{"as_of":"2026-08-13T04:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e758ea056a3d4c3284cd1848afed0da7d218cd72acf011e1473c423a64308c92","coverage":[{"denominator":163,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T19:25:25.747329Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2412.06894/citation-record","integrity":"/paper/2412.06894/integrity","json":"/paper/2412.06894/citation-record.json","paper":"/paper/2412.06894"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:25:25.399898Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.399898Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:57b7df1b8af5b409c6ef899e41e3e9ed1204bd316faab68808c64cb8ed92f0c7","observation_id":"bad6b962-f96d-4e17-bf7a-49d31591a685","resolution":{"observed_at":"2026-08-11T19:25:25.399898Z","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":"2026-08-11T19:25:25.404949Z","title":"2024, A&A, 685, A1, doi: 10.1051/0004-6361/202348407","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.404949Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:c6eedd11ef8d79e3065c4265236056f39ce4487223982e55c509fcabed780dbd","observation_id":"efe70a69-d44b-4f30-b7f3-3d70c5454d8e","resolution":{"observed_at":"2026-08-11T19:25:25.404949Z","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":"2026-08-11T19:25:25.409232Z","title":"2016, ApJ, 832, 56, doi: 10.3847/0004-637X/832/1/56 Alcalde Pampliega, B., P´erez-Gonz´alez, P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.409232Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:e5efcf6f1791333dca986c138d715f20bfc72753fb40c29366017107320b23ee","observation_id":"f34459e6-b97c-41bd-beec-b40da724066b","resolution":{"observed_at":"2026-08-11T19:25:25.409232Z","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":"2026-08-11T19:25:25.412731Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.412731Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:a287ee26832c51b654b8ee79083d4624bec166b7308eebcb29f461a8642f330d","observation_id":"a3e15ede-c20c-424a-a545-b6c241d72dce","resolution":{"observed_at":"2026-08-11T19:25:25.412731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.04284","last_updated":"2020-09-23T00:39:17Z","snapshot_observed_at":"2026-08-10T07:18:39.549824Z","submitted_at":"2020-06-07T23:09:06Z","title":"The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The nature of the faintest dusty star-forming galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.04284","snapshot_observed_at":"2026-08-11T19:25:25.416321Z","title":"2020, arXiv e-prints, arXiv:2006.04284","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.416321Z"},"links":{"cited_paper":"/paper/2006.04284","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:c42980729b9d7d38d05481eb14c77c537aedc311c2d389893d6f56b2b8e74577","observation_id":"d04533ca-fa76-4fbd-8ecb-483a7f215de2","resolution":{"observed_at":"2026-08-11T19:25:25.416321Z","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":"2026-08-11T19:25:25.420142Z","title":"M., Evans, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.420142Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:2aef311e0c2cc908f4423a205de5606deae53d1193ed474f638b6c9ac45c9a2e","observation_id":"5250be32-5ea3-4823-8c3e-a4fd0210744d","resolution":{"observed_at":"2026-08-11T19:25:25.420142Z","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":"2026-08-11T19:25:25.423815Z","title":"2011, LePHARE: Photometric Analysis for Redshift Estimate, Astrophysics Source Code Library, record ascl:1108.009 Astropy Collaboration, Robitaille, T","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.423815Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:a98a9b51ae881a66031fdafd2c1ec6ce086ae7357713cac236db326d86fbf2d8","observation_id":"db777baf-72ed-461d-af57-ebe81df5ebf0","resolution":{"observed_at":"2026-08-11T19:25:25.423815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08052","last_updated":"2024-04-11T18:00:05Z","snapshot_observed_at":"2026-08-13T00:32:24.042346Z","submitted_at":"2024-04-11T18:00:05Z","title":"Quiescent or dusty? Unveiling the nature of extremely red galaxies at $z>3$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.08052","snapshot_observed_at":"2026-08-11T19:25:25.426879Z","title":"2024, arXiv e-prints, arXiv:2404.08052, doi: 10.48550/arXiv.2404.08052","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.426879Z"},"links":{"cited_paper":"/paper/2404.08052","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:4fe719693712d1e704134b8dc8de2b2215d81cdf9faa06b8ebc60baafe18fe8a","observation_id":"ae6aab9e-92e3-4174-addf-3fc747dec6e6","resolution":{"observed_at":"2026-08-11T19:25:25.426879Z","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":"2026-08-11T19:25:25.430442Z","title":"E., Alexander, D","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.430442Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:f11a44e6c71d27779b6e3806a28bb2798c73ea28880d1b4d06238fa169b6830f","observation_id":"680e3f2e-468d-437a-a6a0-c61ce14653fc","resolution":{"observed_at":"2026-08-11T19:25:25.430442Z","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":"2026-08-11T19:25:25.434053Z","title":"2024, A&A, 686, A3, doi: 10.1051/0004-6361/202348845","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.434053Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:3481fe7c6ddfb0d2e17942cb167bd7c251d48e71f6dc6d91789ad60bb167387e","observation_id":"1bbb6aa9-de62-479e-884c-6bc93b0554bf","resolution":{"observed_at":"2026-08-11T19:25:25.434053Z","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":"2026-08-11T19:25:25.437239Z","title":"A., Gillman, S., Melinder, J., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.437239Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:cd0ddb70e77a78f8a336735f22b3112b79781be6369a9b6038dbe09e603b3da7","observation_id":"30a65a46-9b6e-4fdf-9407-e4df1863c654","resolution":{"observed_at":"2026-08-11T19:25:25.437239Z","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":"2026-08-11T19:25:25.440418Z","title":"2019, A&A, 622, A103, doi: 10.1051/0004-6361/201834156","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.440418Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:7b7a07d385f004123629ac3d9870beddae1018c76345c700e270a0c20ef57b56","observation_id":"53fc455d-146e-4ee8-b007-7c6d6f9a4455","resolution":{"observed_at":"2026-08-11T19:25:25.440418Z","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":"2026-08-11T19:25:25.443742Z","title":"2020, ApJ, 