{"as_of":"2026-08-10T19:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5fa8b75cfbccb2944df53540d75a00669119cfca5c51ec3db04f8be8cddf541e","coverage":[{"denominator":55,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":55,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T16:30:11.651238Z","state":"measured"},{"denominator":55,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":55,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+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/2502.01150/citation-record","integrity":"/paper/2502.01150/integrity","json":"/paper/2502.01150/citation-record.json","paper":"/paper/2502.01150"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T16:30:11.370576Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.370576Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:ded4bfdf564c27bac24c78d2ec1f445125c8dcbdbc4da367f6a7de22fd0f3e6f","observation_id":"cbab720a-ec22-46a4-8ece-3b4ede6a75ee","resolution":{"observed_at":"2026-08-09T16:30:11.370576Z","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":"2026-08-09T16:30:11.377130Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.377130Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:ba42aaa7adebca6fb38d5ae7b90e29784b7e9a050d2cc7317cff814c92ff0ab6","observation_id":"21e1043e-9376-47cf-8798-51ff87b5c5a4","resolution":{"observed_at":"2026-08-09T16:30:11.377130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9506063","last_updated":"1995-06-09T13:19:55Z","snapshot_observed_at":"2026-08-06T17:03:39.287382Z","submitted_at":"1995-06-09T01:34:08Z","title":"Unified Schemes for Radio-Loud Active Galactic Nuclei","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9506063","snapshot_observed_at":"2026-08-09T16:30:11.382388Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.382388Z"},"links":{"cited_paper":"/paper/astro-ph/9506063","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:d0d9d3689e9d375e511cc3ef3efe3e056190488000ad3eae108a47430d02f23c","observation_id":"1c317332-a3e1-48fd-96e0-f7509e5b7673","resolution":{"observed_at":"2026-08-09T16:30:11.382388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.06025","last_updated":"2018-12-14T16:58:45Z","snapshot_observed_at":"2026-08-10T15:21:22.350140Z","submitted_at":"2018-12-14T16:58:45Z","title":"Relativistic Jets in Active Galactic Nuclei","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.06025","snapshot_observed_at":"2026-08-09T16:30:11.387556Z","title":"Blandford , author D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.387556Z"},"links":{"cited_paper":"/paper/1812.06025","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:17d4b375fdb600027cf4c43f33e18d2504527e8ed658b7207228fd973b6c28db","observation_id":"301c5ad0-fa17-41f8-974b-7046181e1880","resolution":{"observed_at":"2026-08-09T16:30:11.387556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.0999","last_updated":"2012-01-04T21:00:03Z","snapshot_observed_at":"2026-07-06T02:40:24.511144Z","submitted_at":"2012-01-04T21:00:03Z","title":"Spectroscopy of Broad Line Blazars from 1LAC","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.0999","snapshot_observed_at":"2026-08-09T16:30:11.392763Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.392763Z"},"links":{"cited_paper":"/paper/1201.0999","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:4d3c5ea0ae461bd9931b157d7765c22ea804d5572d0801c8eae01ca14d206085","observation_id":"3d7f21d2-5456-46c5-a401-4cc29bbf733b","resolution":{"observed_at":"2026-08-09T16:30:11.392763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.0323","last_updated":"2013-01-02T21:00:02Z","snapshot_observed_at":"2026-08-07T13:30:55.549178Z","submitted_at":"2013-01-02T21:00:02Z","title":"Spectroscopy of The Largest Ever Gamma-ray Selected BL Lac Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.0323","snapshot_observed_at":"2026-08-09T16:30:11.397825Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.397825Z"},"links":{"cited_paper":"/paper/1301.0323","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:be0334919e7a382570be05ac0b6294455cdcad51cfeb410d46b6aae4ab28df81","observation_id":"2fb50c5a-f979-40c9-8300-6ada6b9ec7d3","resolution":{"observed_at":"2026-08-09T16:30:11.397825Z","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":"2026-08-09T16:30:11.402807Z","title":"Ghisellini , author A","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.402807Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:32da9c0b18d64781b5133f9d18356d752b82395a480d55f065dad5c86030b680","observation_id":"604b6ae0-ac91-4446-aa66-bd9dca9b2752","resolution":{"observed_at":"2026-08-09T16:30:11.402807Z","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":"2026-08-09T16:30:11.407383Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.407383Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:22e3a3bfb8a42d14681e48493a1c8215face7a05c171c73f4e6a552fa91d5bda","observation_id":"a9e4379e-15f2-4048-b99e-5d8f1fe7251a","resolution":{"observed_at":"2026-08-09T16:30:11.407383Z","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":"2026-08-09T16:30:11.412423Z","title":"Maraschi , author G","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.412423Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:98d6e3ecd7688418b2a511f33d4da98065a658a4753321820045f02fec9e1b01","observation_id":"178712d8-adde-4b31-a16e-cdd08d0267f6","resolution":{"observed_at":"2026-08-09T16:30:11.412423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0008154","last_updated":"2000-08-09T21:33:13Z","snapshot_observed_at":"2026-07-07T00:12:28.123751Z","submitted_at":"2000-08-09T21:33:13Z","title":"Comptonization of Infrared Radiation from Hot Dust by Relativistic Jets in Quasars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0008154","snapshot_observed_at":"2026-08-09T16:30:11.417138Z","title":"B a \\.z ejowski , author M","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.417138Z"},"links":{"cited_paper":"/paper/astro-ph/0008154","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:6d24da09b85bbdd854a6f74e86e974f6f2a00af5bfc9ab7db1e6261fafe9e708","observation_id":"0b54512e-0e77-4043-a7ef-3dafd6a7144b","resolution":{"observed_at":"2026-08-09T16:30:11.417138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.06185","last_updated":"2017-05-17T14:43:16Z","snapshot_observed_at":"2026-08-09T18:41:27.911250Z","submitted_at":"2017-05-17T14:43:16Z","title":"Clues on High Energy Emission Mechanism from Blazar 3C 454.3 during 2015 August Flare","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.06185","snapshot_observed_at":"2026-08-09T16:30:11.421962Z","title":"Shah , author S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.421962Z"},"links":{"cited_paper":"/paper/1705.06185","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:3161e2019ffc3230ea8689ccfa9175d41eaa4dc5ba9d0415b1cb0cac560e586b","observation_id":"48a2f9e9-cd8e-4473-96fc-4cb677056cf4","resolution":{"observed_at":"2026-08-09T16:30:11.421962Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0912.2040","last_updated":"2009-12-10T16:38:42Z","snapshot_observed_at":"2026-08-07T18:55:13.001804Z","submitted_at":"2009-12-10T16:38:42Z","title":"The Spectral Energy Distribution of Fermi bright blazars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.2040","snapshot_observed_at":"2026-08-09T16:30:11.426989Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.426989Z"},"links":{"cited_paper":"/paper/0912.2040","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:d76a9d5d29830fcdf9660dc05b53dc19d927b3a537f2d38b09ecbff145257a7b","observation_id":"e5c0afed-2e0f-4980-9de7-61835c7b6a3d","resolution":{"observed_at":"2026-08-09T16:30:11.426989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.10771","last_updated":"2020-05-28T07:54:00Z","snapshot_observed_at":"2026-07-06T07:55:34.712383Z","submitted_at":"2019-05-26T09:51:57Z","title":"The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.10771","snapshot_observed_at":"2026-08-09T16:30:11.432090Z","title":"Ajello , author R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.432090Z"},"links":{"cited_paper":"/paper/1905.10771","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:7c73b86b1a5e903986602b82cf36cfe7187589e68994c14ecfa43f2ecdf7e254","observation_id":"b4efea5d-9dce-4c5c-b7f8-b6ed645ec7ce","resolution":{"observed_at":"2026-08-09T16:30:11.432090Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0807.2822","last_updated":"2008-07-17T17:47:03Z","snapshot_observed_at":"2026-07-06T01:44:52.907188Z","submitted_at":"2008-07-17T17:47:03Z","title":"Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0807.2822","snapshot_observed_at":"2026-08-09T16:30:11.436851Z","title":"Albert , author E","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.436851Z"},"links":{"cited_paper":"/paper/0807.2822","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:f293b96f4fa94c85c2ee26076f616e149f67006000c7dd3c7c137a09069a64e2","observation_id":"ef3a73a0-0888-4783-a8db-37a1c11249a2","resolution":{"observed_at":"2026-08-09T16:30:11.436851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.04434","last_updated":"2015-12-14T18:00:00Z","snapshot_observed_at":"2026-07-06T04:39:51.329643Z","submitted_at":"2015-12-14T18:00:00Z","title":"Gamma rays from the quasar PKS 1441+25: story of an