{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:BRNB7YCVIZ7W3LEACUP34CIYK7","short_pith_number":"pith:BRNB7YCV","schema_version":"1.0","canonical_sha256":"0c5a1fe055467f6dac80151fbe091857de6ae0a2fe92007e9890afa61c2140b5","source":{"kind":"arxiv","id":"1104.5495","version":2},"attestation_state":"computed","paper":{"title":"Rest-frame properties of 32 gamma-ray bursts observed by the Fermi Gamma-Ray Burst Monitor","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Goldstein, A. J. van der Horst, A. Rau, A. von Kienlin, C. A. Meegan, C. Kouveliotou, C. Wilson-Hodge, D.Gruber, D. Tierney, E. Bissaldi, F. Olivares E., G. Fitzpatrick, G. J. Fishman, J. Greiner, J. M. Burgess, L. Lin, M. H. Gibby, M. M. Giles, M. Nardini, M. S. Briggs, P. N. Bhat, R. Diehl, R. D. Preece, R. M. Kippen, S.Foley, S. Guiriec, S. McBreen, V. Connaughton, V. L. Chaplin, W. S. Paciesas","submitted_at":"2011-04-28T20:00:03Z","abstract_excerpt":"Aims: In this paper we study the main spectral and temporal properties of gamma-ray bursts (GRBs) observed by Fermi/GBM. We investigate these key properties of GRBs in the rest-frame of the progenitor and test for possible intra-parameter correlations to better understand the intrinsic nature of these events. Methods: Our sample comprises 32 GRBs with measured redshift that were observed by GBM until August 2010. 28 of them belong to the long-duration population and 4 events were classified as short/hard bursts. For all of these events we derive, where possible, the intrinsic peak energy in th"},"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":"1104.5495","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-04-28T20:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"05d97906ae8f7a979723cba49f99aa48f9c87f493990c06e0f02a955966807a8","abstract_canon_sha256":"f655259a5e3395e7d4e7ddce73a99fb2551ca78c27ebebb1d2e267b8c2329f55"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:02:13.342508Z","signature_b64":"J2ppRTUitGXS3zDluxtQnOgJMdFS1+LcL+f/RTCcV4NI0+6f+KT9/O8ccEjbichtFOjQRBFv+yfPHRQonRX0Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c5a1fe055467f6dac80151fbe091857de6ae0a2fe92007e9890afa61c2140b5","last_reissued_at":"2026-05-18T02:02:13.341805Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:02:13.341805Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rest-frame properties of 32 gamma-ray bursts observed by the Fermi Gamma-Ray Burst Monitor","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Goldstein, A. J. van der Horst, A. Rau, A. von Kienlin, C. A. Meegan, C. Kouveliotou, C. Wilson-Hodge, D.Gruber, D. Tierney, E. Bissaldi, F. Olivares E., G. Fitzpatrick, G. J. Fishman, J. Greiner, J. M. Burgess, L. Lin, M. H. Gibby, M. M. Giles, M. Nardini, M. S. Briggs, P. N. Bhat, R. Diehl, R. D. Preece, R. M. Kippen, S.Foley, S. Guiriec, S. McBreen, V. Connaughton, V. L. Chaplin, W. S. Paciesas","submitted_at":"2011-04-28T20:00:03Z","abstract_excerpt":"Aims: In this paper we study the main spectral and temporal properties of gamma-ray bursts (GRBs) observed by Fermi/GBM. We investigate these key properties of GRBs in the rest-frame of the progenitor and test for possible intra-parameter correlations to better understand the intrinsic nature of these events. Methods: Our sample comprises 32 GRBs with measured redshift that were observed by GBM until August 2010. 28 of them belong to the long-duration population and 4 events were classified as short/hard bursts. For all of these events we derive, where possible, the intrinsic peak energy in th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.5495","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":"1104.5495","created_at":"2026-05-18T02:02:13.341908+00:00"},{"alias_kind":"arxiv_version","alias_value":"1104.5495v2","created_at":"2026-05-18T02:02:13.341908+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1104.5495","created_at":"2026-05-18T02:02:13.341908+00:00"},{"alias_kind":"pith_short_12","alias_value":"BRNB7YCVIZ7W","created_at":"2026-05-18T12:26:24.575870+00:00"},{"alias_kind":"pith_short_16","alias_value":"BRNB7YCVIZ7W3LEA","created_at":"2026-05-18T12:26:24.575870+00:00"},{"alias_kind":"pith_short_8","alias_value":"BRNB7YCV","created_at":"2026-05-18T12:26:24.575870+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/BRNB7YCVIZ7W3LEACUP34CIYK7","json":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7.json","graph_json":"https://pith.science/api/pith-number/BRNB7YCVIZ7W3LEACUP34CIYK7/graph.json","events_json":"https://pith.science/api/pith-number/BRNB7YCVIZ7W3LEACUP34CIYK7/events.json","paper":"https://pith.science/paper/BRNB7YCV"},"agent_actions":{"view_html":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7","download_json":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7.json","view_paper":"https://pith.science/paper/BRNB7YCV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1104.5495&json=true","fetch_graph":"https://pith.science/api/pith-number/BRNB7YCVIZ7W3LEACUP34CIYK7/graph.json","fetch_events":"https://pith.science/api/pith-number/BRNB7YCVIZ7W3LEACUP34CIYK7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7/action/storage_attestation","attest_author":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7/action/author_attestation","sign_citation":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7/action/citation_signature","submit_replication":"https://pith.science/pith/BRNB7YCVIZ7W3LEACUP34CIYK7/action/replication_record"}},"created_at":"2026-05-18T02:02:13.341908+00:00","updated_at":"2026-05-18T02:02:13.341908+00:00"}