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20002023
most citedCIGALE: a python Code Investigating GALaxy Emission

1.3k citations · 10.1k across the 146 of their papers we have counts for

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Showing 2017 · astro-ph.GAShow all

5 papers · 2 filters

astro-ph.GA2017★ 126 cited

SILVERRUSH. V. Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC

Yuichi Harikane, Masami Ouchi, Takatoshi Shibuya +23

We investigate Lya, [OIII]5007, Ha, and [CII]158um emission from 1124 galaxies at z=4.9-7.0. Our sample is composed of 1092 Lya emitters (LAEs) at z=4.9, 5.7, 6.6, and 7.0 identifi…

astro-ph.GA2017★ 14 cited

The effect of radiation pressure on spatial distribution of dust inside HII regions

Shohei Ishiki, Takashi Okamoto, Akio K. Inoue

We investigate the impact of radiation pressure on spatial dust distribution inside H regions using one-dimensional radiation hydrodynamic simulations, which include…

astro-ph.GA2017

SILVERRUSH. IV. Ly Luminosity Functions at and Studied with 1,300 LAEs on the deg Sky

Akira Konno, Masami Ouchi, Takatoshi Shibuya +18

We present the Ly luminosity functions (LFs) at 5.7 and 6.6 derived from a new large sample of 1,266 Ly emitters (LAEs) identified in total areas of 14 and 21 deg, re…

astro-ph.GA2017★ 221 cited

Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program Strategy and Clustering Properties of ~2,000 Lya Emitters at z=6-7 over the 0.3-0.5 Gpc Survey Area

Masami Ouchi, Yuichi Harikane, Takatoshi Shibuya +17

We present the SILVERRUSH program strategy and clustering properties investigated with Ly emitters at and found in the early data of the Hyper Suprime…

astro-ph.GA2017★ 16 cited

Imaging of diffuse HI absorption structure in the SSA22 proto-cluster region at z = 3.1

Ken Mawatari, Akio K. Inoue, Toru Yamada +6

Using galaxies as background light sources to map intervening Lya absorption is a novel approach to study the interplay among galaxies, the circum-galactic medium (CGM), and the in…