{"as_of":"2026-08-16T21:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c0636f8b19a38524779bf9d0c840bc17d779241aa53f6b201e90c5de2da8db8d","coverage":[{"denominator":45,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":45,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T04:33:47.853253Z","state":"measured"},{"denominator":45,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":45,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2412.18772/citation-record","integrity":"/paper/2412.18772/integrity","json":"/paper/2412.18772/citation-record.json","paper":"/paper/2412.18772"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.687076Z","title":"3C 273 : A Star-Like Object with Large Red-Shift","venue":null,"work_id":null,"year":1963},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.687076Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:e412bfb077e9f992d1fb2ec78b9293ad2ea93c232196e1d7f6ccbd0fd68a7972","observation_id":"82ac0884-ab1c-4d88-908e-14f2c5d092b6","resolution":{"observed_at":"2026-08-11T04:33:47.687076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.691201Z","title":"Unified models for active galactic nuclei and quasars","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.691201Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:f244437feb56b004565545633975aafce1e89b974132664c4a0d000545ae743d","observation_id":"054c5c8d-3ee1-435f-b536-3cde725923aa","resolution":{"observed_at":"2026-08-11T04:33:47.691201Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.00811","last_updated":"2015-05-04T21:01:35Z","snapshot_observed_at":"2026-08-14T22:49:53.974249Z","submitted_at":"2015-05-04T21:01:35Z","title":"Revisiting the Unified Model of Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.00811","snapshot_observed_at":"2026-08-11T04:33:47.694655Z","title":"Revisiting the Unified Model of Active Galactic Nuclei","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.694655Z"},"links":{"cited_paper":"/paper/1505.00811","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:526bbec3fc7f4680a2492e38b560363dd2e16e66dca5b85d45540e9c35aee46d","observation_id":"ce43f0fe-d5e4-4c3b-a4e7-b5805aac5895","resolution":{"observed_at":"2026-08-11T04:33:47.694655Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.00019","last_updated":"2017-08-31T18:01:49Z","snapshot_observed_at":"2026-08-14T20:37:11.732061Z","submitted_at":"2017-08-31T18:01:49Z","title":"Nuclear obscuration in active galactic nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.00019","snapshot_observed_at":"2026-08-11T04:33:47.698375Z","title":"Nuclear obscuration in active galactic nuclei","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.698375Z"},"links":{"cited_paper":"/paper/1709.00019","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:73213e4cc96cf4ab5b551f2fb47f657fa3cbea108c2a4ce0baf10b5c5e9140a0","observation_id":"70c3611e-6798-456a-8cdf-08e69cce2d9a","resolution":{"observed_at":"2026-08-11T04:33:47.698375Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0386","last_updated":"2009-10-16T05:09:43Z","snapshot_observed_at":"2026-08-15T06:39:47.430551Z","submitted_at":"2009-08-04T05:58:34Z","title":"What broad emission lines tell us about how active galactic nuclei work","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0908.0386","snapshot_observed_at":"2026-08-11T04:33:47.702343Z","title":"What broad emission lines tell us about how active galactic nuclei work","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.702343Z"},"links":{"cited_paper":"/paper/0908.0386","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:e460805fa43217f177be8f1bd9357d5a354d8b1a9f12d36bc81c09b21ddbc774","observation_id":"ad22197b-df74-4136-ae2f-6d2fe1f4248a","resolution":{"observed_at":"2026-08-11T04:33:47.702343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.706416Z","title":"The environment of active galactic nuclei","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.706416Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:cee4aa7d5517740a0c06223c3663a8722236bc0368e269fcf11b1ebd0faf9b65","observation_id":"f1da040a-11d8-4998-ba67-a9abf0b08e4f","resolution":{"observed_at":"2026-08-11T04:33:47.706416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0306389","last_updated":"2003-06-19T09:00:34Z","snapshot_observed_at":"2026-07-07T00:34:15.172651Z","submitted_at":"2003-06-19T09:00:34Z","title":"Accretion