{"as_of":"2026-08-11T01:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b6791e43b762a736125fb9b5b749c672bef1d1ec42f818bf335f783dc114ba59","coverage":[{"denominator":68,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":68,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-11T03:11:10.401986Z","state":"measured"},{"denominator":69,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":69,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-28T00:23:19.443839Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"cited_work":{"arxiv_id":"2605.07976","doi":"10.48550/arxiv.2605.07976","metadata_source":"pith","pith_arxiv_id":"2605.07976","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","venue":"astro-ph.GA","work_id":"3381fccc-730d-4e42-abd3-b300d3945b93","year":2026},"citing_paper":{"arxiv_id":"2606.06585","last_updated":"2026-06-04T18:00:02Z","snapshot_observed_at":"2026-08-02T11:45:56.898689Z","submitted_at":"2026-06-04T18:00:02Z","title":"A Population of Red Galaxies with Very Strong Emission Lines at $z > 5$ Revealed by the NIRCam Medium Bands: ''Classic'' LRDs, Dusty Star-Forming Galaxies, and a Missing Population of LRDs","version":1},"reference_index":120,"source":"arxiv_source","source_observed_at":"2026-06-28T00:23:19.443839Z"},"links":{"cited_paper":"/paper/2605.07976","citing_paper":"/paper/2606.06585"},"observation_digest":"sha256:f20ab7e6d3ce80a2061a6706aa2aa1a5021f55244f0967956f0743454da8d17a","observation_id":"161a7b93-e3ba-498a-9f15-dde972878e78","resolution":{"observed_at":"2026-06-28T01:41:30.082582Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2605.07976/citation-record","integrity":"/paper/2605.07976/integrity","json":"/paper/2605.07976/citation-record.json","paper":"/paper/2605.07976"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"B., Casey, C","venue":null,"work_id":"fdcb5290-1900-4f5c-86b5-8c01e1d8d44f","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:8bafe576e02ba2f032a1534cfcbd367e3e562fd591f0d901fc9396f9e3f50d3c","observation_id":"ac29994d-4e99-4608-8ad2-74c7de3b376c","resolution":{"observed_at":"2026-05-14T10:54:13.628774Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2601.10573","last_updated":"2026-05-10T12:00:37Z","snapshot_observed_at":"2026-08-02T23:58:02.305689Z","submitted_at":"2026-01-15T16:40:03Z","title":"Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN","version":3},"cited_work":{"arxiv_id":"2601.10573","doi":"10.48550/arxiv.2601.10573","metadata_source":"pith","pith_arxiv_id":"2601.10573","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN","venue":"astro-ph.GA","work_id":"17119633-e3c8-4915-a6cc-48f7a07e8901","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2601.10573","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:6791954be46f28d3aeb0d51e64d1878765a489f626905b817f934307ba36b4a1","observation_id":"d8468d69-c21f-405b-94a8-afc7e9f250a9","resolution":{"observed_at":"2026-05-12T02:44:56.814185Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:42.925567+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:42.925567+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2602.02702","last_updated":"2026-05-12T16:24:20Z","snapshot_observed_at":"2026-08-10T11:30:34.020180Z","submitted_at":"2026-02-02T19:13:11Z","title":"Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation","version":4},"cited_work":{"arxiv_id":"2602.02702","doi":"10.48550/arxiv.2602.02702","metadata_source":"pith","pith_arxiv_id":"2602.02702","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation","venue":"astro-ph.GA","work_id":"2f526279-62b2-445f-a0b9-b976b21be991","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2602.02702","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:7b57be61624aa477921517e85ae63e5a453d924e5dd523f7fe1c69be9c2679ea","observation_id":"f1a1f491-d36f-404d-8a28-cdd853e6d3aa","resolution":{"observed_at":"2026-05-12T02:44:58.033141Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"9a5483d5-4d0e-4059-b914-754c4a2b6dfa","year":2023},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:23c1ec3baa61a7fd99d8557794e02367ea11c6bb11cf8be3e59fb08ffb7ce07c","observation_id":"800a9f92-e0e8-4d3d-a9d1-43118ce3d734","resolution":{"observed_at":"2026-05-14T10:54:13.627122Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-05T03:10:38.379569Z","title":null,"venue":null,"work_id":"dbcc924f-9238-4194-90f4-913853ac58fe","year":1977},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:9aabde98321f008296339691bdcfcf4d964026a871485fd90268d06d7edd8898","observation_id":"0a351b7b-4018-416e-a5c9-1463c6775db1","resolution":{"observed_at":"2026-05-14T10:54:13.622380Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.15853","doi":"10.48550/arxiv.2512.15853","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"G., Kocevski, D., et