{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:YVAQLQJTI3O7YVLLYCOPRBDIXX","short_pith_number":"pith:YVAQLQJT","schema_version":"1.0","canonical_sha256":"c54105c13346ddfc556bc09cf88468bdde054070ebee20e63b1f59e3fef997ac","source":{"kind":"arxiv","id":"1504.05592","version":2},"attestation_state":"computed","paper":{"title":"The Subaru FMOS Galaxy Redshift Survey (FastSound). II. The Emission Line Catalog and Properties of Emission Line Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Andrew J. Bunker, Chiaki Hikage, Fumihide Iwamuro, Gavin Dalton, Hiroyuki Okada, Ikkoh Shimizu, Karl Glazebrook, Kiyoto Yabe, Kouji Ohta, Masayuki Akiyama, Motonari Tonegawa, Naoyuki Tamura, Naruhisa Takato, Takashi Ishikawa, Teppei Okumura, Tomonori Totani, Tomotsugu Goto","submitted_at":"2015-04-21T20:01:40Z","abstract_excerpt":"We present basic properties of $\\sim$3,300 emission line galaxies detected by the FastSound survey, which are mostly H$\\alpha$ emitters at $z \\sim$ 1.2-1.5 in the total area of about 20 deg$^2$, with the H$\\alpha$ flux sensitivity limit of $\\sim 1.6 \\times 10^{-16} \\rm erg \\ cm^{-2} s^{-1}$ at 4.5 sigma. This paper presents the catalogs of the FastSound emission lines and galaxies, which will be open to the public in the near future. We also present basic properties of typical FastSound H$\\alpha$ emitters, which have H$\\alpha$ luminosities of $10^{41.8}$-$10^{43.3}$ erg/s, SFRs of 20--500 $M_\\"},"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":"1504.05592","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-04-21T20:01:40Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"936276ac537f90d69a94677c6f249450e2ac129329f95245e75fdf518d347a45","abstract_canon_sha256":"e0de6788104fdaf3fecd388c06eb04a3efc6a6238bd9d24043a7819c6933e7d5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:16.802743Z","signature_b64":"inZPxl5BjecjfGWSQN79k8jCOd4s8txVfSszrLm2vEWTSOiKlvg2+RzW4GeDdgwwBSKzbizuI3L3Cw/AjwYcCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c54105c13346ddfc556bc09cf88468bdde054070ebee20e63b1f59e3fef997ac","last_reissued_at":"2026-05-18T01:13:16.802131Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:16.802131Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Subaru FMOS Galaxy Redshift Survey (FastSound). II. The Emission Line Catalog and Properties of Emission Line Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Andrew J. Bunker, Chiaki Hikage, Fumihide Iwamuro, Gavin Dalton, Hiroyuki Okada, Ikkoh Shimizu, Karl Glazebrook, Kiyoto Yabe, Kouji Ohta, Masayuki Akiyama, Motonari Tonegawa, Naoyuki Tamura, Naruhisa Takato, Takashi Ishikawa, Teppei Okumura, Tomonori Totani, Tomotsugu Goto","submitted_at":"2015-04-21T20:01:40Z","abstract_excerpt":"We present basic properties of $\\sim$3,300 emission line galaxies detected by the FastSound survey, which are mostly H$\\alpha$ emitters at $z \\sim$ 1.2-1.5 in the total area of about 20 deg$^2$, with the H$\\alpha$ flux sensitivity limit of $\\sim 1.6 \\times 10^{-16} \\rm erg \\ cm^{-2} s^{-1}$ at 4.5 sigma. This paper presents the catalogs of the FastSound emission lines and galaxies, which will be open to the public in the near future. We also present basic properties of typical FastSound H$\\alpha$ emitters, which have H$\\alpha$ luminosities of $10^{41.8}$-$10^{43.3}$ erg/s, SFRs of 20--500 $M_\\"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.05592","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":"1504.05592","created_at":"2026-05-18T01:13:16.802233+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.05592v2","created_at":"2026-05-18T01:13:16.802233+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.05592","created_at":"2026-05-18T01:13:16.802233+00:00"},{"alias_kind":"pith_short_12","alias_value":"YVAQLQJTI3O7","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_16","alias_value":"YVAQLQJTI3O7YVLL","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_8","alias_value":"YVAQLQJT","created_at":"2026-05-18T12:29:52.810259+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/YVAQLQJTI3O7YVLLYCOPRBDIXX","json":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX.json","graph_json":"https://pith.science/api/pith-number/YVAQLQJTI3O7YVLLYCOPRBDIXX/graph.json","events_json":"https://pith.science/api/pith-number/YVAQLQJTI3O7YVLLYCOPRBDIXX/events.json","paper":"https://pith.science/paper/YVAQLQJT"},"agent_actions":{"view_html":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX","download_json":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX.json","view_paper":"https://pith.science/paper/YVAQLQJT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.05592&json=true","fetch_graph":"https://pith.science/api/pith-number/YVAQLQJTI3O7YVLLYCOPRBDIXX/graph.json","fetch_events":"https://pith.science/api/pith-number/YVAQLQJTI3O7YVLLYCOPRBDIXX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX/action/storage_attestation","attest_author":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX/action/author_attestation","sign_citation":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX/action/citation_signature","submit_replication":"https://pith.science/pith/YVAQLQJTI3O7YVLLYCOPRBDIXX/action/replication_record"}},"created_at":"2026-05-18T01:13:16.802233+00:00","updated_at":"2026-05-18T01:13:16.802233+00:00"}