collaborators

6 papers

astro-ph.HE2026

Zooming in on the GeV -ray flare of the blazar PKS 1725+123 with a multimessenger lens

Suvas Chandra Chaudhary, Saikat Das, Raj Prince +1

Blazars are promising sources of extragalactic high-energy astrophysical neutrinos, detected at energies TeV by the IceCube neutrino observatory. Here, we report the f…

astro-ph.HE2026

ZTF Monitoring of ray emitting Narrow Line Seyfert 1 Galaxies

Aman Kumar, Suvas Chandra Chaudhary, Raj Prince +2

The -ray-emitting narrow-line Seyfert-I (-NLSy1) are among the most interesting systems for studying disk-jet coupling. The soft X-ray properties of these systems suggest t…

astro-ph.HE2025

Unveiling the X-ray Secrets of Fermi-detected Narrow-Line Seyfert 1 Galaxies with XMM-Newton Observations

Suvas Chandra Chaudhary, Raj Prince, Brian van Soelen +1

In the innermost regions of active galactic nuclei, where the accretion disk, corona, and jet processes are closely coupled, X-ray observations offer a direct probe to study the ph…

astro-ph.HE2025

Exploring Hard X-ray Properties of -ray Emitting Narrow Line Seyfert-I Galaxies through NuSTAR Observations

Suvas Chandra Chaudhary, Raj Prince, Brian van Soelen +1

We studied the six gamma-ray-detected Narrow Line Seyfert 1 (NLSy1) galaxies using the hard X-ray observations from Nuclear Spectroscopic Telescope Array (NuSTAR) and optical g- \&…

astro-ph.HE2025

Deterministic and Stochastic Study of the X-ray Emission from the TeV Blazar Mrk~421

Radim Pánis, Gopal Bhatta, Tek P. Adhikari +6

We present a comprehensive timing analysis of X-ray data from the {\it XMM-Newton} satellite, examining 50 light curves covering 17 years of observations of the blazar Mrk~421. Thi…

astro-ph.HE2025

Probing X-ray Timing and Spectral Variability in the Blazar PKS 2155-304 Over a Decade of XMM-Newton Observations

Gopal Bhatta, Suvas C. Chaudhary, Niraj Dhital +5

Blazars, a class of active galactic nuclei (AGN) powered by supermassive black holes, are known for their remarkable variability across multiple timescales and wavelengths. Despite…