al","venue":null,"work_id":"4e2effdc-0d2f-46c5-8e37-bbfea900b465","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:e5d9dc79d68e207cad4714901d42da7e6f200d076b77601affca865c4e9ceb6f","observation_id":"8e641f4a-3b81-4089-a18d-eae42cc60269","resolution":{"observed_at":"2026-05-11T03:15:55.112530Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-05-22T21:56:48.666962+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-22T21:56:48.666962+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/2041-8205/763/1/l6","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"G., Kocevski, D","venue":"The Astrophysical Journal","work_id":"f1c0f277-90af-4ca4-80bb-d316f0d785b0","year":2013},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:33ae7e262a427bb10f35e68acfc2e7b86f50d3615eea30c0967d34ac29308e19","observation_id":"21c4656d-d62e-41e6-9a00-f407a4b4945e","resolution":{"observed_at":"2026-05-14T10:54:13.638209Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2026, A&A, 706, A29","venue":null,"work_id":"68f0567c-3cbf-4829-8368-b6b083bf9c35","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:2e444f0f52aa0d3e4e67540e4d58bbb354b15ad796a6498481411f7873383489","observation_id":"9404a124-f2cd-4850-8e37-8a582a8d22c1","resolution":{"observed_at":"2026-05-14T10:54:13.646502Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"& Valentino, F","venue":null,"work_id":"a78a9aeb-c0b5-4f6f-9c9f-c323c002fdb8","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:1d17cc22e7ad6d60f0ac0193fcec7e9555dec54bbc3c8a6e1597f381f2555bab","observation_id":"a913bdfb-87f5-4b06-b918-73029c61b333","resolution":{"observed_at":"2026-05-14T10:54:13.630429Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T02:25:56.081929Z","title":"C., et al","venue":null,"work_id":"682f8dbb-729b-43a4-9f3b-79a5e2a7ad2b","year":2000},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:772bc5966533651be63529e24e6dfe5974ba84415d4560180a075c4ae09569ce","observation_id":"03e93302-2d93-460c-ae24-6eb24e90dd3c","resolution":{"observed_at":"2026-05-14T10:54:13.620924Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T02:25:56.649922Z","title":"C., McLure, R","venue":null,"work_id":"3ed3125a-894c-4438-ab34-e8863421c520","year":2018},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:eb3536289a14ef78d10ad327905eb6b9e74602761859d0ec82c2105577354502","observation_id":"4326e932-6dd2-47c5-82cc-c34204361338","resolution":{"observed_at":"2026-05-14T10:54:13.619477Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T04:33:20.429933Z","title":"M., Akins, H","venue":null,"work_id":"4640cfb4-aa4f-470e-ab50-f34aaf15f72c","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a80e9b2615cfa57d480a5facb971b35462badd07cb90ed3511f4f1a431f46b5a","observation_id":"77b12694-8b81-4b94-a050-31ea60566263","resolution":{"observed_at":"2026-05-14T10:54:13.639812Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"M., Akins, H","venue":null,"work_id":"a09988b6-2029-468e-92a5-71654ec91e68","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:80e21bf098de6ff9e0fb5dcadfd95fd0afc03c2968794a05178076dadcb52d2e","observation_id":"7f20bd90-582a-4213-844e-499e4b715207","resolution":{"observed_at":"2026-05-14T10:54:13.644970Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T17:07:25.977230Z","title":"2003, PASP, 115, 763","venue":null,"work_id":"4220c305-df50-4441-9f74-0df268840ca9","year":2003},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:d238b6b7a9342e07e2c9ccedec5a3360c8ce2589386b542176ba3420e83f6ead","observation_id":"1d14da8f-e77a-4387-bd39-a588af950426","resolution":{"observed_at":"2026-05-14T10:54:13.617966Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2603.24700","doi":"10.48550/arxiv.2603.24700","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"P., Whitaker, K","venue":null,"work_id":"c613a0f8-7e8b-4f24-a6eb-c6d4d69e0f8c","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:7c9d13610509bde3597a05efa87a8bd177dbe8785a610c76f2a05a940729e1dc","observation_id":"65ffcde6-8b1c-4a3e-8f55-d10228b9a531","resolution":{"observed_at":"2026-05-11T03:15:55.046781Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-20T15:22:44.996428+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-20T15:22:44.996428+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T17:07:25.849812Z","title":"J., Chatzikos, M., Guzmán, F., et