{"as_of":"2026-08-12T18:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:136b733a29335f2481eb0865d7b7abf485ed3fc957ad5bbfda579618ea477e92","coverage":[{"denominator":162,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-08-12T06:34:41.77262+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/2607.10407/citation-record","integrity":"/paper/2607.10407/integrity","json":"/paper/2607.10407/citation-record.json","paper":"/paper/2607.10407"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", year = 1970, month = apr, volume =","venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:def2ac8831a85f96f7616798956e3f82b6911116101113d001a64519579d45fa","observation_id":"64b3ea69-f20c-499c-8852-a28926de5314","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.02408","last_updated":"2018-04-06T18:00:29Z","snapshot_observed_at":"2026-07-06T06:32:10.317421Z","submitted_at":"2018-04-06T18:00:29Z","title":"On the origin of gamma rays in Fermi blazars: beyond the broad line region","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.02408","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1804.02408","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:1cbd100d0b97290c6efab8846214482afbee4d8c059395604019074fbf13d7ce","observation_id":"95d39eb1-d427-4f9a-9500-6c03ab909436","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.04166","last_updated":"2015-09-01T12:53:08Z","snapshot_observed_at":"2026-08-04T17:51:57.377517Z","submitted_at":"2015-02-14T04:45:59Z","title":"The extragalactic background light, the Hubble constant, and anomalies: conclusions from 20 years of TeV gamma-ray observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.04166","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1502.04166","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:8dd778a0ee9a970a22597435a350a818c9fccfbd038723024687533bff2c1fa5","observation_id":"d87d9c63-9a71-47e7-a509-ffb7c3c02e50","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.4661","last_updated":"2012-10-10T21:34:05Z","snapshot_observed_at":"2026-07-06T02:56:02.143664Z","submitted_at":"2012-09-20T20:22:48Z","title":"The Extragalactic Background Light and the Gamma-ray Opacity of the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.4661","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":"Astroparticle Physics , keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1209.4661","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:9d18725c988118c3b181134b3af90bf0c79d63d7be3acb2aea98786f239a2cd7","observation_id":"a57502c9-b9cf-4615-8fe0-c80ea6e4da71","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0604119","last_updated":"2006-04-06T04:25:48Z","snapshot_observed_at":"2026-07-07T00:59:35.765812Z","submitted_at":"2006-04-06T04:25:48Z","title":"The First VERITAS Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0604119","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":"Astroparticle Physics , keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0604119","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:6c70e2f16014b4a6711281cfb6d2e4997b95d6f6b97a4e443a4aa20799f6a051","observation_id":"601e94ed-2415-4526-a7d7-138952937201","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.5594","last_updated":"2015-02-20T09:02:00Z","snapshot_observed_at":"2026-07-06T03:54:59.281617Z","submitted_at":"2014-09-19T10:47:43Z","title":"The major upgrade of the MAGIC telescopes, Part II: A performance study using observations of the Crab Nebula","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.5594","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":"Astroparticle Physics , keywords =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1409.5594","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:e6d2a03255f29e30e38e1d15d6834e40d6c6ed578a59d90758f5d5e4c89fc09d","observation_id":"509e0004-3064-46fd-ab4a-03f0642e3361","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0403052","last_updated":"2004-03-02T08:59:54Z","snapshot_observed_at":"2026-07-07T00:40:56.495670Z","submitted_at":"2004-03-02T08:59:54Z","title":"The Status of the H.E.S.S. Project","version":1},"cited_work":{"arxiv_id":"astro-ph/0403052","doi":"10.1016/j.newar.2003.12.004","metadata_source":"pith","pith_arxiv_id":"astro-ph/0403052","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Status of the H.E.S.S. Project","venue":"astro-ph","work_id":"01ffb270-d74e-486d-a214-a83c18893c0e","year":2004},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0403052","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:f2fe06c24c51037d203e061282c79e37d4a0f0f2cd7756c04f860afa4fe20623","observation_id":"71391ea5-ee2a-4e5e-ac8c-154fc2249f7a","resolution":{"observed_at":"2026-07-14T12:00:26.684341Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:31.44766+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:31.44766+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.10771","last_updated":"2020-05-28T07:54:00Z","snapshot_observed_at":"2026-08-11T09:49:26.330185Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1905.10771","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:9279fe3104e391de6eba47f451f88d680ffd3e541189730b8e7458d07804082f","observation_id":"d310fc18-6c71-4aee-95d5-be49378b33dc","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.07913","last_updated":"2015-11-05T08:02:56Z","snapshot_observed_at":"2026-08-12T12:26:56.889004Z","submitted_at":"2015-10-27T14:11:41Z","title":"Spectral analysis of Fermi-LAT blazars above 50 GeV","version":2},"cited_work":{"arxiv_id":"1510.07913","doi":"10.1088/2041-8205/813/2/l34","metadata_source":"pith","pith_arxiv_id":"1510.07913","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Spectral analysis of Fermi-LAT blazars above 50 GeV","venue":"astro-ph.HE","work_id":"7165a65b-934c-4e63-8ed2-5ac434a1c013","year":2015},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1510.07913","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:833053b23319a56f6ff0d3015258d17e245626e10529d6424ee57c4b7963be86","observation_id":"a64aa644-0ab8-46ae-b065-86d23aa1a6f9","resolution":{"observed_at":"2026-07-14T12:00:26.489144Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:32.053372+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:32.053372+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":"The Astronomer's Telegram , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:587c376df05a9cbcf1c9157e3bc17351907d9b928cd94469e32f76597d06b816","observation_id":"72e6d877-8cd2-4892-92ec-1d9e0c2f47a5","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":"The Astronomer's Telegram , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:675adbe70ef230b7298a6e73ef0192ba3671992820a5099d5c7b08399e8e58d0","observation_id":"3c1f57fd-d15b-41d7-bb28-ffe00182b755","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.0291","last_updated":"2014-02-03T06:31:23Z","snapshot_observed_at":"2026-07-06T03:34:58.579637Z","submitted_at":"2014-02-03T06:31:23Z","title":"Search for Very-High-Energy Gamma Rays from the z = 0.896 Quasar 4C +55.17 with the MAGIC telescopes","version":1},"cited_work":{"arxiv_id":"1402.0291","doi":"10.1093/mnras/stu227","metadata_source":"pith","pith_arxiv_id":"1402.0291","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Search for Very-High-Energy Gamma Rays from the z = 0.896 Quasar 4C +55.17 with the MAGIC telescopes","venue":"astro-ph.HE","work_id":"dfbca423-6c12-4d4b-b36a-5ae02c58b7f3","year":2014},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1402.0291","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:c0790f96c2106f009dbbcee722e1124460184fc133f3c6696524700cc706e6bd","observation_id":"668280ae-f55f-4999-a417-a7dd7be9248d","resolution":{"observed_at":"2026-07-14T12:00:26.610148Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:32.380757+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:32.380757+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.06744","last_updated":"2024-10-09T10:25:19Z","snapshot_observed_at":"2026-08-03T18:31:08.696209Z","submitted_at":"2024-10-09T10:25:19Z","title":"Hidden by