AstroSat/LAXPC reveals the high energy variability of GRS 1915+105 in the chi class
J S Yadav, Ranjeev Misra, Jai Verdhan Chauhan, P C Agrawal, H M Antia,, Mayukh Pahari, Dhiraj Dedhia, Tilak Katoch, P. Madhwani, R K Manchanda, B, Paul, Parag Shah, C H Ishwara-Chandra

TL;DR
This study uses AstroSat's LAXPC instrument to analyze high energy variability in GRS 1915+105 during the chi class, revealing detailed spectral and timing features including QPOs and energy-dependent lags.
Contribution
First detailed high-energy variability analysis of GRS 1915+105 with AstroSat's LAXPC, demonstrating its capability for flux and spectro-timing studies.
Findings
Detection of a strong 2-8 Hz LFQPO and its harmonic.
Energy-dependent time-lags showing non-monotonic behavior.
High frequency power spectra match Poisson noise up to 50 kHz.
Abstract
We present the first quick look analysis of data from nine {\it AstroSat}'s LAXPC observations of GRS 1915+105 during March 2016 when the source had the characteristics of being in Radio-quiet class. We find that a simple empirical model of a disk blackbody emission, with Comptonization and a broad Gaussian Iron line can fit the time averaged 3--80 keV spectrum with a systematic uncertainty of 1.5\% and a background flux uncertainty of 4\%. A simple deadtime-corrected Poisson noise level spectrum matches well with the observed high frequency power spectra till 50 kHz and as expected the data show no significant high frequency ( Hz) features. Energy dependent power spectra reveal a strong low frequency (2 - 8 Hz) Quasi-periodic oscillation (LFQPO) and its harmonic along with broad band noise. The QPO frequency changes rapidly with flux (nearly 4 Hz in ~ 5 hours). With…
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