{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:5TJH5BCZCOFWBUYF7Z5XNKWWHY","short_pith_number":"pith:5TJH5BCZ","schema_version":"1.0","canonical_sha256":"ecd27e8459138b60d305fe7b76aad63e0cdfbd02bca2cd4c38b1aca43d7d3065","source":{"kind":"arxiv","id":"1307.3556","version":1},"attestation_state":"computed","paper":{"title":"Herschel reveals the obscured star formation in HiZELS H\\alpha\\ emitters at z=1.47","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cava, A. Conley, A.J. Smith, B. Magnelli, B. Schulz, D. Farrah, D. Lutz, D. Sobral, E. Ibar, E. Le Floc'h, F. Pozzi, G. Magdis, G. Marsden, I. Smail, J. Bock, J. Wardlow, K. Kohno, L. Riguccini, L. Wang, M. B\\'ethermin, M.J. Page, M. Symeonidis, M. Zemcov, N. Seymour, P.N. Best, R.J. Ivison, S. Berta, S. Ikarashi, S.J. Oliver, V. Arumugam","submitted_at":"2013-07-12T20:00:04Z","abstract_excerpt":"We describe the far-infrared (FIR; rest-frame 8--1000\\mu m) properties of a sample of 443 H\\alpha-selected star-forming galaxies in the COSMOS and UDS fields detected by the HiZELS imaging survey. Sources are identified using narrow-band filters in combination with broad-band photometry to uniformly select H\\alpha\\ (and [OII] if available) emitters in a narrow redshift slice at z = 1.47+/-0.02. We use a stacking approach in Spitzer, Herschel (from PEP and HerMES surveys) and AzTEC images to describe their typical FIR properties. We find that HiZELS galaxies with observed H\\alpha\\ luminosities "},"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":"1307.3556","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-07-12T20:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"5f01d95d3b986c61c5f59a192216a944f6e0abbe5c4f57edee1c9be6797a5a90","abstract_canon_sha256":"a7758dccec9fb40503c400c23462533d1e9aa44525a03de99537824d8abf20ba"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:48:50.824174Z","signature_b64":"xluoI2kFqYmK03HC7WUVlNXfWBqXHla3BIjLg35YDapelm1eXwftQnx3f1Ka9u4SIGFw3fXfBR6+TyDMP8wXCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ecd27e8459138b60d305fe7b76aad63e0cdfbd02bca2cd4c38b1aca43d7d3065","last_reissued_at":"2026-05-18T01:48:50.823452Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:48:50.823452Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel reveals the obscured star formation in HiZELS H\\alpha\\ emitters at z=1.47","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cava, A. Conley, A.J. Smith, B. Magnelli, B. Schulz, D. Farrah, D. Lutz, D. Sobral, E. Ibar, E. Le Floc'h, F. Pozzi, G. Magdis, G. Marsden, I. Smail, J. Bock, J. Wardlow, K. Kohno, L. Riguccini, L. Wang, M. B\\'ethermin, M.J. Page, M. Symeonidis, M. Zemcov, N. Seymour, P.N. Best, R.J. Ivison, S. Berta, S. Ikarashi, S.J. Oliver, V. Arumugam","submitted_at":"2013-07-12T20:00:04Z","abstract_excerpt":"We describe the far-infrared (FIR; rest-frame 8--1000\\mu m) properties of a sample of 443 H\\alpha-selected star-forming galaxies in the COSMOS and UDS fields detected by the HiZELS imaging survey. Sources are identified using narrow-band filters in combination with broad-band photometry to uniformly select H\\alpha\\ (and [OII] if available) emitters in a narrow redshift slice at z = 1.47+/-0.02. We use a stacking approach in Spitzer, Herschel (from PEP and HerMES surveys) and AzTEC images to describe their typical FIR properties. We find that HiZELS galaxies with observed H\\alpha\\ luminosities "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.3556","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":"1307.3556","created_at":"2026-05-18T01:48:50.823580+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.3556v1","created_at":"2026-05-18T01:48:50.823580+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.3556","created_at":"2026-05-18T01:48:50.823580+00:00"},{"alias_kind":"pith_short_12","alias_value":"5TJH5BCZCOFW","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"5TJH5BCZCOFWBUYF","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"5TJH5BCZ","created_at":"2026-05-18T12:27:34.582898+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/5TJH5BCZCOFWBUYF7Z5XNKWWHY","json":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY.json","graph_json":"https://pith.science/api/pith-number/5TJH5BCZCOFWBUYF7Z5XNKWWHY/graph.json","events_json":"https://pith.science/api/pith-number/5TJH5BCZCOFWBUYF7Z5XNKWWHY/events.json","paper":"https://pith.science/paper/5TJH5BCZ"},"agent_actions":{"view_html":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY","download_json":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY.json","view_paper":"https://pith.science/paper/5TJH5BCZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.3556&json=true","fetch_graph":"https://pith.science/api/pith-number/5TJH5BCZCOFWBUYF7Z5XNKWWHY/graph.json","fetch_events":"https://pith.science/api/pith-number/5TJH5BCZCOFWBUYF7Z5XNKWWHY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY/action/storage_attestation","attest_author":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY/action/author_attestation","sign_citation":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY/action/citation_signature","submit_replication":"https://pith.science/pith/5TJH5BCZCOFWBUYF7Z5XNKWWHY/action/replication_record"}},"created_at":"2026-05-18T01:48:50.823580+00:00","updated_at":"2026-05-18T01:48:50.823580+00:00"}