a star: the redshift and the offset broad line of the Flat Spectrum Radio Quasar PKS 0903-57","version":1},"cited_work":{"arxiv_id":"2410.06744","doi":"10.1051/0004-6361/202451609","metadata_source":"pith","pith_arxiv_id":"2410.06744","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Hidden by a star: the redshift and the offset broad line of the Flat Spectrum Radio Quasar PKS 0903-57","venue":"astro-ph.HE","work_id":"c5a1e99e-4f48-45a6-a985-4a5385495a44","year":2024},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2410.06744","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d930e16d192674970102cb4b233dbc6eb7762ba7f5cb3ce89e9057529ccc8ee6","observation_id":"eafae474-fb38-4dd3-ad65-1d7da32b13ff","resolution":{"observed_at":"2026-07-14T12:00:26.707958Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:32.647116+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:32.647116+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":"The Astronomer's Telegram , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:64b2a290b155627e0fd063dd51686a9fc22a5ffe5c74803d480ca655ac5a2eb3","observation_id":"50f36920-2b38-4e68-9b0a-549e1005863c","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410692","last_updated":"2004-10-28T11:39:10Z","snapshot_observed_at":"2026-07-07T00:45:40.229852Z","submitted_at":"2004-10-28T11:39:10Z","title":"ESO-VLT optical spectroscopy of BL Lac objects: I. new redshifts","version":1},"cited_work":{"arxiv_id":"astro-ph/0410692","doi":"10.1086/427138","metadata_source":"pith","pith_arxiv_id":"astro-ph/0410692","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"ESO-VLT optical spectroscopy of BL Lac objects: I. new redshifts","venue":"astro-ph","work_id":"98fe1f5f-c1bc-4da9-943d-01ac806a64d3","year":2004},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0410692","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:76e5ef0d0fd336858f3367da64c3f9c72fe3a9e6d86145d8171dffabf1d66856","observation_id":"4d2570bb-8aac-4d08-9189-d90c9f83b415","resolution":{"observed_at":"2026-07-14T12:00:26.478722Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:32.896764+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:32.896764+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:a3b7eaf849cee21e56c51d2185e0397db39915c954b34fb270b0f60a737dad95","observation_id":"35896c3f-e04b-4177-a5f6-d1051f492085","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"10.1051/0004-6361/202557228","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"detection and multi-wavelength study of the z 1 blazar PKS 0346 - 27","venue":"Astronomy and Astrophysics","work_id":"4d982e76-5005-4a20-abe7-90d4b646e660","year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:eb16db3d54f41f4293f6f2537816b620ebabee4241f36ff66305c8d832f34cff","observation_id":"6ca207cd-561d-471c-bfa5-28c68fc5986e","resolution":{"observed_at":"2026-07-14T12:00:26.859287Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:33.56175+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:33.56175+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207355","last_updated":"2002-07-17T13:42:35Z","snapshot_observed_at":"2026-07-07T00:27:27.276456Z","submitted_at":"2002-07-17T13:42:35Z","title":"Broad-band continuum and line emission of the gamma-ray blazar PKS 0537-441","version":1},"cited_work":{"arxiv_id":"astro-ph/0207355","doi":"10.1051/0004-6361:20020881","metadata_source":"pith","pith_arxiv_id":"astro-ph/0207355","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Broad-band continuum and line emission of the gamma-ray blazar PKS 0537-441","venue":"astro-ph","work_id":"b1b4918e-7c06-48dc-ad15-f2c05b7e35ef","year":2002},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0207355","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:22d03e7be5093610411b3744b98f7fd2824b3f8dafc4777202df219f7e962d0e","observation_id":"934df349-6b2b-4a89-882e-1b75f37a6f59","resolution":{"observed_at":"2026-07-14T12:00:26.409894Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:33.883087+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:33.883087+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1201.0999","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:314d67ef4767a945946f29891af14f7590c67788dab2b30e2cd136fe46e970b9","observation_id":"f47f227a-6043-4ab3-8f95-18ae49553099","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.14573","last_updated":"2022-01-18T10:47:29Z","snapshot_observed_at":"2026-08-12T12:31:48.217420Z","submitted_at":"2021-12-29T14:29:30Z","title":"agnpy: An open-source python package modelling the radiative processes of jetted active galactic nuclei","version":2},"cited_work":{"arxiv_id":"2112.14573","doi":null,"metadata_source":"pith","pith_arxiv_id":"2112.14573","snapshot_observed_at":"2026-07-14T12:00:26.474803Z","title":"agnpy: An open-source python package modelling the radiative processes of jetted active galactic nuclei","venue":"astro-ph.IM","work_id":"a31ac7f4-63eb-4ae1-8f6f-a6e760b29649","year":2021},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2112.14573","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:b4268432ad90dc9ab8164740295113f338cfd0be2056e389b11b461683c6e856","observation_id":"0815f763-6751-45c3-be6f-ed15fb64a35c","resolution":{"observed_at":"2026-07-14T12:00:26.477157Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1005.3792","last_updated":"2010-06-24T07:45:32Z","snapshot_observed_at":"2026-07-06T02:10:45.145032Z","submitted_at":"2010-05-20T19:02:55Z","title":"GeV breaks in blazars as a result of gamma-ray absorption within the broad-line region","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.3792","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1005.3792","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:5c8205cb67a792db6766541083118c6cd90782f3f04e40b01d5640ba8986d453","observation_id":"21c3f4a3-f8d2-4719-ac97-712830c3aa05","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.01607","last_updated":"2023-02-14T21:24:43Z","snapshot_observed_at":"2026-08-10T15:20:32.249686Z","submitted_at":"2023-01-04T13:20:30Z","title":"The Fermi-LAT Light Curve Repository","version":2},"cited_work":{"arxiv_id":"2301.01607","doi":null,"metadata_source":"pith","pith_arxiv_id":"2301.01607","snapshot_observed_at":"2026-07-14T12:00:26.518380Z","title":"The Fermi-LAT Light Curve Repository","venue":"astro-ph.HE","work_id":"24d36a4e-15bd-48b7-b3e4-e9eea089deb8","year":2023},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2301.01607","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:000201fda1684c2407f7106a58fc3a85c62ac0b8a07a39bd07f5e7e145315f2c","observation_id":"ceb29a2b-1ca7-4a5d-80ea-94b7bda6a026","resolution":{"observed_at":"2026-07-14T12:00:26.520295Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1806.05367","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:476db356f98a298b6ef161d45d2107d3832d623faf9d308b8a2910839b96aacf","observation_id":"b67cbe29-515f-48f5-8089-333c8e9dbab2","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:90d6dca749e9b3fa730fa08071a85bac352892e152564d674c52b33d97ee2a0a","observation_id":"b90b78bd-81f3-4430-8e3c-7c612b49d008","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1512.04434","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:07ee412074ffe49ee49217fcee4a25bfacd02809b3d4f8cfc8b2489725b2a757","observation_id":"7a4d7a85-a391-4b38-bc1a-6f1d3f2e50b3","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1512.04435","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:795852b54ca7a9f1b5bdd9bb0245f78b1728d22a55a36443e455149b0769d923","observation_id":"9b6d5c67-8246-4def-8df3-d574bd4925a2","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.0595","last_updated":"2013-09-27T19:15:21Z","snapshot_observed_at":"2026-07-06T03:19:52.397836Z","submitted_at":"2013-08-02T20:00:01Z","title":"Fermi Large Area Telescope Detection of Two Very-High-Energy (E>100 GeV) Gamma-ray Photons from the z = 1.1 Blazar PKS 0426-380","version":2},"cited_work":{"arxiv_id":"1308.0595","doi":"10.1088/2041-8205/777/1/l18","metadata_source":"pith","pith_arxiv_id":"1308.0595","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Fermi