{"as_of":"2026-08-16T17:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:137403a4343cda255216393e5daf2a1600432fee8b78f35b8b5b26e6e916f544","coverage":[{"denominator":73,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":73,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:50:49.234264Z","state":"measured"},{"denominator":76,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":76,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:16:58.648844Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":1,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.08855","snapshot_observed_at":"2026-08-16T05:16:58.648844Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.21207","last_updated":"2025-07-16T17:37:06Z","snapshot_observed_at":"2026-08-16T11:10:17.414359Z","submitted_at":"2025-04-29T22:23:35Z","title":"The inner structure and thermodynamics of a thin accretion disc","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-16T05:16:58.648844Z"},"links":{"cited_paper":"/paper/2505.08855","citing_paper":"/paper/2504.21207"},"observation_digest":"sha256:8f52848b9740075f1269cfe920f665dac94b6227263cc035896a376f6dbd0874","observation_id":"3ed34590-202d-4b76-9857-aae2c3b36864","resolution":{"observed_at":"2026-08-16T05:16:58.648844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"cited_work":{"arxiv_id":"2505.08855","doi":"10.48550/arxiv.2505.08855","metadata_source":"arxiv_reference","pith_arxiv_id":"2505.08855","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"ArXiv.org","work_id":"bebb871d-19cf-444e-8c6c-243598fb9a01","year":2025},"citing_paper":{"arxiv_id":"2604.25996","last_updated":"2026-04-28T18:00:01Z","snapshot_observed_at":"2026-08-15T04:40:29.916167Z","submitted_at":"2026-04-28T18:00:01Z","title":"Distortion of a relativistic jet echoing a magnetic flux eruption","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-05-07T15:19:19.748918Z"},"links":{"cited_paper":"/paper/2505.08855","citing_paper":"/paper/2604.25996"},"observation_digest":"sha256:45fe88f854437ff05e6cd452b8d18ce3b6bd746f0ec0d979a74a6149a5679745","observation_id":"4b5e995c-bfeb-4a60-a3b0-88e1ce0d5c0a","resolution":{"observed_at":"2026-05-12T00:26:18.036258Z","resolver_source":"arxiv_id","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":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"cited_work":{"arxiv_id":"2505.08855","doi":"10.48550/arxiv.2505.08855","metadata_source":"arxiv_reference","pith_arxiv_id":"2505.08855","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"ArXiv.org","work_id":"bebb871d-19cf-444e-8c6c-243598fb9a01","year":2025},"citing_paper":{"arxiv_id":"2605.20317","last_updated":"2026-05-19T18:00:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-19T18:00:00Z","title":"Simulation-Based Prediction of Black Hole Fe K$\\alpha$ Line Profiles","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-05-21T01:25:53.670807Z"},"links":{"cited_paper":"/paper/2505.08855","citing_paper":"/paper/2605.20317"},"observation_digest":"sha256:ff41dbf652360ebdc95696506c575eb5c613c9d797e01b505ae1c0ad6dc51cc3","observation_id":"78ddf745-a33f-465b-bbf3-e23567615a53","resolution":{"observed_at":"2026-05-21T01:29:22.228418Z","resolver_source":"arxiv_id","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"}}],"links":{"evidence":"/evidence","html":"/paper/2505.08855/citation-record","integrity":"/paper/2505.08855/integrity","json":"/paper/2505.08855/citation-record.json","paper":"/paper/2505.08855"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:50.061755Z","title":"Additionally, large cooling rates can lead to numerical errors if the associated decrease in en- ergy exceeds the cell internal energy","venue":null,"work_id":"a39c86c0-06b0-483a-ac07-290baddacbd0","year":null},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.943093Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:7eec6902e72be5f44ba88d27b4a48dc6cb36f9b33e769a025f0eeac63ddb07b8","observation_id":"973ed726-ac49-461a-8480-dd602315a985","resolution":{"observed_at":"2026-08-15T21:50:50.065176Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:50.052786Z","title":"truncated thin disk+ RIAF","venue":null,"work_id":"c6e51c3c-3624-41ba-bf27-32cd15d9cb06","year":null},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.946815Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:025a2ce434a332cdef5b3018c5aa6c0b534e387fd03377d2ff2e967365974eee","observation_id":"34fb3270-3dab-4e56-a0f7-7bddf5735284","resolution":{"observed_at":"2026-08-15T21:50:50.056006Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:50.014762Z","title":"Fender and T","venue":null,"work_id":"f00fe55a-f44e-4ff1-958a-6cbe6a582e21","year":2012},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.968878Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:e2c0669b0e9e9fd4fb222e9d99b0048891a31592ce53f8fc320caa20690cdaa4","observation_id":"7cf5de72-a92e-476c-a4fb-1460115f1767","resolution":{"observed_at":"2026-08-15T21:50:50.018158Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:50.043221Z","title":"The ob- jective was to quantify the time advantage gained by comput- ing values from a pre-calculated cooling table compared to real-time calculations executed by the code","venue":null,"work_id":"6e2797d4-e0bc-4b3f-b32d-67d933bee765","year":2000},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.951267Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:8f93316f953b8f4a6e3aaca066e87e70f2e9e72d23217afd486826fc61a1a7ee","observation_id":"151a2a3b-864e-437d-b0dd-10d6af2d9279","resolution":{"observed_at":"2026-08-15T21:50:50.046849Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:50.033549Z","title":"We also per- form an extra simulation using the standard RAD M1 module implemented in