al","venue":null,"work_id":"bfee9702-fbd0-42ec-9b67-6ca40473f58b","year":2017},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:b4ccfe8a59103388ac4431bbd4fcfc1ac07b2beecd285dbdba7c384f82033725","observation_id":"8d8baedc-83a5-473b-a65f-4b369b1f79de","resolution":{"observed_at":"2026-05-14T10:54:13.643375Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2024, A&A, 684, A207","venue":null,"work_id":"a5cb9b20-5671-4a1b-aa42-ad4a7fc342cc","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:ad512860196845f990e1a2dee92d72eacd2fcf17118cfc6f763c176b35b7a83e","observation_id":"2d9ed624-d8c1-4815-bea4-5a32583151c9","resolution":{"observed_at":"2026-05-14T10:54:13.641685Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J., Secunda, A","venue":null,"work_id":"39e29872-bd6d-423e-9b09-5711c88a008d","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:48cfc4d3f1a87ee7b8f75e1b70d302c6d9c6064cecdca4df2f6603670c276312","observation_id":"b7813b6c-6469-4c11-8c87-178974be791b","resolution":{"observed_at":"2026-05-14T10:54:13.648004Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"D., Clayton, G","venue":null,"work_id":"428c1640-629f-4742-b644-ddd56dd50846","year":2003},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:4c151ef167370bd115bae2578ccf6b41fb4d26ef622bee229f43f923e37892e8","observation_id":"c30b990f-dddd-4db3-ae88-afcd0b808e10","resolution":{"observed_at":"2026-05-14T10:54:13.625427Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"c4174306-4e24-4b2f-9e05-af072820f8ef","year":2005},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:d629908b7a52a67af6a1894450bd8b2b72ad735f0dd0aa7c207afd257dc86d0e","observation_id":"1efb6051-e5d6-492c-90de-ce053ef05909","resolution":{"observed_at":"2026-05-14T10:54:13.636729Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-06T22:42:59.273543Z","title":"E., Labbe, I., Goulding, A","venue":null,"work_id":"54ba0224-55b5-4854-97ff-2f0f267bd3bc","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:dda92a64166317e98908df4084d8b8bc79e44baf043693cf7ed6da80a9d8eb2c","observation_id":"490da211-150c-4ad5-8289-834bde987e4a","resolution":{"observed_at":"2026-05-14T10:54:13.635216Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"A., Pacucci, F., & Kocevski, D","venue":null,"work_id":"6646ec4f-d2a4-4867-8ca4-bbe4b8db9860","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a13922ac13e94b2a66a105e0d0c215d80485ea28ff16075996b4fcd06e6bfd2d","observation_id":"52925120-cd64-440d-92f4-45f08c17ca68","resolution":{"observed_at":"2026-05-14T10:54:13.631907Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T04:33:20.191878Z","title":"E., de Graaff, A., Miller, T","venue":null,"work_id":"8627cf33-a7bb-44e8-92bf-e8e7097248a5","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:69f9c728941234fc8ea06821a2ac4c4173952ecd8dfc7d63cebac0c6e080a554","observation_id":"d6de1353-f31a-45b0-bc1f-d4dee8b60d70","resolution":{"observed_at":"2026-05-14T10:54:13.633559Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2025, ApJ, 988, L22","venue":null,"work_id":"e0c3185f-44bf-4032-b58a-c490a6bb68fc","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:3a4c511456d0a6f0738ee2243a21828ba742c39fedefd182c90b1e87ec5382f9","observation_id":"61020cbd-8b3c-42bc-aa46-f33ecd9331a0","resolution":{"observed_at":"2026-05-14T10:59:15.430216Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T02:25:56.125853Z","title":"& Maiolino, R","venue":null,"work_id":"b249d63e-de4d-4a7b-ae6b-2ca7f33127da","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:506b035f500dd2d01e8265fee168e43af241eea961065b631e1048eebfd16b19","observation_id":"bd175d8e-8a8d-4574-b6a6-b7423115f581","resolution":{"observed_at":"2026-05-14T10:59:15.468451Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2026, ApJ, 1000, 