Large Area Telescope Detection of Two Very-High-Energy (E>100 GeV) Gamma-ray Photons from the z = 1.1 Blazar PKS 0426-380","venue":"astro-ph.HE","work_id":"faa561be-cb1b-4fa4-85a5-036ecb60ba5f","year":2013},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1308.0595","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:90567262aa294e12a418bb07bd72c24658079d34faa8a18f993e0541267701ec","observation_id":"f2643c52-acc1-44ef-99a3-3d97bb0c4e67","resolution":{"observed_at":"2026-07-14T12:00:26.888026Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:38.333651+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:38.333651+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:26dcd6216273e2c9f6e51cfe050cb321677d8bf58067ba4e3b8ef8751b0a8328","observation_id":"5f7fbc43-af46-4225-aaef-7e5fdc844fef","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2602.22148","last_updated":"2026-04-29T08:08:37Z","snapshot_observed_at":"2026-08-12T14:16:17.173348Z","submitted_at":"2026-02-25T17:56:01Z","title":"Fermi-LAT 16-year Source List","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2602.22148","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2602.22148","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:5c683e5135fb1a55a03b0ce225b4e9e3eefd6e5cc791d5b15aec0664b1872fc6","observation_id":"48bf09b3-abeb-4139-9c74-7550ced90399","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10192","last_updated":"2024-10-14T06:26:17Z","snapshot_observed_at":"2026-08-07T10:15:53.808079Z","submitted_at":"2024-10-14T06:26:17Z","title":"Radio Morphology of Gamma-ray Sources: Double-Lobed Radio Sources","version":1},"cited_work":{"arxiv_id":"2410.10192","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.10192","snapshot_observed_at":"2026-07-14T12:00:26.876724Z","title":"Radio Morphology of Gamma-ray Sources: Double-Lobed Radio Sources","venue":"astro-ph.HE","work_id":"842cb34d-6499-40fd-bf85-b9927926a58f","year":2024},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2410.10192","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:a658959b7aa85dfbb122193aec0b1e5fb959ca4cf16b2afe3f3d86ec74cfc368","observation_id":"4daa37ab-e182-415a-90f9-438ef8c48b86","resolution":{"observed_at":"2026-07-14T12:00:26.878789Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.08497","last_updated":"2025-06-10T06:49:47Z","snapshot_observed_at":"2026-08-12T12:31:04.592286Z","submitted_at":"2025-06-10T06:49:47Z","title":"Catalog of very-high-energy emitting active galactic nuclei at high Galactic latitudes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.08497","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2506.08497","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:670100051bdfc779e06982cf84139194ecbeb845539d652b8a5cbaef1916288f","observation_id":"ec9d8f66-6cdf-4c15-a976-d79278614eef","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2025.100454","doi":"10.1016/j.jheap.2025.100454","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Journal of High Energy Astrophysics , keywords =","venue":"Journal of High Energy Astrophysics","work_id":"3c990ee4-69a9-404b-b137-a287ca3d6e53","year":2025},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:a156d1ff4fadda8dfca10ca884e68811cff3074cddd44b3a648023d4b5038b96","observation_id":"e6db7c15-842b-4b20-a789-e0a8a24d9c5b","resolution":{"observed_at":"2026-07-14T12:00:26.690464Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:39.621327+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:39.621327+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.03035","last_updated":"2021-09-28T12:25:07Z","snapshot_observed_at":"2026-08-10T20:24:00.086357Z","submitted_at":"2020-12-05T14:10:41Z","title":"An observational determination of the evolving extragalactic background light from the multiwavelength HST/CANDELS survey in the Fermi and CTA era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.03035","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2012.03035","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:2188308868d79037e5cf1f12a9edaa7fd1e2d01dac6b507fb3ef2e8209767266","observation_id":"11d2f06c-b9d9-475e-95b0-11481d13579e","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"1911.04761","doi":null,"metadata_source":"pith","pith_arxiv_id":"1911.04761","snapshot_observed_at":"2026-07-14T12:00:26.428751Z","title":"H.E.S.S. detection of very-high-energy gamma-ray emission from the quasar PKS 0736+017","venue":"astro-ph.HE","work_id":"82b3d86a-5fb8-4757-beeb-2bd1c9efcb7c","year":2019},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1911.04761","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:49ef279e210dc4ef53281376e9b9baa50f5282486b41c4570e8c190dd0152141","observation_id":"cbf9b06e-0ae6-486d-93ce-e3e5c8b33f59","resolution":{"observed_at":"2026-07-14T12:00:26.430652Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201629461","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Astronomy and Astrophysics","work_id":"50561c78-dca0-4ea8-b0d8-8b63d84a3131","year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:a9723b3f949ee4e47de00bf2ceb8094227eafd0980904117681bcae1b06e5b9b","observation_id":"e63ce29f-2150-4f2d-91eb-51cc76b54ad5","resolution":{"observed_at":"2026-07-14T12:00:26.363267Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:40.680891+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:40.680891+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-07-14T11:59:02.708257Z","title":"Astroparticle Physics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0202068","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d57b0c92d95033f055206c77f632d666fda68a52267eccc80ad42eb1d504c16e","observation_id":"1ac59df4-e767-486e-8607-a3368a01a90c","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1603.02785","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:157df571356968ebd070b526f7b3b64648b5d4577e260acd02d92eab0ad82c9a","observation_id":"966e1806-9ed6-48d6-ae67-69fc93d29470","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.06282","last_updated":"2018-04-05T15:43:06Z","snapshot_observed_at":"2026-08-05T14:44:58.772483Z","submitted_at":"2017-11-16T19:02:00Z","title":"The NuSTAR view on Hard-TeV BL Lacs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.06282","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1711.06282","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:c6a752863838629b314cbf447475b02471b710c267a1fa736b86fb09fe3abad9","observation_id":"6abfa148-7dd8-4736-8077-84372c802ebc","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:ea0e9f1cbdca274c2fdf3ccfa0d901530741b64f22ce33d8e00adc0a96b001ef","observation_id":"20d3feb5-a464-4232-8670-a4f7b8d0cf06","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/9506063","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:bde8a35528de81b17c1b0999c25f74813aa95f5438e803e3f1711a5fc09b82b4","observation_id":"efcd15c1-f3a5-490a-bb5b-603517890ada","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1812.06025","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:433b7463308f454ad65684d4830e4fd5b3d5a60c2fc840c1fa26096499455edf","observation_id":"2d796b1e-b8b1-4105-9353-8e50e60bce74","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003282","last_updated":"2000-03-20T13:47:34Z","snapshot_observed_at":"2026-08-12T16:45:41.467828Z","submitted_at":"2000-03-20T13:47:34Z","title":"Hadronic blazar models and correlated X-ray/TeV flares","version":1},"cited_work":{"arxiv_id":"astro-ph/0003282","doi":"10.1063/1.1291342","metadata_source":"pith","pith_arxiv_id":"astro-ph/0003282","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Hadronic blazar models and correlated X-ray/TeV