{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:EYENCC4I6GRKQFZO52Y4Q27YOA","short_pith_number":"pith:EYENCC4I","schema_version":"1.0","canonical_sha256":"2608d10b88f1a2a8172eeeb1c86bf8701631318611ee12396006fd2dabf94e6a","source":{"kind":"arxiv","id":"1711.08583","version":1},"attestation_state":"computed","paper":{"title":"Broadband study of blazar 1ES 1959+650 during flaring state in 2016","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Shukla, B. J. Nagare, B. S. Acharya, D. Dorner, K. Mannheim, S. R. Patel, V. R. Chitnis","submitted_at":"2017-11-23T06:15:32Z","abstract_excerpt":"Aim : The nearby TeV blazar 1ES 1959+650 (z=0.047) was reported to be in flaring state during June - July 2016 by Fermi-LAT, FACT, MAGIC and VERITAS collaborations. We studied the spectral energy distributions (SEDs) in different states of the flare during MJD 57530 - 57589 using simultaneous multiwaveband data to understand the possible broadband emission scenario during the flare. Methods : The UV/optical and X-ray data from UVOT and XRT respectively on board Swift and high energy $\\gamma$-ray data from Fermi-LAT are used to generate multiwaveband lightcurves as well as to obtain high flux s"},"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":"1711.08583","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-23T06:15:32Z","cross_cats_sorted":[],"title_canon_sha256":"696349ad0a8065e99ae8a8fc885111047d9bf913ca79fbac2dab91678829382b","abstract_canon_sha256":"a54be4eae68e186cf5913a32b7c53eb8efcd552b3066b4b6c09ef8c49b99a253"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:20:38.209484Z","signature_b64":"hRUFN6UqEpE7/BYNNfRkDBrjasA64m77vQNvalwx7Ts6I71KYHLrE0xg26ZoOxkz600Bk6n0qU7ZfPNP9LGfCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2608d10b88f1a2a8172eeeb1c86bf8701631318611ee12396006fd2dabf94e6a","last_reissued_at":"2026-05-18T00:20:38.208953Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:20:38.208953Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Broadband study of blazar 1ES 1959+650 during flaring state in 2016","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Shukla, B. J. Nagare, B. S. Acharya, D. Dorner, K. Mannheim, S. R. Patel, V. R. Chitnis","submitted_at":"2017-11-23T06:15:32Z","abstract_excerpt":"Aim : The nearby TeV blazar 1ES 1959+650 (z=0.047) was reported to be in flaring state during June - July 2016 by Fermi-LAT, FACT, MAGIC and VERITAS collaborations. We studied the spectral energy distributions (SEDs) in different states of the flare during MJD 57530 - 57589 using simultaneous multiwaveband data to understand the possible broadband emission scenario during the flare. Methods : The UV/optical and X-ray data from UVOT and XRT respectively on board Swift and high energy $\\gamma$-ray data from Fermi-LAT are used to generate multiwaveband lightcurves as well as to obtain high flux s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.08583","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":"1711.08583","created_at":"2026-05-18T00:20:38.209034+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.08583v1","created_at":"2026-05-18T00:20:38.209034+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.08583","created_at":"2026-05-18T00:20:38.209034+00:00"},{"alias_kind":"pith_short_12","alias_value":"EYENCC4I6GRK","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_16","alias_value":"EYENCC4I6GRKQFZO","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_8","alias_value":"EYENCC4I","created_at":"2026-05-18T12:31:12.930513+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/EYENCC4I6GRKQFZO52Y4Q27YOA","json":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA.json","graph_json":"https://pith.science/api/pith-number/EYENCC4I6GRKQFZO52Y4Q27YOA/graph.json","events_json":"https://pith.science/api/pith-number/EYENCC4I6GRKQFZO52Y4Q27YOA/events.json","paper":"https://pith.science/paper/EYENCC4I"},"agent_actions":{"view_html":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA","download_json":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA.json","view_paper":"https://pith.science/paper/EYENCC4I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.08583&json=true","fetch_graph":"https://pith.science/api/pith-number/EYENCC4I6GRKQFZO52Y4Q27YOA/graph.json","fetch_events":"https://pith.science/api/pith-number/EYENCC4I6GRKQFZO52Y4Q27YOA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA/action/storage_attestation","attest_author":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA/action/author_attestation","sign_citation":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA/action/citation_signature","submit_replication":"https://pith.science/pith/EYENCC4I6GRKQFZO52Y4Q27YOA/action/replication_record"}},"created_at":"2026-05-18T00:20:38.209034+00:00","updated_at":"2026-05-18T00:20:38.209034+00:00"}