disk wind in the AGN broad-line region: Spectroscopically resolved line profile variations in Mrk110","version":1},"cited_work":{"arxiv_id":"astro-ph/0306389","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0306389","snapshot_observed_at":"2026-08-11T04:33:48.295428Z","title":"Accretion disk wind in the AGN broad-line region: Spectroscopically resolved line profile variations in Mrk110","venue":"astro-ph","work_id":"de499eb5-e1a5-47b9-8aeb-95fc4f206e11","year":2003},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.710546Z"},"links":{"cited_paper":"/paper/astro-ph/0306389","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:577d7d390201570e483e49812a9e65d84f38d9da3604326f7e5566b81b8c7648","observation_id":"72d61376-b41f-4eee-bc1f-a2f157dea5d9","resolution":{"observed_at":"2026-08-11T04:33:48.299357Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.7312","last_updated":"2015-01-09T10:51:56Z","snapshot_observed_at":"2026-08-14T23:18:05.696882Z","submitted_at":"2014-09-25T16:10:11Z","title":"The dust origin of the Broad Line Region and the model consequences for AGN unification scheme","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.7312","snapshot_observed_at":"2026-08-11T04:33:47.714480Z","title":"The dust origin of the Broad Line Region and the model consequences for AGN unification scheme","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.714480Z"},"links":{"cited_paper":"/paper/1409.7312","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:164a18beeed0bdeff5fc4bb78c227907908317985289d875551c7f81bbdc525c","observation_id":"9eee6b1a-e28b-480d-9c2b-469a7cf6d53c","resolution":{"observed_at":"2026-08-11T04:33:47.714480Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701437","last_updated":"2007-01-15T22:03:52Z","snapshot_observed_at":"2026-07-07T01:06:12.971026Z","submitted_at":"2007-01-15T22:03:52Z","title":"Photoionization Models of the Broad-line Region","version":1},"cited_work":{"arxiv_id":"astro-ph/0701437","doi":"10.48550/arxiv.astro-ph/0701437","metadata_source":"pith","pith_arxiv_id":"astro-ph/0701437","snapshot_observed_at":"2026-08-11T06:16:19.390415Z","title":"Photoionization Models of the Broad-line Region","venue":"astro-ph","work_id":"6dfb0c20-477b-4309-ae79-3831298ae537","year":2007},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.718433Z"},"links":{"cited_paper":"/paper/astro-ph/0701437","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:86193d02cc8232e69c974b4a35a05f18312efd1b15bcb719eae38cee7a1be263","observation_id":"4fb43135-36eb-444a-95e7-e7010b2ab995","resolution":{"observed_at":"2026-08-11T04:33:47.971259Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603460","last_updated":"2006-03-24T13:25:19Z","snapshot_observed_at":"2026-07-07T00:59:11.610338Z","submitted_at":"2006-03-17T09:42:21Z","title":"Systematic Effects in Measurement of Black Hole Masses by Emission-Line Reverberation of Active Galactic Nuclei: Eddington Ratio and Inclination","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603460","snapshot_observed_at":"2026-08-11T04:33:47.722318Z","title":"Systematic effects in measurement of black hole masses by emission-line reverberation of active galactic nuclei: Eddington ratio and inclination","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.722318Z"},"links":{"cited_paper":"/paper/astro-ph/0603460","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:5abcf74f3d2c315a6ebcc75fd074d3ed5fc4050bef2be2b483d8d0e67c698ade","observation_id":"c39207aa-39d2-4686-907d-2e7d1db901fd","resolution":{"observed_at":"2026-08-11T04:33:47.722318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.11195","last_updated":"2018-11-27T19:00:18Z","snapshot_observed_at":"2026-08-14T17:52:28.582206Z","submitted_at":"2018-11-27T19:00:18Z","title":"Spatially resolved rotation of the broad-line region of a quasar at sub-parsec scale","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.11195","snapshot_observed_at":"2026-08-11T04:33:47.726360Z","title":"Spatially resolved rotation of the broad-line region of a quasar at sub-parsec