activity
20022017
most citedGamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni

231 citations · 963 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2017★ 69 cited

The TOP-SCOPE survey of Planck Galactic Cold Clumps: Survey overview and results of an exemplar source, PGCC G26.53+0.17

Tie Liu, Kee-Tae Kim, Mika Juvela +11

The low dust temperatures (<14 K) of Planck Galactic Cold Clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. TOP-SCOPE i…

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.HE2010★ 231 cited

Gamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni

LAT Collaboration

Novae are thermonuclear explosions on a white dwarf surface fueled by mass accreted from a companion star. Current physical models posit that shocked expanding gas from the nova sh…

astro-ph.HE2009★ 44 cited

Spectropolarimetry of the Unique Type Ib Supernova 2005bf: Larger Asymmetry Revealed by Later-Phase Data

Masaomi Tanaka, Koji S. Kawabata, Keiichi Maeda +6

We present an optical spectropolarimetric observation of the unique Type Ib supernova (SN) 2005bf at 8 days after the second maximum. The data, combined with the polarization spect…

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-ph.SR2009★ 34 cited

The Extremely Luminous Supernova 2006gy at Late Phase: Detection of Optical Emission from Supernova

Koji S. Kawabata, Masaomi Tanaka, Keiichi Maeda +4

We performed optical spectroscopy and photometry of SN 2006gy at late time, ~400 days after the explosion, with the Subaru/FOCAS in a good seeing condition. We found that the SN fa…