{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:QLU5JJN3TGIH6YQQOUJYE4WWV3","short_pith_number":"pith:QLU5JJN3","schema_version":"1.0","canonical_sha256":"82e9d4a5bb99907f621075138272d6aed750718df60106d1ddc9e3293e73e9cb","source":{"kind":"arxiv","id":"1901.05268","version":2},"attestation_state":"computed","paper":{"title":"Inverse Compton Scattering Spectra of Gamma-Ray Burst Prompt Emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jin-Jun Geng, Yong-Feng Huang, Yue Zhang","submitted_at":"2019-01-16T13:18:46Z","abstract_excerpt":"Although the physical origin of gamma-ray burst (GRB) prompt emission is still controversial, synchrotron radiation from accelerated electrons is a promising mechanism. It is believed that electrons are accelerated continuously by ultra-relativistic shocks or magnetic reconnections. At the same time, these electrons will be cooled via several processes (mainly adiabatic expansion, synchrotron radiation and inverse Compton scattering (ICS)), which regulate the distribution of electrons. An extra high-energy spectrum component is expected to be induced by ICS. However, the gamma-gamma annihilati"},"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":"1901.05268","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-01-16T13:18:46Z","cross_cats_sorted":[],"title_canon_sha256":"387f7b89aa6b2674b5a948cdc547c2ad863b2094577633713908df4dc2ee7554","abstract_canon_sha256":"7c7baed840c55bc21c627be26a53fd7605d3878e84771b56a12adc72ace9beb9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:44:21.842973Z","signature_b64":"g53pIpxaYH4ZZQ+Rcb5nPINVbh/w6OUhHnrgtJUTKQi4rSrHopLc/0VkySu0DK7CZ42DOGaKB2BXxfJ3DFNzDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"82e9d4a5bb99907f621075138272d6aed750718df60106d1ddc9e3293e73e9cb","last_reissued_at":"2026-05-17T23:44:21.842344Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:44:21.842344Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inverse Compton Scattering Spectra of Gamma-Ray Burst Prompt Emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jin-Jun Geng, Yong-Feng Huang, Yue Zhang","submitted_at":"2019-01-16T13:18:46Z","abstract_excerpt":"Although the physical origin of gamma-ray burst (GRB) prompt emission is still controversial, synchrotron radiation from accelerated electrons is a promising mechanism. It is believed that electrons are accelerated continuously by ultra-relativistic shocks or magnetic reconnections. At the same time, these electrons will be cooled via several processes (mainly adiabatic expansion, synchrotron radiation and inverse Compton scattering (ICS)), which regulate the distribution of electrons. An extra high-energy spectrum component is expected to be induced by ICS. However, the gamma-gamma annihilati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.05268","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":"1901.05268","created_at":"2026-05-17T23:44:21.842456+00:00"},{"alias_kind":"arxiv_version","alias_value":"1901.05268v2","created_at":"2026-05-17T23:44:21.842456+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1901.05268","created_at":"2026-05-17T23:44:21.842456+00:00"},{"alias_kind":"pith_short_12","alias_value":"QLU5JJN3TGIH","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_16","alias_value":"QLU5JJN3TGIH6YQQ","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_8","alias_value":"QLU5JJN3","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/QLU5JJN3TGIH6YQQOUJYE4WWV3","json":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3.json","graph_json":"https://pith.science/api/pith-number/QLU5JJN3TGIH6YQQOUJYE4WWV3/graph.json","events_json":"https://pith.science/api/pith-number/QLU5JJN3TGIH6YQQOUJYE4WWV3/events.json","paper":"https://pith.science/paper/QLU5JJN3"},"agent_actions":{"view_html":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3","download_json":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3.json","view_paper":"https://pith.science/paper/QLU5JJN3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1901.05268&json=true","fetch_graph":"https://pith.science/api/pith-number/QLU5JJN3TGIH6YQQOUJYE4WWV3/graph.json","fetch_events":"https://pith.science/api/pith-number/QLU5JJN3TGIH6YQQOUJYE4WWV3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3/action/storage_attestation","attest_author":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3/action/author_attestation","sign_citation":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3/action/citation_signature","submit_replication":"https://pith.science/pith/QLU5JJN3TGIH6YQQOUJYE4WWV3/action/replication_record"}},"created_at":"2026-05-17T23:44:21.842456+00:00","updated_at":"2026-05-17T23:44:21.842456+00:00"}