scale","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.726360Z"},"links":{"cited_paper":"/paper/1811.11195","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:1ac62d771bc68f167fecd74b60db9ebeec6680c6b42fc712fe95c5bbe887d488","observation_id":"925a852e-9fc2-4b8d-b559-f6be64e97041","resolution":{"observed_at":"2026-08-11T04:33:47.726360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.4312","last_updated":"2013-06-26T01:41:27Z","snapshot_observed_at":"2026-08-15T00:13:38.159983Z","submitted_at":"2013-06-18T20:00:00Z","title":"Dust in the polar region as a major contributor to the IR emission of AGN","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.4312","snapshot_observed_at":"2026-08-11T04:33:47.730266Z","title":"Dust in the Polar Region as a Major Contributor to the Infrared Emission of Active Galactic Nuclei","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.730266Z"},"links":{"cited_paper":"/paper/1306.4312","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:a20b49f98583e8cb2b255a62fdfa644dc1f54ef07629cfc7369a23662f35735c","observation_id":"beec9ee3-427b-42e8-b9c7-3e1cd9b64396","resolution":{"observed_at":"2026-08-11T04:33:47.730266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0605686","last_updated":"2006-08-04T16:10:42Z","snapshot_observed_at":"2026-08-16T12:25:37.511099Z","submitted_at":"2006-05-28T07:31:52Z","title":"The AGN Obscuring Torus -- End of the \"Doughnut\" Paradigm?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0605686","snapshot_observed_at":"2026-08-11T04:33:47.734063Z","title":"Doughnut","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.734063Z"},"links":{"cited_paper":"/paper/astro-ph/0605686","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:63363cc33c0e19c33741912ff036b21346f11152163df3fa65397268dddf7e1b","observation_id":"b35a8ae5-c020-4057-b408-bf674ceb5c86","resolution":{"observed_at":"2026-08-11T04:33:47.734063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005315","last_updated":"2000-05-15T21:57:39Z","snapshot_observed_at":"2026-07-07T00:11:18.128450Z","submitted_at":"2000-05-15T21:57:39Z","title":"Dynamics of line-driven disk winds in Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005315","snapshot_observed_at":"2026-08-11T04:33:47.737923Z","title":"Dynamics of Line-driven Disk Winds in Active Galactic Nuclei","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.737923Z"},"links":{"cited_paper":"/paper/astro-ph/0005315","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:66e4b4a6e26bd2da8bf93bac83799a7fd4b9be73bd07ed72111b77c1d13d67ec","observation_id":"cc4d40aa-0d26-4cf8-b8c5-c87aaacdeb30","resolution":{"observed_at":"2026-08-11T04:33:47.737923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.00336","last_updated":"2021-07-12T13:29:06Z","snapshot_observed_at":"2026-08-16T20:33:55.205325Z","submitted_at":"2021-01-30T23:18:57Z","title":"The picture of BLR in 2.5-D FRADO: Dynamics & Geometry","version":2},"cited_work":{"arxiv_id":"2102.00336","doi":null,"metadata_source":"pith","pith_arxiv_id":"2102.00336","snapshot_observed_at":"2026-08-11T04:33:48.220308Z","title":"The picture of BLR in 2.5-D FRADO: Dynamics & Geometry","venue":"astro-ph.GA","work_id":"7163088d-0e1c-45af-ab9f-f78d75d3ace9","year":2021},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.742043Z"},"links":{"cited_paper":"/paper/2102.00336","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:2861ba2665b5cf7c9367ffbfe4d4f88547f295fdd66a9010d73972c94bce474b","observation_id":"601793dd-7d29-45c9-ac97-c79e30a420c7","resolution":{"observed_at":"2026-08-11T04:33:48.223757Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.746113Z","title":"Dust in the Narrow-Line Region of Active Galactic Nuclei","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.746113Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:78328d3b57fa09dfbd217ff918647e6d6272a3af9a297094bc1c52d34c53a600","observation_id":"9f52f3db-c5c7-4a41-8287-71a11d7a59d3","resolution":{"observed_at":"2026-08-11T04:33:47.746113Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9912524","last_updated":"1999-12-27T20:40:38Z","snapshot_observed_at":"2026-08-15T12:50:10.110159Z","submitted_at":"1999-12-27T20:40:38Z","title":"Broad Emission Line Regions in AGN: the Link with the Accretion