flares","venue":"astro-ph","work_id":"cbc27e75-b88d-483c-abed-1529b02ab10a","year":2000},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0003282","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:7554857e8416d2b5703fda255787c00f3d494110284444b6c6b2714b13b4e052","observation_id":"e2f1fa25-7ab0-4b6d-924b-bfa677dc9a0c","resolution":{"observed_at":"2026-07-14T12:00:26.429508Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:42.145729+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:42.145729+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0912.2040","last_updated":"2009-12-10T16:38:42Z","snapshot_observed_at":"2026-08-10T21:14:17.437262Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2040},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/0912.2040","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:6679b2315bc64080cac94b0c0d59406006c0cf405707e8c5d1ca45fdf5c6f29d","observation_id":"0b0dcdd4-9db1-4c21-82ec-941b62af9495","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3185","last_updated":"2008-10-16T21:04:29Z","snapshot_observed_at":"2026-08-06T21:44:07.623528Z","submitted_at":"2008-08-25T14:36:24Z","title":"Gamma-Ray Studies of Blazars: Synchro-Compton Analysis of Flat Spectrum Radio Quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3185","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/0808.3185","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:3a3695b563752729d9f844b12f5f1f4a2438818e46dc6b7f2916b2058ba5aa75","observation_id":"d07212d2-d129-4aa9-a425-a99b8275b2df","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.17659","last_updated":"2025-08-25T04:46:11Z","snapshot_observed_at":"2026-08-05T16:46:04.428109Z","submitted_at":"2025-08-25T04:46:11Z","title":"The Detection of Teraelectronvolt Radiation from a Flat Spectrum Radio Quasar","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.17659","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2508.17659","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:8d695e9c9f7e8f71a0b3f155d706e6e78a6edbdec97d63d189a7c197daae8f69","observation_id":"10f5cf6f-e540-48d5-b576-af723ad47e7e","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":"The Astrophysical Journal Supplement Series , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:914d20b5de98c2f8b70688155c0aef11b93bd4ccf7fdd0c8cac12f246bc1e8f5","observation_id":"0ab83524-6dcd-47a5-9942-58cc21d03ad3","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.12546","last_updated":"2024-07-24T16:42:02Z","snapshot_observed_at":"2026-08-06T19:02:53.102574Z","submitted_at":"2023-07-24T06:24:23Z","title":"Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4)","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.12546","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2307.12546","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:0273bbd24b261e9e186e0427e059306f6b100c6abf0c759775f86d0a5ebeb485","observation_id":"e836b1b5-c297-402f-bef7-6ca3403d0310","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05409","last_updated":"2018-11-16T09:38:06Z","snapshot_observed_at":"2026-08-11T11:25:33.878699Z","submitted_at":"2018-10-12T08:48:41Z","title":"Radio Galaxies at VHE energies","version":2},"cited_work":{"arxiv_id":"1810.05409","doi":"10.3390/galaxies6040116","metadata_source":"pith","pith_arxiv_id":"1810.05409","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Radio Galaxies at VHE energies","venue":"astro-ph.HE","work_id":"bef67544-25aa-4711-b24b-ccc3ebcfb942","year":2018},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1810.05409","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d23908189df69508190cce92ae64317be9a36fe1cb8a077b7c5f37400ea0af82","observation_id":"f49a28f8-4e15-4d5e-b027-4a76efdfe78d","resolution":{"observed_at":"2026-07-14T12:00:26.549971Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:43.771005+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:43.771005+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.01559","last_updated":"2018-06-05T08:47:13Z","snapshot_observed_at":"2026-08-05T20:01:12.479196Z","submitted_at":"2018-06-05T08:47:13Z","title":"Gamma-ray flaring activity of NGC 1275 in 2016-2017 measured by MAGIC","version":1},"cited_work":{"arxiv_id":"1806.01559","doi":"10.1051/0004-6361/201832895","metadata_source":"pith","pith_arxiv_id":"1806.01559","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Gamma-ray flaring activity of NGC 1275 in 2016-2017 measured by MAGIC","venue":"astro-ph.HE","work_id":"840c05e1-0eb5-4e81-96a2-b233fa205d67","year":2018},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1806.01559","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:df9c1c41a3421e80a2075459754cdccda5fe19370626940762a7800e65614f67","observation_id":"8579718a-9bbf-4f45-bb17-c90e572d2460","resolution":{"observed_at":"2026-07-14T12:00:26.508274Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:44.067046+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:44.067046+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.09179","last_updated":"2021-12-16T20:05:56Z","snapshot_observed_at":"2026-07-06T12:19:44.050065Z","submitted_at":"2021-12-16T20:05:56Z","title":"Study of the Very High Energy emission of M87 through its broadband spectral energy distribution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.09179","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2112.09179","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:7f3eb17aa6117ab9580b2e35ea282a0832d835d29045082cabed43faafd65158","observation_id":"efb99bf8-3a6b-4764-b459-5aef9ac00435","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.5907","last_updated":"2012-06-27T10:29:37Z","snapshot_observed_at":"2026-08-12T11:18:53.446515Z","submitted_at":"2012-02-27T12:27:07Z","title":"Interpretation of the flares of M87 at TeV energies in the cloud-jet interaction scenario","version":2},"cited_work":{"arxiv_id":"1202.5907","doi":"10.1088/0004-637x/755/2/170","metadata_source":"pith","pith_arxiv_id":"1202.5907","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Interpretation of the flares of M87 at TeV energies in the cloud-jet interaction scenario","venue":"astro-ph.HE","work_id":"da892e91-ff6e-4864-ac06-2c4fe7d204fa","year":2012},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1202.5907","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:bd33001d12b36edbef2716284afed963658701321c0fedf1602bc2642378c426","observation_id":"88733879-378c-4af3-8406-8da82feab2ca","resolution":{"observed_at":"2026-07-14T12:00:26.698549Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:44.684051+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:44.684051+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.12298","last_updated":"2020-11-10T19:00:28Z","snapshot_observed_at":"2026-08-11T07:57:10.052032Z","submitted_at":"2020-05-25T18:00:06Z","title":"High-resolution VLA low radio frequency observations of the Perseus cluster: radio lobes, mini-halo and bent-jet radio galaxies","version":2},"cited_work":{"arxiv_id":"2005.12298","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.12298","snapshot_observed_at":"2026-07-14T12:00:26.575612Z","title":"High-resolution VLA low radio frequency observations of the Perseus cluster: radio lobes, mini-halo and bent-jet radio galaxies","venue":"astro-ph.GA","work_id":"c16fdef8-7422-4b16-86c9-a9f9bfb7d567","year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2005.12298","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:27128feed20986855ff366cce9966b8c5d4e3a9c8eeb9e070022b279c756ad7b","observation_id":"81db1b5e-d691-43ce-905e-e3f85bd7a834","resolution":{"observed_at":"2026-07-14T12:00:26.578105Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.09441","last_updated":"2025-02-13T16:08:43Z","snapshot_observed_at":"2026-08-10T03:27:23.122081Z","submitted_at":"2025-02-13T16:08:43Z","title":"Multiwavelength investigations of PKS 2300-18: S-shaped radio quasar with precessing jets and double-peaked broad emission-line spectrum","version":1},"cited_work":{"arxiv_id":"2502.09441","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.09441","snapshot_observed_at":"2026-07-14T12:00:26.621949Z","title":"Multiwavelength investigations of PKS 2300-18: S-shaped radio quasar with precessing jets and double-peaked broad emission-line