activity
20152021
most citedThe RS CVn type star GT Mus shows most energetic X-ray flares throughout the 2010s

29 citations · 71 across the 9 of their papers we have counts for

collaborators

12 papers

astro-ph.HE20213 cited

Discovery of a strong 6.6 keV emission feature from EXO 1745248 after the superburst in 2011 October

Wataru B. Iwakiri, Motoko Serino, Tatehiro Mihara +4

We discover an unidentified strong emission feature in the X-ray spectrum of EXO 1745248 obtained by RXTE at 40 hr after the peak of a superburst. The structure was centered at…

gr-qc20215 cited

Gravitational Wave Physics and Astronomy in the nascent era

Makoto Arimoto, Hideki Asada, Michael L. Cherry +50

The detections of gravitational waves (GW) by LIGO/Virgo collaborations provide various possibilities to physics and astronomy. We are quite sure that GW observations will develop…

astro-ph.HE202129 cited

The RS CVn type star GT Mus shows most energetic X-ray flares throughout the 2010s

Ryo Sasaki, Yohko Tsuboi, Wataru Iwakiri +14

We report that the RS CVn-type star GT Mus (HR 4492, HD 101379 + HD 101380) was the most active star in the X-ray sky in the last decade in terms of the scale of recurrent energeti…

astro-ph.HE2019

Less noticeable shallow decay phase in early X-ray afterglows of GeV/TeV-detected gamma-ray bursts

Ryo Yamazaki, Yuri Sato, Takanori Sakamoto +1

The nature of the shallow decay phase in the X-ray afterglow of the gamma-ray burst (GRB) is not yet clarified. We analyze the data of early X-ray afterglows of 26 GRBs triggered b…

astro-ph.HE2018

The 7-year MAXI/GSC X-ray Source Catalog in the High Galactic-Latitude Sky (3MAXI)

Taiki Kawamuro, Yoshihiro Ueda, Megumi Shidatsu +28

We present the third MAXI/GSC catalog in the high Galactic-latitude sky () based on the 7-year data from 2009 August 13 to 2016 July 31, complementary to that in th…

astro-ph.HE2018

MAXI upper limits of the electromagnetic counterpart of GW170817

Satoshi Sugita, Nobuyuki Kawai, Satoshi Nakahira +5

We report the MAXI observation of the gravitational-wave (GW) event GW170817 and the electromagnetic counterpart of GW170817. GW170817 is a binary neutron star coalescence candidat…