{"as_of":"2026-08-16T10:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c1ff719edfc22aac40d292372b48bf2aecfe2dfdeec51abae9168bc430bab122","coverage":[{"denominator":68,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":68,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:41:37.710758Z","state":"measured"},{"denominator":68,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":68,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.09355/citation-record","integrity":"/paper/2505.09355/integrity","json":"/paper/2505.09355/citation-record.json","paper":"/paper/2505.09355"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:41:38.962876Z","title":"Fender, in Compact stellar X-ray sources , Vol","venue":null,"work_id":"ac1c7b72-28eb-4a00-b13c-d36547ad4f52","year":2006},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.402281Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:400b8d69e262194f22db0223763c4871c320993ca6d439904c4de646432b2410","observation_id":"30ea4649-eb01-481d-9068-92a114152e7f","resolution":{"observed_at":"2026-08-15T21:41:38.967779Z","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":"1106.2059","last_updated":"2011-06-10T13:59:09Z","snapshot_observed_at":"2026-08-15T04:44:14.019928Z","submitted_at":"2011-06-10T13:59:09Z","title":"Multifrequency Behavior of Microquasars in the GeV--TeV era: A review","version":1},"cited_work":{"arxiv_id":"1106.2059","doi":null,"metadata_source":"pith","pith_arxiv_id":"1106.2059","snapshot_observed_at":"2026-08-15T21:41:38.561557Z","title":"Multifrequency Behavior of Microquasars in the GeV--TeV era: A review","venue":"astro-ph.HE","work_id":"6d2f5a65-ec9d-487c-9a31-f965c399fe48","year":2011},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.408689Z"},"links":{"cited_paper":"/paper/1106.2059","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:c20789e5f89efe2051d6913f55763d71e3f65bb3fc600f746dcbcf5f4e6e70ba","observation_id":"babd34db-c938-41c3-9e2d-844979839e93","resolution":{"observed_at":"2026-08-15T21:41:38.566619Z","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":"1104.5499","last_updated":"2013-01-21T13:58:08Z","snapshot_observed_at":"2026-08-15T04:48:10.538900Z","submitted_at":"2011-04-28T20:00:20Z","title":"Foundations of Black Hole Accretion Disk Theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.5499","snapshot_observed_at":"2026-08-15T21:41:37.414544Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.414544Z"},"links":{"cited_paper":"/paper/1104.5499","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:68877b839b91578e4d41fe879b2484a9adb12bcf2a2a05c7e8dec8b6698b28e5","observation_id":"59d96417-a3f7-40d9-9368-7f72e875f32f","resolution":{"observed_at":"2026-08-15T21:41:37.414544Z","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":"2026-08-15T21:41:38.948905Z","title":null,"venue":null,"work_id":"7116cbf8-ae5a-4888-ab76-767d15fa0400","year":2014},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.419453Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:b88bcce13e71f70fbfa7441976fe57a8fbcf96830acd6fe3d0e1a656719a7d64","observation_id":"75a2ca59-011e-4767-88d1-d3bf9113dc0c","resolution":{"observed_at":"2026-08-15T21:41:38.953100Z","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":"2026-08-15T21:41:38.934131Z","title":null,"venue":null,"work_id":"7f123522-2a7a-4b68-b3e2-0a7f213f9393","year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.424180Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:3664f7b9307c8d31384c194542b0ca97c526562e2c6c72c214c1f781f2cd7425","observation_id":"f0e70013-367c-41d7-9bbc-a3028a5ed3d7","resolution":{"observed_at":"2026-08-15T21:41:38.938688Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:41:37.429087Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.429087Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:a78c66633607a0e9153fcf67c8704ef1fc04c940f5cf6ea82cea6780d7e0246e","observation_id":"513f5c2e-13fb-48bf-8e23-c8460255a419","resolution":{"observed_at":"2026-08-15T21:41:37.429087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-15T21:41:37.434269Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.434269Z"},"links":{"cited_paper":"/paper/2101.08839","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:b101ddd0f659872a3bfee0ffd4dd3d1c7965778a0b7478bc19ce838b1bf6074d","observation_id":"7ba2fab1-5b77-4d54-a3ae-e57ae2a6f508","resolution":{"observed_at":"2026-08-15T21:41:37.434269Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.00870","last_updated":"2020-04-02T08:34:58Z","snapshot_observed_at":"2026-08-03T23:33:38.436902Z","submitted_at":"2020-04-02T08:34:58Z","title":"GRMHD large eddy simulations with gradient subgrid-scale model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.00870","snapshot_observed_at":"2026-08-15T21:41:37.439129Z","title":"Vigan` o, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.439129Z"},"links":{"cited_paper":"/paper/2004.00870","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:79116822f348a65522c4b74a84fedc770ddec4596cf22c0d7b2b5303b4194b2b","observation_id":"3b288395-4b76-4212-8366-cd39bc81fff8","resolution":{"observed_at":"2026-08-15T21:41:37.439129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.01021","last_updated":"2015-02-03T21:00:12Z","snapshot_observed_at":"2026-08-14T23:01:30.729203Z","submitted_at":"2015-02-03T21:00:12Z","title":"Relativistic Jets Shine through Shocks or Magnetic Reconnection?