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19942024
most citedThe Hyper Suprime-Cam SSP Survey: Overview and Survey Design

1.1k citations · 8.1k across the 100 of their papers we have counts for

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Showing 2005Show all

6 papers · 1 filter

astro-ph2005★ 10 cited

Direct Detection of Intermediate Mass Compact Objects via Submillilensing

Kaiki Taro Inoue, Masashi Chiba

A galaxy-sized halo may contain a large number of intermediate mass (10^{2-4} solar mass) compact objects (IMCOs), which can be intermediate mass black holes (IMBHs) or the CDM sub…

astro-ph2005★ 31 cited

Impact of dark matter subhalos on extended HI disks of galaxies: Possible formation of HI fine structures and stars

Kenji Bekki, Masashi Chiba

Recent observations have discovered star formation activities in the extreme outer regions of disk galaxies. However it remains unclear what physical mechanisms are responsible for…

astro-ph2005★ 4 cited

Dark and stellar matter in strong lensing galaxies from a joint lensing and stellar dynamics

Takashi Hamana, Youichi Ohyama, Masashi Chiba +1

We present Subaru spectroscopy of the early-type lensing galaxies in the lens systems HST14113+5211 (z=0.464) and B2045+265 (z=0.868), being aimed at measuring the velocity dispers…

astro-ph2005★ 20 cited

Fossil records of cosmic reionization in galactic stellar halos

Kenji Bekki, Masashi Chiba

Galactic stellar halos have long been considered to contain fossil information on early dynamical and chemical evolution of galaxies. We propose that the surface brightness distrib…

astro-ph2005★ 102 cited

Subaru Mid-infrared Imaging of the Quadruple Lenses PG1115+080 and B1422+231: Limits on Substructure Lensing

Masashi Chiba, Takeo Minezaki, Nobunari Kashikawa +2

We present mid-infrared imaging at 11.7 mu m for the quadruple lens systems, PG1115+080 and B1422+231, using the cooled mid-infrared camera and spectrometer (COMICS) attached on th…

astro-ph2005★ 31 cited

Three-dimensional Mapping of CDM Substructure at Submillimeter Wavelengths

Kaiki Taro Inoue, Masashi Chiba

The cold dark matter (CDM) structure formation model predicts that about 5-10 percent of a typical galactic halo of mass $\sim 10^{12} \ms$ is in substructures with masses $\lesssi…