activity
19952010
most citedLooking Into the Fireball: ROTSE-III and Swift Observations of Early GRB Afterglows

111 citations · 185 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2010★ 31 cited

GRB 081008: from burst to afterglow and the transition phase in between

F. Yuan, P. Schady, J. L. Racusin +30

We present a multi-wavelength study of GRB 081008, at redshift 1.967, by Swift, ROTSE-III and GROND. Compared to other Swift GRBs, GRB 081008 has a typical gamma-ray isotropic equi…

astro-ph.HE2009★ 111 cited

Looking Into the Fireball: ROTSE-III and Swift Observations of Early GRB Afterglows

E. S. Rykoff, F. Aharonian, C. W. Akerlof +21

We report on a complete set of early optical afterglows of gamma-ray bursts (GRBs) obtained with the ROTSE-III telescope network from March 2005 through June 2007. This set is comp…

astro-ph2005★ 22 cited

Optical Lightcurve & Cooling Break of GRB 050502A

S. A. Yost, K. Alatalo, E. S. Rykoff +29

We present lightcurves of the afterglow of GRB050502A, including very early data at t-t_{GRB} < 60s. The lightcurve is composed of unfiltered ROTSE-IIIb optical observations from 4…

astro-ph2005★ 10 cited

X-ray outburst of 4U 0115+634 and ROTSE Observations of its Optical Counterpart V635 Cas

A. Baykal, U. Kiziloglu, N. Kiziloglu +2

ROTSE IIId (The Robotic Optical Transient Experiment) observations of X-ray binary system 4U 0115+634/V635 Cas obtained during 2004 June and 2005 January make possible, for the fir…

astro-ph2000★ 11 cited

ROSAT Observations of the Vela Pulsar

F. D. Seward, M. A. Alpar, C. Flanagan +4

The ROSAT HRI was used to monitor X-ray emission from the Vela Pulsar. Six observations span 2-1/2 years and 3 glitches. The summed data yield a determination of the pulse shape, a…

astro-ph1995

X-ray variability and 1mHz oscillations in TT ARI

A. Bayka, A. Esendemir, U. Kiziloglu +4

Using the archival ROSAT observation of TT Ari, X-ray energy spectra in different orbital phases and power spectra of the intensity time series are presented. Spectral fits show th…