{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:MUHRUG5PHZDLKGPCIM6442FFOG","short_pith_number":"pith:MUHRUG5P","schema_version":"1.0","canonical_sha256":"650f1a1baf3e46b519e2433dce68a571b11e6878aa6009eb97f4e187509a59c9","source":{"kind":"arxiv","id":"1509.01592","version":1},"attestation_state":"computed","paper":{"title":"Extra-galactic high-energy transients: event rate densities and luminosity functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"2, 2), 2) ((1) Peking University, (2) Kavli Institute for Astronomy, 3), (3) UNLV), Astrophysics, Bing Zhang (1, Hui Sun (1, PKU, Zhuo Li (1","submitted_at":"2015-09-04T20:07:50Z","abstract_excerpt":"Several types of extra-galactic high-energy transients have been discovered, which include high-luminosity and low-luminosity long-duration gamma-ray bursts (GRBs), short-duration GRBs, supernova shock breakouts (SBOs), and tidal disruption events (TDEs) without or with an associated relativistic jet. In this paper, we apply a unified method to systematically study the redshift-dependent event rate densities and the global luminosity functions (ignoring redshift evolution) of these transients. We introduce some empirical formulae for the redshift-dependent event rate densities for different ty"},"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":"1509.01592","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-09-04T20:07:50Z","cross_cats_sorted":[],"title_canon_sha256":"3ee915ab9bd8b50a5c1b160681c89020b29036a9123f7a06c2e04b47ed3fe5bd","abstract_canon_sha256":"6b5e2512459b52bdc9100bd878036ef64d92bbd86ee8de97c4b2b20dcb32648b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:30:18.001069Z","signature_b64":"Vy8tCxWRt+XicLVipCwho9pin1+DKNw5uBO2Y8ajnME9MtfI7zsofmDC0UNdYi/+LlU5xSCcKervC9eKkYEkAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"650f1a1baf3e46b519e2433dce68a571b11e6878aa6009eb97f4e187509a59c9","last_reissued_at":"2026-05-18T01:30:18.000582Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:30:18.000582Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Extra-galactic high-energy transients: event rate densities and luminosity functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"2, 2), 2) ((1) Peking University, (2) Kavli Institute for Astronomy, 3), (3) UNLV), Astrophysics, Bing Zhang (1, Hui Sun (1, PKU, Zhuo Li (1","submitted_at":"2015-09-04T20:07:50Z","abstract_excerpt":"Several types of extra-galactic high-energy transients have been discovered, which include high-luminosity and low-luminosity long-duration gamma-ray bursts (GRBs), short-duration GRBs, supernova shock breakouts (SBOs), and tidal disruption events (TDEs) without or with an associated relativistic jet. In this paper, we apply a unified method to systematically study the redshift-dependent event rate densities and the global luminosity functions (ignoring redshift evolution) of these transients. We introduce some empirical formulae for the redshift-dependent event rate densities for different ty"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1509.01592","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":"1509.01592","created_at":"2026-05-18T01:30:18.000650+00:00"},{"alias_kind":"arxiv_version","alias_value":"1509.01592v1","created_at":"2026-05-18T01:30:18.000650+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1509.01592","created_at":"2026-05-18T01:30:18.000650+00:00"},{"alias_kind":"pith_short_12","alias_value":"MUHRUG5PHZDL","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_16","alias_value":"MUHRUG5PHZDLKGPC","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_8","alias_value":"MUHRUG5P","created_at":"2026-05-18T12:29:32.376354+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/MUHRUG5PHZDLKGPCIM6442FFOG","json":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG.json","graph_json":"https://pith.science/api/pith-number/MUHRUG5PHZDLKGPCIM6442FFOG/graph.json","events_json":"https://pith.science/api/pith-number/MUHRUG5PHZDLKGPCIM6442FFOG/events.json","paper":"https://pith.science/paper/MUHRUG5P"},"agent_actions":{"view_html":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG","download_json":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG.json","view_paper":"https://pith.science/paper/MUHRUG5P","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1509.01592&json=true","fetch_graph":"https://pith.science/api/pith-number/MUHRUG5PHZDLKGPCIM6442FFOG/graph.json","fetch_events":"https://pith.science/api/pith-number/MUHRUG5PHZDLKGPCIM6442FFOG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG/action/storage_attestation","attest_author":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG/action/author_attestation","sign_citation":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG/action/citation_signature","submit_replication":"https://pith.science/pith/MUHRUG5PHZDLKGPCIM6442FFOG/action/replication_record"}},"created_at":"2026-05-18T01:30:18.000650+00:00","updated_at":"2026-05-18T01:30:18.000650+00:00"}