H-AMR","venue":null,"work_id":"7e44b7cb-1fbc-47c0-8dcd-38ec27534a86","year":2000},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.956732Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:b08287217d3e83697c25090241f357752bb3fed006d85e03aa372251da0dd6e2","observation_id":"8ef312a3-f147-4a32-b10e-d4e14590d78e","resolution":{"observed_at":"2026-08-15T21:50:50.037276Z","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":"astro-ph/9705237","last_updated":"1997-06-04T21:01:20Z","snapshot_observed_at":"2026-07-07T01:17:22.474642Z","submitted_at":"1997-05-29T16:22:44Z","title":"Advection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9705237","snapshot_observed_at":"2026-08-15T21:50:48.960430Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.960430Z"},"links":{"cited_paper":"/paper/astro-ph/9705237","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:761de5e51186735d3387024eb78b1c7252462024aa71a9e16e6a29957bdbf703","observation_id":"94656e2b-6df3-4569-914a-2cb747bdf9bf","resolution":{"observed_at":"2026-08-15T21:50:48.960430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:50.024565Z","title":null,"venue":null,"work_id":"57ae303e-c55c-429e-a244-4415a0fc7dfa","year":2006},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.964534Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:06acd50db4f60fb6971bd27d105b03c383db17e81bfefe6b6276660b01b25fc2","observation_id":"217ffb13-0b7f-4817-8e0e-0d0e6656a554","resolution":{"observed_at":"2026-08-15T21:50:50.027715Z","resolver_source":"raw_fallback","status":"unresolved"},"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/9601074","last_updated":"1996-01-12T22:32:37Z","snapshot_observed_at":"2026-08-01T07:25:22.269158Z","submitted_at":"1996-01-12T22:32:37Z","title":"Hot One-Temperature Accretion Flows Around Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9601074","snapshot_observed_at":"2026-08-15T21:50:48.989960Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.989960Z"},"links":{"cited_paper":"/paper/astro-ph/9601074","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:71d602a2e9563e104a2f5ebe36357a5058904ea812c0ec0d9c09c7da489e5da3","observation_id":"8aeb3850-2528-4984-8010-29a3709921f3","resolution":{"observed_at":"2026-08-15T21:50:48.989960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205402","last_updated":"2002-05-23T13:23:28Z","snapshot_observed_at":"2026-08-16T10:45:36.530812Z","submitted_at":"2002-05-23T13:23:28Z","title":"Near-infrared synchrotron emission from the compact jet of GX339-4","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0205402","snapshot_observed_at":"2026-08-15T21:50:48.972671Z","title":"Corbel and R","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.972671Z"},"links":{"cited_paper":"/paper/astro-ph/0205402","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:aa767954eb46e865c0d861c26dd937ec819ef23d3e47ad80e40c92a8bd46f154","observation_id":"994e5d7f-8c05-445a-814c-19e42d6a71f9","resolution":{"observed_at":"2026-08-15T21:50:48.972671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409360","last_updated":"2004-09-15T09:10:32Z","snapshot_observed_at":"2026-08-12T04:06:24.784502Z","submitted_at":"2004-09-15T09:10:32Z","title":"Towards a unified model for black hole X-ray binary jets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409360","snapshot_observed_at":"2026-08-15T21:50:48.976614Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.976614Z"},"links":{"cited_paper":"/paper/astro-ph/0409360","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:ecc2b1f4f2503c6c1d356a8694f952c715a3c97fffe62727731abecc0016d55e","observation_id":"24634190-3215-4f12-8917-54a6434b8e23","resolution":{"observed_at":"2026-08-15T21:50:48.976614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3283","last_updated":"2009-09-17T17:37:25Z","snapshot_observed_at":"2026-08-15T05:38:50.878329Z","submitted_at":"2009-09-17T17:37:25Z","title":"The infrared/X-ray correlation of GX 339-4: Probing hard X-ray emission in accreting black holes","version":1},"cited_work":{"arxiv_id":"0909.3283","doi":null,"metadata_source":"pith","pith_arxiv_id":"0909.3283","snapshot_observed_at":"2026-08-15T21:50:49.649125Z","title":"The infrared/X-ray correlation of GX 339-4: Probing hard X-ray emission in accreting black holes","venue":"astro-ph.HE","work_id":"13866432-f767-4895-80e2-a1be7ce574fa","year":2009},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.981023Z"},"links":{"cited_paper":"/paper/0909.3283","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:ed459dbb2fb9b361e24553bb988d20778732ac3b7304a2662a6916082e637bd3","observation_id":"9ce98fad-1b92-4a7d-b2de-bfa2bb70634a","resolution":{"observed_at":"2026-08-15T21:50:49.654138Z","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":"2026-08-15T21:50:50.004958Z","title":"Coriat, S","venue":null,"work_id":"0c1f8a77-d015-49af-8f60-4fbbff3d8e65","year":2011},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.986366Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:e3fe477bd8490eb03870c77ab17e711cc353bb7bc07fa06510100040f86d56bd","observation_id":"129c5469-a36b-41ba-9be8-254b82d65bf7","resolution":{"observed_at":"2026-08-15T21:50:50.008311Z","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":"1101.2336","last_updated":"2014-03-06T10:37:11Z","snapshot_observed_at":"2026-08-15T04:57:44.925180Z","submitted_at":"2011-01-12T12:11:11Z","title":"A physical model for the continuum variability and QPO in accreting black holes","version":4},"cited_work":{"arxiv_id":"1101.2336","doi":null,"metadata_source":"pith","pith_arxiv_id":"1101.2336","snapshot_observed_at":"2026-08-15T21:50:49.617535Z","title":"A physical model for the continuum variability and QPO in accreting black holes","venue":"astro-ph.SR","work_id":"02e0ec39-271e-41a7-986e-aad5fd1dfcd4","year":2011},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.009457Z"},"links":{"cited_paper":"/paper/1101.2336","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:10c50a60c2d5f80413993a69d0501c3a8fbdc200013a55681093820684b81d5b","observation_id":"634b8d15-211b-4190-b3fa-26ad03cdab9d","resolution":{"observed_at":"2026-08-15T21:50:49.621936Z","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":"1401.0586","last_updated":"2014-01-03T05:17:27Z","snapshot_observed_at":"2026-08-14T23:49:41.645357Z","submitted_at":"2014-01-03T05:17:27Z","title":"Hot