activity
20222026
most citedUNIONS: The Ultraviolet Near-Infrared Optical Northern Survey

2 citations · 5 across the 15 of their papers we have counts for

collaborators
Showing 2024Show all

6 papers · 1 filter

astro-ph.GA2024

EMPRESS. X. Spatially resolved mass-metallicity relation in extremely metal-poor galaxies: evidence of episodic star-formation fueled by a metal-poor gas infall

Kimihiko Nakajima, Masami Ouchi, Yuki Isobe +47

Using the Subaru/FOCAS IFU capability, we examine the spatially resolved relationships between gas-phase metallicity, stellar mass, and star-formation rate surface densities (Sigma…

astro-ph.GA2024

Triangulum IV: A Possible Ultra-Diffuse Satellite of M33

Itsuki Ogami, Yutaka Komiyama, Masashi Chiba +8

We report the detection of a dwarf satellite candidate (Triangulum IV: Tri IV) of the Triangulum galaxy (M33) using the deep imaging of Subaru/Hyper Suprime-Cam (HSC). From the app…

astro-ph.GA2024

Chemo-dynamical Evolution of Simulated Satellites for a Milky Way-like Galaxy

Yutaka Hirai, Evan N. Kirby, Masashi Chiba +5

The chemical abundances of Milky Way's satellites reflect their star formation histories (SFHs), yet, due to the difficulty of determining the ages of old stars, the SFHs of most s…

astro-ph.GA2024

Disentangling gamma-beta: the 4th-order velocity moments based on spherical Jeans analysis

Dafa Wardana, Masashi Chiba, Kohei Hayashi

Distinguishing a core and a cusp within dark matter halos is complexified by the existence of mass-anisotropy degeneracy, where various combinations of velocity anisotropy () an…

astro-ph.GA2024

Detection of a Spatially Extended Stellar Population in M33: A Shallow Stellar Halo?

Itsuki Ogami, Yutaka Komiyama, Masashi Chiba +8

We analyze the outer regions of M33, beyond 15 kpc in projected distance from its center using Subaru/HSC multi-color imaging. We identify Red Giant Branch (RGB) stars and Red Clum…

astro-ph.GA2024

The structure of the stellar halo of the Andromeda galaxy explored with the NB515 for Subaru/HSC. I.: New Insights on the stellar halo up to 120 kpc

Itsuki Ogami, Mikito Tanaka, Yutaka Komiyama +16

We analyse the M31 halo and its substructure within a projected radius of 120 kpc using a combination of Subaru/HSC and CFHT/MegaCam - \& -…