670 citations · 1.8k across the 12 of their papers we have counts for
12 papers
Stellar Populations of Lyman-alpha Emitters at z=4.86: A Comparison to LBGs
Suraphong Yuma, Kouji Ohta, Kiyoto Yabe +5
(abridged) We present a study of stellar population of LAEs at z=4.86 in GOODS-N and its flanking field. With the publicly available IRAC data in GOODS-N and further IRAC observati…
Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models
Masami Ouchi, Kazuhiro Shimasaku, Hisanori Furusawa +12
We present Lya luminosity function (LF), clustering measurements, and Lya line profiles based on the largest sample, to date, of 207 Lya emitters (LAEs) at z=6.6 on the 1-deg^2 sky…
Stellar Populations of Lyman Alpha Emitters at z = 3 - 4 Based on Deep Large Area Surveys in the Subaru-SXDS/UKIDSS-UDS Field
Yoshiaki Ono, Masami Ouchi, Kazuhiro Shimasaku +7
We investigate the stellar populations of Lyman alpha emitters (LAEs) at z=3.1 and 3.7 in 0.65 deg^2 of the Subaru/XMM-Newton Deep Field, based on rest-frame UV-to-optical photomet…
Lyman Break Galaxies at z~1.8-2.8: GALEX/NUV Imaging of the Subaru Deep Field
Chun Ly, Matthew A. Malkan, Tommaso Treu +7
Abridged: A photometric sample of ~7100 V<25.3 Lyman break galaxies (LBGs) has been selected by combining Subaru/Suprime-Cam BVRci'z' data with deep GALEX/NUV imaging of the Subaru…
Photometric H alpha and [O II] Luminosity Function of SDF and SXDF Galaxies: Implications for Future Baryon Oscillation Surveys
Masanao Sumiyoshi, Tomonori Totani, Shunsuke Oshige +9
Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy…
Star Formation Rates and Metallicities of K-selected Star Forming Galaxies at z~2
Masao Hayashi, Kentaro Motohara, Kazuhiro Shimasaku +7
We present spectroscopy of 15 star-forming BzK galaxies (sBzKs) with K(AB)<23 in the Subaru Deep Field, for which Halpha and some other emission lines are detected in 0.9 to 2.3 mi…