Accretion Flows Around Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.0586","snapshot_observed_at":"2026-08-15T21:50:48.993917Z","title":"Yuan and R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.993917Z"},"links":{"cited_paper":"/paper/1401.0586","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:b4951d8d4a3f7e7bcb1cff341e515f5418ccb791658cdcff513f8709140f9b42","observation_id":"f24d95f6-608c-49a0-8cc4-58fb89240e28","resolution":{"observed_at":"2026-08-15T21:50:48.993917Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.995645Z","title":null,"venue":null,"work_id":"d30f5a2a-4311-4abe-afbf-e3432def80f0","year":1973},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.998333Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:1e2693399322d39e40f71768a538bbcf5ba0c006df845b631243b0afe3990ad9","observation_id":"2f5a4f0f-080b-4635-ab5d-f7e52c16456c","resolution":{"observed_at":"2026-08-15T21:50:49.998844Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.985833Z","title":null,"venue":null,"work_id":"771bbf1c-6d88-4dba-ad17-04b450cf0618","year":1973},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.001945Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:6ec95be1427006d076d3eae9fcc3c438d1381b7f3dc8ec19422f238ffd74098d","observation_id":"d8bc1a7d-ef3e-4baa-9a88-f380db1007aa","resolution":{"observed_at":"2026-08-15T21:50:49.989099Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.976190Z","title":null,"venue":null,"work_id":"421b9bab-61cb-4c18-9434-41748f729548","year":2007},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.005625Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:25e7ff55636f1e386a03120a630b78365c3bd427f8cf2049762b713324133c0a","observation_id":"18ef09d3-2531-4e1a-b563-4e7845ed05ce","resolution":{"observed_at":"2026-08-15T21:50:49.979480Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.966272Z","title":"Ferreira, P.-O","venue":null,"work_id":"ed0874a1-6a14-4121-ac9b-99d71e5b9521","year":2006},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.030528Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:c970f081ba1f69b332a2cee2abd9e7002c7ec86ac8722e6932e548855e191f49","observation_id":"9b115e1f-9e76-4291-8753-32a5891faa8c","resolution":{"observed_at":"2026-08-15T21:50:49.969897Z","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":"1404.7498","last_updated":"2014-04-29T20:00:03Z","snapshot_observed_at":"2026-08-14T23:35:50.511166Z","submitted_at":"2014-04-29T20:00:03Z","title":"Revealing accretion onto black holes: X-ray reflection throughout three outbursts of GX 339-4","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.7498","snapshot_observed_at":"2026-08-15T21:50:49.013479Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.013479Z"},"links":{"cited_paper":"/paper/1404.7498","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:11afac50b8cbc772630529c924965184f34e5d4ceb0e61cacaf461721598da22","observation_id":"9b7ba1fa-244c-481c-bd0d-abe96bc7ff39","resolution":{"observed_at":"2026-08-15T21:50:49.013479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.03607","last_updated":"2015-09-28T14:44:39Z","snapshot_observed_at":"2026-08-14T22:48:38.779580Z","submitted_at":"2015-05-14T03:32:16Z","title":"X-ray Reflection Spectroscopy of the Black Hole GX 339-4: Exploring the Hard State with Unprecedented Sensitivity","version":2},"cited_work":{"arxiv_id":"1505.03607","doi":null,"metadata_source":"pith","pith_arxiv_id":"1505.03607","snapshot_observed_at":"2026-08-15T21:50:49.593112Z","title":"X-ray Reflection Spectroscopy of the Black Hole GX 339-4: Exploring the Hard State with Unprecedented Sensitivity","venue":"astro-ph.HE","work_id":"8b924fbe-daf0-4bcf-8caf-798ae3dff86b","year":2015},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.018255Z"},"links":{"cited_paper":"/paper/1505.03607","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:d84a059f15352996283d5ee25d709aec7abc7558162982f71246677d87e5fc34","observation_id":"06f810bf-f7a5-459d-b187-ceefe2c1e38c","resolution":{"observed_at":"2026-08-15T21:50:49.598608Z","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":"1901.03877","last_updated":"2019-01-12T16:44:51Z","snapshot_observed_at":"2026-08-14T17:31:53.135899Z","submitted_at":"2019-01-12T16:44:51Z","title":"The corona contracts in a black-hole transient","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03877","snapshot_observed_at":"2026-08-15T21:50:49.022064Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.022064Z"},"links":{"cited_paper":"/paper/1901.03877","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:75ac2393017818d859709fe43aebcb27f724215edecd40811eb7620ac19f5d0a","observation_id":"dda037c0-24a2-421e-82ed-eca91e8cc360","resolution":{"observed_at":"2026-08-15T21:50:49.022064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.05616","last_updated":"2021-03-09T18:38:46Z","snapshot_observed_at":"2026-08-13T20:00:58.094753Z","submitted_at":"2021-03-09T18:38:46Z","title":"Disk, Corona, Jet Connection in the Intermediate State of MAXI J1820+070 Revealed by NICER Spectral-Timing Analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.05616","snapshot_observed_at":"2026-08-15T21:50:49.025605Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.025605Z"},"links":{"cited_paper":"/paper/2103.05616","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:507475a1fd18241d314ebab1f80a8ac4b4685eedfc37262c350a3c9b1deb47e2","observation_id":"cfee9d60-c56d-4720-ba63-8baed6cae176","resolution":{"observed_at":"2026-08-15T21:50:49.025605Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.05057","last_updated":"2019-05-13T14:35:38Z","snapshot_observed_at":"2026-08-14T16:33:11.964867Z","submitted_at":"2019-05-13T14:35:38Z","title":"A unified accretion-ejection paradigm for black hole X-ray binaries. IV. Replication