902, 112, doi: 10.3847/1538-4357/abb830","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.443742Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:931acc2aea9319701ef1821ca34d5623a6e24c2c5cddf442544060f0b8081af4","observation_id":"5524d844-6808-4885-b02a-44e0280f79a3","resolution":{"observed_at":"2026-08-11T19:25:25.443742Z","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":"2026-08-11T19:25:25.447032Z","title":"J., Illingworth, G","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.447032Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:b859043079c7ca04d83fe5f92ab3dd05fb981b0045a3aa9c92319204a3f534b9","observation_id":"e60da22f-c837-4c72-97c4-7683dc1a8114","resolution":{"observed_at":"2026-08-11T19:25:25.447032Z","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":"2026-08-11T19:25:25.449983Z","title":"2024, astropy/photutils: 1.12.0, 1.12.0, Zenodo, doi: 10.5281/zenodo.10967176","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.449983Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:0ca32b0d3b01bebfb540fc8b20e59384fdffd7708985f31059876e558d062420","observation_id":"5beb2d4d-1db3-40ee-bf16-d248cf15a04f","resolution":{"observed_at":"2026-08-11T19:25:25.449983Z","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":"2026-08-11T19:25:25.453218Z","title":"2003, MNRAS, 344, 1000, doi: 10.1046/j.1365-8711.2003.06897.x","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.453218Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:c032b24ebc4ee856891dc411a29b06220771cd02fe1b4e131226210151983f72","observation_id":"45fa4c51-6c48-4a78-a1aa-57fcae35f9c0","resolution":{"observed_at":"2026-08-11T19:25:25.453218Z","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":"2026-08-11T19:25:25.456197Z","title":"2013, A&A, 554, A70, doi: 10.1051/0004-6361/201321651","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.456197Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:fb4aaba105a9018c4d5b5b90f9183a3fa59ef3cf17b19139766d130b247d6067","observation_id":"d97d014c-5cba-46fe-9cc1-da8126a889ab","resolution":{"observed_at":"2026-08-11T19:25:25.456197Z","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.7829329","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:28:41.353208Z","title":"2023, JWST Calibration Pipeline, 1.10.2, Zenodo, doi: 10.5281/zenodo.7829329","venue":null,"work_id":"3c1ac61e-b34b-4719-9481-baac96eb6b08","year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.459710Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:b79ecf09d5da8f3100a976f11c132d8e87f5c1ef31c6105072168a8c3870f8a8","observation_id":"f1650af7-bc9b-435e-ae10-e87a024061eb","resolution":{"observed_at":"2026-08-11T19:28:41.368477Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.10323","last_updated":"2023-07-25T16:16:20Z","snapshot_observed_at":"2026-08-10T09:11:09.738324Z","submitted_at":"2023-02-20T21:28:06Z","title":"Bright submillimeter galaxies do trace galaxy protoclusters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.10323","snapshot_observed_at":"2026-08-11T19:25:25.462910Z","title":"2023, arXiv e-prints, arXiv:2302.10323, doi: 10.48550/arXiv.2302.10323","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.462910Z"},"links":{"cited_paper":"/paper/2302.10323","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:1e10df53ced68517fcd7609726e147052de33088b960394e262f55d7706cde09","observation_id":"ff2f8b1a-044f-40f7-bdeb-9248b45c89db","resolution":{"observed_at":"2026-08-11T19:25:25.462910Z","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":"2026-08-11T19:25:25.466330Z","title":"2021, MNRAS, 502, 4558, doi: 10.1093/mnras/staa4037","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.466330Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:8404a53fa9b26ca84dc72069772087e9dbc7339da391c15b2943d87dc8bd85a4","observation_id":"0a063554-496b-465b-966c-3a43a23b3993","resolution":{"observed_at":"2026-08-11T19:25:25.466330Z","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":"2026-08-11T19:25:25.469460Z","title":"1997, in American Institute of Physics Conference","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.469460Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:8d49a018f66fcf5e89bc777ca0d7b99bda140e5611f4e62a74c716d07ace571a","observation_id":"431fab17-3071-408e-b14c-6cdd63531815","resolution":{"observed_at":"2026-08-11T19:25:25.469460Z","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":"2026-08-11T19:25:25.472644Z","title":"408, The ultraviolet universe at low and High redshift, ed","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.472644Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:489856fa96b694861ef01c935a42b84f22a250022cf2200183611830becb62c1","observation_id":"190736f2-54ae-4ba7-bbdb-3dd1710cc073","resolution":{"observed_at":"2026-08-11T19:25:25.472644Z","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":"2026-08-11T19:25:25.476506Z","title":"C., et al","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.476506Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:3ea4a13a46db98d5c9c55ec79cd8eb727ad9a8608c3624c267b9df1edcb0e6ca","observation_id":"780de99c-b9b5-4117-abcf-adca92436ff0","resolution":{"observed_at":"2026-08-11T19:25:25.476506Z","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":"2026-08-11T19:25:25.480376Z","title":"I., Dunlop, J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.480376Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:c2ecff34fd682fde15ea92514c3c4397ee2618c69742bd1531d32c879d887c71","observation_id":"04009049-f8fc-4820-8f87-5fd7a89f577d","resolution":{"observed_at":"2026-08-11T19:25:25.480376Z","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":"2026-08-11T19:25:25.484233Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.484233Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:b21c4d80712003ac3022abab0f0c9fdb62e905cd5836a429a4cfc9c05daf36e5","observation_id":"bf36fe8c-21ab-45f6-9011-5c2791ce954c","resolution":{"observed_at":"2026-08-11T19:25:25.484233Z","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":"2026-08-11T19:25:25.488121Z","title":"M., Hodge, J., Zavala, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.488121Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:55149fd1f10c7f6524981f5ffc9d2b2a1dadc1f136fe0c9ceea2e45b5982b075","observation_id":"4afbda73-a8cf-4042-acaf-8b3a49064467","resolution":{"observed_at":"2026-08-11T19:25:25.488121Z","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":"2026-08-11T19:25:25.491997Z","title":"M., Narayanan, D., & Cooray, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.491997Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:1a624f94e7ebc34bd5d083fad102321a7f413597e08f0838f8d3dd8656a42b3c","observation_id":"b1be4338-993e-482b-9ba4-7c5851aff4a9","resolution":{"observed_at":"2026-08-11T19:25:25.491997Z","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":"2026-08-11T19:25:25.495725Z","title":"M., Chen, C.