escape","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.04434","snapshot_observed_at":"2026-08-09T16:30:11.441876Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.441876Z"},"links":{"cited_paper":"/paper/1512.04434","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:a48897fc6f0d1627230c369414641773df667268aa30b8946f1ef9ecf56bc063","observation_id":"54db1b1e-25fc-4854-bb05-4023c28d6097","resolution":{"observed_at":"2026-08-09T16:30:11.441876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.04761","last_updated":"2019-11-12T09:52:16Z","snapshot_observed_at":"2026-07-06T08:36:19.641682Z","submitted_at":"2019-11-12T09:52:16Z","title":"H.E.S.S. detection of very-high-energy gamma-ray emission from the quasar PKS 0736+017","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.04761","snapshot_observed_at":"2026-08-09T16:30:11.447082Z","title":"o hr , author R. Blackwell , author M. B \\","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.447082Z"},"links":{"cited_paper":"/paper/1911.04761","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:b2ca58497d7f5f312271529e82eaba5e9117a118a03f842189b1468d341a0b0d","observation_id":"e9f17d5b-4067-476d-8207-883230676ede","resolution":{"observed_at":"2026-08-09T16:30:11.447082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0202068","last_updated":"2002-02-04T08:35:06Z","snapshot_observed_at":"2026-07-07T00:24:54.447383Z","submitted_at":"2002-02-04T08:35:06Z","title":"Radiation fields of disk, BLR and torus in quasars and blazars: implications for gamma-ray absorption","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0202068","snapshot_observed_at":"2026-08-09T16:30:11.452070Z","title":"Donea , author R","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.452070Z"},"links":{"cited_paper":"/paper/astro-ph/0202068","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:f6a9bb8d5e0b4d0ac9dc111da4470265e2b9d366f0e9ccbe3718c268f0583f44","observation_id":"fa40a685-ed6f-4b13-8945-d9ef6bfdb441","resolution":{"observed_at":"2026-08-09T16:30:11.452070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02785","last_updated":"2016-03-09T05:31:09Z","snapshot_observed_at":"2026-07-06T04:48:50.430645Z","submitted_at":"2016-03-09T05:31:09Z","title":"Gamma-Gamma Absorption in the Broad Line Region Radiation Fields of Gamma-Ray Blazars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02785","snapshot_observed_at":"2026-08-09T16:30:11.457022Z","title":"B \\\"o ttcher , author P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.457022Z"},"links":{"cited_paper":"/paper/1603.02785","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:930d3545715be23e08f9bdf9d00dcf8deee4074a6d9bfee5b99c152c8b71a922","observation_id":"84007faa-8d0c-4c16-b119-fa6b2336573e","resolution":{"observed_at":"2026-08-09T16:30:11.457022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.1867","last_updated":"2012-11-28T21:27:46Z","snapshot_observed_at":"2026-07-06T02:49:37.373072Z","submitted_at":"2012-06-08T20:20:15Z","title":"Dust extinction from Balmer decrements of star-forming galaxies at 0.75<z<1.5 with HST/WFC3 spectroscopy from the WISP survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.1867","snapshot_observed_at":"2026-08-09T16:30:11.461616Z","title":"Dom \\' nguez , author B","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.461616Z"},"links":{"cited_paper":"/paper/1206.1867","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:e1c6daf7c24bb70ea93d31687ac48c266a7bc470046505b0684dadac870350b5","observation_id":"6e0360c6-5b68-4e19-a1b5-414bccdae2c0","resolution":{"observed_at":"2026-08-09T16:30:11.461616Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01157","last_updated":"2022-10-03T18:09:07Z","snapshot_observed_at":"2026-08-09T15:51:54.016034Z","submitted_at":"2022-10-03T18:09:07Z","title":"Modeling the Extragalactic Background Light and the Cosmic Star Formation History","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.01157","snapshot_observed_at":"2026-08-09T16:30:11.466531Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.466531Z"},"links":{"cited_paper":"/paper/2210.01157","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:e5d14791e9cec66916f5cbe6936a2b0334a781fb6b99d069bb690fe7893c6413","observation_id":"d0f1b834-6797-4bf8-b89d-eeffcc00eadf","resolution":{"observed_at":"2026-08-09T16:30:11.466531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.09222","last_updated":"2020-07-24T07:27:47Z","snapshot_observed_at":"2026-07-06T08:52:40.994329Z","submitted_at":"2020-01-24T23:00:53Z","title":"Progress in unveiling extreme particle acceleration in persistent astrophysical jets","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.09222","snapshot_observed_at":"2026-08-09T16:30:11.472002Z","title":"Biteau , author E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.472002Z"},"links":{"cited_paper":"/paper/2001.09222","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:c37c8e0e73c66012b462ba95784ba351a5bdfcee5d377c2f94a971bba7eb070a","observation_id":"17469ff0-dd94-4821-a994-b2f324af1d94","resolution":{"observed_at":"2026-08-09T16:30:11.472002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.3828","last_updated":"2010-04-22T02:10:11Z","snapshot_observed_at":"2026-07-06T02:09:37.445124Z","submitted_at":"2010-04-22T02:10:11Z","title":"A