of the 2010--2011 activity cycle of GX 339-4","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.05057","snapshot_observed_at":"2026-08-15T21:50:49.049846Z","title":"Marcel, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.049846Z"},"links":{"cited_paper":"/paper/1905.05057","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:eeaefbe0ca1e2b8596a5b06b19c0ee159d82c080bc39af4032e15851de407684","observation_id":"f4ae3172-61ac-4222-bb0d-f402597ac306","resolution":{"observed_at":"2026-08-15T21:50:49.049846Z","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":"2026-08-15T21:50:49.034207Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.034207Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:b99304747bbbedd96c44df990218205e42e05e2b3a0241b20d7a7f5a61246774","observation_id":"0a663078-30f8-49a2-a6ca-a57765e08000","resolution":{"observed_at":"2026-08-15T21:50:49.034207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:50.070977Z","title":"Their results showed a truncated cold disk embedded in a hot corona, with the inner radius of the cold disk following rin = 42rg ( ˙m/0.1)−0.60","venue":null,"work_id":"8df35897-749d-4302-a9c3-693bf562397d","year":null},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:48.937995Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:9cd37a18a4798f0835eadd915086ba97e8eb5104ac98d750f822582c7cdb6830","observation_id":"dd8a182a-b91e-49f9-93eb-fbfdd6caf193","resolution":{"observed_at":"2026-08-15T21:50:50.074530Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.951659Z","title":null,"venue":null,"work_id":"1d349b7b-09b3-4e47-875b-c83354a0759e","year":1982},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.038721Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:838b089770567f80b23555874706cec07ed0233b610a9712c536cdb6a2bddf7b","observation_id":"82c85330-9e6d-426b-8624-3f981c6a6dbd","resolution":{"observed_at":"2026-08-15T21:50:49.954882Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.942426Z","title":"Marcel, J","venue":null,"work_id":"8434fd7e-3e76-4896-b2bd-d0e1de99c155","year":2018},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.042640Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:8b05d0e07a6edf82ffba8474737aa1df6498e5f5e9e380b42a0a534cd486530c","observation_id":"43938dcc-9406-450a-99b0-10009617611f","resolution":{"observed_at":"2026-08-15T21:50:49.945704Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.933746Z","title":"Marcel, J","venue":null,"work_id":"17218857-b0cb-4102-a7a6-20be46dff765","year":2018},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.046559Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:e4b0fdeb920bc787b77b472cf4f34387aa20c55c8af9ec806f9f4909295f59db","observation_id":"f026d176-b212-42f1-8769-86359c2dd7e0","resolution":{"observed_at":"2026-08-15T21:50:49.936780Z","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":"2101.08839","last_updated":"2021-01-21T20:23:54Z","snapshot_observed_at":"2026-07-06T10:34:29.894974Z","submitted_at":"2021-01-21T20:23:54Z","title":"Magnetohydrodynamic Simulations of Active Galactic Nucleus Disks and Jets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08839","snapshot_observed_at":"2026-08-15T21:50:49.054545Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.054545Z"},"links":{"cited_paper":"/paper/2101.08839","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:244dbb646cbe077632cdcc043841ff7357e231c15e10df5cbab25420da7af3e7","observation_id":"a04a7efa-8d3f-42a7-a668-56207b39ffa5","resolution":{"observed_at":"2026-08-15T21:50:49.054545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.11429","last_updated":"2024-04-25T20:23:07Z","snapshot_observed_at":"2026-08-16T15:31:48.814000Z","submitted_at":"2023-05-19T04:57:55Z","title":"Emergence of hot corona and truncated disk in simulations of accreting stellar mass black holes","version":2},"cited_work":{"arxiv_id":"2305.11429","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.11429","snapshot_observed_at":"2026-08-15T21:50:49.543815Z","title":"Emergence of hot corona and truncated disk in simulations of accreting stellar mass black holes","venue":"astro-ph.HE","work_id":"221ddadb-bab3-4699-80e2-783cf1f8fb83","year":2023},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.059578Z"},"links":{"cited_paper":"/paper/2305.11429","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:2e6d218f56cf6f34a77fca4fa28a40735389fd0060898e27302b02f866710a0c","observation_id":"588d0ab4-5ace-4195-b47b-11e4cec3825d","resolution":{"observed_at":"2026-08-15T21:50:49.548974Z","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":"2026-08-15T21:50:49.063347Z","title":"Narayan, I","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.063347Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:6b8a6649439b90afcdd4dd017d2ff259e5f7dcf332cf3c35909edb949929a468","observation_id":"8464f87d-2a11-43e7-a36b-192473802fee","resolution":{"observed_at":"2026-08-15T21:50:49.063347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0301402","last_updated":"2003-04-09T16:31:51Z","snapshot_observed_at":"2026-08-11T20:53:52.571215Z","submitted_at":"2003-01-21T00:07:08Z","title":"Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0301402","snapshot_observed_at":"2026-08-15T21:50:49.067074Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.067074Z"},"links":{"cited_paper":"/paper/astro-ph/0301402","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:ffd8065c964e70ff1b3ccbf3e78b3841c135390ec70d87d96c84c6a705ac57e0","observation_id":"150882b6-ca83-4c70-8e73-35671346e931","resolution":{"observed_at":"2026-08-15T21:50:49.067074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.924955Z","title":"Tchekhovskoy, R","venue":null,"work_id":"6bc21258-803a-4de5-81ab-ce13e9882749","year":2011},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.072192Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:542c5ecc84c003a99a483fb205bf13465934a4560cb1f52f8060d95de17c2ebe","observation_id":"d216a8a7-ffd8-43c9-9508-257886f200a3","resolution":{"observed_at":"2026-08-15T21:50:49.928032Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.915804Z","title":"Tchekhovskoy