Power","version":1},"cited_work":{"arxiv_id":"astro-ph/9912524","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9912524","snapshot_observed_at":"2026-08-11T04:33:48.206016Z","title":"Broad Emission Line Regions in AGN: the Link with the Accretion Power","venue":"astro-ph","work_id":"6b9919cc-a398-4f5e-b1cc-369017e1b1e5","year":1999},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.750003Z"},"links":{"cited_paper":"/paper/astro-ph/9912524","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:5f3d75e4c0ac330bad12995ad1914bee715ce1247d4e83aeff68c5d809e1f4d8","observation_id":"ec5d76d6-b4ef-4792-b304-d1d6565bc6d8","resolution":{"observed_at":"2026-08-11T04:33:48.209806Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1010.6201","last_updated":"2010-11-19T15:04:28Z","snapshot_observed_at":"2026-08-15T05:04:28.151574Z","submitted_at":"2010-10-29T13:21:38Z","title":"The origin of the Broad Line Region in Active Galactic Nuclei","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.6201","snapshot_observed_at":"2026-08-11T04:33:47.754171Z","title":"The origin of the broad line region in active galactic nuclei","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.754171Z"},"links":{"cited_paper":"/paper/1010.6201","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:2a83365e7ad63c13f25b3b2425c002716714af81a4ecb78e174d5b583b58bb4a","observation_id":"b920f4b4-7eb5-4d6d-a2aa-04207bf6bfe9","resolution":{"observed_at":"2026-08-11T04:33:47.754171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.14963","last_updated":"2022-04-13T11:02:48Z","snapshot_observed_at":"2026-08-16T17:38:26.617714Z","submitted_at":"2021-11-29T21:17:41Z","title":"Radiation pressure on dust explains the Low Ionized Broad Emission Lines in Active Galactic Nuclei","version":3},"cited_work":{"arxiv_id":"2111.14963","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.14963","snapshot_observed_at":"2026-08-11T04:33:48.180899Z","title":"Radiation pressure on dust explains the Low Ionized Broad Emission Lines in Active Galactic Nuclei","venue":"astro-ph.GA","work_id":"cd94c6a4-9db9-43d1-bdde-bce892968e69","year":2021},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.758487Z"},"links":{"cited_paper":"/paper/2111.14963","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:3144a259f748d4bfd27ba90aa5ac94fe053626538468435511faee3d9795e9a1","observation_id":"afdcdfb5-b4ed-4f20-b30d-568a6e016822","resolution":{"observed_at":"2026-08-11T04:33:48.185091Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.762337Z","title":"Accretion Disk Winds from Active Galactic Nuclei","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.762337Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:e7141ed774b5bd84e0367212ab76c4c1611dcb83baa2d5b23abecf70a32e87a7","observation_id":"da9c5406-2893-4888-a3a0-0489a13a9fd8","resolution":{"observed_at":"2026-08-11T04:33:47.762337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.00420","last_updated":"2016-10-03T06:34:01Z","snapshot_observed_at":"2026-08-14T21:37:04.820336Z","submitted_at":"2016-10-03T06:34:01Z","title":"Test of the Formation mechanism of the Broad Line Region in Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.00420","snapshot_observed_at":"2026-08-11T04:33:47.765967Z","title":"A Test of the Formation Mechanism of the Broad Line Region in Active Galactic Nuclei","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.765967Z"},"links":{"cited_paper":"/paper/1610.00420","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:6bec4e074bd5192c0483e32bf63ac1106c345403ffa059cff162ffff017e6f22","observation_id":"532b553c-20fc-4538-aba1-2906270c16c6","resolution":{"observed_at":"2026-08-11T04:33:47.765967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.07958","last_updated":"2017-08-22T08:53:25Z","snapshot_observed_at":"2026-08-14T20:51:55.188714Z","submitted_at":"2017-06-24T13:49:43Z","title":"Failed radiatively Accelerated Dusty Outflow model of the Broad Line Region in Active Galactic Nuclei. I. Analytical solution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.07958","snapshot_observed_at":"2026-08-11T04:33:47.769776Z","title":"Failed Radiatively Accelerated Dusty Outflow Model of the Broad Line Region in Active Galactic