activity
20122023
most citedLog-normal flux distribution of bright Fermi blazars

61 citations · 190 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2023

Understanding the Very High Energy γ-ray excess in nearby blazars using leptonic model

Aaqib Manzoor, Sunder Sahayanathan, Zahir Shah +3

The availability of simultaneous X-ray and Very High Energy (VHE) observations of blazars helps to identify the plausible radiative contributors to the VHE emission. Under leptonic…

astro-ph.HE2022★ 10 cited

Multi-wavelength study of blazar 4C +01.02 during its long-term flaring activity in 2014-2017

Malik Zahoor, Shah Zahir, Sunder Sahayanathan +2

We conducted a detailed long-term spectral and temporal study of flat spectrum radio quasar 4C +01.02, by using the multi-wavelength observations from Fermi-LAT, Swift-XRT, and Swi…

astro-ph.HE2022★ 4 cited

Very High Energy Flat Spectral Radio Quasar Candidates

Zahoor Malik, Sunder Sahayanathan, Zahir Shah +2

The attenuation of very high energy (VHE) photons by the extragalactic background light (EBL) prevents the observation of high redshift flat spectrum radio quasars (FSRQs). However…

gr-qc2022★ 1 cited

Statistical description of galaxy clusters in Finzi model of gravity

Abdul W. Khanday, Sudhaker Upadhyay, Naseer Iqbal +1

We exploit a new theory of gravity proposed by Finzi, which gives stronger interaction at large scales, to study the thermodynamic description of galaxy clusters. We employ a stati…

astro-ph.HE2021★ 9 cited

Model-independent Redshift Estimation of BL Lac Objects through VHE Observations

Malik Zahoor, Sunder Sahayanathan, Shah Zahir +3

The very high energy (VHE) gamma-ray spectral indices of blazars show strong correlation with the source redshift. Absence of any such correlation in low energy gamma rays and X-ra…

astro-ph.HE2021★ 13 cited

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.HE2019★ 31 cited

Study on Temporal and Spectral behavior of 3C 279 during 2018 January flare

Zahir Shah, V. Jithesh, S. Sahayanathan +2

We present a detailed temporal and spectral study of the blazar 3C\,279 using multi-wavelength observations from Swift-XRT, Swift-UVOT and Fermi-LAT during a flare in 2018 January.…

astro-ph.HE2018★ 61 cited

Log-normal flux distribution of bright Fermi blazars

Zahir Shah, N. Mankuzhiyil, A. Sinha +3

We present the results of the -ray flux distribution study on the brightest blazars which are observed by the \emph{Fermi}-LAT. We selected 50 brightest blazars based on the max…

astro-ph.HE2017★ 6 cited

Modeling the response of a standard accretion disc to stochastic viscous fluctuations

Naveel Ahmad, Ranjeev Misra, Naseer Iqbal +2

The observed variability of X-ray binaries over a wide range of time-scales can be understood in the framework of a stochastic propagation model, where viscous fluctuations at diff…

astro-ph.HE2017★ 36 cited

Clues on High Energy Emission Mechanism from Blazar 3C 454.3 during 2015 August Flare

Zahir Shah, S. Sahayanathan, Nijil Mankuzhiyil +3

We perform a detailed spectral study of a recent flaring activity from the Flat Spectrum Radio Quasar (FSRQ), 3C\,454.3, observed simultaneously in optical, UV, X-ray and -ray e…

astro-ph.HE2016★ 13 cited

A model for the energy-dependent time-lag and rms of the heartbeat oscillations in GRS 1915+105

Mubashir Hamid Mir, Ranjeev Misra, Mayukh Pahari +2

Energy dependent phase lags reveal crucial information about the causal relation between various spectral components and about the nature of the accretion geometry around the compa…

astro-ph.HE2015★ 2 cited

The Effect of X-ray Irradiation on the Time Dependent Behaviour of Accretion Disks with Stochastic Perturbations

Bari Maqbool, Ranjeev Misra, Naseer Iqbal +1

The UV emission from X-ray binaries, is more likely to be produced by reprocessing of X-rays by the outer regions of an accretion disk. The structure of the outer disk may be alter…

astro-ph.CO2013

The peculiar velocity and temperature profile of galaxy clusters

Tabasum Masood, Naseer Iqbal

Dynamical parameters like average velocity dispersion and temperature profile of galaxy clusters are determined using a quasi equilibrium thermodynamic theory. The calculated veloc…

astro-ph.CO2012★ 4 cited

Correlation functions for extended mass galaxy clusters

Naseer Iqbal, Naveel Ahmad, Mubashir Hamid +1

The phenomenon of clustering of galaxies on the basis of correlation functions in an expanding Universe is studied by using equation of state, taking gravitational interaction betw…