and D","venue":null,"work_id":"8a010230-a9e8-44f4-a0ab-7357843c3806","year":2015},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.076090Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:4f18d125788ac30adf288db9c0cc724521980ed49d7389f64746dea33c987b6c","observation_id":"183973ac-9a52-42ce-b855-013d37206fce","resolution":{"observed_at":"2026-08-15T21:50:49.918833Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.906790Z","title":"Jacquemin-Ide, G","venue":null,"work_id":"0e56604b-a430-4abb-bafc-96f0fe7587e1","year":2021},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.079782Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:e065ba7af99a2d7dabaacef0e6f7500f90670d6151254ddff74782c9ae1b7e43","observation_id":"e13a4695-afb1-4e6d-be69-652f14023c70","resolution":{"observed_at":"2026-08-15T21:50:49.909970Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.897521Z","title":"Liska, A","venue":null,"work_id":"b57fa34a-f2b2-439b-b8e1-21fffedc8518","year":2020},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.084220Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:569d98beaa2812369d5f0574099443d334cf6969befe61be4f8df1dbf9e8827b","observation_id":"bdc591d8-8d12-4544-a29f-658d9ece84fe","resolution":{"observed_at":"2026-08-15T21:50:49.901045Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.888803Z","title":"Jacquemin-Ide, F","venue":null,"work_id":"e6feb2f0-0719-42fc-bba4-285217b6df24","year":2024},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.088639Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:32a7304cb6645eb4833f17d0eb96e71e5a81504087695f690dafcfe6cf4ea2c3","observation_id":"8f42f54a-d529-42df-b0ac-309112087d33","resolution":{"observed_at":"2026-08-15T21:50:49.891751Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.880127Z","title":null,"venue":null,"work_id":"49c3663a-c73d-4462-86d6-a1eaf8268db0","year":2016},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.092266Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:b4993a8404f435a59b55a402104b35b44f897d03efafffba03ddf96bf1dae7d2","observation_id":"c51a4a58-be47-47c2-9527-be67dacc8499","resolution":{"observed_at":"2026-08-15T21:50:49.883177Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.871045Z","title":"Dexter, N","venue":null,"work_id":"6b63fcc9-304a-420d-b0df-17fbb3fa0caa","year":2021},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.100758Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:edfb709326867c95aeeaef755652591ecbf388629b32d4dc28590d455fcc7440","observation_id":"602e2c49-0ff6-4a62-afd8-717c231a9f35","resolution":{"observed_at":"2026-08-15T21:50:49.874134Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.862447Z","title":"Hankla and J","venue":null,"work_id":"7103751c-fa62-4ca2-b36a-c5c40ffb4991","year":2025},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.104683Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:7c27ce472a75617a5d809988518b562dfe41bf7a6cd5a34d6d6ea7f333f02820","observation_id":"9381a1e9-7466-4435-bd5b-bb207bd751e6","resolution":{"observed_at":"2026-08-15T21:50:49.865450Z","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":"astro-ph/9411059","last_updated":"1995-07-29T21:47:14Z","snapshot_observed_at":"2026-08-06T11:34:53.714240Z","submitted_at":"1994-11-15T23:54:11Z","title":"Advection-Dominated Accretion: Underfed Black Holes and Neutron Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9411059","snapshot_observed_at":"2026-08-15T21:50:49.108313Z","title":"Narayan and I","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.108313Z"},"links":{"cited_paper":"/paper/astro-ph/9411059","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:cf3d5fa2d31b29f2421ac0e047ab74fda6d0003466e001643d7733291dea7ccb","observation_id":"f71ba5f4-1145-4d64-8aa4-2183bb631c86","resolution":{"observed_at":"2026-08-15T21:50:49.108313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.853662Z","title":null,"venue":null,"work_id":"c27fe3d6-076a-4e99-aef5-c7dbb2fe7ca4","year":2022},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.113100Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:581eb2182c259a46fb7c32c9cf132a34b595317b6b1cc92f97653daad00e7b88","observation_id":"f1901e37-13f1-4c69-86f3-2ffb3cc0033a","resolution":{"observed_at":"2026-08-15T21:50:49.856752Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2201.03526","last_updated":"2022-08-09T22:19:37Z","snapshot_observed_at":"2026-08-11T21:10:34.021865Z","submitted_at":"2022-01-10T18:37:31Z","title":"Formation of Magnetically Truncated Accretion Disks in 3D Radiation-Transport Two-Temperature GRMHD Simulations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.03526","snapshot_observed_at":"2026-08-15T21:50:49.116694Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.116694Z"},"links":{"cited_paper":"/paper/2201.03526","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:c11e4bc7d8b303f37886e5510cc4f84abb86111bb454f7f6a3d805ce85224de1","observation_id":"f063edc8-9405-4bb0-a6d8-0c9bc99bff28","resolution":{"observed_at":"2026-08-15T21:50:49.116694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.844527Z","title":null,"venue":null,"work_id":"29793863-6fae-4e3b-8782-d34fd6c6a1fd","year":2015},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.120190Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:ef6b21536f3f4719117eeb08d98c8d6155c9fcb718bb53616aedb960d0ce92af","observation_id":"7080b97f-559f-4db5-af6f-26eaa42f2a80","resolution":{"observed_at":"2026-08-15T21:50:49.847684Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.835910Z","title":null,"venue":null,"work_id":"2278540b-1c08-4a2e-8d3e-dd59d99c2a43","year":1970},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.123750Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:5accdf2774dca9a02b9bde62d69011fd9e30