425 citations
- National Astronomical Observatory of JapanJP60 papers
- The University of TokyoJP32 papers
- Kyoto UniversityJP25 papers
- The Graduate University for Advanced Studies, SOKENDAIJP25 papers
- Nagoya UniversityJP23 papers
- The University of OsakaJP22 papers
- Tohoku UniversityJP18 papers
- Kavli Institute for the Physics and Mathematics of the UniverseJP14 papers
- Centre National de la Recherche ScientifiqueFR13 papers
- Chiba UniversityJP13 papers
- Institute of Astronomy and Astrophysics, Academia SinicaTW13 papers
- Seoul National UniversityKR13 papers
5 papers · 2 filters
The Milky Way Tomography with Subaru Hyper Suprime-Cam. I. Halo substructures
Yoshihisa Suzuki, Masashi Chiba, Yutaka Komiyama +7
We analyze the photometric data in the Wide layer of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) over deg to uncover new halo substructures beyond t…
Ultra-Diffuse Galaxies (UDGs) with Hyper Suprime-Cam I: Revised Catalog of Coma Cluster UDGs
Jose Miguel Bautista, Jin Koda, Masafumi Yagi +2
This is the first in a series of papers on the properties of ultra-diffuse galaxies (UDGs) in clusters of galaxies. We present an updated catalog of UDGs in the Coma cluster using…
Triple spiral arms of a triple protostar system imaged in molecular lines
Jeong-Eun Lee, Tomoaki Matsumoto, Hyun-Jeong Kim +9
Most stars form in multiple star systems. For a better understanding of their formation processes, it is important to resolve the individual protostellar components and the surroun…
EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely-Metal Poor Galaxies
Yi Xu, Masami Ouchi, Yuki Isobe +49
We present demography of the dynamics and gas-mass fraction of 33 extremely metal-poor galaxies (EMPGs) with metallicities of and low stellar masses of $10^4-…
UV & Ly halos of Ly emitters across environments at z=2.84
Satoshi Kikuta, Yuichi Matsuda, Shigeki Inoue +7
We present UV and Ly radial surface brightness (SB) profiles of Ly emitters (LAEs) at detected with the Hyper Suprime-Cam (HSC) on the Subaru Telescope. The depth of…