{"as_of":"2026-08-08T14:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:46e123e30b6093fc2e54e56141803f84002a4c9257fa34694e7cb608be19c395","coverage":[{"denominator":98,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":98,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T11:54:41.168646Z","state":"measured"},{"denominator":98,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":98,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+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/2506.01218/citation-record","integrity":"/paper/2506.01218/integrity","json":"/paper/2506.01218/citation-record.json","paper":"/paper/2506.01218"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:29.733474Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:29.733474Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:df6952143f81a5d52d153c5d6181a9aaca1bf0a7ebd59b96f79ede44c44a9fd6","observation_id":"a01478b1-e74d-44be-9dc9-c1968681aab2","resolution":{"observed_at":"2026-08-07T11:54:29.733474Z","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":"2026-08-07T11:54:29.783712Z","title":"M., & Hickox, R","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:29.783712Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:e0c2fb2a70f6c730687a1f2a6c101edd4ef61fd63bae87a1d51deba3c1bb9456","observation_id":"78dffede-9f58-4c5d-ad5a-e86d459e9f55","resolution":{"observed_at":"2026-08-07T11:54:29.783712Z","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":"2026-08-07T11:54:29.902061Z","title":"M., Brandt, W","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:29.902061Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:5001982cc8a40412aa93da0607e8bf511465f20a60f5396108bab003f49349e6","observation_id":"d3509be4-0d3e-42f5-a2a2-603fb80d8990","resolution":{"observed_at":"2026-08-07T11:54:29.902061Z","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":"2026-08-07T11:54:30.017840Z","title":"F., Argudo-Fern´ andez, M., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.017840Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:ffb792818e36c98ecf6808482d977ba411beb28c296236958e93635f47290110","observation_id":"ae152bdf-6a39-473c-b765-99f5035c5923","resolution":{"observed_at":"2026-08-07T11:54:30.017840Z","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":"2026-08-07T11:54:30.132954Z","title":"J., Eisenhardt, P","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.132954Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:ce7a1c39f62d180faf1cbe7472911c4b7677ae699f17d139c84476e001829b5d","observation_id":"4d6dbf78-8458-4936-b7b5-bb0c43a2ec56","resolution":{"observed_at":"2026-08-07T11:54:30.132954Z","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":"2026-08-07T11:54:30.225832Z","title":"J., Walton, D","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.225832Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:19c5ff5a654384e5e960f3e0521f882299cd7a213520549d4eb729adb11543bc","observation_id":"a1bb5a03-0467-40e1-9a60-2646f02bef87","resolution":{"observed_at":"2026-08-07T11:54:30.225832Z","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":"2026-08-07T11:54:30.346588Z","title":"J., Brightman, M., Walton, D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.346588Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:0e4884ac01025a1e8415c59f81f8d3d14fe46932560aa2c8422db60b2026f018","observation_id":"d4c272b9-590f-4a35-97db-f03e168b14d9","resolution":{"observed_at":"2026-08-07T11:54:30.346588Z","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":"2026-08-07T11:54:30.469474Z","title":"J., Bauer, F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.469474Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:2fce57e4ecbf9e2adf69eb5c863e6adfea262127411d86930e223e64828e6229","observation_id":"7c743e68-afdc-4b6a-b918-bea7c4224cd7","resolution":{"observed_at":"2026-08-07T11:54:30.469474Z","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":"2026-08-07T11:54:30.584848Z","title":"F., McIntosh, D","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.584848Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:6346dc8fa8dcdbf9189443090b58ba3b5c5ae12447e9e1675a746588769fc80a","observation_id":"a923f892-68ff-4783-bd8b-610e7b2b259b","resolution":{"observed_at":"2026-08-07T11:54:30.584848Z","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":"2026-08-07T11:54:30.669074Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.669074Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:e66c4ac7f6c43f3013eafcaef9190164bae0b88dcdb328ab497ea0450399b8b6","observation_id":"77405c8b-e9c1-4798-b83a-d617cfc78303","resolution":{"observed_at":"2026-08-07T11:54:30.669074Z","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":"2026-08-07T11:54:30.783238Z","title":"2007, A&A, 472, 443, doi: 10.1051/0004-6361:20077611","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.783238Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:963ba161ec095ecbb48d688308ba8a9a3a9dd256aa44d0ca2d0b2ef797e4da86","observation_id":"2b94587f-c3e0-4f3d-a351-7ad102c4456f","resolution":{"observed_at":"2026-08-07T11:54:30.783238Z","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":"2026-08-07T11:54:30.864878Z","title":"2014, MNRAS, 443, 2077, doi: 10.1093/mnras/stu1248","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.864878Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:49df9310c564981da855ffbf74504eba97bffc744e7c6fe0b71fbfb72a5e5925","observation_id":"80024792-32a1-44f4-90c7-a6d5545fef7f","resolution":{"observed_at":"2026-08-07T11:54:30.864878Z","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":"2026-08-07T11:54:30.922554Z","title":"2019, A&A, 