activity
20172021
most citedClues on High Energy Emission Mechanism from Blazar 3C 454.3 during 2015 August Flare

36 citations · 98 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202115 cited

Understanding the X-ray spectral curvature of Mkn 421 using broadband AstroSat observations

Jyotishree Hota, Zahir Shah, Rukaiya Khatoon +3

We present a time-resolved X-ray spectral study of the high energy peaked blazar Mkn 421 using simultaneous broadband observations from the LAXPC and SXT instruments on-board Astro…

astro-ph.HE2021

The long-term X-ray flux distribution of Cygnus X-1 using RXTE-ASM and MAXI observations

Kabita Deka, Zahir Shah, Ranjeev Misra +1

We studied the long term flux distribution of Cygnus X-1 using RXTE-ASM lightcurves in two energy bands B (3-5 keV) & C (5-12.1 keV) as well as MAXI lightcurves in energy bands B (…

astro-ph.HE2021

AstroSat observation of the HBL 1ES 1959+650 during its October 2017 flaring

Zahir Shah, Savithri H. Ezhikode, Ranjeev Misra +1

We present the results of the X-ray flaring activity of 1ES 1959+650 during October 25-26, 2017 using AstroSat observations. The source was variable in the X-ray. We investigated t…

astro-ph.HE202113 cited

Correlation between optical and -ray flux variations in BL Lacs

Bhoomika Rajput, Zahir Shah, C. S. Stalin +2

We report here results on the analysis of correlated flux variations between the optical and GeV -ray bands in three bright BL Lac objects, namely AO\, 0235+164, OJ 287 and PKS…

astro-ph.HE2021

Unveiling the broadband spectral and temporal properties of PKS\,0903-57 during its brightest flare

Zahir Shah, V. Jithesh, S. Sahayanathan +1

We carried a detailed spectral and temporal study of blazar, \mbox{PKS\,0903-57} using the \emph{Fermi}-LAT and \emph{Swift}-XRT/UVOT observations, during its brightest flaring per…

astro-ph.HE202013 cited

On the determination of log-normal flux distributions for astrophysical systems

Zahir Shah, Ranjeev Misra, Atreyee Sinha

Determining whether the flux distribution of an Astrophysical source is a Gaussian or a log-normal, provides key insight into the nature of its variability. For lightcurves of mode…