{"as_of":"2026-08-14T15:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e979ac8d160b586491fd38e16ba6d641cc52d0654170df68b252e64a1befb216","coverage":[{"denominator":296,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:20:28.499254Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+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/2608.10067/citation-record","integrity":"/paper/2608.10067/integrity","json":"/paper/2608.10067/citation-record.json","paper":"/paper/2608.10067"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:20:28.095801Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.095801Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:4579cefcf301349de8d042d74f6f19561a912b4757a355c23af8585962155754","observation_id":"6286779b-28ae-437d-a577-b706a3a2e6bb","resolution":{"observed_at":"2026-08-14T04:20:28.095801Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.10285","last_updated":"2021-06-18T18:00:01Z","snapshot_observed_at":"2026-07-06T11:20:49.881453Z","submitted_at":"2021-06-18T18:00:01Z","title":"Numerical Analysis of Long-term Variability of AGN Jets through RMHD Simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.10285","snapshot_observed_at":"2026-08-14T04:20:28.100060Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.100060Z"},"links":{"cited_paper":"/paper/2106.10285","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:b268a29550559ba7551f86a9dd13f377477b9a703a73947a5ec102256765b605","observation_id":"43814cf9-b77b-48bb-a30e-116cb35740c5","resolution":{"observed_at":"2026-08-14T04:20:28.100060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.14976","last_updated":"2020-11-17T15:50:17Z","snapshot_observed_at":"2026-07-06T09:33:01.372590Z","submitted_at":"2020-06-26T13:20:56Z","title":"Kink-driven magnetic reconnection in relativistic jets: consequences for X-ray polarimetry of BL Lacs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.14976","snapshot_observed_at":"2026-08-14T04:20:28.104163Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.104163Z"},"links":{"cited_paper":"/paper/2006.14976","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8983a243525b1b0f4dd2a21b4a49f564d1ea11df3c1f07f1c6e39967b2e95e1d","observation_id":"d99e62e6-7ee4-4786-8d1d-6aebd1631b8e","resolution":{"observed_at":"2026-08-14T04:20:28.104163Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.07765","last_updated":"2020-03-17T15:28:44Z","snapshot_observed_at":"2026-07-06T09:05:20.235460Z","submitted_at":"2020-03-17T15:28:44Z","title":"Kink Instabilities In Relativistic Jets Can Drive Quasi-Periodic Radiation Signatures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.07765","snapshot_observed_at":"2026-08-14T04:20:28.108434Z","title":", keywords =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.108434Z"},"links":{"cited_paper":"/paper/2003.07765","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:983b5c3525c85437a3ec6f40031b8d217da02c6b89970c765455f4fbda72e482","observation_id":"a9bc4823-ff92-4032-bd2e-8448083e285f","resolution":{"observed_at":"2026-08-14T04:20:28.108434Z","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":"2026-08-14T04:20:28.113049Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.113049Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:3c1cb004528c637fc8337413ccfdbe519342e59dfe6a310f04bf1987b0aae783","observation_id":"4ae1a788-2c24-4e67-99c8-0cf289b84ca6","resolution":{"observed_at":"2026-08-14T04:20:28.113049Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.4089","last_updated":"2014-06-17T07:30:18Z","snapshot_observed_at":"2026-08-10T07:14:31.751018Z","submitted_at":"2014-03-17T13:35:40Z","title":"Diffuse Neutrino Intensity from the Inner Jets of Active Galactic Nuclei: Impacts of External Photon Fields and the Blazar Sequence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.4089","snapshot_observed_at":"2026-08-14T04:20:28.118013Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.118013Z"},"links":{"cited_paper":"/paper/1403.4089","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8eed99c6961eaade2a89d721a7d4b7f02bc33698636a9c5ff0e02c4f6c2357e3","observation_id":"347cbe9a-a26e-4049-8e32-e6dad52714a4","resolution":{"observed_at":"2026-08-14T04:20:28.118013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.05654","last_updated":"2019-07-08T11:17:24Z","snapshot_observed_at":"2026-08-07T14:09:50.756738Z","submitted_at":"2018-12-13T19:50:09Z","title":"Cascading Constraints from Neutrino Emitting Blazars: The case of TXS 0506+056","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.05654","snapshot_observed_at":"2026-08-14T04:20:28.126248Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.126248Z"},"links":{"cited_paper":"/paper/1812.05654","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:d5f4886f1c4d1d90893b950c9a6591c5e8cecb4b516cd14cda4556a694c13d19","observation_id":"3ac7d549-0fdd-4a41-a314-ce67b04025de","resolution":{"observed_at":"2026-08-14T04:20:28.126248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.04915","last_updated":"2021-06-09T08:50:54Z","snapshot_observed_at":"2026-08-13T19:07:19.244663Z","submitted_at":"2021-06-09T08:50:54Z","title":"From electrons to Janskys: Full stokes polarized radiative transfer in 3D relativistic particle-in-cell jet simulations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.04915","snapshot_observed_at":"2026-08-14T04:20:28.129908Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.129908Z"},"links":{"cited_paper":"/paper/2106.04915","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:159022a38072fb67bfe0ec948024785d192ea00a8cbe46c768c7a9a86c2045e7","observation_id":"dabb36cf-a4d4-40c8-a37c-5bc415151d9e","resolution":{"observed_at":"2026-08-14T04:20:28.129908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207249","last_updated":"2002-07-11T17:13:59Z","snapshot_observed_at":"2026-07-07T00:27:22.572646Z","submitted_at":"2002-07-11T17:13:59Z","title":"AGN Black Hole Masses and Bolometric Luminosities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207249","snapshot_observed_at":"2026-08-14T04:20:28.133543Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.133543Z"},"links":{"cited_paper":"/paper/astro-ph/0207249","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:4df0b57e023f1917947b249290dffe102ed1b4d58e49a6de50dd2ccf47b53110","observation_id":"38f111bb-eba6-4062-ad02-7ea478b01b88","resolution":{"observed_at":"2026-08-14T04:20:28.133543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9903478","last_updated":"1999-03-31T13:36:46Z","snapshot_observed_at":"2026-07-07T01:25:23.293384Z","submitted_at":"1999-03-31T13:36:46Z","title":"Monte-Carlo simulations of photohadronic processes in astrophysics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9903478","snapshot_observed_at":"2026-08-14T04:20:28.136930Z","title":"Computer Physics Communications , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.136930Z"},"links":{"cited_paper":"/paper/astro-ph/9903478","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:849084f65d98e54bcd795ab9e41814ca7ff5bf02ce22c3dde28eb7ed6df6996e","observation_id":"78dfeb15-c732-4645-95a5-e8e83536b33a","resolution":{"observed_at":"2026-08-14T04:20:28.136930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0688","last_updated":"2009-01-16T15:04:30Z","snapshot_observed_at":"2026-08-13T05:16:14.474405Z","submitted_at":"2008-03-05T15:55:57Z","title":"Energy spectra of gamma-rays, electrons and neutrinos produced at interactions of relativistic