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20132017
most citedWhat is the physical origin of strong Lya emission? II. Gas Kinematics and Distribution of Lya Emitters

154 citations · 372 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2017★ 44 cited

The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at

Haruka Kusakabe, Kazuhiro Shimasaku, Masami Ouchi +7

We present average stellar population properties and dark matter halo masses of \lya emitters (LAEs) from SED fitting and clustering analysis, respectively, using $\sime…

astro-ph.GA2016★ 31 cited

Ly Emitters with Very Large Ly Equivalent Widths, EW(Ly) Å, at

Takuya Hashimoto, Masami Ouchi, Kazuhiro Shimasaku +6

We present physical properties of spectroscopically confirmed Ly emitters (LAEs) with very large rest-frame Ly equivalent widths EW(Ly). Although the definition…

astro-ph.GA2015★ 30 cited

Physical conditions of the interstellar medium in star-forming galaxies at z~1.5

Masao Hayashi, Chun Ly, Kazuhiro Shimasaku +6

We present results from Subaru/FMOS near-infrared (NIR) spectroscopy of 118 star-forming galaxies at in the Subaru Deep Field. These galaxies are selected as [OII]372…

astro-ph.GA2015★ 105 cited

A Close Comparison between Observed and Modeled Lyα Lines for z ~ 2.2 Lyman Alpha Emitters

Takuya Hashimoto, Anne Verhamme, Masami Ouchi +7

We present the results of a Lya profile analysis of 12 Lya emitters (LAEs) at z = 2.2 with high-resolution Lya spectra. We find that all 12 objects have a Lya profile with the main…

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…

astro-ph.CO2013★ 8 cited

The stellar mass function and efficiency of galaxy formation with a varying initial mass function

Sean L. McGee, Ryosuke Goto, Michael L. Balogh

Several recent observational studies have concluded that the initial mass function (IMF) of stars varies systematically with galaxy properties such as velocity dispersion. In this…