f5c5d9d0ee4056473","observation_id":"1cdc316b-7ca9-4c2f-b603-e1fd0caf66a7","resolution":{"observed_at":"2026-08-16T00:14:35.521120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.525596Z","title":"and Hoyle, F","venue":null,"work_id":null,"year":1944},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.525596Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:1edc73c7afadc121b3052cb793d6066a2917d602cd8072e188005eeb90baefde","observation_id":"b0776862-d051-42eb-82ea-6ac0865854fa","resolution":{"observed_at":"2026-08-16T00:14:35.525596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.02006","last_updated":"2016-09-07T14:52:09Z","snapshot_observed_at":"2026-08-14T21:40:57.333696Z","submitted_at":"2016-09-07T14:52:09Z","title":"Convolution kernels for multi-wavelength imaging","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.02006","snapshot_observed_at":"2026-08-16T00:14:35.529840Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.529840Z"},"links":{"cited_paper":"/paper/1609.02006","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:d44af3dc099a0773419b038715184a066c30546880f28896e2d881a038e144a1","observation_id":"19e481c6-e97e-4e8d-bea3-c58b9b6925ea","resolution":{"observed_at":"2026-08-16T00:14:35.529840Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.534041Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.534041Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:ef040ab3ff96fa0ab828abe8af33c7386b951fa33f6584ff76ec6fb3e1ff6a8d","observation_id":"25fceae7-700b-4085-8608-807baa76745e","resolution":{"observed_at":"2026-08-16T00:14:35.534041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0807.1533","last_updated":"2008-07-10T18:00:36Z","snapshot_observed_at":"2026-08-15T10:11:27.491954Z","submitted_at":"2008-07-10T18:00:36Z","title":"EAZY: A Fast, Public Photometric Redshift Code","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0807.1533","snapshot_observed_at":"2026-08-16T00:14:35.538123Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.538123Z"},"links":{"cited_paper":"/paper/0807.1533","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:c955f41d9cd7adb1731488892dc05bfc7eacbde471f14123aaaeae184b7fcc06","observation_id":"6077a9f0-2773-44e6-8b09-4afe14705d64","resolution":{"observed_at":"2026-08-16T00:14:35.538123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.542262Z","title":"doi:10.5281/zenodo.8319596 , url =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.542262Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:81adafb4bfabc325fe7d281093f5ea8097a97bad94820c4b2f897e54a94de25b","observation_id":"ab896d84-e3bf-446c-a768-159dfc7a9635","resolution":{"observed_at":"2026-08-16T00:14:35.542262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.546962Z","title":"Spectral evolution of galaxies","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.546962Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:29569e4d3367f5a2eb4287127c8e48fa8cef34b34dc9d3c6113b5a7a8520e8c6","observation_id":"d0838047-a434-4b1c-810a-c0d442f4774d","resolution":{"observed_at":"2026-08-16T00:14:35.546962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.551128Z","title":", keywords =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.551128Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e07092625f2f71155e1f7b6f91e03d7652dffe60031af7c1e4b6c304a80f955b","observation_id":"160ff0be-ea8a-4dbc-b13d-28f564d50a6d","resolution":{"observed_at":"2026-08-16T00:14:35.551128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.08452","last_updated":"2024-02-13T13:39:37Z","snapshot_observed_at":"2026-08-16T14:18:59.072326Z","submitted_at":"2024-02-13T13:39:37Z","title":"The SRG/eROSITA All-Sky Survey: The first catalog of galaxy clusters and groups in the Western Galactic Hemisphere","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.08452","snapshot_observed_at":"2026-08-16T00:14:35.555245Z","title":"The first catalog of galaxy clusters and groups in the Western Galactic Hemisphere","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.555245Z"},"links":{"cited_paper":"/paper/2402.08452","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:880e6ae743e0c85744425c87b3976400eb301a8acda5e2ed2d0828c8ff45336b","observation_id":"2bd587f1-1850-41c7-b89d-1505f006bd99","resolution":{"observed_at":"2026-08-16T00:14:35.555245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.02467","last_updated":"2024-05-31T16:07:03Z","snapshot_observed_at":"2026-08-16T15:26:44.079526Z","submitted_at":"2023-06-04T20:44:23Z","title":"JADES NIRSpec Initial Data Release for the Hubble Ultra Deep Field: Redshifts and Line Fluxes of Distant Galaxies from the Deepest JWST Cycle 1 NIRSpec Multi-Object Spectroscopy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.02467","snapshot_observed_at":"2026-08-16T00:14:35.559393Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.559393Z"},"links":{"cited_paper":"/paper/2306.02467","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e161e65dd1af16cab09660c7c0b6441b3b78817f0901c8510e0b44dcace2c35f","observation_id":"2366ca09-ce2c-4fb3-9fb1-41d3dcca437e","resolution":{"observed_at":"2026-08-16T00:14:35.559393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.1629","last_updated":"2014-10-07T07:18:24Z","snapshot_observed_at":"2026-08-14T23:16:43.246190Z","submitted_at":"2014-10-07T07:18:24Z","title":"SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.1629","snapshot_observed_at":"2026-08-16T00:14:35.564007Z","title":"Astronomy and Computing , keywords =","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.564007Z"},"links":{"cited_paper":"/paper/1410.1629","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:4fc83527d589efa98a1acd0df03c7ca457c1037c474fb9b2fab54b8a5b210faa","observation_id":"737d0929-a07c-48c4-a896-b5de5cfa6266","resolution":{"observed_at":"2026-08-16T00:14:35.564007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.568437Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.568437Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:fdc2490ec86d36797d2ea265cd31a3afe8d4d920d0da88b91714c9fc08100c40","observation_id":"c641e8b4-5fed-4583-8214-2603ee92dca1","resolution":{"observed_at":"2026-08-16T00:14:35.568437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9911459","last_updated":"1999-11-24T20:56:27Z","snapshot_observed_at":"2026-08-04T15:42:16.020141Z","submitted_at":"1999-11-24T20:56:27Z","title":"The