activity
20002023
most citedThe Hyper Suprime-Cam SSP Survey: Overview and Survey Design

1.1k citations · 1.6k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.HE2023★ 2 cited

Observing Cosmic-Ray Extensive Air Showers with a Silicon Imaging Detector

Satoshi Kawanomoto, Michitaro Koike, Fraser Bradfield +7

Extensive air showers induced from high-energy cosmic rays provide a window into understanding the most energetic phenomena in the universe. We present a new method for observing t…

astro-ph.GA2020★ 11 cited

Velocity Dispersions of Massive Quiescent Galaxies from Weak Lensing and Spectroscopy

Yousuke Utsumi, Margaret J. Geller, Harus J. Zahid +6

We use MMT spectroscopy and deep Subaru Hyper Suprime-Cam (HSC) imaging to compare the spectroscopic central stellar velocity dispersion of quiescent galaxies with the effective di…

astro-ph.GA2019★ 19 cited

CHORUS. III. Photometric and Spectroscopic Properties of Ly Blobs at

Haibin Zhang, Masami Ouchi, Ryohei Itoh +20

We report the Subaru Hyper Suprime-Cam (HSC) discovery of two Ly blobs (LABs), dubbed z70-1 and z49-1 at and respectively, that are Ly emitters with a bri…

astro-ph.SR2018★ 16 cited

Photospheric carbon, nitrogen, and oxygen abundances of A-type main-sequence stars

Yoichi Takeda, Satoshi Kawanomoto, Naoko Ohishi +4

Based on the spectrum fitting method applied to CI 5380, NI 7486, and OI 6156-8 lines, we determined the abundances of C, N, and O for 100 mostly A-type main-sequence stars (late B…

astro-ph.GA2018★ 60 cited

CHORUS II. Subaru/HSC Determination of the Ly Luminosity Function at : Constraints on Cosmic Reionization Model Parameter

Ryohei Itoh, Masami Ouchi, Haibin Zhang +16

We present the Ly luminosity function (LF) derived from 34 Ly emitters (LAEs) at on the sky of deg, the largest sample compared to those in the literature o…

astro-ph.SR2017★ 3 cited

Fourier analysis of He 4471/Mg 4481 line profiles for separating rotational velocity and axial inclination in rapidly-rotating B-type stars

Y. Takeda, S. Kawanomoto, N. Ohishi

While the effect of rotation on spectral lines is complicated in rapidly-rotating stars because of the appreciable gravity-darkening effect differing from line to line, it is possi…