Maurizio Paolillo

Professore Ordinario

Università degli Studi di Napoli Federico II

Italy

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Maurizio Paolillo is a Professore Ordinario at Università degli Studi di Napoli Federico II, Italy. His research focuses on active galactic nuclei (AGN) variability, star formation rates, and astronomical imaging techniques. Recent publications include studies on the optical-UV and X-ray variability of AGN, as well as the tracing of globular cluster populations in galaxy groups. He employs advanced methods such as random forest algorithms and transfer learning to enhance the understanding of astronomical phenomena.

Maurizio Paolillo

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Articles (21)

ULISSE: Determination of the star formation rate and stellar mass based on the one-shot galaxy imaging technique

Continuum optical-UV and X-ray variability of AGN: current results and future challenges

Navigating AGN variability with self-organizing maps

Selection of optically variable active galactic nuclei via a random forest algorithm

Ensemble X-ray variability of optically selected QSOs: dependence on black hole mass and Eddington ratio

Identification of problematic epochs in astronomical time series through transfer learning

Ensemble power spectral density of SDSS quasars in UV/optical bands

Recovered supernova Ia rate from simulated LSST images

VEGAS-SSS: Tracing globular cluster populations in the interacting NGC 3640 galaxy group

Investigating the nuclear properties of highly accreting active galactic nuclei with XMM-Newton

X-Ray Unveiling Events in a z ≈ 1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South

The universal shape of the X-ray variability power spectrum of AGN up to z ∼ 3

Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies

ulisse: A tool for one-shot sky exploration and its application for detection of active galactic nuclei

Spatial Structures in the Globular Cluster Distribution of Fornax Cluster Galaxies

Blazar Variability with the Vera C. Rubin Legacy Survey of Space and Time

The connection between star formation and supermassive black hole activity in the local Universe

Exploratory X-Ray Monitoring of Luminous Radio-quiet Quasars at High Redshift: Extended Time-series Analyses and Stacked Imaging Spectroscopy

Exploring black hole scaling relations via the ensemble variability of active galactic nuclei

Photometric Redshifts in the W-CDF-S and ELAIS-S1 Fields Based on Forced Photometry from 0.36 to 4.5 Microns

MOCCA Survey Database: extra Galactic globular clusters. I. Method and first results

Collaborators (11)

Andreas Zezas

Francisco J. Carrera

Demetra De Cicco

Cristian Vignali

Giuseppina Fabbiano

Antonio La Marca

Mara Salvato

Iossif Papadakis

Massimo Villata

William Clarkson

James Aird

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