{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:DO6K36HEETIXVGKEQ2V4RIXHFF","short_pith_number":"pith:DO6K36HE","schema_version":"1.0","canonical_sha256":"1bbcadf8e424d17a994486abc8a2e72962aa2b1017e81f388e24370b95a66d25","source":{"kind":"arxiv","id":"1308.5129","version":2},"attestation_state":"computed","paper":{"title":"A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Fumihide Iwamuro, Gavin Dalton, Jean Coupon, Karl Glazebrook, Kiyoto Yabe, Lee R. Spitler, Masanao Sumiyoshi, Masayuki Akiyama, Motonari Tonegawa, Naoyuki Tamura, Tomonori Totani, Tomotsugu Goto","submitted_at":"2013-08-23T14:08:43Z","abstract_excerpt":"The efficient selection of high-redshift emission galaxies is important for future large galaxy redshift surveys for cosmology. Here we describe the target selection methods for the FastSound project, a redshift survey for H alpha emitting galaxies at z=1.2-1.5 using Subaru/FMOS to measure the linear growth rate f\\sigma 8 via Redshift Space Distortion (RSD) and constrain the theory of gravity. To select ~400 target galaxies in the 0.2 deg^2 FMOS field-of-view from photometric data of CFHTLS-Wide (u*g'r'i'z'), we test several different methods based on color-color diagrams or photometric redshi"},"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":"1308.5129","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-08-23T14:08:43Z","cross_cats_sorted":[],"title_canon_sha256":"322d474fa59c7435b8d1dda1b910d397d0cf03ea2957b2213a79f18c83878cfd","abstract_canon_sha256":"524cb9106b4f81e33649c395d5d530e423f6949853c578071885aca51bccb66f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:14:09.637653Z","signature_b64":"PEbDSBmwOaLMV+HSCOlyxDLrFaBbO9lqTx2QJBt1i3tzcyRkmuz5LAEfdsg1oi71R61awYmvil7Q1XD69o0IAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1bbcadf8e424d17a994486abc8a2e72962aa2b1017e81f388e24370b95a66d25","last_reissued_at":"2026-05-18T01:14:09.637100Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:14:09.637100Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Fumihide Iwamuro, Gavin Dalton, Jean Coupon, Karl Glazebrook, Kiyoto Yabe, Lee R. Spitler, Masanao Sumiyoshi, Masayuki Akiyama, Motonari Tonegawa, Naoyuki Tamura, Tomonori Totani, Tomotsugu Goto","submitted_at":"2013-08-23T14:08:43Z","abstract_excerpt":"The efficient selection of high-redshift emission galaxies is important for future large galaxy redshift surveys for cosmology. Here we describe the target selection methods for the FastSound project, a redshift survey for H alpha emitting galaxies at z=1.2-1.5 using Subaru/FMOS to measure the linear growth rate f\\sigma 8 via Redshift Space Distortion (RSD) and constrain the theory of gravity. To select ~400 target galaxies in the 0.2 deg^2 FMOS field-of-view from photometric data of CFHTLS-Wide (u*g'r'i'z'), we test several different methods based on color-color diagrams or photometric redshi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.5129","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":"1308.5129","created_at":"2026-05-18T01:14:09.637184+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.5129v2","created_at":"2026-05-18T01:14:09.637184+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.5129","created_at":"2026-05-18T01:14:09.637184+00:00"},{"alias_kind":"pith_short_12","alias_value":"DO6K36HEETIX","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_16","alias_value":"DO6K36HEETIXVGKE","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_8","alias_value":"DO6K36HE","created_at":"2026-05-18T12:27:43.054852+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/DO6K36HEETIXVGKEQ2V4RIXHFF","json":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF.json","graph_json":"https://pith.science/api/pith-number/DO6K36HEETIXVGKEQ2V4RIXHFF/graph.json","events_json":"https://pith.science/api/pith-number/DO6K36HEETIXVGKEQ2V4RIXHFF/events.json","paper":"https://pith.science/paper/DO6K36HE"},"agent_actions":{"view_html":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF","download_json":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF.json","view_paper":"https://pith.science/paper/DO6K36HE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.5129&json=true","fetch_graph":"https://pith.science/api/pith-number/DO6K36HEETIXVGKEQ2V4RIXHFF/graph.json","fetch_events":"https://pith.science/api/pith-number/DO6K36HEETIXVGKEQ2V4RIXHFF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF/action/storage_attestation","attest_author":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF/action/author_attestation","sign_citation":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF/action/citation_signature","submit_replication":"https://pith.science/pith/DO6K36HEETIXVGKEQ2V4RIXHFF/action/replication_record"}},"created_at":"2026-05-18T01:14:09.637184+00:00","updated_at":"2026-05-18T01:14:09.637184+00:00"}