Dust Content and Opacity of Actively Star-Forming Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9911459","snapshot_observed_at":"2026-08-16T00:14:35.572456Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.572456Z"},"links":{"cited_paper":"/paper/astro-ph/9911459","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:89288a882f2ae003fa5d84da818aeef4a4441a2b0b5511d6a3c1a40e1a5498f0","observation_id":"4d88eca6-f619-4779-9807-04c438eb0d0d","resolution":{"observed_at":"2026-08-16T00:14:35.572456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.04452","last_updated":"2024-02-06T20:24:26Z","snapshot_observed_at":"2026-08-14T05:13:33.583805Z","submitted_at":"2017-12-12T19:00:01Z","title":"Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.04452","snapshot_observed_at":"2026-08-16T00:14:35.576809Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.576809Z"},"links":{"cited_paper":"/paper/1712.04452","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a5e0c13ae81091216ac16dff0a4e01856ec70ba81ea431557f0f95d798c3fab3","observation_id":"cd11afb7-1582-4244-b32a-4a9c3dd9cbd2","resolution":{"observed_at":"2026-08-16T00:14:35.576809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18485","last_updated":"2024-09-20T07:20:10Z","snapshot_observed_at":"2026-08-16T13:48:29.615362Z","submitted_at":"2024-05-28T18:00:06Z","title":"Spectroscopic confirmation of two luminous galaxies at $z\\sim14$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.18485","snapshot_observed_at":"2026-08-16T00:14:35.580893Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.580893Z"},"links":{"cited_paper":"/paper/2405.18485","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:573038ee4e7853135397ca5ff9111fbeaff77e642d4b6dc341a4ef958c51c5a7","observation_id":"da92d7fc-9f99-4f16-bb09-c5148b7b54c5","resolution":{"observed_at":"2026-08-16T00:14:35.580893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.08985","last_updated":"2018-05-23T07:33:29Z","snapshot_observed_at":"2026-08-14T19:12:11.046349Z","submitted_at":"2018-05-23T07:33:29Z","title":"GLACiAR, an open-source python tool for simulations of source recovery and completeness in galaxy surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.08985","snapshot_observed_at":"2026-08-16T00:14:35.584949Z","title":", keywords =","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.584949Z"},"links":{"cited_paper":"/paper/1805.08985","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:9c6bc9f37145a766a50d28dada5b94ee1f462f65b17136b657f445c130113dbf","observation_id":"1641876e-a473-4ba2-9016-44de2cf65cf6","resolution":{"observed_at":"2026-08-16T00:14:35.584949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0304382","last_updated":"2003-07-09T01:38:17Z","snapshot_observed_at":"2026-08-14T16:34:27.563513Z","submitted_at":"2003-04-22T15:16:01Z","title":"Galactic Stellar and Substellar Initial Mass Function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0304382","snapshot_observed_at":"2026-08-16T00:14:35.589153Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.589153Z"},"links":{"cited_paper":"/paper/astro-ph/0304382","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:dd21684bf84f12c88a7ecb118a719e730159d197ef7395fe7e5acced0e0ad1cd","observation_id":"5ad5b7cf-d345-4341-ac1a-e99559abdcd6","resolution":{"observed_at":"2026-08-16T00:14:35.589153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003128","last_updated":"2000-03-09T07:29:19Z","snapshot_observed_at":"2026-08-11T08:36:37.085392Z","submitted_at":"2000-03-09T07:29:19Z","title":"A Simple Model for the Absorption of Starlight by Dust in Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0003128","snapshot_observed_at":"2026-08-16T00:14:35.593121Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.593121Z"},"links":{"cited_paper":"/paper/astro-ph/0003128","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e113273cf16a43bc58f569696aca221204ea9f87284b74bde66673b327743da5","observation_id":"73f37085-73f7-4722-be51-0e349cc16d3a","resolution":{"observed_at":"2026-08-16T00:14:35.593121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.03037","last_updated":"2016-10-05T12:38:29Z","snapshot_observed_at":"2026-08-15T22:21:07.629474Z","submitted_at":"2016-03-09T21:00:00Z","title":"Modelling and interpreting spectral energy distributions of galaxies with BEAGLE","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.03037","snapshot_observed_at":"2026-08-16T00:14:35.597445Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.597445Z"},"links":{"cited_paper":"/paper/1603.03037","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a59a107f59808ba35cf6feaf7f33ff17f5f7d9c6cf29427f3eaa920d2de8d0a9","observation_id":"294ef3cf-306f-41ce-8e36-6e491f1f5944","resolution":{"observed_at":"2026-08-16T00:14:35.597445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06015","last_updated":"2018-07-16T18:00:00Z","snapshot_observed_at":"2026-08-14T18:51:24.598131Z","submitted_at":"2018-07-16T18:00:00Z","title":"ALMA [CI]$^{3}P_{1}-^{3}P_{0}$ observations of NGC6240: a puzzling molecular outflow, and the role of outflows in the global $\\alpha_{\\rm CO}$ factor of (U)LIRGs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06015","snapshot_observed_at":"2026-08-16T00:14:35.601504Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.601504Z"},"links":{"cited_paper":"/paper/1807.06015","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:8cd812f4ce911091dae07a91d83fe92d6b1a22d7762f563a9221c102c936ae87","observation_id":"2527e296-98c9-4102-80b8-54f03c15c78d","resolution":{"observed_at":"2026-08-16T00:14:35.601504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.605444Z","title":"Modeling the Panchromatic Spectral Energy Distributions of Galaxies , type =","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.605444Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:6413c2c28b4a481b863dae5a66a6769ab836b2a247a11c307e068ae0fe6bc751","observation_id":"fb5068d3-995d-4a24-9b31-443d55c5b7af","resolution":{"observed_at":"2026-08-16T00:14:35.605444Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.11611","last_updated":"2024-11-18T20:03:01Z","snapshot_observed_at":"2026-08-16T13:42:14.101711Z","submitted_at":"2024-06-17T14:58:23Z","title":"Wide