activity
20172021
most citedStrong Soft X-ray Excess in 2015 XMM-Newton Observation of BL--Lac OJ~287

27 citations · 82 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.HE202115 cited

Spectral States of OJ 287 blazar from Multi-wavelength Observations with

K. P. Singh, P. Kushwaha, A. Sinha +3

We present {\it AstroSat} soft X-ray, near-UV (NUV), and far-UV (FUV) observations of a blazar, OJ~287, carried out in 2017, 2018, and 2020. The simultaneous observations with NuST…

astro-ph.HE2021

Spectro-Timing Analysis of a highly variable narrow-line Seyfert 1 galaxy NGC 4748 with AstroSat and XMM-Newton

Main Pal, Neeraj Kumari, Pankaj Kushwaha +8

We present a detailed timing and spectral study of an extremely variable narrow-line Seyfert~1 galaxy NGC 4748 using observations in the year 2017 and 2014 performed with AstroSat…

astro-ph.HE2020

Blazar OJ 287 After First VHE Activity: Tracking the Re-emergence of the HBL like Component in 2020

Pankaj Kushwaha, Main Pal, Nibedita Kalita +5

We report the re-emergence of a new broadband emission through a detailed and systematic study of the multi-wavelength spectral and temporal behavior of OJ 287 after its first-ever…

astro-ph.HE20209 cited

Short-term X-ray Variability during Different Activity Phases of Blazars S5 0716+714 and PKS 2155-304

Pankaj Kushwaha, Main Pal

We explored the statistical properties of short-term X-ray variability using long-exposure {\it XMM-Newton} data during high X-ray variability phases of blazars S5 0716+714 and PKS…

astro-ph.HE201927 cited

Strong Soft X-ray Excess in 2015 XMM-Newton Observation of BL--Lac OJ~287

Main Pal, Pankaj Kushwaha, Gulab C. Dewangan +1

We report a strong soft X-ray excess in the BL--Lacartae -ray blazar OJ~287 during the long exposure in May 2015, amongst two of the latest \xmm~{} observations performed in May…

astro-ph.HE201812 cited

UV to X-ray Comptonization delay in Mrk 493

Oluwashina Adegoke, Gulab C. Dewangan, Pramod Pawar +1

The broadband X-ray emission from type 1 active galactic nuclei, dominated by a powerlaw continuum, is thought to arise from repeated inverse Compton scattering of seed optical/UV…