change in the optical polarization associated with a gamma-ray flare in the blazar 3C 279","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.3828","snapshot_observed_at":"2026-08-09T16:30:11.477141Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.477141Z"},"links":{"cited_paper":"/paper/1004.3828","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:ae2137d424637349a0824ec7a673d729893ef3c8a1ccf746fbc270407d1c4d05","observation_id":"52f8a267-41d7-42da-a134-646e45202296","resolution":{"observed_at":"2026-08-09T16:30:11.477141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.4552","last_updated":"2012-10-16T20:00:03Z","snapshot_observed_at":"2026-07-06T02:57:48.078347Z","submitted_at":"2012-10-16T20:00:03Z","title":"Herschel PACS and SPIRE observations of blazar PKS 1510-089: a case for two blazar zones","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.4552","snapshot_observed_at":"2026-08-09T16:30:11.482154Z","title":"Nalewajko , author M","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.482154Z"},"links":{"cited_paper":"/paper/1210.4552","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:ed69c172d59a0280532ea947aba4df25ddf8a10ca36b69c4e98376749ce57d3e","observation_id":"4afdb952-63d9-421e-be7d-8b5b8db1740b","resolution":{"observed_at":"2026-08-09T16:30:11.482154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.2522","last_updated":"2013-07-09T17:29:03Z","snapshot_observed_at":"2026-07-06T03:17:48.534791Z","submitted_at":"2013-07-09T17:29:03Z","title":"A Tight Connection between Gamma-Ray Outbursts and Parsec-Scale Jet Activity in the Quasar 3C 454.3","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.2522","snapshot_observed_at":"2026-08-09T16:30:11.487169Z","title":"a hteenm \\","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.487169Z"},"links":{"cited_paper":"/paper/1307.2522","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:37d7cef2648a95bb8574b5675d8f823df9feba9bf459492408fbc48a2c719216","observation_id":"cc3298ff-919a-4ef3-b88e-ec20899322ca","resolution":{"observed_at":"2026-08-09T16:30:11.487169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.05660","last_updated":"2015-02-19T18:11:33Z","snapshot_observed_at":"2026-07-06T04:09:42.648645Z","submitted_at":"2015-02-19T18:11:33Z","title":"Awakening of The High Redshift Blazar CGRaBS J0809+5341","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.05660","snapshot_observed_at":"2026-08-09T16:30:11.492241Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.492241Z"},"links":{"cited_paper":"/paper/1502.05660","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:d062664dc33b6910a5e516acb6a8dd9b66031a7813aa250a3f84e46faa6109a0","observation_id":"b7e5c5d3-d63d-40f0-9eb6-493249722a37","resolution":{"observed_at":"2026-08-09T16:30:11.492241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.07363","last_updated":"2015-01-29T07:47:00Z","snapshot_observed_at":"2026-07-06T04:07:33.068993Z","submitted_at":"2015-01-29T07:47:00Z","title":"Multi-wavelength observations of 3C 279 during the extremely bright gamma-ray flare in 2014 March-April","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.07363","snapshot_observed_at":"2026-08-09T16:30:11.498330Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.498330Z"},"links":{"cited_paper":"/paper/1501.07363","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:6352ab8d6547059986d1109ad11c49fb8e0c1244e05b32584a4d83b64049693a","observation_id":"02dd9721-2280-42f2-99ab-4af6b06c357f","resolution":{"observed_at":"2026-08-09T16:30:11.498330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.05367","last_updated":"2018-09-03T15:25:35Z","snapshot_observed_at":"2026-07-06T06:44:46.378532Z","submitted_at":"2018-06-14T05:20:41Z","title":"Detection of persistent VHE gamma-ray emission from PKS 1510-089 by the MAGIC telescopes during low states between 2012 and 2017","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.05367","snapshot_observed_at":"2026-08-09T16:30:11.503424Z","title":"a hteenm \\","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.503424Z"},"links":{"cited_paper":"/paper/1806.05367","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:ba7fbf1b1ccbb7328847feaa96c12dd24c4c2081bfd8f7baf22211ea8ca5ca70","observation_id":"88adeae4-a7f9-4dd3-93b7-3e8b55e1219c","resolution":{"observed_at":"2026-08-09T16:30:11.503424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.13657","last_updated":"2021-03-25T08:12:26Z","snapshot_observed_at":"2026-08-09T18:41:26.452037Z","submitted_at":"2021-03-25T08:12:26Z","title":"Unveiling the broadband spectral and temporal properties of PKS\\,0903-57 during its