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01021","snapshot_observed_at":"2026-08-15T21:41:37.443678Z","title":"Sironi, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.443678Z"},"links":{"cited_paper":"/paper/1502.01021","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:7177dedfca6b72d56599959488cdcd709a4ef35a1bc6aed48c3a795ffd2ddb58","observation_id":"cc2ffe41-a4ed-4a0f-b9bb-d00f97273d10","resolution":{"observed_at":"2026-08-15T21:41:37.443678Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-15T21:41:37.448337Z","title":"Yuan and R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.448337Z"},"links":{"cited_paper":"/paper/1401.0586","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:b76865444e33ba7fbc2318f8824db00bb3f5d4f53574be800790600add319f6b","observation_id":"dcfc262d-0e15-4449-a807-ce6933845da8","resolution":{"observed_at":"2026-08-15T21:41:37.448337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.06587","last_updated":"2020-03-14T09:37:17Z","snapshot_observed_at":"2026-08-13T17:21:34.460869Z","submitted_at":"2020-03-14T09:37:17Z","title":"Particle acceleration in astrophysical jets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.06587","snapshot_observed_at":"2026-08-15T21:41:37.453177Z","title":"Matthews, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.453177Z"},"links":{"cited_paper":"/paper/2003.06587","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:14400aa48d7850144ee26575dee2d783ef3a78178e0a252460ccefa101c67aeb","observation_id":"33e0f18f-832d-4112-80ee-e38b06dcace4","resolution":{"observed_at":"2026-08-15T21:41:37.453177Z","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":"2026-08-15T21:41:38.919238Z","title":"Brandenburg, A","venue":null,"work_id":"8c8e1ea5-9958-454b-b331-0760dc54fbf6","year":1995},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.457803Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:81ce70ee4680cc883a2d80c5d4a297c4a90c0f3234ca4469aa683f2a129acff1","observation_id":"5567a00d-283c-4066-9af9-65af423d5386","resolution":{"observed_at":"2026-08-15T21:41:38.923804Z","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":"0906.2784","last_updated":"2009-10-15T22:33:13Z","snapshot_observed_at":"2026-08-15T05:46:08.771695Z","submitted_at":"2009-06-15T20:18:46Z","title":"Transport of Large Scale Poloidal Flux in Black Hole Accretion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.2784","snapshot_observed_at":"2026-08-15T21:41:37.461813Z","title":"Beckwith, J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.461813Z"},"links":{"cited_paper":"/paper/0906.2784","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:4dec69c2a93b1fe4f2672b757c22230f084643e7e55e24bb6794376a50e034e2","observation_id":"695e53bd-4334-4c9c-8803-0610631938fc","resolution":{"observed_at":"2026-08-15T21:41:37.461813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0412","last_updated":"2011-08-30T10:39:40Z","snapshot_observed_at":"2026-08-15T04:39:21.658469Z","submitted_at":"2011-08-01T20:00:01Z","title":"Efficient Generation of Jets from Magnetically Arrested Accretion on a Rapidly Spinning Black Hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.0412","snapshot_observed_at":"2026-08-15T21:41:37.466087Z","title":"Tchekhovskoy, R","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.466087Z"},"links":{"cited_paper":"/paper/1108.0412","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:df928f0c594e2798cb23dbabe94c756ee14ebf346e270b9c14d5a9798a5b4b7b","observation_id":"0e3dbff5-ee3f-4aac-9bca-e1a449a09a50","resolution":{"observed_at":"2026-08-15T21:41:37.466087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11238","last_updated":"2019-06-26T18:06:46Z","snapshot_observed_at":"2026-08-13T13:53:05.353909Z","submitted_at":"2019-06-26T18:06:46Z","title":"First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11238","snapshot_observed_at":"2026-08-15T21:41:37.470214Z","title":"Akiyama et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.470214Z"},"links":{"cited_paper":"/paper/1906.11238","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:41a66d987a90fbc1367fd32e42e40b436bf04182b4fa03b798431f3e0b22ca27","observation_id":"f9d1a0ec-0441-4ebf-a9f9-517c7771e36e","resolution":{"observed_at":"2026-08-15T21:41:37.470214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.04923","last_updated":"2019-08-05T19:18:38Z","snapshot_observed_at":"2026-08-14T16:48:59.934839Z","submitted_at":"2019-04-09T21:45:17Z","title":"The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.04923","snapshot_observed_at":"2026-08-15T21:41:37.474359Z","title":"Porth et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.474359Z"},"links":{"cited_paper":"/paper/1904.04923","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:16561d5663966c0df147414bb625bd2d16102bb31417a29b1fccce38ca99ce2b","observation_id":"b0621887-fdb3-4d92-92f0-928ee8bbf42d","resolution":{"observed_at":"2026-08-15T21:41:37.474359Z","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":"2026-08-15T21:41:38.902451Z","title":"Chandrasekhar, Hydrodynamic and Hydromagnetic Stability, International Series of Mono- graphs on Physics (Oxford, Clarendon Press, 1961)","venue":null,"work_id":"dcaef54e-1729-4680-ad6c-a3b87a32f565","year":1961},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.478387Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:bda755b147d6734933a190e2804fa4d433d6bc99ffbb38b8fb2a344237898bf8","observation_id":"63d5c819-888f-491c-b1ca-093fc1945619","resolution":{"observed_at":"2026-08-15T21:41:38.908294Z","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":"1904.09677","last_updated":"2019-04-23T02:52:02Z","snapshot_observed_at":"2026-08-14T16:43:25.000567Z","submitted_at":"2019-04-21T23:20:41Z","title":"Magnetic