f5973d2bc3510e4ed6b36c2488ad","observation_id":"09a87e5f-a714-48a4-bb88-0b627b5b7803","resolution":{"observed_at":"2026-08-15T21:50:49.838877Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"ph/9601073","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.444629Z","title":"Mahadevan, R","venue":null,"work_id":"7b131299-f499-4684-879d-50ddb28885d5","year":1996},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.127281Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:29da027604e87c635d4c9dea5eefaa081cd03aba489fefaa8168f4ec31724142","observation_id":"21eb5650-5f8f-47a1-a55e-6a46a3a42b1e","resolution":{"observed_at":"2026-08-15T21:50:49.450000Z","resolver_source":"raw_fallback","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":"0810.1082","last_updated":"2008-10-07T01:52:43Z","snapshot_observed_at":"2026-08-15T10:05:02.051049Z","submitted_at":"2008-10-07T01:52:43Z","title":"General Relativistic Magnetohydrodynamic Simulations of the Hard State as a Magnetically-Dominated Accretion Flow","version":1},"cited_work":{"arxiv_id":"0810.1082","doi":null,"metadata_source":"pith","pith_arxiv_id":"0810.1082","snapshot_observed_at":"2026-08-15T21:50:49.378414Z","title":"General Relativistic Magnetohydrodynamic Simulations of the Hard State as a Magnetically-Dominated Accretion Flow","venue":"astro-ph","work_id":"e855251b-4283-4ea9-88ba-8a1ae3a3c12e","year":2008},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.130793Z"},"links":{"cited_paper":"/paper/0810.1082","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:d5220e52010dcd58cb4696ccb0be941fba3f720ec729c917957dedb87ea8a283","observation_id":"cc08dd64-d89d-469d-a137-956cf8c73ccc","resolution":{"observed_at":"2026-08-15T21:50:49.383329Z","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":"2026-08-15T21:50:49.826920Z","title":null,"venue":null,"work_id":"0ff31093-924a-41a7-9fb7-4d29f50afad7","year":1991},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.134611Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:fc9423d54bb1e99bfc7ef8f898fce7ba41188cbb326eb5d3f53b8517ccc70c3d","observation_id":"0ce1d264-2464-4435-9bd9-326d111a7e10","resolution":{"observed_at":"2026-08-15T21:50:49.830259Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.817708Z","title":"Hubeny, Vertical Structure of Accretion Disks: A Simplified Analytical Model, Astrophys","venue":null,"work_id":"195220ce-b7af-4aca-8cea-ec3b9e69eeeb","year":1990},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.138287Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:88b80af43daff6ba1a90a72fb350dba90c0120424c6975f02e1deb3e8b58429e","observation_id":"8d2fd543-eeb7-4157-8377-443c29ed69fe","resolution":{"observed_at":"2026-08-15T21:50:49.821218Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.809048Z","title":"Sadowski, M","venue":null,"work_id":"17019825-ad76-4abb-a493-30f806d4fe4e","year":2016},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.142101Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:8c4ffa0c454ce01d6e224038919468558aa02bd4c879efdc932f19597733ed8e","observation_id":"baac3de7-1e0e-47dd-8bc3-e3841dff000b","resolution":{"observed_at":"2026-08-15T21:50:49.812103Z","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":"1607.01788","last_updated":"2016-09-22T19:59:48Z","snapshot_observed_at":"2026-08-14T21:49:30.737500Z","submitted_at":"2016-07-06T20:00:03Z","title":"Hydrodynamical Coupling of Mass and Momentum in Multiphase Galactic Winds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.01788","snapshot_observed_at":"2026-08-15T21:50:49.145609Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.145609Z"},"links":{"cited_paper":"/paper/1607.01788","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:89e8f8239cbfb43528d19db529d21a0c80be687c593c61fc1fae51cbdc1c6559","observation_id":"6d293adb-7851-4bac-aac0-7e2a42523291","resolution":{"observed_at":"2026-08-15T21:50:49.145609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.4194","last_updated":"2015-03-06T23:18:58Z","snapshot_observed_at":"2026-08-14T23:15:34.129531Z","submitted_at":"2014-10-15T20:00:05Z","title":"Cholla : A New Massively-Parallel Hydrodynamics Code For Astrophysical Simulation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.4194","snapshot_observed_at":"2026-08-15T21:50:49.149412Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.149412Z"},"links":{"cited_paper":"/paper/1410.4194","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:4bcd5c4381e51b084437b7fd5faacef4c47ecf86ae0c2600c1c7994308b054c4","observation_id":"ab7067a8-4b3f-4806-9eb0-4014c1da467a","resolution":{"observed_at":"2026-08-15T21:50:49.149412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.799314Z","title":null,"venue":null,"work_id":"90b33610-70e2-4cdd-a373-0220051ba788","year":2014},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.153604Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:9ace8d6f35e0e62a13677f4a0620409fe1435ebb494dbc95c28c665c5c7e496a","observation_id":"9982d941-de0c-41b8-9300-84dc88d53638","resolution":{"observed_at":"2026-08-15T21:50:49.802417Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.790170Z","title":null,"venue":null,"work_id":"a39227a0-a1a6-4aef-80e1-9d93f7a28558","year":1976},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.157222Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:6e562d09d2daa23be8c7b0bb85aa1c4a8526d5cfc14b64a63deb85f65cda24d4","observation_id":"f72ab671-6759-43c2-b3cc-7c0e3aebae5f","resolution":{"observed_at":"2026-08-15T21:50:49.793324Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.781046Z","title":"Jiang, J","venue":null,"work_id":"9b7aa3c2-8216-435d-b1ad-aaed48ac4a1a","year":2013},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.161342Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:1ac304b00095e6e8847d423ba95e91f428905962b904626a844f05b8cd522d8e","observation_id":"6cbfe15c-1652-4fd7-9ab6-49386f875c74","resolution":{"observed_at":"2026-08-15T21:50:49.784190Z","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":"0808.3140","last_updated":"2008-08-22T20:03:07Z","snapshot_observed_at":"2026-08-15T10:08:24.373733Z","submitted_at":"2008-08-22T20:03:07Z","title":"Direct