brightest flare","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.13657","snapshot_observed_at":"2026-08-09T16:30:11.508800Z","title":"Shah , author V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.508800Z"},"links":{"cited_paper":"/paper/2103.13657","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:ca83d11e76a75b03be6a569cafb79059c33521caf3ecd878de6d9ac5d0f9724a","observation_id":"24d4b6e3-7def-4c00-9777-411fd49671b8","resolution":{"observed_at":"2026-08-09T16:30:11.508800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T16:30:12.868843Z","title":"Bartolini , author F","venue":null,"work_id":"58a21d5c-4f32-4eec-8210-3eeaaa09d357","year":2023},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.514368Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:a7560690595570d32c9f51c17aad70c0e8ff8f198feb3c95025d355c24c23e3f","observation_id":"86872f05-24a4-4da4-8487-64386e78a430","resolution":{"observed_at":"2026-08-09T16:30:12.873698Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T16:30:12.853327Z","title":null,"venue":null,"work_id":"099dd207-a117-4f26-a551-c3f33b4b6f06","year":2023},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.519410Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:7e8f139c33800ed84f705366c116b3c434f821b01adbfd4c456dad401e40532a","observation_id":"4a260b5e-6268-43db-8e25-5a8860714fa2","resolution":{"observed_at":"2026-08-09T16:30:12.858119Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T16:30:12.837783Z","title":"Bartolini , title Fermi-LAT detection of renewed gamma-ray activity from the FSRQ OP 313 , journal The Astronomer's Telegram volume 16497 ( year 2024 ) pages 1","venue":null,"work_id":"3e42d66e-a190-467b-b0fc-399fe86ae093","year":2024},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.523979Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:01c6f70ed9505a1833ef4a8e9ce762830d2b2d395f17aaee9a1b7fbae091c828","observation_id":"57400fdd-4b13-46d6-a29e-826f19fac5ac","resolution":{"observed_at":"2026-08-09T16:30:12.842855Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0902.1089","last_updated":"2009-02-06T17:44:53Z","snapshot_observed_at":"2026-07-06T01:50:51.056470Z","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":"2026-08-09T16:30:11.528786Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.528786Z"},"links":{"cited_paper":"/paper/0902.1089","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:2236b1ab17dfee62d6cf898dc7a2c99fb8a3776f540cf11af892ad2dc4c76372","observation_id":"9fa9600b-760a-4a8c-91ee-72333cd65246","resolution":{"observed_at":"2026-08-09T16:30:11.528786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T16:30:12.821827Z","title":null,"venue":null,"work_id":"8c776d16-cd42-4fd0-b73d-7c0144c4390e","year":1996},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.538533Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:f0979818da8181939077fe7d61f10f032e743a26570f83b183916635fe45829c","observation_id":"441c69b7-5dce-409d-8f25-ae8a69502736","resolution":{"observed_at":"2026-08-09T16:30:12.826758Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504140","last_updated":"2005-04-06T10:22:38Z","snapshot_observed_at":"2026-08-04T02:37:28.240341Z","submitted_at":"2005-04-06T10:22:38Z","title":"The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504140","snapshot_observed_at":"2026-08-09T16:30:11.543162Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.543162Z"},"links":{"cited_paper":"/paper/astro-ph/0504140","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:8865cfb3ec5ef906f5ae68d054b1775d905f9306cfcf8d92c6071cc4c64b5432","observation_id":"c16e1fe4-9e8a-4c71-88ac-f166c4d37f40","resolution":{"observed_at":"2026-08-09T16:30:11.543162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1012.4804","last_updated":"2011-09-22T21:24:18Z","snapshot_observed_at":"2026-07-06T02:21:05.525174Z","submitted_at":"2010-12-21T21:00:01Z","title":"Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.4804","snapshot_observed_at":"2026-08-09T16:30:11.548120Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.548120Z"},"links":{"cited_paper":"/paper/1012.4804","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:86dd936d1977dd837c636582ac56e7504e6a92c311c84edd4a0a16995eae5451","observation_id":"df52e050-051a-4948-a228-e4d3bad2dd94","resolution":{"observed_at":"2026-08-09T16:30:11.548120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.2053","last_updated":"2012-09-10T16:24:43Z","snapshot_observed_at":"2026-07-06T02:55:18.980149Z","submitted_at":"2012-09-10T16:24:43Z","title":"A method for localizing energy dissipation in blazars using Fermi variability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.2053","snapshot_observed_at":"2026-08-09T16:30:11.552883Z","title":"Dotson , author