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20012024
most citedGRB Formation Rates inferred from the Spectral Peak Energy - Luminosity Relation

720 citations · 5.2k across the 72 of their papers we have counts for

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astro-ph2008★ 36 cited

Cosmological Constraints from calibrated Yonetoku and Amati relation implies Fundamental plane of Gamma-ray bursts

Ryo Tsutsui, Takashi Nakamura, Daisuke Yonetoku +3

We consider two empirical relations using data only from the prompt emission of Gamma-Ray Bursts (GRBs), peak energy () - peak luminosity () relation (so called Yonetoku…

astro-ph2008★ 27 cited

Suzaku Observations of SGR 1900+14 and SGR 1806-20

Yujin E. Nakagawa, Tatehiro Mihara, Atsumasa Yoshida +8

Spectral and timing studies of Suzaku ToO observations of two SGRs, 1900+14 and 1806-20, are presented. The X-ray quiescent emission spectra were well fitted by a two blackbody fun…

astro-ph2008★ 36 cited

Constraints on and of Dark Energy from High Redshift Gamma Ray Bursts

Ryo Tsutsui, Takashi Nakamura, Daisuke Yonetoku +4

We extend the Hubble diagram up to using 63 gamma-ray bursts (GRBs) via peak energy-peak luminosity relation (so called Yonetoku relation), and obtain constraints on cosm…

astro-ph2008★ 97 cited

Gamma-Ray Bursts in Suggest that the Time Variation of the Dark Energy is Small

Yoshiki Kodama, Daisuke Yonetoku, Toshio Murakami +3

We calibrated the peak energy-peak luminosity relation of GRBs (so called Yonetoku relation) using 33 events with the redshift without assuming any cosmological models.…

astro-ph2007★ 47 cited

In Orbit Timing Calibration of the Hard X-Ray Detector on Board Suzaku

Yukikatsu Terada, Teruaki Enoto, Ryouhei Miyawaki +28

The hard X-ray detector (HXD) on board the X-ray satellite Suzaku is designed to have a good timing capability with a 61 s time resolution. In addition to detailed descriptions…

astro-ph2007★ 2 cited

Redshift Dependent Lag-Luminosity Relation in 565 BASTE Gamma Ray Bursts

Ryo Tsutsui, Takashi Nakamura, Daisuke Yonetoku +3

We compared redshifts from Yonetoku relation and from the lag-luminosity relation for 565 BASTE GRBs and were surprised to find that the correlation is very low. As…