spectrum","venue":"astro-ph.GA","work_id":"c0b42dee-75bb-4651-bd52-48b3e11db089","year":2025},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2502.09441","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:f9c4d86206936520862c2227083a574acfb2aef2ad7b52f2c2ab46a850ce84a7","observation_id":"6e7cbc34-9bb3-4819-942f-fc8b1999d332","resolution":{"observed_at":"2026-07-14T12:00:26.623800Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.08785","last_updated":"2022-03-03T09:48:00Z","snapshot_observed_at":"2026-08-09T12:24:45.486117Z","submitted_at":"2022-02-17T17:45:04Z","title":"Hunting extreme BL Lacertae blazars with Fermi-LAT","version":2},"cited_work":{"arxiv_id":"2202.08785","doi":"10.1093/mnras/stac491","metadata_source":"pith","pith_arxiv_id":"2202.08785","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Hunting extreme BL Lacertae blazars with Fermi-LAT","venue":"astro-ph.HE","work_id":"5bc875bc-ea93-44f2-8f97-9ba02a0bf0f9","year":2022},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2202.08785","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:ce0ff7ecf31dbf9a40f5f2e100b62382f18b34a20f904e991ecbea43accc9931","observation_id":"a222b01d-ad38-4206-b59c-28d200065351","resolution":{"observed_at":"2026-07-14T12:00:26.401295Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:45.649835+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:45.649835+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.09551","last_updated":"2017-07-29T19:34:22Z","snapshot_observed_at":"2026-08-08T12:40:40.502697Z","submitted_at":"2017-07-29T19:34:22Z","title":"Fermipy: An open-source Python package for analysis of Fermi-LAT Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.09551","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":"35th International Cosmic Ray Conference (ICRC2017) , year = 2017, series =","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1707.09551","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:7a7477a295b974e6739b79e6b66321ba17c8508bbde988cca5f3e2262da855ca","observation_id":"0b51bbc3-6aa0-40e2-b979-0d482ba5e1ce","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.03105","last_updated":"2025-07-03T18:22:48Z","snapshot_observed_at":"2026-08-06T20:15:35.972551Z","submitted_at":"2025-07-03T18:22:48Z","title":"Radio Morphology of Gamma-ray Sources -- II. Giant Radio Galaxies","version":1},"cited_work":{"arxiv_id":"2507.03105","doi":"10.48550/arxiv.2507.03105","metadata_source":"pith","pith_arxiv_id":"2507.03105","snapshot_observed_at":"2026-07-14T12:15:04.098795Z","title":"Radio Morphology of Gamma-ray Sources -- II. Giant Radio Galaxies","venue":"astro-ph.HE","work_id":"92e9e6dc-f5de-4232-81dd-4a73a74730eb","year":2025},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2507.03105","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:b1b53f7c5c670ede34c5e46b0f0680f20d744b9da0804027746b99481b9138c9","observation_id":"abc59c01-c516-487b-bf18-9b08e2a0ae8c","resolution":{"observed_at":"2026-07-14T12:00:26.905921Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:46.187203+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:46.187203+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:209b35fb01b6eba1cb17e04ae46e914ffd041eb9b747ac8a33090f11af641617","observation_id":"6a6e5836-4b48-4b77-98d9-854f2b26a9e9","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.08855","last_updated":"2018-08-27T14:11:41Z","snapshot_observed_at":"2026-08-05T13:26:32.307214Z","submitted_at":"2018-08-27T14:11:41Z","title":"Evidence of jet-clump interaction: a flip of the radio jet head of 3C~84","version":1},"cited_work":{"arxiv_id":"1808.08855","doi":null,"metadata_source":"pith","pith_arxiv_id":"1808.08855","snapshot_observed_at":"2026-07-14T12:00:26.620104Z","title":"Evidence of jet-clump interaction: a flip of the radio jet head of 3C~84","venue":"astro-ph.HE","work_id":"7cc83b76-a20d-477c-abae-67c0660e2492","year":2018},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1808.08855","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:ab1e6b1c5a89252d5f32d6e1bd980c4482d98cc63e155f3b684cd8ec91dc75c7","observation_id":"296e233c-fb7b-4d75-adfa-11f2bcca924a","resolution":{"observed_at":"2026-07-14T12:00:26.622156Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":"Galaxies , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:f3ed4db7d6c82d689805fecd2dd2d37f8d3192ef7adc9d76fb06c8e44718299d","observation_id":"e4ceb53b-5f79-4ca1-ab5b-fcf7e7415eb4","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.10504","last_updated":"2017-11-28T19:00:08Z","snapshot_observed_at":"2026-07-06T06:11:40.457629Z","submitted_at":"2017-11-28T19:00:08Z","title":"LOFAR-Bo\\\"otes: Properties of high- and low-excitation radio galaxies at $0.5 < z < 2.0$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.10504","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1711.10504","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:f8062dbff1827d651ff3d12ed6745172ace5c8bde3f5a09717212643e99f0b9d","observation_id":"4154cab5-7026-4e68-a057-fa9ff3328292","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.06833","last_updated":"2020-02-17T08:34:54Z","snapshot_observed_at":"2026-08-12T16:52:57.057680Z","submitted_at":"2020-02-17T08:34:54Z","title":"Morphology of TeV gamma-ray emission from the kpc scale jets in radio galaxies","version":1},"cited_work":{"arxiv_id":"2002.06833","doi":"10.3847/1538-4357/ab774b","metadata_source":"pith","pith_arxiv_id":"2002.06833","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Morphology of TeV gamma-ray emission from the kpc scale jets in radio galaxies","venue":"astro-ph.HE","work_id":"ebaf9edf-5266-40ac-abb6-8fc5bb35d7a6","year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2002.06833","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:71a3faa1e657db27ddb92127e5eb8f6609fb9b0f4dcd081a8b45b39836b8061c","observation_id":"065995c2-a949-4a00-8e53-cc7614061e3b","resolution":{"observed_at":"2026-07-14T12:00:26.761706Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:47.564651+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:47.564651+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1809.08144","last_updated":"2018-09-21T14:29:08Z","snapshot_observed_at":"2026-08-10T16:51:45.869625Z","submitted_at":"2018-09-21T14:29:08Z","title":"The distribution and lifetime of powerful radio galaxies as a function of environment and redshift","version":1},"cited_work":{"arxiv_id":"1809.08144","doi":"10.1038/s41598-018-33532-6","metadata_source":"pith","pith_arxiv_id":"1809.08144","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The distribution and lifetime of powerful radio galaxies as a function of environment and redshift","venue":"astro-ph.HE","work_id":"15aad8e1-5a73-46b5-8a0e-c6aa6ca3f054","year":2018},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1809.08144","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:fc4bf84d4aa8cc66eec23517eb23381bc30c620e4388867ddf12b8c45292646b","observation_id":"1006b7fa-9316-4477-9f26-e50beac7c110","resolution":{"observed_at":"2026-07-14T12:00:26.393166Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[{"edge_observation":{"observed_at":"2026-07-15T06:31:00.83654+00:00","source":"paper_reference_links","state":"open"},"event_date":"2019-04-15","event_type":"correction","notice_doi":"10.1038/s41598-019-41871-1","provenance":{"observed_at":"2026-07-11T03:05:15.310369+00:00","source":"crossref","source_record_id":"10.1038/s41598-019-41871-1->10.1038/s41598-018-33532-6:correction"}}],"reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.03110","last_updated":"2020-05-06T19:57:26Z","snapshot_observed_at":"2026-07-06T09:18:15.568507Z","submitted_at":"2020-05-06T19:57:26Z","title":"VERITAS Discovery of VHE Emission from the Radio Galaxy 3C 264: A Multi-Wavelength Study","version":1},"cited_work":{"arxiv_id":"2005.03110","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.03110","snapshot_observed_at":"2026-07-14T12:00:26.700623Z","title":"VERITAS Discovery of VHE Emission from the Radio Galaxy 3C 264: A Multi-Wavelength