ISSI meeting Mar 2011.pptx - User Web Pages - Monash University

Result #4• Combined study of the bursting behaviour ofthe182newJ. Cheneveztransientet al.IGR J17473-2721IGR J17473–2721 outburst 2008 and burst timesRXTE #32Bolometric fluxRXTE/ASM (1.5–12 keV)Swift/BAT (15–50 keV)INTEGRAL/JEMXRXTE/PCAFlux (10 –9 erg/cm 2 /s)0 5 10 15JEMX #1SuperAGILESwiftRXTE #35RXTE #33+34RXTE #36RXTE #41RXTE #42500 550 600 650 700 750Time (MJD – 54000)Figure 1. Broad-band X-ray light curves for IGR J17473−2721 during the 2008 outburst, combining all available RXTE and Swift/BAT 1-day averaged data.Galloway, “The Multi-INstrument Burst ARchive – MINBAR”The bolometric fluxes are derived from RXTE/(PCA+HEXTE) fits (see the text) and have been connected for clarity. Every PCA observation is representedby a black dot. The observed X-ray bursts are represented by stars, with circles for the four PRE ones, and those indicated by names delineate the transitionsbetween different phases of burst behaviour (see Sections 3.3 and 4.1).