activity
20242026
most citedSpatially resolved broad line region in a quasar at z=4: Dynamical black hole mass and prominent outflow

10 citations · 10 across the 9 of their papers we have counts for

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12 papers · 1 filter

astro-ph.GA2026

OzSSy1: The Australian Southern Seyfert-1 Spectroscopic Atlas and Catalogue at z < 0.1

Neelesh Amrutha, Christian Wolf, Christopher A. Onken +3

We present a spectroscopic atlas of 887 broad-line active galactic nuclei (AGNs) in the Southern sky, spanning redshifts , declinations deg and Galactic latitudes…

astro-ph.GA2026

Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves

Ashley Hai Tung Tan, Christian Wolf, Neelesh Amrutha +3

The origin of the optical flux variability in active galactic nuclei (AGN) is largely unknown. Previous studies have correlated features of the variability structure function (SF)…

astro-ph.GA2026

Continuum Reverberation in Bright Quasars Using NASA/ATLAS

Zachary Steyn, Christian Wolf, Christopher Onken +5

Variable continuum emission from AGN can be used to probe the structure of their accretion disks via reverberation mapping. Assuming a variable, hot inner light source irradiates t…

astro-ph.GA2026

Cepheid-based Distances to NGC 4303 and NGC 1068

Madison Markham, Misty C. Bentz, Laura Ferrarese +2

We present Cepheid-based distances to two canonical AGN: NGC 4303 (M 61) and NGC 1068. Data were obtained using the Hubble Space Telescope with nonredundant time spacing over 12 vi…

astro-ph.GA2026

A catalogue of Type 2 active galactic nuclei in the 6dF Galaxy Survey

Sruthi Suresh, Wei Jeat Hon, Rachel L Webster +2

Active galactic nuclei (AGNs) are the compact, energetic central regions of galaxies, powered by supermassive black holes that accrete surrounding gas and dust. Their optical spect…

astro-ph.GA202510 cited

Spatially resolved broad line region in a quasar at z=4: Dynamical black hole mass and prominent outflow

GRAVITY+ Collaboration, K. Abd El Dayem, N. Aimar +92

We present the first near-infrared interferometric data of a QSO at z=4. The K-band observations were performed with GRAVITY+ on the VLTI using all four UTs, detecting a differenti…