90","venue":null,"work_id":"1eed3e75-9b87-4ae9-86e3-14dd468a7a15","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:4116ed957beffdebaabcdd572c5fbe61dc4701f89e5b4e70ba5ec9708ca8c7c0","observation_id":"6c6dfb14-3e64-41e6-8a2f-ed078b88a2f3","resolution":{"observed_at":"2026-05-14T10:54:13.623832Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.05322","last_updated":"2026-04-28T06:55:15Z","snapshot_observed_at":"2026-07-06T21:20:55.836867Z","submitted_at":"2025-05-08T15:08:46Z","title":"The Emergence of Little Red Dots from Binary Massive Black Holes","version":2},"cited_work":{"arxiv_id":"2505.05322","doi":"10.48550/arxiv.2505.05322","metadata_source":"pith","pith_arxiv_id":"2505.05322","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"The Emergence of Little Red Dots from Binary Massive Black Holes","venue":"astro-ph.HE","work_id":"c6051a03-49ad-466b-8e1b-9f54b0660dca","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2505.05322","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:998b966482d7ea51283eb3bdf203cfef5a5641c9afee860d96c4702668f2129b","observation_id":"f972b9ad-78ea-461d-8300-4f7b08b66948","resolution":{"observed_at":"2026-05-11T03:15:55.042179Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-05-22T21:52:44.97136+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-22T21:52:44.97136+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T05:13:21.761442Z","title":"2022, A&A, 661, A80","venue":null,"work_id":"67efa4c2-f7ae-4958-b0a9-551e3a39bd98","year":2022},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:9f564a9133663681ffbea89346373548ce5b60856f67d2960abd6fe51efeaebd","observation_id":"6d320a91-22b0-463f-8c04-6e8a110d7815","resolution":{"observed_at":"2026-05-14T10:59:15.466694Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2026, MNRAS, 545, staf2235","venue":null,"work_id":"7fa5ee5a-fc08-4771-a277-eae0ef19539d","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a483a24b6d5dbb1bc7b9861ee19c1e927f1eb53f2c0976803d7c80a6b00d30e4","observation_id":"25e65925-52d4-4318-b2e1-6b85d8c5e9ab","resolution":{"observed_at":"2026-05-14T10:59:15.455558Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2025, MNRAS, 544","venue":null,"work_id":"ef71d8c8-ec18-44a6-958f-6d8e49ac6b62","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:3d45fdfb875bbb87a9cd745fea6785a0b4c98eb84950c6d4e6fd6a32139b27ff","observation_id":"32248349-18ec-4b97-be14-f7b5e2dd9134","resolution":{"observed_at":"2026-05-14T10:59:15.459305Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2508.21748","last_updated":"2025-09-01T10:05:21Z","snapshot_observed_at":"2026-08-05T14:08:46.913088Z","submitted_at":"2025-08-29T16:20:50Z","title":"A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization","version":2},"cited_work":{"arxiv_id":"2508.21748","doi":"10.48550/arxiv.2508.21748","metadata_source":"pith","pith_arxiv_id":"2508.21748","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"arXiv e-prints , keywords =","venue":"astro-ph.GA","work_id":"acd32913-a25f-473c-ab82-6608f54b5c6a","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2508.21748","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:c7ae6e4d8c8d88b1a460bce3fd76a0cec6629b2a2183e1e8e0d8c3690f1ca1d8","observation_id":"f693dcfa-2eff-45ba-8329-2be55a884cb9","resolution":{"observed_at":"2026-06-01T02:02:17.864017Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-05-24T15:24:49.478236+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T15:24:49.478236+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T05:23:21.675122Z","title":null,"venue":null,"work_id":"d08f8702-ce26-4fce-bf49-fbb7de92e4c2","year":1998},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:b5c4f61ebbd8393c58199d4b940619c2bd312ade76af677d307a5ed4a4eca107","observation_id":"89d1e9a4-d5e9-46e2-a038-fdfc2a9d25d5","resolution":{"observed_at":"2026-05-14T10:59:15.438976Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"eecaf26f-f0e2-473a-9f28-a9ac4780b593","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:e1503aa15189271badb07d900109691a32381e61f6ac3d666b41d5f1e3425dcc","observation_id":"cd96beee-c11c-40c3-97b6-b16e0c9e144f","resolution":{"observed_at":"2026-05-14T10:59:15.451480Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T02:25:56.112206Z","title":"D., Finkelstein, S","venue":null,"work_id":"f58b36e0-6efe-49a0-aaa9-3a39cfec419d","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:2301d4e77db9979a2d8c3b8b8961373ce609223aa20b1496e2c788a4d7652812","observation