{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:YVLIGWUCRDR2467MGBMPT7ANCX","short_pith_number":"pith:YVLIGWUC","schema_version":"1.0","canonical_sha256":"c556835a8288e3ae7bec3058f9fc0d15f824fda2a260015ef786e6193d22b265","source":{"kind":"arxiv","id":"astro-ph/0310836","version":2},"attestation_state":"computed","paper":{"title":"The high energy tail of gamma-ray burst 941017: Comptonization of synchrotron self absorbed photons","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Asaf Pe'er, Eli Waxman","submitted_at":"2003-10-29T16:35:10Z","abstract_excerpt":"The recent detection of an unusually hard spectral component in GRB941017 extending to $\\ge200$ MeV is hard to explain as a synchrotron emission from shock-accelerated electrons.\n  It was argued to imply acceleration of protons to ultra-high energy. We show here that the \"high energy tail\" can be explained as emission from shock-accelerated electrons in the early afterglow epoch, taking into account the effect of synchrotron self-absorption. High energy observations set in this case stringent constraints on model parameters: A lower limit to the total explosion energy $E\\gsim5 \\times 10^{53}$ "},"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":"astro-ph/0310836","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-10-29T16:35:10Z","cross_cats_sorted":[],"title_canon_sha256":"dd335d747d7ba7b87210483a8e03f2d65537a3d923b58e6472d28647689b9915","abstract_canon_sha256":"dec90e4706ea7977533247c28d3e8ca6c728186b78be77b6158ebe0793488db6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:37:38.237683Z","signature_b64":"czP6rJUhl0cSVb1i3STMSIBmoK2GY+DQGGcFVRdH/FdZlfwLefUbqxd3gdrKSlDEJ5cekVPnQSFwK6xUR+IJDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c556835a8288e3ae7bec3058f9fc0d15f824fda2a260015ef786e6193d22b265","last_reissued_at":"2026-07-04T16:37:38.237287Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:37:38.237287Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The high energy tail of gamma-ray burst 941017: Comptonization of synchrotron self absorbed photons","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Asaf Pe'er, Eli Waxman","submitted_at":"2003-10-29T16:35:10Z","abstract_excerpt":"The recent detection of an unusually hard spectral component in GRB941017 extending to $\\ge200$ MeV is hard to explain as a synchrotron emission from shock-accelerated electrons.\n  It was argued to imply acceleration of protons to ultra-high energy. We show here that the \"high energy tail\" can be explained as emission from shock-accelerated electrons in the early afterglow epoch, taking into account the effect of synchrotron self-absorption. High energy observations set in this case stringent constraints on model parameters: A lower limit to the total explosion energy $E\\gsim5 \\times 10^{53}$ "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0310836","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0310836/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":"astro-ph/0310836","created_at":"2026-07-04T16:37:38.237346+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0310836v2","created_at":"2026-07-04T16:37:38.237346+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0310836","created_at":"2026-07-04T16:37:38.237346+00:00"},{"alias_kind":"pith_short_12","alias_value":"YVLIGWUCRDR2","created_at":"2026-07-04T16:37:38.237346+00:00"},{"alias_kind":"pith_short_16","alias_value":"YVLIGWUCRDR2467M","created_at":"2026-07-04T16:37:38.237346+00:00"},{"alias_kind":"pith_short_8","alias_value":"YVLIGWUC","created_at":"2026-07-04T16:37:38.237346+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1909.02802","citing_title":"Searching for GRBs at VHE with MAGIC: the status before CTA","ref_index":7,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX","json":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX.json","graph_json":"https://pith.science/api/pith-number/YVLIGWUCRDR2467MGBMPT7ANCX/graph.json","events_json":"https://pith.science/api/pith-number/YVLIGWUCRDR2467MGBMPT7ANCX/events.json","paper":"https://pith.science/paper/YVLIGWUC"},"agent_actions":{"view_html":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX","download_json":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX.json","view_paper":"https://pith.science/paper/YVLIGWUC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0310836&json=true","fetch_graph":"https://pith.science/api/pith-number/YVLIGWUCRDR2467MGBMPT7ANCX/graph.json","fetch_events":"https://pith.science/api/pith-number/YVLIGWUCRDR2467MGBMPT7ANCX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX/action/storage_attestation","attest_author":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX/action/author_attestation","sign_citation":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX/action/citation_signature","submit_replication":"https://pith.science/pith/YVLIGWUCRDR2467MGBMPT7ANCX/action/replication_record"}},"created_at":"2026-07-04T16:37:38.237346+00:00","updated_at":"2026-07-04T16:37:38.237346+00:00"}