-C., Cowie, L","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.495725Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:2083b2ce3213312292713d96915fe61ab1ef1c2154a691cdadded048b9f7348e","observation_id":"e94dfbfa-2296-40f0-a9e4-b351a77afe69","resolution":{"observed_at":"2026-08-11T19:25:25.495725Z","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":"2026-08-11T19:25:25.499357Z","title":"M., Scoville, N","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.499357Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:1da89ebe519adb806d107233c275e08b5d41b997aa72fe9adfd59d7404c41d82","observation_id":"13add364-40fa-4e18-93f6-156a90bc7e2d","resolution":{"observed_at":"2026-08-11T19:25:25.499357Z","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":"2026-08-11T19:25:25.503214Z","title":"M., Zavala, J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.503214Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:92c3d21415203bdcaebb4a3ec1c4cf230f148747e3aca200888aa164f30a91cb","observation_id":"91bfa06e-431f-4d8a-ba76-6f6de51c2023","resolution":{"observed_at":"2026-08-11T19:25:25.503214Z","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":"2026-08-11T19:25:25.507001Z","title":"M., Zavala, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.507001Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:3e645b7fbfe5f7132e44b051f50e210752587f146a17022f16489b689265f30b","observation_id":"ff680103-0eca-4a44-9395-e66a5f45d482","resolution":{"observed_at":"2026-08-11T19:25:25.507001Z","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":"2026-08-11T19:25:25.510263Z","title":"M., Zavala, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.510263Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:3281f9e7f15795d727bdf3567969e58cefbd36d08fc79e441815880628b0da5b","observation_id":"7c95ff3c-425f-495b-8f2c-fbb7f354d3cd","resolution":{"observed_at":"2026-08-11T19:25:25.510263Z","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":"2026-08-11T19:25:25.513472Z","title":"2003, PASP, 115, 763, doi: 10.1086/376392","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.513472Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:3864c071c9777b26d51ecb57da670c62e840c92dd291db95281bd3fd075ab535","observation_id":"81e59ec1-31be-407c-a913-4fcba7cbc15d","resolution":{"observed_at":"2026-08-11T19:25:25.513472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.03826","last_updated":"2025-02-20T22:11:00Z","snapshot_observed_at":"2026-08-12T22:30:30.219597Z","submitted_at":"2024-10-04T18:00:07Z","title":"A Quasar-Anchored Protocluster at z=6.6 in the ASPIRE Survey: I. Properties of [OIII] Emitters in a 10 Mpc Overdensity Structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.03826","snapshot_observed_at":"2026-08-11T19:25:25.516973Z","title":"B., Wang, F., Zhang, H., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.516973Z"},"links":{"cited_paper":"/paper/2410.03826","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:f1a9ddd818d986af651fc74fee110155350bf1afd6397fbab962f6988cdd02b6","observation_id":"19561e30-9469-40f9-be77-ec0077caa8ae","resolution":{"observed_at":"2026-08-11T19:25:25.516973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.03827","last_updated":"2025-02-20T22:16:00Z","snapshot_observed_at":"2026-08-12T22:30:30.137480Z","submitted_at":"2024-10-04T18:00:09Z","title":"A Quasar-Anchored Protocluster at z=6.6 in the ASPIRE Survey: II. An Environmental Analysis of Galaxy Properties in an Overdense Structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.03827","snapshot_observed_at":"2026-08-11T19:25:25.520586Z","title":"B., Wang, F., Yang, J., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.520586Z"},"links":{"cited_paper":"/paper/2410.03827","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:9a3147d7f72e9e534e531888fd6be8b7362e4093383932de6e0328afc35d0ed9","observation_id":"d7f814c3-1c2f-4647-a44d-04fecaa26484","resolution":{"observed_at":"2026-08-11T19:25:25.520586Z","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":"2026-08-11T19:25:25.524184Z","title":"2001, ApJ, 556, 562, doi: 10.1086/321609 24","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.524184Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:40ac3dbaac684f76ae708bca4384fadc89ee53519c2a0d9fe6467c16b7383edf","observation_id":"be28028e-b46d-447d-869c-be87fae4bb89","resolution":{"observed_at":"2026-08-11T19:25:25.524184Z","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":"2026-08-11T19:25:25.527372Z","title":"2022, ApJ, 929, 159, doi: 10.3847/1538-4357/ac61df","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.527372Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:5b53acd10a87ec88d52a2c5bbda6fefacfc5f2ab1205e6b2d0692818e6357b04","observation_id":"efe7310b-430c-4109-bf90-a7d35a77e897","resolution":{"observed_at":"2026-08-11T19:25:25.527372Z","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":"2026-08-11T19:25:25.530400Z","title":"J., Zwaan, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.530400Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:ad39856f933fea7fe79c5fb1f05c4eb1df914b55bad9032099abee154b27e249","observation_id":"41d036ff-fa9c-4210-a875-eb82fb9db2f3","resolution":{"observed_at":"2026-08-11T19:25:25.530400Z","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":"2026-08-11T19:25:25.533454Z","title":"2023, A&A, 673, L6, doi: 