{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:WZ23EEFCLGIKSHCEJ3YBXEPTJ5","short_pith_number":"pith:WZ23EEFC","schema_version":"1.0","canonical_sha256":"b675b210a25990a91c444ef01b91f34f554bced0f6aafbb4e2dfa3ed0339147d","source":{"kind":"arxiv","id":"1012.3968","version":1},"attestation_state":"computed","paper":{"title":"Fermi/GBM and BATSE Gamma-Ray Bursts: comparison of the spectral properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Annalisa Celotti, Gabriele Ghisellini, Giancarlo Ghirlanda, Lara Nava","submitted_at":"2010-12-17T19:27:42Z","abstract_excerpt":"The Gamma-ray Burst Monitor (GBM) on board Fermi allows to study the spectra of Gamma Ray Bursts (GRBs) over an unprecedented wide energy range (8 keV - 35 MeV). We compare the spectral properties of short and long GRBs detected by the GBM (up to March 2010) with those of GRBs detected by the BATSE instrument on board the CGRO. GBM and BATSE long bursts have similar distributions of fluence (F), Epeak and peak flux (P) but GBM bursts have a slightly harder low-energy spectral index \\alpha with respect to BATSE GRBs. GBM and BATSE short bursts have similar distributions of fluence, \\alpha and p"},"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":"1012.3968","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-12-17T19:27:42Z","cross_cats_sorted":[],"title_canon_sha256":"b1ced9455f5bd10cfdc9bd1bbb78f19244cde5f91c40561957b185195c0209d3","abstract_canon_sha256":"c82d75b37d2f21289943479f6cec2e291281f9e7c3d41af926fe0b90d497b5a7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:22.913734Z","signature_b64":"Vosn8DzrLvcwRLcAEvEyOLC0jSwnpXAuJ3WMmIJMb8Aklq9JGwT/Zrg17b38nF0TSonHqP8AMjsZzDpa9JOmBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b675b210a25990a91c444ef01b91f34f554bced0f6aafbb4e2dfa3ed0339147d","last_reissued_at":"2026-05-18T02:04:22.913069Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:22.913069Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermi/GBM and BATSE Gamma-Ray Bursts: comparison of the spectral properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Annalisa Celotti, Gabriele Ghisellini, Giancarlo Ghirlanda, Lara Nava","submitted_at":"2010-12-17T19:27:42Z","abstract_excerpt":"The Gamma-ray Burst Monitor (GBM) on board Fermi allows to study the spectra of Gamma Ray Bursts (GRBs) over an unprecedented wide energy range (8 keV - 35 MeV). We compare the spectral properties of short and long GRBs detected by the GBM (up to March 2010) with those of GRBs detected by the BATSE instrument on board the CGRO. GBM and BATSE long bursts have similar distributions of fluence (F), Epeak and peak flux (P) but GBM bursts have a slightly harder low-energy spectral index \\alpha with respect to BATSE GRBs. GBM and BATSE short bursts have similar distributions of fluence, \\alpha and p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.3968","kind":"arxiv","version":1},"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":"1012.3968","created_at":"2026-05-18T02:04:22.913172+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.3968v1","created_at":"2026-05-18T02:04:22.913172+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.3968","created_at":"2026-05-18T02:04:22.913172+00:00"},{"alias_kind":"pith_short_12","alias_value":"WZ23EEFCLGIK","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"WZ23EEFCLGIKSHCE","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"WZ23EEFC","created_at":"2026-05-18T12:26:17.028572+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/WZ23EEFCLGIKSHCEJ3YBXEPTJ5","json":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5.json","graph_json":"https://pith.science/api/pith-number/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/graph.json","events_json":"https://pith.science/api/pith-number/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/events.json","paper":"https://pith.science/paper/WZ23EEFC"},"agent_actions":{"view_html":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5","download_json":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5.json","view_paper":"https://pith.science/paper/WZ23EEFC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.3968&json=true","fetch_graph":"https://pith.science/api/pith-number/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/graph.json","fetch_events":"https://pith.science/api/pith-number/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/action/storage_attestation","attest_author":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/action/author_attestation","sign_citation":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/action/citation_signature","submit_replication":"https://pith.science/pith/WZ23EEFCLGIKSHCEJ3YBXEPTJ5/action/replication_record"}},"created_at":"2026-05-18T02:04:22.913172+00:00","updated_at":"2026-05-18T02:04:22.913172+00:00"}