activity
20242026
collaborators

20 papers

astro-ph.HE2026

Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars

P N Naseef Mohammed, Vaidehi S. Paliya, C D Ravikumar

The observation of broad emission lines in the optical spectra of flat-spectrum radio quasars (FSRQs) suggests radiatively efficient accretion powering these objects. In such broad…

astro-ph.HE2026

A Rare Gamma-ray Flaring episode of the Narrow-Line Seyfert 1 Galaxy 1H 0323+342

Aminabi Thekkoth, Vaidehi S. Paliya, Preeti Kharb

Gamma-ray-emitting narrow-line Seyfert 1 (-NLSy1) galaxies represent an enigmatic class of active galactic nuclei (AGNs) bridging populations of radio-quiet and radio-loud AGNs…

astro-ph.HE2026

The Emerging Population of High-energy Emitting Radio Galaxies

G. Bruni, V. S. Paliya, D. J. Saikia +22

High-energy emission from radio galaxies provides a unique laboratory to study the connection between accretion, jet formation, and particle acceleration in active galactic nuclei…

astro-ph.GA2026

The Quasar Main Sequence of Super-Eddington NLSy1 Galaxies

Alberto Domínguez, Alberto Domínguez, Suvendu Rakshit +3

The quasar main sequence, or Eigenvector 1 (EV1), describes the optical diversity of active galactic nuclei (AGN), with Narrow-Line Seyfert 1 (NLSy1) galaxies anchoring the high-ac…

astro-ph.GA2026

Narrow-Line Seyfert 1 Galaxies in the Dark Energy Spectroscopic Instrument Data Release 1

Vaidehi S. Paliya, Suvendu Rakshit, Alberto Dominguez +2

Narrow-line Seyfert 1 (NLSy1) galaxies are peculiar active galactic nuclei (AGN) known to exhibit a variety of intriguing observational features from low-frequency radio waves to h…

astro-ph.HE2026

A TeV-based Determination of the Local Extragalactic Background Light and its Consistency with Galaxy Counts and Direct Measurements

J. Baxter, A. Dominguez, J. D. Finke +5

The extragalactic background light (EBL), the cumulative radiation from all extragalactic sources, traces galaxy formation and cosmic evolution. High-energy rays attenuated vi…