SMA observations on faint Submillimeter Galaxies with S < 2 mJy: Ultra Dusty Low-Luminosity Galaxies at High Redshift
arXiv:1311.2943 · doi:10.1088/0004-637X/789/1/12
Abstract
We obtained SMA observations of eight faint (intrinsic 850 m fluxes 2 mJy) submillimeter galaxies (SMGs) discovered in SCUBA images of the massive lensing cluster fields A370, A2390, and A1689 and detected five. In total, we obtain 5 SMA detections, all of which have de-lensed fluxes 1 mJy with estimated total infrared luminosities 10 , comparable to luminous infrared galaxies (LIRGs) and normal star-forming galaxies. Based on the latest number counts, these galaxies contribute 70% of the 850 m extragalactic background light and represent the dominant star-forming galaxy population in the dusty universe. However, only 40% of our faint SMGs would be detected in deep optical or near-infrared surveys, which suggests many of these sources are at high redshifts () or extremely dusty, and they are not included in current star formation history estimates.
12 pages, 11 figures, ApJ in press
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