activity
20172026
most citedKojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star

32 citations · 40 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2026

Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass

Masafumi Niwano, Nobuyuki Kawai, Michael Fausnaugh

The observational determination of the lower limit of neutron star masses is crucial for the physics of core-collapse supernovae. In this light, SMC X-1 is an important object beca…

astro-ph.HE20244 cited

Evolution of Accretion Disk Structure of the Black Hole X-ray Binary MAXI J1820070 during the Rebrightening Phase

Tomohiro Yoshitake, Megumi Shidatsu, Yoshihiro Ueda +18

To understand the evolution of global accretion disk structure in the ``rebrightening'' phase of MAXI J1820070, we perform a comprehensive analysis of its near infrared/optical/…

astro-ph.SR2024

Possible anti-correlations between pulsation amplitudes and the disk growth of Be stars in giant-outbursting Be X-ray binaries

Masafumi Niwano, Michael M. Fausnaugh, Ryan M. Lau +15

The mechanism of X-ray outbursts in Be X-ray binaries remains a mystery, and understanding their circumstellar disks is crucial for a solution of the mass-transfer problem. In part…

astro-ph.EP201932 cited

Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star

A. Fukui, D. Suzuki, N. Koshimoto +56

We report the analysis of additional multiband photometry and spectroscopy and new adaptive optics (AO) imaging of the nearby planetary microlensing event TCP J05074264+2447555 (Ko…

astro-ph.HE20174 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…