622, A103, doi: 10.1051/0004-6361/201834156","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:30.922554Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:62fcf3fcb45fd51fd9327556b5d6e21625be580d3545accd9af9ab14c4816036","observation_id":"ee87ae87-c0bb-4b22-9580-1c08eaf51096","resolution":{"observed_at":"2026-08-07T11:54:30.922554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/491617","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:45.142276Z","title":"C., et al","venue":null,"work_id":"60a282c1-5628-48c4-9c0d-57030065ac54","year":2005},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.047951Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:1e16737274146cd0dfa205466364dec46f179d6366f9e28bd3305b6c83a57f53","observation_id":"5c25ae13-7c16-4f98-a007-ce2d49e2ee0d","resolution":{"observed_at":"2026-08-07T11:54:45.177067Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:31.139501Z","title":"2003, MNRAS, 344, 1000, doi: 10.1046/j.1365-8711.2003.06897.x","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.139501Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:da22e769081d4590babbaac96d873bb3b64bfd480dac9ebb27bdb6287a7f7608","observation_id":"29507595-0d14-4e7e-b572-80be8df5bfe9","resolution":{"observed_at":"2026-08-07T11:54:31.139501Z","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":"2026-08-07T11:54:31.246648Z","title":"C., et al","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.246648Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:ed5e51eaa6f8db1f47a24ad237fe43040d17d478c434634bb11c7926adcaac17","observation_id":"1abe2788-9184-4bd4-9b50-4330036f7702","resolution":{"observed_at":"2026-08-07T11:54:31.246648Z","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":"2026-08-07T11:54:31.355936Z","title":"2003, PASP, 115, 763, doi: 10.1086/376392","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.355936Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:de12ca076d611c9e269a64681c7c0f394856297c38b534e01422f418900d0d0a","observation_id":"5d06a3b0-92be-4f9b-a307-b19ac47cdc8a","resolution":{"observed_at":"2026-08-07T11:54:31.355936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.05560","last_updated":"2019-01-29T02:52:28Z","snapshot_observed_at":"2026-08-02T14:41:30.671146Z","submitted_at":"2016-12-16T17:14:23Z","title":"The Pan-STARRS1 Surveys","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.05560","snapshot_observed_at":"2026-08-07T11:54:31.432571Z","title":"C., Magnier, E","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.432571Z"},"links":{"cited_paper":"/paper/1612.05560","citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:fb29d25ceda150bfb8cfc58b1a19f2e427de7fd8a1d39bd9f63cd3b7f590b6a6","observation_id":"4e671855-0cec-44a5-80c2-b70877c04c41","resolution":{"observed_at":"2026-08-07T11:54:31.432571Z","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":"2026-08-07T11:54:31.526348Z","title":"M., Wright, E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.526348Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:2b775128b6cd0207e6bd5289e6cbadec7a32ab51eff8c0763c08929e717f7d7f","observation_id":"8f665bca-3133-4f02-b378-e72336782738","resolution":{"observed_at":"2026-08-07T11:54:31.526348Z","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":"2026-08-07T11:54:31.641997Z","title":"P., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.641997Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:64498a64041339c83127dbc5c14b3b4c2eaf82eddff475f2e1e5b41b3ae2a110","observation_id":"2834dfd1-fd22-4a46-b2b0-bf71a01c1d72","resolution":{"observed_at":"2026-08-07T11:54:31.641997Z","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":"2026-08-07T11:54:31.794197Z","title":"J., Blain, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.794197Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:e4ef194958e3ce1ec7352fa4ea2a58fca02fdc392992cb272a407e60d95e3eee","observation_id":"05ded788-2d55-41e7-bde5-b7b3d2cc2b81","resolution":{"observed_at":"2026-08-07T11:54:31.794197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-07T11:54:31.888652Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.888652Z"},"links":{"cited_paper":"/paper/2111.08721","citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:10693171a3ec862fb893208944277c11fd151f435e4cfa6a4db2b2d67ec9f1a6","observation_id":"3e826e86-6866-4cff-b4c6-641919bfb49b","resolution":{"observed_at":"2026-08-07T11:54:31.888652Z","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":"2026-08-07T11:54:31.984288Z","title":"2020, ApJ, 888, 37, doi: 10.3847/1538-4357/ab5b90","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:31.984288Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:fb74a008cf732f59c2f6c4a765c89ca2850f56867039e174946ad5708f17462e","observation_id":"e77d834f-b96a-4075-9bfb-665c669888da","resolution":{"observed_at":"2026-08-07T11:54:31.984288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staa2992","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:44.956898Z","title":"2021b, MNRAS, 501, 269, doi: 10.1093/mnras/staa2992","venue":null,"work_id":"5151caf7-10a0-468e-9917-b5265fc43c82","year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.086150Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:7a2c6ade990375feba852e249c4f129a38bd2dcc459fd015bf53ed3cba772e53","observation_id":"cf7374c5-bc62-4de3-bebf-a0f00774fd8e","resolution":{"observed_at":"2026-08-07T11:54:44.991695Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:32.185350Z","title":"D., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.185350Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:dd16aaf280e183157d2cf3a751ce833db4d87aaffbadb90235929b0bc15a9418","observation_id":"f406a8ef-7324-4b59-bdfa-3390437e1f46","resolution":{"observed_at":"2026-08-07T11:54:32.185350Z","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":"2026-08-07T11:54:32.319210Z","title":"2017, A&A, 