M","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.552883Z"},"links":{"cited_paper":"/paper/1209.2053","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:07eabcfaa580447798e49480fd66e63f2a0c4d362d3a9945634f092eecb82b6d","observation_id":"292ff95f-255e-4d16-a7a5-193572ba5210","resolution":{"observed_at":"2026-08-09T16:30:11.552883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.1508","last_updated":"2013-02-06T20:47:38Z","snapshot_observed_at":"2026-07-06T03:05:50.205378Z","submitted_at":"2013-02-06T20:47:38Z","title":"Improved AGN light curve analysis with the z-transformed discrete correlation function","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.1508","snapshot_observed_at":"2026-08-09T16:30:11.557661Z","title":"Alexander , title Improved AGN light curve analysis with the z-transformed discrete correlation function , journal arXiv e-prints ( year 2013 ) pages arXiv:1302.1508","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.557661Z"},"links":{"cited_paper":"/paper/1302.1508","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:da81bfda057db7d5743f91bb3b8e6005b000bb04a481b86ff7b102d6780c4fb6","observation_id":"6a4ec3db-8b44-4a7b-aa36-fc6a8a35c785","resolution":{"observed_at":"2026-08-09T16:30:11.557661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.1085","last_updated":"2011-04-26T17:02:34Z","snapshot_observed_at":"2026-08-02T16:16:38.958042Z","submitted_at":"2011-01-05T21:00:03Z","title":"Search for the shortest variability at gamma rays in flat-spectrum radio quasars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.1085","snapshot_observed_at":"2026-08-09T16:30:11.567501Z","title":"Foschini , author G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.567501Z"},"links":{"cited_paper":"/paper/1101.1085","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:382e8efc0afc48f2d0257c8353b7a3baf7f046854b79d030cefd797ebe800592","observation_id":"c71ff989-612a-430e-809c-e18f23294e22","resolution":{"observed_at":"2026-08-09T16:30:11.567501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1302.4444","last_updated":"2013-03-30T14:38:21Z","snapshot_observed_at":"2026-07-06T03:06:43.390662Z","submitted_at":"2013-02-18T21:00:02Z","title":"The red blazar PMN J2345-1555 becomes blue","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1302.4444","snapshot_observed_at":"2026-08-09T16:30:11.572312Z","title":"Ghisellini , author F","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.572312Z"},"links":{"cited_paper":"/paper/1302.4444","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:706dbbda5314f897bec501b6c8ffd9ba8eb849a40bef1b5c8a23df60d05b83eb","observation_id":"9af74149-bfc1-4e22-bc8f-afdec65f30bc","resolution":{"observed_at":"2026-08-09T16:30:11.572312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T16:30:12.804993Z","title":null,"venue":null,"work_id":"597bd2e2-ecf8-477d-b579-081cb2610f41","year":1970},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.577836Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:5fd25d5731b1e42a91375ea5c2770c0ff8e3f19846849fb06da6a5f3e5b4b183","observation_id":"184b2594-2ec9-4d0b-928d-60fcc7af8f86","resolution":{"observed_at":"2026-08-09T16:30:12.810558Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9801265","last_updated":"1998-01-27T14:39:24Z","snapshot_observed_at":"2026-07-07T01:19:40.671608Z","submitted_at":"1998-01-27T14:39:24Z","title":"Particle acceleration and synchrotron emission in blazar jets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9801265","snapshot_observed_at":"2026-08-09T16:30:11.582644Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.582644Z"},"links":{"cited_paper":"/paper/astro-ph/9801265","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:1d3517352a22f66583060605127c99753700ea4b446669cc9129319b98e5d8e9","observation_id":"718ea02d-beb2-4452-9713-30cd93f4ac2c","resolution":{"observed_at":"2026-08-09T16:30:11.582644Z","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":"2026-08-09T16:30:11.587622Z","title":"Chiaberge , author G","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.587622Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:f55e910ebae8bf893f76088ae37785d3a1a8932e6f34e5430019b265899fd7f1","observation_id":"2de19e8c-ba07-4a17-b76c-8cb554effaed","resolution":{"observed_at":"2026-08-09T16:30:11.587622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.0348","last_updated":"2010-04-02T15:31:46Z","snapshot_observed_at":"2026-07-06T02:09:02.050124Z","submitted_at":"2010-04-02T15:31:46Z","title":"Gamma-ray Light Curves and Variability of Bright Fermi-Detected