Nuclei","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.769776Z"},"links":{"cited_paper":"/paper/1706.07958","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:59ade94f518f737865bcf24f4a26f29f402346aec0e22d1e179f47553b1a0299","observation_id":"211a4666-5797-447a-98f4-0a8eb257e8bf","resolution":{"observed_at":"2026-08-11T04:33:47.769776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.773410Z","title":"Infrared Radiation from Dust in Seyfert Galaxies","venue":null,"work_id":null,"year":1969},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.773410Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:fedc50a433b103a8ad3afa59207841f0e3c44e6a088d1c3c3811fae3fa89f084","observation_id":"7219385d-dc44-44e4-a0b1-d36b66853400","resolution":{"observed_at":"2026-08-11T04:33:47.773410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.1458","last_updated":"2007-10-08T07:13:48Z","snapshot_observed_at":"2026-08-15T10:30:29.546984Z","submitted_at":"2007-10-08T07:13:48Z","title":"Broad-line Balmer Decrements in Blue Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":"0710.1458","doi":null,"metadata_source":"pith","pith_arxiv_id":"0710.1458","snapshot_observed_at":"2026-08-11T04:33:48.144477Z","title":"Broad-line Balmer Decrements in Blue Active Galactic Nuclei","venue":"astro-ph","work_id":"05a71f6f-9207-418e-a0f7-d9c55853df08","year":2007},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.776432Z"},"links":{"cited_paper":"/paper/0710.1458","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:2c43bd8874043910a580595d8ca9119e1a8333f44e53b0977ccefbe7486a9ea8","observation_id":"14ca2a0e-4e97-4485-a3ff-024568d806de","resolution":{"observed_at":"2026-08-11T04:33:48.148798Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.00278","last_updated":"2020-06-04T12:47:10Z","snapshot_observed_at":"2026-07-06T08:41:08.798994Z","submitted_at":"2019-11-30T22:48:08Z","title":"R-L Relation in Realistic FRADO Model","version":2},"cited_work":{"arxiv_id":"1912.00278","doi":null,"metadata_source":"pith","pith_arxiv_id":"1912.00278","snapshot_observed_at":"2026-08-11T04:33:48.128154Z","title":"R-L Relation in Realistic FRADO Model","venue":"astro-ph.HE","work_id":"f2f8a1b9-e61a-4303-b6ae-b2deb08b9b8f","year":2019},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.779735Z"},"links":{"cited_paper":"/paper/1912.00278","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:5b328d6df75d762ba743d3d3f06b7e5d3a73dbcbfd59ba7e1097d7d4ce52c0a9","observation_id":"30c62504-0e66-4ee8-a3fd-e453bf89a80f","resolution":{"observed_at":"2026-08-11T04:33:48.132785Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:48.448423Z","title":"Black holes in binary systems","venue":null,"work_id":"d15f7f3d-d463-4e6b-9ff1-b0e157735697","year":1973},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.783037Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:2ddb086ff999a8ba2456f703f793767cde4894ea5536f23c42338d6bdcadc76e","observation_id":"8acab77b-8f00-499d-9e07-ce41325d19c7","resolution":{"observed_at":"2026-08-11T04:33:48.451894Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.09304","last_updated":"2022-09-19T19:00:02Z","snapshot_observed_at":"2026-08-16T16:31:23.355381Z","submitted_at":"2022-09-19T19:00:02Z","title":"The Wind Dynamics of Super-Eddington Sources in FRADO","version":1},"cited_work":{"arxiv_id":"2209.09304","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.09304","snapshot_observed_at":"2026-08-11T04:33:48.111505Z","title":"The Wind Dynamics of Super-Eddington Sources in FRADO","venue":"astro-ph.GA","work_id":"d04fecc1-dc85-4443-ac8e-aee50d4bcc14","year":2022},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.786482Z"},"links":{"cited_paper":"/paper/2209.09304","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:99bd57730a8ab3d4db82d4839e76ce54d464debdcaec4bb088efc7e8bc5c697d","observation_id":"0e48ea35-f1a3-4958-b6b8-f44785a0ae1a","resolution":{"observed_at":"2026-08-11T04:33:48.116167Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.789786Z","title":"Active Galactic Nuclei Disk Winds, Absorption Lines, and Warm