Fields in Accretion Disks: A Review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.09677","snapshot_observed_at":"2026-08-15T21:41:37.482989Z","title":"Jafari, (2019), arXiv:1904.09677 [astro-ph.HE]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.482989Z"},"links":{"cited_paper":"/paper/1904.09677","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:cb17792fa02fa0af74daaf6cc2226455fb97d0a0476d31a297f9396303814f0a","observation_id":"22684c01-2e8c-4521-918d-635902f567b0","resolution":{"observed_at":"2026-08-15T21:41:37.482989Z","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":"2026-08-15T21:41:37.487840Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.487840Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:0a7088621576307c2713457f9370c6e543f1f0121eacd0c705c390aca275ea70","observation_id":"349d2ed1-b2f0-4cde-b4f7-34d1042c386c","resolution":{"observed_at":"2026-08-15T21:41:37.487840Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-15T21:41:37.492264Z","title":"Narayan, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.492264Z"},"links":{"cited_paper":"/paper/1206.1213","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:fda1bd14e23a4fc92d0698f0bd974e505cd6e7ebfbe871ac981165ef3934ac7d","observation_id":"6e491488-427a-4101-822e-80f48055dc0c","resolution":{"observed_at":"2026-08-15T21:41:37.492264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.06025","last_updated":"2018-12-14T16:58:45Z","snapshot_observed_at":"2026-08-14T17:43:29.821403Z","submitted_at":"2018-12-14T16:58:45Z","title":"Relativistic Jets in Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.06025","snapshot_observed_at":"2026-08-15T21:41:37.496858Z","title":"Blandford, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.496858Z"},"links":{"cited_paper":"/paper/1812.06025","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:67316ecb09daf1d8b49dd8b8706221f5baa546c9f4e0538449157f47406a17dd","observation_id":"8a1912be-8a8a-4d0a-bde5-339be058b941","resolution":{"observed_at":"2026-08-15T21:41:37.496858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.06322","last_updated":"2020-08-15T10:45:16Z","snapshot_observed_at":"2026-08-15T05:58:59.729748Z","submitted_at":"2020-03-13T14:33:44Z","title":"Relativistic Jets of Blazars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.06322","snapshot_observed_at":"2026-08-15T21:41:37.501601Z","title":"Hovatta and E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.501601Z"},"links":{"cited_paper":"/paper/2003.06322","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:0e895682256c2a42893d6cafe79a37deb6232cb0f6be1ca5eeb92eeac4f29415","observation_id":"0df993ae-f733-4b3f-ace1-221cef1b1083","resolution":{"observed_at":"2026-08-15T21:41:37.501601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02439","last_updated":"2022-02-14T21:31:15Z","snapshot_observed_at":"2026-08-10T13:01:00.360995Z","submitted_at":"2021-11-03T18:01:15Z","title":"What really makes an accretion disc MAD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02439","snapshot_observed_at":"2026-08-15T21:41:37.506079Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.506079Z"},"links":{"cited_paper":"/paper/2111.02439","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:7508953b3cbd523bef2a7bb9e0c05fb88387a6c21511ef21dd7b5e3f48afb72c","observation_id":"1edbdef0-b426-4522-b9d8-0cd1cc67b912","resolution":{"observed_at":"2026-08-15T21:41:37.506079Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.01169","last_updated":"2021-05-03T21:12:04Z","snapshot_observed_at":"2026-08-03T17:10:04.111086Z","submitted_at":"2021-05-03T21:12:04Z","title":"First M87 Event Horizon Telescope Results. VII. Polarization of the Ring","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.01169","snapshot_observed_at":"2026-08-15T21:41:37.510606Z","title":"Akiyama et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.510606Z"},"links":{"cited_paper":"/paper/2105.01169","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:4c4b1f52d571e9048edb387fabe5bd9ac0344ccee6df235b321676cd6d1644cb","observation_id":"36d65833-12c2-4f67-b7a4-d2751214c851","resolution":{"observed_at":"2026-08-15T21:41:37.510606Z","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":"2026-08-15T21:41:38.877440Z","title":"Ichimaru, Astrophys","venue":null,"work_id":"ea9a81b0-dee4-4d3d-b937-3ca14372606a","year":1977},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.515228Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:62655ace0505c3b349ded7b4dd3b305073230bd280bff3d42c9c4f51d4ea227c","observation_id":"b0661a1e-a995-4784-98c5-2c75727ff3bd","resolution":{"observed_at":"2026-08-15T21:41:38.882270Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:41:37.519450Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.519450Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:6a4a7ad2b54fbac021996347973999cd5d126c451876630273a14f707111cdbb","observation_id":"b05fe993-8fe8-4b3b-b946-2c330e76cef2","resolution":{"observed_at":"2026-08-15T21:41:37.519450Z","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":"ph/9906213","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:41:38.237299Z","title":null,"venue":null,"work_id":"a0f8e458-5ea1-4ca8-bb6b-5a87b880d283","year":2000},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.523940Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:3a2d4730ab6ae9aff04b766fe8075f055f26a5ba9762506f245aeceffdd4194e","observation_id":"92a0a6c1-3628-46eb-875b-1d08c6695476","resolution":{"observed_at":"2026-08-15T21:41:38.244948Z","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":"astro-ph/0506367","last_updated":"2005-07-15T01:03:45Z","snapshot_observed_at":"2026-07-07T00:51:24.821839Z","submitted_at":"2005-06-16T17:53:25Z","title":"Total