Study","venue":"astro-ph.HE","work_id":"056a64f9-9a36-45f1-bd1d-d2d17c80109d","year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2005.03110","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:07336a61a75f391b4164fe42637b49e4a4ce0235bf6d9b38f1cea525e6fb12c4","observation_id":"19955694-f2c1-4522-8d1a-b9bdcf946795","resolution":{"observed_at":"2026-07-14T12:00:26.702201Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.13181","last_updated":"2021-10-25T18:04:37Z","snapshot_observed_at":"2026-07-06T12:01:37.448605Z","submitted_at":"2021-10-25T18:04:37Z","title":"Variability and Spectral Characteristics of Three Flaring Gamma-ray Quasars Observed by VERITAS and Fermi-LAT","version":1},"cited_work":{"arxiv_id":"2110.13181","doi":null,"metadata_source":"pith","pith_arxiv_id":"2110.13181","snapshot_observed_at":"2026-07-14T12:00:26.397590Z","title":"Variability and Spectral Characteristics of Three Flaring Gamma-ray Quasars Observed by VERITAS and Fermi-LAT","venue":"astro-ph.HE","work_id":"3738700c-d8ec-4fa4-a4b8-0f70c18ecccd","year":2021},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2110.13181","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:f5cf01464b973fb676d6a8c9f191207fb4a505571a1cde92ca993ab4340d7a0a","observation_id":"bc5d5589-d0d1-49e3-9bc1-3b82d0bb3bf3","resolution":{"observed_at":"2026-07-14T12:00:26.399384Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1101.4645","last_updated":"2011-03-04T13:29:02Z","snapshot_observed_at":"2026-08-03T14:39:57.695779Z","submitted_at":"2011-01-24T20:51:14Z","title":"MAGIC discovery of VHE Emission from the FSRQ PKS 1222+21","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.4645","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1101.4645","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:9e0847ffd7edd5aaea7d7462c68adb8f61189c162f62e551e4d01622b73c7d75","observation_id":"e3d87ff0-c766-4ffe-9ea5-27ebe07d43de","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.04075","last_updated":"2022-06-08T18:00:02Z","snapshot_observed_at":"2026-08-05T04:16:41.280852Z","submitted_at":"2022-06-08T18:00:02Z","title":"The isotropic $\\gamma$-ray emission above 100 GeV: where do very high energy $\\gamma$ rays come from?","version":1},"cited_work":{"arxiv_id":"2206.04075","doi":"10.3847/1538-4357/ac771d","metadata_source":"pith","pith_arxiv_id":"2206.04075","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The isotropic $\\gamma$-ray emission above 100 GeV: where do very high energy $\\gamma$ rays come from?","venue":"astro-ph.HE","work_id":"26591718-65d6-427c-b9b6-9cab0ba2025c","year":2022},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2206.04075","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:062763b4050f4771ee348f4ad2f80985f6cf22061e81e1e7e5834fc77aa96ff9","observation_id":"0f2a3716-005f-4ec3-9491-29d631f64376","resolution":{"observed_at":"2026-07-14T12:00:26.373934Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:49.126265+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:49.126265+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04591","last_updated":"2024-02-23T02:05:29Z","snapshot_observed_at":"2026-07-06T17:26:39.109878Z","submitted_at":"2024-02-07T05:29:54Z","title":"Fermi Large Area Telescope Detection of Gamma-Rays from NGC 6251 Radio Lobe","version":2},"cited_work":{"arxiv_id":"2402.04591","doi":"10.3847/1538-4357/ad2e07","metadata_source":"pith","pith_arxiv_id":"2402.04591","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Fermi Large Area Telescope Detection of Gamma-Rays from NGC 6251 Radio Lobe","venue":"astro-ph.HE","work_id":"70c5a233-272a-4422-bddd-a899d0eb8831","year":2024},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2402.04591","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:c13c61db00618d9a070c10b01ffb777302ab48674026385f52133776382f4339","observation_id":"9b1e342c-02e2-4e68-96ad-2d5edb60c389","resolution":{"observed_at":"2026-07-14T12:00:26.850338Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:49.498727+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:49.498727+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.14019","last_updated":"2022-04-29T11:28:42Z","snapshot_observed_at":"2026-07-06T13:05:04.107254Z","submitted_at":"2022-04-29T11:28:42Z","title":"High energy emission component, population, and contribution to the extragalactic gamma-ray background of gamma-ray emitting radio galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.14019","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2204.14019","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:b6488bab3798089dc9ce22dd3735061117500d305466249e2908c4f470501058","observation_id":"8cc66b08-59a7-4c90-8a25-2b3bc09c72ee","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.0908","last_updated":"2013-11-18T10:41:32Z","snapshot_observed_at":"2026-08-11T18:05:39.597205Z","submitted_at":"2013-04-03T10:50:45Z","title":"Diffuse $\\gamma$-ray emission from misaligned active galactic nuclei","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.0908","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1304.0908","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:9f3610929cce5f4a1bce68d5f266d7339d62caa841e2036a83aed9b82942c5ca","observation_id":"fd8b8768-202b-474d-ab6d-b6f69c09ada5","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2001.09222","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.09222","snapshot_observed_at":"2026-07-14T12:00:26.694683Z","title":"Progress in unveiling extreme particle acceleration in persistent astrophysical jets","venue":"astro-ph.HE","work_id":"7f0b0569-506f-4886-aa7b-10d4b2fc2925","year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2001.09222","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:4682e16d7f988c09fda15f9fff47cfbef34a3b57bc702ab5a339fefd1a857f7d","observation_id":"7bded51b-bb90-4092-bb8c-ed22a274a524","resolution":{"observed_at":"2026-07-14T12:00:26.696364Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/219.3.545","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"11bf955c-adc6-4438-b21c-08835928c409","year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:141d269271269aa94efa544da23c41691f7169af0937acecc99e5484b31aca23","observation_id":"a04ff784-c018-4ab3-8947-23e3537e94d5","resolution":{"observed_at":"2026-07-14T12:00:26.529463Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:50.703511+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:50.703511+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:fc3ad0d8cbc7aa97610fbd1fddebaa7490e1822c678a52a7bca59dc0d5b343ee","observation_id":"896ea9d3-bc10-4d8e-928d-69dad2af3ebe","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", year = 1990, month = oct, volume =","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:1d634855c8e4a4e23c49e6ba7bdcfb1a3d5bb0c8eafb8401e03718d451faf825","observation_id":"d17bdf00-a954-4837-89a7-0c683d5a0c55","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0006150","last_updated":"2000-06-10T17:59:03Z","snapshot_observed_at":"2026-07-07T00:11:41.387151Z","submitted_at":"2000-06-10T17:59:03Z","title":"M87 at 90cm: A Different Picture","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0006150","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0006150","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:6852d1b9993015e785a36c2a21d4f52f872ae8ddcfa91539138742daade30d23","observation_id":"12fab2b3-2533-4865-bd66-90de5bed1a84","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.0077","last_updated":"2011-07-12T00:23:50Z","snapshot_observed_at":"2026-08-11T14:13:21.879933Z","submitted_at":"2011-04-01T04:41:04Z","title":"The radio continuum structure of Centaurus A at 1.4 GHz","version":2},"cited_work":{"arxiv_id":"1104.0077","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.0077","snapshot_observed_at":"2026-07-14T12:00:26.613249Z","title":"The radio continuum structure of Centaurus A at 1.4 GHz","venue":"astro-ph.CO","work_id":"b18f60b3-c35a-49d4-ab9c-920aef5333b7","year":2011},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1104.0077","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:ee2d7702958ea42183904aaa095f2954198c7d76afb658308854737d23b86664","observation_id":"ba14ca7d-1736-4c6c-b111-c1384fd2bf2a","resolution":{"observed_at":"2026-07-14T12:00:26.615415Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1812.01031","last_updated":"2018-12-03T19:06:31Z","snapshot_observed_at":"2026-08-09T07:19:17.085161Z","submitted_at":"2018-12-03T19:06:31Z","title":"A $\\gamma$-ray determination of the Universe's star-formation history","version":1},"cited_work":{"arxiv_id":"1812.01031","doi":null,"metadata_source":"pith","pith_arxiv_id":"1812.01031","snapshot_observed_at":"2026-07-14T12:00:26.414575Z","title":"A $\\gamma$-ray determination of the Universe's star-formation history","venue":"astro-ph.HE","work_id":"f56d489d-0b4c-4397-a849-31487fbfe4f0","year":2018},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1812.01031","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:8edd65f77a0509b5162c3fb325c6a3062b9ea8843596e5b62570d2791744597d","observation_id":"8e65c95d-fc44-4fd1-9979-560cf88e30ca","resolution":{"observed_at":"2026-07-14T12:00:26.416278Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0311077","last_updated":"2003-11-04T11:26:46Z","snapshot_observed_at":"2026-07-07T00:37:59.870819Z","submitted_at":"2003-11-04T11:26:46Z","title":"The inner kiloparsec of the jet in 3C264","version":1},"cited_work":{"arxiv_id":"astro-ph/0311077","doi":"10.1051/0004-6361:20034317","metadata_source":"pith","pith_arxiv_id":"astro-ph/0311077","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The inner kiloparsec of the jet in 3C264","venue":"astro-ph","work_id":"fb6dd633-1442-443b-a3d2-af9ff23c9c2f","year":2003},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/astro-ph/0311077","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:b6068c925ca019f165e7505a3147b50519be83d74180cf50194583b3d94abf35","observation_id":"c22cbe23-6693-41ec-9998-d2b2058b2932","resolution":{"observed_at":"2026-07-14T12:00:26.544024Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:51.789538+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:51.789538+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/112995","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astronomical Journal","work_id":"12546b09-755f-4498-9198-59e0414d16d3","year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:9b67f1444102ca22695251168bafa8ecbdafd5f6e6b0540a1b3ccd711dd56dd6","observation_id":"03213fd8-9715-47b0-a4c8-fb7f87122f74","resolution":{"observed_at":"2026-07-14T12:00:26.817288Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:52.043241+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:52.043241+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0802.1529","last_updated":"2008-06-10T15:46:33Z","snapshot_observed_at":"2026-07-06T01:38:39.345161Z","submitted_at":"2008-02-11T21:04:18Z","title":"Synchrotron Self-Compton Analysis of TeV X-ray Selected BL Lacertae Objects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0802.1529","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/0802.1529","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d604e66dfc70784a09ca36b6aa586dd134bf39ef6a641d065eb88d2694986366","observation_id":"659ae750-c5b0-4d73-bbc3-4131c164759f","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.07145","last_updated":"2016-09-22T20:00:02Z","snapshot_observed_at":"2026-08-11T08:08:06.690275Z","submitted_at":"2016-09-22T20:00:02Z","title":"The Chandra Survey of Extragalactic Sources in the 3CR Catalog: X-ray Emission from Nuclei, Jets, and Hotspots in the Chandra Archival Observations","version":1},"cited_work":{"arxiv_id":"1609.07145","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.07145","snapshot_observed_at":"2026-07-14T12:00:26.675003Z","title":"The Chandra Survey of Extragalactic Sources in the 3CR Catalog: X-ray Emission from Nuclei, Jets, and Hotspots in the Chandra Archival Observations","venue":"astro-ph.HE","work_id":"1e38eaa2-3a5d-4c75-a598-36fbabe1e0ef","year":2016},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1609.07145","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:94e7b86fc689daf0fadf2c5b87de1f1f0bfd95ad809a06ccf34cacb85767a7e3","observation_id":"818e063f-1d44-428d-af0b-8fa386767975","resolution":{"observed_at":"2026-07-14T12:00:26.677135Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/316777","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal","work_id":"d0016363-1d23-4408-acbc-c933ef68a3e9","year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:b224757cd48c941aa40eb05aa979bce1f3d87fdf3a4188e910948fa617a7a935","observation_id":"d180c915-ed53-4194-9b04-8281c9687bee","resolution":{"observed_at":"2026-07-14T12:00:26.587497Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:52.832961+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:52.832961+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":"ArXiv e-prints , archivePrefix = \"arXiv\", eprint =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d2553776d9906f8413af7fa54515a30e3d7d073cfd4c858492b21560ac87103b","observation_id":"2b65b186-6fff-40f7-bfe8-8c6a6dc3536e","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.12629","last_updated":"2020-03-27T20:34:36Z","snapshot_observed_at":"2026-08-10T15:20:27.536665Z","submitted_at":"2020-03-27T20:34:36Z","title":"Optical spectroscopic observations of gamma-ray blazar candidates. X. Results from the 2018--2019 SOAR and OAN-SPM observations of blazar candidates of uncertain type","version":1},"cited_work":{"arxiv_id":"2003.12629","doi":"10.1007/s10509-020-3727-5","metadata_source":"pith","pith_arxiv_id":"2003.12629","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Optical spectroscopic observations of gamma-ray blazar candidates. X. Results from the 2018--2019 SOAR and OAN-SPM observations of blazar candidates of uncertain type","venue":"astro-ph.HE","work_id":"2ec5931a-4fd4-4678-a1a9-d6756ce0af9f","year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2003.12629","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d7e9e9867cb473f82e0d50015e4d3c29ab483d420577ef9bbcb83a0322ab0792","observation_id":"65d1a4f3-7f0c-4fa3-af2f-4a2089d5454d","resolution":{"observed_at":"2026-07-14T12:00:26.455993Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:53.134799+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:53.134799+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.10849","last_updated":"2021-01-26T15:14:53Z","snapshot_observed_at":"2026-08-12T18:21:18.505638Z","submitted_at":"2021-01-26T15:14:53Z","title":"The Central Engines of Fermi Blazars","version":1},"cited_work":{"arxiv_id":"2101.10849","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.10849","snapshot_observed_at":"2026-07-14T12:00:26.419064Z","title":"The Central Engines of Fermi Blazars","venue":"astro-ph.HE","work_id":"2c9506a4-be19-436e-9db7-975205cc5c56","year":2021},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2101.10849","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:26a96d3e3c4dcbb404873df8ff9398003d0901c33d5c7c9d4f1959445afacaed","observation_id":"ede99d55-b682-44f6-a060-07e005f92636","resolution":{"observed_at":"2026-07-14T12:00:26.420717Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:1901f7d332e116ea00ed6c42c2b43d3443f43a5be453d818f0aa2d1a944ede08","observation_id":"f6f8942c-20bd-4080-b4ca-55b0f5469dab","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:489795b4598bb9e729b04f8cd4a301cc899693ad6c3a4ddc604fd6c53d34aff4","observation_id":"d5d40693-0ebb-4f33-906b-63c33e60cab5","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.06544","last_updated":"2019-05-21T15:44:23Z","snapshot_observed_at":"2026-07-06T07:39:32.345831Z","submitted_at":"2019-03-15T13:32:48Z","title":"The Extragalactic Gamma-Ray Background from Core Dominated Radio Galaxies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.06544","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1903.06544","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:a1d3c950b4f4403c37282fac08a5979f9364ebd3d166ad91da9cec201cba2309","observation_id":"42663953-9e08-41fd-845b-566fd9865d49","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.4302","last_updated":"2011-07-21T15:51:51Z","snapshot_observed_at":"2026-08-05T21:28:25.961783Z","submitted_at":"2011-07-21T15:51:51Z","title":"Implications