{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:JRDLILTQQ3NWLL4QWZT7Z7A7CP","short_pith_number":"pith:JRDLILTQ","schema_version":"1.0","canonical_sha256":"4c46b42e7086db65af90b667fcfc1f13ceaafa5f694fa9f390eb6835eddf4f52","source":{"kind":"arxiv","id":"1705.01222","version":2},"attestation_state":"computed","paper":{"title":"SILVERRUSH. IV. Ly$\\alpha$ Luminosity Functions at $z = 5.7$ and $6.6$ Studied with $\\sim$ 1,300 LAEs on the $14-21$ deg$^2$ Sky","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akio K. Inoue, Akira Konno, Haruka Kusakabe, Hisanori Furusawa, Kazuhiro Shimasaku, Kimihiko Nakajima, Masakazu A. R. Kobayashi, Masami Ouchi, Masamune Oguri, Masaru Kajisawa, Nobunari Kashikawa, Ryo Higuchi, Satoshi Miyazaki, Shiang-Yu Wang, Takatoshi Shibuya, Tohru Nagao, Tomotsugu Goto, Yoshiaki Ono, Yoshiaki Taniguchi, Yuichi Harikane, Yutaka Komiyama","submitted_at":"2017-05-03T01:35:12Z","abstract_excerpt":"We present the Ly$\\alpha$ luminosity functions (LFs) at $z=$5.7 and 6.6 derived from a new large sample of 1,266 Ly$\\alpha$ emitters (LAEs) identified in total areas of 14 and 21 deg$^2$, respectively, based on the early narrowband data of the Subaru/Hyper Suprime-Cam (HSC) survey. Together with careful Monte-Carlo simulations that account for the incompleteness of the LAE selection and the flux estimate systematics in the narrowband imaging, we have determined the Ly$\\alpha$ LFs with the unprecedentedly small statistical and systematic uncertainties in a wide Ly$\\alpha$ luminosity range of $1"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1705.01222","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-03T01:35:12Z","cross_cats_sorted":[],"title_canon_sha256":"cda5bfa78d2abbf730864ea7d02c7f969e7b321baa7c76e40777aee0ffc0cc80","abstract_canon_sha256":"660395894ad8bf76f3efffba7a0d2b3f72f739d1fefe655d279f29339ff7c715"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:30.142833Z","signature_b64":"BZeGa/BIHiarQEpx69M90snV3GXvBoPhf1QjQsjcebzHeCKMPQlTq2DxTNCAcZ8exksB+bQvLoKEwdHtiHioDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4c46b42e7086db65af90b667fcfc1f13ceaafa5f694fa9f390eb6835eddf4f52","last_reissued_at":"2026-05-18T00:26:30.142015Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:30.142015Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SILVERRUSH. IV. Ly$\\alpha$ Luminosity Functions at $z = 5.7$ and $6.6$ Studied with $\\sim$ 1,300 LAEs on the $14-21$ deg$^2$ Sky","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akio K. Inoue, Akira Konno, Haruka Kusakabe, Hisanori Furusawa, Kazuhiro Shimasaku, Kimihiko Nakajima, Masakazu A. R. Kobayashi, Masami Ouchi, Masamune Oguri, Masaru Kajisawa, Nobunari Kashikawa, Ryo Higuchi, Satoshi Miyazaki, Shiang-Yu Wang, Takatoshi Shibuya, Tohru Nagao, Tomotsugu Goto, Yoshiaki Ono, Yoshiaki Taniguchi, Yuichi Harikane, Yutaka Komiyama","submitted_at":"2017-05-03T01:35:12Z","abstract_excerpt":"We present the Ly$\\alpha$ luminosity functions (LFs) at $z=$5.7 and 6.6 derived from a new large sample of 1,266 Ly$\\alpha$ emitters (LAEs) identified in total areas of 14 and 21 deg$^2$, respectively, based on the early narrowband data of the Subaru/Hyper Suprime-Cam (HSC) survey. Together with careful Monte-Carlo simulations that account for the incompleteness of the LAE selection and the flux estimate systematics in the narrowband imaging, we have determined the Ly$\\alpha$ LFs with the unprecedentedly small statistical and systematic uncertainties in a wide Ly$\\alpha$ luminosity range of $1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.01222","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":"1705.01222","created_at":"2026-05-18T00:26:30.142162+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.01222v2","created_at":"2026-05-18T00:26:30.142162+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.01222","created_at":"2026-05-18T00:26:30.142162+00:00"},{"alias_kind":"pith_short_12","alias_value":"JRDLILTQQ3NW","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"JRDLILTQQ3NWLL4Q","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"JRDLILTQ","created_at":"2026-05-18T12:31:24.725408+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2602.15803","citing_title":"Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP","json":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP.json","graph_json":"https://pith.science/api/pith-number/JRDLILTQQ3NWLL4QWZT7Z7A7CP/graph.json","events_json":"https://pith.science/api/pith-number/JRDLILTQQ3NWLL4QWZT7Z7A7CP/events.json","paper":"https://pith.science/paper/JRDLILTQ"},"agent_actions":{"view_html":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP","download_json":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP.json","view_paper":"https://pith.science/paper/JRDLILTQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.01222&json=true","fetch_graph":"https://pith.science/api/pith-number/JRDLILTQQ3NWLL4QWZT7Z7A7CP/graph.json","fetch_events":"https://pith.science/api/pith-number/JRDLILTQQ3NWLL4QWZT7Z7A7CP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP/action/storage_attestation","attest_author":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP/action/author_attestation","sign_citation":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP/action/citation_signature","submit_replication":"https://pith.science/pith/JRDLILTQQ3NWLL4QWZT7Z7A7CP/action/replication_record"}},"created_at":"2026-05-18T00:26:30.142162+00:00","updated_at":"2026-05-18T00:26:30.142162+00:00"}