{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:EUF5CRYAMTINQFCTCSEPDZGHE2","short_pith_number":"pith:EUF5CRYA","schema_version":"1.0","canonical_sha256":"250bd1470064d0d814531488f1e4c7268399df311356b1c8f068043ad89b32df","source":{"kind":"arxiv","id":"1710.05620","version":2},"attestation_state":"computed","paper":{"title":"Binary neutron star merger rate via the luminosity function of short gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Debdutta Paul","submitted_at":"2017-10-16T11:00:35Z","abstract_excerpt":"The luminosity function of short Gamma Ray Bursts (GRBs) is modelled by using the available catalogue data of all short GRBs (sGRBs) detected till October, 2017. The luminosities are estimated via the `pseudo-redshifts' obtained from the `Yonetoku correlation', assuming a standard delay distribution between the cosmic star formation rate and the production rate of their progenitors. While the simple powerlaw is ruled out to high confidence, the data is fit well both by exponential cutoff powerlaw and broken powerlaw models. Using the derived parameters of these models along with conservative v"},"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":"1710.05620","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-16T11:00:35Z","cross_cats_sorted":[],"title_canon_sha256":"3d4fa6f89a86fb0a29bd480f6b78349f2c46268cdc8b1acbaeed863c74f3eddd","abstract_canon_sha256":"32a9153cb5ced94a69ff3a0a49d1be2be5d5d82282cafe9a11e9713bef9e692d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:18:16.679304Z","signature_b64":"UEY0+wN88OdHG0JyAdAKMdoohe5F/t3WJHgHS4/RobtHY0gXU7zUv93E+15IyD+epEQO2HjTLWbW9+LbN3XYDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"250bd1470064d0d814531488f1e4c7268399df311356b1c8f068043ad89b32df","last_reissued_at":"2026-05-18T00:18:16.678756Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:18:16.678756Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Binary neutron star merger rate via the luminosity function of short gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Debdutta Paul","submitted_at":"2017-10-16T11:00:35Z","abstract_excerpt":"The luminosity function of short Gamma Ray Bursts (GRBs) is modelled by using the available catalogue data of all short GRBs (sGRBs) detected till October, 2017. The luminosities are estimated via the `pseudo-redshifts' obtained from the `Yonetoku correlation', assuming a standard delay distribution between the cosmic star formation rate and the production rate of their progenitors. While the simple powerlaw is ruled out to high confidence, the data is fit well both by exponential cutoff powerlaw and broken powerlaw models. Using the derived parameters of these models along with conservative v"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.05620","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":"1710.05620","created_at":"2026-05-18T00:18:16.678837+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.05620v2","created_at":"2026-05-18T00:18:16.678837+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.05620","created_at":"2026-05-18T00:18:16.678837+00:00"},{"alias_kind":"pith_short_12","alias_value":"EUF5CRYAMTIN","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_16","alias_value":"EUF5CRYAMTINQFCT","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_8","alias_value":"EUF5CRYA","created_at":"2026-05-18T12:31:12.930513+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/EUF5CRYAMTINQFCTCSEPDZGHE2","json":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2.json","graph_json":"https://pith.science/api/pith-number/EUF5CRYAMTINQFCTCSEPDZGHE2/graph.json","events_json":"https://pith.science/api/pith-number/EUF5CRYAMTINQFCTCSEPDZGHE2/events.json","paper":"https://pith.science/paper/EUF5CRYA"},"agent_actions":{"view_html":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2","download_json":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2.json","view_paper":"https://pith.science/paper/EUF5CRYA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.05620&json=true","fetch_graph":"https://pith.science/api/pith-number/EUF5CRYAMTINQFCTCSEPDZGHE2/graph.json","fetch_events":"https://pith.science/api/pith-number/EUF5CRYAMTINQFCTCSEPDZGHE2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2/action/storage_attestation","attest_author":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2/action/author_attestation","sign_citation":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2/action/citation_signature","submit_replication":"https://pith.science/pith/EUF5CRYAMTINQFCTCSEPDZGHE2/action/replication_record"}},"created_at":"2026-05-18T00:18:16.678837+00:00","updated_at":"2026-05-18T00:18:16.678837+00:00"}