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Masashi Chiba

Researcher at Tohoku University

Publications -  200
Citations -  11817

Masashi Chiba is an academic researcher from Tohoku University. The author has contributed to research in topics: Galaxy & Milky Way. The author has an hindex of 49, co-authored 192 publications receiving 10656 citations. Previous affiliations of Masashi Chiba include National Institutes of Natural Sciences, Japan & Graduate University for Advanced Studies.

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Journal ArticleDOI

Kinematics of Metal-poor Stars in the Galaxy. III. Formation of the Stellar Halo and Thick Disk as Revealed from a Large Sample of Nonkinematically Selected Stars

TL;DR: In this paper, a detailed analysis of the space motions of 1203 solar-neighborhood stars with metal abundances [Fe/H] ≤ -0.6 is presented.
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Two stellar components in the halo of the Milky Way

TL;DR: It is shown that the halo is indeed clearly divisible into two broadly overlapping structural components—an inner and an outer halo—that exhibit different spatial density profiles, stellar orbits and stellar metallicities (abundances of elements heavier than helium).
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Structure and Kinematics of the Stellar Halos and Thick Disks of the Milky Way Based on Calibration Stars from Sloan Digital Sky Survey DR7

TL;DR: In this article, the structure and kinematics of the recognized stellar components of the Milky Way are explored, based on well-determined atmospheric parameters and Kinematic quantities for 32360 "calibration stars" from the Sloan Digital Sky Survey (SDSS) and its first extension, which included the sub-survey Sloan Extension for Galactic Understanding and Exploration (SEGUE).
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The Hyper Suprime-Cam SSP Survey: Overview and Survey Design

Hiroaki Aihara, +141 more
TL;DR: Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2m Subaru telescope on the summit of Maunakea in Hawaii as mentioned in this paper.
Journal ArticleDOI

Structure and Kinematics of the Stellar Halos and Thick Disks of the Milky Way Based on Calibration Stars from SDSS DR7

TL;DR: In this article, the structure and kinematics of the recognized stellar components of the Milky Way are explored, based on well-determined atmospheric parameters and Kinematic quantities for 32360 calibration stars from the Sloan Digital Sky Survey (SDSS) and its first extension, which included the sub-survey SEGUE: Sloan Extension for Galactic Understanding and Exploration.