{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:6FTKFPDCK2JDYMYLGTMM3DRF53","short_pith_number":"pith:6FTKFPDC","schema_version":"1.0","canonical_sha256":"f166a2bc6256923c330b34d8cd8e25eeda1e25ef702c2ea1ac6dde1d9f538b40","source":{"kind":"arxiv","id":"1307.0950","version":1},"attestation_state":"computed","paper":{"title":"A method for quantifying the Gamma Ray Burst \"bias\". Application in the redshift range 0-1.1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"E. Le Floc'h, N. Prantzos, R. Salvaterra, S. Basa, S. Boissier, S.D. Vergani, S. Savaglio, V. Buat","submitted_at":"2013-07-03T09:41:15Z","abstract_excerpt":"Long Gamma Ray Bursts (LGRBs) are related to the final stages of evolution of massive stars. As such, they should follow the star formation rate (SFR) of galaxies. We can use them to probe for star-forming galaxies (SFGs) in the distant universe following this assumption. The relation between the rate of LGRBs in a given galaxy and its SFR (that we call the LGRB \"bias\") may be complex, as we have indications that the LGRB hosts are not perfect analogues to the general population of SFGs. In this work, we try to quantify the dependence of the LGRB bias on physical parameters of their host galax"},"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":"1307.0950","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-07-03T09:41:15Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"fe06550fa31877cbdc978345c95c6ed92c4e8d10cbd1a5d90de6e6fa146e6c71","abstract_canon_sha256":"cb57800603cfe32ae682dc5b99ede938a5757e2fe3c21892a3772bea0d53b4a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:00.301343Z","signature_b64":"2HUGxHWUwzEdngXrpQT0hY4UhwBOKWKm4Z85MuNutKtYzh7M2w1MIp9OvNLbxae4kWgN+hcQv++jSWO3fQ9KBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f166a2bc6256923c330b34d8cd8e25eeda1e25ef702c2ea1ac6dde1d9f538b40","last_reissued_at":"2026-05-18T01:49:00.300768Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:00.300768Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A method for quantifying the Gamma Ray Burst \"bias\". Application in the redshift range 0-1.1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"E. Le Floc'h, N. Prantzos, R. Salvaterra, S. Basa, S. Boissier, S.D. Vergani, S. Savaglio, V. Buat","submitted_at":"2013-07-03T09:41:15Z","abstract_excerpt":"Long Gamma Ray Bursts (LGRBs) are related to the final stages of evolution of massive stars. As such, they should follow the star formation rate (SFR) of galaxies. We can use them to probe for star-forming galaxies (SFGs) in the distant universe following this assumption. The relation between the rate of LGRBs in a given galaxy and its SFR (that we call the LGRB \"bias\") may be complex, as we have indications that the LGRB hosts are not perfect analogues to the general population of SFGs. In this work, we try to quantify the dependence of the LGRB bias on physical parameters of their host galax"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.0950","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":"1307.0950","created_at":"2026-05-18T01:49:00.300859+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.0950v1","created_at":"2026-05-18T01:49:00.300859+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.0950","created_at":"2026-05-18T01:49:00.300859+00:00"},{"alias_kind":"pith_short_12","alias_value":"6FTKFPDCK2JD","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_16","alias_value":"6FTKFPDCK2JDYMYL","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_8","alias_value":"6FTKFPDC","created_at":"2026-05-18T12:27:36.564083+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/6FTKFPDCK2JDYMYLGTMM3DRF53","json":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53.json","graph_json":"https://pith.science/api/pith-number/6FTKFPDCK2JDYMYLGTMM3DRF53/graph.json","events_json":"https://pith.science/api/pith-number/6FTKFPDCK2JDYMYLGTMM3DRF53/events.json","paper":"https://pith.science/paper/6FTKFPDC"},"agent_actions":{"view_html":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53","download_json":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53.json","view_paper":"https://pith.science/paper/6FTKFPDC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.0950&json=true","fetch_graph":"https://pith.science/api/pith-number/6FTKFPDCK2JDYMYLGTMM3DRF53/graph.json","fetch_events":"https://pith.science/api/pith-number/6FTKFPDCK2JDYMYLGTMM3DRF53/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53/action/storage_attestation","attest_author":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53/action/author_attestation","sign_citation":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53/action/citation_signature","submit_replication":"https://pith.science/pith/6FTKFPDCK2JDYMYLGTMM3DRF53/action/replication_record"}},"created_at":"2026-05-18T01:49:00.300859+00:00","updated_at":"2026-05-18T01:49:00.300859+00:00"}