{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:VQE73BA5VWTEGNAHPXSF3FTBY7","short_pith_number":"pith:VQE73BA5","schema_version":"1.0","canonical_sha256":"ac09fd841dada64334077de45d9661c7e2852a0fde2217e5bb19845dfcda461f","source":{"kind":"arxiv","id":"1206.5605","version":2},"attestation_state":"computed","paper":{"title":"Analysis of GRB 080319B and GRB 050904 within the fireshell model: evidence for a broader spectral energy distribution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Barbara Patricelli, Carlo Luciano Bianco, Gregory Vereshchagin, Gustavo De Barros, Letizia Caito, Luca Izzo, Maria Grazia Bernardini, Remo Ruffini","submitted_at":"2012-06-25T08:44:01Z","abstract_excerpt":"(Shortened) GRB080319B, with an isotropic energy E_{iso}=1.32x10^{54}erg, and GRB050904, with E_{iso}=1.04x10^{54}erg, offer the possibility of studying the spectral properties of the prompt radiation of two of the most energetic Gamma-Ray Bursts (GRBs). This allows us to probe the validity of the fireshell model for GRBs beyond 10^{54}erg, well outside the energy range where it has been successfully tested up to now (10^{49}-10^{53}erg). We find that in the low energy region, the prompt emission spectra observed by Swift BAT reveals more power than theoretically predicted. The opportunities o"},"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":"1206.5605","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-06-25T08:44:01Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"64d089c1d3ad1c7b7558953d42a5280df77e0a6e240575c7505735a0e3d74489","abstract_canon_sha256":"639809497524c894be240a1bb6086c66d771983b4930740bbda1e4ecc42014ff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:47:00.711046Z","signature_b64":"cpTWntUcXxQJqXNxblptN0V0550R2u8j9O9MG7slfIluOI7Xyu2nkL2FLc7JikBaUbBzJ9Yz703Ws4XRMY4yDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ac09fd841dada64334077de45d9661c7e2852a0fde2217e5bb19845dfcda461f","last_reissued_at":"2026-05-18T03:47:00.710467Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:47:00.710467Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Analysis of GRB 080319B and GRB 050904 within the fireshell model: evidence for a broader spectral energy distribution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Barbara Patricelli, Carlo Luciano Bianco, Gregory Vereshchagin, Gustavo De Barros, Letizia Caito, Luca Izzo, Maria Grazia Bernardini, Remo Ruffini","submitted_at":"2012-06-25T08:44:01Z","abstract_excerpt":"(Shortened) GRB080319B, with an isotropic energy E_{iso}=1.32x10^{54}erg, and GRB050904, with E_{iso}=1.04x10^{54}erg, offer the possibility of studying the spectral properties of the prompt radiation of two of the most energetic Gamma-Ray Bursts (GRBs). This allows us to probe the validity of the fireshell model for GRBs beyond 10^{54}erg, well outside the energy range where it has been successfully tested up to now (10^{49}-10^{53}erg). We find that in the low energy region, the prompt emission spectra observed by Swift BAT reveals more power than theoretically predicted. The opportunities o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.5605","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":"1206.5605","created_at":"2026-05-18T03:47:00.710538+00:00"},{"alias_kind":"arxiv_version","alias_value":"1206.5605v2","created_at":"2026-05-18T03:47:00.710538+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1206.5605","created_at":"2026-05-18T03:47:00.710538+00:00"},{"alias_kind":"pith_short_12","alias_value":"VQE73BA5VWTE","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_16","alias_value":"VQE73BA5VWTEGNAH","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_8","alias_value":"VQE73BA5","created_at":"2026-05-18T12:27:25.539911+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/VQE73BA5VWTEGNAHPXSF3FTBY7","json":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7.json","graph_json":"https://pith.science/api/pith-number/VQE73BA5VWTEGNAHPXSF3FTBY7/graph.json","events_json":"https://pith.science/api/pith-number/VQE73BA5VWTEGNAHPXSF3FTBY7/events.json","paper":"https://pith.science/paper/VQE73BA5"},"agent_actions":{"view_html":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7","download_json":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7.json","view_paper":"https://pith.science/paper/VQE73BA5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1206.5605&json=true","fetch_graph":"https://pith.science/api/pith-number/VQE73BA5VWTEGNAHPXSF3FTBY7/graph.json","fetch_events":"https://pith.science/api/pith-number/VQE73BA5VWTEGNAHPXSF3FTBY7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7/action/storage_attestation","attest_author":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7/action/author_attestation","sign_citation":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7/action/citation_signature","submit_replication":"https://pith.science/pith/VQE73BA5VWTEGNAHPXSF3FTBY7/action/replication_record"}},"created_at":"2026-05-18T03:47:00.710538+00:00","updated_at":"2026-05-18T03:47:00.710538+00:00"}