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20242026
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astro-ph.GA2026

Enhanced activity in close dual-AGN systems in the local Universe

Lorenzo Battistini, Alessandra De Rosa, Paola Severgnini +16

We present the study of an X-ray selected sample of active galactic nuclei (AGN) in pairs at projected spatial separations 1 </kpc < 100 at z < 0.1, using XMM-Newton and Chan…

astro-ph.GA2025

Variability in the supermassive black hole binary candidate SDSS J2320+0024: No evidence of periodic modulation

Fabio Rigamonti, Lorenzo Bertassi, Riccardo Buscicchio +5

Supermassive black hole binaries (SBHBs) are a natural outcome of galaxy mergers, and they are expected to be among the loudest gravitational-wave sources at low frequencies. The s…

astro-ph.GA2025

X-ray investigation of possible super-Eddington accretion in a radio-loud quasar at

L. Ighina, A. Caccianiga, T. Connor +19

We present radio and X-ray observations of the recently discovered radio-powerful quasar RACS J032021.44352104.1 using uGMRT, ATCA, LBA, and Chandra. The observed radio…

astro-ph.GA2025

ESPRESSO reveals a single but perturbed broad-line region in the supermassive black hole binary candidate PG 1302-102

Fabio Rigamonti, Paola Severgnini, Erika Sottocorno +12

We present a new, Bayesian analysis of the highest-resolution optical spectrum of the supermassive black hole (SMBH) binary candidate PG 1302-102, obtained with ESPRESSO@VLT (R \si…

astro-ph.GA2024

SDSS J222428.53+261423.2: unique emission lines properties unveil a sub-kiloparsec dual AGN candidate

Qi Zheng, XueGuang Zhang, QiRong Yuan +2

In this paper, we presented a detailed analysis of the Sloan Digital Sky Survey optical spectrum of a new sub-kpc scale dual AGN candidate SDSS J222428.53+261423.2 (=SDSS J2224). T…