Absorbers","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.789786Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:f41dea36fc880c3e79473634e6c55fd142b0ad0726297212f57820d154a39988","observation_id":"3335f82c-ea83-407a-9910-fbec3ffefd33","resolution":{"observed_at":"2026-08-11T04:33:47.789786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.793148Z","title":"Radiation-driven winds in Of stars","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.793148Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:33931769a0cb840561ea415129843f47fab6f02ca51c7247bde563302cb0d03f","observation_id":"fb2af947-021c-4481-a370-ccb7d9cf42ff","resolution":{"observed_at":"2026-08-11T04:33:47.793148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.796789Z","title":"Predictions of the effect of clumping on the wind properties of O-type stars","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.796789Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:458ee41eb1328860509c22e516c3001bc76f2b4c78d9c56a70d1c375e81f6212","observation_id":"92d9569a-8b12-43ca-8bbb-20a56fd9fbf6","resolution":{"observed_at":"2026-08-11T04:33:47.796789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.800511Z","title":"The Role of Radiative Acceleration in Outflows from Broad Absorption Line QSOs","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.800511Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:8e0f07d8b48c7fba72d4514982b701c659f6068e2f1ae89b1e40381027354329","observation_id":"b8000b6a-aa3c-4be7-9d07-609af62a3e72","resolution":{"observed_at":"2026-08-11T04:33:47.800511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.804117Z","title":"Terminal Velocities and the Bistability of Stellar Winds","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.804117Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:0e8951494da8b55a4f84db061db2cf3f31d7b2eb877408129c0a30cdd61fe81b","observation_id":"3fbbdedd-0a7e-4d39-9c71-5ce8d8d3ff3d","resolution":{"observed_at":"2026-08-11T04:33:47.804117Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0308344","last_updated":"2003-08-20T11:44:16Z","snapshot_observed_at":"2026-07-07T00:35:40.627025Z","submitted_at":"2003-08-20T11:44:16Z","title":"Rosseland and Planck Mean Opacities for Protoplanetary Discs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0308344","snapshot_observed_at":"2026-08-11T04:33:47.807659Z","title":"Rosseland and Planck mean opacities for protoplanetary discs","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.807659Z"},"links":{"cited_paper":"/paper/astro-ph/0308344","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:8cffbb8fc58380ee63e3c10a6c22641ec23da3e243cff837521b5f8e90757517","observation_id":"33142e13-d077-48e7-8763-ada15cf590ba","resolution":{"observed_at":"2026-08-11T04:33:47.807659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0105231","last_updated":"2001-05-14T17:29:00Z","snapshot_observed_at":"2026-07-07T00:18:25.513971Z","submitted_at":"2001-05-14T17:29:00Z","title":"Composite Quasar Spectra From the Sloan Digital Sky Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0105231","snapshot_observed_at":"2026-08-11T04:33:47.811888Z","title":"Composite Quasar Spectra from the Sloan Digital Sky Survey.AJ 2001, 122, 549–564, [arXiv:astro-ph/astro-ph/0105231]","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.811888Z"},"links":{"cited_paper":"/paper/astro-ph/0105231","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:924740e3290c4d57277460a75c8e66b53df9fa48d75d30bc3ea386670641b264","observation_id":"ecff50e2-96e5-4a96-902f-7c53be2ba552","resolution":{"observed_at":"2026-08-11T04:33:47.811888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.5178","last_updated":"2011-05-02T19:32:20Z","snapshot_observed_at":"2026-08-15T05:15:16.253308Z","submitted_at":"2010-06-27T02:19:19Z","title":"A Catalog of Quasar Properties from SDSS DR7","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1006.5178","snapshot_observed_at":"2026-08-11T04:33:47.815889Z","title":"A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 7","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.815889Z"},"links":{"cited_paper":"/paper/1006.5178","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:a45d233f0f46b173ac740383c83db14884dbfad225e647de7a7526825dd7263c","observation_id":"1928578f-f7b5-4a26-895c-5572597333ce","resolution":{"observed_at":"2026-08-11T04:33:47.815889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.819683Z","title":"Misaligned