Speaker
Description
To understand the X-ray spectra of one of the superluminal X-ray binaries, we used RXTE/PCA and AstroSat/LAXPC data of GRS 1915+105.Where we can see significant photon counts variability in the X-ray light curves within 3.0–80.0 keV energy range.Out of 12 classes of X-ray variability, only few classes have significant higher and lower photons count.So We extract the higher(High flux) and lower(Low flux) photon counts from the light curves for different observations(For
Presentation Type | Poster |
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