{"paper":{"title":"SXDF-ALMA 2-arcmin^2 Deep Survey: Stacking of Rest-Frame Near-Infrared Selected Objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bau-ching Hsieh, Bunyo Hatsukade, Daisuke Iono, David Hughes, Grant W. Wilson, Hideki Umehata, Itziar Aretxaga, James S. Dunlop, Jean Coupon, Karina I. Caputi, Ken-ichi Tadaki, Kentaro Motohara, Kotaro Kohno, Kouichiro Nakanish, Kouji Ohta, Minju Lee, Min S. Yun, Rob J. Ivison, Ryu Makiya, Sebastien Foucaud, Soh Ikarashi, Tadayuki Kodama, Wei-hao Wang, Wiphu Rujopakarn, Yoichi Tamura, Yuichi Matsuda, Yuki Yamaguchi","submitted_at":"2016-09-28T05:09:06Z","abstract_excerpt":"We present stacking analyses on our ALMA deep 1.1 mm imaging in the SXDF using 1.6 {\\mu}m and 3.6 {\\mu}m selected galaxies in the CANDELS WFC3 catalog. We detect a stacked flux of ~0.03-0.05 mJy, corresponding to LIR < 10^11 Lsun and a star formation rate (SFR) of ~ 15 Msun/yr at z = 2. We find that galaxies brighter in the rest-frame near-infrared tend to be also brighter at 1.1 mm, and galaxies fainter than m[3.6um] = 23 do not produce detectable 1.1 mm emission. This suggests a correlation between stellar mass and SFR, but outliers to this correlation are also observed, suggesting strongly "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.08772","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"}