and Jet Blandford-Znajek Power in Presence of Accretion Disk","version":2},"cited_work":{"arxiv_id":"astro-ph/0506367","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0506367","snapshot_observed_at":"2026-08-15T21:41:38.104552Z","title":"Total and Jet Blandford-Znajek Power in Presence of Accretion Disk","venue":"astro-ph","work_id":"418480d7-5cb7-455d-872b-9c4f73bb35db","year":2005},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.528305Z"},"links":{"cited_paper":"/paper/astro-ph/0506367","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:7d7dce4073e9326b11c8203c8921b79e3cc585be0dcf138cc54b594159e4053b","observation_id":"deb16ba5-5a51-4b39-8dcf-f7df0d2ee4fc","resolution":{"observed_at":"2026-08-15T21:41:38.109425Z","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":"1809.04608","last_updated":"2022-08-10T16:39:14Z","snapshot_observed_at":"2026-08-14T18:29:16.416036Z","submitted_at":"2018-09-12T18:00:06Z","title":"Large-Scale Poloidal Magnetic Field Dynamo Leads to Powerful Jets in GRMHD Simulations of Black Hole Accretion with Toroidal Field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.04608","snapshot_observed_at":"2026-08-15T21:41:37.532952Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.532952Z"},"links":{"cited_paper":"/paper/1809.04608","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:c4b5c7880e26185d2a629989acfa030665b6853327ba3433a973fde22a810340","observation_id":"a0ffa5d8-514c-4928-863d-df50316b4584","resolution":{"observed_at":"2026-08-15T21:41:37.532952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01197","last_updated":"2015-01-06T15:22:53Z","snapshot_observed_at":"2026-08-14T23:05:05.321002Z","submitted_at":"2015-01-06T15:22:53Z","title":"Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01197","snapshot_observed_at":"2026-08-15T21:41:37.537411Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.537411Z"},"links":{"cited_paper":"/paper/1501.01197","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:b46fe0af1403446827908854e05ea318a952c955ede513553c696edde3ab6465","observation_id":"ca217193-a4f4-4cc3-8910-6709651c4fd4","resolution":{"observed_at":"2026-08-15T21:41:37.537411Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.02680","last_updated":"2019-10-23T00:11:00Z","snapshot_observed_at":"2026-08-14T18:18:58.851574Z","submitted_at":"2018-10-05T13:45:02Z","title":"Fundamental Physics with the Square Kilometre Array","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.02680","snapshot_observed_at":"2026-08-15T21:41:37.542149Z","title":"Weltman et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.542149Z"},"links":{"cited_paper":"/paper/1810.02680","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:c187692bf9b99ba68d9d2e91d1f1fecd32abf8c0ec779ae27932ee016bf68ff1","observation_id":"17495ef6-3e47-4640-8f44-c2c87787a226","resolution":{"observed_at":"2026-08-15T21:41:37.542149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.12380","last_updated":"2022-01-27T19:07:34Z","snapshot_observed_at":"2026-08-13T18:22:02.034744Z","submitted_at":"2021-08-27T16:31:56Z","title":"Jets in Magnetically Arrested Hot Accretion Flows: Geometry, Power and Black Hole Spindown","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.12380","snapshot_observed_at":"2026-08-15T21:41:37.546894Z","title":"Narayan, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.546894Z"},"links":{"cited_paper":"/paper/2108.12380","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:6261b3185af67284ece9c19f4431c62b509f3538a225517653ce9939cd78b970","observation_id":"a86c8df1-72f3-4216-b097-5531ce9e3382","resolution":{"observed_at":"2026-08-15T21:41:37.546894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03538","last_updated":"2025-02-05T19:00:07Z","snapshot_observed_at":"2026-08-09T04:31:48.817367Z","submitted_at":"2025-02-05T19:00:07Z","title":"Simulating ULXs and blazars as GRMHD accretion flows around a black hole","version":1},"cited_work":{"arxiv_id":"2502.03538","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.03538","snapshot_observed_at":"2026-08-15T21:41:38.021577Z","title":"Simulating ULXs and blazars as GRMHD accretion flows around a black hole","venue":"astro-ph.HE","work_id":"4feaae33-cf24-4e7c-8152-01ee57678d18","year":2025},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.551603Z"},"links":{"cited_paper":"/paper/2502.03538","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:ae2ac3f59788a0e95909bf57aac6693e68d4fb686322e176551db1bef34d20ab","observation_id":"e0cb2a60-9ae2-4630-88da-79ab3814a0fd","resolution":{"observed_at":"2026-08-15T21:41:38.026948Z","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":"2026-08-15T21:41:38.853843Z","title":null,"venue":null,"work_id":"01864695-27bc-49b5-96c3-ac1c707b3f61","year":1982},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.556387Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:880b125a0548fb97a31f83592ae09f98dcb795a6b5768d8533b135a0df1669a4","observation_id":"ac110156-6ab8-4643-b401-a534995446b3","resolution":{"observed_at":"2026-08-15T21:41:38.858140Z","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":"2026-08-15T21:41:38.840390Z","title":null,"venue":null,"work_id":"a5f40c74-4873-41dc-8346-71760e70a3bd","year":1989},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.561248Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:f02e11d00e253bab3104f5dc965218c637fd16b7b3d4e658d8fab6057144676a","observation_id":"b1a6cc65-c65f-4e18-bd39-ffe765167cfa","resolution":{"observed_at":"2026-08-15T21:41:38.844628Z","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":"2026-08-15T21:41:38.826716Z","title":"Mukhanov