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20142026
most citedThe Hyper Suprime-Cam SSP Survey: Overview and Survey Design

1.1k citations · 8.7k across the 180 of their papers we have counts for

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Showing 2020Show all

11 papers · 1 filter

astro-ph.GA2020★ 8 cited

A puzzling non-detection of [O III] and [C II] from a galaxy observed with ALMA

C. Binggeli, A. K. Inoue, T. Hashimoto +12

Characterizing the galaxy population in the early Universe holds the key to understanding the evolution of these objects and the role they played in cosmic reionization. However, t…

astro-ph.GA2020★ 9 cited

Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ~ 4

Hisakazu Uchiyama, Masayuki Akiyama, Jun Toshikawa +16

Characterizing high-z quasar environments is key to understanding the co-evolution of quasars and the surrounding galaxies. To restrict their global picture, we statistically exami…

astro-ph.GA2020★ 19 cited

FIR-luminous [CII] emitters in the ALMA-SCUBA-2 COSMOS survey (AS2COSMOS): The nature of submillimeter galaxies in a 10 comoving Mpc-scale structure at z~4.6

Ikki Mitsuhashi, Yuichi Matsuda, Ian Smail +20

We report the discovery of a 10 comoving Mpc-scale structure traced by massive submillimeter galaxies (SMGs) at z~4.6. These galaxies are selected from an emission line search of A…

astro-ph.GA2020★ 18 cited

CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview

Akio K. Inoue, Satoshi Yamanaka, Masami Ouchi +28

To determine the dominant sources for cosmic reionization, the evolution history of the global ionizing fraction, and the topology of the ionized regions, we have conducted a deep…

astro-ph.GA2020★ 30 cited

Broad-band selection, spectroscopic identification, and physical properties of a population of extreme emission line galaxies at 3<z<3.7

Masato Onodera, Rhythm Shimakawa, Tomoko L. Suzuki +7

We present the selection, spectroscopic identification, and physical properties of extreme emission line galaxies (EELGs) at aiming at studying physical properties of an…

astro-ph.GA2020★ 73 cited

The Faint End of the Quasar Luminosity Function at from the Subaru Hyper Suprime-Cam Survey

Mana Niida, Tohru Nagao, Hiroyuki Ikeda +17

We present the quasar luminosity function at derived from the optical wide-field survey data obtained as a part of the Subaru strategic program (SSP) with Hyper Suprime-…

astro-ph.GA2020★ 17 cited

Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). III. Discovery of a z = 4.72 Radio Galaxy with Lyman Break Technique

Takuji Yamashita, Tohru Nagao, Hiroyuki Ikeda +17

We report a discovery of radio galaxy, HSC J083913.17+011308.1, by using the Lyman break technique with the Hyper Suprime-Cam Subaru Strategic Survey (HSC-SSP) catalog f…

astro-ph.GA2020★ 45 cited

EMPRESS. II. Highly Fe-Enriched Metal-poor Galaxies with (Fe/O) and (O/H) : Possible Traces of Super Massive () Stars in Early Galaxies

Takashi Kojima, Masami Ouchi, Michael Rauch +18

We present element abundance ratios and ionizing radiation of local young low-mass (~ M_sun) extremely metal poor galaxies (EMPGs) with a 2% solar oxygen abundance (O/H)_su…

astro-ph.GA2020★ 62 cited

The Mass-Metallicity Relation at z=8: Direct-Method Metallicity Constraints and Near-Future Prospects

Tucker Jones, Ryan Sanders, Guido Roberts-Borsani +4

Physical properties of galaxies at z>7 are of interest for understanding both the early phases of star formation and the process of cosmic reionization. Chemical abundance measurem…

astro-ph.GA2020★ 23 cited

The Mean Absorption Line Spectra of a Selection of Luminous z~6 Lyman Break Galaxies

Yuichi Harikane, Nicolas Laporte, Richard S. Ellis +1

We examine the absorption line spectra of a sample of 31 luminous (M_UV=-23) Lyman break galaxies at redshift z~6 using data taken with the FOCAS and OSIRIS spectrographs on the Su…

astro-ph.GA2020★ 20 cited

EMPRESS. III. Morphology, Stellar Population, and Dynamics of Extremely Metal Poor Galaxies (EMPGs): Are EMPGs Local Analogs of High- Young Galaxies?

Yuki Isobe, Masami Ouchi, Takashi Kojima +16

We present the morphology and stellar population of 27 extremely metal poor galaxies (EMPGs) at with metallicities of 0.01--0.1 Z. We conduct multi-component sur…