activity
20072017
most citedGamma-Ray Bursts in Suggest that the Time Variation of the Dark Energy is Small

97 citations · 367 across the 14 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2013★ 15 cited

On the Subclasses in Swift Long Gamma-Ray Bursts: A Clue to Different Central Engines

Ryo Tsutsui, Toshikazu Shigeyama

Analyzing light curves of a complete sample of bright Swift long gamma-ray bursts (LGRBs) of which the peak photon fluxes constructed with the bin width of 1 second in the Swift 15…

astro-ph.HE2013★ 2 cited

Universal scaling law in long gamma-ray bursts

Ryo Tsutsui, Toshikazu Shigeyama

Overwhelming diversity of long gamma-ray bursts (LGRBs), discovered after the launch of {\it Swift} satellite, is a major obstacle to LGRB studies. Recently, it is shown that the p…

astro-ph.HE2012★ 67 cited

Possible existence of Ep-Lp and Ep-Eiso correlations for Short Gamma-Ray Bursts with a factor 5 to 100 dimmer than those for Long Gamma-Ray Bursts

Ryo Tsutsui, Daisuke Yonetoku Takashi Nakamura, Keitaro Takahashi +1

We analyzed correlations among the rest frame spectral peak energy , the observed frame 64ms peak isotropic luminosity and the isotropic energy …

astro-ph.HE2012★ 86 cited

Possible Origins of Dispersion of the Peak Energy--Brightness Correlations of Gamma-Ray Bursts

Daisuke Yonetoku, Toshio Murakami, Ryo Tsutsui +3

We collect and reanalyze about 200 GRB data of prompt-emission with known redshift observed until the end of 2009, and select 101 GRBs which were well observed to have good spectra…

astro-ph.HE2010★ 3 cited

Intrisic Dispersion of Correlations among Ep, Lp, and Eiso of Gamma Ray Bursts depends on the quality of Data Set

Ryo Tsutsui, Takashi Nakamura, Daisuke Yonetoku +2

We reconsider correlations among the spectral peak energy (), 1-second peak luminosity () and isotropic energy (\Eiso), using the database constructed by \citet{yonetoku1…

astro-ph.HE2010

Testing two-component jet models of GRBs with orphan afterglows

Kohei Inayoshi, Ryo Tsutsui

In the \swift era, two-component jet models were introduced to explain the complex temporal profiles and the diversity of early afterglows. In this paper, we concentrate on the two…