activity
20022022
most citedFast transition of type-B QPO in the black hole transient XTE J1817-330

31 citations · 236 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.HE2022

Dependency of Optical/UV parameters on X-ray spectral index in AGNs

D. Nour, K. Sriram

The study of Active Galactic Nuclei (AGNs) is vital in order to understand their respective nuclei bounded activity primarily triggered by the accretion disk and the associated cor…

astro-ph.HE2022★ 2 cited

Association of Optical, Ultraviolet and Soft X-ray excess Emissions in AGNs

D. Nour, K. Sriram

Soft X-ray emission (0.5--2.0 keV) plays a pivotal role in regulating the optical and UV emission in the AGNs. We collected a sample of 1811 AGNs from the SDSS database and obtaine…

astro-ph.HE2022★ 14 cited

Constraining the Coronal Heights and Readjustment Velocities Based on the Detection of a Few Hundred Seconds Delays in the Z Source GX 17+2

K. Sriram, S. Malu, C. S. Choi

Neutron star Z type sources provide a unique platform in order to understand the structure of accretion disk-corona geometry emitting close to the Eddington luminosity. Using RXTE…

astro-ph.HE2022★ 6 cited

Anti-Correlated lags in a Neutron star Z source GX 5-1: AstroSat's View

Chiranjeevi Pallerla, K. Sriram

We report the cross-correlation function studies of a Neutron star low mass X-ray binary, a Z source GX 5-1 using SXT and LAXPC energy bands onboard AstroSat. For the first time, w…

astro-ph.HE2021★ 5 cited

Influence of Comptonization region over the ambiance of accretion disc in Active Galactic Nucleus

K. Sriram, D. Nour, C. S. Choi

Understanding the radiative and physical structures of inner region of a few 100 pc of AGNs is important to constrain the causes of their activities. Although the X-ray emission fr…

astro-ph.HE2021★ 4 cited

Investigating the coronal structure by studying time lags in the Atoll source 4U 1705-44 using AstroSat

S. Malu, S. Harikrishna, K. Sriram +1

We performed a detailed timing study of the Atoll source 4U 1705-44 in order to understand the accretion disk geometry. Cross correlation function (CCF) studies were performed betw…