Blazars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.0348","snapshot_observed_at":"2026-08-09T16:30:11.592222Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.592222Z"},"links":{"cited_paper":"/paper/1004.0348","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:581e4c6821884aac2ca60e83b4ed73bda9d6d197895e7c17bd7ceeac1b9d2aae","observation_id":"b0f589ef-637a-4f8d-ab1b-515ca347d6da","resolution":{"observed_at":"2026-08-09T16:30:11.592222Z","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":"2026-08-09T16:30:11.596814Z","title":"Ghisellini , author F","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.596814Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:683178432f1989656255fda5551757450555d931c8d71e08dec740bf0fee5461","observation_id":"01fe3a5b-8806-4c73-b704-9162c5437569","resolution":{"observed_at":"2026-08-09T16:30:11.596814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.10849","last_updated":"2021-01-26T15:14:53Z","snapshot_observed_at":"2026-08-03T01:17:37.061677Z","submitted_at":"2021-01-26T15:14:53Z","title":"The Central Engines of Fermi Blazars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.10849","snapshot_observed_at":"2026-08-09T16:30:11.601156Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.601156Z"},"links":{"cited_paper":"/paper/2101.10849","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:1aefd5848b0b9af35819ce0629f44c655a00215e55b3cfc333be456d2204b2d1","observation_id":"dd1a1019-08f0-44c2-adca-d45b76a26dbf","resolution":{"observed_at":"2026-08-09T16:30:11.601156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.00685","last_updated":"2018-01-02T15:26:50Z","snapshot_observed_at":"2026-07-06T06:16:52.477660Z","submitted_at":"2018-01-02T15:26:50Z","title":"Broadband Spectral Fitting of Blazars using XSPEC","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.00685","snapshot_observed_at":"2026-08-09T16:30:11.606090Z","title":"Sahayanathan , author A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.606090Z"},"links":{"cited_paper":"/paper/1801.00685","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:da77374656288afbf92306a2a60296748c918ed591ca771bb2c4d41a9153feae","observation_id":"5d27ce2f-ae49-4425-a9cf-0c4ad4f6b2d6","resolution":{"observed_at":"2026-08-09T16:30:11.606090Z","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":"2026-08-09T16:30:11.611076Z","title":"Celotti , author G","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.611076Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:d5e65b3afbd1c18b85f3613c3b46a9087d7874bde098152537c1b0d137acbb54","observation_id":"ec24b4ca-ec4d-488a-9b43-1c773bdbf821","resolution":{"observed_at":"2026-08-09T16:30:11.611076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.04435","last_updated":"2018-01-12T19:12:17Z","snapshot_observed_at":"2026-07-06T04:39:51.329643Z","submitted_at":"2015-12-14T18:00:46Z","title":"Very-high-energy gamma-rays from the Universe's middle age: detection of the z=0.940 blazar PKS 1441+25 with MAGIC","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.04435","snapshot_observed_at":"2026-08-09T16:30:11.616047Z","title":"a hteenm \\","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.616047Z"},"links":{"cited_paper":"/paper/1512.04435","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:0d19f47c1b990635f62886c91e39029d9e3cf58479571f2c67e6a7701203f135","observation_id":"8820c10c-1684-4eeb-87f1-9bc99991cd9a","resolution":{"observed_at":"2026-08-09T16:30:11.616047Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.0734","last_updated":"2013-06-27T10:46:40Z","snapshot_observed_at":"2026-07-06T03:15:02.698703Z","submitted_at":"2013-06-04T11:32:54Z","title":"The far emission region of the gamma-ray blazar PKS B1424-418","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.0734","snapshot_observed_at":"2026-08-09T16:30:11.621060Z","title":"Tavecchio , author L","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.621060Z"},"links":{"cited_paper":"/paper/1306.0734","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:677ed44613a011d216ee3e31f2883608d43ed78f93adf7216c3b2266622d0e62","observation_id":"51489430-830e-4d2a-8eaa-4a50467554be","resolution":{"observed_at":"2026-08-09T16:30:11.621060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.08314","last_updated":"2019-06-19T19:16:11Z","snapshot_observed_at":"2026-08-09T15:47:42.610956Z","submitted_at":"2019-06-19T19:16:11Z","title":"The large gamma-ray flare of the FSRQ PKS 0346-27","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.08314","snapshot_observed_at":"2026-08-09T16:30:11.626831Z","title":"Angioni , author R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.626831Z"},"links":{"cited_paper":"/paper/1906.08314","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:59c3f3dd064affd34b6fea58331f08f14f5263d7926aa3168159833426d1a307","observation_id":"7877519d-217c-4c64-85fa-b8975086e8ab","resolution":{"observed_at":"2026-08-09T16:30:11.626831Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.04379","last_updated":"2021-11-08T10:57:26Z","snapshot_observed_at":"2026-08-02T20:53:10.924321Z","submitted_at":"2021-11-08T10:57:26Z","title":"On