{"as_of":"2026-08-07T07:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2e6876f212a2dbe8bbb039949bcedccbe28fefd2be763f2b858d1c3967f58341","coverage":[{"denominator":76,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":76,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T12:23:28.768069Z","state":"measured"},{"denominator":76,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":76,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+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/2509.01674/citation-record","integrity":"/paper/2509.01674/integrity","json":"/paper/2509.01674/citation-record.json","paper":"/paper/2509.01674"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:47.212381Z","title":"B \\'e thermin , Y","venue":null,"work_id":"ec7c5a0b-e703-440c-9454-9137204a32a2","year":2020},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:20.730454Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:26c0ed6db4edd1222caa0aab29299d5956729025b3b899b308d647805daabe2c","observation_id":"da6a330f-e2e9-4e28-866a-517e0145a988","resolution":{"observed_at":"2026-08-05T12:23:47.332763Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:20.810408Z","title":"Schreiber , M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:20.810408Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:88994a7e74dff7dff5591f60b6cc41b48f4ebdcd829167ebb3b89aa6e19db3f2","observation_id":"cb8ce0f3-e05c-4005-9852-c08fd2a34dc5","resolution":{"observed_at":"2026-08-05T12:23:20.810408Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:46.972279Z","title":"Conroy , J","venue":null,"work_id":"99dafa31-4a00-4d7a-a98d-816fb6d19657","year":2009},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:20.898961Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:f179a544db4368eb53285288335a294d3bb523b2e72f2f6687bd5605b0b8afd8","observation_id":"d3ed0351-def4-42c9-b965-be81070ab128","resolution":{"observed_at":"2026-08-05T12:23:47.088386Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:46.807219Z","title":"Conroy and J","venue":null,"work_id":"02728ee3-bb5f-43ed-a5cc-f7f6a02e73e1","year":2010},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.024183Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:fb2568270c83e01bc6c9b868e9e320f4ee1c8633531d3d70cf801d86e58b0384","observation_id":"17aafa34-cf80-43f4-a1b5-573ec32699cc","resolution":{"observed_at":"2026-08-05T12:23:46.878958Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:46.542872Z","title":"Johnson, D","venue":null,"work_id":"80b7adb1-dd71-4212-93d6-6ddab18adab2","year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.157999Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:d831cf20fa2ebe4b32791ea570ea20043cf3bd729d03f74e2e038a96de685629","observation_id":"fded2ed6-e321-41ba-ba3e-99b9fbd0073a","resolution":{"observed_at":"2026-08-05T12:23:46.678171Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:46.332842Z","title":"Le F \\`e vre , M","venue":null,"work_id":"2f29c2e5-2eee-442c-bf4c-5c69aaf3f9ca","year":2020},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.348805Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:10cead8af340404e77166cf1d9b51363b1d53741842751815668a97ee2feffdc","observation_id":"f3d80cca-d8a1-4181-9c7e-49b1f2eab67d","resolution":{"observed_at":"2026-08-05T12:23:46.438218Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:46.160075Z","title":null,"venue":null,"work_id":"81fb2807-1eb0-4a86-8f79-592427e3b0a2","year":2020},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.439146Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:e369a658cf4a4293deb95bfede0a5c0f11446a17b06612a4f126797fe40fbbdd","observation_id":"21e9c6da-3891-477a-bbd4-25bfcc59623e","resolution":{"observed_at":"2026-08-05T12:23:46.237825Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:45.954898Z","title":null,"venue":null,"work_id":"743f0d30-0225-46b7-be69-dd352e208a90","year":2022},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.570210Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:2d7f23aafdc5f69c5e9d9f36f7adc082428df3c9002b0dd2ca5ca52286b391cc","observation_id":"adb185b7-4892-4f63-aadf-b6a9a47853bf","resolution":{"observed_at":"2026-08-05T12:23:46.043037Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:45.790732Z","title":null,"venue":null,"work_id":"15b7e7b6-c44c-467d-af11-38b97ea52de3","year":2021},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.671934Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:ad05c5b99dda99419acff0b6e9604a5a010d0f71de1ed9e4edf0d0902c87c5f8","observation_id":"548cf1a6-59f7-4a69-842b-8842b83a9227","resolution":{"observed_at":"2026-08-05T12:23:45.861791Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.14546","last_updated":"2024-08-26T18:00:28Z","snapshot_observed_at":"2026-08-07T05:09:36.712679Z","submitted_at":"2024-08-26T18:00:28Z","title":"The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5$\\sigma$ Source Catalog and Redshift Distribution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.14546","snapshot_observed_at":"2026-08-05T12:23:21.806074Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.806074Z"},"links":{"cited_paper":"/paper/2408.14546","citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:87827c1df48cafd68cc9bb4fbdcd72eb3e956cdb0849122930c8fee9af436f89","observation_id":"b152911f-8fdb-44a0-9228-e686ead55b26","resolution":{"observed_at":"2026-08-05T12:23:21.806074Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:45.606935Z","title":"Gruppioni , M","venue":null,"work_id":"3b04ccdc-3222-4e48-a0be-cbaf7725b6ff","year":2020},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:21.954284Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:377ce8ff7e66a3ee2a484eafe91fab4ba2b391228fc7bed9ebdd3df7ecf8d8c9","observation_id":"fefee269-bd43-4bb5-b648-cd480ebb933f","resolution":{"observed_at":"2026-08-05T12:23:45.712913Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:45.394461Z","title":"Fudamoto , P","venue":null,"work_id":"77314f3d-b163-4728-bea1-8fd17768083a","year":2020},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.070904Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:166525719dbdebd9234dc77701908a775ffc4b5f3d92d762718a8b075f893936","observation_id":"3163c3da-bb8a-453b-afaa-2d7867286de5","resolution":{"observed_at":"2026-08-05T12:23:45.490672Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:45.033189Z","title":"Fudamoto , P","venue":null,"work_id":"75dd2bf5-13b0-444d-a550-54ca49aec91a","year":2021},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.146594Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:0df9c84296a5ded7c15439582555b430e0de8ca66f4f95af774b883dbfa36007","observation_id":"381e97a0-b5ca-46e6-b42a-e83a81bcd10b","resolution":{"observed_at":"2026-08-05T12:23:45.265442Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:44.725851Z","title":"Talia , A","venue":null,"work_id":"67e17ba5-e5cb-4f28-896c-e42d29ea69c7","year":2021},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.301720Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:e23ec5aa133bd7f467e4fa672bb5c1fdd24353cd2548912ccb19f0a6cd332dc8","observation_id":"58ca0bae-fd33-4bb6-9edd-cf47f56fca3a","resolution":{"observed_at":"2026-08-05T12:23:44.837966Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:44.519422Z","title":"Inami , H","venue":null,"work_id":"284b9119-d4dd-4a08-9560-497884793a6e","year":2022},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.429419Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:6efa534e717f78b73147e8821e88d6b3a2139c3ca760743c77aa2ee25e4d943d","observation_id":"0586ca24-1f50-4f44-852f-68b36dd6bf54","resolution":{"observed_at":"2026-08-05T12:23:44.627917Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:44.237215Z","title":"Gentile , M","venue":null,"work_id":"d53943dc-3731-4798-9f27-b1fc4c9d54d6","year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.519997Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:a363e5be1a154a5ccf91cb2ce14103b18fcc0cc5ace56ce4672bf62030b37326","observation_id":"d7c7857f-7a82-4f21-8f55-b9425d808a80","resolution":{"observed_at":"2026-08-05T12:23:44.396218Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:44.054355Z","title":"Scoville , H","venue":null,"work_id":"5d1a29e0-d24f-4b0d-a248-d792ede37ec6","year":2007},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.653021Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:ab3e7820babea31671be5151b9102e4805a47e3e6e3de154b053f734fb82f6c7","observation_id":"cac3d1f7-e4c0-4045-bef0-0e5aa3dca6bc","resolution":{"observed_at":"2026-08-05T12:23:44.135777Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:43.840632Z","title":null,"venue":null,"work_id":"dfec5cd3-7561-4982-8714-ac455bacc904","year":2009},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.734130Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:dbab8dba19d9ecc68981d5c1913eede810fa76f4f24432bf744cd60cdaa41fa2","observation_id":"18a8befb-4543-479b-af4c-3643fa9e7394","resolution":{"observed_at":"2026-08-05T12:23:43.951231Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:43.586135Z","title":"Franco , D","venue":null,"work_id":"a6666462-b765-49ea-9770-f4a3cd863999","year":2018},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.841752Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:6023a80f8871727e1a8620e8d34968a00f75f216a469132c3fc551e0cd3e482f","observation_id":"59dc6e01-fde6-42b0-916f-643c53ef8ee7","resolution":{"observed_at":"2026-08-05T12:23:43.706178Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:43.386644Z","title":"Wang , C","venue":null,"work_id":"ce1e8a1a-8fae-4322-8353-01347c3a4ccf","year":2019},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:22.963527Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:8e8fee4210cfc80076ed446d57fe74f3be06eba9a99dede568a312ec72823afd","observation_id":"5afe8202-4583-4578-a1d8-b10c79157bc4","resolution":{"observed_at":"2026-08-05T12:23:43.452898Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:43.021380Z","title":"Schreiber , M","venue":null,"work_id":"18d2cf85-1ff4-4f56-b21c-c65b5a285233","year":2017},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:23.032862Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:cdfa94cf9846a70521a3b9b27a5e5f9ee67a3422f75cab3433ea4437ebdea4e5","observation_id":"ec047a17-a2de-4b07-aff5-9674c3375e06","resolution":{"observed_at":"2026-08-05T12:23:43.226274Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:41.781140Z","title":"Schreiber , D","venue":null,"work_id":"a0cb5df1-f72f-4206-9d7e-36f02a7e2de2","year":2018},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:23.126111Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:85b905c5404c2d342dab29916436c47fd82fea69ca5da3a8741649cf5cbd53c4","observation_id":"9fa0b217-470b-4ec3-8ffc-b8dcc4b6a44e","resolution":{"observed_at":"2026-08-05T12:23:42.762340Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:39.533402Z","title":"B \\'e thermin , E","venue":null,"work_id":"bae3bf96-a142-452f-a29c-7252ac4ee082","year":2015},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:23.232409Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:4380f1bf0243e3aa64bdace8c6206b68ee81e748753fcba9df35c038260e8fd5","observation_id":"6b8fe297-5f9f-4c3c-bb4d-00fc0af981df","resolution":{"observed_at":"2026-08-05T12:23:39.974881Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:39.329905Z","title":null,"venue":null,"work_id":"1eb84d8a-d169-44c5-8415-8ce916e51166","year":2017},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:23.394154Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:3e1d7fe8bff5ad6e7075781580b192c3cb200d01e85ef9f58e9119542c60809e","observation_id":"7cce4c31-f02e-44de-885a-0bad8601217e","resolution":{"observed_at":"2026-08-05T12:23:39.380766Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:39.142463Z","title":"Ding , J","venue":null,"work_id":"1207a7d0-281a-42a0-95cf-719313396281","year":2022},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:23.568218Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:c4a345b17a2529650f850c6be23623bc21a06b0e42b769b12e5a77e176185fef","observation_id":"b1fb9d24-a1f8-4bb8-817b-1e6cbd28e9ff","resolution":{"observed_at":"2026-08-05T12:23:39.231966Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:38.884132Z","title":null,"venue":null,"work_id":"b8372d62-1ffe-4496-aebf-1eab855ee711","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:23.766183Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:1de99023969a645351823615143eddd66b925de97f6e6088f7870c41f967f87c","observation_id":"db596adf-8ae8-4ebc-beb6-6f4c41972f1a","resolution":{"observed_at":"2026-08-05T12:23:38.958823Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:23.876035Z","title":"Matthee , R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:23.876035Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:711b2aa9d959b64bbedca7b8d3e9649bc40959497621295b874dab9c251f5083","observation_id":"5b0392c5-92bc-4f0f-a7c1-78ce404bd8ab","resolution":{"observed_at":"2026-08-05T12:23:23.876035Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:38.623232Z","title":"Harikane , Y","venue":null,"work_id":"0e4abf96-ca69-4b22-95f6-5af0a28034f6","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:24.005647Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:23b42c2fbe8e8d63f4c37570b26e3a604b5ccb1300e727cbb236092f30b2f4ac","observation_id":"8477bb21-984e-4127-b5c3-6a870d1f02df","resolution":{"observed_at":"2026-08-05T12:23:38.734801Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10341","last_updated":"2024-06-14T18:00:04Z","snapshot_observed_at":"2026-07-06T18:31:17.512404Z","submitted_at":"2024-06-14T18:00:04Z","title":"COSMOS-Web: The over-abundance and physical nature of \"little red dots\"--Implications for early galaxy and SMBH assembly","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.10341","snapshot_observed_at":"2026-08-05T12:23:24.204896Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:24.204896Z"},"links":{"cited_paper":"/paper/2406.10341","citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:96f856777f5990702578196f39b34d384f0f04562634add8a731ea8c60270acc","observation_id":"7387c8e3-1b89-4859-9bfa-d75efc4ad985","resolution":{"observed_at":"2026-08-05T12:23:24.204896Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:38.323497Z","title":null,"venue":null,"work_id":"436c8bb5-dbf8-46fc-9ead-cda1dc9feb87","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:24.317724Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:cef82b3688fa74d3c85d05148c04c8aae8eb357b55abbdcc0020c784c4f04ec6","observation_id":"8189d1b7-9e46-4b36-9473-7666a11cc101","resolution":{"observed_at":"2026-08-05T12:23:38.489629Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:38.031985Z","title":"Dubois , R","venue":null,"work_id":"f4150ea0-c4f9-4bd4-91a5-22865f690fa9","year":2013},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:24.495544Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:2265e02fc64da9c211742de8f4699bc1ab54d9436b1c9e6c130302efddd0b683","observation_id":"764a1580-b31d-4be7-a71e-95ab1f2dbc26","resolution":{"observed_at":"2026-08-05T12:23:38.163637Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:24.694497Z","title":"Moullet , T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:24.694497Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:f772f3e27ae6e93c39ba52d87fec78f0086642cffd9e0b6dabdb9c80516ba80b","observation_id":"85b50d47-4a5c-4b10-a9ec-4a808fc205a0","resolution":{"observed_at":"2026-08-05T12:23:24.694497Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:37.742564Z","title":null,"venue":null,"work_id":"6f3015fd-4e52-40dc-9f70-b12f340ddce8","year":1974},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:24.876968Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:67182f0cc27f42687ab345ee74f96a33d4825f0458c3f564d6a740a29dca2197","observation_id":"442b8ff5-3afe-43f6-8847-06651c1a3214","resolution":{"observed_at":"2026-08-05T12:23:37.884805Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:37.415565Z","title":"Chabrier , `` Galactic Stellar and Substellar Initial Mass Function ,'' 115 , 763--795 (2003)","venue":null,"work_id":"b00f2ace-0ff7-48fa-b668-f04f694ed606","year":2003},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.017093Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:e126ddee044c3929a75f10a7a47ea8a488208b17cd98c88ca511f7b668715ea3","observation_id":"96819e3a-4b93-4729-b594-7f29ae54f8df","resolution":{"observed_at":"2026-08-05T12:23:37.534068Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:37.241681Z","title":null,"venue":null,"work_id":"b5542027-8c42-47fc-9a5e-4e07056fe745","year":2020},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.199361Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:1402539c13b0e0ab4d42030bb4176083c3d6eff6290daacb3abf3b6a7e3e75ba","observation_id":"92cee26c-7275-4e6e-b038-9b3e6d948679","resolution":{"observed_at":"2026-08-05T12:23:37.317708Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:37.063285Z","title":"Kirkpatrick , A","venue":null,"work_id":"e2a34e22-d62a-48c8-b131-f861e4b2a371","year":2012},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.402995Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:600f0e66e43b3cfb84a0549cdc7c41fc1f975f0c9c6e5beb6b5b54f96b69d673","observation_id":"b2e42481-a690-44e6-b8a3-eb439acf5b45","resolution":{"observed_at":"2026-08-05T12:23:37.157121Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:36.862475Z","title":null,"venue":null,"work_id":"48ff0c89-e4f1-4bcc-9634-55b199b866ab","year":2019},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.580093Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:24836bbea2a001dfef86b77a0924b532c66cb95a9917569dd67ad774b6290d0c","observation_id":"c6f52f0d-3407-46b7-b32c-cd7ac9983861","resolution":{"observed_at":"2026-08-05T12:23:36.931147Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:36.653209Z","title":"Bing , M","venue":null,"work_id":"df0344fe-6f84-4508-ad8e-8e26e6fe6216","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.707413Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:6d95d6375c96880bf6a15dab24d6e1dcb9aab2a93832957cc307600b0f534f67","observation_id":"ac668fe0-171d-4ef6-96a8-2db44cbaac6d","resolution":{"observed_at":"2026-08-05T12:23:36.760853Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:36.433978Z","title":null,"venue":null,"work_id":"91e10228-a4c2-4423-be19-a219034d6c18","year":2018},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.783248Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:830fa964d756582370fdbd9436a0242a35a642b2dd4994773f1e28068b932b58","observation_id":"03de9bbc-4446-4006-9b45-f4620b83fca1","resolution":{"observed_at":"2026-08-05T12:23:36.569068Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:36.249596Z","title":null,"venue":null,"work_id":"74de22ee-e480-42b4-91ae-b1cbcf1ca012","year":2009},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.860252Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:1ce90a616da53ce490c7ee81767cacb4b5b018033046bb146f0e025e9197286e","observation_id":"e4aacff8-2339-41b1-8f34-4a19e022f2bf","resolution":{"observed_at":"2026-08-05T12:23:36.364113Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:36.020506Z","title":"Kirkpatrick , A","venue":null,"work_id":"bb0e5c30-52cc-40ea-a4ec-3e970d4e6ba7","year":2015},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:25.965681Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:a80dbb90bfb165d4caee962cc9d3e16c14185abb6acfee8995480bc4386327fa","observation_id":"a6b4e4d8-3cd1-412c-86b8-000ab0e0d3d0","resolution":{"observed_at":"2026-08-05T12:23:36.129974Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:35.832921Z","title":"Young , A","venue":null,"work_id":"e22b02cd-72f8-47ba-8726-d46221c694b9","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.028126Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:86ad69842ebc1387f363471ec6e1e22b6e8d1f98a2d56e7464b94adb3e6c19f7","observation_id":"8364c19e-b7fc-496e-b17e-b56d7c4f1517","resolution":{"observed_at":"2026-08-05T12:23:35.926182Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:35.669718Z","title":null,"venue":null,"work_id":"c51f6f80-ff93-4dea-a1d3-5c2b7a5b2924","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.128541Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:c766a11a0669ba21692c6ac302cdcb13de98abdb04acac772e6bd50d8b00e19a","observation_id":"dc0e93bb-8ade-49a0-a6b3-7a1aa3282323","resolution":{"observed_at":"2026-08-05T12:23:35.749140Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:35.458279Z","title":null,"venue":null,"work_id":"0639b9d9-06c7-49f7-b574-ec9d8cfb1883","year":2022},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.215022Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:3ecbc2b1276e3e89893c5d918c24c89043df22ad48ccc9428e92569131f0ef84","observation_id":"351377dc-e8dc-4511-b48a-a5dfc265def6","resolution":{"observed_at":"2026-08-05T12:23:35.572068Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:35.264222Z","title":null,"venue":null,"work_id":"361ef2f7-da24-4c13-9afd-9f3b658cbc44","year":1998},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.308450Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:3341c3e4112f26fcf14efe1c328d01a1f023ab64ed71d8a7a3f554318002eeac","observation_id":"a794d463-e2c6-4328-8176-e5f7e4c61ca8","resolution":{"observed_at":"2026-08-05T12:23:35.336704Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:35.044320Z","title":"Khusanova , M","venue":null,"work_id":"c2555d9b-b1ad-4040-a1e3-56fa428df050","year":2021},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.430870Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:b7cabfc4e9a92dc05c57738b0c412c552637de8b872073548dc9c8c1406a7441","observation_id":"4183cac1-812c-40e8-850e-6f90a5aed85c","resolution":{"observed_at":"2026-08-05T12:23:35.131914Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:34.704119Z","title":"Le F \\`e vre , P","venue":null,"work_id":"c52d5134-70f6-4cc1-8cc3-3abceee28be2","year":2013},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.507293Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:128d74782d6d2aac4c71ab6c712e38ce306c9b1f011b3610f089ddf4e2dd342e","observation_id":"994188b2-be28-4cb8-a1ce-5b3c74e40c30","resolution":{"observed_at":"2026-08-05T12:23:34.872849Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:34.353563Z","title":"Hasinger , P","venue":null,"work_id":"95f1d243-11eb-4635-8f3f-203ce109829d","year":2018},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.567022Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:6137f1f28353701c497dcdfa51bbf48aff60dd8a4c72ce732759471ba539044d","observation_id":"dbd581c1-2d7e-4d4e-a3ef-9db4b7278ccf","resolution":{"observed_at":"2026-08-05T12:23:34.516782Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:26.649032Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.649032Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:b4ea485f4f8a7680f5b16029f13f46b97b0fbc36ddffefbafd780a78655808ec","observation_id":"ad233b78-eaa2-4356-b172-e3309a724187","resolution":{"observed_at":"2026-08-05T12:23:26.649032Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:33.999410Z","title":null,"venue":null,"work_id":"5ea359e1-f769-4487-aa75-9932d48c9fb6","year":2007},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.716004Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:8499c41531e82901f489dbb7d6ec639a7872d7e307b6b2fd3157e350e3ed1886","observation_id":"f03f7de6-b9e4-4f9d-a3f6-067e6ac08c09","resolution":{"observed_at":"2026-08-05T12:23:34.134284Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:33.803111Z","title":null,"venue":null,"work_id":"4735ee2a-962c-4639-b70b-1d61cbb55ef0","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.773970Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:db4757a85d499d1a8fd1d3abd88673c67c07bb69321ab02625ea9a47f903a4c0","observation_id":"4f881527-df00-49fa-b62f-cbced2038183","resolution":{"observed_at":"2026-08-05T12:23:33.876392Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:33.491370Z","title":null,"venue":null,"work_id":"16d98341-5a43-403f-badd-d181e3b02159","year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.860371Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:d5cf45f5bf919bef71d6f4dd17b25bf2a5ad895e6e6d7127b3d5c394abd4f66a","observation_id":"b8cafabd-6adc-4549-b106-f77f0a269d7c","resolution":{"observed_at":"2026-08-05T12:23:33.653696Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:33.241200Z","title":null,"venue":null,"work_id":"633500a3-e3ae-492c-85d7-7caaef27a6c5","year":2006},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:26.957650Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:0051f082b18c73f9f7dac2496e0721aaa9f217cba1f338e377394864b990f614","observation_id":"0b39d022-3cb4-4ca6-81ed-9ed051695e3d","resolution":{"observed_at":"2026-08-05T12:23:33.363070Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:27.029184Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.029184Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:803a8fe8b73008a1b55c656005c2cffcbe779a557aadb3f17338082b2620c6aa","observation_id":"b5686d50-9e40-446a-b124-150f55771a3e","resolution":{"observed_at":"2026-08-05T12:23:27.029184Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:32.956772Z","title":null,"venue":null,"work_id":"c6a5fcd5-2373-4486-a146-6766e9b52b38","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.106528Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:bf9db603b12be1d467a0ddb138b27d5d18126cfc255485a99344df3d8a3db8a1","observation_id":"af3abf1e-e691-41d1-a4ec-1949c9bcab47","resolution":{"observed_at":"2026-08-05T12:23:33.106734Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:27.177305Z","title":"Spinoglio , J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.177305Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:00fa8de199fb7f927c2f8352d74cbfb0efcd04b3e79190c31bf2c19f67f6dda9","observation_id":"e1d51ff2-71d3-460c-a1d7-49832557b9d6","resolution":{"observed_at":"2026-08-05T12:23:27.177305Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:32.661206Z","title":"Shen , P","venue":null,"work_id":"2e97a97b-7499-4cfb-8067-d30cb0b9e9c4","year":2020},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.233640Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:0a8d21b92130b8fe2e9fb74b2c2a1d80f20f19a649d7432bf1d69de39ca76c9e","observation_id":"76a47e64-3148-4c02-84e3-777ec4f1c86c","resolution":{"observed_at":"2026-08-05T12:23:32.758256Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:32.444120Z","title":"Lusso , A","venue":null,"work_id":"a27c8bb4-42aa-48c0-8c15-27ccf351a9bd","year":2012},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.322470Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:4843e4daaa74b40d74824443397f0c9650a8e6d9daf2575499d18cf8adc7d005","observation_id":"9fef4a17-0c54-49ec-b593-1dca1b9bda9b","resolution":{"observed_at":"2026-08-05T12:23:32.560628Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:32.252736Z","title":null,"venue":null,"work_id":"d8dff976-6bc2-4ee4-97c4-a31d1162eadc","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.357379Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:b9c1e58bb09ee4b2feaf404cbdd0f62d1cd698cbba52dba941a60c8f466a9d70","observation_id":"c55d6d3f-244f-471e-bcf8-6958e163662f","resolution":{"observed_at":"2026-08-05T12:23:32.316748Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:31.943518Z","title":"Alonso-Herrero , C","venue":null,"work_id":"098c27f5-b45d-4eca-8e18-65d8e22b206a","year":2014},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.452344Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:4ce014c152ff44afa02d04472dacea8a8a478a90d5821972d79b0cdda4194d99","observation_id":"abd00d74-1923-4081-b3bb-e513af8bed8f","resolution":{"observed_at":"2026-08-05T12:23:32.089409Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:31.657406Z","title":"Garc \\' a-Bernete , D","venue":null,"work_id":"4f4f5b27-02c4-4ce1-9f1e-1b85dbbf879e","year":2022},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.514944Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:0028e108399493b72d092817796a1546776e3dc9e1445de165ca0abc709760a1","observation_id":"ce31b95c-3af2-4256-8f1c-06157fcc93f5","resolution":{"observed_at":"2026-08-05T12:23:31.812778Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:31.429654Z","title":"Vignali , E","venue":null,"work_id":"cb3f18b8-e9da-4215-945d-838547eb7ebf","year":2068},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.606833Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:c10060aaaa0661e63fc579eada611feae8b54b327c501ea192d8c45bfb79fd47","observation_id":"d24fc34d-10fc-4f49-babb-5af218c6619f","resolution":{"observed_at":"2026-08-05T12:23:31.518625Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:31.177127Z","title":"Gonz \\'a lez-Mart \\' n , J","venue":null,"work_id":"fdf5640e-b3d0-4f3a-8e02-3e1f19ccb000","year":2013},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.697416Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:e4740e44f20d59eacef699244f11b36be03bcbe2079dd987a630c5a2c45bd4f7","observation_id":"27aaff5c-a837-4ef9-8b91-d12f78fc6171","resolution":{"observed_at":"2026-08-05T12:23:31.341310Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:30.984794Z","title":null,"venue":null,"work_id":"02ae20f9-4556-41dd-8b47-77d228b53b8f","year":2019},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.752617Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:6589e7ba2a18fe693eee909141da96453eda098d69dc663c82e2387f4e26cdf7","observation_id":"2799415c-f6aa-453e-a1d4-db0fad815109","resolution":{"observed_at":"2026-08-05T12:23:31.078985Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:30.666325Z","title":null,"venue":null,"work_id":"43645664-c460-4230-8cd4-aa5886ccee8c","year":2012},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.872360Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:166af944c79f06472813ad99e2c8ee939182bf0e909fd25df4a2dd3e41bf65ee","observation_id":"2960a5a9-9d39-493f-a509-520fc54e5bd5","resolution":{"observed_at":"2026-08-05T12:23:30.787792Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:30.466336Z","title":"McKinney , S","venue":null,"work_id":"1f55c25b-016e-4e51-a00a-6860ac38d30b","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:27.951385Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:a8658068dad462df0172e482ca38a6e70479eb143fa50a4cf52e6aca7ba86115","observation_id":"cdbaebe3-f31c-4854-9da6-185bb41c9c30","resolution":{"observed_at":"2026-08-05T12:23:30.540430Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:28.017253Z","title":"B \\'e thermin , A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.017253Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:3298a9b1bccb2664af97431ba49d9124da5abefcae108281e3a63b7359bec239","observation_id":"5d177cf1-efed-446b-b83c-0577ed980279","resolution":{"observed_at":"2026-08-05T12:23:28.017253Z","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":"2026-08-05T12:23:28.079577Z","title":null,"venue":null,"work_id":null,"year":1966},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.079577Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:a57d7f099d08cda05206dfeca970a003ddb07cb27664fd69000aa5f987fa2228","observation_id":"524c4462-4500-40a5-9b07-fafc558358b6","