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19992026
most citedThe Hyper Suprime-Cam SSP Survey: Overview and Survey Design

1.1k citations · 16.4k across the 247 of their papers we have counts for

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Showing 2011Show all

8 papers · 1 filter

astro-ph.CO2011★ 96 cited

Stellar metallicity of star-forming galaxies at z ~ 3

Veronica Sommariva, Filippo Mannucci, Giovanni Cresci +5

The stellar metallicity is a direct measure of the amount of metals present in a galaxy, as a large part of the metals lie in its stars. In this paper we investigate new stellar me…

astro-ph.CO2011★ 17 cited

Keck Spectroscopy of Lyman-break Galaxies and its Implications for the UV-continuum and Ly_alpha Luminosity Functions at z>6

Linhua Jiang, Eiichi Egami, Nobunari Kashikawa +6

We present Keck spectroscopic observations of z>6 Lyman-break galaxy (LBG) candidates in the Subaru Deep Field (SDF). The candidates were selected as i'-dropout objects down to z'=…

astro-ph.CO2011★ 17 cited

Chemical properties in the most distant radio galaxy

Kenta Matsuoka, Tohru Nagao, Roberto Maiolino +2

We present a deep optical spectrum of TN J0924-2201, the most distant radio galaxy at z = 5.19, obtained with FOCAS on the Subaru Telescope. We successfully detect, for the first t…

astro-ph.CO2011★ 239 cited

Completing the Census of Ly-alpha Emitters at the Reionization Epoch

Nobunari Kashikawa, Kazuhiro Shimasaku, Yuichi Matsuda +16

We carried out extended spectroscopic confirmations of Ly-alpha emitters (LAEs) at z=6.5 and 5.7 in the Subaru Deep Field. Now, the total number of spectroscopically confirmed LAEs…

astro-ph.CO2011★ 65 cited

Enhanced [CII] emission in a z=4.76 submillimetre galaxy

Carlos De Breuck, Roberto Maiolino, Paola Caselli +3

We present the detection of bright [CII] emission in the z=4.76 submillimetre galaxy LESS J033229.4-275619 using the Atacama Pathfinder EXperiment. This represents the highest reds…

astro-ph.CO2011★ 47 cited

A Census of Star-Forming Galaxies at z = 1-3 in the Subaru Deep Field

Chun Ly, Matthew A. Malkan, Masao Hayashi +5

Several UV and near-infrared color selection methods have identified galaxies at z = 1-3. Since each method suffers from selection biases, we have applied three leading techniques…