{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:4V4WSSZAKZBP3X2TOOUXAR3YKK","short_pith_number":"pith:4V4WSSZA","schema_version":"1.0","canonical_sha256":"e579694b205642fddf5373a970477852ac69fd80387caba4de0bc2dfa2ab1b5b","source":{"kind":"arxiv","id":"2605.22573","version":1},"attestation_state":"computed","paper":{"title":"Iron Fluorescence in X-class Solar Flares: Aditya-L1/SoLEXS Observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Abhilash R. Sarwade, Ankur Kushwaha, Kiran Lakshmipathaiah, K. Sankarasubramanian, M.C. Ramadevi, Monoj Bug, Smrati Verma, Vaishali Sharan","submitted_at":"2026-05-21T14:50:24Z","abstract_excerpt":"Iron fluorescence is produced by the irradiation of the solar photosphere by coronal X-rays during flares. This study presents the first comprehensive analysis of iron K$\\alpha$ fluorescence characteristics in 47 X-class flares observed during the inaugural year of the Solar Low Energy X-ray Spectrometer (SoLEXS) on board India's Aditya-L1 mission. Leveraging the capability of modern silicon drift detectors (SDDs) for simultaneous broadband continuum and line measurements, the Fe K$\\alpha$ flux and the exciting flux ($F_{>7.11 \\text{ keV}}$) are quantified for each event, establishing a well-d"},"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":"2605.22573","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-05-21T14:50:24Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"5222dc490ab2f321f233b1f636d576b5eff70961f11e6d6568e9671f7754cdd9","abstract_canon_sha256":"d1430d667952e9b6aaeab7cbd2e77856042bfefc78ed5a3150bca217ebf461f2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-22T01:04:58.284866Z","signature_b64":"ka6UwJ+3WoY+2fBR3DNOZdtnURPnmUxw1VMVOz/kOuqT6XpVNKhjo0i6LPabb+ATTB8WP8tkt8OacEL49XumBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e579694b205642fddf5373a970477852ac69fd80387caba4de0bc2dfa2ab1b5b","last_reissued_at":"2026-05-22T01:04:58.284075Z","signature_status":"signed_v1","first_computed_at":"2026-05-22T01:04:58.284075Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Iron Fluorescence in X-class Solar Flares: Aditya-L1/SoLEXS Observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Abhilash R. Sarwade, Ankur Kushwaha, Kiran Lakshmipathaiah, K. Sankarasubramanian, M.C. Ramadevi, Monoj Bug, Smrati Verma, Vaishali Sharan","submitted_at":"2026-05-21T14:50:24Z","abstract_excerpt":"Iron fluorescence is produced by the irradiation of the solar photosphere by coronal X-rays during flares. This study presents the first comprehensive analysis of iron K$\\alpha$ fluorescence characteristics in 47 X-class flares observed during the inaugural year of the Solar Low Energy X-ray Spectrometer (SoLEXS) on board India's Aditya-L1 mission. Leveraging the capability of modern silicon drift detectors (SDDs) for simultaneous broadband continuum and line measurements, the Fe K$\\alpha$ flux and the exciting flux ($F_{>7.11 \\text{ keV}}$) are quantified for each event, establishing a well-d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.22573","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.22573/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2605.22573","created_at":"2026-05-22T01:04:58.284193+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.22573v1","created_at":"2026-05-22T01:04:58.284193+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.22573","created_at":"2026-05-22T01:04:58.284193+00:00"},{"alias_kind":"pith_short_12","alias_value":"4V4WSSZAKZBP","created_at":"2026-05-22T01:04:58.284193+00:00"},{"alias_kind":"pith_short_16","alias_value":"4V4WSSZAKZBP3X2T","created_at":"2026-05-22T01:04:58.284193+00:00"},{"alias_kind":"pith_short_8","alias_value":"4V4WSSZA","created_at":"2026-05-22T01:04:58.284193+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/4V4WSSZAKZBP3X2TOOUXAR3YKK","json":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK.json","graph_json":"https://pith.science/api/pith-number/4V4WSSZAKZBP3X2TOOUXAR3YKK/graph.json","events_json":"https://pith.science/api/pith-number/4V4WSSZAKZBP3X2TOOUXAR3YKK/events.json","paper":"https://pith.science/paper/4V4WSSZA"},"agent_actions":{"view_html":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK","download_json":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK.json","view_paper":"https://pith.science/paper/4V4WSSZA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.22573&json=true","fetch_graph":"https://pith.science/api/pith-number/4V4WSSZAKZBP3X2TOOUXAR3YKK/graph.json","fetch_events":"https://pith.science/api/pith-number/4V4WSSZAKZBP3X2TOOUXAR3YKK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK/action/storage_attestation","attest_author":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK/action/author_attestation","sign_citation":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK/action/citation_signature","submit_replication":"https://pith.science/pith/4V4WSSZAKZBP3X2TOOUXAR3YKK/action/replication_record"}},"created_at":"2026-05-22T01:04:58.284193+00:00","updated_at":"2026-05-22T01:04:58.284193+00:00"}