activity
20232026
collaborators

7 papers

astro-ph.SR2026

A systematic study of quiescent and outburst properties of X-ray-bright young stellar objects using XMM-Newton

Koki Sakuta, Ikuyuki Mitsuishi, Seiya Sasamata +6

Young Stellar Objects (YSOs) exhibit strong X-ray emission, widely attributed to magnetic reconnection and magnetospheric accretion; however, owing primarily to limited photon stat…

astro-ph.CO2026

XMM-Newton observations of ten high-redshift CAMIRA clusters of galaxies

Naomi Ota, Ikuyuki Mitsuishi, Nobuhiro Okabe +9

We present results from XMM-Newton observations of ten high-redshift () galaxy clusters selected from the CAMIRA catalog based on high richness (). These m…

astro-ph.IM2026

Development of Electroformed X-ray Optics Bridging Synchrotron Technology and Space Astronomy

Ryuto Fujii, Koki Sakuta, Kazuki Ampuku +21

We have developed X-ray telescope mirrors using an original electroforming replication technique established through the fabrication of millimeter-aperture, ultra-short-focal-lengt…

astro-ph.SR2025

X-ray emission of F-type stars and its analogy with G-type stars

Takuma Shimura, Ikuyuki Mitsuishi, Masanobu Kunitomo +3

We conducted a systematic spectral study for single F-type main-sequence (MS) stars without significant X-ray outbursts to investigate X-ray spectral properties such as temperature…

astro-ph.GA2024

AGN properties of ~1 million member galaxies of galaxy groups and clusters at z < 1.4 based on the Subaru Hyper Suprime-Cam survey

Yoshiki Toba, Aoi Hashiguchi, Naomi Ota +17

Herein, we present the statistical properties of active galactic nuclei (AGNs) for approximately 1 million member galaxies of galaxy groups and clusters, with 0.1 cluster redsh…

astro-ph.HE2023

Soft X-ray Energy Spectra in the Wide-Field Galactic Disk Area Revealed with HaloSat

Kazuki Ampuku, Ikuyuki Mitsuishi, Koki Sakuta +3

We analyzed data from HaloSat observations for five fields in the Galactic disk located far away from the Galactic center (135 254) to understand th…

astro-ph.GA2023

AGN number fraction in galaxy groups and clusters at z < 1.4 from the Subaru Hyper Suprime-Cam survey

Aoi Hashiguchi, Yoshiki Toba, Naomi Ota +20

One of the key questions on active galactic nuclei (AGN) in galaxy clusters is how AGN could affect the formation and evolution of member galaxies and galaxy clusters in the histor…