266 citations · 2.4k across the 29 of their papers we have counts for
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Detection of Strong Millimeter Emission from the Circumstellar Dust Disk Around V1094 Sco: Cold and Massive Disk around a T Tauri Star in a Quiescent Accretion Phase?
Takashi Tsukagoshi, Masao Saito, Yoshimi Kitamura +16
We present the discovery of a cold massive dust disk around the T Tauri star V1094 Sco in the Lupus molecular cloud from the 1.1 millimeter continuum observations with AzTEC on AST…
AzTEC/ASTE 1.1-mm Survey of the AKARI Deep Field South: source catalogue and number counts
B. Hatsukade, K. Kohno, I. Aretxaga +20
We present results of a 1.1 mm deep survey of the AKARI Deep Field South (ADF-S) with AzTEC mounted on the Atacama Submillimetre Telescope Experiment (ASTE). We obtained a map of 0…
Origins of the extragalactic background at 1mm from a combined analysis of the AzTEC and MAMBO data in GOODS-N
Kyle Penner, Alexandra Pope, Edward L. Chapin +13
We present a study of the cosmic infrared background, which is a measure of the dust obscured activity in all galaxies in the Universe. We venture to isolate the galaxies responsib…
Detection of an ultra-bright submillimeter galaxy in the Subaru/XMM-Newton Deep Field using AzTEC/ASTE
S. Ikarashi, K. Kohno, J. E. Aguirre +40
We report the detection of an extremely bright (37 mJy at 1100 m and 91 mJy at 880 m) submillimeter galaxy (SMG), AzTEC-ASTE-SXDF1100.001 (hereafter referred to a…
Deep 1.1 mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts
K. S. Scott, M. S. Yun, G. W. Wilson +20
[Abridged] We present the first results from a 1.1 mm confusion-limited map of the GOODS-S field taken with AzTEC on the ASTE telescope. We imaged a 270 sq. arcmin field to a 1σdep…
An Investigation of the Dust Content in the Galaxy pair NGC 1512/1510 from Near-Infrared to Millimeter Wavelengths
Guilin Liu, Daniela Calzetti, Min S. Yun +10
We combine new ASTE/AzTEC 1.1 mm maps of the galaxy pair NGC 1512/1510 with archival Spitzer IRAC and MIPS images covering the wavelength range 3.6--160 um from the SINGS project t…