10.1051/0004-6361/202346535","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.533454Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:98d5a3f0d64bc56804de8c89e7a8f520c436d64c90044a9687d7edf588e59a5a","observation_id":"c3c6658d-6283-4e19-9fd2-6b25fb8c776a","resolution":{"observed_at":"2026-08-11T19:25:25.533454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08387","last_updated":"2024-10-10T21:46:54Z","snapshot_observed_at":"2026-08-12T22:25:53.922142Z","submitted_at":"2024-10-10T21:46:54Z","title":"RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at $z\\sim2$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.08387","snapshot_observed_at":"2026-08-11T19:25:25.536385Z","title":"R., Brammer, G., Heintz, K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.536385Z"},"links":{"cited_paper":"/paper/2410.08387","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:3b59faeb7db6788ad4ca0cc6e66bb68d6546849731135ac1b84f243ebe69c9b8","observation_id":"666b6d97-4871-420a-bca6-c29ea8237cd5","resolution":{"observed_at":"2026-08-11T19:25:25.536385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/339545","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:28:41.116630Z","title":"L., Garmire, G","venue":null,"work_id":"1d9bbcb5-6f12-4a9b-9950-40734559b75e","year":2002},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.539803Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:2eed0f1b60d61b9d4cef6dea9d1a2af50133519525250b0d6cc2767dbb39b062","observation_id":"f5e1baed-fbbe-45da-a3eb-44d1d4dff20a","resolution":{"observed_at":"2026-08-11T19:28:41.122238Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:25:25.543216Z","title":"2012, A&A, 539, A31, doi: 10.1051/0004-6361/201118010 da Cunha, E., Groves, B., Walter, F., et al","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.543216Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:f35e07726c31eb9c0bba89976955026ec4c3ee8b2acac7846da2384ea07522aa","observation_id":"d6c88a39-a2bd-4631-a292-6d39826a146c","resolution":{"observed_at":"2026-08-11T19:25:25.543216Z","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":"2026-08-11T19:25:25.546246Z","title":"P., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.546246Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:9d452da9a2dbff981aa1ad6e51dfca09a0c8150936095c8b30ca868e6a1bd140","observation_id":"149043bf-2321-41a0-bda9-733ac918b155","resolution":{"observed_at":"2026-08-11T19:25:25.546246Z","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":"2026-08-11T19:25:25.549514Z","title":"J., Lang, D., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.549514Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:27325106b77bcf136502f577a9e1047f32972a0e39cfb7eb3fdb552c1037cc08","observation_id":"4b485855-6847-4479-9451-7af815848bab","resolution":{"observed_at":"2026-08-11T19:25:25.549514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.16655","last_updated":"2022-03-30T20:15:41Z","snapshot_observed_at":"2026-08-13T01:42:30.417551Z","submitted_at":"2022-03-30T20:15:41Z","title":"No Redshift Evolution of Dust Temperatures from $0 < z < 2$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.16655","snapshot_observed_at":"2026-08-11T19:25:25.552523Z","title":"M., & Casey, C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.552523Z"},"links":{"cited_paper":"/paper/2203.16655","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:752e5a3403a834570ddbec7ca090fa9291f97686b16eb39fb13173760d9936fb","observation_id":"06e90682-9831-4584-9e2d-36f302b797f6","resolution":{"observed_at":"2026-08-11T19:25:25.552523Z","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":"2026-08-11T19:25:25.555953Z","title":"P., & Robotham, A","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.555953Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:54867acae3be3b7fb2c0e302395d3bcdec6147c2ccc7edce390a44fa77d2d344","observation_id":"6dc336c4-afbe-4dbd-aa8a-69e75e530b61","resolution":{"observed_at":"2026-08-11T19:25:25.555953Z","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":"2026-08-11T19:25:25.559107Z","title":"S., McLure, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.559107Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:8a69f812e26d7bad215c1f78238d0f11b19e6d199861e6aace565a0989c2b755","observation_id":"9a765170-76f6-4b5e-8a63-8f455976db2e","resolution":{"observed_at":"2026-08-11T19:25:25.559107Z","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":"2026-08-11T19:25:25.562558Z","title":"2022, ApJ, 927, 204, doi: 10.3847/1538-4357/ac51ca","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.562558Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:64fde3253dec364ee9cbd4bb32a5853498a687157e3c8b4679f9574c36c89380","observation_id":"0b2009c1-11bf-4e89-b0b2-5bef7714364c","resolution":{"observed_at":"2026-08-11T19:25:25.562558Z","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":"2026-08-11T19:25:25.565807Z","title":"L., Fudamoto, Y ., Oesch, P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.565807Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:321cc2d5ec3fb2847e73f7435279405e5578cbf640a3a82fb636f90ef92e3cbe","observation_id":"8f685528-2900-4a2c-94ac-c6c5b820588b","resolution":{"observed_at":"2026-08-11T19:25:25.565807Z","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":"2026-08-11T19:25:25.569226Z","title":"L., Ryan, Russell E., J., Papovich, C., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.569226Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:85022b99da617881fca0dea243b5d1a584600afc42df3b385059cec0d47aa34a","observation_id":"9851e7e5-64de-4df9-b1b7-9f8dbbdb7c08","resolution":{"observed_at":"2026-08-11T19:25:25.569226Z","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":"2026-08-11T19:25:25.572716Z","title":"W., Lang, D., & Goodman, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.572716Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:d2ce3b6aa8c0b23c0cd3f33363327b85ba0eaa8c265721fe5198fbd749bef914","observation_id":"bc5871bc-c111-45f0-86e2-0f0e300cfcd7","resolution":{"observed_at":"2026-08-11T19:25:25.572716Z","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":"2026-08-11T19:25:25.576461Z","title":"2018, A&A, 620, A152, doi: 