activity
19982026
most citedDiscovery of the black hole X-ray binary transient MAXIJ1348-630

48 citations · 66 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Vigorous turbulence driven by quasar-mode feedback in a cluster core

Satoshi Yamada, Shutaro Ueda, Hirofumi Noda +9

Quasars are among the most luminous objects. They are powered by accretion onto supermassive black holes. They are thought to impact cosmological evolution primarily through energe…

astro-ph.HE2025★ 12 cited

Delving into the depths of NGC 3783 with XRISM II. Cross-calibration of X-ray instruments used in the large, multi-mission observational campaign

XRISM collaboration

Accurate X-ray spectroscopic measurements are fundamental for deriving basic physical parameters of the most abundant baryon components in the Universe. The plethora of X-ray obser…

astro-ph.HE2020★ 48 cited

Discovery of the black hole X-ray binary transient MAXIJ1348-630

Mayu Tominaga, Satoshi Nakahira, Megumi Shidatsu +8

We report the first half-year monitoring of the new Galactic black hole candidate MAXI J1348-630, discovered on 2019 January 26 with the Gas Slit Camera (GSC) on-board MAXI. During…

astro-ph.HE2009

Anti-Correlation of the Near-Infrared and X-Ray Variations of the Microquasar GRS 1915+105 in Soft State

Akira Arai, Makoto Uemura, Mahito Sasada +21

We report detailed, long term near-infrared (NIR) light curves of GRS 1915+105 in 2007-2008, covering its long "soft state" for the first time. From our NIR monitoring and the X-ra…

astro-ph2002

AGN Populations from Optical Identification of ASCA Surveys

Masayuki Akiyama, Yoshihiro Ueda, Kouji Ohta

To understand luminous AGNs in the z<1 universe, the ASCA AGN samples are the best at present. Combining the identified sample of AGNs from ASCA Large Sky Survey and Medium Sensiti…

astro-ph1998★ 6 cited

The Cosmic X-ray Background spectrum observed with ROSAT and ASCA

T. Miyaji, Y. Ishisaki, Y. Ogasaka +4

We have made a series of joint spectral fits for two blank fields, the Lockman Hole and the Lynx-3A field, where a significant amount of both ASCA and ROSAT PSPC data exist after t…