_id":"6fafad7d-379b-4a72-8407-8abf833d53eb","resolution":{"observed_at":"2026-05-14T10:54:13.662135Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"& Harikane, Y","venue":null,"work_id":"ab41b442-95b7-4edf-9168-7b014b98ce81","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:43f4aa089232a99ebb77bb95def5285473b68ba8760ca86e5a57194c65f5c1be","observation_id":"b589eb7b-8a86-41b8-a33b-5e464f237344","resolution":{"observed_at":"2026-05-14T10:59:15.447461Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2604.08687","last_updated":"2026-04-09T18:20:33Z","snapshot_observed_at":"2026-07-06T22:57:45.084987Z","submitted_at":"2026-04-09T18:20:33Z","title":"GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy","version":1},"cited_work":{"arxiv_id":"2604.08687","doi":"10.48550/arxiv.2604.08687","metadata_source":"pith","pith_arxiv_id":"2604.08687","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy","venue":"astro-ph.GA","work_id":"cc63428e-f167-476d-8e88-0956405a459b","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2604.08687","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:d96042f3f5e1bd8b526ae072d9b04d6bb71340a108f9866e0352e5231f3c03ca","observation_id":"42f19a4b-a052-432d-ab63-ab1609882a63","resolution":{"observed_at":"2026-05-11T03:15:55.118062Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T02:25:56.146374Z","title":"E., Bezanson, R., et al","venue":null,"work_id":"93a81c9d-bd97-42dc-bf00-8314c9f312c9","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:45ee4fbccfb448d31015d4625aa933fd637cbe3c8b95f6fde04893d3604d2414","observation_id":"8707d830-1b04-4c19-9390-e99c996cc557","resolution":{"observed_at":"2026-05-14T10:54:13.663565Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.04557","last_updated":"2024-12-05T19:00:30Z","snapshot_observed_at":"2026-08-06T08:42:37.843324Z","submitted_at":"2024-12-05T19:00:30Z","title":"An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy","version":1},"cited_work":{"arxiv_id":"2412.04557","doi":"10.48550/arxiv.2412.04557","metadata_source":"pith","pith_arxiv_id":"2412.04557","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., Matthee, J., et al","venue":"astro-ph.GA","work_id":"e9acc8dd-fa6a-4867-818b-fa914c8c77d1","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2412.04557","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:ed745cfeb8161eb04752d88e298c469832a419c29303d39c5f423406b5e78c4e","observation_id":"dbc2ae48-aba8-4e93-9cbd-f5d4b6e46ab8","resolution":{"observed_at":"2026-05-11T03:15:55.106282Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:49.448347+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:49.448347+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"C., Johnson, B","venue":null,"work_id":"4f24e260-a750-4bca-907d-cf8659884298","year":2019},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:66bc0a5f0fd2db3185044940abdc95da11aa10f3706f8976b0c35d7d69195252","observation_id":"1e858bf4-90eb-4818-9fa8-404a8c63490c","resolution":{"observed_at":"2026-05-14T10:54:13.665061Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2023, ApJ, 950, 85","venue":null,"work_id":"5e6479a1-737d-40c8-b2a5-b8dc82de9f93","year":2023},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:bd443e632cbff2b9244186c023a7f2d87394cde9822b99cfe41a19876e1108e5","observation_id":"9c551d92-d0d3-4dfd-b03b-71b5ebddf3fa","resolution":{"observed_at":"2026-05-14T10:59:15.449534Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2025, ApJ, 980, L34","venue":null,"work_id":"8444d0d3-bc56-460e-82ca-4c7900ba8c37","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:e6d4d4efdac97b3df3106ac02a60783ee0167e208a6ead2e6dc34319e2419c80","observation_id":"e5d0b37e-3e6c-4278-b708-1089b129ae8c","resolution":{"observed_at":"2026-05-14T10:59:15.436275Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2024, A&A, 689, A128","venue":null,"work_id":"aedf8f8a-1f91-427e-b416-0ed4b9135836","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:46fc3fce3056c53338d7997aad0223e7bf8534665a823af3537e981e6fc163af","observation_id":"b4dcb9e7-2986-4b93-9184-86d559e5f6fa","resolution":{"observed_at":"2026-05-14T10:59:15.433324Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"E., Setton, D","venue":null,"work_id":"30a62ace-fab8-4c9a-a9e6-a55f4599358e","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a3ba4b4b2d5e78d21441a6290434343fe26af0878e4001f4e1cbed2f7d836a06","observation_id":"2e32c8f8-89cb-4416-9a5c-992d47d2b8ce","resolution":{"observed_at":"2026-05-14T10:59:15.461186Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2014, ApJ, 