calculation of the radiative efficiency of an accretion disk around a black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3140","snapshot_observed_at":"2026-08-15T21:50:49.164942Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.164942Z"},"links":{"cited_paper":"/paper/0808.3140","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:f555a68c8ecc18eb2476381a7083eb2d2fa272ce43b495c33833d9c6eefdb58d","observation_id":"e81c2ecc-f08d-474e-a306-0c692411d1bd","resolution":{"observed_at":"2026-08-15T21:50:49.164942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.771827Z","title":null,"venue":null,"work_id":"605c4b4d-cd78-49d3-b74e-84bc4d09c1b0","year":1976},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.168522Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:5d55edde1bd92b48a4fd619148845b647f976e3fda670a5921bf1e335fdfa939","observation_id":"dc9dbe58-dea2-45b3-a453-a9ff3e83e8bc","resolution":{"observed_at":"2026-08-15T21:50:49.774934Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2309.15926","last_updated":"2024-03-27T15:25:15Z","snapshot_observed_at":"2026-08-16T14:57:05.747329Z","submitted_at":"2023-09-27T18:05:02Z","title":"Magnetic flux plays an important role during a BHXRB outburst in radiative 2T GRMHD simulations","version":2},"cited_work":{"arxiv_id":"2309.15926","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.15926","snapshot_observed_at":"2026-08-15T21:50:49.337664Z","title":"Magnetic flux plays an important role during a BHXRB outburst in radiative 2T GRMHD simulations","venue":"astro-ph.HE","work_id":"029bda68-9929-4c3c-a176-13a8cb07ea10","year":2023},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.173654Z"},"links":{"cited_paper":"/paper/2309.15926","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:eae657a89a1c0507d8cac5398072bfa7b3379400417a517dc13306b1c4ab41ea","observation_id":"5f5df0c4-899b-41b4-bc25-836fd06446ce","resolution":{"observed_at":"2026-08-15T21:50:49.342798Z","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":"2026-08-15T21:50:49.762803Z","title":null,"venue":null,"work_id":"12acd111-3ad0-4bd1-8552-8c9800cb86bd","year":2025},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.177579Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:e08c94082c1b87a58d48e40678eba6a393e4679ed1980c03c05f7ac25adeb492","observation_id":"4b8e803d-57e5-433a-aa92-fb87bfdfca49","resolution":{"observed_at":"2026-08-15T21:50:49.765857Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.753432Z","title":"Scepi, M","venue":null,"work_id":"9ffd514f-0ebb-437b-b37a-e985cb2a2f49","year":2023},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.181007Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:72a16802babe7d6fe37d73f9abb9605eb3c6c2a751bf98358b862cd8b9a3c8dd","observation_id":"a44f489e-55b9-465d-9fec-88ff696de09e","resolution":{"observed_at":"2026-08-15T21:50:49.756594Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.741793Z","title":"Lowell, J","venue":null,"work_id":"118dce5e-536d-487f-9938-21e60b024156","year":2025},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.186061Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:94958eebe7b4df6490398daaff85e36a4b0b125450a9fb544a8fefe55e9bed8d","observation_id":"49969f0b-1880-4228-ac3e-c7d6e9b5297a","resolution":{"observed_at":"2026-08-15T21:50:49.746005Z","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":"1206.1213","last_updated":"2012-09-03T14:06:10Z","snapshot_observed_at":"2026-08-15T00:57:44.969552Z","submitted_at":"2012-06-06T13:17:44Z","title":"GRMHD Simulations of Magnetized Advection Dominated Accretion on a Non-Spinning Black Hole: Role of Outflows","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.1213","snapshot_observed_at":"2026-08-15T21:50:49.189893Z","title":"Narayan, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.189893Z"},"links":{"cited_paper":"/paper/1206.1213","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:2351242fec523d5087e081f89ceb45437d2007a8a82535e6bf1a381d8b0aca61","observation_id":"0e464949-2c84-48c6-8245-587ca8569415","resolution":{"observed_at":"2026-08-15T21:50:49.189893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.730518Z","title":"Chen and J","venue":null,"work_id":"76e01414-5fa0-4f02-8659-dba09abb7fcc","year":1989},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.193770Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:d59b46d23636cfed538b4db36b136da14333afda1a99c9502d30c373cda68830","observation_id":"efbbe1a6-e614-459e-9a8a-bb3e87273fea","resolution":{"observed_at":"2026-08-15T21:50:49.734678Z","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":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/asna.20230020","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T11:08:47.750906Z","title":"Barnier, P.-O","venue":"Astronomische Nachrichten","work_id":"812f4f39-d063-477d-b3b7-6ba13ce98c4f","year":2023},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.197832Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:a3a2194693a00c8e6ca0a2d1e9e7b464db067423a8ec1e708fe3d6909f3b6fba","observation_id":"72a3fa5e-8f4b-4a79-8392-b6996a8cdb06","resolution":{"observed_at":"2026-08-15T21:50:49.267201Z","resolver_source":"doi","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":"1508.05323","last_updated":"2016-02-12T23:42:21Z","snapshot_observed_at":"2026-08-14T22:35:41.207670Z","submitted_at":"2015-08-21T16:04:39Z","title":"Efficiency of Thin Magnetically-Arrested Disks