{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:XC3KGNFBVYATS4CNB2Z43FZR32","short_pith_number":"pith:XC3KGNFB","schema_version":"1.0","canonical_sha256":"b8b6a334a1ae0139704d0eb3cd9731de8e43e9215161b08c7833ba2e24703d43","source":{"kind":"arxiv","id":"astro-ph/0503508","version":1},"attestation_state":"computed","paper":{"title":"A contemporaneous infrared flash from a long gamma-ray burst: an echo from the central engine","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Ghez, A. Parsons, A. Szentgyorgyi, C. B. Markwardt, C. H. Blake, C. McCabe, D. Hullinger, D. L. Starr, D. Palmer, E. E. Falco, E. E. Fenimore, F. Chaffee, G. Duchene, H. A. Krimm, J. R. Cummings, J. S. Bloom, J. Tueller, J. X. Prochaska, K. Hurley, K. McLean, K. Stapelfeldt, M. Kassis, M. Skrutskie, N. Gehrels, Q. Konopacky, R. Campbell, S. Barthelmy, S. Hornstein","submitted_at":"2005-03-23T21:00:02Z","abstract_excerpt":"The explosion that results in a cosmic gamma-ray burst (GRB) is thought to produce emission from two physical processes -- the activity of the central engine gives rise to the high-energy emission of the burst through internal shocking and the subsequent interaction of the flow with the external environment produces long-wavelength afterglow. While afterglow observations continue to refine our understanding of GRB progenitors and relativistic shocks, gamma-ray observations alone have not yielded a clear picture of the origin of the prompt emission nor details of the central engine. Only one co"},"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":"astro-ph/0503508","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-03-23T21:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"6b3331bbde8eabea3246271343b70cff89caa65cf5c8fdcb53422598251f92cd","abstract_canon_sha256":"3c51bf3a0596b3cf7635ffd65d2664535f1909db4d9f4eb5d36e7450d9380f38"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:38:06.000878Z","signature_b64":"TeH9xKCGJ/aA7BRD7pBMoS5VI4ZMV4NYLZRZ6G+37RtK3jjwSpEXSr/+lmU/1n3EmfT27peteVdtyK+OoP62Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b8b6a334a1ae0139704d0eb3cd9731de8e43e9215161b08c7833ba2e24703d43","last_reissued_at":"2026-07-04T15:38:06.000458Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:38:06.000458Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A contemporaneous infrared flash from a long gamma-ray burst: an echo from the central engine","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Ghez, A. Parsons, A. Szentgyorgyi, C. B. Markwardt, C. H. Blake, C. McCabe, D. Hullinger, D. L. Starr, D. Palmer, E. E. Falco, E. E. Fenimore, F. Chaffee, G. Duchene, H. A. Krimm, J. R. Cummings, J. S. Bloom, J. Tueller, J. X. Prochaska, K. Hurley, K. McLean, K. Stapelfeldt, M. Kassis, M. Skrutskie, N. Gehrels, Q. Konopacky, R. Campbell, S. Barthelmy, S. Hornstein","submitted_at":"2005-03-23T21:00:02Z","abstract_excerpt":"The explosion that results in a cosmic gamma-ray burst (GRB) is thought to produce emission from two physical processes -- the activity of the central engine gives rise to the high-energy emission of the burst through internal shocking and the subsequent interaction of the flow with the external environment produces long-wavelength afterglow. While afterglow observations continue to refine our understanding of GRB progenitors and relativistic shocks, gamma-ray observations alone have not yielded a clear picture of the origin of the prompt emission nor details of the central engine. Only one co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0503508","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0503508/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0503508","created_at":"2026-07-04T15:38:06.000520+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0503508v1","created_at":"2026-07-04T15:38:06.000520+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0503508","created_at":"2026-07-04T15:38:06.000520+00:00"},{"alias_kind":"pith_short_12","alias_value":"XC3KGNFBVYAT","created_at":"2026-07-04T15:38:06.000520+00:00"},{"alias_kind":"pith_short_16","alias_value":"XC3KGNFBVYATS4CN","created_at":"2026-07-04T15:38:06.000520+00:00"},{"alias_kind":"pith_short_8","alias_value":"XC3KGNFB","created_at":"2026-07-04T15:38:06.000520+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.28267","citing_title":"Early Optical Follow-up of Gamma-Ray Bursts: The Critical Role of Robotic Telescopes","ref_index":218,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32","json":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32.json","graph_json":"https://pith.science/api/pith-number/XC3KGNFBVYATS4CNB2Z43FZR32/graph.json","events_json":"https://pith.science/api/pith-number/XC3KGNFBVYATS4CNB2Z43FZR32/events.json","paper":"https://pith.science/paper/XC3KGNFB"},"agent_actions":{"view_html":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32","download_json":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32.json","view_paper":"https://pith.science/paper/XC3KGNFB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0503508&json=true","fetch_graph":"https://pith.science/api/pith-number/XC3KGNFBVYATS4CNB2Z43FZR32/graph.json","fetch_events":"https://pith.science/api/pith-number/XC3KGNFBVYATS4CNB2Z43FZR32/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32/action/storage_attestation","attest_author":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32/action/author_attestation","sign_citation":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32/action/citation_signature","submit_replication":"https://pith.science/pith/XC3KGNFBVYATS4CNB2Z43FZR32/action/replication_record"}},"created_at":"2026-07-04T15:38:06.000520+00:00","updated_at":"2026-07-04T15:38:06.000520+00:00"}