{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:I346X2NHN5BAKA3CAQ3657POII","short_pith_number":"pith:I346X2NH","schema_version":"1.0","canonical_sha256":"46f9ebe9a76f420503620437eefdee423ccebea869c0dfad257add6cbe1c9cb2","source":{"kind":"arxiv","id":"1106.4594","version":1},"attestation_state":"computed","paper":{"title":"Multiwavelength Observations of the VHE Blazar 1ES 2344+514","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Cannon, A. Falcone, A. Furniss, A. Imran, A. Konopelko, A. N. Otte, A. Pichel, A. Varlotta, A. Weinstein, A. W. Smith, B. Zitzer, C. M. Hui, D. A. Williams, D. Boltuch, D. Gall, D. Hanna, D. Horan, D. Kieda, D. Pandel, D. Steele, E. Aliu, F. Krennrich, G. Gyuk, G. H. Gillanders, G. H. Sembroski, G. Maier, H. J. Rose, H. Krawczynski, J. A. Toner, J. E. Ward, J. Grube, J. Holder, J. Kildea, J. P. Finley, J. Quinn, J. S. Perkins, K. Ragan, L. Ciupik, L. F. Fortson, M. Beilicke, M. J. Lang, M. Kertzman, M. Pohl, M. Schroedter, M. Theiling, M. Wood, N. Karlsson, P. Cogan, P. Colin, P. Fortin, P. Kaaret, P. Moriarty, P. T. Reynolds, R. A. Ong, R. Dickherber, R. Guenette, R. Mukherjee, R. Wagner, S. J. Fegan, S. LeBohec, S. P. Swordy, S. P. Wakely, S. Vincent, S. Wissel, T. Arlen, T. Aune, T. B. Humensky, T. C. Weekes, T. Weisgarber, V. A. Acciari, V. Bugaev, V. V. Vassiliev, W. Benbow","submitted_at":"2011-06-22T23:18:34Z","abstract_excerpt":"Multiwavelength observations of the high-frequency-peaked blazar 1ES2344+514 were performed from 2007 October to 2008 January. The campaign represents the first contemporaneous data on the object at very high energy (VHE, E >100 GeV) {\\gamma}-ray, X-ray, and UV energies. Observations with VERITAS in VHE {\\gamma}-rays yield a strong detection of 20 {\\sigma} with 633 excess events in a total exposure of 18.1 hours live-time. A strong VHE {\\gamma}-ray flare on 2007 December 7 is measured at F(>300 GeV) = (6.76 \\pm 0.62) \\times 10-11 ph cm-2 s-1, corresponding to 48% of the Crab Nebula flux. Exclu"},"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":"1106.4594","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-06-22T23:18:34Z","cross_cats_sorted":[],"title_canon_sha256":"46ddb3da1bb7c439d7229f0cef14bd420060fa107b8635581a02b13c3ffbdef9","abstract_canon_sha256":"847067420e8b85d2ed7ef0dcfeb27d3a0ef7e338182bef81d55809df7b1f2733"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:31.820941Z","signature_b64":"6uegHTOEFtAmVSw0jhQfeFSQ9KunkmZF5LGnx4rCRcKsRbTYwvn5PzFteQLpsA5fuvsLHm44yBKXn62lcYBJDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"46f9ebe9a76f420503620437eefdee423ccebea869c0dfad257add6cbe1c9cb2","last_reissued_at":"2026-05-18T02:01:31.820499Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:31.820499Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiwavelength Observations of the VHE Blazar 1ES 2344+514","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Cannon, A. Falcone, A. Furniss, A. Imran, A. Konopelko, A. N. Otte, A. Pichel, A. Varlotta, A. Weinstein, A. W. Smith, B. Zitzer, C. M. Hui, D. A. Williams, D. Boltuch, D. Gall, D. Hanna, D. Horan, D. Kieda, D. Pandel, D. Steele, E. Aliu, F. Krennrich, G. Gyuk, G. H. Gillanders, G. H. Sembroski, G. Maier, H. J. Rose, H. Krawczynski, J. A. Toner, J. E. Ward, J. Grube, J. Holder, J. Kildea, J. P. Finley, J. Quinn, J. S. Perkins, K. Ragan, L. Ciupik, L. F. Fortson, M. Beilicke, M. J. Lang, M. Kertzman, M. Pohl, M. Schroedter, M. Theiling, M. Wood, N. Karlsson, P. Cogan, P. Colin, P. Fortin, P. Kaaret, P. Moriarty, P. T. Reynolds, R. A. Ong, R. Dickherber, R. Guenette, R. Mukherjee, R. Wagner, S. J. Fegan, S. LeBohec, S. P. Swordy, S. P. Wakely, S. Vincent, S. Wissel, T. Arlen, T. Aune, T. B. Humensky, T. C. Weekes, T. Weisgarber, V. A. Acciari, V. Bugaev, V. V. Vassiliev, W. Benbow","submitted_at":"2011-06-22T23:18:34Z","abstract_excerpt":"Multiwavelength observations of the high-frequency-peaked blazar 1ES2344+514 were performed from 2007 October to 2008 January. The campaign represents the first contemporaneous data on the object at very high energy (VHE, E >100 GeV) {\\gamma}-ray, X-ray, and UV energies. Observations with VERITAS in VHE {\\gamma}-rays yield a strong detection of 20 {\\sigma} with 633 excess events in a total exposure of 18.1 hours live-time. A strong VHE {\\gamma}-ray flare on 2007 December 7 is measured at F(>300 GeV) = (6.76 \\pm 0.62) \\times 10-11 ph cm-2 s-1, corresponding to 48% of the Crab Nebula flux. Exclu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.4594","kind":"arxiv","version":1},"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":"1106.4594","created_at":"2026-05-18T02:01:31.820561+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.4594v1","created_at":"2026-05-18T02:01:31.820561+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.4594","created_at":"2026-05-18T02:01:31.820561+00:00"},{"alias_kind":"pith_short_12","alias_value":"I346X2NHN5BA","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"I346X2NHN5BAKA3C","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"I346X2NH","created_at":"2026-05-18T12:26:30.835961+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/I346X2NHN5BAKA3CAQ3657POII","json":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII.json","graph_json":"https://pith.science/api/pith-number/I346X2NHN5BAKA3CAQ3657POII/graph.json","events_json":"https://pith.science/api/pith-number/I346X2NHN5BAKA3CAQ3657POII/events.json","paper":"https://pith.science/paper/I346X2NH"},"agent_actions":{"view_html":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII","download_json":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII.json","view_paper":"https://pith.science/paper/I346X2NH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.4594&json=true","fetch_graph":"https://pith.science/api/pith-number/I346X2NHN5BAKA3CAQ3657POII/graph.json","fetch_events":"https://pith.science/api/pith-number/I346X2NHN5BAKA3CAQ3657POII/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII/action/storage_attestation","attest_author":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII/action/author_attestation","sign_citation":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII/action/citation_signature","submit_replication":"https://pith.science/pith/I346X2NHN5BAKA3CAQ3657POII/action/replication_record"}},"created_at":"2026-05-18T02:01:31.820561+00:00","updated_at":"2026-05-18T02:01:31.820561+00:00"}