... Printed in U.S.A. A THE RADIO AFTERGLOW AND HOST GALAXY OF THE DARK GRB 020819 P. Jakobsson, 1, 2 D. A. Frail,3 D. B. Fox,4 D.-S. Moon,4, 5, 6 P. A. Price,7, 8 S. R. Kulkarni,4 J. P. U. Fynbo, J. Hjorth ... April 25 ed 1 ABSTRACT Of the 14 gamma-ray bursts (GRBs) localized to better than 20 radius with the SXC on HETE-2, only two lack optical ... 2003; Fynbo et al. 2003; Christensen et al. 2004). ... REFERENCES Andersen, M. I., Masi, G., Jensen, B. L., & Hjorth, J. 2003, GCN Circ. ...
... Reports on progress and error are always recorded in the log file of the program. ... UT date of the measurement finish in YYYY-MM-DD format UT time of the measurement finish in hh:mm:ss format Average flux in A aperture Average flux in B aperture Average flux in C aperture Average flux in D aperture Normalized variance of flux in A aperture Normalized variance of flux in B aperture Normalized variance of flux in C aperture Normalized variance of flux in D ...
... X-ray data of GX 3+1 (4U 1744-26) obtained in broad energy ranges using BeppoSAX (0.1200 keV) and Rossi X-Ray Timing Explorer (RXTE) (3200 keV) offer a unique The Astrophysical Journal, 747:99 (15pp), 2012 March 10 Seifina & Titarchuk possibility to further investigate, in detail, the evolution of X-ray spectral properties during transition events. ... In Figure 2, we illustrate our spectral model as a basic model for fitting the BeppoSAX and RXTE spectral data for GX 3+1. ... Figure 4. ...