the Origin of Gamma-ray Flares from Bright Fermi Blazars","version":1},"cited_work":{"arxiv_id":"2111.04379","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.04379","snapshot_observed_at":"2026-08-09T16:30:11.912745Z","title":"On the Origin of Gamma-ray Flares from Bright Fermi Blazars","venue":"astro-ph.HE","work_id":"40a172cb-d095-4008-a503-c38617ec2454","year":2021},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.631847Z"},"links":{"cited_paper":"/paper/2111.04379","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:c75e7bd59b1d199b611d0f3b95c764f31ae4d275d128c80f40150dcfa9d9cd16","observation_id":"9a20e351-8d69-4f9d-90d4-6606c9db6da8","resolution":{"observed_at":"2026-08-09T16:30:11.917621Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.09137","last_updated":"2024-04-14T04:24:40Z","snapshot_observed_at":"2026-08-01T16:27:34.210172Z","submitted_at":"2024-04-14T04:24:40Z","title":"Gamma-ray variability and multi-wavelength insights into the unprecedented outburst from 4C 31.03","version":1},"cited_work":{"arxiv_id":"2404.09137","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.09137","snapshot_observed_at":"2026-08-09T16:30:11.891057Z","title":"Gamma-ray variability and multi-wavelength insights into the unprecedented outburst from 4C 31.03","venue":"astro-ph.HE","work_id":"37b0f51b-ac49-4e71-8c04-5ed26888b65b","year":2024},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.636789Z"},"links":{"cited_paper":"/paper/2404.09137","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:9f382bd1e893e0e130ccd3455614b88fc184b3e575283a0c1b9b4dcf028fee20","observation_id":"d09e7946-fa2b-43e7-8254-e8622efbcf82","resolution":{"observed_at":"2026-08-09T16:30:11.897031Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2012.11380","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T16:30:11.864596Z","title":"a hteenm \\","venue":null,"work_id":"211f73ca-ab3d-41af-a177-7673e6aa72fe","year":2020},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.641480Z"},"links":{"citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:900463100e78ca7e5a571f7cb123c0228e2fb71a4c3cc369a05e8127f5dd9d15","observation_id":"15803ef6-490d-4e7b-8bcf-31729e40f3f7","resolution":{"observed_at":"2026-08-09T16:30:11.873861Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.12680","last_updated":"2024-01-23T11:44:44Z","snapshot_observed_at":"2026-07-06T17:19:19.377937Z","submitted_at":"2024-01-23T11:44:44Z","title":"Multi-wavelength spectral modelling of the candidate neutrino blazar PKS 0735+178","version":1},"cited_work":{"arxiv_id":"2401.12680","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.12680","snapshot_observed_at":"2026-08-09T16:30:11.763022Z","title":"Multi-wavelength spectral modelling of the candidate neutrino blazar PKS 0735+178","venue":"astro-ph.HE","work_id":"1de28e5c-e565-4549-ab10-1bb4945d9466","year":2024},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.646422Z"},"links":{"cited_paper":"/paper/2401.12680","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:83f885c19e44e3f65e7da2c388b4c2f752d7e00726ebf1852ec8bce5befd69e2","observation_id":"9cf798ae-9bad-4998-a93e-e291e178afcf","resolution":{"observed_at":"2026-08-09T16:30:11.770417Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1502.04699","last_updated":"2015-04-02T07:12:16Z","snapshot_observed_at":"2026-08-09T18:40:39.178275Z","submitted_at":"2015-02-16T21:00:06Z","title":"Rapid Variability of Blazar 3C 279 during Flaring States in 2013-2014 with Joint Fermi-LAT, NuSTAR, Swift, and Ground-Based Multi-wavelength Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.04699","snapshot_observed_at":"2026-08-09T16:30:11.651238Z","title":"Hayashida , author K","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-09T16:30:11.651238Z"},"links":{"cited_paper":"/paper/1502.04699","citing_paper":"/paper/2502.01150"},"observation_digest":"sha256:22ee6846cdddbf179d9402113249a74ef60a93c3c9ebfb0c270bbf9b578b0f76","observation_id":"db67056b-c943-4939-8e70-af0b4286236e","resolution":{"observed_at":"2026-08-09T16:30:11.651238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2502.01150","last_updated":"2025-02-04T06:32:40Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-09T20:56:01.171635Z","submitted_at":"2025-02-03T08:42:05Z","title":"Deciphering the Multi-Wavelength Flares of the Most Distant Very High-Energy (>100 GeV) Gamma-ray Emitting Blazar"},"reference_resolution":{"displayed":55,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":49,"verified_exact":4,"verified_fuzzy":2},"total_outbound_references":55},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 55 of 55 outbound references and 0 inbound Pith citation observations for arXiv:2502.01150."}