{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:5UY5ZJYSFT5Y3RWC72CFS7GT3I","short_pith_number":"pith:5UY5ZJYS","schema_version":"1.0","canonical_sha256":"ed31dca7122cfb8dc6c2fe84597cd3da0c4c400f09d774a331be7492178b3ef4","source":{"kind":"arxiv","id":"1903.02744","version":1},"attestation_state":"computed","paper":{"title":"ALMA twenty-six arcmin$^2$ survey of GOODS-S at one-millimeter (ASAGAO): Near-infrared-dark faint ALMA sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bunyo Hatsukade, Daniel Espada, Eiichi Egami, Haruka Kusakabe, Hideki Umehata, James S. Dunlop, Karina I. Caputi, Ken-ichi Tadaki, Kotaro Kohno, Masami Ouchi, Min S. Yun, Natsuki H. Hayatsu, Rob J. Ivison, Seiji Fujimoto, Tadayuki Kodama, Tao Wang, Tohru Nagao, Wei-hao Wang, Wiphu Rujopakarn, Yiping Ao, Yoichi Tamura, Yoshihiro Ueda, Yuki Yamaguchi, Yuki Yoshimura","submitted_at":"2019-03-07T06:45:19Z","abstract_excerpt":"We report detections of two 1.2 mm continuum sources ($S_\\mathrm{1.2mm}$ ~ 0.6 mJy) without any counterparts in the deep $H$- and/or $K$-band image (i.e., $K$-band magnitude $\\gtrsim$ 26 mag). These near-infrared-dark faint millimeter sources are uncovered by ASAGAO, a deep and wide-field ($\\simeq$ 26 arcmin$^2$) Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm survey. One has a red IRAC (3.6 and 4.5 $\\mu$m) counterpart, and the other has been independently detected at 850 and 870 $\\mu$m using SCUBA2 and ALMA Band 7, respectively. Their optical to radio spectral energy distributions "},"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":"1903.02744","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-03-07T06:45:19Z","cross_cats_sorted":[],"title_canon_sha256":"98656c0fcd06b716df95395800d186e38a64cde5f6f510d3744e207514f21ac5","abstract_canon_sha256":"9c35418bea3b122f9387fd7c08432bcd25b073c0fb018b58dbf92009753826ee"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:43:03.116573Z","signature_b64":"RO/zOigUJ99H0GwJlnt+8e99jh/DUNTrU7PgUUFzbRC2hpumLTAekJAkvFph2NwprhofRWO6gommNLs6bBW+CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ed31dca7122cfb8dc6c2fe84597cd3da0c4c400f09d774a331be7492178b3ef4","last_reissued_at":"2026-05-17T23:43:03.116070Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:43:03.116070Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA twenty-six arcmin$^2$ survey of GOODS-S at one-millimeter (ASAGAO): Near-infrared-dark faint ALMA sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bunyo Hatsukade, Daniel Espada, Eiichi Egami, Haruka Kusakabe, Hideki Umehata, James S. Dunlop, Karina I. Caputi, Ken-ichi Tadaki, Kotaro Kohno, Masami Ouchi, Min S. Yun, Natsuki H. Hayatsu, Rob J. Ivison, Seiji Fujimoto, Tadayuki Kodama, Tao Wang, Tohru Nagao, Wei-hao Wang, Wiphu Rujopakarn, Yiping Ao, Yoichi Tamura, Yoshihiro Ueda, Yuki Yamaguchi, Yuki Yoshimura","submitted_at":"2019-03-07T06:45:19Z","abstract_excerpt":"We report detections of two 1.2 mm continuum sources ($S_\\mathrm{1.2mm}$ ~ 0.6 mJy) without any counterparts in the deep $H$- and/or $K$-band image (i.e., $K$-band magnitude $\\gtrsim$ 26 mag). These near-infrared-dark faint millimeter sources are uncovered by ASAGAO, a deep and wide-field ($\\simeq$ 26 arcmin$^2$) Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm survey. One has a red IRAC (3.6 and 4.5 $\\mu$m) counterpart, and the other has been independently detected at 850 and 870 $\\mu$m using SCUBA2 and ALMA Band 7, respectively. Their optical to radio spectral energy distributions "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.02744","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":"1903.02744","created_at":"2026-05-17T23:43:03.116150+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.02744v1","created_at":"2026-05-17T23:43:03.116150+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.02744","created_at":"2026-05-17T23:43:03.116150+00:00"},{"alias_kind":"pith_short_12","alias_value":"5UY5ZJYSFT5Y","created_at":"2026-05-18T12:33:10.108867+00:00"},{"alias_kind":"pith_short_16","alias_value":"5UY5ZJYSFT5Y3RWC","created_at":"2026-05-18T12:33:10.108867+00:00"},{"alias_kind":"pith_short_8","alias_value":"5UY5ZJYS","created_at":"2026-05-18T12:33:10.108867+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/5UY5ZJYSFT5Y3RWC72CFS7GT3I","json":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I.json","graph_json":"https://pith.science/api/pith-number/5UY5ZJYSFT5Y3RWC72CFS7GT3I/graph.json","events_json":"https://pith.science/api/pith-number/5UY5ZJYSFT5Y3RWC72CFS7GT3I/events.json","paper":"https://pith.science/paper/5UY5ZJYS"},"agent_actions":{"view_html":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I","download_json":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I.json","view_paper":"https://pith.science/paper/5UY5ZJYS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.02744&json=true","fetch_graph":"https://pith.science/api/pith-number/5UY5ZJYSFT5Y3RWC72CFS7GT3I/graph.json","fetch_events":"https://pith.science/api/pith-number/5UY5ZJYSFT5Y3RWC72CFS7GT3I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I/action/storage_attestation","attest_author":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I/action/author_attestation","sign_citation":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I/action/citation_signature","submit_replication":"https://pith.science/pith/5UY5ZJYSFT5Y3RWC72CFS7GT3I/action/replication_record"}},"created_at":"2026-05-17T23:43:03.116150+00:00","updated_at":"2026-05-17T23:43:03.116150+00:00"}