{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:7JAQLTQOTVSRAA6VVTQEICLAVV","short_pith_number":"pith:7JAQLTQO","schema_version":"1.0","canonical_sha256":"fa4105ce0e9d651003d5ace0440960ad4870d91f1d03381875034c6b9ee694f2","source":{"kind":"arxiv","id":"astro-ph/0204141","version":2},"attestation_state":"computed","paper":{"title":"The Broadband Afterglow of GRB980329","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. A. Frail, D. Reichart, D. S. Shepherd, D. W. Fox, E. Berger, F. A. Harrison, F. Walter, G. B. Taylor, G. H. Moriarty-Schieven, J. E. Larkin, J. S. Bloom, P. A. Price, R. Sari, R. W. Goodrich, S. A. Yost, S. G. Djorgovski, S. R. Kulkarni, T. J. Galama","submitted_at":"2002-04-08T21:36:02Z","abstract_excerpt":"We present radio observations of the afterglow of the bright gamma-ray burst GRB980329 made between one month and several years after the burst, a re-analysis of previously published submillimeter data, and late-time optical and near-infrared (NIR) observations of the host galaxy. From the absence of a spectral break in the optical/NIR colors of the host galaxy, we exclude the earlier suggestion that GRB980329 lies at a redshift of z >~5. We combine our data with the numerous multi-wavelength observations of the early afterglow, fit a comprehensive afterglow model to the entire broadband datas"},"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/0204141","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-04-08T21:36:02Z","cross_cats_sorted":[],"title_canon_sha256":"be2802be47262630430c004b26da7f9f36bc0a0199f3723ce72e0fb08ad9a063","abstract_canon_sha256":"0b0dae5f98511895f0717758db53c72f9c47cc676816671e25e4db7c2db994c9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:28:33.229561Z","signature_b64":"YwF8FDutoIu/i3QYdIoqDEtq2IA15Vjwly4ReBxF97nFlqejmcYt4k0UDnTkBS02cUrb68tw1GqKNPc0qN8lAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa4105ce0e9d651003d5ace0440960ad4870d91f1d03381875034c6b9ee694f2","last_reissued_at":"2026-07-04T17:28:33.229052Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:28:33.229052Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Broadband Afterglow of GRB980329","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. A. Frail, D. Reichart, D. S. Shepherd, D. W. Fox, E. Berger, F. A. Harrison, F. Walter, G. B. Taylor, G. H. Moriarty-Schieven, J. E. Larkin, J. S. Bloom, P. A. Price, R. Sari, R. W. Goodrich, S. A. Yost, S. G. Djorgovski, S. R. Kulkarni, T. J. Galama","submitted_at":"2002-04-08T21:36:02Z","abstract_excerpt":"We present radio observations of the afterglow of the bright gamma-ray burst GRB980329 made between one month and several years after the burst, a re-analysis of previously published submillimeter data, and late-time optical and near-infrared (NIR) observations of the host galaxy. From the absence of a spectral break in the optical/NIR colors of the host galaxy, we exclude the earlier suggestion that GRB980329 lies at a redshift of z >~5. We combine our data with the numerous multi-wavelength observations of the early afterglow, fit a comprehensive afterglow model to the entire broadband datas"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0204141","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0204141/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/0204141","created_at":"2026-07-04T17:28:33.229120+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0204141v2","created_at":"2026-07-04T17:28:33.229120+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0204141","created_at":"2026-07-04T17:28:33.229120+00:00"},{"alias_kind":"pith_short_12","alias_value":"7JAQLTQOTVSR","created_at":"2026-07-04T17:28:33.229120+00:00"},{"alias_kind":"pith_short_16","alias_value":"7JAQLTQOTVSRAA6V","created_at":"2026-07-04T17:28:33.229120+00:00"},{"alias_kind":"pith_short_8","alias_value":"7JAQLTQO","created_at":"2026-07-04T17:28:33.229120+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/7JAQLTQOTVSRAA6VVTQEICLAVV","json":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV.json","graph_json":"https://pith.science/api/pith-number/7JAQLTQOTVSRAA6VVTQEICLAVV/graph.json","events_json":"https://pith.science/api/pith-number/7JAQLTQOTVSRAA6VVTQEICLAVV/events.json","paper":"https://pith.science/paper/7JAQLTQO"},"agent_actions":{"view_html":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV","download_json":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV.json","view_paper":"https://pith.science/paper/7JAQLTQO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0204141&json=true","fetch_graph":"https://pith.science/api/pith-number/7JAQLTQOTVSRAA6VVTQEICLAVV/graph.json","fetch_events":"https://pith.science/api/pith-number/7JAQLTQOTVSRAA6VVTQEICLAVV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV/action/storage_attestation","attest_author":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV/action/author_attestation","sign_citation":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV/action/citation_signature","submit_replication":"https://pith.science/pith/7JAQLTQOTVSRAA6VVTQEICLAVV/action/replication_record"}},"created_at":"2026-07-04T17:28:33.229120+00:00","updated_at":"2026-07-04T17:28:33.229120+00:00"}