{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:AYXTNY3ZBQDKYCLRH3OSVUAUMH","short_pith_number":"pith:AYXTNY3Z","schema_version":"1.0","canonical_sha256":"062f36e3790c06ac09713edd2ad01461e302c136623e59bd215b0117d4baf1fe","source":{"kind":"arxiv","id":"0907.2462","version":2},"attestation_state":"computed","paper":{"title":"A new analysis of the short-duration, hard-spectrum GRB 051103, a possible extragalactic SGR giant flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. B. Sanin, A. Fruchter, A. Levan, A. Rau, A. Rowlinson, A. S. Kozyrev, A. von Kienlin, C. Fellows, C. Wigger, D. Bersier, D. M. Palmer, D. M. Smith, D. Perley, D. V. Golovin, E. Bellm, E. Rol, G. Ricker, H. Krimm, I. G. Mitrofanov, J.J. Kavelaars, J.-L. Atteia, J. Rhoads, K. Harshmann, K. Hurley, K. Wiersema, K. Yamaoka, M. L. Litvak, M. Ohno, N. Gehrels, N.R. Tanvir, P.T. O'Brien, R. C. Duncan, R. Vanderspek, T. Cline, W. Boynton, W. Hajdas, Y. E. Nakagawa","submitted_at":"2009-07-14T22:04:46Z","abstract_excerpt":"GRB 051103 is considered to be a candidate soft gamma repeater (SGR) extragalactic giant magnetar flare by virtue of its proximity on the sky to M81/M82, as well as its time history, localization, and energy spectrum. We have derived a refined interplanetary network localization for this burst which reduces the size of the error box by over a factor of two. We examine its time history for evidence of a periodic component, which would be one signature of an SGR giant flare, and conclude that this component is neither detected nor detectable under reasonable assumptions. We analyze the time-reso"},"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":"0907.2462","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-07-14T22:04:46Z","cross_cats_sorted":[],"title_canon_sha256":"eaa94867b90aab4bb0866fa8b02693edc2d59303a14e1638f3e0c8b08f74d2dd","abstract_canon_sha256":"e3e5c562ba57e87346a9bd1cdf23ae432ec8158cd603ecc5c15517e53dfafc81"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:03.059929Z","signature_b64":"qE1flFhsjotE/qV1v4eETL5wZbVcPZXjuAa1JnDNXXKYEjLW9FMopdQsnF1O2CwVo8z4qw54u9z3NjRL81pvDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"062f36e3790c06ac09713edd2ad01461e302c136623e59bd215b0117d4baf1fe","last_reissued_at":"2026-05-18T02:13:03.059468Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:03.059468Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A new analysis of the short-duration, hard-spectrum GRB 051103, a possible extragalactic SGR giant flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. B. Sanin, A. Fruchter, A. Levan, A. Rau, A. Rowlinson, A. S. Kozyrev, A. von Kienlin, C. Fellows, C. Wigger, D. Bersier, D. M. Palmer, D. M. Smith, D. Perley, D. V. Golovin, E. Bellm, E. Rol, G. Ricker, H. Krimm, I. G. Mitrofanov, J.J. Kavelaars, J.-L. Atteia, J. Rhoads, K. Harshmann, K. Hurley, K. Wiersema, K. Yamaoka, M. L. Litvak, M. Ohno, N. Gehrels, N.R. Tanvir, P.T. O'Brien, R. C. Duncan, R. Vanderspek, T. Cline, W. Boynton, W. Hajdas, Y. E. Nakagawa","submitted_at":"2009-07-14T22:04:46Z","abstract_excerpt":"GRB 051103 is considered to be a candidate soft gamma repeater (SGR) extragalactic giant magnetar flare by virtue of its proximity on the sky to M81/M82, as well as its time history, localization, and energy spectrum. We have derived a refined interplanetary network localization for this burst which reduces the size of the error box by over a factor of two. We examine its time history for evidence of a periodic component, which would be one signature of an SGR giant flare, and conclude that this component is neither detected nor detectable under reasonable assumptions. We analyze the time-reso"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0907.2462","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":"0907.2462","created_at":"2026-05-18T02:13:03.059536+00:00"},{"alias_kind":"arxiv_version","alias_value":"0907.2462v2","created_at":"2026-05-18T02:13:03.059536+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0907.2462","created_at":"2026-05-18T02:13:03.059536+00:00"},{"alias_kind":"pith_short_12","alias_value":"AYXTNY3ZBQDK","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_16","alias_value":"AYXTNY3ZBQDKYCLR","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_8","alias_value":"AYXTNY3Z","created_at":"2026-05-18T12:25:58.837520+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/AYXTNY3ZBQDKYCLRH3OSVUAUMH","json":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH.json","graph_json":"https://pith.science/api/pith-number/AYXTNY3ZBQDKYCLRH3OSVUAUMH/graph.json","events_json":"https://pith.science/api/pith-number/AYXTNY3ZBQDKYCLRH3OSVUAUMH/events.json","paper":"https://pith.science/paper/AYXTNY3Z"},"agent_actions":{"view_html":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH","download_json":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH.json","view_paper":"https://pith.science/paper/AYXTNY3Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0907.2462&json=true","fetch_graph":"https://pith.science/api/pith-number/AYXTNY3ZBQDKYCLRH3OSVUAUMH/graph.json","fetch_events":"https://pith.science/api/pith-number/AYXTNY3ZBQDKYCLRH3OSVUAUMH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH/action/storage_attestation","attest_author":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH/action/author_attestation","sign_citation":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH/action/citation_signature","submit_replication":"https://pith.science/pith/AYXTNY3ZBQDKYCLRH3OSVUAUMH/action/replication_record"}},"created_at":"2026-05-18T02:13:03.059536+00:00","updated_at":"2026-05-18T02:13:03.059536+00:00"}