Area VISTA Extra-galactic Survey (WAVES): Unsupervised star-galaxy separation on the WAVES-Wide photometric input catalogue using UMAP and ${\\rm{\\scriptsize HDBSCAN}}$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.11611","snapshot_observed_at":"2026-08-16T00:14:35.609181Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.609181Z"},"links":{"cited_paper":"/paper/2406.11611","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:ecc176e812d5d098a62d2cf13824a8e8d374ba2577f9f4050e8e1df3d4b0bc70","observation_id":"d627d665-ad20-48a8-ac50-2e8c4dc1d86f","resolution":{"observed_at":"2026-08-16T00:14:35.609181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.17075","last_updated":"2023-09-29T09:10:48Z","snapshot_observed_at":"2026-08-16T14:56:35.326889Z","submitted_at":"2023-09-29T09:10:48Z","title":"Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.17075","snapshot_observed_at":"2026-08-16T00:14:35.613712Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.613712Z"},"links":{"cited_paper":"/paper/2309.17075","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a596a550b948b2797f05f2ef5452eeabaacd958bd1cbf0dcf0b997d5f0c0f202","observation_id":"88219b07-2b7f-4fd6-ae48-7f883aae8885","resolution":{"observed_at":"2026-08-16T00:14:35.613712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.11017","last_updated":"2024-04-17T02:48:13Z","snapshot_observed_at":"2026-08-16T14:00:17.245792Z","submitted_at":"2024-04-17T02:48:13Z","title":"SPHEREx: NASA's Near-Infrared Spectrophotmetric All-Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.11017","snapshot_observed_at":"2026-08-16T00:14:35.617757Z","title":"Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave , year = 2020, editor =","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.617757Z"},"links":{"cited_paper":"/paper/2404.11017","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:4e99ae3971b26a88b5753f2a534ca38afe67fd8624af2bcaf49c5ae788d58752","observation_id":"b5254a38-c5fd-4f46-bf7f-06128c31202b","resolution":{"observed_at":"2026-08-16T00:14:35.617757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.621668Z","title":", keywords =","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.621668Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:20765984b78e469a2c48e631f81d58568612a543cda0e48fa659a14e06ea06d8","observation_id":"59907400-e27b-4a27-bd49-3f0cb51b5eda","resolution":{"observed_at":"2026-08-16T00:14:35.621668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.04709","last_updated":"2016-01-22T02:02:26Z","snapshot_observed_at":"2026-08-16T05:59:05.879344Z","submitted_at":"2016-01-18T21:00:04Z","title":"Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.04709","snapshot_observed_at":"2026-08-16T00:14:35.625479Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.625479Z"},"links":{"cited_paper":"/paper/1601.04709","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e0eedbe4f53e45b8c5551251de4025a5a4e66af001423803b694001a05e9fa23","observation_id":"5680cca3-f542-4aa8-8c47-ba8d5e3a909f","resolution":{"observed_at":"2026-08-16T00:14:35.625479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.5353","last_updated":"2013-08-24T18:37:56Z","snapshot_observed_at":"2026-08-15T06:15:43.823146Z","submitted_at":"2013-08-24T18:37:56Z","title":"A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.5353","snapshot_observed_at":"2026-08-16T00:14:35.629602Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.629602Z"},"links":{"cited_paper":"/paper/1308.5353","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:2c90b822cf0fc54e75a8d637ae719ba6cf0f31d964d731bc6a2f58d9c4cec2a3","observation_id":"53e6c3e9-58cf-4008-aff8-4757e3e0ec25","resolution":{"observed_at":"2026-08-16T00:14:35.629602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.02335","last_updated":"2023-07-06T05:24:06Z","snapshot_observed_at":"2026-08-16T15:18:32.549486Z","submitted_at":"2023-07-05T14:43:27Z","title":"The Classification of Galaxy Morphology in H-band of COSMOS-DASH Field: a combination-based machine learning clustering model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.02335","snapshot_observed_at":"2026-08-16T00:14:35.633554Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.633554Z"},"links":{"cited_paper":"/paper/2307.02335","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:ff6fd5e115c8c4f00c07c8073d7d01844c90f1b048d43782afde5e7023cd63f3","observation_id":"64737d2f-5a08-47ac-9c7a-c335e477cfd5","resolution":{"observed_at":"2026-08-16T00:14:35.633554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.637887Z","title":", year = 1964, month = jan, volume =","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.637887Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a74bb822163c05bad6c38f147ae44b4a68ff9735e618ef4134010bac6d9fe679","observation_id":"3641c43f-2c12-4166-87f5-9ebf621e5d16","resolution":{"observed_at":"2026-08-16T00:14:35.637887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9906332","last_updated":"1999-06-24T10:32:24Z","snapshot_observed_at":"2026-08-15T11:03:56.862915Z","submitted_at":"1999-06-21T10:59:48Z","title":"Galaxy Modelling -- I. Spectral Energy Distributions from Far-UV to Sub-mm Wavelengths","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9906332","snapshot_observed_at":"2026-08-16T00:14:35.641703Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.641703Z"},"links":{"cited_paper":"/paper/astro-ph/9906332","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:9704f25df114e7d818bfbbd37c36432a4c34fe8775f4863d7887fe0d2868129f","observation_id":"00ed6953-aa1f-40cb-97ba-afc6df479ffe","resolution":{"observed_at":"2026-08-16T00:14:35.641703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10714","last_updated":"2019-06-20T21:00:59Z","snapshot_observed_at":"2026-08-14T17:10:07.634839Z","submitted_at":"2019-02-27T19:00:01Z","title":"Atomic and molecular gas in IllustrisTNG galaxies at low redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10714","snapshot_observed_at":"2026-08-16T00:14:35.645963Z","title":", keywords =","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.645963Z"},"links":{"cited_paper":"/paper/1902.10714","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:5a4594092b833beeb3b3b8e6cdc3e3939bd109ee9b1407b1d41d509015f6947e","observation_id":"24ea760f-a739-4d34-bf39-ac017b0473ec","resolution":{"observed_at":"2026-08-16T00:14:35.645963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00558","last_updated":"2018-11-01T18:00:01Z","snapshot_observed_at":"2026-08-16T05:39:28.808168Z","submitted_at":"2018-11-01T18:00:01Z","title":"A Review of the Theory of Galactic Winds Driven by Stellar Feedback","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.00558","snapshot_observed_at":"2026-08-16T00:14:35.650094Z","title":"Galaxies , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.650094Z"},"links":{"cited_paper":"/paper/1811.00558","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e720ec376b9fea38fe5d2abfc5d96dde9c75c27c08a3e4771ba40fb6308479b3","observation_id":"0f6073de-18a0-43f9-a792-468ae4ef5e77","resolution":{"observed_at":"2026-08-16T00:14:35.650094Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03171","last_updated":"2024-08-24T09:47:08Z","snapshot_observed_at":"2026-08-16T14:12:33.395986Z","submitted_at":"2024-03-05T18:06:01Z","title":"JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\\mathbf{z \\simeq 9-15}$","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03171","snapshot_observed_at":"2026-08-16T00:14:35.654079Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.654079Z"},"links":{"cited_paper":"/paper/2403.03171","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:8899163e6141ebbc1b23bbe98423da141c1878c66046c8f8e78d4bb8313cf207","observation_id":"52afef63-941b-452d-894a-f2ecbb500394","resolution":{"observed_at":"2026-08-16T00:14:35.654079Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.658337Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.658337Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:92751d6f6143031d551995d289fb580f35bd36ea6f3a0f34c99fa573346b5715","observation_id":"eeffd09a-f351-4e27-a1de-09db12d509ba","resolution":{"observed_at":"2026-08-16T00:14:35.658337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.662265Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.662265Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:c4c8cf216f8fea4e6c3ce08778be33f7345b19e9fe286f904c40e5da055d44b5","observation_id":"2132d39f-1873-4182-95ea-be567c70f92f","resolution":{"observed_at":"2026-08-16T00:14:35.662265Z","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":"2026-08-16T00:14:35.665782Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.665782Z"},"links":{"cited_paper":"/paper/2306.02465","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:fbbd2c880fd2126126443cc12e5a7670d00713baccf9b1a15024fc3d62f425b5","observation_id":"f44c1779-b7f2-4324-b032-047c58cd2583","resolution":{"observed_at":"2026-08-16T00:14:35.665782Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.4114","last_updated":"2012-04-18T15:56:34Z","snapshot_observed_at":"2026-08-15T04:12:39.569546Z","submitted_at":"2012-04-18T15:56:34Z","title":"Observational Evidence of AGN Feedback","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.4114","snapshot_observed_at":"2026-08-16T00:14:35.670394Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.670394Z"},"links":{"cited_paper":"/paper/1204.4114","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:32c9fcfcf7bba5c3104ce2b87489c0482c8c63dd5258ca973b1ba46330fed624","observation_id":"09e5418d-59d3-4755-b5f7-df8b6d33ee67","resolution":{"observed_at":"2026-08-16T00:14:35.670394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0512082","last_updated":"2006-03-19T04:20:18Z","snapshot_observed_at":"2026-08-05T23:28:57.001095Z","submitted_at":"2005-12-04T17:04:02Z","title":"Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z ~ 6 Quasars II: A Sample of 19 Quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0512082","snapshot_observed_at":"2026-08-16T00:14:35.675067Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.675067Z"},"links":{"cited_paper":"/paper/astro-ph/0512082","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:603fec81fc6869fb60dcc97c77ded84ab6e29ae8dfe4619d0f753c8e6c6d84ba","observation_id":"71e97869-84c8-4bd1-bac5-58cf370c24b8","resolution":{"observed_at":"2026-08-16T00:14:35.675067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.08217","last_updated":"2015-11-25T21:00:05Z","snapshot_observed_at":"2026-08-14T22:21:17.752310Z","submitted_at":"2015-11-25T21:00:05Z","title":"Nuclear activity versus star formation: emission-line diagnostics at ultraviolet and optical wavelengths","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.08217","snapshot_observed_at":"2026-08-16T00:14:35.679116Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.679116Z"},"links":{"cited_paper":"/paper/1511.08217","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:7e9070b73f452a791e734b80f00ba93c6f7a91ed2d1e94791d71c4ac6a382164","observation_id":"82ef9a97-2079-400a-88e3-3b6739fe8c95","resolution":{"observed_at":"2026-08-16T00:14:35.679116Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.4485","last_updated":"2013-02-18T23:53:08Z","snapshot_observed_at":"2026-08-15T00:28:19.568644Z","submitted_at":"2013-02-18T23:53:08Z","title":"The 2013 Release of Cloudy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.4485","snapshot_observed_at":"2026-08-16T00:14:35.682812Z","title":", keywords =","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.682812Z"},"links":{"cited_paper":"/paper/1302.4485","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:696a6d60d9385d30fd5d9024f7d89bff60cc02ccd6cde797fe662345689eeb27","observation_id":"efb7dfd3-07e6-42fa-b35c-d8393a395b87","resolution":{"observed_at":"2026-08-16T00:14:35.682812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.5439","last_updated":"2015-06-06T07:43:33Z","snapshot_observed_at":"2026-08-14T23:14:59.176661Z","submitted_at":"2014-10-20T20:00:40Z","title":"The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.5439","snapshot_observed_at":"2026-08-16T00:14:35.686826Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.686826Z"},"links":{"cited_paper":"/paper/1410.5439","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:9912a6765cfc896cfc788e786436a27be65c35b4a2935739c91fc77c056f958e","observation_id":"32322201-e738-4697-bc83-d769f83faf10","resolution":{"observed_at":"2026-08-16T00:14:35.686826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.13813","last_updated":"2021-11-19T21:40:03Z","snapshot_observed_at":"2026-08-16T18:14:25.075691Z","submitted_at":"2021-06-25T18:00:02Z","title":"A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.13813","snapshot_observed_at":"2026-08-16T00:14:35.690863Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.690863Z"},"links":{"cited_paper":"/paper/2106.13813","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:fef22562fe806be694c9a7d27f1af791a2a8bd2123b7e1b76974daddda28c3db","observation_id":"323b73e1-f6bf-447c-992c-80fd24d4f7da","resolution":{"observed_at":"2026-08-16T00:14:35.690863Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.04279","last_updated":"2023-11-07T19:00:03Z","snapshot_observed_at":"2026-08-16T14:45:10.237053Z","submitted_at":"2023-11-07T19:00:03Z","title":"The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.04279","snapshot_observed_at":"2026-08-16T00:14:35.695324Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.695324Z"},"links":{"cited_paper":"/paper/2311.04279","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:0144c6448d7f2aee23242f762df37bc996776859241db59e5962c57ced6f5e02","observation_id":"67aae2b3-a12e-4872-b93c-0a80c28c58e5","resolution":{"observed_at":"2026-08-16T00:14:35.695324Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.04085","last_updated":"2025-01-07T19:00:02Z","snapshot_observed_at":"2026-08-16T04:41:42.045802Z","submitted_at":"2025-01-07T19:00:02Z","title":"The Cosmic Evolution Early Release Science Survey (CEERS)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.04085","snapshot_observed_at":"2026-08-16T00:14:35.699568Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.699568Z"},"links":{"cited_paper":"/paper/2501.04085","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:3abf891c0f4a97e033240692a6e35988f32c2df6b2a7e8a108515bd4c5fd4925","observation_id":"27aad07b-b2a7-4259-ac7c-0d5e9af5713e","resolution":{"observed_at":"2026-08-16T00:14:35.699568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.19166","last_updated":"2023-08-01T17:27:53Z","snapshot_observed_at":"2026-08-16T15:28:15.099737Z","submitted_at":"2023-05-30T16:12:12Z","title":"FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.19166","snapshot_observed_at":"2026-08-16T00:14:35.703814Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.703814Z"},"links":{"cited_paper":"/paper/2305.19166","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:1debf35005567b976ef1423f0a8b1d4ac0466943f62d0f9abe19fd17cf702722","observation_id":"339d3baf-0299-4a6f-900f-5fa6fa12ac25","resolution":{"observed_at":"2026-08-16T00:14:35.703814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.04153","last_updated":"2016-09-14T07:23:20Z","snapshot_observed_at":"2026-08-14T21:39:56.797989Z","submitted_at":"2016-09-14T07:23:20Z","title":"The Gaia mission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.04153","snapshot_observed_at":"2026-08-16T00:14:35.707897Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.707897Z"},"links":{"cited_paper":"/paper/1609.04153","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:80712520612ff70146b857c7223b0a58320d04f257a00560c85da3e5782305af","observation_id":"d099b86a-5398-4449-8823-d68fabf72746","resolution":{"observed_at":"2026-08-16T00:14:35.707897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.00211","last_updated":"2022-07-30T13:18:15Z","snapshot_observed_at":"2026-08-16T16:42:17.573519Z","submitted_at":"2022-07-30T13:18:15Z","title":"Gaia Data Release 3: Summary of the content and survey properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.00211","snapshot_observed_at":"2026-08-16T00:14:35.711885Z","title":"Summary of the content and survey properties","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.711885Z"},"links":{"cited_paper":"/paper/2208.00211","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a41b05a8ca06cd97a63554cf9a9ad36b39ac09705b20167931e41645518ce9f3","observation_id":"f9d2141e-f55a-47fc-a9a3-2a6945ef3634","resolution":{"observed_at":"2026-08-16T00:14:35.711885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.1823","last_updated":"2013-05-06T18:48:02Z","snapshot_observed_at":"2026-08-15T08:20:19.304270Z","submitted_at":"2013-05-06T18:48:02Z","title":"CANDELS Multiwavelength catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-Deep Survey Field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.1823","snapshot_observed_at":"2026-08-16T00:14:35.715852Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.715852Z"},"links":{"cited_paper":"/paper/1305.1823","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:9fdcbb812717d010a3867226f0a68658a802408319221d9041dabc95c8158fb8","observation_id":"1ff47c4b-92af-43d2-b513-8a8d5cb2c34b","resolution":{"observed_at":"2026-08-16T00:14:35.715852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9711093","last_updated":"1997-11-10T16:05:51Z","snapshot_observed_at":"2026-08-13T10:38:42.089906Z","submitted_at":"1997-11-10T16:05:51Z","title":"The ESO-Sculptor Survey: Spectral classification of galaxies with z < 0.5","version":1},"cited_work":{"arxiv_id":"astro-ph/9711093","doi":"10.48550/arxiv.astro-ph/9711093","metadata_source":"pith","pith_arxiv_id":"astro-ph/9711093","snapshot_observed_at":"2026-08-16T12:16:17.039197Z","title":"The ESO-Sculptor Survey: Spectral classification of galaxies with z < 0.5","venue":"astro-ph","work_id":"8b98c7f0-7790-4c2e-94e9-22a30417ee3d","year":1997},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.719717Z"},"links":{"cited_paper":"/paper/astro-ph/9711093","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:0bffc88455892ac481d530d7894b24caf722ba4789b93682947d9f9d465820a1","observation_id":"786ea4e3-f6c0-4c12-851d-ea6d4b7b1343","resolution":{"observed_at":"2026-08-16T00:14:36.565561Z","resolver_source":"local_arxiv","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":"2502.02637","last_updated":"2026-01-16T16:03:52Z","snapshot_observed_at":"2026-08-02T05:15:17.075129Z","submitted_at":"2025-02-04T19:00:01Z","title":"Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.02637","snapshot_observed_at":"2026-08-16T00:14:35.723738Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.723738Z"},"links":{"cited_paper":"/paper/2502.02637","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:d4d130e6e75f9c1b9af1afdc0b2188111d2ef7728e5bd9fad8e30c3fbc0a29b0","observation_id":"976f5146-f538-4074-a811-a048138bbb91","resolution":{"observed_at":"2026-08-16T00:14:35.723738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0002151","last_updated":"2000-05-04T18:28:34Z","snapshot_observed_at":"2026-08-02T23:43:31.938839Z","submitted_at":"2000-02-07T16:14:36Z","title":"Effect