{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:PC2OUH2KYNX6XGETLCIEUXB2QP","short_pith_number":"pith:PC2OUH2K","schema_version":"1.0","canonical_sha256":"78b4ea1f4ac36feb989358904a5c3a83c54c9e883b431b7da6e76dafef6c3ac5","source":{"kind":"arxiv","id":"1705.00733","version":2},"attestation_state":"computed","paper":{"title":"SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Akira Konno, Chien-Hsiu Lee, Crystal L. Martin, Haruka Kusakabe, Hisanori Furusawa, Kazuhiro Shimasaku, Kimihiko Nakajima, Masakazu A. R. Kobayashi, Masami Ouchi, Masaru Kajisawa, Masayuki Tanaka, Michael Rauch, Nobunari Kashikawa, Rieko Momose, Ryo Higuchi, Shiang-Yu Wang, Shiro Mukae, Suraphong Yuma, Takashi Kojima, Takatoshi Shibuya, Tohru Nagao, Tomotsugu Goto, Yoshiaki Ono, Yoshiaki Taniguchi, Yuichi Harikane, Yutaka Komiyama","submitted_at":"2017-05-01T22:41:55Z","abstract_excerpt":"We present Lya and UV-nebular emission line properties of bright Lya emitters (LAEs) at z=6-7 with a luminosity of log L_Lya/[erg s-1] = 43-44 identified in the 21-deg2 area of the SILVERRUSH early sample developed with the Subaru Hyper Suprime-Cam (HSC) survey data. Our optical spectroscopy newly confirm 21 bright LAEs with clear Lya emission, and contribute to make a spectroscopic sample of 96 LAEs at z=6-7 in SILVERRUSH. From the spectroscopic sample, we select 7 remarkable LAEs as bright as Himiko and CR7 objects, and perform deep Keck/MOSFIRE and Subaru/nuMOIRCS near-infrared spectroscopy"},"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":"1705.00733","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-01T22:41:55Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"065a175c6d12689f0c626dd1329ea5a10584f0d7d22e2933ca9190219fa61959","abstract_canon_sha256":"a7a66ee7132bce37f68ceb2369a98108a8eab8ab17ea6638cac2f8a563f80db0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:30.162311Z","signature_b64":"TJmPtWg3bsOcBtPLkxXWluBx82rOHiHni8L9V2T8J5A5nxs6C8rN0QwU1Miu6DMVt+NDdLDoDvLQ21HoAX+UDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"78b4ea1f4ac36feb989358904a5c3a83c54c9e883b431b7da6e76dafef6c3ac5","last_reissued_at":"2026-05-18T00:26:30.161745Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:30.161745Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Akira Konno, Chien-Hsiu Lee, Crystal L. Martin, Haruka Kusakabe, Hisanori Furusawa, Kazuhiro Shimasaku, Kimihiko Nakajima, Masakazu A. R. Kobayashi, Masami Ouchi, Masaru Kajisawa, Masayuki Tanaka, Michael Rauch, Nobunari Kashikawa, Rieko Momose, Ryo Higuchi, Shiang-Yu Wang, Shiro Mukae, Suraphong Yuma, Takashi Kojima, Takatoshi Shibuya, Tohru Nagao, Tomotsugu Goto, Yoshiaki Ono, Yoshiaki Taniguchi, Yuichi Harikane, Yutaka Komiyama","submitted_at":"2017-05-01T22:41:55Z","abstract_excerpt":"We present Lya and UV-nebular emission line properties of bright Lya emitters (LAEs) at z=6-7 with a luminosity of log L_Lya/[erg s-1] = 43-44 identified in the 21-deg2 area of the SILVERRUSH early sample developed with the Subaru Hyper Suprime-Cam (HSC) survey data. Our optical spectroscopy newly confirm 21 bright LAEs with clear Lya emission, and contribute to make a spectroscopic sample of 96 LAEs at z=6-7 in SILVERRUSH. From the spectroscopic sample, we select 7 remarkable LAEs as bright as Himiko and CR7 objects, and perform deep Keck/MOSFIRE and Subaru/nuMOIRCS near-infrared spectroscopy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.00733","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":""},"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":"1705.00733","created_at":"2026-05-18T00:26:30.161867+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.00733v2","created_at":"2026-05-18T00:26:30.161867+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.00733","created_at":"2026-05-18T00:26:30.161867+00:00"},{"alias_kind":"pith_short_12","alias_value":"PC2OUH2KYNX6","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_16","alias_value":"PC2OUH2KYNX6XGET","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_8","alias_value":"PC2OUH2K","created_at":"2026-05-18T12:31:37.085036+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/PC2OUH2KYNX6XGETLCIEUXB2QP","json":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP.json","graph_json":"https://pith.science/api/pith-number/PC2OUH2KYNX6XGETLCIEUXB2QP/graph.json","events_json":"https://pith.science/api/pith-number/PC2OUH2KYNX6XGETLCIEUXB2QP/events.json","paper":"https://pith.science/paper/PC2OUH2K"},"agent_actions":{"view_html":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP","download_json":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP.json","view_paper":"https://pith.science/paper/PC2OUH2K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.00733&json=true","fetch_graph":"https://pith.science/api/pith-number/PC2OUH2KYNX6XGETLCIEUXB2QP/graph.json","fetch_events":"https://pith.science/api/pith-number/PC2OUH2KYNX6XGETLCIEUXB2QP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP/action/storage_attestation","attest_author":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP/action/author_attestation","sign_citation":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP/action/citation_signature","submit_replication":"https://pith.science/pith/PC2OUH2KYNX6XGETLCIEUXB2QP/action/replication_record"}},"created_at":"2026-05-18T00:26:30.161867+00:00","updated_at":"2026-05-18T00:26:30.161867+00:00"}