collaborators

6 papers

astro-ph.GA2026

Feature-driven anomaly flagging in obscured active galactic nucleus light curves with autoencoders

Natale De Bonis, Demetra De Cicco, Stefano Cavuoti +5

Active galactic nuclei (AGN) are among the most complex classes of astrophysical objects, displaying a wide range of variability and observational properties. Identifying unusual A…

astro-ph.CO2026

A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation

Giuseppe Sarracino, Vincenzo Fabrizio Cardone, Roberto Scaramella +14

An Amplitude-Encoded Quantum Genetic Algorithm (AEQGA) has been developed to minimize functions of different cosmological probes (Supernovae Type Ia, Baryon Acoustic Oscilla…

astro-ph.IM2025

Euclid preparation: The NISP spectroscopy channel, on ground performance and calibration

Euclid Collaboration, W. Gillard, T. Maciaszek +356

ESA's Euclid cosmology mission relies on the very sensitive and accurately calibrated spectroscopy channel of the Near-Infrared Spectrometer and Photometer (NISP). With three opera…

astro-ph.CO2025

Quantum Markov Chain Monte Carlo for Cosmological Functions

Giuseppe Sarracino, Vincenzo Fabrizio Cardone, Roberto Scaramella +14

We present an implementation of Quantum Computing for a Markov Chain Monte Carlo method with an application to cosmological functions, to derive posterior distributions from cosmol…

astro-ph.IM2025

Navigating AGN variability with self-organizing maps

Ylenia Maruccia, Demetra De Cicco, Stefano Cavuoti +6

Context. The classification of active galactic nuclei (AGNs) is a challenge in astrophysics. Variability features extracted from light curves offer a promising avenue for distingui…

astro-ph.GA2025

The Evolutionary Path of Star-Forming Clumps in Hi-GAL

Ylenia Maruccia, Stefano Cavuoti, Massimo Brescia +4

Star formation (SF) studies are benefiting from the huge amount of data made available by recent large-area Galactic plane surveys conducted between 2 μm and 3 mm. Fully character…