{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:R3SGFXC42HE2PFPPMG63J4IWAX","short_pith_number":"pith:R3SGFXC4","schema_version":"1.0","canonical_sha256":"8ee462dc5cd1c9a795ef61bdb4f11605d0647f99ce5f358a27541d680f91bb71","source":{"kind":"arxiv","id":"1211.2807","version":1},"attestation_state":"computed","paper":{"title":"ALMA Submillimeter Continuum Imaging of the Host Galaxies of GRB021004 and GRB080607","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Hsiao-Wen Chen (KICP/UChicago), Kui-Yun Huang (ASIAA), Wei-Hao Wang (ASIAA)","submitted_at":"2012-11-12T21:00:02Z","abstract_excerpt":"We report 345 GHz continuum observations of the host galaxies of gamma-ray bursts (GRBs) 021004 and 080607 at z>2 using the Atacama Large Millimeter/Submillimeter Array (ALMA) in Cycle 0. Of the two bursts, GRB021004 is one of the few GRBs that originates in a Lyman limit host, while GRB080607 is classified as a \"dark burst\" and its host galaxy is a candidate of dusty star forming galaxy at z~3. With an order of magnitude improvement in the sensitivities of the new imaging searches, we detect the host galaxy of GRB080607 with a flux of S_{345} = 0.31+/-0.09 mJy and a corresponding infrared lum"},"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":"1211.2807","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-11-12T21:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"86d82670a2dca37bcde6d576a4a1c76a1581d462b44d886a1513131c560e22fa","abstract_canon_sha256":"d3c43f9c18f2270da25ffc54a73fc97243cc7144e5875a41fa0dc0e92f0e7beb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:16.529376Z","signature_b64":"qCrkAb7OQbGC8smHMbXZvh9kK64x1Vub85jMQZj29g0lVuQa6dMpCPje4jYMOSFmjsUSFoq89xP/s7XA/qfJAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8ee462dc5cd1c9a795ef61bdb4f11605d0647f99ce5f358a27541d680f91bb71","last_reissued_at":"2026-05-18T01:53:16.528917Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:16.528917Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA Submillimeter Continuum Imaging of the Host Galaxies of GRB021004 and GRB080607","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Hsiao-Wen Chen (KICP/UChicago), Kui-Yun Huang (ASIAA), Wei-Hao Wang (ASIAA)","submitted_at":"2012-11-12T21:00:02Z","abstract_excerpt":"We report 345 GHz continuum observations of the host galaxies of gamma-ray bursts (GRBs) 021004 and 080607 at z>2 using the Atacama Large Millimeter/Submillimeter Array (ALMA) in Cycle 0. Of the two bursts, GRB021004 is one of the few GRBs that originates in a Lyman limit host, while GRB080607 is classified as a \"dark burst\" and its host galaxy is a candidate of dusty star forming galaxy at z~3. With an order of magnitude improvement in the sensitivities of the new imaging searches, we detect the host galaxy of GRB080607 with a flux of S_{345} = 0.31+/-0.09 mJy and a corresponding infrared lum"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.2807","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":"1211.2807","created_at":"2026-05-18T01:53:16.528992+00:00"},{"alias_kind":"arxiv_version","alias_value":"1211.2807v1","created_at":"2026-05-18T01:53:16.528992+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.2807","created_at":"2026-05-18T01:53:16.528992+00:00"},{"alias_kind":"pith_short_12","alias_value":"R3SGFXC42HE2","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_16","alias_value":"R3SGFXC42HE2PFPP","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_8","alias_value":"R3SGFXC4","created_at":"2026-05-18T12:27:20.899486+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/R3SGFXC42HE2PFPPMG63J4IWAX","json":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX.json","graph_json":"https://pith.science/api/pith-number/R3SGFXC42HE2PFPPMG63J4IWAX/graph.json","events_json":"https://pith.science/api/pith-number/R3SGFXC42HE2PFPPMG63J4IWAX/events.json","paper":"https://pith.science/paper/R3SGFXC4"},"agent_actions":{"view_html":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX","download_json":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX.json","view_paper":"https://pith.science/paper/R3SGFXC4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1211.2807&json=true","fetch_graph":"https://pith.science/api/pith-number/R3SGFXC42HE2PFPPMG63J4IWAX/graph.json","fetch_events":"https://pith.science/api/pith-number/R3SGFXC42HE2PFPPMG63J4IWAX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX/action/storage_attestation","attest_author":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX/action/author_attestation","sign_citation":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX/action/citation_signature","submit_replication":"https://pith.science/pith/R3SGFXC42HE2PFPPMG63J4IWAX/action/replication_record"}},"created_at":"2026-05-18T01:53:16.528992+00:00","updated_at":"2026-05-18T01:53:16.528992+00:00"}