and S","venue":null,"work_id":"e896c6dd-3329-42dd-a56a-634004453678","year":2007},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.565819Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:63b6528f59129fd5b7ca7d56b9d436ad8607ad4729e9d70d813c97c0cf4ac12f","observation_id":"11c35113-d35f-4aea-ad9e-93d0b3fa7fa5","resolution":{"observed_at":"2026-08-15T21:41:38.830892Z","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":"2026-08-15T21:41:38.812320Z","title":null,"venue":null,"work_id":"3659c6af-472b-48f1-84be-41ce29f715a7","year":2009},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.570417Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:990c319cd706b8139db261ecaf8b980fa37130375849270f8ec3f81d4661103e","observation_id":"7d190fc3-09b7-4e66-9220-18c47106cf1f","resolution":{"observed_at":"2026-08-15T21:41:38.817121Z","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":"2026-08-15T21:41:38.797039Z","title":null,"venue":null,"work_id":"9eccc8c4-f8bf-425c-b6a3-c512a067a480","year":2020},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.575002Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:45bf33243e954db695b015402cd3f0fdee2cb4d6fa029f81f4e79b8cae014acb","observation_id":"312e7d12-c77c-42f8-8dfb-07ee37890645","resolution":{"observed_at":"2026-08-15T21:41:38.801655Z","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":"1508.02546","last_updated":"2015-08-11T10:21:41Z","snapshot_observed_at":"2026-08-16T02:20:41.517540Z","submitted_at":"2015-08-11T10:21:41Z","title":"Disks and Jets - Gravity, Rotation and Magnetic Fields","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.02546","snapshot_observed_at":"2026-08-15T21:41:37.579106Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.579106Z"},"links":{"cited_paper":"/paper/1508.02546","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:a9c2031a2c102bb538801770ef00bc96124e8c116f17ec0adc1ad0c5ade937f2","observation_id":"11b5e627-b19a-4260-ac22-3a77bf6fda63","resolution":{"observed_at":"2026-08-15T21:41:37.579106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06533","last_updated":"2022-04-13T17:24:31Z","snapshot_observed_at":"2026-08-15T00:17:21.985054Z","submitted_at":"2022-04-13T17:24:31Z","title":"Modified theories of Gravity: Why, How and What?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.06533","snapshot_observed_at":"2026-08-15T21:41:37.583385Z","title":"Shankaranarayanan and J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.583385Z"},"links":{"cited_paper":"/paper/2204.06533","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:7269772a4c44107ccad963b40a3619eac53d2fc78330aea62dd58faee82d79c9","observation_id":"72c0bdd2-6dd5-4eaa-a0cd-db82235374ff","resolution":{"observed_at":"2026-08-15T21:41:37.583385Z","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":"2026-08-15T21:41:38.781422Z","title":null,"venue":null,"work_id":"4ecf5218-d657-4f60-98ff-db48d8448cd4","year":1985},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.587464Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:29acdc13d04b8f7387a93dbf5a61714e2011ddb5ca12b4d8e25feeceba54c626","observation_id":"e9914efc-a845-4099-9ffe-d157818323ec","resolution":{"observed_at":"2026-08-15T21:41:38.786066Z","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/0305261","last_updated":"2003-07-16T13:31:34Z","snapshot_observed_at":"2026-08-10T07:14:18.969864Z","submitted_at":"2003-05-15T08:35:41Z","title":"A fundamental plane of black hole activity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0305261","snapshot_observed_at":"2026-08-15T21:41:37.591661Z","title":"Merloni, S","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.591661Z"},"links":{"cited_paper":"/paper/astro-ph/0305261","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:e776efa3cb225a5880cb5d38cd9c5dc2b76619fb97fe6f78e27cc5b28f0fd83e","observation_id":"acbb07b9-656d-4665-ade3-3b04f4a22d00","resolution":{"observed_at":"2026-08-15T21:41:37.591661Z","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":"2026-08-15T21:41:38.766439Z","title":null,"venue":null,"work_id":"b39b5ec9-694c-470b-9b4f-4b22f86a85f8","year":2009},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.596951Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:5da867bdd4abf8a84f7f9cafaf5852d33632676d9b9b64838853b62ca26fcc3e","observation_id":"46abbfdc-729d-4de6-97af-8da0878cc1ae","resolution":{"observed_at":"2026-08-15T21:41:38.771074Z","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":"1911.01517","last_updated":"2019-11-04T22:23:42Z","snapshot_observed_at":"2026-07-06T08:34:41.399203Z","submitted_at":"2019-11-04T22:23:42Z","title":"The Next Generation Very Large Array","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.01517","snapshot_observed_at":"2026-08-15T21:41:37.601005Z","title":"Di Francesco and Others, in Canadian Long Range Plan for Astronomy and Astrophysics White