most citedGalactic Archaeology with the Subaru `Ōnohi`ula Prime Focus Spectrograph Strategic Program

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11 papers

astro-ph.GA20261 cited

Galactic Archaeology with the Subaru `Ōnohi`ula Prime Focus Spectrograph Strategic Program

Masashi Chiba, Rosemary F. G. Wyse, Evan N. Kirby +47

The recently commissioned Subaru `Ōnohi`ula Prime Focus Spectrograph (PFS) will obtain spectra from nearly 2,400 fibers that cover 1.24 square degrees. The 360 night Subaru Strate…

astro-ph.GA2026

A Long Stellar Stream in M83: Possible Connection Between XUV Disks and Minor Mergers?

Itsuki Ogami, Sakurako Okamoto, Annette M. N. Ferguson +5

We present the confirmation and characterization of a long stream (S-stream) in the southern part of M83. This feature is revealed using deep wide-field photometric data obtained b…

astro-ph.GA2026

Subaru/HSC NB395 view of NGC 5466: metallicity, mass function, and the nature of its tidal stream

Itsuki Ogami, Miho N. Ishigaki, Pete B. Kuzma +6

We present a deep photometric study of the globular cluster NGC 5466 and its tidal stream using Subaru/Hyper Suprime-Cam (HSC) imaging with the metallicity-sensitive narrowband fil…

astro-ph.GA2025

Machine Learning Techniques to Distinguish Giant Stars from Dwarf Stars Using Only Photometry -- Pushing Redwards

Keyi Ding, Carrie Filion, Rosemary F. G. Wyse +6

We present our photometric method, which combines Subaru/HSC , g, and i band filters to distinguish giant stars in Local Group galaxies from Milky Way dwarf contamination. T…

astro-ph.GA2025

The Extended Stellar Distribution in the Outskirts of the Ursa Minor Dwarf Spheroidal Galaxy

Kyosuke S. Sato, Sakurako Okamoto, Masafumi Yagi +7

We discover an extended distribution of main-sequence (MS) stars along the minor axis of the Ursa Minor (UMi) dwarf spheroidal galaxy (dSph). This study is enabled by deep, wide Su…

astro-ph.GA2025

The Star Formation and Chemical Evolution Histories of Ursa Minor Dwarf Spheroidal Galaxy

Kyosuke S. Sato, Yutaka Komiyama, Sakurako Okamoto +8

We derive the star formation history (SFH) and chemical evolution history (CEH) of the Ursa Minor (UMi) dwarf spheroidal galaxy (dSph). We detect two distinct stellar populations t…