{"as_of":"2026-08-11T01:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5a44a3e8347436e9fb4bb85f383695cbb9c167c7f0cc2afebdc2e99879103167","coverage":[{"denominator":166,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T04:20:27.683116Z","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":"2026-08-10T06:31:04.303077+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/2608.07461/citation-record","integrity":"/paper/2608.07461/integrity","json":"/paper/2608.07461/citation-record.json","paper":"/paper/2608.07461"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T04:20:27.105550Z","title":", keywords =","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.105550Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:a1720107971067597515b8f37f6015812e8b4d352b60ae8e39668b1e3b144a13","observation_id":"5144e888-8eca-46d0-bd54-ce7124736e3e","resolution":{"observed_at":"2026-08-10T04:20:27.105550Z","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":"2026-08-10T04:20:27.112526Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.112526Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:732a2aa005ced92a13ba7499544e3f2f969e1be29fc827009efac6fdaf9079d1","observation_id":"ff9cc5c1-d667-418a-aa91-c179f2ac02b2","resolution":{"observed_at":"2026-08-10T04:20:27.112526Z","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":"2026-07-06T14:14:31.396297Z","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":"2026-08-10T04:20:27.117753Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.117753Z"},"links":{"cited_paper":"/paper/2211.02495","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:ea9d920b6fce0369371e699ead2e57214742cbeeb82938d1daf386a6a763561d","observation_id":"f4a3f943-f848-4639-8f49-410ff8ecae58","resolution":{"observed_at":"2026-08-10T04:20:27.117753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.05466","last_updated":"2023-02-10T19:00:06Z","snapshot_observed_at":"2026-08-08T09:18:44.802636Z","submitted_at":"2023-02-10T19:00:06Z","title":"The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.05466","snapshot_observed_at":"2026-08-10T04:20:27.123535Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.123535Z"},"links":{"cited_paper":"/paper/2302.05466","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:8878f62d86ecba455764bcaa6e5a764f47cb2f780e3dda90ff6a074dd0d6de45","observation_id":"e24780a9-0ffa-4ed2-8fdf-30605df7d330","resolution":{"observed_at":"2026-08-10T04:20:27.123535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.12980","last_updated":"2022-05-25T18:00:04Z","snapshot_observed_at":"2026-07-06T13:13:58.646908Z","submitted_at":"2022-05-25T18:00:04Z","title":"Bright z~9 Galaxies in Parallel: The Bright End of the Rest-UV Luminosity Function from HST Parallel Programs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.12980","snapshot_observed_at":"2026-08-10T04:20:27.129392Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.129392Z"},"links":{"cited_paper":"/paper/2205.12980","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:11eab3e15172a9a950b6024584bbe49bf5b6702eb418372d1f3aa0b2479bfb11","observation_id":"eb7dea14-4b5d-4c36-8eb4-9a4549efd8e1","resolution":{"observed_at":"2026-08-10T04:20:27.129392Z","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":"2026-08-10T04:20:27.134565Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.134565Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:26d36f22948cd7ad9aad132f372457f3487c22b0883579e6c9b6d9e23b4493a1","observation_id":"4ec7db51-367c-4ec8-a1ec-4512806d77b1","resolution":{"observed_at":"2026-08-10T04:20:27.134565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.23668","last_updated":"2026-04-26T12:09:01Z","snapshot_observed_at":"2026-07-06T23:09:52.860780Z","submitted_at":"2026-04-26T12:09:01Z","title":"Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Ultra-cool Brown Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.23668","snapshot_observed_at":"2026-08-10T04:20:27.139618Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.139618Z"},"links":{"cited_paper":"/paper/2604.23668","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:5ad13c8ea649170734747caf17976f70e6be1bb49077d5483a396cb5829b1030","observation_id":"8ee8b16a-8652-40ec-a863-ee2ab3e19788","resolution":{"observed_at":"2026-08-10T04:20:27.139618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10988","last_updated":"2025-02-03T17:27:27Z","snapshot_observed_at":"2026-08-08T02:50:30.065952Z","submitted_at":"2024-10-14T18:15:54Z","title":"The evolution of [OIII]$+\\rm{H}\\beta$ equivalent width from $\\mathbf{z\\simeq3-8}$: implications for the production and escape of ionizing photons during reionization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10988","snapshot_observed_at":"2026-08-10T04:20:27.146470Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.146470Z"},"links":{"cited_paper":"/paper/2410.10988","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:433e0eba84488ce9a9bfa52fee683ac84217956b077bc56f07a84293625ff9d5","observation_id":"43395e25-4c95-490d-85c3-a8383aabf397","resolution":{"observed_at":"2026-08-10T04:20:27.146470Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.5643","last_updated":"2014-03-05T14:23:13Z","snapshot_observed_at":"2026-08-08T01:03:32.012539Z","submitted_at":"2013-12-19T17:11:19Z","title":"The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.5643","snapshot_observed_at":"2026-08-10T04:20:27.154655Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.154655Z"},"links":{"cited_paper":"/paper/1312.5643","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:104cd3e4831cc8a658506679e451520e951e77af3ff4361782ee46be1598cac7","observation_id":"2a6ff666-1ebc-4764-a119-43e08d1a152b","resolution":{"observed_at":"2026-08-10T04:20:27.154655Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.2976","last_updated":"2015-06-25T14:12:50Z","snapshot_observed_at":"2026-07-06T04:00:14.074677Z","submitted_at":"2014-11-11T21:00:07Z","title":"The galaxy luminosity function at z ~ 6 and evidence for rapid evolution in the bright end from z ~ 7 to 5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.2976","snapshot_observed_at":"2026-08-10T04:20:27.161279Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.161279Z"},"links":{"cited_paper":"/paper/1411.2976","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:fc8053692553b9912a2ce0aeec417725fa1482d4fbd1dc96e1ef7709d29c4ceb","observation_id":"105ad807-b32a-448d-8909-6ad162ea52ef","resolution":{"observed_at":"2026-08-10T04:20:27.161279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.12832","last_updated":"2020-01-30T15:53:35Z","snapshot_observed_at":"2026-07-06T08:40:41.866674Z","submitted_at":"2019-11-28T19:00:15Z","title":"A lack of evolution in the very bright-end of the galaxy luminosity function from z = 8-10","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.12832","snapshot_observed_at":"2026-08-10T04:20:27.166828Z","title":", keywords =","venue":null,"work_id":null,"year":1911},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.166828Z"},"links":{"cited_paper":"/paper/1911.12832","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:cceaa4553211e50b3a13a4963dafd89488acd224f5f1ad8cc90e0b710144e4fc","observation_id":"25baee46-e2b4-4f63-8e70-49dd811accf4","resolution":{"observed_at":"2026-08-10T04:20:27.166828Z","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":"2026-08-06T03:27:46.997797Z","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":"2026-08-10T04:20:27.173174Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.173174Z"},"links":{"cited_paper":"/paper/2405.18485","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:b9d6002a7d4c46429506428fd343652dbe81f7290ecb15de2223a317bb9375fb","observation_id":"a6ce54df-2486-4b3a-8fb0-7ce59d11649b","resolution":{"observed_at":"2026-08-10T04:20:27.173174Z","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":"2026-08-10T04:20:27.179551Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.179551Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:b9516871a26bf80f1e7a19d1fc6fde485c81598acd6b98a7f7c2c166ac9d559d","observation_id":"77e05c43-b459-422e-8fca-f74d77e3797a","resolution":{"observed_at":"2026-08-10T04:20:27.179551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.12356","last_updated":"2022-11-24T11:45:40Z","snapshot_observed_at":"2026-08-07T13:03:17.763864Z","submitted_at":"2022-07-25T17:15:51Z","title":"The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.12356","snapshot_observed_at":"2026-08-10T04:20:27.184841Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.184841Z"},"links":{"cited_paper":"/paper/2207.12356","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:cfa88b0274fc8a6c5ce7a5aa245c96465ff58179d2767974c12c8ee2b8f81b88","observation_id":"aeef09d1-dbc9-4b11-a1e4-255a4ed6b834","resolution":{"observed_at":"2026-08-10T04:20:27.184841Z","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":"2026-08-08T10:12:20.916101Z","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":"2026-08-10T04:20:27.191106Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.191106Z"},"links":{"cited_paper":"/paper/2403.03171","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:bee117837525a4e7a1263bd9c07d79496b59c3c6c0c9e8a6f0f2262c00caf648","observation_id":"650ac4a3-74b8-40a4-9ea7-116b443a9f6b","resolution":{"observed_at":"2026-08-10T04:20:27.191106Z","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":"2026-08-10T04:20:27.197182Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.197182Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:421b32dc9264f4212831597783b7eb96ac2ae006ba75a7535c2593d0a51b496b","observation_id":"435ebec4-1148-4e85-9356-b403ff661271","resolution":{"observed_at":"2026-08-10T04:20:27.197182Z","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":"2026-08-10T04:20:27.202497Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.202497Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:712cae2f0972de19019fa0ee5465a688594a371efeae4470aa3091b2a1a30a27","observation_id":"ddda7a84-efee-4945-8637-679cf8016e55","resolution":{"observed_at":"2026-08-10T04:20:27.202497Z","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":"2026-08-10T04:20:27.207815Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.207815Z"},"links":{"cited_paper":"/paper/2306.02465","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:26056af3271d88a8e0a2dd7b8bccca5a17d024a480a418d8741301a4841ec2f3","observation_id":"b6f9065a-d076-4d75-ab59-f9f5ea0bc7e5","resolution":{"observed_at":"2026-08-10T04:20:27.207815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.12474","last_updated":"2022-09-07T20:55:00Z","snapshot_observed_at":"2026-08-05T12:36:53.684049Z","submitted_at":"2022-07-25T18:55:02Z","title":"A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.12474","snapshot_observed_at":"2026-08-10T04:20:27.213392Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.213392Z"},"links":{"cited_paper":"/paper/2207.12474","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:7580f0e34b645a77dd844b29a9462d414dd897e5fc2e1768edb1b4df092c3189","observation_id":"41e801e8-7e9d-4b66-b7a0-f57bd359e7fe","resolution":{"observed_at":"2026-08-10T04:20:27.213392Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.05792","last_updated":"2023-11-04T12:38:19Z","snapshot_observed_at":"2026-07-06T14:16:52.598523Z","submitted_at":"2022-11-10T19:00:02Z","title":"CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.05792","snapshot_observed_at":"2026-08-10T04:20:27.219570Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.219570Z"},"links":{"cited_paper":"/paper/2211.05792","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:e09d1d5f7d11e7ac35f25cca2201c558dcb1491716eb35b876c7ac1be294145f","observation_id":"af3f4c6d-1b40-4b5d-b373-04416262a267","resolution":{"observed_at":"2026-08-10T04:20:27.219570Z","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":"2026-08-02T19:03:03.607657Z","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":"2026-08-10T04:20:27.225190Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.225190Z"},"links":{"cited_paper":"/paper/2311.04279","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:9829c66eaea1f54905437cee6fcd18ec654068fa06353ea46170308200b19212","observation_id":"3cbf5152-ab4a-49a0-b88b-cb399a77c71e","resolution":{"observed_at":"2026-08-10T04:20:27.225190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.04791","last_updated":"2025-08-06T18:05:56Z","snapshot_observed_at":"2026-08-09T00:07:43.250788Z","submitted_at":"2025-08-06T18:05:56Z","title":"Physical properties of galaxies and the UV Luminosity Function from $z\\sim6$ to $z\\sim14$ in COSMOS-Web","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.04791","snapshot_observed_at":"2026-08-10T04:20:27.230026Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.230026Z"},"links":{"cited_paper":"/paper/2508.04791","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:7ed4d25344c448fb947a6f8632416d0084fc5b03cdc18198a32382c9520b3657","observation_id":"c887a646-0d09-4a6c-b68c-e8e4b680b230","resolution":{"observed_at":"2026-08-10T04:20:27.230026Z","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":"2026-08-10T04:20:27.236305Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.236305Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:e1c983de4ecf233318b69a8c9a8c00609511d43b8707bc3ff9a8e09d2c9f1ed4","observation_id":"cc46524e-88e1-49bc-8d7b-2d35db143817","resolution":{"observed_at":"2026-08-10T04:20:27.236305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.15959","last_updated":"2026-05-19T18:00:14Z","snapshot_observed_at":"2026-07-06T22:42:43.581560Z","submitted_at":"2026-01-22T13:43:14Z","title":"JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.15959","snapshot_observed_at":"2026-08-10T04:20:27.241249Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.241249Z"},"links":{"cited_paper":"/paper/2601.15959","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:464c52a30adb055fd49ff91a228e9814e0d2bcfe4d8a867cc6e8ca9c577280d6","observation_id":"e99e0ac8-ec5f-4f31-bbc2-f3cd0b468d50","resolution":{"observed_at":"2026-08-10T04:20:27.241249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2510.00111","last_updated":"2026-05-19T18:00:11Z","snapshot_observed_at":"2026-08-07T01:12:17.463051Z","submitted_at":"2025-09-30T18:00:06Z","title":"JADES: An Abundance of Ultra-Distant T- and Y-Dwarfs in Deep Extragalactic Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.00111","snapshot_observed_at":"2026-08-10T04:20:27.246251Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.246251Z"},"links":{"cited_paper":"/paper/2510.00111","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:6301452ff49d00407a90b8909d325fbbacc46015aae71545eda362bceb645215","observation_id":"66ca2166-c535-4a24-b07a-91dbe334b379","resolution":{"observed_at":"2026-08-10T04:20:27.246251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01612","last_updated":"2022-12-09T16:26:58Z","snapshot_observed_at":"2026-08-03T05:05:20.265457Z","submitted_at":"2022-08-02T17:44:17Z","title":"A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01612","snapshot_observed_at":"2026-08-10T04:20:27.252784Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.252784Z"},"links":{"cited_paper":"/paper/2208.01612","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:5ad57c4eec23da85514b8c1a339d79f5407a1e5486451bf7d1bd8d726014b95b","observation_id":"120fb685-cf89-41e4-987c-0dbb22ebdf85","resolution":{"observed_at":"2026-08-10T04:20:27.252784Z","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":"2026-08-10T04:20:27.258288Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.258288Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:f4fb6e83148fc422f9883433807d9a838de2a35aeba63c4f2c9dc23805450c9f","observation_id":"5317d584-f7d3-4d73-8448-f74dc5ff44c6","resolution":{"observed_at":"2026-08-10T04:20:27.258288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.1472","last_updated":"2015-05-15T15:11:34Z","snapshot_observed_at":"2026-07-06T04:02:33.136517Z","submitted_at":"2014-12-03T21:00:00Z","title":"New redshift z ~ 9 galaxies in the Hubble Frontier Fields: Implications for early evolution of the UV luminosity