{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:2DDCZYOLPIRZVO2A7PMQFZXIRF","short_pith_number":"pith:2DDCZYOL","schema_version":"1.0","canonical_sha256":"d0c62ce1cb7a239abb40fbd902e6e8897d94ef8ffc615d1f9caae98b81c4bba5","source":{"kind":"arxiv","id":"1307.7293","version":1},"attestation_state":"computed","paper":{"title":"Study of luminosity and time evolution in X-ray afterglows of GRBs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jack Singal, Maria Giovanna Dainotti, Michal Ostrowski, Vahe' Petrosian","submitted_at":"2013-07-27T18:28:32Z","abstract_excerpt":"Gamma-ray bursts (GRBs), which have been observed up to redshifts $z \\approx 9.5$ can be good probes of the early universe and have the potential of testing cosmological models. The analysis by Dainotti of GRB Swift afterglow lightcurves with known redshifts and definite X-ray plateau shows an anti-correlation between the \\underline{rest frame} time when the plateau ends (the plateau end time) and the calculated luminosity at that time (or approximately an anti-correlation between plateau duration and luminosity). We present here an update of this correlation with a larger data sample of 101 G"},"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":"1307.7293","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-07-27T18:28:32Z","cross_cats_sorted":[],"title_canon_sha256":"29fcc78fd1e786a04ae8d2c05ce92d2d7549d68b3bd8eb58bddef54e4cb92bcd","abstract_canon_sha256":"3d3c47683a1aba1e6284e35c5c44f6aa125b4f1ce936075d91632eb109c1cdcf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:17:23.685782Z","signature_b64":"VRd0Q8tqScSzRKbi8rkiSk7slJw5ie3ilqXLQG1sphmdhx+S1mPu/TfOrxUjnAI81gYaF6O4v8cq1lzTXsaJAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0c62ce1cb7a239abb40fbd902e6e8897d94ef8ffc615d1f9caae98b81c4bba5","last_reissued_at":"2026-05-18T03:17:23.685067Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:17:23.685067Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Study of luminosity and time evolution in X-ray afterglows of GRBs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jack Singal, Maria Giovanna Dainotti, Michal Ostrowski, Vahe' Petrosian","submitted_at":"2013-07-27T18:28:32Z","abstract_excerpt":"Gamma-ray bursts (GRBs), which have been observed up to redshifts $z \\approx 9.5$ can be good probes of the early universe and have the potential of testing cosmological models. The analysis by Dainotti of GRB Swift afterglow lightcurves with known redshifts and definite X-ray plateau shows an anti-correlation between the \\underline{rest frame} time when the plateau ends (the plateau end time) and the calculated luminosity at that time (or approximately an anti-correlation between plateau duration and luminosity). We present here an update of this correlation with a larger data sample of 101 G"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.7293","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":"1307.7293","created_at":"2026-05-18T03:17:23.685184+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.7293v1","created_at":"2026-05-18T03:17:23.685184+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.7293","created_at":"2026-05-18T03:17:23.685184+00:00"},{"alias_kind":"pith_short_12","alias_value":"2DDCZYOLPIRZ","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_16","alias_value":"2DDCZYOLPIRZVO2A","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_8","alias_value":"2DDCZYOL","created_at":"2026-05-18T12:27:30.460161+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/2DDCZYOLPIRZVO2A7PMQFZXIRF","json":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF.json","graph_json":"https://pith.science/api/pith-number/2DDCZYOLPIRZVO2A7PMQFZXIRF/graph.json","events_json":"https://pith.science/api/pith-number/2DDCZYOLPIRZVO2A7PMQFZXIRF/events.json","paper":"https://pith.science/paper/2DDCZYOL"},"agent_actions":{"view_html":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF","download_json":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF.json","view_paper":"https://pith.science/paper/2DDCZYOL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.7293&json=true","fetch_graph":"https://pith.science/api/pith-number/2DDCZYOLPIRZVO2A7PMQFZXIRF/graph.json","fetch_events":"https://pith.science/api/pith-number/2DDCZYOLPIRZVO2A7PMQFZXIRF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF/action/storage_attestation","attest_author":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF/action/author_attestation","sign_citation":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF/action/citation_signature","submit_replication":"https://pith.science/pith/2DDCZYOLPIRZVO2A7PMQFZXIRF/action/replication_record"}},"created_at":"2026-05-18T03:17:23.685184+00:00","updated_at":"2026-05-18T03:17:23.685184+00:00"}