Papers, Vol","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.601005Z"},"links":{"cited_paper":"/paper/1911.01517","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:2d989baa4bf0ba3fe518b972b86d6c21160a05be1a8b99ce2bebc16e46ebb259","observation_id":"fd9ee2d9-7900-458b-9082-482bcb216d20","resolution":{"observed_at":"2026-08-15T21:41:37.601005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.07648","last_updated":"2019-07-17T17:14:55Z","snapshot_observed_at":"2026-08-14T13:34:12.267382Z","submitted_at":"2019-07-17T17:14:55Z","title":"The DSA-2000 -- A Radio Survey Camera","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.07648","snapshot_observed_at":"2026-08-15T21:41:37.606273Z","title":"Hallinan and Others, in Bulletin of the American Astronomical Society , Vol","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.606273Z"},"links":{"cited_paper":"/paper/1907.07648","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:d988af52d78f6e72d716906f39c74f2a201cd597e57075deb73e27e28f452f9f","observation_id":"8d58497a-e896-4e2d-baa4-244139f3e7ef","resolution":{"observed_at":"2026-08-15T21:41:37.606273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.3550","last_updated":"2013-05-19T14:14:48Z","snapshot_observed_at":"2026-08-15T00:17:44.832543Z","submitted_at":"2013-05-15T17:17:23Z","title":"LOFAR: The LOw-Frequency ARray","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.3550","snapshot_observed_at":"2026-08-15T21:41:37.610987Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.610987Z"},"links":{"cited_paper":"/paper/1305.3550","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:f3a309c9a2cdb97e7e7407116788ada916f3300ca457ed147771121fcfa1d7c0","observation_id":"e2431dec-526d-42df-9962-b17cc2894207","resolution":{"observed_at":"2026-08-15T21:41:37.610987Z","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":"2026-08-15T21:41:38.750953Z","title":"Chen, H.-Y","venue":null,"work_id":"97983cd1-d2db-4183-9028-d91034f3138a","year":2020},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.615714Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:093492cdaa6baecfbdadf0bff0c657febe54cc2fe17d88354f1ba5bd62f4680b","observation_id":"7e04e213-3b8e-4397-9709-40b29130eec2","resolution":{"observed_at":"2026-08-15T21:41:38.756024Z","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":"2026-08-15T21:41:38.736111Z","title":"Akiyama et al","venue":null,"work_id":"fd4e7609-e35f-4949-8db7-f192116077de","year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.620059Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:d13ea196a1fb60430b5dbe439e224c2171d84a09bd53ed4c2a4e3cf7487068b7","observation_id":"d60344e4-5d52-4961-a8b2-ac4d5cba15e2","resolution":{"observed_at":"2026-08-15T21:41:38.740275Z","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":"2026-08-15T21:41:38.722104Z","title":null,"venue":null,"work_id":"d6ffb19a-e97a-4522-8232-6f4ecd0f1d01","year":1980},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.624456Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:1a8f511930e49be0c707c2a155b9dbca433bf6e95eed17bcf9aed6156e27df67","observation_id":"0e42c003-2d70-4995-a038-05d3e8d1966e","resolution":{"observed_at":"2026-08-15T21:41:38.726533Z","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":"2026-08-15T21:41:38.708634Z","title":"Akiyama et al","venue":null,"work_id":"87304416-c60a-4604-b821-7ee6e9484fde","year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.628952Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:f1796e52b148b249d8f2729f541deef43b538d35c64f8a14adda73981f78637c","observation_id":"c7b88985-6ee5-4b27-878d-18fc77f31d1c","resolution":{"observed_at":"2026-08-15T21:41:38.712600Z","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/9706112","last_updated":"1997-08-25T15:39:17Z","snapshot_observed_at":"2026-07-07T01:17:27.247423Z","submitted_at":"1997-06-11T20:15:11Z","title":"Advection-Dominated Accretion Model of Sagittarius A*: Evidence for a Black Hole at the Galactic Center","version":2},"cited_work":{"arxiv_id":"astro-ph/9706112","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9706112","snapshot_observed_at":"2026-08-15T21:41:37.910048Z","title":"Advection-Dominated Accretion Model of Sagittarius A*: Evidence for a Black Hole at the Galactic Center","venue":"astro-ph","work_id":"68fc1fd4-92df-46b3-9d64-a4675386e514","year":1997},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.633670Z"},"links":{"cited_paper":"/paper/astro-ph/9706112","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:5b1e6bfcb3f7ca958152cfba54614bd0c631786440361801f843b82ec5a61209","observation_id":"d7d15798-5b07-4777-9cc1-cf2974594258","resolution":{"observed_at":"2026-08-15T21:41:37.915151Z","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":"2026-08-15T21:41:38.693917Z","title":null,"venue":null,"work_id":"14d4adda-8c55-48f4-b786-c05d4cd7a246","year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.638493Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:87200180f63334b6d4724ab2c83cdfa76530161b7d38e9b33aee033ea20fffec","observation_id":"87d2a837-7009-4e02-a625-382c61f25aab","resolution":{"observed_at":"2026-08-15T21:41:38.698524Z","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":"2026-08-15T21:41:38.678717Z","title":null,"venue":null,"work_id":"23f6eb49-0f8c-4925-99e8-87a7db51ab96","year":1973},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.642932Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:d305fd6ac66b2991dd63fab335d9638afd9ac7098fdf31ae0614311c251ba2f1","observation_id":"bc163077-62e2-4a03-9b5a-1856ad00a3de","resolution":{"observed_at":"2026-08-15T21:41:38.683225Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T21:41:37.647295Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