784, L38","venue":null,"work_id":"f3b13d49-8d08-4837-bc76-52b772c572cd","year":2014},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a0f034542e5d3c10181a7bcd7794a346b7cfa501e267d9bec84cc8c9913ce420","observation_id":"1d6ef0ff-2191-4130-9178-f1b7df5f8ff8","resolution":{"observed_at":"2026-05-14T10:59:15.445380Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2602.22386","last_updated":"2026-07-17T16:36:24Z","snapshot_observed_at":"2026-08-02T20:50:25.916963Z","submitted_at":"2026-02-25T20:32:56Z","title":"Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model","version":2},"cited_work":{"arxiv_id":"2602.22386","doi":"10.48550/arxiv.2602.22386","metadata_source":"arxiv_reference","pith_arxiv_id":"2602.22386","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, arXiv e-prints","venue":"Open MIND","work_id":"1e082e13-8aa2-4547-bef1-e4303d236cc6","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2602.22386","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:8445d3db237211c0063c3c87a42949194286be02c1ff1dac7447466399d9659a","observation_id":"d69bd229-65a3-4b00-ab68-ecf092ffac6f","resolution":{"observed_at":"2026-07-20T03:19:15.500417Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:50.967816+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:50.967816+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2024, A&A, 691, A145 Matthee , J., Naidu, R","venue":null,"work_id":"aa7e8b4d-eefd-40a1-b97f-b0c351303643","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:90fd86c9dfcb02fc88c0419582573c5e9c5f330459c410fdbcc8cb5f0f514d2f","observation_id":"ad575e11-c164-4bdb-a301-7b124b99813f","resolution":{"observed_at":"2026-05-14T10:59:15.443100Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"P., Kotiwale, G., et al","venue":null,"work_id":"497541f7-1abf-4f2f-8e45-80cc59036a9e","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:6fe5fb43b75b731f80be0b5ce479c7a2824fbc698508eaf277fd97af545c4d8e","observation_id":"6d371ba6-c0a5-453c-9425-ba2e88a054c6","resolution":{"observed_at":"2026-05-14T10:59:15.453368Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.16596","last_updated":"2025-03-20T18:00:00Z","snapshot_observed_at":"2026-07-06T20:56:18.361337Z","submitted_at":"2025-03-20T18:00:00Z","title":"A \"Black Hole Star\" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots","version":1},"cited_work":{"arxiv_id":"2503.16596","doi":"10.48550/arxiv.2503.16596","metadata_source":"pith","pith_arxiv_id":"2503.16596","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"A \"Black Hole Star\" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots","venue":"astro-ph.GA","work_id":"29ad597d-865f-4cdf-8b1b-38e2a6dd6d6c","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2503.16596","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:d70f8f6cceea25dd785ec88ef3e9dbed7d306324c0a2db104c4b344fc838db95","observation_id":"e4f10479-9ef8-4928-a49b-11278b14d674","resolution":{"observed_at":"2026-05-16T08:53:14.890938Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:52.688025+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:52.688025+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2601.14368","doi":"10.48550/arxiv.2601.14368","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Pacucci, A","venue":"arXiv (Cornell University)","work_id":"f41343b1-74fe-4e8a-ac5b-c4e0079ea371","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:ea26d32d192612c655680c99d506046c79e0308829011ba35541957107b22f80","observation_id":"61824f68-eb49-4a37-9b77-72314fce2cbe","resolution":{"observed_at":"2026-05-11T03:15:55.081049Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:53.140287+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:53.140287+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"cb30c30e-be2e-4847-8125-a08518767053","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a8e1665996e4909d0c2c507ea8e963b6503b1cc17645785e666c6ea9c2617263","observation_id":"d0ce5a91-f6e5-41c4-941e-0eab4088e427","resolution":{"observed_at":"2026-05-14T10:59:15.424928Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"F., Schaye, J., et