collaborators

8 papers

astro-ph.GA2026

A new era for Dual AGN science with SHARP

P. Severgnini, C. Vignali, A. De Rosa +21

The search for and the characterization of ultra-compact dual active galactic nuclei (AGN) are among the hottest topics of current extragalactic astrophysics. These systems involve…

astro-ph.GA2026

Identification of periodicities with arbitrary shapes in AGN light curves

Lorenzo Bertassi, Maria Charisi, Riccardo Buscicchio +3

Massive black hole binaries are expected to be observable as periodic AGN in time-domain photometric surveys. Periodicities may originate from different physical processes, includi…

astro-ph.HE2026

Even a precessing clock is right twice per orbit -- The super-periods of eRO-QPE2 and challenges for quasi-periodic eruption orbital models

R. Arcodia, G. Miniutti, J. Chakraborty +25

We present OC (``observed minus calculated'') timing analysis of the quasi-periodic eruption (QPE) source eRO-QPE2 with a multi-mission X-ray campaign, which includes 32 observe…

astro-ph.HE2026

Searching for unresolved massive black hole pairs through AGN photometric variability

Lorenzo Bertassi, Maria Charisi, Fabio Rigamonti +2

Since their discovery, AGN light curves are known to be intrinsically variable. In the optical/UV band, this variability is consistent with correlated or red noise and is particula…

astro-ph.GA2025

Testing compact massive black hole binary candidates through multi-epoch spectroscopy

Lorenzo Bertassi, Erika Sottocorno, Fabio Rigamonti +4

Emission from two massive black holes (MBHs) bound in a close binary is expected to be modulated by different processes, such as the Doppler boost due to the orbital motion, accret…

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…