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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 -…
A dominant population of optically invisible massive galaxies in the early Universe
T. Wang, C. Schreiber, C. Elbaz +9
Our current knowledge of cosmic star-formation history during the first two billion years (corresponding to redshift z >3) is mainly based on galaxies identified in rest-frame ultr…
ALMA twenty-six arcmin survey of GOODS-S at one-millimeter (ASAGAO): Near-infrared-dark faint ALMA sources
Yuki Yamaguchi, Kotaro Kohno, Bunyo Hatsukade +21
We report detections of two 1.2 mm continuum sources ( ~ 0.6 mJy) without any counterparts in the deep - and/or -band image (i.e., -band magnitude $\gtrs…
Detections of [OIII] 88 m in Two Quasars in the Reionization Epoch
Takuya Hashimoto, Akio K. Inoue, Yoichi Tamura +3
With the Atacama Large Millimeter/sub-millimeter Array (ALMA), we report detections of the far-infrared (FIR) [OIII] 88 m line and the underlying dust continuum in the two quasa…
Alma Twenty-six Arcmin^2 Survey Of Goods-s At One-millimeter (asagao): Source Catalog And Number Counts
Bunyo Hatsukade, Kotaro Kohno, Yuki Yamaguchi +29
We present the survey design, data reduction, construction of images, and source catalog of the Atacama Large Millimeter/submillimeter Array (ALMA) twenty-six arcmin^2 survey of GO…
Molecular gas reservoirs in cluster galaxies at z=1.46
Masao Hayashi, Ken-ichi Tadaki, Tadayuki Kodama +7
We present molecular gas reservoirs of eighteen galaxies associated with the XMMXCS J2215.9-1738 cluster at z=1.46. From Band 7 and Band 3 data of the Atacama Large Millimeter/subm…
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) III. Star formation properties of the host galaxies at studied with ALMA
Takuma Izumi, Masafusa Onoue, Hikari Shirakata +26
We present our ALMA Cycle 4 measurements of the [CII] emission line and the underlying far-infrared (FIR) continuum emission from four optically low-luminosity ($M_{\rm 1450} > -25…
ALMA 26 Arcmin Survey of GOODS-S at One-millimeter (ASAGAO): Average Morphology of High- Dusty Star-Forming Galaxies is an Exponential-Disk ()
Seiji Fujimoto, Masami Ouchi, Kotaro Kohno +24
We present morphological properties of dusty star-forming galaxies at z=1-3 determined with high-resolution (FWHM~0"19) Atacama Large Milllimeter/submilimeter Array (ALMA) 1-mm ban…
Blind millimeter line emitter search using ALMA data toward gravitational lensing clusters
Yuki Yamaguchi, Kotaro Kohno, Yoichi Tamura +10
We present the results of a blind millimeter line emitter search using ALMA Band 6 data with a single frequency tuning toward four gravitational lensing clusters (RXJ1347.5-1145, A…
Evolutionary phases of gas-rich galaxies in a galaxy cluster at z=1.46
Masao Hayashi, Tadayuki Kodama, Kotaro Kohno +7
We report a survey of molecular gas in galaxies in the XMMXCS J2215.9-1738 cluster at . We have detected emission lines from 17 galaxies within a radius of from t…
ALMA Deep Field in SSA22: Blindly Detected CO Emitters and [CII] Emitter Candidates
N. H. Hayatsu, Y. Matsuda, H. Umehata +21
We report the identification of four millimeter line emitting galaxies with the Atacama Large Milli/submillimeter Array (ALMA) in SSA22 Field (ADF22). We analyze the ALMA 1.1 mm su…
SXDF-ALMA 2-arcmin^2 Deep Survey: Stacking of Rest-Frame Near-Infrared Selected Objects
Wei-Hao Wang, Kotaro Kohno, Bunyo Hatsukade +24
We present stacking analyses on our ALMA deep 1.1 mm imaging in the SXDF using 1.6 μm and 3.6 μm selected galaxies in the CANDELS WFC3 catalog. We detect a stacked flux of ~0.03-0.…
SXDF-ALMA 2 Arcmin^2 Deep Survey: Resolving and Characterizing the Infrared Extragalactic Background Light Down to 0.5 mJy
Yuki Yamaguchi, Yoichi Tamura, Kotaro Kohno +22
We present a multi-wavelength analysis of five submillimeter sources (S_1.1mm = 0.54-2.02 mJy) that were detected during our 1.1-mm-deep continuum survey in the SXDF-UDS-CANDELS fi…
Detection of an oxygen emission line from a high redshift galaxy in the reionization epoch
Akio K. Inoue, Yoichi Tamura, Hiroshi Matsuo +14
The physical properties and elemental abundances of the interstellar medium in galaxies during cosmic reionization are important for understanding the role of galaxies in this proc…
SXDF-UDS-CANDELS-ALMA 1.5 arcmin deep survey
K. Kohno, Y. Yamaguchi, Y. Tamura +26
We have conducted 1.1 mm ALMA observations of a contiguous or 1.5 arcmin window in the SXDF-UDS-CANDELS. We achieved a 5 sensitivity of 0.28 mJy, providi…
ALMA Deep Field in SSA22: A concentration of dusty starbursts in a z=3.09 protocluster core
H. Umehata, Y. Tamura, K. Kohno +20
We report the results of mapping at 1.1~mm with the Atacama Large Millimeter/submillimeter Array (ALMA) toward the central region of the SS…
SXDF-ALMA 1.5 arcmin^2 deep survey. A compact dusty star-forming galaxy at z=2.5
Ken-ichi Tadaki, Kotaro Kohno, Tadayuki Kodama +23
We present first results from the SXDF-ALMA 1.5 arcmin^2 deep survey at 1.1 mm using Atacama Large Millimeter Array (ALMA). The map reaches a 1sigma depth of 55 uJy/beam and covers…
The ALMA Patchy Deep Survey: A blind search for [CII] emitters at z~4.5
Y. Matsuda, T. Nagao, D. Iono +5
We present a result of a blind search for [CII] 158 m emitters at using ALMA Cycle~0 archival data. We collected extra-galactic data covering at 330-360 GHz (band~7)…