density","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.1472","snapshot_observed_at":"2026-08-10T04:20:27.263130Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.263130Z"},"links":{"cited_paper":"/paper/1412.1472","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:d1fe7dd54ce1ee7a1734d34598844439996238d8add3ff863790719fce10d293","observation_id":"724901f7-2e08-4702-aac9-92d07952af2f","resolution":{"observed_at":"2026-08-10T04:20:27.263130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.05199","last_updated":"2016-02-16T21:00:05Z","snapshot_observed_at":"2026-08-06T02:16:20.099886Z","submitted_at":"2016-02-16T21:00:05Z","title":"The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: The z=9 LF and further evidence for a smooth decline in UV luminosity at z >= 8","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.05199","snapshot_observed_at":"2026-08-10T04:20:27.269537Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.269537Z"},"links":{"cited_paper":"/paper/1602.05199","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:bdc092c141365d4a81bee9f0dc9b728a0bb3d829d2fc0f223f4530c4ea6fc520","observation_id":"6e281d1c-7c90-434c-93f0-4415b02072c7","resolution":{"observed_at":"2026-08-10T04:20:27.269537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.14469","last_updated":"2023-11-09T01:37:39Z","snapshot_observed_at":"2026-07-06T15:20:57.161336Z","submitted_at":"2023-04-27T19:12:17Z","title":"The galaxy UV luminosity function at $\\mathbf{z \\simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.14469","snapshot_observed_at":"2026-08-10T04:20:27.275333Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.275333Z"},"links":{"cited_paper":"/paper/2304.14469","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:b594d756185b2d614e458f7c818da157370b6237f8b82591a20065c17bf12104","observation_id":"5c524a1c-c11a-48a9-86a4-7e1dd5498df9","resolution":{"observed_at":"2026-08-10T04:20:27.275333Z","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":"2026-08-10T04:20:27.281613Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.281613Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:c542956bf8c79535404b6f7e031c4633c18f7d9364e070cb665f0441b6f5b4c3","observation_id":"b25e0651-08af-4930-9ecc-349df6c59504","resolution":{"observed_at":"2026-08-10T04:20:27.281613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.00756","last_updated":"2024-02-01T16:47:44Z","snapshot_observed_at":"2026-08-09T16:17:25.902943Z","submitted_at":"2024-02-01T16:47:44Z","title":"The Sonora Substellar Atmosphere Models. IV. Elf Owl: Atmospheric Mixing and Chemical Disequilibrium with Varying Metallicity and C/O Ratios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.00756","snapshot_observed_at":"2026-08-10T04:20:27.286834Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.286834Z"},"links":{"cited_paper":"/paper/2402.00756","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:ab711d0f411e7ba1b3320516b6e76ec1a76fbc4b33ac61ae0071bb5faf2d363a","observation_id":"76459e39-be6e-4247-9525-2ae46d407a8f","resolution":{"observed_at":"2026-08-10T04:20:27.286834Z","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":"10.5281/zenodo.15150865","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"doi:10.5281/zenodo.15150865 , url =","venue":"Zenodo (CERN European Organization for Nuclear Research)","work_id":"d04571bd-27fe-4514-8d0a-ff2e0d2840b2","year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.292557Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:3cc3976f904f02d47de330c12c0b6bc610fb642c34d3a45dda090a226f02151f","observation_id":"6e406349-5943-41e7-be9b-0f4327042bb4","resolution":{"observed_at":"2026-08-10T04:20:28.794655Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.19706","last_updated":"2025-07-25T22:51:37Z","snapshot_observed_at":"2026-08-09T03:10:54.794057Z","submitted_at":"2025-07-25T22:51:37Z","title":"MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.19706","snapshot_observed_at":"2026-08-10T04:20:27.298053Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.298053Z"},"links":{"cited_paper":"/paper/2507.19706","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:5d2f77e23c867eeff7a3f042e069c371d0cb8b208f64e8ae3db6d16b441dfcc1","observation_id":"e0fff534-e78b-4b2c-bbf3-88d61b4902a2","resolution":{"observed_at":"2026-08-10T04:20:27.298053Z","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":"2026-08-10T04:20:27.304348Z","title":"The Open Journal of Astrophysics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.304348Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:6941ddb46d7c7063d175b6b00fe5a686059a284552a1f57cf6978f1a0a52f7c6","observation_id":"b274fb03-06a5-473b-a756-90d1e87fe880","resolution":{"observed_at":"2026-08-10T04:20:27.304348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.11131","last_updated":"2018-02-27T08:35:33Z","snapshot_observed_at":"2026-07-06T06:06:48.906444Z","submitted_at":"2017-10-30T18:00:01Z","title":"The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.11131","snapshot_observed_at":"2026-08-10T04:20:27.309819Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.309819Z"},"links":{"cited_paper":"/paper/1710.11131","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:b01340d072d8e9ad736ad1ba446ac12982bb633bb429e24503853fb74840bab6","observation_id":"c42f5cda-1e92-476f-8e0d-928789b9f74b","resolution":{"observed_at":"2026-08-10T04:20:27.309819Z","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":"2026-08-10T04:20:27.317107Z","title":", year = 1974, month = feb, volume =","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.317107Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:03a1929a094dcf6cac63e59d016330c802a25294101a0dc2bb0bda4c2d9431bc","observation_id":"f9c9b41e-cab1-436e-8150-997110a50d10","resolution":{"observed_at":"2026-08-10T04:20:27.317107Z","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":"2026-08-10T04:20:27.323643Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.323643Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:a46d6c90f2abac34a9ffc99b0b6bb2c8e505f8fa0fa81eb8ca6e20a5c019de67","observation_id":"cc523aba-2c40-4c3a-8fd2-37dfe99c0e1d","resolution":{"observed_at":"2026-08-10T04:20:27.323643Z","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":"2026-08-10T04:20:27.330695Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.330695Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:aa7d6b3103259ad620f0e0e526e07a6cc8dd8685ff1726478ff49a985388cd8b","observation_id":"3cdfa893-9bcc-40f8-94ed-93aab02fa3b1","resolution":{"observed_at":"2026-08-10T04:20:27.330695Z","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":"2026-08-10T04:20:27.336810Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.336810Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:df0ffa561eee121de1256cb8cf0c765ebfba651045f6d77f3b32078db73142ac","observation_id":"7ba76536-1c2a-4485-a957-fd3012f2f878","resolution":{"observed_at":"2026-08-10T04:20:27.336810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.22245","last_updated":"2026-07-01T15:02:28Z","snapshot_observed_at":"2026-08-03T06:48:31.504513Z","submitted_at":"2026-01-29T19:10:45Z","title":"Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.22245","snapshot_observed_at":"2026-08-10T04:20:27.342412Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.342412Z"},"links":{"cited_paper":"/paper/2601.22245","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:ff3d2eb8fd45881fe724a925f4b88d66de113d8b98cb9c73add028fdecef31d6","observation_id":"767e0fd9-5cb4-4cf7-9d7d-6079fdd54058","resolution":{"observed_at":"2026-08-10T04:20:27.342412Z","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":"2026-08-10T04:20:27.348667Z","title":"doi:10.5479/ADS/bib/2012ivoa.rept.1015R , adsurl =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.348667Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:084d03acb32f95ca5377b659ee1a883d031f82e456d0bfbe2e42757cc460cb18","observation_id":"7f97377d-ab20-44eb-b091-937b498ea600","resolution":{"observed_at":"2026-08-10T04:20:27.348667Z","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":"2026-08-10T04:20:27.355457Z","title":"XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society , year = 2020, month = jul, eid =","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.355457Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:51df26ac5045cfeb95466c920c3cb6e2a131e0d8ba610a8f998cbbbff3064e1d","observation_id":"9f7f1eb2-23fa-42ee-bab5-14249dcfacf0","resolution":{"observed_at":"2026-08-10T04:20:27.355457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.06292","last_updated":"2026-05-31T09:33:06Z","snapshot_observed_at":"2026-08-08T21:40:56.983055Z","submitted_at":"2025-07-08T18:00:01Z","title":"Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\\sim9 -17$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.06292","snapshot_observed_at":"2026-08-10T04:20:27.361420Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.361420Z"},"links":{"cited_paper":"/paper/2507.06292","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:11965d339df8214344302e8bdf86180acd8691450c2ec0c033ef9e167e7cf78a","observation_id":"3e3b9914-82f5-459c-a54d-47eac51e9247","resolution":{"observed_at":"2026-08-10T04:20:27.361420Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.04119","last_updated":"2022-11-29T04:09:51Z","snapshot_observed_at":"2026-08-09T13:44:35.193849Z","submitted_at":"2022-09-09T05:00:25Z","title":"JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.04119","snapshot_observed_at":"2026-08-10T04:20:27.366190Z","title":"Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.366190Z"},"links":{"cited_paper":"/paper/2209.04119","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:7aab079dc7964933154f31f376793ce8601c9b27abe0b38729547784d413ac00","observation_id":"3d3f7fe0-05e2-4f59-a896-6c4faa54c82f","resolution":{"observed_at":"2026-08-10T04:20:27.366190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508555","last_updated":"2005-08-25T19:44:35Z","snapshot_observed_at":"2026-07-07T00:53:16.117498Z","submitted_at":"2005-08-25T19:44:35Z","title":"Constraining the Distribution of L- & T-Dwarfs in the Galaxy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508555","snapshot_observed_at":"2026-08-10T04:20:27.370865Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.370865Z"},"links":{"cited_paper":"/paper/astro-ph/0508555","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:008e41b01c53a87f92fea58e7a7c3cef4442a1f19a7ed7add2f7018209236918","observation_id":"4b60eff3-b482-4893-ba94-2f3393725501","resolution":{"observed_at":"2026-08-10T04:20:27.370865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.10806","last_updated":"2019-03-26T11:32:50Z","snapshot_observed_at":"2026-07-06T07:41:41.488860Z","submitted_at":"2019-03-26T11:32:50Z","title":"Brown dwarf census with the Dark Energy Survey year 3 data and the thin disk scale height of early L types","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.10806","snapshot_observed_at":"2026-08-10T04:20:27.375848Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.375848Z"},"links":{"cited_paper":"/paper/1903.10806","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:0d8d582bd3326d2ebd61076ddca78657fb7f4c2a00c9fe269293bbcf8e7d959f","observation_id":"4cb4c7c2-b218-46af-b0ca-1bcc5a4faba4","resolution":{"observed_at":"2026-08-10T04:20:27.375848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.07496","last_updated":"2018-11-19T04:38:05Z","snapshot_observed_at":"2026-07-06T07:15:30.564175Z","submitted_at":"2018-11-19T04:38:05Z","title":"Evaluation of the Vertical Scale Height of L dwarfs in the Galactic Thin Disk","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.07496","snapshot_observed_at":"2026-08-10T04:20:27.381322Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.381322Z"},"links":{"cited_paper":"/paper/1811.07496","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:57b6bcf274f5e638c38c676b1436ddd1960c79ea270154666458ecd17e85a216","observation_id":"10482913-40df-4588-aa54-a740642361be","resolution":{"observed_at":"2026-08-10T04:20:27.381322Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.3008","last_updated":"2008-09-17T20:55:19Z","snapshot_observed_at":"2026-07-06T01:42:49.380549Z","submitted_at":"2008-09-17T20:55:19Z","title":"The Brown Dwarf Kinematics Project (BDKP) I. Proper Motions and Tangential Velocities for a Large Sample of Late-type M, L and T Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.3008","snapshot_observed_at":"2026-08-10T04:20:27.386182Z","title":"Proper Motions and Tangential Velocities for a Large Sample of Late-Type M, L, and T Dwarfs","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.386182Z"},"links":{"cited_paper":"/paper/0809.3008","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:2a61542f840b7e22aba4baa9c6a0de3f5b07391d0aac2352c6a0f26ff93f875a","observation_id":"4e7046bf-3c80-45ee-9b81-2c62708b5bca","resolution":{"observed_at":"2026-08-10T04:20:27.386182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0706.0784","last_updated":"2007-06-06T08:47:40Z","snapshot_observed_at":"2026-07-06T01:30:35.861566Z","submitted_at":"2007-06-06T08:47:40Z","title":"Space Velocities of L- and T-type Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0706.0784","snapshot_observed_at":"2026-08-10T04:20:27.392793Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.392793Z"},"links":{"cited_paper":"/paper/0706.0784","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:6f998918d4c5f42daefcce1e84e336b6a81b8244580f02c113878cf0a52e80c7","observation_id":"cfa4a2f8-bf98-45c3-ab2d-5cadb35ae22d","resolution":{"observed_at":"2026-08-10T04:20:27.392793Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701055","last_updated":"2007-01-03T02:06:36Z","snapshot_observed_at":"2026-08-07T09:39:34.140815Z","submitted_at":"2007-01-03T02:06:36Z","title":"Activity and Kinematics of Ultracool Dwarfs Including An Amazing Flare Observation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0701055","snapshot_observed_at":"2026-08-10T04:20:27.399652Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.399652Z"},"links":{"cited_paper":"/paper/astro-ph/0701055","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:fdb346980efc4969a5a7d6db1476cfacb0ccfb454a4516623c8843d3dba510b3","observation_id":"16ebab8f-9de1-495a-8b61-383ac41c04a1","resolution":{"observed_at":"2026-08-10T04:20:27.399652Z","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":"2026-08-10T04:20:27.407009Z","title":"Astronomical Data Analysis Software and Systems XII , year = 2003, editor =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.407009Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:ac56a985560b7ae89319bcff2466aa30c3be0c030a30c077f3d1e98317d57ada","observation_id":"5595ff2a-2455-41ff-a6fc-a358784b6bf9","resolution":{"observed_at":"2026-08-10T04:20:27.407009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.07374","last_updated":"2026-05-12T08:57:11Z","snapshot_observed_at":"2026-07-06T22:41:24.948774Z","submitted_at":"2026-01-12T09:56:45Z","title":"Possible evidence for a pair-instability supernova nature of ultra-early JWST sources","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.07374","snapshot_observed_at":"2026-08-10T04:20:27.413716Z","title":"The Open Journal of Astrophysics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.413716Z"},"links":{"cited_paper":"/paper/2601.07374","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:1db57d8d451b7d2bfceeff829b01aa485462e583c8904dfa36952c46378fe67c","observation_id":"d4645263-eee9-4f70-932e-fd3b85f6ec0c","resolution":{"observed_at":"2026-08-10T04:20:27.413716Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.11515","last_updated":"2026-04-07T10:33:26Z","snapshot_observed_at":"2026-07-31T10:48:30.313906Z","submitted_at":"2026-01-16T18:51:25Z","title":"Spectroscopic confirmation of a large and luminous galaxy with weak emission lines at $\\mathbf{z = 13.53}$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.11515","snapshot_observed_at":"2026-08-10T04:20:27.419106Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.419106Z"},"links":{"cited_paper":"/paper/2601.11515","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:167ea2d3428c54d65dd835a4025e1d65b8733b196d90720639afdd18f73f5a90","observation_id":"483c0fb2-8bb5-4d32-aca9-95e91336e895","resolution":{"observed_at":"2026-08-10T04:20:27.419106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.17963","last_updated":"2026-08-06T14:57:41Z","snapshot_observed_at":"2026-08-09T23:12:11.716250Z","submitted_at":"2026-04-20T08:45:57Z","title":"BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.17963","snapshot_observed_at":"2026-08-10T04:20:27.424973Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.424973Z"},"links":{"cited_paper":"/paper/2604.17963","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:7f8ad1f0b2a638b299a7ef5fb72667350f25c93b390f4e7b27d078ee81875d85","observation_id":"31ee53de-51a8-4eaa-a417-4ae7dc00d3e4","resolution":{"observed_at":"2026-08-10T04:20:27.424973Z","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":"2026-08-10T04:20:27.431556Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.431556Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:3c7342a7b7cfc90c3aaba51bed25e6d03fb41ac330126f24109f93f2a356678b","observation_id":"95358567-c7f4-490e-85ad-0e1f23c8214e","resolution":{"observed_at":"2026-08-10T04:20:27.431556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.18972","last_updated":"2026-07-21T11:04:49Z","snapshot_observed_at":"2026-08-07T21:32:03.376706Z","submitted_at":"2026-07-21T11:04:49Z","title":"A Type Ia Supernova Candidate at $z\\sim4.3$: A Transient Interloper in the Search for $z\\sim14$ Galaxies","version":1},"cited_work":{"arxiv_id":"2607.18972","doi":"10.48550/arxiv.2607.18972","metadata_source":"pith","pith_arxiv_id":"2607.18972","snapshot_observed_at":"2026-08-10T06:16:20.510975Z","title":"A Type Ia Supernova Candidate at $z\\sim4.3$: A Transient Interloper in the Search for $z\\sim14$ Galaxies","venue":"astro-ph.HE","work_id":"691df2ca-fa3d-4ce0-b567-bfb0fdbf2d36","year":2026},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.438052Z"},"links":{"cited_paper":"/paper/2607.18972","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:1d616b68d766255b263124590a7c7174fc8278f9caaa420451fee4ede73538f3","observation_id":"36c1f884-71d2-495b-9b5e-809274d8f674","resolution":{"observed_at":"2026-08-10T04:20:28.546574Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03250","last_updated":"2024-01-19T17:55:17Z","snapshot_observed_at":"2026-08-06T04:44:08.199374Z","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":"2026-08-10T04:20:27.444008Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.444008Z"},"links":{"cited_paper":"/paper/2309.03250","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:96c1bb1fc15502e21941c5526ce5e01cb661013c3a385e4b2af364296d56121b","observation_id":"efa4b010-a40b-4718-a34c-7a5605903ec8","resolution":{"observed_at":"2026-08-10T04:20:27.444008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.2122","last_updated":"2012-05-09T23:16:26Z","snapshot_observed_at":"2026-07-06T02:47:50.465016Z","submitted_at":"2012-05-09T23:16:26Z","title":"Further Defining Spectral Type \"Y\" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.2122","snapshot_observed_at":"2026-08-10T04:20:27.451010Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.451010Z"},"links":{"cited_paper":"/paper/1205.2122","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:a0db3a45a4e7d09e6b3234908091fe6412e62f819066b6d881bcd3e764071f9e","observation_id":"24d0979d-8bcd-4724-9676-1c06b8b935b1","resolution":{"observed_at":"2026-08-10T04:20:27.451010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.4678","last_updated":"2011-08-23T19:32:04Z","snapshot_observed_at":"2026-08-02T00:31:52.010623Z","submitted_at":"2011-08-23T19:32:04Z","title":"The Discovery of Y Dwarfs Using Data from the Wide-field Infrared Survey Explorer (WISE)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.4678","snapshot_observed_at":"2026-08-10T04:20:27.456841Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.456841Z"},"links":{"cited_paper":"/paper/1108.4678","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:094fe76288960a8957a73917c3dc021468cfdb7f758803954954fe6cf11253a1","observation_id":"5e083814-8373-46b4-adb7-d41018c32172","resolution":{"observed_at":"2026-08-10T04:20:27.456841Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.00696","last_updated":"2021-07-01T18:41:47Z","snapshot_observed_at":"2026-07-06T11:25:11.934030Z","submitted_at":"2021-07-01T18:41:47Z","title":"Measuring and Replicating the 1-20 um Energy Distributions of the Coldest Brown Dwarfs: Rotating, Turbulent and Non-Adiabatic Atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.00696","snapshot_observed_at":"2026-08-10T04:20:27.462196Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.462196Z"},"links":{"cited_paper":"/paper/2107.00696","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:0ab29b9781a8e5f93bc8dbd7566ed9f81b6f6d16377c54208b95286c1ba442a4","observation_id":"6c43517e-be04-406c-b5f7-2130261cb2a9","resolution":{"observed_at":"2026-08-10T04:20:27.462196Z","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":"2026-08-10T04:20:27.467326Z","title":"Near-infrared photometry","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.467326Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:2c2e6b22c8b91cade7d5ba9a85aa0d553b601451ec51963cd348ad9f1cbf7ca0","observation_id":"3c6098aa-e6ba-499e-81f3-860dd21383c5","resolution":{"observed_at":"2026-08-10T04:20:27.467326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.11616","last_updated":"2020-11-23T18:45:26Z","snapshot_observed_at":"2026-07-06T10:17:07.117391Z","submitted_at":"2020-11-23T18:45:26Z","title":"The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.11616","snapshot_observed_at":"2026-08-10T04:20:27.472204Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.472204Z"},"links":{"cited_paper":"/paper/2011.11616","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:730359022fa794e40b629563f5d79bc8ba90811fee62999d82b9dde3b93837ec","observation_id":"2ade7485-fd49-4cd9-b157-93d2014d2119","resolution":{"observed_at":"2026-08-10T04:20:27.472204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.16679","last_updated":"2025-01-07T21:16:22Z","snapshot_observed_at":"2026-08-04T06:52:21.740731Z","submitted_at":"2024-12-21T16:10:32Z","title":"The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- II. Parallaxes and Proper Motions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.16679","snapshot_observed_at":"2026-08-10T04:20:27.477691Z","title":"Parallaxes and proper motions","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.477691Z"},"links":{"cited_paper":"/paper/2412.16679","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:b495f8140b922e9051a1df4bc478352926d578211a219f5336115d368eeeceb7","observation_id":"fb763d36-a899-4a0b-8a51-2322e1ec40ab","resolution":{"observed_at":"2026-08-10T04:20:27.477691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.01599","last_updated":"2025-03-03T14:34:53Z","snapshot_observed_at":"2026-08-07T17:33:29.494525Z","submitted_at":"2025-03-03T14:34:53Z","title":"A temperate super-Jupiter imaged with JWST in the mid-infrared","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.01599","snapshot_observed_at":"2026-08-10T04:20:27.482895Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.482895Z"},"links":{"cited_paper":"/paper/2503.01599","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:4a236bafc9cb168eb9549cbff66d3a492ab8c11487e53c0253a2c1b543758536","observation_id":"d54258aa-099d-4ca1-ac5e-2cdbef412d79","resolution":{"observed_at":"2026-08-10T04:20:27.482895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.03084","last_updated":"2015-10-09T17:04:57Z","snapshot_observed_at":"2026-08-02T02:04:34.590653Z","submitted_at":"2015-08-12T22:07:18Z","title":"Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.03084","snapshot_observed_at":"2026-08-10T04:20:27.490123Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.490123Z"},"links":{"cited_paper":"/paper/1508.03084","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:5d3f130a1841b20aee9f5ff8ad0b54b6ef0338e56ce160e1e226eb98d15d0696","observation_id":"1638d887-49d8-4e3f-89f0-68f16a65a86e","resolution":{"observed_at":"2026-08-10T04:20:27.490123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.15081","last_updated":"2025-02-20T22:50:39Z","snapshot_observed_at":"2026-08-10T18:12:32.950368Z","submitted_at":"2025-02-20T22:50:39Z","title":"Evidence for a sub-jovian planet in the young TWA7 disk","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.15081","snapshot_observed_at":"2026-08-10T04:20:27.496739Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.496739Z"},"links":{"cited_paper":"/paper/2502.15081","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:4bc5244e24a5815c0668b4673446e6502e0daa79220f527f9398acc54f592989","observation_id":"2e2ff747-c2d2-4f06-8401-bf1fd31b4ecf","resolution":{"observed_at":"2026-08-10T04:20:27.496739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.19932","last_updated":"2025-06-24T18:17:33Z","snapshot_observed_at":"2026-08-06T22:58:15.760072Z","submitted_at":"2025-06-24T18:17:33Z","title":"Follow-Up Exploration of the TWA 7 Planet-Disk System with JWST NIRCam","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.19932","snapshot_observed_at":"2026-08-10T04:20:27.501703Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.501703Z"},"links":{"cited_paper":"/paper/2506.19932","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:9b94143655bd76a01c5d0b32f1492321124497f399cad2cec9df66a943ade75a","observation_id":"cb852e23-a6b4-466a-83bc-b9c995d5e1a7","resolution":{"observed_at":"2026-08-10T04:20:27.501703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09201","last_updated":"2025-06-10T19:42:42Z","snapshot_observed_at":"2026-08-08T06:27:13.074241Z","submitted_at":"2025-06-10T19:42:42Z","title":"JWST Coronagraphic Images of 14 Her c: a Cold Giant Planet in a Dynamically Hot, Multi-planet System","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.09201","snapshot_observed_at":"2026-08-10T04:20:27.506670Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.506670Z"},"links":{"cited_paper":"/paper/2506.09201","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:4304126c2806e17b67e5d179a79f7a7b369e85291ace226c138154b5ac21dde8","observation_id":"baec30cf-e788-41a5-aeef-66bb9b8fa6e4","resolution":{"observed_at":"2026-08-10T04:20:27.506670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.23789","last_updated":"2026-06-22T18:00:02Z","snapshot_observed_at":"2026-08-09T02:04:57.653819Z","submitted_at":"2026-06-22T18:00:02Z","title":"Discovery of an Exterior Third Planet Orbiting $\\beta$ Pictoris","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.23789","snapshot_observed_at":"2026-08-10T04:20:27.511566Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.511566Z"},"links":{"cited_paper":"/paper/2606.23789","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:adcaf8ed830c80aa3766abe39eca5b30b85881156648d17b663c27e6fdfea202","observation_id":"a81d5270-4207-4dc2-8819-f437c2255974","resolution":{"observed_at":"2026-08-10T04:20:27.511566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.23801","last_updated":"2026-07-13T16:06:16Z","snapshot_observed_at":"2026-08-06T03:30:57.396972Z","submitted_at":"2026-06-22T18:00:04Z","title":"Direct Imaging Discovery of Giant Exoplanet $\\beta$ Pictoris d: A Decade-Long Game of Hide-and-Seek","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.23801","snapshot_observed_at":"2026-08-10T04:20:27.517673Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.517673Z"},"links":{"cited_paper":"/paper/2606.23801","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:cd294ef06ee7fc619c5e0e33b88301cf32242712eeb7a3d15e1c2bb33fe8e366","observation_id":"7739a5f1-53f6-4806-88ea-9f6568d3fbfd","resolution":{"observed_at":"2026-08-10T04:20:27.517673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.2886","last_updated":"2013-08-12T20:59:01Z","snapshot_observed_at":"2026-07-06T03:17:54.778024Z","submitted_at":"2013-07-10T19:29:05Z","title":"Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.2886","snapshot_observed_at":"2026-08-10T04:20:27.523449Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.523449Z"},"links":{"cited_paper":"/paper/1307.2886","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:705516ae5700ca44036c8d820c0109291bd6d087c063b699de68ccd8f1a109fb","observation_id":"fb310e19-2d3a-4007-a767-5478a8e9feb4","resolution":{"observed_at":"2026-08-10T04:20:27.523449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.04902","last_updated":"2016-05-16T20:00:00Z","snapshot_observed_at":"2026-08-10T18:12:31.179696Z","submitted_at":"2016-05-16T20:00:00Z","title":"The First Spectrum of the Coldest Brown Dwarf","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.04902","snapshot_observed_at":"2026-08-10T04:20:27.529319Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.529319Z"},"links":{"cited_paper":"/paper/1605.04902","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:a07ac31944096d57759e665373780119d4fffbb9370ae7e65ed9409b71a286de","observation_id":"76880ef9-d7b2-4924-8688-14599b459d51","resolution":{"observed_at":"2026-08-10T04:20:27.529319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04686","last_updated":"2019-03-12T01:30:11Z","snapshot_observed_at":"2026-08-01T16:04:13.974596Z","submitted_at":"2019-03-12T01:30:11Z","title":"Discovery of Cold Brown Dwarfs or Free-Floating Giant Planets Close to the Sun","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04686","snapshot_observed_at":"2026-08-10T04:20:27.535226Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.535226Z"},"links":{"cited_paper":"/paper/1903.04686","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:2cce4fb558c5690d7b23bc38a94b3d0562712f88e164d6fa75e68cf1562085ba","observation_id":"e8b98413-ae7d-4037-bdca-859b52affa7c","resolution":{"observed_at":"2026-08-10T04:20:27.535226Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.4671","last_updated":"2014-09-04T11:26:20Z","snapshot_observed_at":"2026-07-06T03:52:11.352673Z","submitted_at":"2014-08-20T14:25:09Z","title":"Indications of Water Clouds in the Coldest Known Brown Dwarf","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.4671","snapshot_observed_at":"2026-08-10T04:20:27.541058Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.541058Z"},"links":{"cited_paper":"/paper/1408.4671","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:e2a7fdb8b214ae32aef189a6322e0ee3f527eace36531099d7ffe3949748bb1a","observation_id":"46054c44-ca48-425f-a1e3-db3e76cab0db","resolution":{"observed_at":"2026-08-10T04:20:27.541058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.1422","last_updated":"2013-09-05T18:07:52Z","snapshot_observed_at":"2026-07-06T03:22:18.698870Z","submitted_at":"2013-09-05T18:07:52Z","title":"Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.1422","snapshot_observed_at":"2026-08-10T04:20:27.546593Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.546593Z"},"links":{"cited_paper":"/paper/1309.1422","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:f97d635e1faf778a90390885466a9b15c90c11f18c8173cf364d0c6eab922178","observation_id":"a97dccd4-f9c3-4faf-a8f0-dac157596db3","resolution":{"observed_at":"2026-08-10T04:20:27.546593Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.1194","last_updated":"2014-02-09T05:34:11Z","snapshot_observed_at":"2026-07-06T03:32:35.866926Z","submitted_at":"2014-01-06T20:40:31Z","title":"WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.1194","snapshot_observed_at":"2026-08-10T04:20:27.552111Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.552111Z"},"links":{"cited_paper":"/paper/1401.1194","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:18f3250cf658a8d0fcf4b25746b27e1d04c9bae6a403374088218514100f1993","observation_id":"29752af6-ba17-495b-873a-7cc6d8cfb5d8","resolution":{"observed_at":"2026-08-10T04:20:27.552111Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.16295","last_updated":"2023-03-28T20:18:57Z","snapshot_observed_at":"2026-07-06T15:09:17.982917Z","submitted_at":"2023-03-28T20:18:57Z","title":"Self-consistent Models of Y Dwarf Atmospheres with Water Clouds and Disequilibrium Chemistry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.16295","snapshot_observed_at":"2026-08-10T04:20:27.557799Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.557799Z"},"links":{"cited_paper":"/paper/2303.16295","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:381f6fa8eb5dd535b20d21cf1fe020f53c2d57fa45b29603d2227c0727c1ae17","observation_id":"d11c4826-5108-4bdf-93c6-163a45e67d57","resolution":{"observed_at":"2026-08-10T04:20:27.557799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.01355","last_updated":"2022-03-15T21:23:44Z","snapshot_observed_at":"2026-07-06T12:33:56.572349Z","submitted_at":"2022-02-03T00:50:53Z","title":"Microphysics of Water Clouds in the Atmospheres of Y Dwarfs and Temperate Giant Planets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.01355","snapshot_observed_at":"2026-08-10T04:20:27.563461Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.563461Z"},"links":{"cited_paper":"/paper/2202.01355","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:5134020fea7e2774e4ff8cb62e135e705a8bdf01985637788f118020412dcd90","observation_id":"6f1995a8-04d2-4e01-a549-a4c34bfafb58","resolution":{"observed_at":"2026-08-10T04:20:27.563461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.10305","last_updated":"2025-02-14T11:00:23Z","snapshot_observed_at":"2026-07-06T19:51:01.075884Z","submitted_at":"2024-11-15T16:01:13Z","title":"Three-dimensional dynamical evolution of cloud particle microphysics in sub-stellar atmospheres I. Description and exploring Y-dwarf atmospheric variability","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.10305","snapshot_observed_at":"2026-08-10T04:20:27.568862Z","title":"Description and exploring Y-dwarf atmospheric variability","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.568862Z"},"links":{"cited_paper":"/paper/2411.10305","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:b7074035972023e63f0f6193e5fafa703ddc3dd1411a43f1d1cbfb9a5cfb6c58","observation_id":"aa216b95-6f9f-43cb-a5f2-c5844d0e093c","resolution":{"observed_at":"2026-08-10T04:20:27.568862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.0863","last_updated":"2014-06-03T20:14:18Z","snapshot_observed_at":"2026-07-06T03:45:24.749581Z","submitted_at":"2014-06-03T20:14:18Z","title":"Spectral Variability from the Patchy Atmospheres of T and Y Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.0863","snapshot_observed_at":"2026-08-10T04:20:27.574850Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.574850Z"},"links":{"cited_paper":"/paper/1406.0863","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:b47e9b581356fbd418777b98070d55c13b4ce1721d6576a007a3ad7777ee6c9d","observation_id":"2856dbb9-d5d1-4d1c-8cbf-6baa18f8cf1e","resolution":{"observed_at":"2026-08-10T04:20:27.574850Z","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":"2026-08-10T04:20:27.581199Z","title":"Science Advances , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.581199Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:a8fe183a6e88303752b7542c3aac362f1eec32eb8dfbdcb02ba6df283f93accd","observation_id":"9bfb8ff3-674d-4475-a6a0-57de2ed5f05a","resolution":{"observed_at":"2026-08-10T04:20:27.581199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.13717","last_updated":"2020-03-30T18:03:55Z","snapshot_observed_at":"2026-07-06T09:08:28.873280Z","submitted_at":"2020-03-30T18:03:55Z","title":"A new set of atmosphere and evolution models for cool T-Y brown dwarfs and giant exoplanets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.13717","snapshot_observed_at":"2026-08-10T04:20:27.588772Z","title":", keywords =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.588772Z"},"links":{"cited_paper":"/paper/2003.13717","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:3dc88b5379a01a89aa404264dcb3135470f22cbb7c164cf5ee82206e308eef62","observation_id":"5f5121ee-8ee2-46b5-9fc5-ad5eaf09877c","resolution":{"observed_at":"2026-08-10T04:20:27.588772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.10770","last_updated":"2020-04-28T00:24:26Z","snapshot_observed_at":"2026-08-08T22:57:15.774442Z","submitted_at":"2020-04-22T18:00:46Z","title":"Observations of Disequilibrium CO Chemistry in the Coldest Brown Dwarfs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.10770","snapshot_observed_at":"2026-08-10T04:20:27.595388Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.595388Z"},"links":{"cited_paper":"/paper/2004.10770","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:bbe39e35200483c80aa553d0c267f424bacbeda3c8074aa74d32b41d66e3763a","observation_id":"50e88a74-c588-4570-9059-55dd20dec37e","resolution":{"observed_at":"2026-08-10T04:20:27.595388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.13873","last_updated":"2020-11-27T17:57:54Z","snapshot_observed_at":"2026-07-06T10:18:25.252546Z","submitted_at":"2020-11-27T17:57:54Z","title":"The Y dwarf population with HST: unlocking the secrets of our coolest neighbours -- I. Overview & First astrometric results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.13873","snapshot_observed_at":"2026-08-10T04:20:27.600695Z","title":"Overview and first astrometric results","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.600695Z"},"links":{"cited_paper":"/paper/2011.13873","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:8b612adc4b0b66b07e4c86da1864cebf7a06d15d22e15b8dfeb01ee2e5bc553d","observation_id":"a77c58aa-391e-43b1-9b79-5088e213fe7e","resolution":{"observed_at":"2026-08-10T04:20:27.600695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.01208","last_updated":"2018-12-04T04:07:12Z","snapshot_observed_at":"2026-08-06T05:39:04.108135Z","submitted_at":"2018-12-04T04:07:12Z","title":"Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the \"Planetary\" Mass Regime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.01208","snapshot_observed_at":"2026-08-10T04:20:27.605993Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.605993Z"},"links":{"cited_paper":"/paper/1812.01208","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:29b911ddf44bbae76ad9789b1406d16bedda1a4e04fb73bae6eff05b473ed1d9","observation_id":"55ea4776-db26-4779-94bd-bef4429b80d4","resolution":{"observed_at":"2026-08-10T04:20:27.605993Z","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":"2026-08-10T04:20:27.611351Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.611351Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:463c802ef1848bb9b30c13440e7acbf4851cb07553cbabb86c53328b1d2fae86","observation_id":"719151ae-67d7-4e4a-8d76-45a8ab6422de","resolution":{"observed_at":"2026-08-10T04:20:27.611351Z","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":"2026-08-10T04:20:27.616019Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.616019Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:82112a910e08d842bae5aa4946c433795d44aa2dddddd17bfd240ad892ddaba4","observation_id":"bb5963ac-a134-4f0d-83bc-041e1f712bad","resolution":{"observed_at":"2026-08-10T04:20:27.616019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.12107","last_updated":"2024-02-08T03:00:51Z","snapshot_observed_at":"2026-07-06T16:09:32.179653Z","submitted_at":"2023-08-22T17:46:06Z","title":"UNCOVER: JWST Spectroscopy of Three Cold Brown Dwarfs at Kiloparsec-scale Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.12107","snapshot_observed_at":"2026-08-10T04:20:27.621544Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.621544Z"},"links":{"cited_paper":"/paper/2308.12107","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:2ba75548a6141169f542212a8f6e3895f3270bcc43782a044e002f9ce5056156","observation_id":"35eba4fe-3d93-461e-ba78-519098d029e4","resolution":{"observed_at":"2026-08-10T04:20:27.621544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.10900","last_updated":"2023-11-09T19:29:41Z","snapshot_observed_at":"2026-07-06T16:08:41.390521Z","submitted_at":"2023-08-21T17:59:27Z","title":"Little Red Dots or Brown Dwarfs? NIRSpec Discovery of Three Distant Brown Dwarfs Masquerading as NIRCam-Selected Highly-Reddened AGNs","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.10900","snapshot_observed_at":"2026-08-10T04:20:27.627571Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.627571Z"},"links":{"cited_paper":"/paper/2308.10900","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:c86cca5cbcfedaabfad1cc9d66f2dbe1ebcdf0056172c81064428fa9d21097ae","observation_id":"fc402fa8-3fb4-4fd4-b61c-f9ba3f252bd3","resolution":{"observed_at":"2026-08-10T04:20:27.627571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08781","last_updated":"2024-09-30T18:00:13Z","snapshot_observed_at":"2026-08-03T23:49:03.952884Z","submitted_at":"2024-07-11T18:00:03Z","title":"JADES: Spectroscopic Confirmation and Proper Motion for a T-Dwarf at 2 Kiloparsecs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08781","snapshot_observed_at":"2026-08-10T04:20:27.633119Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.633119Z"},"links":{"cited_paper":"/paper/2407.08781","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:a4111b5defed76ff36443fcb43dc2f5731e91860a17c7b89021c8c7a5fb4013b","observation_id":"e4c550b3-0b56-4885-9722-b6a74ab414b3","resolution":{"observed_at":"2026-08-10T04:20:27.633119Z","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":"2026-08-10T04:20:27.638297Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.638297Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:5cf1375d74cc256737e5305125da1afe1941c757fd6b21dfd2636e0a77a1626c","observation_id":"2622b58a-d03a-43d4-9039-ac80d418867d","resolution":{"observed_at":"2026-08-10T04:20:27.638297Z","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":"2026-08-10T04:20:27.643352Z","title":"and others , title =","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.643352Z"},"links":{"citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:e48e353deb220001db72be2f43c75ac5deb79c42a50c8a5fd66e35daf1698ed5","observation_id":"76c9d03d-bce9-4308-a1c7-48546221eb3b","resolution":{"observed_at":"2026-08-10T04:20:27.643352Z","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":"2026-07-06T05:10:44.708185Z","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":"2026-08-10T04:20:27.648064Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.648064Z"},"links":{"cited_paper":"/paper/1609.04153","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:8ea327100166f6655227972aa3821ef80457997a315bb7c3829169f9d652ced6","observation_id":"cc73acb8-3909-4d7e-94bd-0db6d4f9cd08","resolution":{"observed_at":"2026-08-10T04:20:27.648064Z","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":"2026-08-08T06:26:45.516905Z","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":"2026-08-10T04:20:27.653366Z","title":"Summary of the content and survey properties","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.653366Z"},"links":{"cited_paper":"/paper/2208.00211","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:22a3fcd0537be6372b4644204f061b13aa9e40c4db54dd1fe3407ed718069b63","observation_id":"aae7e137-568f-43a6-a543-720b8f27429c","resolution":{"observed_at":"2026-08-10T04:20:27.653366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.3051","last_updated":"2014-11-12T02:42:40Z","snapshot_observed_at":"2026-07-06T04:00:16.092779Z","submitted_at":"2014-11-12T02:42:40Z","title":"Weather on Other Worlds. II. Survey Results: Spots Are Ubiquitous on L and T Dwarfs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.3051","snapshot_observed_at":"2026-08-10T04:20:27.659262Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.659262Z"},"links":{"cited_paper":"/paper/1411.3051","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:2c96e3b91e086de87f13760564612645868eaeff1ad9d657f4a7a6b54551530e","observation_id":"7a9cbc0a-9699-409e-b408-4d53fcb85294","resolution":{"observed_at":"2026-08-10T04:20:27.659262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.04711","last_updated":"2022-01-12T21:51:03Z","snapshot_observed_at":"2026-08-07T21:03:36.033632Z","submitted_at":"2022-01-12T21:51:03Z","title":"Let the Great World Spin: Revealing the Stormy, Turbulent Nature of Young Giant Exoplanet Analogs with the Spitzer Space Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.04711","snapshot_observed_at":"2026-08-10T04:20:27.665507Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.665507Z"},"links":{"cited_paper":"/paper/2201.04711","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:1c6b0e906333ab4cfcffd8113b40a316dca8cfb49714113e6e4bf260504501b1","observation_id":"a7a404b7-b56a-45f4-92a8-c6c8a626c573","resolution":{"observed_at":"2026-08-10T04:20:27.665507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07218","last_updated":"2023-11-28T21:46:35Z","snapshot_observed_at":"2026-07-06T16:46:30.470666Z","submitted_at":"2023-11-13T10:25:06Z","title":"A Near-infrared Variability Survey of Young Planetary-mass Objects","version":2},"cited_work":{"arxiv_id":"2311.07218","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.07218","snapshot_observed_at":"2026-08-10T04:20:30.513175Z","title":"A Near-infrared Variability Survey of Young Planetary-mass Objects","venue":"astro-ph.EP","work_id":"d1203eac-f811-4599-b264-f20bcb3f07a9","year":2023},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.671111Z"},"links":{"cited_paper":"/paper/2311.07218","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:7259e93e47ae33732f2ca203098c0aebe848b6210c39adf3ae6b42f6c36d675d","observation_id":"72fa8779-dfca-4390-a9c4-7b4af4610923","resolution":{"observed_at":"2026-08-10T04:20:30.518652Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2606.26411","last_updated":"2026-06-24T22:10:59Z","snapshot_observed_at":"2026-08-03T12:21:43.555379Z","submitted_at":"2026-06-24T22:10:59Z","title":"A Spitzer Space Telescope Exploration Science Program to Search for Y Dwarf Variability","version":1},"cited_work":{"arxiv_id":"2606.26411","doi":"10.48550/arxiv.2606.26411","metadata_source":"pith","pith_arxiv_id":"2606.26411","snapshot_observed_at":"2026-08-10T06:16:20.510975Z","title":"A Spitzer Space Telescope Exploration Science Program to Search for Y Dwarf Variability","venue":"astro-ph.SR","work_id":"8d60cb27-6cc9-47f0-a216-0ad2898268e9","year":2026},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.677097Z"},"links":{"cited_paper":"/paper/2606.26411","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:3a802d6a33cad96f65e62c1b8d8b27efeef3b74dcfa2cf85f2a9c3aba43fc845","observation_id":"78ddb666-d526-4a6f-bdab-427f81030ca7","resolution":{"observed_at":"2026-08-10T04:20:28.497644Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.02464","last_updated":"2022-10-05T18:00:01Z","snapshot_observed_at":"2026-07-06T14:00:05.253488Z","submitted_at":"2022-10-05T18:00:01Z","title":"Roaring Storms in the Planetary-Mass Companion VHS 1256-1257 b: Hubble Space Telescope Multi-epoch Monitoring Reveals Vigorous Evolution in an Ultra-cool Atmosphere","version":1},"cited_work":{"arxiv_id":"2210.02464","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.02464","snapshot_observed_at":"2026-08-10T04:20:30.485675Z","title":"Roaring Storms in the Planetary-Mass Companion VHS 1256-1257 b: Hubble Space Telescope Multi-epoch Monitoring Reveals Vigorous Evolution in an Ultra-cool Atmosphere","venue":"astro-ph.EP","work_id":"34425eb3-4e28-40f7-aba1-bb403189f13e","year":2022},"citing_paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-10T04:20:27.683116Z"},"links":{"cited_paper":"/paper/2210.02464","citing_paper":"/paper/2608.07461"},"observation_digest":"sha256:3bf84c6521116213c4f1e61e95ca861db30b06d31f104f54f0c733a98b46b108","observation_id":"daf9bf90-8e29-4bad-9d34-7c12b020cc26","resolution":{"observed_at":"2026-08-10T04:20:30.492480Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.07461","last_updated":"2026-08-07T17:55:50Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-11T00:13:53.678398Z","submitted_at":"2026-08-07T17:55:50Z","title":"A clear detection of proper motion confirms that the claimed $\\mathbf{z\\simeq32}$ galaxy candidate, \"Capotauro'', is a Y-type brown dwarf"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":95,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":166},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 100 of 166 outbound references and 0 inbound Pith citation observations for arXiv:2608.07461."}