10.1051/0004-6361/201832928","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.576461Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:de288a17abfb862c22803364f18cee4b09099559710ddbbb6633d5bbb2197953","observation_id":"dd11b56b-6ef8-471b-baee-7c2cdf8edc5c","resolution":{"observed_at":"2026-08-11T19:25:25.576461Z","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":"2026-08-11T19:25:25.580076Z","title":"A., Faisst, A., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.580076Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:cc8fe885c97fc56050a11c5f49c4147be66fc81c33834e7eff1a45cb54e4cce3","observation_id":"96e56d10-693c-4eb3-ab6c-e2acc128fac7","resolution":{"observed_at":"2026-08-11T19:25:25.580076Z","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":"2026-08-11T19:25:25.584955Z","title":"A., Schouws, S., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.584955Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:f5e16e028016e7eb0c01a28998e24e01e3c06b80723d6b952d292633afeeeddd","observation_id":"bb4990fa-cb2f-4590-bc4c-25d63479c16e","resolution":{"observed_at":"2026-08-11T19:25:25.584955Z","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":"2026-08-11T19:25:25.588677Z","title":"2016, ApJS, 222, 1, doi: 10.3847/0067-0049/222/1/1","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.588677Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:78644f757eb433716d87f5e5a33f2c183b5eb1a58157c19b92bb790d609dee3d","observation_id":"4b13b715-5aa4-44ed-bda9-75d969821d14","resolution":{"observed_at":"2026-08-11T19:25:25.588677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.01658","last_updated":"2024-06-20T17:15:14Z","snapshot_observed_at":"2026-07-06T14:58:10.658020Z","submitted_at":"2023-03-03T01:29:45Z","title":"ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at $z\\simeq1-8$","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.01658","snapshot_observed_at":"2026-08-11T19:25:25.592850Z","title":"2023, arXiv e-prints, arXiv:2303.01658, doi: 10.48550/arXiv.2303.01658 Gaia Collaboration, Vallenari, A., Brown, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.592850Z"},"links":{"cited_paper":"/paper/2303.01658","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:0a270db22e2bad0a33856bf3cbb66df8d3b6fa0a58ba8eb9402b88653769c0be","observation_id":"bc96ca57-8e66-48e8-b2d7-f75d077ab0a0","resolution":{"observed_at":"2026-08-11T19:25:25.592850Z","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":"2026-08-11T19:25:25.596766Z","title":"P., Mather, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.596766Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:b9e27c7ce9d2bc2b209c4afcb9d5917e8d24af54d6bf4c7f0b541367891cd6ea","observation_id":"5f603a30-b121-4fc2-b061-fafa96857c2a","resolution":{"observed_at":"2026-08-11T19:25:25.596766Z","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":"2026-08-11T19:25:25.600545Z","title":"E., Dunlop, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.600545Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:66c84668980e656e7c64a6c439263e275bac357e0d86814f93fee500606bad7a","observation_id":"316accbb-f8f1-4f7f-b09d-4576cce97e08","resolution":{"observed_at":"2026-08-11T19:25:25.600545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.07199","last_updated":"2020-02-17T19:00:21Z","snapshot_observed_at":"2026-08-07T22:32:44.264630Z","submitted_at":"2020-02-17T19:00:21Z","title":"The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.07199","snapshot_observed_at":"2026-08-11T19:25:25.603512Z","title":"1986, ApJ, 303, 336, doi: 10.1086/164079 Gim´enez-Arteaga, C., Brammer, G","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.603512Z"},"links":{"cited_paper":"/paper/2002.07199","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:e3978065dbd63943ae213c12538dbcfa853cfd76bbd42f847de1a91dbfaa1dac","observation_id":"e98d4739-64a6-4829-8f27-7b0d7f00db0b","resolution":{"observed_at":"2026-08-11T19:25:25.603512Z","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":"2026-08-11T19:25:25.606853Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.606853Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:36f53be1e9ec67be46661e25c35bbbb722b01df5af01ca7e9252701ffb16bc13","observation_id":"8119c653-8812-40c6-b6e5-bf8506575dc2","resolution":{"observed_at":"2026-08-11T19:25:25.606853Z","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":"2026-08-11T19:25:25.609804Z","title":"A., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.609804Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:bdb6147a309f40cc40405b0500010374c1d4646eed110ebece6ff990e60f2d35","observation_id":"08853fd1-c723-4ed0-bc12-9d53885f4d37","resolution":{"observed_at":"2026-08-11T19:25:25.609804Z","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":"2026-08-11T19:25:25.613239Z","title":"2013, MNRAS, 432, 23, doi: 10.1093/mnras/stt308","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.613239Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:81cf9a8173bcc47b36c226c9a3f8c161a1a148abe9e929bfa0ea83ee1cb71665","observation_id":"2dcfe664-4aa2-473f-9411-83f7a6114d86","resolution":{"observed_at":"2026-08-11T19:25:25.613239Z","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":"2026-08-11T19:25:25.616619Z","title":"2020, A&A, 643, A8, doi: 10.1051/0004-6361/202038487","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.616619Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:1b91124941ffcd1d6c599133b6d30cc905eea13b878f9011242087d2056fa1b5","observation_id":"09e421f0-473c-463c-9847-3e135b3c74c2","resolution":{"observed_at":"2026-08-11T19:25:25.616619Z","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":"2026-08-11T19:25:25.620081Z","title":"2018, PASJ, 70, 105, doi: 10.1093/pasj/psy104","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.620081Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:d09a812ebe9cd282892708cada49ef4a9710415736fc2316e5d0cd150809dead","observation_id":"7248232b-3920-490e-861d-c7672acb805b","resolution":{"observed_at":"2026-08-11T19:25:25.620081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04525","last_updated":"2023-09-08T18:00:02Z","snapshot_observed_at":"2026-08-06T10:09:09.423747Z","submitted_at":"2023-09-08T18:00:02Z","title":"Mapping dusty galaxy growth at $z>5$ with FRESCO: Detection of H$\\alpha$ in submm galaxy HDF850.1 and the surrounding overdense