Disks as Obscurers in Active Galaxies","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.819683Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:bf0c8ae862df6c1ee7512df6d8190086ed269c8122e01d882b2e08c5e87106bc","observation_id":"598318b1-0a65-469a-8c6d-dcff4647397e","resolution":{"observed_at":"2026-08-11T04:33:47.819683Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.05089","last_updated":"2023-10-25T15:46:51Z","snapshot_observed_at":"2026-08-16T14:54:07.087353Z","submitted_at":"2023-10-08T09:34:32Z","title":"Broad-line region in active galactic nuclei: Dusty or dustless?","version":2},"cited_work":{"arxiv_id":"2310.05089","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.05089","snapshot_observed_at":"2026-08-11T04:33:48.065288Z","title":"Broad-line region in active galactic nuclei: Dusty or dustless?","venue":"astro-ph.GA","work_id":"7b5a5dfc-433f-4f43-8d79-eb3804ad4a75","year":2023},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.823285Z"},"links":{"cited_paper":"/paper/2310.05089","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:dd0e61a23ef39abbfbd8c536431a9adf34a63f8ddd5e37d8063f179dc354df6c","observation_id":"06c4df74-a47a-4688-a179-4747c1cb8b06","resolution":{"observed_at":"2026-08-11T04:33:48.069856Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0408293","last_updated":"2004-08-16T20:11:07Z","snapshot_observed_at":"2026-07-07T00:44:10.542942Z","submitted_at":"2004-08-16T20:11:07Z","title":"Dynamics of Line-Driven Disk Winds in Active Galactic Nuclei II: Effects of Disk Radiation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0408293","snapshot_observed_at":"2026-08-11T04:33:47.827171Z","title":"Dynamics of Line-driven Disk Winds in Active Galactic Nuclei","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.827171Z"},"links":{"cited_paper":"/paper/astro-ph/0408293","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:901377f5a52ae3b3603fa920fd80158d1d0aeb426165d7a89b0c6f99a962aff3","observation_id":"9682b089-59f1-43f8-ad0e-a4f60e6c5d5d","resolution":{"observed_at":"2026-08-11T04:33:47.827171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05181","last_updated":"2016-04-23T16:40:36Z","snapshot_observed_at":"2026-08-14T22:13:56.166828Z","submitted_at":"2016-01-20T06:30:49Z","title":"Reverberation Mapping of the Broad Line Region: application to a hydrodynamical line-driven disk wind solution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.05181","snapshot_observed_at":"2026-08-11T04:33:47.830915Z","title":"Reverberation Mapping of the Broad Line Region: Application to a Hydrodynamical Line-driven Disk Wind Solution","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.830915Z"},"links":{"cited_paper":"/paper/1601.05181","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:2c223ee13af049d593578fb8b1bb5053f6aa1dfa1d71da0cc2a5a74cbc98b613","observation_id":"47238dfc-feda-4595-97d5-229aa0e6e170","resolution":{"observed_at":"2026-08-11T04:33:47.830915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201362","last_updated":"2002-01-22T10:21:25Z","snapshot_observed_at":"2026-08-16T15:45:53.594076Z","submitted_at":"2002-01-22T10:21:25Z","title":"Average Quasar Spectra in the Context of Eigenvector 1","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0201362","snapshot_observed_at":"2026-08-11T04:33:47.834677Z","title":"Average Quasar Spectra in the Context of Eigenvector 1","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.834677Z"},"links":{"cited_paper":"/paper/astro-ph/0201362","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:ada5690a2a7e238512301a78b6083f71a961072683a1856117e352e0cea5a541","observation_id":"a36b9390-083e-49a7-8e44-5ee40641f3c4","resolution":{"observed_at":"2026-08-11T04:33:47.834677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03688","last_updated":"2016-02-11T12:09:29Z","snapshot_observed_at":"2026-08-14T22:10:45.673138Z","submitted_at":"2016-02-11T12:09:29Z","title":"Gravitational Redshift of Emission Lines in the AGN Spectra","version":1},"cited_work":{"arxiv_id":"1602.03688","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.03688","snapshot_observed_at":"2026-08-11T04:33:48.019920Z","title":"Gravitational