protons with low energy radiation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.0688","snapshot_observed_at":"2026-08-14T04:20:28.140133Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.140133Z"},"links":{"cited_paper":"/paper/0803.0688","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:fc8e36187743d9888e26e7f78d732ba412b09209c130477d737a8a3b518c92bc","observation_id":"537d0f27-20eb-46a2-a554-e0024eb89d16","resolution":{"observed_at":"2026-08-14T04:20:28.140133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.0645","last_updated":"2014-06-18T16:57:38Z","snapshot_observed_at":"2026-07-06T03:45:19.685865Z","submitted_at":"2014-06-03T09:45:23Z","title":"TANAMI Blazars in the IceCube PeV Neutrino Fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.0645","snapshot_observed_at":"2026-08-14T04:20:28.143940Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.143940Z"},"links":{"cited_paper":"/paper/1406.0645","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:14b77e8ffd965094566e337bc4fe060f9b3677b2208a07ca857c7bd0c5c2d833","observation_id":"0a1af6e3-b1b0-4f12-8385-e648d91d48f5","resolution":{"observed_at":"2026-08-14T04:20:28.143940Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.03376","last_updated":"2015-02-11T17:02:43Z","snapshot_observed_at":"2026-07-06T04:08:57.861633Z","submitted_at":"2015-02-11T17:02:43Z","title":"Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.03376","snapshot_observed_at":"2026-08-14T04:20:28.148038Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.148038Z"},"links":{"cited_paper":"/paper/1502.03376","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:22c41bde31d2efe5afad5131aca1d63569d93cd4d792d551897559b3dc005bf1","observation_id":"9ebea1a9-5cf6-4d43-b6ad-b26c71e28b73","resolution":{"observed_at":"2026-08-14T04:20:28.148038Z","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":"2026-08-14T04:20:28.152763Z","title":", keywords =","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.152763Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:5ffedf77cb1f0770069b7332c16ef8b7bd59d469454fe95fe49c1aad2948ea56","observation_id":"70a7ba03-4d3e-4853-bc09-9cf6e8879d4f","resolution":{"observed_at":"2026-08-14T04:20:28.152763Z","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":"2026-08-14T04:20:28.157538Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.157538Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:952265ff0ddb26d6405b42097376052853726d7c5dcf43842642625bf9f61425","observation_id":"9a433757-de62-45c2-9d37-c332f29e8f84","resolution":{"observed_at":"2026-08-14T04:20:28.157538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.05325","last_updated":"2021-10-11T14:46:17Z","snapshot_observed_at":"2026-07-06T11:56:37.658013Z","submitted_at":"2021-10-11T14:46:17Z","title":"An expanding one-zone model for studying blazars emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.05325","snapshot_observed_at":"2026-08-14T04:20:28.161016Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.161016Z"},"links":{"cited_paper":"/paper/2110.05325","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:76173869bf8e57d357c7c70e64996d623fe7ca66f57a6475324548be23db14ac","observation_id":"598c5f92-27a8-43c0-b1f0-580bf990b606","resolution":{"observed_at":"2026-08-14T04:20:28.161016Z","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":"2026-08-14T04:20:28.165106Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.165106Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:5d733887a34b9f829bd30f29ecfdc3f339d5f49ac546c5644f7398c1a786a846","observation_id":"61b00940-170a-4ec4-afc2-762b576d4b08","resolution":{"observed_at":"2026-08-14T04:20:28.165106Z","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":"2026-08-14T04:20:28.168742Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.168742Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:e0accce7153055e20c2385311aca99a070b136c6b8d73cd588c8178267633f77","observation_id":"9eb351d5-c0d7-4dbf-a90e-833e82e351be","resolution":{"observed_at":"2026-08-14T04:20:28.168742Z","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":"2026-08-14T04:20:28.172327Z","title":"Highlights of Spanish Astrophysics XII , year = 2025, editor =","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.172327Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:f5cac4395bfd3c32ef2edb5fcd12382a2ea1aeab56acee484223a5c9c51970b8","observation_id":"c75df035-9f7d-427d-afa0-2cdb8af0e920","resolution":{"observed_at":"2026-08-14T04:20:28.172327Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.10732","last_updated":"2018-07-27T17:00:57Z","snapshot_observed_at":"2026-07-06T06:52:45.821495Z","submitted_at":"2018-07-27T17:00:57Z","title":"The Polarization Behavior of Relativistic Synchrotron Jets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.10732","snapshot_observed_at":"2026-08-14T04:20:28.176092Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.176092Z"},"links":{"cited_paper":"/paper/1807.10732","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:b959fe02e7cac7c06341cd004adbfdd985339ca73567b28003571a4c79c9e012","observation_id":"86c3bf13-e597-4cd8-bc26-6e44ea915916","resolution":{"observed_at":"2026-08-14T04:20:28.176092Z","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":"2026-08-14T04:20:28.180532Z","title":", keywords =","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.180532Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:0b13825928c2146f433db5c0f9b85b3c1c772f626cec09495a49eaa1b9f858f8","observation_id":"bc1cb672-8560-4588-895f-919c980881ce","resolution":{"observed_at":"2026-08-14T04:20:28.180532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.11875","last_updated":"2026-04-13T18:00:01Z","snapshot_observed_at":"2026-08-02T14:00:01.040802Z","submitted_at":"2026-04-13T18:00:01Z","title":"Spectral index evolution of the limb-brightened jet in 3C 84","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.11875","snapshot_observed_at":"2026-08-14T04:20:28.185259Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.185259Z"},"links":{"cited_paper":"/paper/2604.11875","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:d1cd5bf01c22acc88d03cf0fa62549f7e2252ee3b98dc96e36f960a0d7034831","observation_id":"75fe7917-a260-4211-be9e-3af31c878944","resolution":{"observed_at":"2026-08-14T04:20:28.185259Z","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":"2026-08-14T04:20:28.189349Z","title":"Journal of Physics G Nuclear Physics , keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.189349Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:b12524d80f7fcb3563f1cf559a31bb165ab0cdfea54de72a10c9c7f7ef37ae8b","observation_id":"4157852f-3646-41b0-8708-597f99373376","resolution":{"observed_at":"2026-08-14T04:20:28.189349Z","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":"2026-08-14T04:20:28.193619Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.193619Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:73a33f539abfcd902ca4ca2b2a6a7fed75c0efcb43238f2f9a083f9eba282135","observation_id":"6293f3c2-4d4e-4dbe-98e9-e70d0c91e9eb","resolution":{"observed_at":"2026-08-14T04:20:28.193619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.09954","last_updated":"2018-07-05T10:08:13Z","snapshot_observed_at":"2026-07-06T05:20:39.825511Z","submitted_at":"2016-11-30T00:41:13Z","title":"Faraday Conversion in Turbulent Blazar Jets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.09954","snapshot_observed_at":"2026-08-14T04:20:28.198012Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.198012Z"},"links":{"cited_paper":"/paper/1611.09954","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:b4b0512484ecea275208696ad4cd00caa71ba9a8901f5bd5ad5fe59e9af8a5a7","observation_id":"85f6e457-3577-4f7e-8fb6-b51d5628608f","resolution":{"observed_at":"2026-08-14T04:20:28.198012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0508200","last_updated":"2005-08-09T10:20:19Z","snapshot_observed_at":"2026-07-07T00:52:50.750906Z","submitted_at":"2005-08-09T10:20:19Z","title":"Imaging redshifts of BL Lac objects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0508200","snapshot_observed_at":"2026-08-14T04:20:28.202320Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.202320Z"},"links":{"cited_paper":"/paper/astro-ph/0508200","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:be3061cd60439e255ee6bbb415f156186a18f30c078349cdd13bb1da3d497d88","observation_id":"685d63a0-6923-4d09-a3b7-21761620f9fc","resolution":{"observed_at":"2026-08-14T04:20:28.202320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.3550","last_updated":"2007-09-21T23:50:37Z","snapshot_observed_at":"2026-07-06T01:29:45.442802Z","submitted_at":"2007-09-21T23:50:37Z","title":"The Outburst of the Blazar AO 0235+164 in 2006 December: Shock-in-Jet Interpretation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.3550","snapshot_observed_at":"2026-08-14T04:20:28.206926Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.206926Z"},"links":{"cited_paper":"/paper/0709.3550","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:3122d3acf9249e5b1219c109e9342db90a9909a07f6f91583281ec7a139b982d","observation_id":"b13ebd25-f2a3-4eb1-8418-7b53a32710c7","resolution":{"observed_at":"2026-08-14T04:20:28.206926Z","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":"2026-08-14T04:20:28.210774Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.210774Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:5052942c96904c131551b3257ca950c87e203e7add444cf4537cb35a9f77282c","observation_id":"bfb67a2f-c292-4451-89eb-160180fb9ec1","resolution":{"observed_at":"2026-08-14T04:20:28.210774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.1904","last_updated":"2009-04-13T04:44:01Z","snapshot_observed_at":"2026-07-31T07:28:42.106251Z","submitted_at":"2009-04-13T04:44:01Z","title":"Fermi Discovery of Gamma-Ray Emission from NGC 1275","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.1904","snapshot_observed_at":"2026-08-14T04:20:28.213752Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.213752Z"},"links":{"cited_paper":"/paper/0904.1904","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:ec45db16b20f172410f5d257a18bbd5b3472bfa026c9fa3bde2cf383a478a1d7","observation_id":"d3a6e993-4fee-4b11-8f17-cd060f5f1908","resolution":{"observed_at":"2026-08-14T04:20:28.213752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.08742","last_updated":"2017-09-25T22:54:24Z","snapshot_observed_at":"2026-07-06T06:01:19.276000Z","submitted_at":"2017-09-25T22:54:24Z","title":"POLAMI: Polarimetric Monitoring of Active Galactic Nuclei at Millimetre Wavelengths. I. The program, calibration, and calibrators data products","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.08742","snapshot_observed_at":"2026-08-14T04:20:28.217494Z","title":"The programme, calibration and calibrator data products","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.217494Z"},"links":{"cited_paper":"/paper/1709.08742","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:f63023500c55a1184f88b1ae27344a9fd47fdcc1ea94f7d11a8a3eb722cc1531","observation_id":"10c3dde3-186b-4e73-b6f6-cfedeb523ac3","resolution":{"observed_at":"2026-08-14T04:20:28.217494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.08744","last_updated":"2017-09-25T22:54:39Z","snapshot_observed_at":"2026-08-05T16:19:17.967146Z","submitted_at":"2017-09-25T22:54:39Z","title":"POLAMI: Polarimetric Monitoring of Active Galactic Nuclei at Millimetre Wavelengths. III. Characterisation of total flux density and polarisation variability of relativistic jets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.08744","snapshot_observed_at":"2026-08-14T04:20:28.220734Z","title":"Characterization of total flux density and polarization variability of relativistic jets","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.220734Z"},"links":{"cited_paper":"/paper/1709.08744","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:408210825e25ffeccabd39fe88a0c9b63a40cf73b6334218f9cb785277cbc9c4","observation_id":"0005fe2e-23db-432a-bcb2-f9a3cce8af45","resolution":{"observed_at":"2026-08-14T04:20:28.220734Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.01832","last_updated":"2025-05-03T14:28:31Z","snapshot_observed_at":"2026-08-07T15:56:47.014749Z","submitted_at":"2025-05-03T14:28:31Z","title":"High optical to X-ray polarization ratio reveals Compton scattering in BL Lacertae's jet","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.01832","snapshot_observed_at":"2026-08-14T04:20:28.224046Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.224046Z"},"links":{"cited_paper":"/paper/2505.01832","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:d71c064bf48dee0f64f8d34e16b2d48d8c32628cf58350ef824523b3157adbc5","observation_id":"56bc8b47-faeb-4caf-a457-9c7cd852ae3b","resolution":{"observed_at":"2026-08-14T04:20:28.224046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0706.0797","last_updated":"2007-06-27T12:39:21Z","snapshot_observed_at":"2026-07-06T01:28:21.745333Z","submitted_at":"2007-06-06T10:14:16Z","title":"An Exceptional VHE Gamma-Ray Flare of PKS 2155-304","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0706.0797","snapshot_observed_at":"2026-08-14T04:20:28.227758Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.227758Z"},"links":{"cited_paper":"/paper/0706.0797","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:c79ced81179f6bd9e39b211f46426eef10dc13ce743b650c8ea5e171d99a9c77","observation_id":"06dee3f0-f820-4886-9918-79bdcebee0f0","resolution":{"observed_at":"2026-08-14T04:20:28.227758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0702008","last_updated":"2007-12-05T00:52:11Z","snapshot_observed_at":"2026-07-07T01:06:44.699931Z","submitted_at":"2007-02-01T17:45:49Z","title":"Variable VHE gamma-ray emission from Markarian 501","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0702008","snapshot_observed_at":"2026-08-14T04:20:28.232284Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.232284Z"},"links":{"cited_paper":"/paper/astro-ph/0702008","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:354a321f29d74c5a885cab8ddf5fd526f8f501a66e9e8d41f339e003ca6c1610","observation_id":"02164aaf-5a66-4cc4-98b6-7d91ba941695","resolution":{"observed_at":"2026-08-14T04:20:28.232284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.3917","last_updated":"2012-03-05T11:30:10Z","snapshot_observed_at":"2026-07-06T02:39:33.682077Z","submitted_at":"2011-12-16T18:43:06Z","title":"Detection of very-high energy \\gamma-ray emission from NGC 1275 by the MAGIC telescopes","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.3917","snapshot_observed_at":"2026-08-14T04:20:28.236395Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.236395Z"},"links":{"cited_paper":"/paper/1112.3917","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:5750ec84e2969c66b9192da98ba421517c7549d70cbc54f15b0e92f3356cd93e","observation_id":"5f14ad36-14c6-4380-9f67-44f2c4c827e7","resolution":{"observed_at":"2026-08-14T04:20:28.236395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.02849","last_updated":"2018-05-08T06:14:33Z","snapshot_observed_at":"2026-07-06T06:37:55.065033Z","submitted_at":"2018-05-08T06:14:33Z","title":"Exploring the Variability of the Flat Spectrum Radio Source 1633+382. II: Physical Properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.02849","snapshot_observed_at":"2026-08-14T04:20:28.240303Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.240303Z"},"links":{"cited_paper":"/paper/1805.02849","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:cd54d3a7269e30180b0c7c0ca011cc054c6975a83b417497e3b8b98d683e11b8","observation_id":"58408e73-1465-49a0-9268-1f8bd4ca480c","resolution":{"observed_at":"2026-08-14T04:20:28.240303Z","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":"2026-08-14T04:20:28.244014Z","title":"IEEE Transactions on Pattern Analysis and Machine Intelligence , keywords =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.244014Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:43cc54e5a1ae01d5cc711eab88c0040e7c847de5ad8f14c8778d2dc66a41ebdf","observation_id":"9b14c842-a2ad-45fa-b910-47b36dc278ec","resolution":{"observed_at":"2026-08-14T04:20:28.244014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.1793","last_updated":"2011-12-26T17:20:37Z","snapshot_observed_at":"2026-07-06T02:35:26.087727Z","submitted_at":"2011-10-09T05:55:35Z","title":"The Structure of the M87 Jet: A Transition from Parabolic to Conical Streamlines","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.1793","snapshot_observed_at":"2026-08-14T04:20:28.247751Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.247751Z"},"links":{"cited_paper":"/paper/1110.1793","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:99d09935fec42e3baea512d18b86a0cc11a42c521f215aa26852dedcd9100cef","observation_id":"76ba4c8b-2169-4754-a3bc-8e744d525b80","resolution":{"observed_at":"2026-08-14T04:20:28.247751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.6212","last_updated":"2013-07-23T20:00:01Z","snapshot_observed_at":"2026-08-05T05:45:26.588200Z","submitted_at":"2013-07-23T20:00:01Z","title":"Astropy: A Community Python Package for Astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.6212","snapshot_observed_at":"2026-08-14T04:20:28.251465Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.251465Z"},"links":{"cited_paper":"/paper/1307.6212","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8b66c356bf6b20d2ac19f39f37ea39c5ce42e85aaca3e9319eb3e5e026b5a0c1","observation_id":"62159061-430b-4d79-95f8-d0b0dca09ca5","resolution":{"observed_at":"2026-08-14T04:20:28.251465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.02634","last_updated":"2018-01-16T15:05:07Z","snapshot_observed_at":"2026-08-14T11:23:56.488556Z","submitted_at":"2018-01-08T19:00:08Z","title":"The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.02634","snapshot_observed_at":"2026-08-14T04:20:28.254807Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.254807Z"},"links":{"cited_paper":"/paper/1801.02634","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:22689876a61fb0779c8b267abf1ae2493233f9b8ff37bb42fce48697d19512f5","observation_id":"4988fdb7-0205-48e1-b37c-6ca81654d2a2","resolution":{"observed_at":"2026-08-14T04:20:28.254807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0902.1089","last_updated":"2009-02-06T17:44:53Z","snapshot_observed_at":"2026-08-13T06:48:01.300851Z","submitted_at":"2009-02-06T17:44:53Z","title":"The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0902.1089","snapshot_observed_at":"2026-08-14T04:20:28.258282Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.258282Z"},"links":{"cited_paper":"/paper/0902.1089","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:302b79f2799772a9f27a540def2298fb0de853313c6e69d3a211a47802468bd2","observation_id":"df070da4-ef41-4b37-8377-21eb36184495","resolution":{"observed_at":"2026-08-14T04:20:28.258282Z","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":"2026-08-14T04:20:28.262419Z","title":", year = 1954, month = jan, volume =","venue":null,"work_id":null,"year":1954},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.262419Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:7a1a6c4532ce35bfccf60f216f99d22c5e82585828c825b7e6d00013bedf193a","observation_id":"5e2e267a-ad27-4478-aca0-16c273fc54d6","resolution":{"observed_at":"2026-08-14T04:20:28.262419Z","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":"2026-08-14T04:20:28.267015Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.267015Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:e229a911603709872bedeb2104dde85cfeebe12d231ce8fb8ae30b7f1ab971d5","observation_id":"d8164ae2-8ba0-48ff-ae22-f6f0d1475af9","resolution":{"observed_at":"2026-08-14T04:20:28.267015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0606050","last_updated":"2006-06-05T08:42:34Z","snapshot_observed_at":"2026-07-07T01:00:49.053341Z","submitted_at":"2006-06-02T12:37:50Z","title":"Structure and flux variability in the VLBI jet of BL Lacertae during the WEBT campaigns (1995--2004)","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0606050","snapshot_observed_at":"2026-08-14T04:20:28.270641Z","title":", keywords =","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.270641Z"},"links":{"cited_paper":"/paper/astro-ph/0606050","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:3b3a95321764f11acf086a35a8a26ed1f90dec474f275199cabb32519fc48aa9","observation_id":"2ec3c4d0-78e2-49d7-9c70-74d15d1618fd","resolution":{"observed_at":"2026-08-14T04:20:28.270641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.07100","last_updated":"2016-05-24T08:13:16Z","snapshot_observed_at":"2026-07-06T04:57:15.827651Z","submitted_at":"2016-05-23T17:17:51Z","title":"A Highly Magnetized Twin-Jet Base Pinpoints a Supermassive Black Hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.07100","snapshot_observed_at":"2026-08-14T04:20:28.274643Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.274643Z"},"links":{"cited_paper":"/paper/1605.07100","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:688085bd7a0b83b256ef78d644fc338ea2139a2c027715cd7168ac5c8bb58776","observation_id":"7becb4e4-760e-42d0-b509-e9093de76cab","resolution":{"observed_at":"2026-08-14T04:20:28.274643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.07071","last_updated":"2015-08-28T02:23:23Z","snapshot_observed_at":"2026-08-05T20:35:07.867996Z","submitted_at":"2015-08-28T02:23:23Z","title":"An Updated Ultraviolet Catalog of GALEX Nearby Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.07071","snapshot_observed_at":"2026-08-14T04:20:28.277831Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.277831Z"},"links":{"cited_paper":"/paper/1508.07071","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:a98269e687e7e43d11bff36243413f794466ac8a6cdf7152d80c6c0ffd679a91","observation_id":"097aeaa8-cdea-4faf-8cb4-6999fdb5aaf9","resolution":{"observed_at":"2026-08-14T04:20:28.277831Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/334131a0","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:20:29.758660Z","title":", keywords =","venue":null,"work_id":"6b24ae55-37b2-4ab4-9a6f-adf8e8783dcf","year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.281168Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8cdd93bcb222a8b193cfd00aa9cb67b15701f4e0e4642747185b0b6b29eadf71","observation_id":"153b863f-e950-45e8-adb7-6d36e28ab2e8","resolution":{"observed_at":"2026-08-14T04:20:29.762852Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1406.1718","last_updated":"2014-10-13T18:38:20Z","snapshot_observed_at":"2026-07-06T03:45:40.711413Z","submitted_at":"2014-06-06T15:54:56Z","title":"The 1% Concordance Hubble Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.1718","snapshot_observed_at":"2026-08-14T04:20:28.283931Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.283931Z"},"links":{"cited_paper":"/paper/1406.1718","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:9170509cd85bc7fd5d9b5e94d5aa24780b797c7413da7a12c25bc05e00007c1a","observation_id":"8b34bf03-f947-4d6b-aa2c-4d619af31583","resolution":{"observed_at":"2026-08-14T04:20:28.283931Z","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":"2026-08-14T04:20:28.286962Z","title":"Physics Uspekhi , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.286962Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:26f830bfb4c38c20f6429d1414e3eafc6555da1f284950e5acfcfb77addcdb50","observation_id":"29b1fdc9-08b1-402b-8e28-5648eb2a1eba","resolution":{"observed_at":"2026-08-14T04:20:28.286962Z","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":"2026-08-14T04:20:28.290244Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.290244Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:e5836ec8afee84149eb71d1a329f481a3c3f881ff65d942b8a4c281426e3364d","observation_id":"a692b2d4-be04-4105-8952-f8868ae5a5e5","resolution":{"observed_at":"2026-08-14T04:20:28.290244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.08832","last_updated":"2019-08-28T16:44:11Z","snapshot_observed_at":"2026-08-02T21:15:43.042642Z","submitted_at":"2019-03-21T05:13:47Z","title":"EHT-HOPS pipeline for millimeter VLBI data reduction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.08832","snapshot_observed_at":"2026-08-14T04:20:28.294429Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.294429Z"},"links":{"cited_paper":"/paper/1903.08832","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:448cdbd52f6bb71eb7b43d3b8e3fbd90d6f65e8803f105d1d30477787f721f42","observation_id":"8f1f1299-01d5-4b5b-99b6-57e37463b8f9","resolution":{"observed_at":"2026-08-14T04:20:28.294429Z","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":"2026-08-14T04:20:28.298248Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.298248Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:c868830c377804308672ca6c120d6bfd5fc13107616efb2a8d5a7e5b27a6f242","observation_id":"488c3faf-4f22-4399-990f-390163aeee1e","resolution":{"observed_at":"2026-08-14T04:20:28.298248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11995","last_updated":"2022-06-13T17:03:27Z","snapshot_observed_at":"2026-08-13T15:55:36.862010Z","submitted_at":"2022-04-25T23:25:00Z","title":"Ergomagnetosphere, Ejection Disc, Magnetopause in M87. I Global Flow of Mass, Angular Momentum, Energy and Current","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.11995","snapshot_observed_at":"2026-08-14T04:20:28.302125Z","title":"Global flow of mass, angular momentum, energy, and current","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.302125Z"},"links":{"cited_paper":"/paper/2204.11995","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:4723e0748bb115862a4763578c72a08f8e268272c4dd4ecbfaead2a5e11f5055","observation_id":"3c1418fe-bf08-43c7-b9ad-d6a7590d4334","resolution":{"observed_at":"2026-08-14T04:20:28.302125Z","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":"2026-08-14T04:20:28.306181Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.306181Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:9ad9ab72ef0290c8651df43985d185a645fad356439e2f22fe08040debb60f13","observation_id":"835b7f3d-6de2-4ab4-a85b-289498ab5add","resolution":{"observed_at":"2026-08-14T04:20:28.306181Z","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":"2026-08-14T04:20:28.310644Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.310644Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:08b7581fde4bde95dc83fb2569d23194084a3657af3b89cac1c4e4300bbbc2f3","observation_id":"3aa809db-9bee-4f14-90da-d68f0d071808","resolution":{"observed_at":"2026-08-14T04:20:28.310644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.02021","last_updated":"2017-05-04T21:11:14Z","snapshot_observed_at":"2026-08-05T01:36:58.801983Z","submitted_at":"2017-05-04T21:11:14Z","title":"Magnetoluminescence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.02021","snapshot_observed_at":"2026-08-14T04:20:28.314363Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.314363Z"},"links":{"cited_paper":"/paper/1705.02021","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:6f0162da641b34fbc0adc051f1e967a855b5aa6433420ee142ba003863faf168","observation_id":"df2d18a6-24e8-46a9-aef6-73d1566d8e05","resolution":{"observed_at":"2026-08-14T04:20:28.314363Z","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":"2026-08-14T04:20:28.318590Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.318590Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:e478505a6eda37b2f969076451f87feeb9fe78fcd493ce204a0aabf3354311e5","observation_id":"ab20e386-8de9-4bc0-9d89-90a9cf803741","resolution":{"observed_at":"2026-08-14T04:20:28.318590Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.06250","last_updated":"2015-09-21T14:51:46Z","snapshot_observed_at":"2026-07-06T04:30:32.328264Z","submitted_at":"2015-09-21T14:51:46Z","title":"The stratified two-sided jet of Cygnus A. Acceleration and collimation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.06250","snapshot_observed_at":"2026-08-14T04:20:28.322342Z","title":"Acceleration and collimation","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.322342Z"},"links":{"cited_paper":"/paper/1509.06250","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:197b1e218bc26af9294e0d80c57ef4a81f80e7c5d774ab710e08ce50ec6ce4a8","observation_id":"ff2c8f5c-5937-4d23-aa1b-bf7789e7dbaa","resolution":{"observed_at":"2026-08-14T04:20:28.322342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.14831","last_updated":"2020-12-29T16:14:51Z","snapshot_observed_at":"2026-08-09T09:39:46.300292Z","submitted_at":"2020-12-29T16:14:51Z","title":"Jet collimation in NGC 315 and other nearby AGN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.14831","snapshot_observed_at":"2026-08-14T04:20:28.326918Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.326918Z"},"links":{"cited_paper":"/paper/2012.14831","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:6ad458426105206b3ec5f00f0bd7c978d274688b1b12043dae9826200b6ee228","observation_id":"8375c11f-dfea-4d46-b12b-de2a5dee1dc5","resolution":{"observed_at":"2026-08-14T04:20:28.326918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0302227","last_updated":"2003-02-11T22:14:05Z","snapshot_observed_at":"2026-07-07T00:31:16.079633Z","submitted_at":"2003-02-11T22:14:05Z","title":"Interferometric Detection of Linear Polarization from Sagittarius A* at 230 GHz","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0302227","snapshot_observed_at":"2026-08-14T04:20:28.331527Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.331527Z"},"links":{"cited_paper":"/paper/astro-ph/0302227","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:f6be50506e76acc4fbbdae3cf6e4a948842840a007b5f118fc092c638c0e79a7","observation_id":"c9d6d516-940a-44eb-9b60-92510f9e61ad","resolution":{"observed_at":"2026-08-14T04:20:28.331527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.00066","last_updated":"2017-12-07T09:16:39Z","snapshot_observed_at":"2026-07-06T05:49:19.425378Z","submitted_at":"2017-06-30T23:32:05Z","title":"What is the Hidden Depolarization Mechanism in Low Luminosity AGN?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.00066","snapshot_observed_at":"2026-08-14T04:20:28.335522Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.335522Z"},"links":{"cited_paper":"/paper/1707.00066","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:0a82a7a430602041bad94fea964a1dbe165664cc2f47903c8d280e75f5580a02","observation_id":"9107c41f-9b6a-4361-8d16-7fbdb3a532c9","resolution":{"observed_at":"2026-08-14T04:20:28.335522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07317","last_updated":"2018-10-16T23:52:12Z","snapshot_observed_at":"2026-07-06T07:08:47.507946Z","submitted_at":"2018-10-16T23:52:12Z","title":"ALMA Polarimetry of Sgr A*: Probing the Accretion Flow from the Event Horizon to the Bondi Radius","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07317","snapshot_observed_at":"2026-08-14T04:20:28.339542Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.339542Z"},"links":{"cited_paper":"/paper/1810.07317","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:1f4a480d7b613c3abf6a55d5bbf52b7b42f23c8e383adcec496750ad6f60576a","observation_id":"faa6e2ec-e712-4be4-b069-f6a8721d87a3","resolution":{"observed_at":"2026-08-14T04:20:28.339542Z","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":"2026-08-14T04:20:28.342878Z","title":"Galaxies , year = 2019, month = aug, volume =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.342878Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:6ee2ffd1ba34cb8cacd1597c7114eb289ebc5a0ea3ef7823ac21659ab6b6505e","observation_id":"5f647080-cd06-45b5-ab63-75bc93f02266","resolution":{"observed_at":"2026-08-14T04:20:28.342878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.08952","last_updated":"2021-03-09T08:29:02Z","snapshot_observed_at":"2026-07-06T10:42:15.700366Z","submitted_at":"2021-02-17T19:00:00Z","title":"The jet collimation profile at high resolution in BL Lacertae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.08952","snapshot_observed_at":"2026-08-14T04:20:28.346763Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.346763Z"},"links":{"cited_paper":"/paper/2102.08952","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:e9c35680d9b6f3df6a1481925fbd031d502fc72173a083116249c38653e6e161","observation_id":"cdd06a2f-d207-4009-a043-9a36add724a1","resolution":{"observed_at":"2026-08-14T04:20:28.346763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.06156","last_updated":"2016-07-13T17:20:27Z","snapshot_observed_at":"2026-07-06T04:56:56.003607Z","submitted_at":"2016-05-19T21:49:06Z","title":"High Resolution Linear Polarimetric Imaging for the Event Horizon Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.06156","snapshot_observed_at":"2026-08-14T04:20:28.350334Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.350334Z"},"links":{"cited_paper":"/paper/1605.06156","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:c470b07e7586639b6e6702624ec1fb04ba16f995ce93507411639c3aaeb342d6","observation_id":"6fba0c40-94ac-4e1e-b24a-ed140a7d3aed","resolution":{"observed_at":"2026-08-14T04:20:28.350334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.07088","last_updated":"2018-03-19T18:00:20Z","snapshot_observed_at":"2026-08-06T12:41:12.828405Z","submitted_at":"2018-03-19T18:00:20Z","title":"Interferometric Imaging Directly with Closure Phases and Closure Amplitudes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.07088","snapshot_observed_at":"2026-08-14T04:20:28.354487Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.354487Z"},"links":{"cited_paper":"/paper/1803.07088","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8a1a5f148a7d8c9b12ad22afb779a8cd8550f78bac2cbeae4f71a4f688cbe176","observation_id":"00b1485e-1622-4c70-9225-f0e6b2874e87","resolution":{"observed_at":"2026-08-14T04:20:28.354487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.01983","last_updated":"2019-04-09T18:29:56Z","snapshot_observed_at":"2026-08-10T12:30:09.521250Z","submitted_at":"2018-10-03T21:42:10Z","title":"Two-temperature, Magnetically Arrested Disc simulations of the jet from the supermassive black hole in M87","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.01983","snapshot_observed_at":"2026-08-14T04:20:28.358988Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.358988Z"},"links":{"cited_paper":"/paper/1810.01983","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:6e1c898d0b725d48c76ea7f4df823f68d6798451a3bd060d58ec141b4a721a21","observation_id":"c3a7239b-fcb0-4e89-a0dd-f3805730cd63","resolution":{"observed_at":"2026-08-14T04:20:28.358988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.01089","last_updated":"2021-06-02T11:45:24Z","snapshot_observed_at":"2026-08-13T19:11:56.531785Z","submitted_at":"2021-06-02T11:45:24Z","title":"Testing the magnetic flux paradigm for AGN radio loudness with a radio intermediate quasar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.01089","snapshot_observed_at":"2026-08-14T04:20:28.363281Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.363281Z"},"links":{"cited_paper":"/paper/2106.01089","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:111e6d598ecadd516c956321b9eba04c33607e39d6dc4cbd17756c81a4cb7d79","observation_id":"e1a0668f-9682-4c5f-a11a-3eea9945d09f","resolution":{"observed_at":"2026-08-14T04:20:28.363281Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.06989","last_updated":"2016-03-22T21:23:02Z","snapshot_observed_at":"2026-08-01T20:51:32.116603Z","submitted_at":"2016-03-22T21:23:02Z","title":"Exploring the nature of broadband variability in the FSRQ 3C 273","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.06989","snapshot_observed_at":"2026-08-14T04:20:28.367967Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.367967Z"},"links":{"cited_paper":"/paper/1603.06989","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:ff42100074dfe499414fc95795c5f6ec71bd9abb25a65161012966b2cbae1050","observation_id":"7297644b-bf97-4378-9ad3-78b588208a85","resolution":{"observed_at":"2026-08-14T04:20:28.367967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.0976","last_updated":"2014-04-03T15:36:48Z","snapshot_observed_at":"2026-07-06T03:40:17.732584Z","submitted_at":"2014-04-03T15:36:48Z","title":"Studies of the Jet in BL Lacertae I. Recollimation Shock and Moving Emission Features","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.0976","snapshot_observed_at":"2026-08-14T04:20:28.372588Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.372588Z"},"links":{"cited_paper":"/paper/1404.0976","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:aee722981d3ce704c85b601b2d43c14ddfdff3c85d857d7cac8fb511c4fa6f54","observation_id":"381de0d8-3b3a-4731-b841-6050f7319abb","resolution":{"observed_at":"2026-08-14T04:20:28.372588Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3599","last_updated":"2015-01-22T15:03:30Z","snapshot_observed_at":"2026-07-06T03:54:16.458401Z","submitted_at":"2014-09-11T21:17:41Z","title":"Studies of the Jet in BL Lacertae. II. Superluminal Alfv\\'en