activity
20092026
most citedA Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch

533 citations · 6.6k across the 107 of their papers we have counts for

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Showing 2014Show all

6 papers · 1 filter

astro-ph.GA2014★ 23 cited

First Infrared-based implications for the dust attenuation and star formation of typical Ly emitters

Haruka Kusakabe, Kazuhiro Shimasaku, Kimihiko Nakajima +1

By stacking publicly available deep Spitzer/MIPS 24 m and Herschel/PACS images for 213 Ly Emitters (LAEs) in GOODS-South, we obtain a strong upper limit to th…

astro-ph.GA2014★ 11 cited

MOSFIRE and LDSS3 Spectroscopy for an [OII] Blob at z=1.18: Gas Outflow and Energy Source

Yuichi Harikane, Masami Ouchi, Suraphong Yuma +3

We report our Keck/MOSFIRE and Magellan/LDSS3 spectroscopy for an [OII] Blob, OIIB10, that is a high- galaxy with spatially extended [OII] emission over 30 kp…

astro-ph.CO2014★ 161 cited

Diffuse Lyman-alpha Halos around Galaxies at z=2.2-6.6: Implications for Galaxy Formation and Cosmic Reionization

Rieko Momose, Masami Ouchi, Kimihiko Nakajima +6

We present diffuse Lyman-alpha halos (LAHs) identified in the composite Subaru narrowband images of 100-3600 Lyman-alpha emitters (LAEs) at z=2.2, 3.1, 3.7, 5.7, and 6.6. First, we…

astro-ph.CO2014★ 171 cited

Accelerated Evolution of Ly Luminosity Function at Revealed by the Subaru Ultra-Deep Survey for Ly Emitters at

Akira Konno, Masami Ouchi, Yoshiaki Ono +8

We present the ultra-deep Subaru narrowband imaging survey for Lya emitters (LAEs) at in SXDS and COSMOS fields with a total integration time of 106 hours. Exploiting our n…

astro-ph.CO2014★ 57 cited

What is the Physical Origin of Strong Lya Emission? I. Demographics of Lya Emitter Structures

Takatoshi Shibuya, Masami Ouchi, Kimihiko Nakajima +5

We present the results of structure analyses for a large sample of 426 Lya emitters (LAEs) at z~2.2 that are observed with HST/ACS and WFC3-IR by deep extra-galactic legacy surveys…

astro-ph.CO2014★ 154 cited

What is the physical origin of strong Lya emission? II. Gas Kinematics and Distribution of Lya Emitters

Takatoshi Shibuya, Masami Ouchi, Kimihiko Nakajima +8

We present a statistical study of velocities of Lya, interstellar (IS) absorption, and nebular lines and gas covering fraction for Lya emitters (LAEs) at z~2. We make a sample of 2…