structures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04525","snapshot_observed_at":"2026-08-11T19:25:25.623537Z","title":"J., Oesch, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.623537Z"},"links":{"cited_paper":"/paper/2309.04525","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:c9ae4fbd6a9ad0d070b7e8fb184576399015b63094eecd8d0a9064cf388ec1eb","observation_id":"96d5a40f-4a7a-4789-be8c-7193be0a5091","resolution":{"observed_at":"2026-08-11T19:25:25.623537Z","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":"2026-08-11T19:25:25.627441Z","title":"A., & da Cunha, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.627441Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:5ae18cd0cd082a8ce6fd2da3a2a45b52dad4944eff0e3f9a62a1e4915e0bd942","observation_id":"bb8a502f-aff9-4ff5-b900-a10f0b3a7e61","resolution":{"observed_at":"2026-08-11T19:25:25.627441Z","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":"2026-08-11T19:25:25.631543Z","title":"1986, PASP, 98, 609, doi: 10.1086/131801","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.631543Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:b669e6749ab2476f66b03a3a20a157afba96c5b2c17e926e8bb2e480ca69c3fa","observation_id":"17d55039-e673-411f-8fc3-a5fa14f6784a","resolution":{"observed_at":"2026-08-11T19:25:25.631543Z","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":"2026-08-11T19:25:25.634818Z","title":"S., Zheng, X","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.634818Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:bd9a656d3d6bf1de4e80f0b8bd5a119cc4a005913849279d35beb31b35318858","observation_id":"810cbc9a-d8b2-4ccc-aace-3ab6cba9c21e","resolution":{"observed_at":"2026-08-11T19:25:25.634818Z","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":"2026-08-11T19:25:25.638163Z","title":"H., Serjeant, S., Dunlop, J., et al","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.638163Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:ffcd919fbbff388d1221412bf86405b7222589275c7e2b383a05a06a9c890558","observation_id":"929206ed-d073-4fb7-bbf8-ad092c100999","resolution":{"observed_at":"2026-08-11T19:25:25.638163Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-11T19:25:25.641359Z","title":"R., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.641359Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:6a3cafc6957e6beca1467bb2dc271c836b054eff300952a5d25a9f473d391a60","observation_id":"7bafd653-7e4d-4222-9616-162e2a4a0fa2","resolution":{"observed_at":"2026-08-11T19:25:25.641359Z","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":"2026-08-11T19:25:25.644501Z","title":"2019a, ApJS, 244, 33, doi: 10.3847/1538-4365/ab3bfe","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.644501Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:6bdbf1a24142c43fda0ff77359cf762015e85ca282c6d5202a38c48e44b02860","observation_id":"f851d037-9be8-4a9a-b37e-1ad0756fa6f2","resolution":{"observed_at":"2026-08-11T19:25:25.644501Z","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":"2026-08-11T19:25:25.647740Z","title":"E., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.647740Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:53f307546196bdbec3763d4036aa2127018a59769792c1df146b6b60e5ac8b26","observation_id":"d906066e-6d76-457d-a1b0-6c5ab185bf74","resolution":{"observed_at":"2026-08-11T19:25:25.647740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07585","last_updated":"2024-10-21T14:35:33Z","snapshot_observed_at":"2026-08-13T01:56:25.708619Z","submitted_at":"2024-07-10T12:17:51Z","title":"A photo-z cautionary tale: Redshift confirmation of COSBO-7 at z=2.625","version":2},"cited_work":{"arxiv_id":"2407.07585","doi":"10.48550/arxiv.2407.07585","metadata_source":"pith","pith_arxiv_id":"2407.07585","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"A photo-z cautionary tale: Redshift confirmation of COSBO-7 at z=2.625","venue":"astro-ph.GA","work_id":"f8b3c732-356d-427f-afca-fa583b8d61c0","year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.651521Z"},"links":{"cited_paper":"/paper/2407.07585","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:533f145f6bfb02f550120484be2eca5460b7d1749ae30d0a59c67eb582444b3f","observation_id":"11f4e053-d2dc-4e66-b067-30f23ec50ba2","resolution":{"observed_at":"2026-08-11T19:28:40.809578Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.01318","last_updated":"2024-10-02T08:22:36Z","snapshot_observed_at":"2026-08-12T22:32:48.255764Z","submitted_at":"2024-10-02T08:22:36Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Supports Earlier Reionization around [OIII] Emitters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.01318","snapshot_observed_at":"2026-08-11T19:25:25.655200Z","title":"2024b, arXiv e-prints, arXiv:2410.01318, doi: 10.48550/arXiv.2410.01318","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.655200Z"},"links":{"cited_paper":"/paper/2410.01318","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:62cfb4013320c7b6c77adce4a140140987a15ade02aac6223e2142f9cad2e087","observation_id":"01c2f0d1-febc-4b7a-8e6b-ff918323d6cc","resolution":{"observed_at":"2026-08-11T19:25:25.655200Z","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":"2026-08-11T19:25:25.658567Z","title":"P., Limousin, M., et al","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.658567Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:1ef556dc8b57870ec87d765ab3e1c7e91aced6468b24ea3a8a610f4363d3b924","observation_id":"cbf38594-d15e-40f4-bbe7-1b046720eafe","resolution":{"observed_at":"2026-08-11T19:25:25.658567Z","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":"2026-08-11T19:25:25.661731Z","title":"1998, ARA&A, 36, 189, doi: 10.1146/annurev.astro.36.1.189","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.661731Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:baf8c773e1ba714cc437b8bf47425b00c7fbf19f597f6fc01df9ef64aa1556ed","observation_id":"fb89037b-d372-4a79-b92a-2584e0b9f403","resolution":{"observed_at":"2026-08-11T19:25:25.661731Z","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":"2026-08-11T19:25:25.664822Z","title":"A., Tsutsumi, T., Brogan, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.664822Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:4457f841a3328d6b5ee6ada7ba3d3bf2a1c1bc860774c34e7a922d925b115d00","observation_id":"fdb7b89b-1e59-49bd-9a4f-6b712865df2d","resolution":{"observed_at":"2026-08-11T19:25:25.664822Z","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":"2026-08-11T19:25:25.668510Z","title":"2021, A&A, 