activity
20022016
most citedThe Discovery of Two Lyman Emitters Beyond Redshift 6 in the Subaru Deep Field

192 citations · 447 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2016★ 70 cited

SXDF-ALMA 2 arcmin Deep Survey: 1.1-mm Number Counts

Bunyo Hatsukade, Kotaro Kohno, Hideki Umehata +18

We report 1.1 mm number counts revealed with the Atacama Large Millimeter/submillimeter Array (ALMA) in the Subaru/XMM-Newton Deep Survey Field (SXDF). The advent of ALMA enables u…

astro-ph.GA2015★ 1 cited

Rest-frame Optical Emission Lines in Far-Infrared Selected Galaxies at z<1.7 from the FMOS-COSMOS Survey

Jeyhan S. Kartaltepe, D. B. Sanders, J. D. Silverman +15

We have used FMOS on Subaru to obtain near-infrared spectroscopy of 123 far-infrared selected galaxies in COSMOS and obtain the key rest-frame optical emission lines. This is the l…

astro-ph2008★ 156 cited

Discovery of a Giant Lya Emitter Near the Reionization Epoch

Masami Ouchi, Yoshiaki Ono, Eiichi Egami +24

We report the discovery of a giant Lya emitter (LAE) with a Spitzer/IRAC counterpart near the reionization epoch at z=6.595. The giant LAE is found from the extensive 1 deg^2 Subar…

astro-ph2007★ 28 cited

Adaptive Optics Rest-Frame V-band Imaging of Lyman Break Galaxies at z~3: High-surface Density Disk-like Galaxies ?

M. Akiyama, Y. Minowa, N. Kobayashi +3

In order to reveal the rest-frame V-band morphology of galaxies at z~3, we conducted AO-assisted K-band imaging observations of z~3 LBGs with Mv*-0.5 to Mv*+3.0 mag. LBGs brighter…

astro-ph2003★ 192 cited

The Discovery of Two Lyman Emitters Beyond Redshift 6 in the Subaru Deep Field

K. Kodaira, Y. Taniguchi, N. Kashikawa +3

We have performed a deep optical imaging survey using a narrowband filter () centered at 9196 Å~ together with and broadband filters covering an 8…

astro-ph2002

AGN Populations from Optical Identification of ASCA Surveys

Masayuki Akiyama, Yoshihiro Ueda, Kouji Ohta

To understand luminous AGNs in the z<1 universe, the ASCA AGN samples are the best at present. Combining the identified sample of AGNs from ASCA Large Sky Survey and Medium Sensiti…