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marco.depetris@uniroma1.it
Marco De Petris
Professore Associato
Struttura:
DIPARTIMENTO DI FISICA
E-mail:
marco.depetris@uniroma1.it
Pagina istituzionale corsi di laurea
Curriculum Sapienza
Pubblicazioni
Titolo
Pubblicato in
Anno
Interpreting millimeter emission from IMEGIN galaxies NGC 2146 and NGC 2976
ASTRONOMY & ASTROPHYSICS
2025
Deep learning generated observations of galaxy clusters from dark-matter-only simulations
RAS TECHNIQUES AND INSTRUMENTS
2025
Euclid preparation: LXVI. Impact of line-of-sight projections on the covariance between galaxy cluster multi-wavelength observable properties: Insights from hydrodynamic simulations
ASTRONOMY & ASTROPHYSICS
2025
The impact of baryons on the sparsity of simulated galaxy clusters from THE THREE HUNDRED Project: Astrophysical and cosmological implications
ASTRONOMY & ASTROPHYSICS
2025
Exploiting high-resolution NIKA2 data to study the intracluster medium and dynamical state of ACT-CL J0240.0+0116
ASTRONOMY & ASTROPHYSICS
2025
Euclid I. Overview of the Euclid mission
ASTRONOMY & ASTROPHYSICS
2025
A panchromatic view of N2CLS GOODS-N: The evolution of the dust cosmic density since z ∼ 7
ASTRONOMY & ASTROPHYSICS
2025
Galaxy cluster mass bias from projected mass maps
ASTRONOMY & ASTROPHYSICS
2024
The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data
ASTRONOMY & ASTROPHYSICS
2024
The three hundred project: mapping the matter distribution in galaxy clusters via deep learning from multiview simulated observations
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2024
CHEX-MATE: Characterization of the intra-cluster medium temperature distribution
ASTRONOMY & ASTROPHYSICS
2024
Impact of filaments on galaxy cluster properties in The Three Hundred simulation
EPJ WEB OF CONFERENCES
2024
LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
2024
The MISTRAL instrument
Memorie della Società Astronomica Italiana
2024
The three hundred. Contrasting cluster galaxy density in hydrodynamical and dark matter simulations
ASTRONOMY & ASTROPHYSICS
2024
Identifying frequency de-correlated dust residuals in B-mode maps by exploiting the spectral capability of bolometric interferometry
ASTRONOMY & ASTROPHYSICS
2024
Observing galaxy clusters and the cosmic web through the Sunyaev Zel’dovich effect with MISTRAL
EPJ WEB OF CONFERENCES
2024
The advantage of Bolometric Interferometry for controlling Galactic foreground contamination in CMB primordial B-modes measurements
EPJ WEB OF CONFERENCES
2024
Measuring the CMB primordial B-modes with bolometric Interferometry. Status and future prospects of the QUBIC experiment
EPJ WEB OF CONFERENCES
2024
OLIMPO: A balloon-borne SZE imager to probe ICM dynamics and the WHIM
EPJ WEB OF CONFERENCES
2024
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ERC
PE9_9
PE9_13
PE9_17
Progetti di Ricerca
Investigating the mass of clusters of galaxies by optical, X-ray and millimetric observations supported by hydrodynamical simulations
Tracing Dark Matter distribution in the Universe by indirect observations and numerical simulations
Gruppi di ricerca
Cosmologia Osservativa
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