.647295Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:7a9d5b7eddac88cf6d9dc93c0176b6381b514ef51dca42a7c54607ea4832a974","observation_id":"b855ea48-10a3-4d2a-b64e-ce44d08fa5d2","resolution":{"observed_at":"2026-08-15T21:41:37.647295Z","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":"2026-08-15T21:41:38.653617Z","title":"Greiner, B","venue":null,"work_id":"e38052fc-e4b3-4e10-8d32-b542361d2987","year":1985},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.651642Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:d18a95cd0ef619418e38471a9bdb02716dc14da781da860453e092d81fd2b1e3","observation_id":"2b82c44e-a67b-40e3-9217-3495c289af84","resolution":{"observed_at":"2026-08-15T21:41:38.658884Z","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":"1212.2040","last_updated":"2012-12-10T11:58:15Z","snapshot_observed_at":"2026-08-15T00:36:35.459752Z","submitted_at":"2012-12-10T11:58:15Z","title":"The magnetic field in the X-ray corona of Cygnus X-1","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.2040","snapshot_observed_at":"2026-08-15T21:41:37.656112Z","title":"Del Santo, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.656112Z"},"links":{"cited_paper":"/paper/1212.2040","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:fc52c74434b80e96ed889dd2cd5ec665216a434c1396ee4e1b82c756f9c24175","observation_id":"96b7084d-1444-49cd-bbaa-a128c0eebe11","resolution":{"observed_at":"2026-08-15T21:41:37.656112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.00902","last_updated":"2016-06-02T21:23:23Z","snapshot_observed_at":"2026-08-14T21:54:26.176733Z","submitted_at":"2016-06-02T21:23:23Z","title":"On the Time Dependence of Adiabatic Particle Number","version":1},"cited_work":{"arxiv_id":"1606.00902","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.00902","snapshot_observed_at":"2026-08-15T21:41:37.872144Z","title":"On the Time Dependence of Adiabatic Particle Number","venue":"hep-th","work_id":"c9f9c870-97b9-4a16-9a3a-718c6f8f174a","year":2016},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.660996Z"},"links":{"cited_paper":"/paper/1606.00902","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:9583a489f31d5a943ef4ba2bf4fe903692829a7562a144ec4d2cb66ec4458a46","observation_id":"1df0fde5-902f-400b-8cb8-0c6e9aa3ffbd","resolution":{"observed_at":"2026-08-15T21:41:37.877174Z","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":"2026-08-15T21:41:38.636520Z","title":"Wilczek and A","venue":null,"work_id":"e5fcb9f7-db84-4b1e-8395-dc7eb1cd0b23","year":1989},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.665591Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:af31eaca34099f4a29327aa22237760e9921a900846ebe3a82019432c3fe0291","observation_id":"8cbaa236-5b49-43c7-a757-6113110e8b5b","resolution":{"observed_at":"2026-08-15T21:41:38.641291Z","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":"2026-08-15T21:41:38.621543Z","title":null,"venue":null,"work_id":"cd14e366-1722-42cd-a5d9-ba16d1e97e16","year":2014},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.669997Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:f1ff0051cd5e8981c764b2e89076bd59daa8363540378e64ab40c47e39c85d1c","observation_id":"e04d8be1-09bc-4963-9c7b-598141fc6a12","resolution":{"observed_at":"2026-08-15T21:41:38.626055Z","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":"0809.4490","last_updated":"2009-03-03T21:44:21Z","snapshot_observed_at":"2026-08-15T10:05:50.145512Z","submitted_at":"2008-09-25T21:27:22Z","title":"Estimating the Parameters of Sgr A*'s Accretion Flow Via Millimeter VLBI","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.4490","snapshot_observed_at":"2026-08-15T21:41:37.674428Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.674428Z"},"links":{"cited_paper":"/paper/0809.4490","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:1d96152e4696a818824a5d21dab32d7087cc76aeea31a39869ccd1389332cf1d","observation_id":"62f72224-ec7e-476f-a4e5-b568d762aa3d","resolution":{"observed_at":"2026-08-15T21:41:37.674428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.09907","last_updated":"2018-12-24T12:49:39Z","snapshot_observed_at":"2026-08-14T17:38:54.246783Z","submitted_at":"2018-12-24T12:49:39Z","title":"Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry","version":1},"cited_work":{"arxiv_id":"1812.09907","doi":null,"metadata_source":"pith","pith_arxiv_id":"1812.09907","snapshot_observed_at":"2026-08-15T21:41:37.834886Z","title":"Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry","venue":"astro-ph.HE","work_id":"ea8023c0-056b-46fc-a2ad-f3ab2337a477","year":2018},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.678965Z"},"links":{"cited_paper":"/paper/1812.09907","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:6ee646ac30e97142d4e5d1e67deaf5133f9377a43fbb6f6fc7b40e6d9a659240","observation_id":"608b92f9-6e38-4f63-b9e9-f6ee34107bfc","resolution":{"observed_at":"2026-08-15T21:41:37.839901Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"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":"2026-08-15T21:41:38.606516Z","title":"Padmanabhan, Theoretical Astrophysics - Volume 1, Astrophysical Processes, Vol","venue":null,"work_id":"c4a60265-9829-4c37-b86e-9f54dd4486c8","year":2000},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.683593Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:f9d59783f65f4f141a5fa73ff1dc863eeeb25bc6f7c0a2de8a8472f92a9afc3f","observation_id":"54c4f11d-45fe-4862-8be4-9ccc81448233","resolution":{"observed_at":"2026-08-15T21:41:38.611456Z","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":"2026-08-15T21:41:38.591713Z","title":"On