for the structure of the relativistic jet from multiwavelength observations of NGC 6251","version":1},"cited_work":{"arxiv_id":"1107.4302","doi":"10.1051/0004-6361/201116808","metadata_source":"pith","pith_arxiv_id":"1107.4302","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Implications for the structure of the relativistic jet from multiwavelength observations of NGC 6251","venue":"astro-ph.CO","work_id":"f1478bd5-9004-406c-b000-43309d29ae4e","year":2011},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1107.4302","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:a8dd9787fc36742ab5bbf1e32d80849ed792db8a197c50a08313c235c1f34d50","observation_id":"3233bd55-8098-4663-aba4-6ea3ac9e440b","resolution":{"observed_at":"2026-07-14T12:00:26.351795Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:54.846943+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:54.846943+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:7772c202bedac200921ab133a69b9374558dbc878ead9f5c3d09814c11bbf021","observation_id":"0aeae0ad-123e-48d0-83db-3be2de72c297","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.12070","last_updated":"2022-10-06T16:12:33Z","snapshot_observed_at":"2026-07-06T13:55:52.772660Z","submitted_at":"2022-09-24T18:38:38Z","title":"The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope -- Data Release 3","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.12070","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2209.12070","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d01ae5c5ee4291698969231575487b9a65f4b8b7b4581a5f99ac5a7724d2bb2a","observation_id":"7e54259a-e0f6-4000-88da-828d03be6684","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":"The Astronomer's Telegram , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:6f76305437c3653992222715156f52bf7c30e34734bee1a5a51c4a59f3afd35c","observation_id":"13480a4f-a5e5-43a4-92f4-9ea4b4bdc6b7","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":"GRB Coordinates Network , year = 2020, month = sep, volume =","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:ba0b3ad022d0edecdbec7f31de395c8a398c3b7567f60c70d213cbff99be9910","observation_id":"50518207-d2bd-4cbf-87c7-6b929fc6b12f","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","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":"2026-07-14T11:59:02.708257Z","title":"The Astronomer's Telegram , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:ec765ad43310b148acdd886942fbfb6dea9119d3f588bc61e0d19d0e44f04b7a","observation_id":"d94b1a69-4ec6-4c0d-8f01-f20540edf716","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.02232","last_updated":"2021-08-04T18:24:16Z","snapshot_observed_at":"2026-08-04T18:20:11.817614Z","submitted_at":"2021-08-04T18:24:16Z","title":"Detection of new Extreme BL Lac objects with H.E.S.S. and Swift XRT","version":1},"cited_work":{"arxiv_id":"2108.02232","doi":"10.22323/1.395.0823","metadata_source":"pith","pith_arxiv_id":"2108.02232","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Detection of new Extreme BL Lac objects with H.E.S.S. and Swift XRT","venue":"astro-ph.HE","work_id":"1a21d379-fc9e-415e-a105-8901e8a0056a","year":2021},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2108.02232","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:d3faf5ae78852952e709b4a86d4fcc6b0ba796d36bccf292e9d64f35b55a833a","observation_id":"ca0838a6-5c7f-4cfd-bfc5-23a099f752fa","resolution":{"observed_at":"2026-07-14T12:00:26.578302Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-15T20:50:55.727249+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-15T20:50:55.727249+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.04176","last_updated":"2020-01-13T12:09:24Z","snapshot_observed_at":"2026-08-06T16:55:46.678699Z","submitted_at":"2020-01-13T12:09:24Z","title":"A search for Centaurus A-like features in the spectra of Fermi-LAT detected radio galaxies","version":1},"cited_work":{"arxiv_id":"2001.04176","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.04176","snapshot_observed_at":"2026-07-14T12:00:26.447548Z","title":"A search for Centaurus A-like features in the spectra of Fermi-LAT detected radio galaxies","venue":"astro-ph.HE","work_id":"2118e6d2-58dc-46cf-bb49-c5cacd97dedf","year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2001.04176","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:59c4d9702f18b13bbdbe114df6c6a32f99ebb21626be9c76cc76a16926ac84e7","observation_id":"8a7b7fb2-010b-44a7-ad12-827de3bfb80c","resolution":{"observed_at":"2026-07-14T12:00:26.449415Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:749d5dfa96fcd935d4bd62780d7ba661d114f7d35373622d20b5e8b4a62c36b3","observation_id":"9d306788-227f-43c0-80ea-c8d6655194c9","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.04823","last_updated":"2020-07-09T14:13:35Z","snapshot_observed_at":"2026-07-06T09:36:54.739609Z","submitted_at":"2020-07-09T14:13:35Z","title":"Resolving acceleration to very high energies along the Jet of Centaurus A","version":1},"cited_work":{"arxiv_id":"2007.04823","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.04823","snapshot_observed_at":"2026-07-14T12:00:26.756936Z","title":"Resolving acceleration to very high energies along the Jet of Centaurus A","venue":"astro-ph.HE","work_id":"e4399145-08e6-4b13-9e57-51fe013ec2f8","year":2020},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/2007.04823","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:66a586286793a31d80cdb56cb2a4cf90a1fd07e700f4b2d03e8f41197ae5f85c","observation_id":"fbd74192-6446-4ff1-9103-859bf3c86370","resolution":{"observed_at":"2026-07-14T12:00:26.760601Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:f9bef81a829a98ad3d79f532734dbc72644bcb4cd37e949721253922f4b64a75","observation_id":"ba9a1dc1-e611-4ec7-904d-45262e6e199a","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.08279","last_updated":"2019-11-26T07:02:47Z","snapshot_observed_at":"2026-07-06T08:22:43.075628Z","submitted_at":"2019-09-18T08:26:57Z","title":"The 3HSP catalogue of Extreme & High Synchrotron Peaked Blazars","version":4},"cited_work":{"arxiv_id":"1909.08279","doi":null,"metadata_source":"pith","pith_arxiv_id":"1909.08279","snapshot_observed_at":"2026-07-14T12:00:26.460229Z","title":"The 3HSP catalogue of Extreme & High Synchrotron Peaked Blazars","venue":"astro-ph.HE","work_id":"ac6f81a8-3315-44e6-a821-b3210f132aef","year":2019},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1909.08279","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:2eef61958e7d04e17ab6c3b3766867eaf159161665e5e61d7e74f9118b219cd7","observation_id":"4a11d6ed-ca1e-4a20-b006-fcdc5847dae9","resolution":{"observed_at":"2026-07-14T12:00:26.461908Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1006.5289","last_updated":"2010-06-29T14:41:38Z","snapshot_observed_at":"2026-07-06T02:12:12.989049Z","submitted_at":"2010-06-28T08:47:18Z","title":"Discovery of VHE gamma-rays from the BL Lac object PKS 0548-322","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1006.5289","snapshot_observed_at":"2026-07-14T11:59:02.708257Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-07-14T11:59:02.708257Z"},"links":{"cited_paper":"/paper/1006.5289","citing_paper":"/paper/2607.10407"},"observation_digest":"sha256:0d0e83c188dc6f2b2ee9d4609a1e4ca1bd78d9f3d978151e1ca048b92e97ae0b","observation_id":"d853491e-1cf1-4ec9-bb8b-d59dd0029592","resolution":{"observed_at":"2026-07-14T11:59:02.708257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.10407","last_updated":"2026-07-11T17:16:07Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-12T16:08:14.731460Z","submitted_at":"2026-07-11T17:16:07Z","title":"Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":4,"parse_uncertain":0,"unresolved":56,"verified_exact":40,"verified_fuzzy":0},"total_outbound_references":162},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 100 of 162 outbound references and 0 inbound Pith citation observations for arXiv:2607.10407."}