activity
20132026
most citedGamma-ray Flux Distribution and Non-linear behavior of Four LAT Bright AGNs

53 citations · 902 across the 48 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.HE2025★ 3 cited

Multiband optical variability on diverse timescales of the blazar Ton 599 from 2011 to 2023

O. Vince, C. M. Raiteri, M. Villata +72

(Shortened)Context: We analyze the optical variability of the FSRQ Ton 599 using BVRI photometry from the WEBT collaboration (2011-2023), complemented by photometric and spectrosco…

astro-ph.HE2025

VHE FSRQs with Fermi-LAT: VHE and even brighter states in high-z FSRQs due to an HBL-like component?

Megha, Pankaj Kushwaha

Very high-energy (VHE) detected flat-spectrum radio quasars (FSRQs) are relatively few despite being the most persistent bright MeV-GeV sources. Focusing on VHE emission, we invest…

astro-ph.HE2025

Curious Case of CGRaBS J0211+1051: Observational Evidence of Lepto-Hadronic Origin of High-Energy Emission?

Sunil Chandra, Pankaj Kushwaha, Pranjupriya Goswami +1

We present an extensive analysis of the multi-wavelength data of the low-synchrotron-peaked BL Lac object CGRaBS J0211+1051, which has been gathered over more than ten years with m…

astro-ph.HE2025

Broad-band temporal and spectral study of TeV blazar TXS 0518+211

Avik Kumar Das, Pankaj Kushwaha, Veeresh Singh +3

We present a long-term broad-band temporal and spectral study of a TeV BL Lac source TXS 0518+211 by analyzing nearly 16 years (MJD 54682 -- 60670) of simultaneous optical, UV and…

astro-ph.HE2025

X-ray variability of VHE detected FSRQs: A comparative study

Lekshmi Dathan, Pankaj Kushwaha

Flat Spectrum Radio Quasars (FSRQs) are weak sources of very high energy (VHE; E>100 GeV) emission, despite exhibiting strong MeV-GeV emissions that dominate their radiative output…

astro-ph.HE2025

Signature of Seyfert-like component in a blazar 3C 273 and its reflection-based explanation

Haritma Gaur, Main Pal, Muhammad S. Anjum +4

We present the results of blazar 3C 273 obtained from simultaneous observations obtained using XMM-Newton and NuSTAR satellites during the period 2015-2019 in five epochs. When the…