activity
20102023
most citedQUBIC: The QU Bolometric Interferometer for Cosmology

66 citations · 283 across the 14 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

10 papers · 1 filter

astro-ph.IM2022★ 1 cited

High angular resolution Sunyaev Zel'dovich observations: the case of MISTRAL

E. S. Battistelli, E. Barbavara, P. de Bernardis +25

The MIllimeter Sardinia radio Telescope Receiver based on Array of Lumped elements kids, MISTRAL, is a millimetric () multipixel camera being built for the Sardinia R…

astro-ph.IM2021★ 6 cited

Total power horn-coupled 150 GHz LEKID array for space applications

A. Paiella, A. Coppolecchia, P. de Bernardis +17

We have developed two arrays of lumped element kinetic inductance detectors working in the D-band, and optimised for the low radiative background conditions of a satellite mission…

astro-ph.IM2020★ 6 cited

A chemically etched corrugated feedhorn array for D-band CMB observations

Stefano Mandelli, Elenia Manzan, Aniello Mennella +19

We present the design, manufacturing, and testing of a 37-element array of corrugated feedhorns for Cosmic Microwave Background (CMB) measurements between and GHz. The…

astro-ph.IM2020★ 10 cited

QUBIC: the Q & U Bolometric Interferometer for Cosmology

E. S. Battistelli, P. Ade, J. G. Alberro +136

The Q & U Bolometric Interferometer for Cosmology, QUBIC, is an innovative experiment designed to measure the polarization of the Cosmic Microwave Background and in particular the…

astro-ph.IM2016★ 25 cited

Multi-mode TES bolometer optimization for the LSPE-SWIPE instrument

R. Gualtieri, E. S. Battistelli, A. Cruciani +6

In this paper we explore the possibility of using transition edge sensor (TES) detectors in multi-mode configuration in the focal plane of the Short Wavelength Instrument for the P…

astro-ph.IM2016★ 24 cited

Development of Lumped Element Kinetic Inductance Detectors for the W-Band

A. Paiella, A. Coppolecchia, M. G. Castellano +6

We are developing a Lumped Element Kinetic Inductance Detector (LEKID) array able to operate in the W-band (75-110 GHz) in order to perform ground-based Cosmic Microwave Background…

astro-ph.IM2012★ 46 cited

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…

astro-ph.IM2012★ 12 cited

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…

astro-ph.IM2012★ 18 cited

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…

astro-ph.IM2010★ 66 cited

QUBIC: The QU Bolometric Interferometer for Cosmology

The QUBIC collaboration, E. Battistelli, A. Baù +57

One of the major challenges of modern cosmology is the detection of B-mode polarization anisotropies in the CMB. These originate from tensor fluctuations of the metric produced dur…