649, A152, doi: 10.1051/0004-6361/202038944","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.668510Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:ff250527474a7f2808df907a219d6209d0546bc0a66cf0089982029b99b9a7fa","observation_id":"d6fbaea9-49c9-48e4-b6f8-14663181e484","resolution":{"observed_at":"2026-08-11T19:25:25.668510Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.15126","last_updated":"2023-05-24T13:19:41Z","snapshot_observed_at":"2026-07-06T15:32:31.593213Z","submitted_at":"2023-05-24T13:19:41Z","title":"Unbiased surveys of dust-enshrouded galaxies using ALMA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.15126","snapshot_observed_at":"2026-08-11T19:25:25.672302Z","title":"2023, arXiv e-prints, arXiv:2305.15126, doi: 10.48550/arXiv.2305.15126","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.672302Z"},"links":{"cited_paper":"/paper/2305.15126","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:c8f1b33763dbb7fc98dc1fcc52ce8399d7190dbd4660d0ca53a9094113a962b0","observation_id":"d0a971df-85f6-4103-9258-0f9f6ee3beec","resolution":{"observed_at":"2026-08-11T19:25:25.672302Z","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":"2026-08-11T19:25:25.676099Z","title":"2022, ApJS, 263, 38, doi: 10.3847/1538-4365/ac9909","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.676099Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:5e7f20c5b9e3ba8680b2261abd238eb11c94c5b2cf47a47e3078265d1b0fa0aa","observation_id":"2264bc3f-8b52-40ef-885b-bbbd8a412718","resolution":{"observed_at":"2026-08-11T19:25:25.676099Z","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":"2026-08-11T19:25:25.679823Z","title":"P., Dunlop, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.679823Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:719e09d23e83a133f419e5366f4991f48ce7b5890d77cbbbcec85c8e96da2f41","observation_id":"1baf1cab-e50f-4dfd-8b8b-a4a92aa402be","resolution":{"observed_at":"2026-08-11T19:25:25.679823Z","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":"2026-08-11T19:25:25.684054Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.684054Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:a57f7ffd5934e7c16de845f8160df57864073d467ad2c341bb2626714c572f30","observation_id":"4c759878-cba6-42a9-8438-7ebc299c0e00","resolution":{"observed_at":"2026-08-11T19:25:25.684054Z","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":"2026-08-11T19:25:25.688016Z","title":"2020, ApJ, 889, 80, doi: 10.3847/1538-4357/ab607f","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.688016Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:887d59d20998e3b598e7187bf12f726b0a5e36c521585ce630c44dd9a2d4068b","observation_id":"83140a93-fb59-430a-b134-a84989b88ff5","resolution":{"observed_at":"2026-08-11T19:25:25.688016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.16649","last_updated":"2024-07-04T05:26:56Z","snapshot_observed_at":"2026-07-06T17:35:32.522920Z","submitted_at":"2024-02-26T15:22:12Z","title":"A Strongly Lensed Dusty Starburst of an Intrinsic Disk Morphology at Photometric Redshift of $z_{\\rm ph}>7$","version":3},"cited_work":{"arxiv_id":"2402.16649","doi":"10.48550/arxiv.2402.16649","metadata_source":"pith","pith_arxiv_id":"2402.16649","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"A Strongly Lensed Dusty Starburst of an Intrinsic Disk Morphology at Photometric Redshift of $z_{\\rm ph}>7$","venue":"astro-ph.GA","work_id":"34f3c9f2-0ab2-4401-8fe9-4bd85adadf3b","year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.691903Z"},"links":{"cited_paper":"/paper/2402.16649","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:851636ef3fca1d12e3b13e8deb2cd9f71eab97629f0e11f7c966807ba6eec5e0","observation_id":"95b32bcc-f853-4e9e-a2a2-14dc89947d70","resolution":{"observed_at":"2026-08-11T19:25:26.614187Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:25:25.695874Z","title":"2018, ApJ, 853, 172, doi: 10.3847/1538-4357/aaa600","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.695874Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:6920a2ab1aa07de41e94eef180ce5c4c17f790a3f43c5ea520fefc68ba39c18d","observation_id":"351073a0-549f-47b7-8f3e-50d351197644","resolution":{"observed_at":"2026-08-11T19:25:25.695874Z","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":"2026-08-11T19:25:25.698930Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.698930Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:ae46f2bc368f42091570f2f91df15f2a5249c56e5045b0fbf589aecc5c4f7b6a","observation_id":"64f5a114-3318-46ef-a677-edff08119a7a","resolution":{"observed_at":"2026-08-11T19:25:25.698930Z","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":"2026-08-11T19:25:25.702012Z","title":"H., & Shi, Y","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.702012Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:7a1f81172f852b85ba4dd93a9e9f6e5a8a77d2b58c1168e6fa3793ba5c54f04b","observation_id":"130b7534-5144-4060-bd47-a8dc73cc0699","resolution":{"observed_at":"2026-08-11T19:25:25.702012Z","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":"2026-08-11T19:25:25.705230Z","title":"2014, ARA&A, 52, 415, doi: 10.1146/annurev-astro-081811-125615","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.705230Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:2e5d2cbbaca0d7586416525a3c34d09a16facfd4f2eb726e10e9c91cd9ce8a58","observation_id":"52ac687b-03f0-4f3a-9106-3a218f636aa3","resolution":{"observed_at":"2026-08-11T19:25:25.705230Z","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":"2026-08-11T19:25:25.708326Z","title":"2014, A&A, 561, A86, doi: 10.1051/0004-6361/201322217","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.708326Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:17f522f732e650d11b0a4848ef46990c80248ffc3ffacb1196b4e0b1099bdf94","observation_id":"960ddca2-4646-4131-a1f7-290c1d9d52dc","resolution":{"observed_at":"2026-08-11T19:25:25.708326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18086","last_updated":"2024-05-28T11:46:22Z","snapshot_observed_at":"2026-08-12T23:56:15.018320Z","submitted_at":"2024-05-28T11:46:22Z","title":"A$^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4 < z < 5$","version":1},"cited_work":{"arxiv_id":"2405.18086","doi":"10.48550/arxiv.2405.18086","metadata_source":"pith","pith_arxiv_id":"2405.18086","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"A$^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4 < z < 5$","venue":"astro-ph.GA","work_id":"1bbd5032-104f-44e5-af3e-52142fd6cfec","year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.712444Z"},"links":{"cited_paper":"/paper/2405.18086","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:02b66e14ef96cd740f2281efdca42f600c1121bd2d0361233da7b170f1e2679f","observation_id":"b662d0d5-1a61-43de-988e-d79e1ee58858","resolution":{"observed_at":"2026-08-11T19:25:26.563059Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T19:25:25.716078Z","title":"M., Casey, C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.716078Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:ceb82f59a5fb4dad2023c31ab2f8415be2aab39d569060c70162393c394f5d57","observation_id":"fa04e06d-768a-4d03-9d99-ef3082a61cf7","resolution":{"observed_at":"2026-08-11T19:25:25.716078Z","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":"2026-08-11T19:25:25.719527Z","title":"P., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.719527Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:c2112c25613e58a8bc8e72d46903f181836ec62c55c3496f6d2a3d9ff92edc0f","observation_id":"302dc1ce-fe2f-4ea6-b151-8e4296dd87da","resolution":{"observed_at":"2026-08-11T19:25:25.719527Z","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":"2026-08-11T19:25:25.722850Z","title":"C., Rosenthal, L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.722850Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:1960bd59fb883cf858b929c904d117198a33e1ed92b39fd27c28afa3d24b8101","observation_id":"ee237a25-c4f0-424a-bfae-aa3043dad3e4","resolution":{"observed_at":"2026-08-11T19:25:25.722850Z","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":"2026-08-11T19:25:25.726102Z","title":"M., Cooper, O","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.726102Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:f1df1db3792a3cb77ccc6e522b145e386a08c8fdd8793af70224748a069972f1","observation_id":"dbb03a17-84be-40c1-8330-8dc92df687d2","resolution":{"observed_at":"2026-08-11T19:25:25.726102Z","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":"2026-08-11T19:25:25.729786Z","title":"M., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.729786Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:0ff4f79dd05b36556290fa5505f8c05fc950bd4b4a22b53d3880f50db5954526","observation_id":"7e9f2563-57f9-4b33-9e2e-84e3c4d7d8ef","resolution":{"observed_at":"2026-08-11T19:25:25.729786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.08346","last_updated":"2024-08-15T18:00:00Z","snapshot_observed_at":"2026-08-12T23:03:00.593580Z","submitted_at":"2024-08-15T18:00:00Z","title":"SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.08346","snapshot_observed_at":"2026-08-11T19:25:25.733399Z","title":"M., Long, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.733399Z"},"links":{"cited_paper":"/paper/2408.08346","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:05a3c0ccd3a79101e2c17334d8e6f0df0815a17f76e4a39a95343518a500206e","observation_id":"574198c7-0f3a-43d9-9ed2-bd1d95be4d82","resolution":{"observed_at":"2026-08-11T19:25:25.733399Z","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":"2026-08-11T19:25:25.737186Z","title":"P., Waters, B., Schiebel, D., Young, W., & Golap, K","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.737186Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:542eed468f1a974f95933905bdf7586e745d02c2665dce4a32e8985cc559a844","observation_id":"78a4eb95-33e2-449c-92ec-0f2ab46fd81b","resolution":{"observed_at":"2026-08-11T19:25:25.737186Z","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":"2026-08-11T19:25:25.740622Z","title":"2017, ApJ, 838, 29, doi: 10.3847/1538-4357/aa6259","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.740622Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:a7c554a38f9397e5dd34b2a3c3dd4d04fe3d46467b1cc2c7a8940c22eb6a20fe","observation_id":"2acca7a5-30b1-4a50-879e-3e92adebe7c0","resolution":{"observed_at":"2026-08-11T19:25:25.740622Z","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":"2026-08-11T19:25:25.743869Z","title":"R., Heckman, T","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.743869Z"},"links":{"citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:68eb5d350e9ae2bf13bd5eef7f936c59d8a14caf3c73e9402786734d94530132","observation_id":"61abba5d-3ab7-4af4-ba1c-184f89649bcf","resolution":{"observed_at":"2026-08-11T19:25:25.743869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.16857","last_updated":"2023-11-28T15:05:15Z","snapshot_observed_at":"2026-07-06T16:53:51.485946Z","submitted_at":"2023-11-28T15:05:15Z","title":"SERENADE II: An ALMA Multi-Band Dust-Continuum Analysis of 28 Galaxies at $5<z<8$ and the Physical Origin of the Dust Temperature Evolution","version":1},"cited_work":{"arxiv_id":"2311.16857","doi":"10.48550/arxiv.2311.16857","metadata_source":"pith","pith_arxiv_id":"2311.16857","snapshot_observed_at":"2026-08-12T00:16:22.474752Z","title":"SERENADE II: An ALMA Multi-Band Dust-Continuum Analysis of 28 Galaxies at $5<z<8$ and the Physical Origin of the Dust Temperature Evolution","venue":"astro-ph.GA","work_id":"67f9bbb6-2fbc-4210-b5ad-383d8ee3c64f","year":2023},"citing_paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-11T19:25:25.747329Z"},"links":{"cited_paper":"/paper/2311.16857","citing_paper":"/paper/2412.06894"},"observation_digest":"sha256:315ee2c658ac71426b136646302e73b5b0a775352254e09fa06d99eaa1c7668e","observation_id":"1b23c118-896e-4f44-9fae-89a82834648b","resolution":{"observed_at":"2026-08-11T19:25:26.491772Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.06894","last_updated":"2024-12-09T19:00:04Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-11T19:16:09.657118Z","submitted_at":"2024-12-09T19:00:04Z","title":"A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":3,"parse_uncertain":0,"unresolved":93,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":163},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 100 of 163 outbound references and 0 inbound Pith citation observations for arXiv:2412.06894."}