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Monitoring Observations of the Jupiter-Family Comet 17P/Holmes during 2014 Perihelion Passage
Yuna Grace Kwon, Masateru Ishiguro, Hidekazu Hanayama +15
We performed a monitoring observation of a Jupiter-Family comet, 17P/Holmes, during its 2014 perihelion passage to investigate its secular change in activity. The comet has drawn t…
The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at
Teppei Okumura, Chiaki Hikage, Tomonori Totani +22
We measure the redshift-space correlation function from a spectroscopic sample of 2783 emission line galaxies from the FastSound survey. The survey, which uses the Subaru Telescope…
The Subaru FMOS Galaxy Redshift Survey (FastSound). III. The mass-metallicity relation and the fundamental metallicity relation at
Kiyoto Yabe, Kouji Ohta, Masayuki Akiyama +13
We present the results from a large near-infrared spectroscopic survey with Subaru/FMOS (\textit{FastSound}) consisting of 4,000 galaxies at with significant H…
Optical-Infrared Properties of Faint 1.3 mm Sources Detected with ALMA
Bunyo Hatsukade, Kouji Ohta, Kiyoto Yabe +3
We report optical-infrared (IR) properties of faint 1.3 mm sources (S_1.3mm = 0.2-1.0 mJy) detected with the Atacama Large Millimeter/submillimeter Array (ALMA) in the Subaru/XMM-N…
The Subaru-XMM-Newton Deep Survey (SXDS) VIII.: Multi-wavelength Identification, Optical/NIR Spectroscopic Properties, and Photometric Redshifts of X-ray Sources
Masayuki Akiyama, Yoshihiro Ueda, Mike G. Watson +27
We report the multi-wavelength identification of the X-ray sources found in the Subaru-XMM-Newton Deep Survey (SXDS) using deep imaging data covering the wavelength range between t…
The Subaru FMOS Galaxy Redshift Survey (FastSound). II. The Emission Line Catalog and Properties of Emission Line Galaxies
Hiroyuki Okada, Tomonori Totani, Motonari Tonegawa +14
We present basic properties of 3,300 emission line galaxies detected by the FastSound survey, which are mostly H emitters at 1.2-1.5 in the total area of about 20…