{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:RAW4QU5XQO4LWLNJQQAVTOARYU","short_pith_number":"pith:RAW4QU5X","schema_version":"1.0","canonical_sha256":"882dc853b783b8bb2da9840159b811c516f7eaa0d2d6a4d45488d118ce1d3a06","source":{"kind":"arxiv","id":"1904.10017","version":1},"attestation_state":"computed","paper":{"title":"Gamma-ray emission from the impulsive phase of the 2017 September 06 X9.3 flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"1) ((1) Ioffe Institute, 126a, 26, Alexandra L. Lysenko (1), Dmitry D. Frederiks (1), Dmitry D. Svinkin (1), Gregory D. Fleishman (3, Irkutsk, Lermontov st., Newark, NJ - United States), Polytekhnicheskaya, - Russian Federation (2) Institute of Solar-Terrestrial Physics (ISZF), - Russian Federation (3) New Jersey Institute of Technology, Sergey A. Anfinogentov (2), St. Petersburg, University Heights","submitted_at":"2019-04-22T18:21:29Z","abstract_excerpt":"We report hard X-ray and gamma-ray observations of the impulsive phase of the SOL2017-09-06T11:55 X9.3 solar flare. We focus on a high-energy part of the spectrum, >100 keV, and perform time resolved spectral analysis for a portion of the impulsive phase, recorded by the Konus-Wind experiment, that displayed prominent gamma-ray emission. Given a variety of possible emission components contributing to the gamma-ray emission, we employ a Bayesian inference to build the most probable fitting model. The analysis confidently revealed contributions from nuclear deexcitation lines, electron-positron "},"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":"1904.10017","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-04-22T18:21:29Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"12e8721f2eebb12b0a53e054e998694fcb7d53706f8d535b407bb10bba231161","abstract_canon_sha256":"5f1497dedcbf5546a8af72fcb9f8541157414caca7f2e8319dff0d5d53b1b714"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:43:49.518293Z","signature_b64":"vub5tob+QMIOb517o1ONEdJ0VtdgL2rg+5vOzcF0aOGfrgrje6T+iG9Ip9lUfGGqniE4C8BXpn4OYTquz1asCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"882dc853b783b8bb2da9840159b811c516f7eaa0d2d6a4d45488d118ce1d3a06","last_reissued_at":"2026-05-17T23:43:49.517664Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:43:49.517664Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma-ray emission from the impulsive phase of the 2017 September 06 X9.3 flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"1) ((1) Ioffe Institute, 126a, 26, Alexandra L. Lysenko (1), Dmitry D. Frederiks (1), Dmitry D. Svinkin (1), Gregory D. Fleishman (3, Irkutsk, Lermontov st., Newark, NJ - United States), Polytekhnicheskaya, - Russian Federation (2) Institute of Solar-Terrestrial Physics (ISZF), - Russian Federation (3) New Jersey Institute of Technology, Sergey A. Anfinogentov (2), St. Petersburg, University Heights","submitted_at":"2019-04-22T18:21:29Z","abstract_excerpt":"We report hard X-ray and gamma-ray observations of the impulsive phase of the SOL2017-09-06T11:55 X9.3 solar flare. We focus on a high-energy part of the spectrum, >100 keV, and perform time resolved spectral analysis for a portion of the impulsive phase, recorded by the Konus-Wind experiment, that displayed prominent gamma-ray emission. Given a variety of possible emission components contributing to the gamma-ray emission, we employ a Bayesian inference to build the most probable fitting model. The analysis confidently revealed contributions from nuclear deexcitation lines, electron-positron "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.10017","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":"1904.10017","created_at":"2026-05-17T23:43:49.517750+00:00"},{"alias_kind":"arxiv_version","alias_value":"1904.10017v1","created_at":"2026-05-17T23:43:49.517750+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1904.10017","created_at":"2026-05-17T23:43:49.517750+00:00"},{"alias_kind":"pith_short_12","alias_value":"RAW4QU5XQO4L","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_16","alias_value":"RAW4QU5XQO4LWLNJ","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_8","alias_value":"RAW4QU5X","created_at":"2026-05-18T12:33:27.125529+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/RAW4QU5XQO4LWLNJQQAVTOARYU","json":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU.json","graph_json":"https://pith.science/api/pith-number/RAW4QU5XQO4LWLNJQQAVTOARYU/graph.json","events_json":"https://pith.science/api/pith-number/RAW4QU5XQO4LWLNJQQAVTOARYU/events.json","paper":"https://pith.science/paper/RAW4QU5X"},"agent_actions":{"view_html":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU","download_json":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU.json","view_paper":"https://pith.science/paper/RAW4QU5X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1904.10017&json=true","fetch_graph":"https://pith.science/api/pith-number/RAW4QU5XQO4LWLNJQQAVTOARYU/graph.json","fetch_events":"https://pith.science/api/pith-number/RAW4QU5XQO4LWLNJQQAVTOARYU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU/action/storage_attestation","attest_author":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU/action/author_attestation","sign_citation":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU/action/citation_signature","submit_replication":"https://pith.science/pith/RAW4QU5XQO4LWLNJQQAVTOARYU/action/replication_record"}},"created_at":"2026-05-17T23:43:49.517750+00:00","updated_at":"2026-05-17T23:43:49.517750+00:00"}