Combined Swift BAT-XRT Lightcurves
In this paper we make an attempt to combine the two kinds of data from the Swift-XRT instrument (windowedtiming and photon counting modes) and the from BAT. A thorough desription of the applied procedure will be given. Weapply various binning techniques to the different data: Bayes blocks, exponential binning and signal-to-noise type of binning.We present a handful of lightcurves and some possible applications.
γ-ray sources γ-ray bursts
P.Veres Z.Bagoly J.Kelemen I.Horvath L.G.Balazs A.Meszaros G.Tusnady
Dept.of Physics of Complex Systems,E(o)tv(o)s University,H-1117 Budapest,P(a)zm(a)ny P.s.l/A,Hungary Dept,of Physics of Complex Systems,E(o)tv(o)s University,H-1117 Budapest,P(a)zm(a)ny.s.l/A,ungary Konkoly Observatory,H-1525 Budapest,POB 67,Hungary Dept.of Physics,Bolyai Military University,H-1581 Budapest,POB 15,Hungary Astronomical Institute of the Charles University,V Hole(s)ovi?kach 2,CZ-180 00 Prague 8,Czech Republ Renyi Institute of Mathematics,Hungarian Academy of Sciences,H-1364 Budapest,POB 127,Hungary
国际会议
2008 NanJing Gamma-Ray Burst Conference(2008年伽马暴国际研讨会)
南京
英文
35-38
2008-06-23(万方平台首次上网日期,不代表论文的发表时间)