604, A67, doi: 10.1051/0004-6361/201731052","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.319210Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:5cfb090460f7624461690ebc73a0cd387d25dde0cdc7ab693e9cf0596a26f341","observation_id":"96f43c13-6b49-4c3b-a507-ce167e394165","resolution":{"observed_at":"2026-08-07T11:54:32.319210Z","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":"2026-08-07T11:54:32.423556Z","title":"A., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.423556Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:c3eb0562e4fd5607a04d65f65f7ab57300683a5986bbab632e9f0c01679133e4","observation_id":"bca9aa2b-68e8-4960-8ff7-1a85703432fa","resolution":{"observed_at":"2026-08-07T11:54:32.423556Z","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":"2026-08-07T11:54:32.542327Z","title":"2013, The Messenger, 154, 32","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.542327Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:fc30058b03d96bba0c0a5e745eb1da7264f6d5bd669b82ebf339e93e2914e911","observation_id":"f4793628-bf03-4cd3-8555-57e2055a6a2c","resolution":{"observed_at":"2026-08-07T11:54:32.542327Z","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":"2026-08-07T11:54:32.658231Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.658231Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:6519de8827824a36a5777efd3639c7981f4bf80875b6a9a82738e853163e5abc","observation_id":"71d4b55d-0265-455f-8f8b-2abd27a85d02","resolution":{"observed_at":"2026-08-07T11:54:32.658231Z","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":"2026-08-07T11:54:32.768953Z","title":"K., & Shu, X","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.768953Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:74965d655e9c1a57198edb62995030db9f9133e8893de6e2313d3e18c1d3f33b","observation_id":"970f7459-3dd5-4c7d-8d9b-75137e774c02","resolution":{"observed_at":"2026-08-07T11:54:32.768953Z","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":"2026-08-07T11:54:32.901075Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:32.901075Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:3b7f0dc23555e88cc44d7243d9b9d642811851648fbf4ec45bc69089317fdffa","observation_id":"4a6b59d3-4e2a-437f-b922-4a5668d3a772","resolution":{"observed_at":"2026-08-07T11:54:32.901075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/aab496","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:44.701984Z","title":"K., Fogasy, J., & Drouart, G","venue":null,"work_id":"37054c41-789a-4775-8d7b-0c76b35b6edb","year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.006629Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:2276712593c44eb72b5ea48ed95bb0e0fed71419d84c29cd425dabff2216dffa","observation_id":"5ca22905-c3d7-4213-b3b6-06c946f88e01","resolution":{"observed_at":"2026-08-07T11:54:44.775959Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:33.117297Z","title":"2016b, ApJL, 822, L32, doi: 10.3847/2041-8205/822/2/L32","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.117297Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:e3cec8ee05b807cf6c13b039db8a6d6d1a886e46305693be37f77ea2795e68ab","observation_id":"3222d102-8ed2-4a01-bd2c-a2f613ad4dff","resolution":{"observed_at":"2026-08-07T11:54:33.117297Z","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":"2026-08-07T11:54:33.195108Z","title":"T., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.195108Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:f3e9dfd9d3b39d1f24a683143ef3db03294312089cf4994d16290a7b40f268b2","observation_id":"f9023d1f-a93f-4cb9-bbb9-cfa40ce86284","resolution":{"observed_at":"2026-08-07T11:54:33.195108Z","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":"2026-08-07T11:54:33.303274Z","title":"A., Magnier, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.303274Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:4b935b14c101fb338b3e319fd5b72999fc6694517b87723c25b43ea2c6f3f872","observation_id":"71ece14a-dba0-4a35-b918-5499d342545c","resolution":{"observed_at":"2026-08-07T11:54:33.303274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/s41467-022-32297-x","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:44.485831Z","title":"2022, Nature Communications, 13, 4574, doi: 10.1038/s41467-022-32297-x","venue":null,"work_id":"27e3a184-fd29-44e7-810c-ce16614d57d3","year":2022},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.400843Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:46641839d974eccf22eebe787b4369e4e9b312599c3fa46fa422436ba2a2a03e","observation_id":"2dfba7db-ad61-4ce6-beb9-d7a3c46b6aaa","resolution":{"observed_at":"2026-08-07T11:54:44.578135Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:33.521350Z","title":"J., Abergel, A., Abreu, A., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.521350Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:6db772bcaeaa93e908ad4d3585e254ced28fe17f6f29d14598118634b5a92153","observation_id":"c793745d-986e-4ee8-8a05-75a17644e1dc","resolution":{"observed_at":"2026-08-07T11:54:33.521350Z","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":"2026-08-07T11:54:33.616343Z","title":"Z., Bai, J.