Around Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.05323","snapshot_observed_at":"2026-08-15T21:50:49.201688Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.201688Z"},"links":{"cited_paper":"/paper/1508.05323","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:cbedd2a6706d95de7647f7b9f61381cee3b8545630d138e7da79f056a028b55b","observation_id":"8484e060-252b-4bb7-b121-fdf0b035739c","resolution":{"observed_at":"2026-08-15T21:50:49.201688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.09698","last_updated":"2025-01-06T11:10:30Z","snapshot_observed_at":"2026-08-16T15:32:46.529070Z","submitted_at":"2023-05-16T06:54:37Z","title":"Impact of radiative cooling on the magnetised geometrically thin accretion disk around Kerr black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.09698","snapshot_observed_at":"2026-08-15T21:50:49.206215Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.206215Z"},"links":{"cited_paper":"/paper/2305.09698","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:5dce0e6a77e333ff5dfafe4360a1539697af4849a32e969d87794e87c51046be","observation_id":"ff786620-14f1-439a-b53a-12de00b9235b","resolution":{"observed_at":"2026-08-15T21:50:49.206215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.4581","last_updated":"2013-09-18T09:00:24Z","snapshot_observed_at":"2026-08-15T00:02:46.773151Z","submitted_at":"2013-09-18T09:00:24Z","title":"Average spectral properties of galactic X-ray binaries with 3 years of MAXI data","version":1},"cited_work":{"arxiv_id":"1309.4581","doi":null,"metadata_source":"pith","pith_arxiv_id":"1309.4581","snapshot_observed_at":"2026-08-15T21:50:49.295179Z","title":"Average spectral properties of galactic X-ray binaries with 3 years of MAXI data","venue":"astro-ph.HE","work_id":"64ebea01-f4c2-453a-801f-97bb6643bfa5","year":2013},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.210240Z"},"links":{"cited_paper":"/paper/1309.4581","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:6801f561e2afdbbeec97629f29a34fda18b32f5088cf8d03c4427346cfa1b895","observation_id":"2209ea8f-b9de-48f8-b412-4b80ed53a430","resolution":{"observed_at":"2026-08-15T21:50:49.300944Z","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":"2026-08-15T21:50:49.719443Z","title":"Carotenuto, S","venue":null,"work_id":"2285ad33-b7f7-4ea3-912c-2144d2d01947","year":2021},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.213964Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:9bee4b896e996c37f78596c5b92678b0857160d0fe42ca83f2ca065cbb8e5d7d","observation_id":"76a8508d-c7e8-48eb-8118-bcfcfbe3c106","resolution":{"observed_at":"2026-08-15T21:50:49.723602Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.708894Z","title":null,"venue":null,"work_id":"9d4c5057-31a5-449d-8b76-18f57779cf64","year":1973},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.217576Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:a9e57248739cfeac107ea0564f56ea6c11087429115a406e9c9f77ea6e12c570","observation_id":"c7940e34-8a53-4d0b-bc48-3d7baa55c0f5","resolution":{"observed_at":"2026-08-15T21:50:49.712663Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-15T21:50:49.698054Z","title":"Sadowski, R","venue":null,"work_id":"48f81d49-4ba1-4e7c-8492-f7ce816d1443","year":2013},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.221256Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:15466cfbfd5000eec1e43d61fb56f8c8c104e9cfb620c4c8506d4835e598ea86","observation_id":"41310697-b030-4dfe-a1d2-12725202f0a5","resolution":{"observed_at":"2026-08-15T21:50:49.701967Z","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":"1311.5900","last_updated":"2013-11-22T21:06:28Z","snapshot_observed_at":"2026-08-14T23:54:14.612510Z","submitted_at":"2013-11-22T21:06:28Z","title":"Numerical simulations of super-critical black hole accretion flows in general relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.5900","snapshot_observed_at":"2026-08-15T21:50:49.226405Z","title":"Sadowski, R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.226405Z"},"links":{"cited_paper":"/paper/1311.5900","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:98448f30d0c1cc8034cbf07ca2c54e759dfbbfb886d51d292c9fb4a8d40760b6","observation_id":"10a7973b-c0e5-4b0b-9100-8e01cdbb7c7e","resolution":{"observed_at":"2026-08-15T21:50:49.226405Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.6127","last_updated":"2013-12-20T21:00:10Z","snapshot_observed_at":"2026-08-14T23:50:45.106636Z","submitted_at":"2013-12-20T21:00:10Z","title":"Three-Dimensional General Relativistic Radiation Magnetohydrodynamical Simulation of Super-Eddington Accretion, using a new code HARMRAD with M1 Closure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.6127","snapshot_observed_at":"2026-08-15T21:50:49.230288Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.230288Z"},"links":{"cited_paper":"/paper/1312.6127","citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:3db9c81e0e5bf83b20c3249c91603e0f309683c1b84235b53b0640bc2aced327","observation_id":"1481c452-7e27-4186-8a2b-b5536eabc182","resolution":{"observed_at":"2026-08-15T21:50:49.230288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:50:49.686442Z","title":null,"venue":null,"work_id":"be339b6a-22a1-4ee5-af6a-89e3c40a21f0","year":2011},"citing_paper":{"arxiv_id":"2505.08855","last_updated":"2025-05-13T18:00:00Z","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-15T21:50:49.234264Z"},"links":{"citing_paper":"/paper/2505.08855"},"observation_digest":"sha256:b5d3a3decc977cc93659d84277814ab17cb755b8b2827d6e6afc50f31e00cf3e","observation_id":"d21d5945-3581-45ea-8251-1765107fecb9","resolution":{"observed_at":"2026-08-15T21:50:49.690756Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2505.08855","last_updated":"2025-05-13T18:00:00Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-15T21:44:03.709885Z","submitted_at":"2025-05-13T18:00:00Z","title":"Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling"},"reference_resolution":{"displayed":73,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":39,"verified_exact":9,"verified_fuzzy":25},"total_outbound_references":73},"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 73 of 73 outbound references and 3 inbound Pith citation observations for arXiv:2505.08855."}