resolution":{"observed_at":"2026-08-05T12:23:28.079577Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:30.230978Z","title":null,"venue":null,"work_id":"502f6d48-2de6-4510-b65a-99961ad1fed5","year":2022},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.190433Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:fdcdf4d447ea2cbb9b7b70fe39cbdc1d8263a9d3fe84510a47e5eff9b24e4ba1","observation_id":"eaba6af2-a686-44ed-a036-e57154beb05f","resolution":{"observed_at":"2026-08-05T12:23:30.346407Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:29.913182Z","title":null,"venue":null,"work_id":"f836d829-587a-4c3c-a885-095383ee5aff","year":2018},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.279193Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:84adfaa9f02d16cd4fb0ec009ffa7b15d1b557646a6e6e52c7cf65d40149c877","observation_id":"367ad714-082b-41cc-bc91-a832bce9bb3a","resolution":{"observed_at":"2026-08-05T12:23:30.008796Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.08721","last_updated":"2021-11-16T19:00:01Z","snapshot_observed_at":"2026-07-06T12:09:12.802530Z","submitted_at":"2021-11-16T19:00:01Z","title":"Galaxy shapes of Light (GaLight): a 2D modeling of galaxy images","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.08721","snapshot_observed_at":"2026-08-05T12:23:28.356865Z","title":"Ding , S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.356865Z"},"links":{"cited_paper":"/paper/2111.08721","citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:52e99aaab77cf1932bf50398b0415f8591858323cb74f2d08e00e481bbd4d841","observation_id":"e71f2eab-5006-49f2-9296-1277c5f62bc3","resolution":{"observed_at":"2026-08-05T12:23:28.356865Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:29.654762Z","title":"Lang , D","venue":null,"work_id":"c6798ba5-463b-4230-b632-21b976b1d1db","year":2016},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.430566Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:204721887e3a962c0ae925a04ee7c0b543cf0732f4a7f44e92048cae293e97be","observation_id":"11225fd7-857c-4f42-927e-44d8f258a506","resolution":{"observed_at":"2026-08-05T12:23:29.767729Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:29.433143Z","title":null,"venue":null,"work_id":"f0dde881-4162-4d70-b054-5066588d74fb","year":2023},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.516747Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:4019db61e056d3cc2066e36d38db1a372c9675e513fae3199cdb764419a3ad2f","observation_id":"d71fc779-2117-4267-8c39-f94954547127","resolution":{"observed_at":"2026-08-05T12:23:29.546191Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:29.313561Z","title":"Prakash , R","venue":null,"work_id":"a3cd7631-a617-4682-bf1e-10f039fd7544","year":2019},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.593295Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:3c7f5800772cc548f113079a450c88281e08f6e2088fcd371288334572d08f55","observation_id":"11422f36-5a99-40e0-bafa-141ed94e8a0c","resolution":{"observed_at":"2026-08-05T12:23:29.390475Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T12:23:29.109199Z","title":null,"venue":null,"work_id":"10c93be5-9ffe-4d43-bc9d-2a176377588b","year":2019},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.664316Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:639366f5d6bdcc55f925d08b0bf5ea26b76462778952f6daf5aaf2c489afc3bb","observation_id":"24273c9b-0bb7-4ea7-9078-6016a513076b","resolution":{"observed_at":"2026-08-05T12:23:29.204453Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-05T12:23:28.768069Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-05T12:23:28.768069Z"},"links":{"citing_paper":"/paper/2509.01674"},"observation_digest":"sha256:228e4e3d0fb83e263b69ce24d7b4570decd4b65e44ba7735b80f831e0a3931c1","observation_id":"7fec321a-ff90-4b48-9376-b270b53d1e96","resolution":{"observed_at":"2026-08-05T12:23:28.768069Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2509.01674","last_updated":"2025-09-01T18:00:19Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-05T12:23:17.512824Z","submitted_at":"2025-09-01T18:00:19Z","title":"Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA"},"reference_resolution":{"displayed":76,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":39,"verified_exact":0,"verified_fuzzy":37},"total_outbound_references":76},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 76 of 76 outbound references and 0 inbound Pith citation observations for arXiv:2509.01674."}