-M., & Han, Z","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.616343Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:8f68d2ccae30f99183c4b5991c4a62cb4ea35ee0cd925c18413e885800e45e9b","observation_id":"f492a9a7-06c0-4bdd-a7d7-e6cf3d6c6efb","resolution":{"observed_at":"2026-08-07T11:54:33.616343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/749/2/123","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:44.246049Z","title":"2012, ApJ, 749, 123, doi: 10.1088/0004-637X/749/2/123 —","venue":null,"work_id":"df175ee1-03c0-4cb3-834b-cc720af3d1f2","year":2012},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.720031Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:c26c402eedae154662b182eda0abfa18b9a1762ea1bf09bb8a04e5a521867f4f","observation_id":"5dad90df-bacf-4133-98a6-a78092e5c4e4","resolution":{"observed_at":"2026-08-07T11:54:44.335654Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:33.810555Z","title":"C., & Alexander, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.810555Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:152c7144a464a4b054eeeb50b566a082c43922d782f75dc767d7f3eb138b59ad","observation_id":"d19beb89-9d0a-4e98-8290-0eb774ac895b","resolution":{"observed_at":"2026-08-07T11:54:33.810555Z","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":"2026-08-07T11:54:33.914028Z","title":"F., Hernquist, L., Cox, T","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:33.914028Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:7a124274d31578c0eac9b7ff019ca395f2d74fb4235c912fc8811c1036825555","observation_id":"5e2bbcaa-1904-47a3-b6f9-14325802a281","resolution":{"observed_at":"2026-08-07T11:54:33.914028Z","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":"2026-08-07T11:54:34.034043Z","title":"2015, ApJ, 803, 57, doi: 10.1088/0004-637X/803/2/57","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.034043Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:17d35c987f96d748a59baf370424bb3301e47bd37467dbe83e4831ba4ec7c09c","observation_id":"761ff40d-3b95-4f68-af6a-af3b8a0484c1","resolution":{"observed_at":"2026-08-07T11:54:34.034043Z","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":"2026-08-07T11:54:34.171659Z","title":"2009, ApJL, 706, L215, doi: 10.1088/0004-637X/706/2/L215","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.171659Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:28f7e7069792990497423000da06357925450ca7afeb90c7e7716385cd9bd659","observation_id":"1ad15a27-0be2-4cc7-9d9f-1b1e08de1f4a","resolution":{"observed_at":"2026-08-07T11:54:34.171659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stu1157","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:43.919486Z","title":"F., Blain, A","venue":null,"work_id":"32fb0df8-8686-478e-a071-77cb93f63700","year":2014},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.301418Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:c019ca8debbe20ffb452b9b53a68c245036002ffb055d226c93f7ab94abbbb22","observation_id":"06952af1-56e7-40e1-bce2-c93ef1d5e4f1","resolution":{"observed_at":"2026-08-07T11:54:44.044325Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:34.416013Z","title":"D., Assef, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.416013Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:e54090ac54219e3752fa31476f8f508ac9dcb30892a16d1898b69dc943589017","observation_id":"6f663b6f-a822-4190-99ea-f4a2be3a3d21","resolution":{"observed_at":"2026-08-07T11:54:34.416013Z","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":"2026-08-07T11:54:34.509114Z","title":"M., Dunkley, J., et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.509114Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:7c9fd6fbf1a092d070413729cc96213eccf879ecd14e0232651711b5aae7c6e8","observation_id":"706beb5a-8632-4016-9d5f-2744e8aebfbf","resolution":{"observed_at":"2026-08-07T11:54:34.509114Z","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":"2026-08-07T11:54:34.629878Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.629878Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:1f84e55dac8884b043d1a02dbbc1ff402f23116d2a4161abb643ee67c46401da","observation_id":"75b323ca-3d45-479d-b866-77049e0460be","resolution":{"observed_at":"2026-08-07T11:54:34.629878Z","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":"2026-08-07T11:54:34.732995Z","title":"J., Almaini, O., et al","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.732995Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:46ccaa19b795cbdb9bb579ee817926d0041007b463b89e3db471a641a9ca5838","observation_id":"d4dc5cf4-831b-440f-94c3-dcd79fe6a1c5","resolution":{"observed_at":"2026-08-07T11:54:34.732995Z","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":"2026-08-07T11:54:34.872637Z","title":"2023a, ApJ, 958, 162, doi: 10.3847/1538-4357/ace25b","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.872637Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:54bab7511b092d12f4500833ad6ff57e36b1955e403a2e05ddae851354589581","observation_id":"6cac2fc4-ef2f-4507-aa4a-d37c79319091","resolution":{"observed_at":"2026-08-07T11:54:34.872637Z","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":"2026-08-07T11:54:34.997390Z","title":"J., Tsai, C.