{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:F6Y2DEUNSCQ55CCFPWMRSXKJJX","short_pith_number":"pith:F6Y2DEUN","schema_version":"1.0","canonical_sha256":"2fb1a1928d90a1de88457d99195d494df26a12366d203ed2ab14acb3c03eee47","source":{"kind":"arxiv","id":"1705.09311","version":3},"attestation_state":"computed","paper":{"title":"Theoretical Description Of GRB 160625B with Wind-to-ISM Transition and Implications for a Magnetized Outflow","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Galvan-Gamez, A. M. Watson, B. B. Zhang, B. Zhang, C. Ordaz-Salazar, N. Fraija, P. Veres, R. Barniol Duran, R. L. Becerra, W. H. Lee","submitted_at":"2017-05-25T18:06:52Z","abstract_excerpt":"GRB 160625B, one of the brightest bursts in recent years, was simultaneously observed by Fermi and Swift satellites, and ground-based optical telescopes in three different events separated by long periods of time. In this paper the non-thermal multiwavelength observations of GRB 160625B are described and a transition phase from wind-type-like medium to interstellar medium between the early (event II) and the late (event III) afterglow is found. The multiwavelength observations of the early afterglow are consistent with the afterglow evolution starting at $\\sim$ 150 s in a stellar wind medium w"},"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":"1705.09311","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-25T18:06:52Z","cross_cats_sorted":[],"title_canon_sha256":"9d666333aebd6b730ca262b9443093dc0997312e3cb323a1632f566b62a13864","abstract_canon_sha256":"7e9d28850875b465bc4d4f18786d7a17c52db2e6522b85c8d0bda5e612827a52"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:33:17.903244Z","signature_b64":"NA8kOrzi/d/Bs7Yg2Mg92gkTA+AAfusnUF5hpkKkqpkbp6GLFwHnSKB7ZpKEvwqxiZxthgjDf+l0IBtG4wBcAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2fb1a1928d90a1de88457d99195d494df26a12366d203ed2ab14acb3c03eee47","last_reissued_at":"2026-05-18T00:33:17.902736Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:33:17.902736Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Theoretical Description Of GRB 160625B with Wind-to-ISM Transition and Implications for a Magnetized Outflow","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Galvan-Gamez, A. M. Watson, B. B. Zhang, B. Zhang, C. Ordaz-Salazar, N. Fraija, P. Veres, R. Barniol Duran, R. L. Becerra, W. H. Lee","submitted_at":"2017-05-25T18:06:52Z","abstract_excerpt":"GRB 160625B, one of the brightest bursts in recent years, was simultaneously observed by Fermi and Swift satellites, and ground-based optical telescopes in three different events separated by long periods of time. In this paper the non-thermal multiwavelength observations of GRB 160625B are described and a transition phase from wind-type-like medium to interstellar medium between the early (event II) and the late (event III) afterglow is found. The multiwavelength observations of the early afterglow are consistent with the afterglow evolution starting at $\\sim$ 150 s in a stellar wind medium w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.09311","kind":"arxiv","version":3},"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":"1705.09311","created_at":"2026-05-18T00:33:17.902817+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.09311v3","created_at":"2026-05-18T00:33:17.902817+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.09311","created_at":"2026-05-18T00:33:17.902817+00:00"},{"alias_kind":"pith_short_12","alias_value":"F6Y2DEUNSCQ5","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"F6Y2DEUNSCQ55CCF","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"F6Y2DEUN","created_at":"2026-05-18T12:31:15.632608+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/F6Y2DEUNSCQ55CCFPWMRSXKJJX","json":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX.json","graph_json":"https://pith.science/api/pith-number/F6Y2DEUNSCQ55CCFPWMRSXKJJX/graph.json","events_json":"https://pith.science/api/pith-number/F6Y2DEUNSCQ55CCFPWMRSXKJJX/events.json","paper":"https://pith.science/paper/F6Y2DEUN"},"agent_actions":{"view_html":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX","download_json":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX.json","view_paper":"https://pith.science/paper/F6Y2DEUN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.09311&json=true","fetch_graph":"https://pith.science/api/pith-number/F6Y2DEUNSCQ55CCFPWMRSXKJJX/graph.json","fetch_events":"https://pith.science/api/pith-number/F6Y2DEUNSCQ55CCFPWMRSXKJJX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX/action/storage_attestation","attest_author":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX/action/author_attestation","sign_citation":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX/action/citation_signature","submit_replication":"https://pith.science/pith/F6Y2DEUNSCQ55CCFPWMRSXKJJX/action/replication_record"}},"created_at":"2026-05-18T00:33:17.902817+00:00","updated_at":"2026-05-18T00:33:17.902817+00:00"}