Waves","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.3599","snapshot_observed_at":"2026-08-14T04:20:28.376888Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.376888Z"},"links":{"cited_paper":"/paper/1409.3599","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:9c568b34c6797c53e3d004076325139156396cc0407e35698d1a33a5e55355fb","observation_id":"c64c8582-61d6-4f9a-a624-18d85a4a10f6","resolution":{"observed_at":"2026-08-14T04:20:28.376888Z","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":"2026-08-14T04:20:28.381722Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.381722Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:fee85e1204c28dd5e9b8a5ff32d916590ba0bff70e7732137c83a88e6cf2626e","observation_id":"2d509361-db15-4f66-b6c9-fe7dd936a959","resolution":{"observed_at":"2026-08-14T04:20:28.381722Z","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":"2026-08-14T04:20:28.390759Z","title":"Publications of Lick Observatory , year = 1918, month = jan, volume =","venue":null,"work_id":null,"year":1918},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.390759Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:9752a7c4c227d71721ac2b88fb8d90068f80717a16b481d34c26abe894a93063","observation_id":"ebd9ec71-be00-4faf-9d68-ec159bbe98b7","resolution":{"observed_at":"2026-08-14T04:20:28.390759Z","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":"2026-08-14T04:20:28.394352Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.394352Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:ed314d8de535d9c8510e456c72e44aea4e7aa9e5cac04a78e8bfa74f4d4e9b45","observation_id":"2a0d097b-4984-4a3a-89f4-70057a9ff493","resolution":{"observed_at":"2026-08-14T04:20:28.394352Z","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":"2026-08-14T04:20:28.397530Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.397530Z"},"links":{"cited_paper":"/paper/2101.08839","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:1066d05f51c73cc7cfcc38882f6a5ff34d9a66694e6d03b52808745afdbddd4a","observation_id":"8b0621bc-9156-4a57-9357-8d4bdc1b2783","resolution":{"observed_at":"2026-08-14T04:20:28.397530Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.03184","last_updated":"2020-01-09T19:01:08Z","snapshot_observed_at":"2026-07-06T08:49:33.404568Z","submitted_at":"2020-01-09T19:01:08Z","title":"Gamma-ray observations of low-luminosity active galactic nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.03184","snapshot_observed_at":"2026-08-14T04:20:28.400919Z","title":", keywords =","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.400919Z"},"links":{"cited_paper":"/paper/2001.03184","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:0b88e8ccf0391df403a67de90295cd1c39b12d22c0a27eb18c5672fb06d5834a","observation_id":"ce5c5cc4-ab4b-409b-a0b1-dc623ffad1c7","resolution":{"observed_at":"2026-08-14T04:20:28.400919Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/313403","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:20:29.704437Z","title":", keywords =","venue":null,"work_id":"44599184-8a06-4d02-9e10-ff211774c223","year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.405073Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:dbd7f74e2693d7709e3a695a5f742b3b4e1b355480ab7d6173dca26ffe91081d","observation_id":"c84c6676-afb8-418d-8542-0572ecaf730a","resolution":{"observed_at":"2026-08-14T04:20:29.708689Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/185808","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:20:29.692630Z","title":", keywords =","venue":null,"work_id":"2151e457-1b58-437f-8ee4-a80bf76f8393","year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.409932Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:f1d8fd30384c3b355cc0f71fe91d655ce2e19cfb99570b13bf0ddf88949f311d","observation_id":"dd682e36-8d17-4219-896b-41302f811ad9","resolution":{"observed_at":"2026-08-14T04:20:29.696504Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/311313","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:20:29.680519Z","title":", keywords =","venue":null,"work_id":"048f88e9-1c0f-456a-83e4-bc7eeb0db255","year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.413840Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8be9bc8fed6105c67cfbd1ed7a8f09a4106cc39ee08a3b03f9416202e8a10c84","observation_id":"4112361c-c943-42bf-8aaf-82c6e17015be","resolution":{"observed_at":"2026-08-14T04:20:29.684251Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+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":"2026-08-14T04:20:28.418215Z","title":"astro2010: The Astronomy and Astrophysics Decadal Survey , year = 2009, volume =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.418215Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:0e98bc32a83644a6c0b93a78b5cd302cd09ea245a74af0b9aad5e079e4fef086","observation_id":"c4ab8fbe-ae59-465f-b900-8e34bae59e55","resolution":{"observed_at":"2026-08-14T04:20:28.418215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0408451","last_updated":"2004-08-24T19:02:30Z","snapshot_observed_at":"2026-07-07T00:44:19.863571Z","submitted_at":"2004-08-24T19:02:30Z","title":"Obscuration and Origin of Nuclear X-ray emission in FR I Radio Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0408451","snapshot_observed_at":"2026-08-14T04:20:28.422028Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.422028Z"},"links":{"cited_paper":"/paper/astro-ph/0408451","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:1528ceaf5ebeb1868838ecca55e430670494f8d3edf6edf9b5f131eece93032b","observation_id":"29081471-e37f-4ad8-b57f-fef0fdf9ed1b","resolution":{"observed_at":"2026-08-14T04:20:28.422028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.3647","last_updated":"2014-05-14T19:55:51Z","snapshot_observed_at":"2026-08-04T10:25:36.685066Z","submitted_at":"2014-05-14T19:55:51Z","title":"A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.3647","snapshot_observed_at":"2026-08-14T04:20:28.425904Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.425904Z"},"links":{"cited_paper":"/paper/1405.3647","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:80ace5f677cb6a9edbe80de8c022d04b00921d9244cb4d49b6b1a907c02ac39a","observation_id":"105e82b0-b4aa-4467-9ef1-d8da8851e68d","resolution":{"observed_at":"2026-08-14T04:20:28.425904Z","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":"2026-08-14T04:20:28.429621Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.429621Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:d827d6c4a5f327568e167f0cf5b419bd9cb9e630837b1f00487a7694abbdf2c7","observation_id":"0b695ab4-afe9-475c-876a-0b06b826ffff","resolution":{"observed_at":"2026-08-14T04:20:28.429621Z","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":"2026-08-14T04:20:28.433440Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.433440Z"},"links":{"cited_paper":"/paper/1906.11238","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:e36a59461ce38d0c0f40225f1be33c4745a3f9d8dd0a1d93d0fb2da1feb823e5","observation_id":"14fd6517-d5cd-4dc3-a8bf-bb758ab24eb7","resolution":{"observed_at":"2026-08-14T04:20:28.433440Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11239","last_updated":"2019-06-26T18:06:47Z","snapshot_observed_at":"2026-08-13T20:35:04.499769Z","submitted_at":"2019-06-26T18:06:47Z","title":"First M87 Event Horizon Telescope Results. II. Array and Instrumentation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11239","snapshot_observed_at":"2026-08-14T04:20:28.438258Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.438258Z"},"links":{"cited_paper":"/paper/1906.11239","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:177456fbb422e0fc8136280f18775e0b00e8aff15e58fdd1a295a177ab7650dc","observation_id":"85ac743f-241a-46f8-91de-993154676d18","resolution":{"observed_at":"2026-08-14T04:20:28.438258Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11240","last_updated":"2019-06-26T18:06:48Z","snapshot_observed_at":"2026-07-06T08:03:03.170900Z","submitted_at":"2019-06-26T18:06:48Z","title":"First M87 Event Horizon Telescope Results. III. Data Processing and Calibration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11240","snapshot_observed_at":"2026-08-14T04:20:28.442331Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.442331Z"},"links":{"cited_paper":"/paper/1906.11240","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:26305f0a58febc27246f5c5613ffdca1a70e65c1775c5b3e1000c3f8dd6e2adf","observation_id":"93a6cc73-73eb-439f-b49c-5937ccacc72c","resolution":{"observed_at":"2026-08-14T04:20:28.442331Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11241","last_updated":"2019-06-26T18:06:49Z","snapshot_observed_at":"2026-08-12T15:02:17.279934Z","submitted_at":"2019-06-26T18:06:49Z","title":"First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11241","snapshot_observed_at":"2026-08-14T04:20:28.445829Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.445829Z"},"links":{"cited_paper":"/paper/1906.11241","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:27c31575c4a4fcc34c6e747069d8c5d9216e4e30f5de18e0ccc7abcb9a8399e4","observation_id":"8970d029-ded4-467e-bc1c-5d7380e7741a","resolution":{"observed_at":"2026-08-14T04:20:28.445829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11242","last_updated":"2019-06-26T18:06:50Z","snapshot_observed_at":"2026-07-06T08:03:03.170900Z","submitted_at":"2019-06-26T18:06:50Z","title":"First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11242","snapshot_observed_at":"2026-08-14T04:20:28.449453Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.449453Z"},"links":{"cited_paper":"/paper/1906.11242","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:aea3491b5c499d5fadd8f2eddbe5329e0f6e1623208fe26e3cb052fc27ff0126","observation_id":"f2799ce9-2995-4a63-a726-a8884a0a3307","resolution":{"observed_at":"2026-08-14T04:20:28.449453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11243","last_updated":"2019-06-26T18:06:51Z","snapshot_observed_at":"2026-07-06T08:03:03.170900Z","submitted_at":"2019-06-26T18:06:51Z","title":"First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11243","snapshot_observed_at":"2026-08-14T04:20:28.452940Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.452940Z"},"links":{"cited_paper":"/paper/1906.11243","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:2d13f0fef57262643559714291039a1ed58d924335bcf6bf1effe56e2e36174d","observation_id":"531589d1-b4d5-4015-962e-9dc107fed8b8","resolution":{"observed_at":"2026-08-14T04:20:28.452940Z","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":"2026-08-14T04:20:28.456416Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.456416Z"},"links":{"cited_paper":"/paper/2105.01169","citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8b42d3477c79a9093dedf0a5277fc6729d14d355a10ac85e32836c08cd766737","observation_id":"a755b644-b6e0-4b80-ba76-82080ded63fd","resolution":{"observed_at":"2026-08-14T04:20:28.456416Z","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":"2026-08-14T04:20:28.460350Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.460350Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:d3a329281665c8788f41f5c5f2d640ba7e8db15023ba9ee5b5599c80188c5627","observation_id":"5be26ddc-d05f-4d62-84f1-fc7860912fbe","resolution":{"observed_at":"2026-08-14T04:20:28.460350Z","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":"2026-08-14T04:20:28.464084Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.464084Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:93f128840716a73a35536f9e5429b6b28e72b87c3841874c603ca32f89e27273","observation_id":"9e7c8a0f-c09d-44d9-be45-b43fe5cade44","resolution":{"observed_at":"2026-08-14T04:20:28.464084Z","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":"2026-08-14T04:20:28.469393Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.469393Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:1ecd18f3750446754b761702272ba340efc0f7704fdfe116eb70eef6d16382f1","observation_id":"35f2ef71-2c95-47c2-947f-7339002c2e82","resolution":{"observed_at":"2026-08-14T04:20:28.469393Z","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":"2026-08-14T04:20:28.474795Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.474795Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:0a3fdb1c9403a920e7bb7d6a38bd85caf3ecf7533e928452afcfca1a683f120d","observation_id":"ff640563-381c-4eb2-8271-71f788040e73","resolution":{"observed_at":"2026-08-14T04:20:28.474795Z","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":"2026-08-14T04:20:28.478427Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.478427Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:66da20f40c078bfeb3ee17eb7f1be056f8f4a5a5453769447e24ac6269ede751","observation_id":"69ae8bd7-e8b6-46e6-9959-fae9e53409e7","resolution":{"observed_at":"2026-08-14T04:20:28.478427Z","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":"2026-08-14T04:20:28.482235Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.482235Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:6e6012c619163eebae9c66c5720080a4250787baf7c6ee5f79552e6d1a8efe2f","observation_id":"46ea8527-96cb-4c0f-a7e8-3ec158311c90","resolution":{"observed_at":"2026-08-14T04:20:28.482235Z","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":"2026-08-14T04:20:28.486670Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.486670Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:618d8f56019feb9bc4a7bd06c220e0e39f651a73ebf89bb72348c595e7c8810e","observation_id":"e9a98c36-926c-424d-a444-01bcaafa1ee4","resolution":{"observed_at":"2026-08-14T04:20:28.486670Z","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":"2026-08-14T04:20:28.491299Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.491299Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:3439795d527ba24203c0ba75b63fced6c11e65461fa0c549b9c31af14d67b465","observation_id":"fd43420c-7cc9-479f-a9af-bef24d0bcd01","resolution":{"observed_at":"2026-08-14T04:20:28.491299Z","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":"2026-08-14T04:20:28.495271Z","title":"Efron and C","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.495271Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:3207d154e8842942d84622668d38d816bb939338ff249c5b4d04615982390f5d","observation_id":"6325dfb8-7588-41fd-a7d3-80506aac8283","resolution":{"observed_at":"2026-08-14T04:20:28.495271Z","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":"2026-08-14T04:20:28.499254Z","title":"Synthesis Imaging in Radio Astronomy II , year = 1999, editor =","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-14T04:20:28.499254Z"},"links":{"citing_paper":"/paper/2608.10067"},"observation_digest":"sha256:8dae370b141353a198531a7e7ccb90db9d3b1593d0dcdee7d07b75452eb6a745","observation_id":"56c163cc-1204-4255-ab4d-9333e0597da6","resolution":{"observed_at":"2026-08-14T04:20:28.499254Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.10067","last_updated":"2026-08-10T18:00:00Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-14T15:10:08.610461Z","submitted_at":"2026-08-10T18:00:00Z","title":"Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":96,"verified_exact":4,"verified_fuzzy":0},"total_outbound_references":296},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 100 of 296 outbound references and 0 inbound Pith citation observations for arXiv:2608.10067."}