-W., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:34.997390Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:bee002b146fd19859fe857e6919592fe3fd1ef4d9ce6b8817495fccce5b09714","observation_id":"ffc2b263-13e4-48ac-9c80-48343f023d65","resolution":{"observed_at":"2026-08-07T11:54:34.997390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.05813","last_updated":"2025-03-04T05:18:04Z","snapshot_observed_at":"2026-07-06T20:33:29.458482Z","submitted_at":"2025-02-09T08:37:45Z","title":"Searching for Low-Redshift Hot Dust-Obscured Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.05813","snapshot_observed_at":"2026-08-07T11:54:35.105258Z","title":"2025, arXiv e-prints, arXiv:2502.05813, doi: 10.48550/arXiv.2502.05813","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.105258Z"},"links":{"cited_paper":"/paper/2502.05813","citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:3c57d1ea574aa66ae102bcd7fd6a95098b84cf61847fe34c36646d4d6ec3d5e3","observation_id":"3bfc1bae-d63e-47a1-b7e5-705e3121f9d7","resolution":{"observed_at":"2026-08-07T11:54:35.105258Z","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":"2026-08-07T11:54:35.198326Z","title":"2024b, ApJ, 961, 19, doi: 10.3847/1538-4357/ad0e0d","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.198326Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:cd9385cf20811b56ace9c260384d2312a4b28666d4e0f0e56aa10c0c56078efd","observation_id":"4a5024f1-ceac-434b-aaf2-8b3b81515d63","resolution":{"observed_at":"2026-08-07T11:54:35.198326Z","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":"2026-08-07T11:54:35.296722Z","title":"D., Ding, X., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.296722Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:ebeb5f8b193939614dec9365d30c1ff75400401278f10e7d2e2fea07abd928df","observation_id":"882692af-947b-4642-ab80-3bc70c9fe5f6","resolution":{"observed_at":"2026-08-07T11:54:35.296722Z","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":"2026-08-07T11:54:35.413169Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.413169Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:4918d99ec705968e8eab2bebd947116d8cb44d48480b2c280ab7518fa5995be9","observation_id":"41d5441e-0860-415b-8a5c-939c9a6928f8","resolution":{"observed_at":"2026-08-07T11:54:35.413169Z","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":"2026-08-07T11:54:35.512826Z","title":"2024, A&A, 685, A121, doi: 10.1051/0004-6361/202348535","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.512826Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:4a6159d6012d423990d08861bac1b54d5bc1dcd74034db46343ee062f13a31c5","observation_id":"bcafd581-f88b-4a29-a21f-c029c0bb46a7","resolution":{"observed_at":"2026-08-07T11:54:35.512826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac8162","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:43.596431Z","title":"2022, ApJ, 935, 80, doi: 10.3847/1538-4357/ac8162","venue":null,"work_id":"f03ce98c-1037-43c1-a908-62fa82de9491","year":2022},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.677238Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:b98738d89d26c2d02c87e69b9a48b961c076a82c51791b1fbfad9d772b18126a","observation_id":"32029e16-8930-4c05-ba54-548548399f94","resolution":{"observed_at":"2026-08-07T11:54:43.711011Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad65da","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:43.430126Z","title":"2024, ApJ, 972, 51, doi: 10.3847/1538-4357/ad65da","venue":null,"work_id":"d2f9720f-52d1-4ff0-80d6-a09fed268bc1","year":2024},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.813648Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:e8918ca18489312821517e96a419fc9ffb78a2660b0d22f7341fe60f85ca1de2","observation_id":"7179b793-d96d-4c60-a845-b01c59216d7f","resolution":{"observed_at":"2026-08-07T11:54:43.509671Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:35.942015Z","title":"W., Higley, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:35.942015Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:58e85500b032e26d46f18fa4b2f22ce9e9421f8fd6b1f19ecbb8860e203f563d","observation_id":"12e587ce-3c33-435f-9103-300cd5d64b50","resolution":{"observed_at":"2026-08-07T11:54:35.942015Z","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":"2026-08-07T11:54:36.059180Z","title":"1998, AJ, 115, 2285, doi: 10.1086/300353","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.059180Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:73eccb4ebd0e4d11d55799991dcfa66e9879cf81193c903796a448209366fd41","observation_id":"69bee92e-63c2-4477-8670-425815b1e710","resolution":{"observed_at":"2026-08-07T11:54:36.059180Z","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":"2026-08-07T11:54:36.139709Z","title":"G., Banerji, M., Gonzalez, E., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.139709Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:7947cbacca27a58ade29a422357d24ddccb00d8e1a021d6101a33267209e19ea","observation_id":"2b7d3d34-37d0-468e-9a54-6db941bf9022","resolution":{"observed_at":"2026-08-07T11:54:36.139709Z","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":"2026-08-07T11:54:36.316312Z","title":"Y., Soifer, B","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.316312Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:adf044e2f592259e895c6bb0cc35af3575c370e280d26a10f1df6885e406ced2","observation_id":"f8d38726-050e-4e54-a9f5-c2c031cc335f","resolution":{"observed_at":"2026-08-07T11:54:36.316312Z","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":"2026-08-07T11:54:36.465290Z","title":"2010, ApJ, 708, 137, doi: 10.1088/0004-637X/708/1/137","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.465290Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:58293987783f3c64de3dec6cff1470565a6bdf09fc83e0b3fd677e902ff9c08d","observation_id":"20499536-0b19-4fc6-b20b-609a582a274a","resolution":{"observed_at":"2026-08-07T11:54:36.465290Z","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":"2026-08-07T11:54:36.596632Z","title":"2014, A&A, 568, A1, doi: 