{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:MAZR6TLUW2I36KWQREABKCDQIQ","short_pith_number":"pith:MAZR6TLU","schema_version":"1.0","canonical_sha256":"60331f4d74b691bf2ad089001508704437db09f9be9c4ef7ac95740f1d740596","source":{"kind":"arxiv","id":"1411.4915","version":2},"attestation_state":"computed","paper":{"title":"Gamma-ray flaring activity from the gravitationally lensed blazar PKS 1830-211 observed by Fermi LAT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Allafort, A. De Angelis, A. Drlica-Wagner, A. Morselli, A. P. Waite, A. Reimer, A. S. Johnson, A. W. Borgland, B. Lott, B. L. Winer, C. C. Cheung, C. Cecchi, C. D. Dermer, C. Favuzzi, C. Romoli, C. Sgr\\`o, D. Bastieri, D. Bulmash, D. F. Torres, D. Gasparrini, D. Hadasch, D. J. Thompson, D. Paneque, E. Bonamente, E. Cavazzuti, E. Charles, E. Hays, E. J. Siskind, E. Nuss, E. Troja, F. D'Ammando, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Piron, G. A. Caliandro, G. Barbiellini, G. Chiaro, G. J\\`ohannesson, G. M. Madejski, G. Pivato, G. Spandre, G. Tosti, G. Vianello, H. Takahashi, I. A. Grenier, I. V. Moskalenko, J. Bregeon, J. B. Thayer, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. E. Grove, J. Finke, J. G. Thayer, J. Kn\\\"odlseder, J. Lande, J. Mehault, J. S. Perkins, J. Vandenbroucke, K. Bechtol, K. S. Wood, L. Baldini, L. C. Reyes, L. Latronico, L. Tibaldo, M. A. Amin, M. Ackermann, M. Ajello, M. Brigida, M. E. Monzani, M. Giroletti, M. Hayashida, M. Kuss, M. N. Lovellette, M. N. Mazziotta, M. Ohno, M. Pesce-Rollins, M. Razzano, M. Roth, M. S. Jackson, M. Tinivella, M. Werner, N. Gehrels, N. Giglietto, O. Reimer, P. A. Caraveo, P. F. Michelson, P. Fusco, P. Lubrano, P. M. Saz Parkinson, P. S. Drell, P. Spinelli, R. A. Cameron, R. Bellazzini, R. Buehler, R. Claus, R. D. Blandford, R. E. Hughes, R. H. D. Corbet, R. Nemmen, R. Rando, S. Buson, S. Ciprini, S. Cutini, S. Guiriec, S. Larsson, S. Murgia, S. Rain\\`o, S. Ritz, T. A. Porter, T. Glanzman, The Fermi LAT Collaboration: A. A. Abdo, T. Jogler, T. Kamae, T. L. Usher, T. Mizuno, T. Ohsugi, T. Tanaka, V. Tronconi, V. Vasileiou, V. Vitale, W. B. Focke, Y. Fukazawa, Y. Inoue, Y. Takeuchi","submitted_at":"2014-11-18T17:08:36Z","abstract_excerpt":"The Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope routinely detects the highly dust-absorbed, reddened, and MeV-peaked flat spectrum radio quasar PKS 1830-211 (z=2.507). Its apparent isotropic gamma-ray luminosity (E>100 MeV) averaged over $\\sim$ 3 years of observations and peaking on 2010 October 14/15 at 2.9 X 10^{50} erg s^{-1}, makes it among the brightest high-redshift Fermi blazars. No published model with a single lens can account for all of the observed characteristics of this complex system. Based on radio observations, one expects time delayed variability to"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1411.4915","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-18T17:08:36Z","cross_cats_sorted":[],"title_canon_sha256":"2ffad50f0f54e93246313d22ab90d4889e18c3531a388ef25ef15138e57d18cc","abstract_canon_sha256":"431ae0a42cb3ebbf3a6b5385b9628fd19b3401e2f9e37496cedc1e4dc235b147"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:29.457440Z","signature_b64":"WyK75OBpL7c7sc+gJcV6Hr5jAO8u4z7bQGRaA6OfjjUJOi2Eb6a7uEEFXT3h+Gk4aDo4p16E0j4lyGXUXNTzDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"60331f4d74b691bf2ad089001508704437db09f9be9c4ef7ac95740f1d740596","last_reissued_at":"2026-05-18T01:41:29.456703Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:29.456703Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma-ray flaring activity from the gravitationally lensed blazar PKS 1830-211 observed by Fermi LAT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Allafort, A. De