activity
20132018
most citedGRB 130427A: a Nearby Ordinary Monster

134 citations · 314 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2018★ 15 cited

State Transitions of GRS 1739278 in the 2014 Outburst

Sili Wang, Nobuyuki Kawai, Megumi Shidatsu +4

We report on the X-ray spectral analysis and time evolution of GRS 1739278 during its 2014 outburst based on MAXI/GSC and Swift/XRT observations. Over the course of the outburst…

astro-ph.HE2018★ 5 cited

Late Engine Activity of GRB 161017A Revealed by Early Optical Observations

Yutaro Tachibana, Makoto Arimoto, Katsuaki Asano +8

The long gamma-ray burst GRB 161017A was detected by Fermi and Swift, and its afterglow was observed by the MITSuME 50-cm optical telescope promptly about 50 s after the burst. Ear…

astro-ph.HE2018★ 25 cited

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.HE2017★ 13 cited

Discovery of the new X-ray transient MAXI J1807+132: a Candidate of a Neutron Star Low-mass X-ray binary

Megumi Shidatsu, Yutaro Tachibana, Taketoshi Yoshii +9

We report on the detection and follow-up multi-wavelength observations of the new X-ray transient MAXI J1807+132 with the MAXI/GSC, Swift, and ground-based optical telescopes. The…

astro-ph.HE2017★ 4 cited

MITSuME observation of V404 Cygni in the 2015 outburst: Two optical variable components with different variability

Y. Tachibana, T. Yoshii, H. Hanayama +1

The black hole binary V404 Cygni (= GS 2023+338) had an outburst on June 15, 2015 after 26 years of quiescence. We report the multi-color optical observation (g', Rc, and Ic) of th…

astro-ph.HE2016★ 20 cited

No Evidence of Intrinsic Optical/Near-Infrared Linear Polarization for V404 Cygni During its Bright Outburst in 2015: Broadband Modeling and Constraint on Jet Parameters

Y. T. Tanaka, R. Itoh, M. Uemura +39

We present simultaneous optical and near-infrared (NIR) polarimetric results for the black hole binary V404 Cygni spanning the duration of its 7-day long optically-brightest phase…

astro-ph.HE2015★ 4 cited

A Soft X-Ray Lag Detected in Centaurus A

Yutaro Tachibana, Taiki Kawamuro, Yoshihiro Ueda +7

We performed time lag analysis on the X-ray light curves of Centaurus A (Cen A) obtained by the Gas Slit Camera (GSC) aboard the Monitor of All-sky X-ray Image ({\it MAXI}) in thre…

astro-ph.HE2015★ 10 cited

Multi-wavelength observations of the black widow pulsar 2FGL J2339.6-0532 with OISTER and Suzaku

Yoichi Yatsu, Jun Kataoka, Yosuke Takahashi +41

Multi-wavelength observations of the black-widow binary system 2FGL J2339.6-0532 are reported. The Fermi gamma-ray source 2FGL J2339.6-0532 was recently categorized as a black wido…

astro-ph.GA2014★ 17 cited

Discovery of Dramatic Optical Variability in SDSS J1100+4421: A Peculiar Radio-Loud Narrow-Line Seyfert 1 Galaxy?

Masaomi Tanaka, Tomoki Morokuma, Ryosuke Itoh +55

We present our discovery of dramatic variability in SDSS J1100+4421 by the high-cadence transient survey Kiso Supernova Survey (KISS). The source brightened in the optical by at le…

astro-ph.SR2014★ 42 cited

Kiso Supernova Survey (KISS): Survey Strategy

Tomoki Morokuma, Nozomu Tominaga, Masaomi Tanaka +58

The Kiso Supernova Survey (KISS) is a high-cadence optical wide-field supernova (SN) survey. The primary goal of the survey is to catch the very early light of a SN, during the sho…

astro-ph.HE2014★ 25 cited

MAXI observations of GRBs

Motoko Serino, Takanori Sakamoto, Nobuyuki Kawai +40

Monitor of all-sky image (MAXI) Gas Slit Camera (GSC) detects gamma-ray bursts (GRBs) including the bursts with soft spectra, such as X-ray flashes (XRFs). MAXI/GSC is sensitive to…

astro-ph.HE2013★ 134 cited

GRB 130427A: a Nearby Ordinary Monster

A. Maselli, A. Melandri, L. Nava +63

Long-duration Gamma-Ray Bursts (GRBs) are an extremely rare outcome of the collapse of massive stars, and are typically found in the distant Universe. Because of its intrinsic lumi…