{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:4GE2CMJ6OMZSSI7TQDAKVWWBJZ","short_pith_number":"pith:4GE2CMJ6","schema_version":"1.0","canonical_sha256":"e189a1313e73332923f380c0aadac14e5b09f8a95a3f72ccafc0283c2093509b","source":{"kind":"arxiv","id":"1112.1700","version":2},"attestation_state":"computed","paper":{"title":"A complete sample of bright Swift Long Gamma-Ray Bursts: Sample presentation, Luminosity Function and evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"A. Melandri, B. Sbarufatti, D. Fugazza, G. Ghirlanda, G. Ghisellini, G. Tagliaferri, H. Flores, L. Nava, P. D'Avanzo, R. Salvaterra, S. Campana, S. Covino, S. D. Vergani, S. Piranomonte","submitted_at":"2011-12-07T21:00:06Z","abstract_excerpt":"We present a carefully selected sub-sample of Swift Long Gamma-ray Bursts (GRBs), that is complete in redshift. The sample is constructed by considering only bursts with favorable observing conditions for ground-based follow-up searches, that are bright in the 15-150 keV Swift/BAT band, i.e. with 1-s peak photon fluxes in excess to 2.6 ph s^-1 cm^-2. The sample is composed by 58 bursts, 52 of them with redshift for a completeness level of 90%, while another two have a redshift constraint, reaching a completeness level of 95%. For only three bursts we have no constraint on the redshift. The hig"},"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":"1112.1700","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-12-07T21:00:06Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"b9bfcc105b3f0d7acce0f6885c5d295a1f18632b40fedde0b6403b59e2da86ce","abstract_canon_sha256":"2a5b517d7ea5e5803cfcc97b22e64e276ff96ed55b35c6fed71a4c2995b79c1f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:15.412868Z","signature_b64":"wIff72eHQLYjtmgmpcvcf2crVaP05+eFnwKx5alodqA4LXSAJNQnimtMHto1V9530CO6c2s5qcgIaSDuel7WCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e189a1313e73332923f380c0aadac14e5b09f8a95a3f72ccafc0283c2093509b","last_reissued_at":"2026-05-18T01:59:15.412193Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:15.412193Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A complete sample of bright Swift Long Gamma-Ray Bursts: Sample presentation, Luminosity Function and evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"A. Melandri, B. Sbarufatti, D. Fugazza, G. Ghirlanda, G. Ghisellini, G. Tagliaferri, H. Flores, L. Nava, P. D'Avanzo, R. Salvaterra, S. Campana, S. Covino, S. D. Vergani, S. Piranomonte","submitted_at":"2011-12-07T21:00:06Z","abstract_excerpt":"We present a carefully selected sub-sample of Swift Long Gamma-ray Bursts (GRBs), that is complete in redshift. The sample is constructed by considering only bursts with favorable observing conditions for ground-based follow-up searches, that are bright in the 15-150 keV Swift/BAT band, i.e. with 1-s peak photon fluxes in excess to 2.6 ph s^-1 cm^-2. The sample is composed by 58 bursts, 52 of them with redshift for a completeness level of 90%, while another two have a redshift constraint, reaching a completeness level of 95%. For only three bursts we have no constraint on the redshift. The hig"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.1700","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":"1112.1700","created_at":"2026-05-18T01:59:15.412333+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.1700v2","created_at":"2026-05-18T01:59:15.412333+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.1700","created_at":"2026-05-18T01:59:15.412333+00:00"},{"alias_kind":"pith_short_12","alias_value":"4GE2CMJ6OMZS","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_16","alias_value":"4GE2CMJ6OMZSSI7T","created_at":"2026-05-18T12:26:20.644004+00:00"},{"alias_kind":"pith_short_8","alias_value":"4GE2CMJ6","created_at":"2026-05-18T12:26:20.644004+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/4GE2CMJ6OMZSSI7TQDAKVWWBJZ","json":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ.json","graph_json":"https://pith.science/api/pith-number/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/graph.json","events_json":"https://pith.science/api/pith-number/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/events.json","paper":"https://pith.science/paper/4GE2CMJ6"},"agent_actions":{"view_html":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ","download_json":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ.json","view_paper":"https://pith.science/paper/4GE2CMJ6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.1700&json=true","fetch_graph":"https://pith.science/api/pith-number/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/graph.json","fetch_events":"https://pith.science/api/pith-number/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/action/storage_attestation","attest_author":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/action/author_attestation","sign_citation":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/action/citation_signature","submit_replication":"https://pith.science/pith/4GE2CMJ6OMZSSI7TQDAKVWWBJZ/action/replication_record"}},"created_at":"2026-05-18T01:59:15.412333+00:00","updated_at":"2026-05-18T01:59:15.412333+00:00"}