of Reionization on the Structure Formation in the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0002151","snapshot_observed_at":"2026-08-16T00:14:35.728338Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.728338Z"},"links":{"cited_paper":"/paper/astro-ph/0002151","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a8920ff4bee37f654960cbb986e3453ad4de3b5d5d81c7d3c8d410846e674f42","observation_id":"add85f59-089b-4a5b-93ec-0b93887a4b4c","resolution":{"observed_at":"2026-08-16T00:14:35.728338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.0003","last_updated":"2010-03-31T20:00:06Z","snapshot_observed_at":"2026-08-15T15:37:46.656730Z","submitted_at":"2010-03-31T20:00:06Z","title":"Environmental Dependence of the Kennicutt-Schmidt Relation in Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.0003","snapshot_observed_at":"2026-08-16T00:14:35.732302Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.732302Z"},"links":{"cited_paper":"/paper/1004.0003","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:b80077fc84fd1e9473419c0c99aa4931bdb592a62308de1672b0e3f22955ac95","observation_id":"91ed4856-979d-4294-bf37-1eb424249700","resolution":{"observed_at":"2026-08-16T00:14:35.732302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0503176","last_updated":"2005-03-08T10:14:42Z","snapshot_observed_at":"2026-08-16T06:54:22.243675Z","submitted_at":"2005-03-08T10:14:42Z","title":"A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0503176","snapshot_observed_at":"2026-08-16T00:14:35.736516Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.736516Z"},"links":{"cited_paper":"/paper/astro-ph/0503176","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:89cdb84ba17f29bee43de57b46383082731c396619721de3ab56a19e73b36f8c","observation_id":"e73e3ef6-9597-42a5-b26d-f70926638ef7","resolution":{"observed_at":"2026-08-16T00:14:35.736516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.5209","last_updated":"2013-07-25T15:35:10Z","snapshot_observed_at":"2026-08-15T00:28:00.317564Z","submitted_at":"2013-02-21T08:21:24Z","title":"The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.5209","snapshot_observed_at":"2026-08-16T00:14:35.741522Z","title":"Probing the evolution of PACS selected Galaxies to z ≃ 4","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.741522Z"},"links":{"cited_paper":"/paper/1302.5209","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a6644d1e3cb11f355f5011ba3efc2a04424b416f70c047e0030cd119b85ec083","observation_id":"2458b0a0-7cd2-4616-b845-529c64911cac","resolution":{"observed_at":"2026-08-16T00:14:35.741522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03250","last_updated":"2024-01-19T17:55:17Z","snapshot_observed_at":"2026-08-16T15:02:46.039374Z","submitted_at":"2023-09-06T17:10:20Z","title":"Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03250","snapshot_observed_at":"2026-08-16T00:14:35.746564Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.746564Z"},"links":{"cited_paper":"/paper/2309.03250","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:47750dd95b3b7418bccbbafa2bb67748c56fd5bd46d9054c71df6047ea203854","observation_id":"b81d6b67-a3d7-4349-b95c-27d3f6216226","resolution":{"observed_at":"2026-08-16T00:14:35.746564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.02468","last_updated":"2024-01-11T18:18:47Z","snapshot_observed_at":"2026-08-16T15:26:44.157480Z","submitted_at":"2023-06-04T20:44:24Z","title":"The Cosmos in its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.02468","snapshot_observed_at":"2026-08-16T00:14:35.751516Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.751516Z"},"links":{"cited_paper":"/paper/2306.02468","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:cd25131f0d86b3f331c8ab893f36981e043de7d18ca640f7767ef1a0bd9900e2","observation_id":"d50c4aae-53ff-4608-b6df-ec884d33c549","resolution":{"observed_at":"2026-08-16T00:14:35.751516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.756338Z","title":"Harris and K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.756338Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:25a814c485741a868ae6a0a6aae2334f9e91cb089a2b14ffc3d9170b18dcf04c","observation_id":"0d8beff2-c951-4cb5-a9e7-605963c539ef","resolution":{"observed_at":"2026-08-16T00:14:35.756338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03908","last_updated":"2025-02-11T17:00:12Z","snapshot_observed_at":"2026-08-16T14:12:13.259619Z","submitted_at":"2024-03-06T18:14:21Z","title":"EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03908","snapshot_observed_at":"2026-08-16T00:14:35.760756Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.760756Z"},"links":{"cited_paper":"/paper/2403.03908","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:55c3c2a70d3d87997bcd1572ddb1939bc0a053f9f08abf6a477d675ced1ae8e6","observation_id":"e51a80db-aa28-4f41-8d3c-620247d6fb5f","resolution":{"observed_at":"2026-08-16T00:14:35.760756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.765489Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.765489Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e37d0f9a1e41e355bbfc93d510c51631bb1e329dfe3c7d8701aaeaa57dcb7436","observation_id":"280f6c5a-6f47-481e-9147-531c279d0bdf","resolution":{"observed_at":"2026-08-16T00:14:35.765489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.06877","last_updated":"2023-02-06T11:11:44Z","snapshot_observed_at":"2026-08-16T16:08:53.301681Z","submitted_at":"2022-12-13T19:49:06Z","title":"The gas and stellar content of a metal-poor galaxy at $z=8.496$ as revealed by JWST and ALMA","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.06877","snapshot_observed_at":"2026-08-16T00:14:35.770283Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.770283Z"},"links":{"cited_paper":"/paper/2212.06877","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:8111af7d4339287fb84a1da08632e9a99e3ab8213dc410e9db611641f98d5eea","observation_id":"256ecdd5-8595-4448-aead-fc8be03e311f","resolution":{"observed_at":"2026-08-16T00:14:35.770283Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.00647","last_updated":"2023-06-01T13:14:39Z","snapshot_observed_at":"2026-08-16T15:27:31.679857Z","submitted_at":"2023-06-01T13:14:39Z","title":"Extreme