Redshift of Emission Lines in the AGN Spectra","venue":"astro-ph.GA","work_id":"11ae34bc-7634-44f9-9629-9bb43becf49b","year":2016},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.838425Z"},"links":{"cited_paper":"/paper/1602.03688","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:70d1a31251bdb5d9d1404d177b30e00a6b7262b2c5e07fdd62b4021b7f70501d","observation_id":"b713fe0b-2ece-46c7-a3d7-7195400f8e26","resolution":{"observed_at":"2026-08-11T04:33:48.023697Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T04:33:47.842136Z","title":"Internal Redshift Difference and Central Mass in QSOs","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.842136Z"},"links":{"citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:fb3a9f436f8820e52e68830a0a635bc2e36a0f833ee0a47d4402b87b587f26bb","observation_id":"7111b0cf-b1a6-43b1-997c-f647b69c5b59","resolution":{"observed_at":"2026-08-11T04:33:47.842136Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.2499","last_updated":"2007-09-16T16:24:18Z","snapshot_observed_at":"2026-08-15T10:32:12.398201Z","submitted_at":"2007-09-16T16:24:18Z","title":"Our Search for an H-R Diagram of Quasars","version":1},"cited_work":{"arxiv_id":"0709.2499","doi":"10.48550/arxiv.0709.2499","metadata_source":"pith","pith_arxiv_id":"0709.2499","snapshot_observed_at":"2026-08-11T06:16:19.390415Z","title":"Our Search for an H-R Diagram of Quasars","venue":"astro-ph","work_id":"dfe58d07-c8a2-49b2-8f0b-d04e1afe3766","year":2007},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.845971Z"},"links":{"cited_paper":"/paper/0709.2499","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:3dfe7a57d6efebe08c270227459058c8e01c1ced0cc477bac340721891d0a1d5","observation_id":"61ae4bce-4a4b-4b39-8034-6e11945b975d","resolution":{"observed_at":"2026-08-11T04:33:47.888926Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.3065","last_updated":"2012-11-13T18:19:50Z","snapshot_observed_at":"2026-08-15T00:39:30.126075Z","submitted_at":"2012-11-13T18:19:50Z","title":"The shape of broad-line profiles in AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.3065","snapshot_observed_at":"2026-08-11T04:33:47.849896Z","title":"The shape of broad-line profiles in active galactic nuclei","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.849896Z"},"links":{"cited_paper":"/paper/1211.3065","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:045283886b5aa7e57454668e9180c27bc6dc8395267fa62f9bbdb0ac89edbf43","observation_id":"41e584be-6d1b-4ed5-8f59-a76c23df5539","resolution":{"observed_at":"2026-08-11T04:33:47.849896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.14434","last_updated":"2023-09-25T18:00:16Z","snapshot_observed_at":"2026-08-16T14:57:44.880342Z","submitted_at":"2023-09-25T18:00:16Z","title":"A disc wind model for blueshifts in quasar broad emission lines","version":1},"cited_work":{"arxiv_id":"2309.14434","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.14434","snapshot_observed_at":"2026-08-11T04:33:47.994460Z","title":"A disc wind model for blueshifts in quasar broad emission lines","venue":"astro-ph.GA","work_id":"49630700-d4ad-4616-81e2-7b5b7175d371","year":2023},"citing_paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T04:33:47.853253Z"},"links":{"cited_paper":"/paper/2309.14434","citing_paper":"/paper/2412.18772"},"observation_digest":"sha256:94cce09abe6a94f19eda98cddf1f1d99105329bc02ea133abd61d4347fe4db52","observation_id":"77095c8d-7552-48b7-8585-9df81efe6357","resolution":{"observed_at":"2026-08-11T04:33:47.998334Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.18772","last_updated":"2024-12-25T04:19:59Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-11T06:52:17.239493Z","submitted_at":"2024-12-25T04:19:59Z","title":"The effect of outflow launching radial efficiency of accretion disk on the shape of emission-line profiles"},"reference_resolution":{"displayed":45,"state_counts":{"malformed_identifier":6,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":27,"verified_exact":11,"verified_fuzzy":1},"total_outbound_references":45},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 45 of 45 outbound references and 0 inbound Pith citation observations for arXiv:2412.18772."}