| Titolo |
Pubblicato in |
Anno |
| Interpreting millimeter emission from IMEGIN galaxies NGC 2146 and NGC 2976 |
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 |
| MISTRAL. Technical commissioning and first W-band photons from the Sardinia radio telescope |
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII |
2024 |
| The W-band LEKID array of the MISTRAL instrument |
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII |
2024 |
| Design and characterization of kinetic inductance detectors for the next-generation OLIMPO experiment |
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII |
2024 |
| Design and performance test of a modular readout electronic for the kinetic inductance detectors for the COSMO experiment based on commercial components |
|
2024 |
| The map-making and data filtering pipeline for the MISTRAL receiver |
|
2024 |
| CHEX-MATE: Turbulence in the intra-cluster medium from X-ray surface brightness fluctuations |
ASTRONOMY & ASTROPHYSICS |
2024 |