10.1051/0004-6361/201423853","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.596632Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:4d2960ae6ac0dccecc51646cf68bc4880d2d7690ff3cc6d605f60171c2767da4","observation_id":"2c873c34-00f7-4fd2-9941-d2c9f608ebd0","resolution":{"observed_at":"2026-08-07T11:54:36.596632Z","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":"2026-08-07T11:54:36.733168Z","title":"M., Ivezi´ c,ˇZ., & Elitzur, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.733168Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:867adab5a11ac0db84f9f5818f8ee0de8e8d80a073384e6e8791e316340f6f3b","observation_id":"569b9e20-49dd-4eb0-8f8b-72ad2dce9755","resolution":{"observed_at":"2026-08-07T11:54:36.733168Z","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":"2026-08-07T11:54:36.880488Z","title":"2008b, ApJ, 685, 160, doi: 10.1086/590483","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.880488Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:5281e490381d291f6079ce3eb09921adcf3cebd8629845ec87da2d26777d0a25","observation_id":"27d1f092-ba50-4640-a9a9-6c3d75e4f5b9","resolution":{"observed_at":"2026-08-07T11:54:36.880488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/799/2/164","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:43.112124Z","title":"N., et al","venue":null,"work_id":"2ad992b7-b02e-4f2a-a5e3-329b1e455a46","year":2015},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:36.959715Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:d4c603a2b407dbfa949dabab4c8883f3341326309f4e8396143ac8db8988f659","observation_id":"8814c6fd-ac7e-4fbf-8afc-4833688f9db5","resolution":{"observed_at":"2026-08-07T11:54:43.230291Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201425324","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:42.912055Z","title":"2015, A&A, 574, L9, doi: 10.1051/0004-6361/201425324","venue":null,"work_id":"30f8084a-1970-4419-b011-52f0bd704e25","year":2015},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:37.093773Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:8bd3b224d656749391748a1dd3480cc39670906a74a386558cca64c1cd8b5df8","observation_id":"d88b9c7b-5066-4a6d-9f0f-bbbb22052895","resolution":{"observed_at":"2026-08-07T11:54:42.986792Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:37.234246Z","title":"L., Riedinger, J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:37.234246Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:9b718a3edfca5a2210b2e06391bc2f70097c9512be37ad59b864442de8d2622e","observation_id":"c535f49a-fb1a-49df-8149-75f982ccccd6","resolution":{"observed_at":"2026-08-07T11:54:37.234246Z","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":"2026-08-07T11:54:37.398135Z","title":"2010, A&A, 518, L2, doi: 10.1051/0004-6361/201014535","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:37.398135Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:6b738e9c09872d42ffb637609412ec2146725b598d80e8637dccf653b0f9af03","observation_id":"bf2f9fe5-ea83-4306-a0b0-938f9dbb9b98","resolution":{"observed_at":"2026-08-07T11:54:37.398135Z","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":"2026-08-07T11:54:37.558733Z","title":"E., Maiolino, R., La Franca, F., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:37.558733Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:48b8d03b2b3a34c32bb706ff0f4495b0ab8d27c18714e8ec4d50f0276ce30155","observation_id":"231d2b9a-7cac-4f11-b6f7-299aeaec380e","resolution":{"observed_at":"2026-08-07T11:54:37.558733Z","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":"2026-08-07T11:54:37.677270Z","title":"F., & Finkbeiner, D","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:37.677270Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:b48e34f8cb14037be4f1f0545406abac4811a2d12e15157bfd9b1c6bfaddeba8","observation_id":"b9758e10-0bdc-4a52-b481-65def9ad180c","resolution":{"observed_at":"2026-08-07T11:54:37.677270Z","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":"2026-08-07T11:54:37.840890Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:37.840890Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:2aa0f92b63c17fcfa67806129e77a12ffc9cdf22880570ec1f64b5002df2e655","observation_id":"6be22402-dd90-428b-8d43-66f78a3f0e02","resolution":{"observed_at":"2026-08-07T11:54:37.840890Z","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":"2026-08-07T11:54:37.980268Z","title":"B., Assef, R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:37.980268Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:26213cb9c48073a675b4dd7e48b9a7addde530951f038e833d66a7b06b19a0a8","observation_id":"a25608a0-cfee-4745-bd09-23933101e2e9","resolution":{"observed_at":"2026-08-07T11:54:37.980268Z","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":"2026-08-07T11:54:38.096303Z","title":"A., Lyu, J., Rieke, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:38.096303Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:7163e4e30335d5742d4a0b45444d8aa5ed4544ee15ef5c8126944416d0b68aeb","observation_id":"92d23120-c69a-411b-a7e4-685f45e3ec7a","resolution":{"observed_at":"2026-08-07T11:54:38.096303Z","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":"2026-08-07T11:54:38.235554Z","title":"2020, ApJ, 889, 32, doi: 10.3847/1538-4357/ab5f5f","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:38.235554Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:643166a9822edf2fca235b5ee57fd6c8a5999738d8bd7d6a604da64d3436ed5a","observation_id":"acba1455-663f-466e-b389-01845cd0eae4","resolution":{"observed_at":"2026-08-07T11:54:38.235554Z","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":"2026-08-07T11:54:38.407976Z","title":"2019, ApJ, 