damped Lyman-$\\alpha$ absorption in young star-forming galaxies at $z=9-11$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.00647","snapshot_observed_at":"2026-08-16T00:14:35.774963Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.774963Z"},"links":{"cited_paper":"/paper/2306.00647","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:a2a06a998c9772063c04d29ae3a0a5b36ea23c8dc52d9671b9be5483f0906028","observation_id":"b48eba7e-7260-4b3b-830a-e359f9007222","resolution":{"observed_at":"2026-08-16T00:14:35.774963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.02211","last_updated":"2024-04-02T18:03:18Z","snapshot_observed_at":"2026-08-16T14:04:12.289519Z","submitted_at":"2024-04-02T18:03:18Z","title":"The JWST-PRIMAL Legacy Survey. A JWST/NIRSpec reference sample for the physical properties and Lyman-$\\alpha$ absorption and emission of $\\sim 500$ galaxies at $z=5.5-13.4$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.02211","snapshot_observed_at":"2026-08-16T00:14:35.779839Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.779839Z"},"links":{"cited_paper":"/paper/2404.02211","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:9205331a8435532c977641ef4915d0c663d03484707265ecd42387abad571313","observation_id":"550faae8-8f0a-4847-9fa8-60dcdd7cebdf","resolution":{"observed_at":"2026-08-16T00:14:35.779839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.00010","last_updated":"2017-08-31T16:38:13Z","snapshot_observed_at":"2026-08-14T20:56:54.223709Z","submitted_at":"2017-05-31T18:00:01Z","title":"Synthetic nebular emission from massive galaxies I: origin of the cosmic evolution of optical emission-line ratios","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.00010","snapshot_observed_at":"2026-08-16T00:14:35.788549Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.788549Z"},"links":{"cited_paper":"/paper/1706.00010","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:8b9d6da707e1747bf23fb3f6c3b79bbe0915a82c5d8959108a0affa597319ef1","observation_id":"c0e4b95d-334a-4f89-b279-df6a74c2207b","resolution":{"observed_at":"2026-08-16T00:14:35.788549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.07909","last_updated":"2018-11-19T19:00:02Z","snapshot_observed_at":"2026-08-14T17:56:36.317275Z","submitted_at":"2018-11-19T19:00:02Z","title":"Synthetic nebular emission from massive galaxies II: ultraviolet-line diagnostics of dominant ionizing sources","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.07909","snapshot_observed_at":"2026-08-16T00:14:35.792663Z","title":"Ultraviolet-line diagnostics of dominant ionizing sources","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.792663Z"},"links":{"cited_paper":"/paper/1811.07909","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:6b57f93a2abb94f903ef319c89ee9e43072c33c06e942f03ccafead70dcf3bfc","observation_id":"e8bd7fde-0605-4ae1-ba38-5e33c5af6146","resolution":{"observed_at":"2026-08-16T00:14:35.792663Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.02522","last_updated":"2022-12-05T19:00:03Z","snapshot_observed_at":"2026-08-16T16:10:50.663383Z","submitted_at":"2022-12-05T19:00:03Z","title":"Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.02522","snapshot_observed_at":"2026-08-16T00:14:35.796834Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.796834Z"},"links":{"cited_paper":"/paper/2212.02522","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:57497c556cac6fb3647b0e2f98144b73b9ed33b896406ae7dbf433a001b441b7","observation_id":"94f5b38f-9f11-4e34-b45c-0c72588ee21c","resolution":{"observed_at":"2026-08-16T00:14:35.796834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.15611","last_updated":"2022-03-29T14:23:55Z","snapshot_observed_at":"2026-08-16T17:10:55.044489Z","submitted_at":"2022-03-29T14:23:55Z","title":"Galaxy And Mass Assembly (GAMA): Self-Organizing Map Application on Nearby Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.15611","snapshot_observed_at":"2026-08-16T00:14:35.801318Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.801318Z"},"links":{"cited_paper":"/paper/2203.15611","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:876028065f209e692926ceccd6e7f3d6f83521200a72db0abd3d1559b9648423","observation_id":"b3b78e9a-fd7b-49d3-8806-8e1ad78bc590","resolution":{"observed_at":"2026-08-16T00:14:35.801318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508299","last_updated":"2005-08-30T18:47:00Z","snapshot_observed_at":"2026-08-13T06:56:10.376871Z","submitted_at":"2005-08-12T21:04:46Z","title":"The Evolution in the Faint-End Slope of the Quasar Luminosity Function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508299","snapshot_observed_at":"2026-08-16T00:14:35.805369Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.805369Z"},"links":{"cited_paper":"/paper/astro-ph/0508299","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:67b9d63e6030f0ad3fab374e312405f19a45e19a26e834336edd38c913b4e2c5","observation_id":"53c3710b-c940-419a-a902-34a2a6741819","resolution":{"observed_at":"2026-08-16T00:14:35.805369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.809335Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.809335Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:7d54f874d20c72220abe1691cf0e199ee9dc529cb0dd2eed303e2437beb554c6","observation_id":"d6e8bb42-ce79-4e9a-955d-b020bef1cb4e","resolution":{"observed_at":"2026-08-16T00:14:35.809335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.813061Z","title":"2022 , doi =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.813061Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:0dfa49f39e5c0958584054fdea72a39fa0f7aad5875a45972fe2e993d3b40123","observation_id":"2121ad3e-406e-47ca-82de-45b26bb9aff7","resolution":{"observed_at":"2026-08-16T00:14:35.813061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.17680","last_updated":"2025-02-24T21:57:39Z","snapshot_observed_at":"2026-08-16T12:55:34.278361Z","submitted_at":"2025-02-24T21:57:39Z","title":"The Spectral Energy Distributions of Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.17680","snapshot_observed_at":"2026-08-16T00:14:35.816833Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.816833Z"},"links":{"cited_paper":"/paper/2502.17680","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:f0e20a1cdf4e515546465e81d37649108448a0804c1237d47653525b926b1d83","observation_id":"8af792c8-e598-434f-9664-2371849e409a","resolution":{"observed_at":"2026-08-16T00:14:35.816833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.821514Z","title":"Feature dimensionality reduction: a review , url =","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.821514Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:8f4bc6f932dd8c1fcb9a7df991b1d5b6997804b28cb2138d1e5eef90926cd565","observation_id":"66e1c774-0b86-4bbd-baee-011dc714aab4","resolution":{"observed_at":"2026-08-16T00:14:35.821514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.01426","last_updated":"2020-12-02T19:00:00Z","snapshot_observed_at":"2026-08-16T18:44:20.554767Z","submitted_at":"2020-12-02T19:00:00Z","title":"Stellar Population Inference with Prospector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.01426","snapshot_observed_at":"2026-08-16T00:14:35.825299Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.825299Z"},"links":{"cited_paper":"/paper/2012.01426","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:7b6b883ffc1d34fcfbca17b2c93cd7f9e43276dedb829bca3204acb7722e7a25","observation_id":"d3bc5dc3-015c-4330-ade3-34bc5ee3da7a","resolution":{"observed_at":"2026-08-16T00:14:35.825299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.829162Z","title":"Principal component analysis: A review and recent developments , volume =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.829162Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:367c00812d7f16a3051bc8cde48b559ff633b04eef002008926e29caa72a40b4","observation_id":"0747525b-d305-4ca6-8b38-7893ac8eef0c","resolution":{"observed_at":"2026-08-16T00:14:35.829162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.07535","last_updated":"2023-08-03T15:31:27Z","snapshot_observed_at":"2026-08-16T15:16:15.945473Z","submitted_at":"2023-07-14T12:03:24Z","title":"EPOCHS VII: Discovery of high redshift ($6.5 < z < 12$) AGN candidates in JWST ERO and PEARLS data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.07535","snapshot_observed_at":"2026-08-16T00:14:35.833270Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.833270Z"},"links":{"cited_paper":"/paper/2307.07535","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:cf7d4f380eaa880a9296573b13d59c5d8d0824f5bfdff7ccb1857730e8c0c4ea","observation_id":"07fb280d-8787-4f83-a6f1-000ad1001a21","resolution":{"observed_at":"2026-08-16T00:14:35.833270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.837727Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.837727Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:ee2ee146686587f007ac35c5ef83776813216a785cfda6f348ea831e9455fc92","observation_id":"cefb47d4-7b49-43bd-9458-eb32140d58b9","resolution":{"observed_at":"2026-08-16T00:14:35.837727Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.00584","last_updated":"2022-04-05T18:56:16Z","snapshot_observed_at":"2026-08-16T17:52:25.484827Z","submitted_at":"2021-10-01T18:00:00Z","title":"Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.00584","snapshot_observed_at":"2026-08-16T00:14:35.841932Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.841932Z"},"links":{"cited_paper":"/paper/2110.00584","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:5e79c05d50a69fd1a04d09b4961f707b567911ff6968a49dd99419802c586479","observation_id":"f0449c42-a232-491b-89b7-2ef5ff8482f4","resolution":{"observed_at":"2026-08-16T00:14:35.841932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.06939","last_updated":"2018-12-17T18:22:52Z","snapshot_observed_at":"2026-08-14T17:42:22.196316Z","submitted_at":"2018-12-17T18:22:52Z","title":"Disentangling the physical parameters of gaseous nebulae and galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.06939","snapshot_observed_at":"2026-08-16T00:14:35.845894Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.845894Z"},"links":{"cited_paper":"/paper/1812.06939","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:ab3ed05055a278265ae8768e6cbf5b5bcbf1a3cd43768ae4dc38f5ce11f8cd26","observation_id":"8a071aaa-1fa5-4c9f-ad34-742c49366c7e","resolution":{"observed_at":"2026-08-16T00:14:35.845894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.850016Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.850016Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:c8d00fe0e9e3120e02eccc952f92ffc500afe81223dac4e840a0f70492b4e2f4","observation_id":"1548193e-8f87-42e7-9524-793cb914d436","resolution":{"observed_at":"2026-08-16T00:14:35.850016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:14:35.853786Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.853786Z"},"links":{"citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:e2c2653e41625613e9748b9ffed96259c53821bfc2e79e398a44608e44328727","observation_id":"7a747c91-fd51-4f35-8a3f-a5709f304c90","resolution":{"observed_at":"2026-08-16T00:14:35.853786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9512123","last_updated":"1995-12-19T12:04:51Z","snapshot_observed_at":"2026-08-09T15:50:41.623906Z","submitted_at":"1995-12-19T12:04:51Z","title":"Disk galaxies at Z=0 and at High Redshift: an explanation of the observed evolution of damped Ly-alpha systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9512123","snapshot_observed_at":"2026-08-16T00:14:35.857803Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-16T00:14:35.857803Z"},"links":{"cited_paper":"/paper/astro-ph/9512123","citing_paper":"/paper/2608.12471"},"observation_digest":"sha256:1a2b5d42020a2a88e086ed9de46236c8489f18d51406ef65009535bf5e4c22cb","observation_id":"0d74f60a-6c98-4689-bab2-1a41e592fb95","resolution":{"observed_at":"2026-08-16T00:14:35.857803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.12471","last_updated":"2026-08-12T18:00:04Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T18:10:19.872771Z","submitted_at":"2026-08-12T18:00:04Z","title":"FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":97,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":188},"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 188 outbound references and 0 inbound Pith citation observations for arXiv:2608.12471."}