the other hand,N (t) =N (t) is an even function (by our choice of B(t) and A∥(t)); hence, N (E) =N (−E)","venue":null,"work_id":"6dc51ace-6e03-419b-bf0a-a534eed6232f","year":null},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.688157Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:c36cf0f4634fc3d67bb78c6c79b076a3be92b00ae6cc77ccd5ea7269fbadcd47","observation_id":"fa50ff1d-67f8-4ad7-94fd-4c0d6c47702c","resolution":{"observed_at":"2026-08-15T21:41:38.596301Z","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":"2501.06333","last_updated":"2025-07-09T14:57:58Z","snapshot_observed_at":"2026-08-10T21:02:16.353215Z","submitted_at":"2025-01-10T20:26:14Z","title":"VLA+VLBA to ngVLA Transition Option Concepts","version":2},"cited_work":{"arxiv_id":"2501.06333","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.06333","snapshot_observed_at":"2026-08-15T21:41:37.814515Z","title":"VLA+VLBA to ngVLA Transition Option Concepts","venue":"astro-ph.IM","work_id":"2bb34a1c-c66e-46cb-87bc-b13dd385d095","year":2025},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.692909Z"},"links":{"cited_paper":"/paper/2501.06333","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:d322e3d4b988129db62e0208f59580135c77537735c477a46066e3db80ae65dd","observation_id":"c1280071-583b-4812-b799-4d0e07d9d99f","resolution":{"observed_at":"2026-08-15T21:41:37.819565Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"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":"2026-08-15T21:41:38.577414Z","title":"Afonso, B","venue":null,"work_id":"9969729c-1ca6-4f5c-9b28-0de36a708dad","year":2001},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.697748Z"},"links":{"citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:692574e10ae551cacf8e0104895682a08927b8417f821d8c4dece7346a2bd200","observation_id":"5661929f-a6be-4724-94ba-bbe42a929619","resolution":{"observed_at":"2026-08-15T21:41:38.581869Z","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":"2308.03837","last_updated":"2023-09-11T11:07:44Z","snapshot_observed_at":"2026-08-13T10:39:10.101186Z","submitted_at":"2023-08-07T18:00:01Z","title":"Radio Emission From a $z =$ 10.1 Black Hole in UHZ1","version":2},"cited_work":{"arxiv_id":"2308.03837","doi":null,"metadata_source":"pith","pith_arxiv_id":"2308.03837","snapshot_observed_at":"2026-08-15T21:41:37.791984Z","title":"Radio Emission From a $z =$ 10.1 Black Hole in UHZ1","venue":"astro-ph.GA","work_id":"f93af752-119f-4492-8a92-96ee1f177deb","year":2023},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.702205Z"},"links":{"cited_paper":"/paper/2308.03837","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:ba4c29cf75b634b7b83eb8d6c4a6883235cd9358bf850a619b63e72c8b4dfdec","observation_id":"95b66763-c02a-4e89-a9ef-f47faa05af3a","resolution":{"observed_at":"2026-08-15T21:41:37.797636Z","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":"2309.13008","last_updated":"2023-09-27T00:04:32Z","snapshot_observed_at":"2026-08-13T10:07:24.550450Z","submitted_at":"2023-09-22T17:16:35Z","title":"PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field","version":2},"cited_work":{"arxiv_id":"2309.13008","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.13008","snapshot_observed_at":"2026-08-15T21:41:37.771048Z","title":"PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field","venue":"astro-ph.GA","work_id":"2d732081-a5ea-480f-a236-0e6e2f35dd2e","year":2023},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.706656Z"},"links":{"cited_paper":"/paper/2309.13008","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:40ec0e240563276437838e10a21f0a8fa068e7bd45453463c7f8602db6aa36e7","observation_id":"6d19aaa3-1fe7-4744-a7a0-f4deacb4e9da","resolution":{"observed_at":"2026-08-15T21:41:37.776135Z","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":"2504.00192","last_updated":"2025-03-31T20:00:51Z","snapshot_observed_at":"2026-08-07T16:19:18.923379Z","submitted_at":"2025-03-31T20:00:51Z","title":"An Updated Repository of Sub-mJy Extragalactic Source-Count Measurements in the Radio Domain","version":1},"cited_work":{"arxiv_id":"2504.00192","doi":null,"metadata_source":"pith","pith_arxiv_id":"2504.00192","snapshot_observed_at":"2026-08-15T21:41:37.747704Z","title":"An Updated Repository of Sub-mJy Extragalactic Source-Count Measurements in the Radio Domain","venue":"astro-ph.GA","work_id":"2a941e3a-96e8-4eff-ab5f-a331b007127b","year":2025},"citing_paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T21:41:37.710758Z"},"links":{"cited_paper":"/paper/2504.00192","citing_paper":"/paper/2505.09355"},"observation_digest":"sha256:8e9862b6f1f9ab520df8ca700f9d6984352a39e9a6189fb9c8e55f92ea8bb62d","observation_id":"09e622f4-718c-442c-8c1f-b3e7fef89ff0","resolution":{"observed_at":"2026-08-15T21:41:37.754380Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2505.09355","last_updated":"2025-05-14T13:05:05Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T05:52:00.608275Z","submitted_at":"2025-05-14T13:05:05Z","title":"Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields"},"reference_resolution":{"displayed":68,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":44,"verified_exact":9,"verified_fuzzy":13},"total_outbound_references":68},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+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 68 of 68 outbound references and 0 inbound Pith citation observations for arXiv:2505.09355."}