46 citations · 257 across the 16 of their papers we have counts for
15 papers · 1 filter
QUBIC IV: Performance of TES Bolometers and Readout Electronics
M. Piat, G. Stankowiak, E. S. Battistelli +126
A prototype version of the Q & U bolometric interferometer for cosmology (QUBIC) underwent a campaign of testing in the laboratory at Astroparticle Physics and Cosmology laboratory…
QUBIC I: Overview and ScienceProgram
J. -Ch. Hamilton, L. Mousset, E. S. Battistelli +127
The Q U Bolometric Interferometer for Cosmology (QUBIC) is a novel kind of polarimeter optimized for the measurement of the B-mode polarization of the Cosmic Microwave Backgro…
QUBIC II: Spectro-Polarimetry with Bolometric Interferometry
L. Mousset, M. M. Gamboa Lerena, E. S. Battistelli +128
Bolometric interferometry is a novel technique that has the ability to perform spectral imaging. A bolometric interferometer observes the sky in a wide frequency band and can recon…
QUBIC VII: The feedhorn-switch system of the technological demonstrator
F. Cavaliere, A. Mennella, M. Zannoni +128
We present the design, manufacturing and performance of the horn-switch system developed for the technological demonstrator of QUBIC (the \& Bolometric Interferometer for Cos…
QUBIC VI: cryogenic half wave plate rotator, design and performances
G. D'Alessandro, L. Mele, F. Columbro +126
Inflation Gravity Waves B-Modes polarization detection is the ultimate goal of modern large angular scale cosmic microwave background (CMB) experiments around the world. A big effo…
QUBIC V: Cryogenic system design and performance
S. Masi, E. S. Battistelli, P. de Bernardis +126
Current experiments aimed at measuring the polarization of the Cosmic Microwave Background (CMB) use cryogenic detector arrays and cold optical systems to boost the mapping speed o…
QUBIC VIII: Optical design and performance
C. O'Sullivan, M. De Petris, G. Amico +126
The Q and U Bolometric Interferometer for Cosmology (QUBIC) is a ground-based experiment that aims to detect B-mode polarisation anisotropies in the CMB at angular scales around th…
QUBIC III: Laboratory Characterization
S. A. Torchinsky, J. -Ch. Hamilton, M. Piat +125
A prototype version of the Q & U Bolometric Interferometer for Cosmology (QUBIC) underwent a campaign of testing in the laboratory at Astroparticle Physics and Cosmology in Paris.…
The long duration cryogenic system of the OLIMPO balloon--borne experiment: design and in--flight performance
A. Coppolecchia, L. Lamagna, S. Masi +18
We describe the design and in--flight performance of the cryostat and the self-contained He refrigerator for the OLIMPO balloon--borne experiment, a spectrophotometer to meas…
QUBIC: using NbSi TESs with a bolometric interferometer to characterize the polarisation of the CMB
M. Piat, B. Bélier, L. Bergé +135
QUBIC (Q \& U Bolometric Interferometer for Cosmology) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwav…
QUBIC: Exploring the primordial Universe with the Q\&U Bolometric Interferometer
Aniello Mennella, Peter Ade, Giorgio Amico +127
In this paper we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the art bolometric de…
Thermal architecture for the QUBIC cryogenic receiver
A. J. May, C. Chapron, G. Coppi +127
QUBIC, the QU Bolometric Interferometer for Cosmology, is a novel forthcoming instrument to measure the B-mode polarization anisotropy of the Cosmic Microwave Background. The detec…
SWIPE: a bolometric polarimeter for the Large-Scale Polarization Explorer
P. de Bernardis, S. Aiola, G. Amico +24
The balloon-borne LSPE mission is optimized to measure the linear polarization of the Cosmic Microwave Background at large angular scales. The Short Wavelength Instrument for the P…
The Large-Scale Polarization Explorer (LSPE)
The LSPE collaboration, S. Aiola, G. Amico +54
The LSPE is a balloon-borne mission aimed at measuring the polarization of the Cosmic Microwave Background (CMB) at large angular scales, and in particular to constrain the curl co…
Intensity and polarization of the atmospheric emission at millimetric wavelengths at Dome Concordia
E. S. Battistelli, G. Amico, A. Baù +32
Atmospheric emission is a dominant source of disturbance in ground-based astronomy at mm wavelengths. The Antarctic plateau is recognized to be an ideal site for mm and sub-mm obse…