Angelis, A. Drlica-Wagner, A. Morselli, A. P. Waite, A. Reimer, A. S. Johnson, A. W. Borgland, B. Lott, B. L. Winer, C. C. Cheung, C. Cecchi, C. D. Dermer, C. Favuzzi, C. Romoli, C. Sgr\\`o, D. Bastieri, D. Bulmash, D. F. Torres, D. Gasparrini, D. Hadasch, D. J. Thompson, D. Paneque, E. Bonamente, E. Cavazzuti, E. Charles, E. Hays, E. J. Siskind, E. Nuss, E. Troja, F. D'Ammando, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Piron, G. A. Caliandro, G. Barbiellini, G. Chiaro, G. J\\`ohannesson, G. M. Madejski, G. Pivato, G. Spandre, G. Tosti, G. Vianello, H. Takahashi, I. A. Grenier, I. V. Moskalenko, J. Bregeon, J. B. Thayer, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. E. Grove, J. Finke, J. G. Thayer, J. Kn\\\"odlseder, J. Lande, J. Mehault, J. S. Perkins, J. Vandenbroucke, K. Bechtol, K. S. Wood, L. Baldini, L. C. Reyes, L. Latronico, L. Tibaldo, M. A. Amin, M. Ackermann, M. Ajello, M. Brigida, M. E. Monzani, M. Giroletti, M. Hayashida, M. Kuss, M. N. Lovellette, M. N. Mazziotta, M. Ohno, M. Pesce-Rollins, M. Razzano, M. Roth, M. S. Jackson, M. Tinivella, M. Werner, N. Gehrels, N. Giglietto, O. Reimer, P. A. Caraveo, P. F. Michelson, P. Fusco, P. Lubrano, P. M. Saz Parkinson, P. S. Drell, P. Spinelli, R. A. Cameron, R. Bellazzini, R. Buehler, R. Claus, R. D. Blandford, R. E. Hughes, R. H. D. Corbet, R. Nemmen, R. Rando, S. Buson, S. Ciprini, S. Cutini, S. Guiriec, S. Larsson, S. Murgia, S. Rain\\`o, S. Ritz, T. A. Porter, T. Glanzman, The Fermi LAT Collaboration: A. A. Abdo, T. Jogler, T. Kamae, T. L. Usher, T. Mizuno, T. Ohsugi, T. Tanaka, V. Tronconi, V. Vasileiou, V. Vitale, W. B. Focke, Y. Fukazawa, Y. Inoue, Y. Takeuchi","submitted_at":"2014-11-18T17:08:36Z","abstract_excerpt":"The Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope routinely detects the highly dust-absorbed, reddened, and MeV-peaked flat spectrum radio quasar PKS 1830-211 (z=2.507). Its apparent isotropic gamma-ray luminosity (E>100 MeV) averaged over $\\sim$ 3 years of observations and peaking on 2010 October 14/15 at 2.9 X 10^{50} erg s^{-1}, makes it among the brightest high-redshift Fermi blazars. No published model with a single lens can account for all of the observed characteristics of this complex system. Based on radio observations, one expects time delayed variability to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.4915","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1411.4915","created_at":"2026-05-18T01:41:29.456829+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.4915v2","created_at":"2026-05-18T01:41:29.456829+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.4915","created_at":"2026-05-18T01:41:29.456829+00:00"},{"alias_kind":"pith_short_12","alias_value":"MAZR6TLUW2I3","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_16","alias_value":"MAZR6TLUW2I36KWQ","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_8","alias_value":"MAZR6TLU","created_at":"2026-05-18T12:28:38.356838+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ","json":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ.json","graph_json":"https://pith.science/api/pith-number/MAZR6TLUW2I36KWQREABKCDQIQ/graph.json","events_json":"https://pith.science/api/pith-number/MAZR6TLUW2I36KWQREABKCDQIQ/events.json","paper":"https://pith.science/paper/MAZR6TLU"},"agent_actions":{"view_html":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ","download_json":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ.json","view_paper":"https://pith.science/paper/MAZR6TLU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.4915&json=true","fetch_graph":"https://pith.science/api/pith-number/MAZR6TLUW2I36KWQREABKCDQIQ/graph.json","fetch_events":"https://pith.science/api/pith-number/MAZR6TLUW2I36KWQREABKCDQIQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ/action/storage_attestation","attest_author":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ/action/author_attestation","sign_citation":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ/action/citation_signature","submit_replication":"https://pith.science/pith/MAZR6TLUW2I36KWQREABKCDQIQ/action/replication_record"}},"created_at":"2026-05-18T01:41:29.456829+00:00","updated_at":"2026-05-18T01:41:29.456829+00:00"}