al","venue":null,"work_id":"3b107921-ed58-47fa-9904-aa6f793c9d81","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:4b0deb394d41998644e084c920ec7a299af395b1a0971411252d728a8ac1ef02","observation_id":"3df1c0b4-8745-41e6-9e87-90514b8b801c","resolution":{"observed_at":"2026-05-14T10:59:15.417370Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2025, A&A, 704, A248","venue":null,"work_id":"ecedaa12-60e1-401b-8a70-5ffe2cacda72","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:ab466c97866de52bc17e760992e07d29bf90ec9e8dd8dc89bb364c73c3872c4c","observation_id":"dc242ea2-1e20-4abe-8c5b-4663c30333ee","resolution":{"observed_at":"2026-05-14T10:59:15.441061Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"78047913-c09f-4abf-837a-6ead032f10df","year":2015},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:06d805cfbe0b35ddb5022dfc22403f79d4a7d8973a686f249f76e88c8268174f","observation_id":"7842b5c0-9f90-43dd-8c55-4b9133b1678d","resolution":{"observed_at":"2026-05-14T10:59:15.463062Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"H., et al","venue":null,"work_id":"1e064007-01c1-4074-8e8d-b4f40d2d41ea","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:caeecb09b06e5e08f561e2263535943c75074e44a4632ba93938e948419943cb","observation_id":"ea831b52-d23a-4522-8990-b1b2d6025e87","resolution":{"observed_at":"2026-05-14T10:59:15.427667Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"P., et al","venue":null,"work_id":"9573c583-c6e7-4705-bedf-8bd8e572f89a","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:745c57d33f5be321c5c3855033a2fd65d3b7270dd77ad479183ce450026a72b0","observation_id":"c3e7862b-7552-420a-b274-59ed8f972ad1","resolution":{"observed_at":"2026-05-14T10:59:15.464892Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2603.22277","doi":"10.48550/arxiv.2603.22277","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, arXiv e-prints, arXiv:2603.22277, doi: 10.48550/arXiv.2603.22277","venue":"arXiv (Cornell University)","work_id":"f47fafb4-31ad-4ca3-bcd1-9a78394122ac","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:3c1a5e694d1312d0636b750b1af4ca0d91ff0e851079ea488f4b42d20ccc173a","observation_id":"4705d13f-10ca-4dcb-b830-97f6a1e7fa05","resolution":{"observed_at":"2026-05-11T03:15:55.076236Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:54.514439+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:54.514439+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T04:33:20.290134Z","title":"J., Greene, J","venue":null,"work_id":"a17a508b-f565-41ba-ba76-73b622020832","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:225f584d4f849143e6e103bdc2b9cc20ef8d4f8f8a98452b5d83d700fba0a17e","observation_id":"5e3a303b-d13c-45be-af0d-12c3a72afb6c","resolution":{"observed_at":"2026-05-14T10:59:15.457420Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"F., Faucher-Giguère, C.-A., et al","venue":null,"work_id":"65bde636-d52f-44cd-8757-203417391ea1","year":2020},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:0c77a8c071c52f343d2822703771c91c2e0f4aea4246a7d6b2ae74789f367a28","observation_id":"c084ec9b-4aff-4012-88c8-ca11133f73cb","resolution":{"observed_at":"2026-05-14T10:59:15.422163Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2601.20929","last_updated":"2026-05-22T00:02:06Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-01-28T19:00:00Z","title":"Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot","version":2},"cited_work":{"arxiv_id":"2601.20929","doi":"10.48550/arxiv.2601.20929","metadata_source":"pith","pith_arxiv_id":"2601.20929","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Q., Naidu, R","venue":"astro-ph.GA","work_id":"f6ac99e1-26aa-493b-b524-86c21e9a7e9f","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2601.20929","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:2e96b534d5ad04044cafb066c69e284be57c3a2a94cd6b05dcff41ffaa5a8363","observation_id":"ae0c192d-091d-497b-a26e-3e67a92c70c1","resolution":{"observed_at":"2026-05-25T03:01:11.256109Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-05-22T21:53:01.596362+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-22T21:53:01.596362+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T04:33:20.305919Z","title":"P., Plat, A., et