activity
20222026
most citedConfirming new changing--look AGNs discovered through optical variability using a random-forest based light curve classifier

41 citations · 220 across the 18 of their papers we have counts for

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Showing 2023Show all

5 papers · 1 filter

astro-ph.HE2023★ 14 cited

BASS-XL: X-ray variability properties of unobscured Active Galactic Nuclei

Alessia Tortosa, Claudio Ricci, Patricia Arévalo +15

We investigate the X-ray variability properties of Seyfert1 Galaxies belonging to the BAT AGN Spectroscopic Survey (BASS). The sample includes 151 unobscured (N c…

astro-ph.GA2023★ 24 cited

Improving the selection of changing-look AGNs through multi-wavelength photometric variability

E. López-Navas, P. Sánchez-Sáez, P. Arévalo +13

We present second epoch optical spectra for 30 changing-look (CL) candidates found by searching for Type-1 optical variability in a sample of active galactic nuclei (AGNs) spectros…

astro-ph.IM2023★ 22 cited

Persistent and occasional: searching for the variable population of the ZTF/4MOST sky using ZTF data release 11

P. Sánchez-Sáez, J. Arredondo, A. Bayo +13

We present a variability, color and morphology based classifier, designed to identify transients, persistently variable, and non-variable sources, from the Zwicky Transient Facilit…

astro-ph.GA2023★ 1 cited

Optical variability in Quasars: Scaling with black hole mass and Eddington ratio depend on the observed timescales

Patricia Arévalo, Paulina Lira, Paula Sánchez-Sáez +4

Quasars emission is highly variable, and this variability gives us clues to understand the accretion process onto supermassive black holes. We can expect variability properties to…

astro-ph.HE2023★ 10 cited

Multiwavelength monitoring of the nucleus in PBC J2333.9-2343: the giant radio galaxy with a blazar-like core

L. Hernández-García, F. Panessa, G. Bruni +12

PBC J2333.9-2343 is a giant radio galaxy at z = 0.047 with a bright central core associated to a blazar nucleus. If the nuclear blazar jet is a new phase of the jet activity, then…