{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:DV5NO5AXVSZ335HFJ2ICBVNK3D","short_pith_number":"pith:DV5NO5AX","schema_version":"1.0","canonical_sha256":"1d7ad77417acb3bdf4e54e9020d5aad8f317fa1ddb81ddb271e181c2a21d0688","source":{"kind":"arxiv","id":"1612.00618","version":4},"attestation_state":"computed","paper":{"title":"Gamma Ray Burst Prompt correlations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Maria Dainotti, Mariusz Tarnopolski, Roberta Del Vecchio","submitted_at":"2016-12-02T10:23:04Z","abstract_excerpt":"The mechanism responsible for the prompt emission of gamma-ray bursts (GRBs) is still a debated issue. The prompt phase-related GRB correlations can allow to discriminate among the most plausible theoretical models explaining this emission. We present an overview of the observational two-parameter correlations, their physical interpretations, their use as redshift estimators and possibly as cosmological tools. The nowadays challenge is to make GRBs, the farthest stellar-scaled objects observed (up to redshift $z=9.4$), standard candles through well established and robust correlations. However,"},"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":"1612.00618","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-12-02T10:23:04Z","cross_cats_sorted":[],"title_canon_sha256":"09bb5771b8cb2dc04f63f5b28db0ad0d7436a0befd14bc907e4205a993e2ffca","abstract_canon_sha256":"22162ab65958d6c58cfe61e63944117118c8247a4d669e26ec7d70cce62a097c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:43.139013Z","signature_b64":"6N6b6tdGOKRGZf5AXJvQv1tYna1UgFWVn/LFVBwzdr81/gfk94c60W/5p2UCbX0lP8d8Q1/9cLxr0Qeyw43EBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1d7ad77417acb3bdf4e54e9020d5aad8f317fa1ddb81ddb271e181c2a21d0688","last_reissued_at":"2026-05-18T00:24:43.138400Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:43.138400Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma Ray Burst Prompt correlations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Maria Dainotti, Mariusz Tarnopolski, Roberta Del Vecchio","submitted_at":"2016-12-02T10:23:04Z","abstract_excerpt":"The mechanism responsible for the prompt emission of gamma-ray bursts (GRBs) is still a debated issue. The prompt phase-related GRB correlations can allow to discriminate among the most plausible theoretical models explaining this emission. We present an overview of the observational two-parameter correlations, their physical interpretations, their use as redshift estimators and possibly as cosmological tools. The nowadays challenge is to make GRBs, the farthest stellar-scaled objects observed (up to redshift $z=9.4$), standard candles through well established and robust correlations. However,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.00618","kind":"arxiv","version":4},"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":"1612.00618","created_at":"2026-05-18T00:24:43.138501+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.00618v4","created_at":"2026-05-18T00:24:43.138501+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.00618","created_at":"2026-05-18T00:24:43.138501+00:00"},{"alias_kind":"pith_short_12","alias_value":"DV5NO5AXVSZ3","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_16","alias_value":"DV5NO5AXVSZ335HF","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_8","alias_value":"DV5NO5AX","created_at":"2026-05-18T12:30:12.583610+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2203.06142","citing_title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","ref_index":294,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D","json":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D.json","graph_json":"https://pith.science/api/pith-number/DV5NO5AXVSZ335HFJ2ICBVNK3D/graph.json","events_json":"https://pith.science/api/pith-number/DV5NO5AXVSZ335HFJ2ICBVNK3D/events.json","paper":"https://pith.science/paper/DV5NO5AX"},"agent_actions":{"view_html":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D","download_json":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D.json","view_paper":"https://pith.science/paper/DV5NO5AX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.00618&json=true","fetch_graph":"https://pith.science/api/pith-number/DV5NO5AXVSZ335HFJ2ICBVNK3D/graph.json","fetch_events":"https://pith.science/api/pith-number/DV5NO5AXVSZ335HFJ2ICBVNK3D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D/action/storage_attestation","attest_author":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D/action/author_attestation","sign_citation":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D/action/citation_signature","submit_replication":"https://pith.science/pith/DV5NO5AXVSZ335HFJ2ICBVNK3D/action/replication_record"}},"created_at":"2026-05-18T00:24:43.138501+00:00","updated_at":"2026-05-18T00:24:43.138501+00:00"}