872, 168, doi: 10.3847/1538-4357/ab01fb","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:38.407976Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:61689f8bc8022e51e4809a68c3725cc2dc9fa3634b1941e48e80f276b87f772c","observation_id":"2ab048ff-d44b-457c-a535-e534e97a1b2e","resolution":{"observed_at":"2026-08-07T11:54:38.407976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad22e3","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:42.608497Z","title":"2024, ApJ, 964, 95, doi: 10.3847/1538-4357/ad22e3","venue":null,"work_id":"c244a161-1c2d-4bea-b902-13cdf5bc30c3","year":2024},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:38.563325Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:ea3356fb1bac066b8c7821695c3b5e936d3bee5c9e549c2b57b8d82147fe3e1d","observation_id":"0457c6cc-2cba-4672-b207-978c7527bc53","resolution":{"observed_at":"2026-08-07T11:54:42.685310Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-07-20T19:22:20.4779+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-20T19:22:20.4779+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:38.692732Z","title":"H., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:38.692732Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:e89774d3d764e4cf51979bb4a4f6932213b278abd70f882c3c78b72f02ce0960","observation_id":"1292bdc2-64da-439c-803e-2d274718ea48","resolution":{"observed_at":"2026-08-07T11:54:38.692732Z","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":"2026-08-07T11:54:38.796328Z","title":"S., Silverman, J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:38.796328Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:bbce405009aee3197a1edc0a7dbc08407b5c5b9d077610be79bc98a976adceaf","observation_id":"00f4cb4f-e49a-45f0-9c45-e08fa99633bd","resolution":{"observed_at":"2026-08-07T11:54:38.796328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab616d","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:42.312035Z","title":"2020, ApJ, 889, 76, doi: 10.3847/1538-4357/ab616d","venue":null,"work_id":"c3f23594-f228-4a75-952b-f5996d4c4729","year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:38.917882Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:6d4d25fd0fa443e395cb403950cd557a4a75b29789f835526253ed4c1e56fd1b","observation_id":"ce921a40-b3a0-4fe9-a8dc-96c53d1fc94d","resolution":{"observed_at":"2026-08-07T11:54:42.465637Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/520633","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:42.081149Z","title":"A., & Blandford, R","venue":null,"work_id":"755688e9-8ca6-474d-a22e-690db1091da1","year":2007},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:39.043818Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:50e16acbb41aa5bd55f0bde3ba6cc155e88b1b2eb93855408071a3c57604a7f8","observation_id":"f9e0a606-b5af-4f72-b636-a82e748ab323","resolution":{"observed_at":"2026-08-07T11:54:42.182986Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14248","last_updated":"2024-12-18T19:00:02Z","snapshot_observed_at":"2026-07-06T20:09:33.491422Z","submitted_at":"2024-12-18T19:00:02Z","title":"Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.14248","snapshot_observed_at":"2026-08-07T11:54:39.178281Z","title":"2024, arXiv e-prints, arXiv:2412.14248, doi: 10.48550/arXiv.2412.14248","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:39.178281Z"},"links":{"cited_paper":"/paper/2412.14248","citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:0abc3e3a6e1efbab806cbfb33e4b73fa71647ad48aeca9a5c315f0e52e89971b","observation_id":"3fe1a35f-92a2-4b6f-b07c-fded573ea4fb","resolution":{"observed_at":"2026-08-07T11:54:39.178281Z","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":"2026-08-07T11:54:39.276577Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:39.276577Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:ef7b91f87f1b54b0b47d3e64bbd1f12144493418e648678ae600d8c09d599cce","observation_id":"513086b9-030f-4e34-a844-1f47a08db096","resolution":{"observed_at":"2026-08-07T11:54:39.276577Z","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":"2026-08-07T11:54:39.419060Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:39.419060Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:3c759b200463580fa909810a2583b7d2dec5395d1d213e4c8b1e19bb0d85cfa5","observation_id":"dad1154c-2285-4d11-a08b-0597f3f35193","resolution":{"observed_at":"2026-08-07T11:54:39.419060Z","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":"2026-08-07T11:54:39.623038Z","title":"2012, ApJ, 757, 125, doi: 10.1088/0004-637X/757/2/125","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:39.623038Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:74cb67d3768859da7ed37b7d4a278c7520e225b8f70e681a7c24d35cb55e137a","observation_id":"41c21610-87f4-41af-a1a6-e6346b122478","resolution":{"observed_at":"2026-08-07T11:54:39.623038Z","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":"2026-08-07T11:54:39.756178Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:39.756178Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:51cebaa6ffe8f586a2c8ae63ca8942d1a6aec771a6919afa59c24bdf5c126615","observation_id":"4247b8e0-2a67-4136-b238-e5b742122cd9","resolution":{"observed_at":"2026-08-07T11:54:39.756178Z","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":"2026-08-07T11:54:39.896430Z","title":"N., Stern, D., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:39.896430Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:3500990666c04c9f40f6455898e51312a57528ed251ea761d5addc26e89739a0","observation_id":"0406cf6c-4194-4a49-b4ed-488864693a45","resolution":{"observed_at":"2026-08-07T11:54:39.896430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/714/1/699","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:41.777323Z","title":"L., Neri, R., et