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A puzzling non-detection of [O III] and [C II] from a galaxy observed with ALMA
C. Binggeli, A. K. Inoue, T. Hashimoto +12
Characterizing the galaxy population in the early Universe holds the key to understanding the evolution of these objects and the role they played in cosmic reionization. However, t…
ALMA Deep Field in SSA22: A near-infrared-dark submillimeter galaxy at z=4.0
Hideki Umehata, Ian Smail, A. M. Swinbank +8
Deep surveys with Atacama Large Millimeter Array (ALMA) have uncovered a population of dusty star-forming galaxies which are faint or even undetected at optical to near-infrared wa…
ALMA 26 arcmin survey of GOODS-S at one-millimeter (ASAGAO): millimeter properties of stellar mass selected galaxies
Y. Yamaguchi, K. Kohno, B. Hatsukade +19
We make use of the ASAGAO, deep 1.2 mm continuum observations of a 26 arcmin region in the GOODS-South field obtained with ALMA, to probe dust-enshrouded star formation in -…
Spatially Resolved Molecular Gas Properties of Host Galaxy of Type I Superluminous Supernova SN 2017egm
Bunyo Hatsukade, Kana Morokuma-Matsui, Masao Hayashi +6
We present the results of CO(1-0) observations of the host galaxy of a Type I superluminous supernova (SLSN-I), SN2017egm, one of the closest SLSNe-I at z = 0.03063, by using the A…
Wind- and Operation-Induced Vibration Measurements of the Main Reflector of the Nobeyama 45 m Radio Telescope
Ikumi Hashimoto, Masakatsu Chiba, Nozomi Okada +5
As deformations of the main reflector of a radio telescope directly affect the observations, the evaluation of the deformation is extremely important. Dynamic characteristics of th…
ALMA CO Observations of the Host Galaxies of Long-duration Gamma-ray Bursts. I: Molecular Gas Scaling Relations
Bunyo Hatsukade, Kouji Ohta, Tetsuya Hashimoto +4
We present the results of CO observations toward 14 host galaxies of long-duration gamma-ray bursts (GRBs) at z = 0.1-2.5 by using the Atacama Large Millimeter/submillimeter Array.…