activity
20242026
most citedApplication of the FRADO model of BLR formation to the Seyfert galaxy NGC 5548 and the first step toward determining the Hubble constant

6 citations · 9 across the 15 of their papers we have counts for

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astro-ph.HE2026

Multi-Band Optical Variability Characteristics of the -ray emitting blazar 1ES 0647+250 during its 2020 flare

K. Subbu Ulaganatha Pandian, C. S. Stalin, S. Muneer +4

We present a multi-band optical variability study of the -ray emitting high-synchrotron-peaked blazar 1ES~0647+250 during its enhanced optical activity in 2020. The analysis uti…

astro-ph.GA2026

Accretion-disk sizes in two quasars with interferometrically resolved broad-line regions at and

Francisco Pozo Nuñez, Eduardo Bañados, Swayamtrupta Panda +3

We present the first direct comparison between accretion-disk (AD) and broad-line region (BLR) sizes in quasars at z > 2, combining continuum reverberation mapping with interferome…

astro-ph.GA2026

HALO II: Constraining Hubble constant through continuum delay fitting of Fairall 9

Amit Kumar Mandal, Francisco Pozo Nuñez, Vikram Kumar Jaiswal +28

The Hubble tension remains one of the most significant unresolved problems in modern cosmology. A key question is whether it may arise from underestimated systematic uncertainties…

astro-ph.GA2026

Consistency between X-ray and UV-Optical reverberation measurements in NGC 5548

Amit Kumar Mandal, Bożena Czerny, Michal Dovčiak +2

The hard X-rayemitting hot corona is a key component of active galaxies. Constraints on the hot corona height can be derived from reverberation studies in both the X-ray and opt…

astro-ph.GA2026

Ultraviolet variability in Radio-Loud Active Galactic Nuclei observed by UVIT onboard AstroSat

M. Reshma, C. S. Stalin, Amit Kumar Mandal +3

Radio-loud active galactic nuclei (AGN) are among the most luminous objects in the Universe, emitting radiation from low-energy radio waves to high energy -rays. They are well k…