al","venue":null,"work_id":"5096daa9-fb1e-45ca-86b2-d6f5eaa349e0","year":2010},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.062896Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:745a04e8bb2251f590eded52dbf843e9e0e4d9dcee8a4fb6cf716d907f586888","observation_id":"7c987352-23a0-4b21-b039-23df520fd73d","resolution":{"observed_at":"2026-08-07T11:54:41.912926Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/588804","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:41.605549Z","title":"A., & Blandford, R","venue":null,"work_id":"514f2246-fc9a-4632-a0a9-e18469ceb4f4","year":2008},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.187144Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:fd988aa32e789a6e355ebe9045c00adc453cc8a93d713e9d3662ccbd5c50f022","observation_id":"477d29a2-d92a-41d3-a915-17e61cd8c75e","resolution":{"observed_at":"2026-08-07T11:54:41.672151Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:40.316405Z","title":"2012, ApJ, 756, 96, doi: 10.1088/0004-637X/756/1/96","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.316405Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:ebc8ee67389ae89f2f9d1c01ed6f033fc5871c3035918bb8247c7c231b5fe319","observation_id":"e54d0844-c373-46dd-9f10-b0573f911298","resolution":{"observed_at":"2026-08-07T11:54:40.316405Z","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":"2026-08-07T11:54:40.409564Z","title":"D., Assef, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.409564Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:c0ff1c56c523405eb7640516bb7987cce92f4560cce644ba7efbc99c3a6effea","observation_id":"3c803bc0-e123-4713-bd74-2d07d0adcc86","resolution":{"observed_at":"2026-08-07T11:54:40.409564Z","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":"2026-08-07T11:54:40.521285Z","title":"2022, ApJS, 263, 42, doi: 10.3847/1538-4365/ac9ead","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.521285Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:dfb8cfa0880003abe17ee13e22b2ab7c3808ba33bdb1281144c2f28597f811ad","observation_id":"fe20e143-8cd8-4ca8-bb2e-89c32165009a","resolution":{"observed_at":"2026-08-07T11:54:40.521285Z","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":"2026-08-07T11:54:40.601406Z","title":"2020, MNRAS, 491, 740, doi: 10.1093/mnras/stz3001 14","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.601406Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:1c90ad1edc33cb86732de823eb6cc9989da95584eff97f9b6115dc1837f0af6a","observation_id":"f7cdfd36-98a9-44d9-9cd5-f640890fc446","resolution":{"observed_at":"2026-08-07T11:54:40.601406Z","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":"2026-08-07T11:54:40.718631Z","title":"2025, ApJ, 978, 164, doi: 10.3847/1538-4357/ad9aa3","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.718631Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:24e1201a6f51084533f02e029451cccdd2a8ae1103a5e4107e5fa84b413dd733","observation_id":"8bda7f44-2f6b-4260-8fc9-aedb499e91ab","resolution":{"observed_at":"2026-08-07T11:54:40.718631Z","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":"2026-08-07T11:54:40.843482Z","title":"A., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.843482Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:79c2c79679d1c524ad9e862b3779078a96ebb9ac0de6e957914fca6c7670436d","observation_id":"da0f532a-1ba3-4d01-92bb-01ae6726f8f4","resolution":{"observed_at":"2026-08-07T11:54:40.843482Z","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":"2026-08-07T11:54:40.970770Z","title":"L., Sun, A.-L., Strauss, M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:40.970770Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:c453b3542396445f926be1e9ec34f0c0df58dee16ea8fdc9bc231d5adb239d4b","observation_id":"77fc8ba9-2539-41e5-9fe2-10a37602f1f2","resolution":{"observed_at":"2026-08-07T11:54:40.970770Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202346695","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T11:54:41.319425Z","title":"J., Mazzucchelli, C., et al","venue":null,"work_id":"5ba3f7f3-00d0-43e2-b3f6-372d5caa83eb","year":2023},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:41.064128Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:311384c0a60b7623965bed9986d1f2670569b63f6c8e8d82760d74cd8fb88ca0","observation_id":"6e5fde0a-a451-41e5-9ad6-f00a4673c234","resolution":{"observed_at":"2026-08-07T11:54:41.430361Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-08-07T11:54:41.168646Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:41.168646Z"},"links":{"citing_paper":"/paper/2506.01218"},"observation_digest":"sha256:79d09281d6c65d17b93f132138dfc35522ba7ff1a41b0464a2b36da1eb3f9b2f","observation_id":"8b98be25-7e96-427a-8662-9ee3ea5c0118","resolution":{"observed_at":"2026-08-07T11:54:41.168646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2506.01218","last_updated":"2025-06-01T23:54:37Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-07T11:45:03.858719Z","submitted_at":"2025-06-01T23:54:37Z","title":"The $M_{\\rm BH}-M_\\star$ Relation of the hyperluminous Dust-obscured Quasars up to $z \\sim 4$"},"reference_resolution":{"displayed":98,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":82,"verified_exact":16,"verified_fuzzy":0},"total_outbound_references":98},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 98 of 98 outbound references and 0 inbound Pith citation observations for arXiv:2506.01218."}