al","venue":null,"work_id":"d4c7fa1a-a070-435f-9358-9098f32ab293","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:16b782dc9fc3f2d5d9eef7c392ff6cec9717b8efc235df4224ab9a9d62530a7d","observation_id":"8faeabfc-a3d3-44a5-b2fc-dc0e00b124fb","resolution":{"observed_at":"2026-05-14T10:54:13.657507Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J., Kokorev, V ., Kocevski, D","venue":null,"work_id":"a57f335f-c752-486f-9b5a-6e34ea24f676","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:dd5f218b3bbd723d4f9f78737a732afc85d9eefa54c6ecd5c2c5e7ca4c319af0","observation_id":"0e231a86-9ea9-4449-ab6d-8ab2cff0a48b","resolution":{"observed_at":"2026-05-14T10:54:13.659099Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"E., Weaver, J","venue":null,"work_id":"5095557f-c561-4827-a472-b5b8727c0521","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:cbf9e1299fb3eddc2da00508af72a344302c12ab43bb76fd03b3422be7bc132c","observation_id":"859db90f-6bc1-44f1-8f06-10f302d63fe5","resolution":{"observed_at":"2026-05-14T10:54:13.660649Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14248","last_updated":"2024-12-18T19:00:02Z","snapshot_observed_at":"2026-08-11T00:20:06.319002Z","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":"2412.14248","doi":"10.48550/arxiv.2412.14248","metadata_source":"arxiv_reference","pith_arxiv_id":"2412.14248","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2024, arXiv e-prints, arXiv:2412.14248, doi: 10.48550/arXiv.2412.14248","venue":"arXiv (Cornell University)","work_id":"f41e31e5-09fb-45b3-bd5c-c79bbbb85b63","year":2024},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"cited_paper":"/paper/2412.14248","citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:05bb88fa28a3bffa5b8c20a68664790bafcc5faa8d1f291cdb15efbd56f4369d","observation_id":"63988257-e28d-43eb-a4ba-8650143e3c8a","resolution":{"observed_at":"2026-05-11T03:15:55.063054Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2026, ApJ, 999, 183","venue":null,"work_id":"a40a8fe2-eb0d-4667-901e-58ffb6bb5ce0","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:264738190b71c8450c03aea35b6e0f730b5bc0cc8fbf49853410a5b65200f3e3","observation_id":"df450592-348e-490b-82d2-99af28ba0ebb","resolution":{"observed_at":"2026-05-14T10:54:13.656032Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T02:25:56.083505Z","title":"L., et al","venue":null,"work_id":"dcbc9e98-d562-46bb-a1d8-245e5e7e9fe9","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a8e726ed7a47fea2d2003aae7f7541a1d55a8691729c2dc5d0217ca7828b91ba","observation_id":"e678a7eb-5954-495e-8b76-a968e9e74805","resolution":{"observed_at":"2026-05-14T10:54:13.651265Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"f8f303c4-c330-4405-8270-b8e54b151366","year":2025},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:49641091a40f41488ac9435c3b7f652eb44765f8ba6aae61f789581059362ef8","observation_id":"01310997-18fe-4646-a8f2-616a3ef96b1a","resolution":{"observed_at":"2026-05-14T10:54:13.652763Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2026, ApJ, 999, 31","venue":null,"work_id":"13c4cebd-dc18-4395-ae75-3c343c9affb1","year":2026},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:a7c5e298c6483dc6f78f21bc482fb93cfa5131c26a5f38b4230db3f91472d230","observation_id":"6ff0fef4-8ed5-4da1-a1df-573ddf28a0af","resolution":{"observed_at":"2026-05-14T10:54:13.654231Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"& King, A","venue":null,"work_id":"411cab7c-bb42-4138-8081-34ea47008d60","year":2021},"citing_paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-11T03:11:10.401986Z"},"links":{"citing_paper":"/paper/2605.07976"},"observation_digest":"sha256:bafb04ac17ce3a3050329740576cfe6f2354f70371b730b04a5d2e2b8d96bdf2","observation_id":"367e593c-d1f6-4049-95cc-cf543f0e9817","resolution":{"observed_at":"2026-05-14T10:54:13.649590Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2605.07976","last_updated":"2026-05-08T16:34:53Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T23:20:15.696237Z","submitted_at":"2026-05-08T16:34:53Z","title":"Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff"},"reference_resolution":{"displayed":68,"state_counts":{"malformed_identifier":0,"metadata_mismatch":4,"parse_uncertain":0,"unresolved":8,"verified_exact":10,"verified_fuzzy":46},"total_outbound_references":68},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 68 of 68 outbound references and 1 inbound Pith citation observation for arXiv:2605.07976."}