S. Masi

A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background \nRadiation

Clouds, filaments, and protostars: The<i>Herschel</i> Hi-GAL Milky Way

Hi-GAL: The Herschel Infrared Galactic Plane Survey

Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR Cosmic Microwave Background Observations

Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension

Cosmology intertwined III: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si4.svg"><mml:mrow><mml:mi>f</mml:mi><mml:msub><mml:mi>σ</mml:mi><mml:mn>8</mml:mn></mml:msub></mml:mrow></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.svg"><mml:msub><mml:mi>S</mml:mi><mml:mn>8</mml:mn></mml:msub></mml:math>

Cosmological parameters from the first results of Boomerang

Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology

A Measurement of the CMB 〈EE〉 Spectrum from the 2003 Flight of BOOMERANG

<i>Planck</i>pre-launch status: The HFI instrument, from specification to actual performance

A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG

PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper