66 citations · 283 across the 14 of their papers we have counts for
14 papers
Observing galaxy clusters and the cosmic web through the Sunyaev Zel'dovich effect with MISTRAL
E. S. Battistelli, E. Barbavara, P. de Bernardis +33
Galaxy clusters and surrounding medium, can be studied using X-ray bremsstrahlung emission and Sunyaev Zel'dovich (SZ) effect. Both astrophysical probes, sample the same environmen…
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…
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…
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…
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…
Strong evidence of Anomalous Microwave Emission from the flux density spectrum of M31
E. S. Battistelli, S. Fatigoni, M. Murgia +21
We have observed the Andromeda galaxy, Messier 31 (M31), at 6.7GHz with the Sardinia Radio Telescope. We mapped the radio emission in the C-band, re-analyzed WMAP and Planck maps,…
Detailed study of the microwave emission of the supernova remnant 3C 396
A. Cruciani, E. S. Battistelli, E. Carretti +8
We have observed the supernova remnant 3C~396 in the microwave region using the Parkes 64-m telescope. Observations have been made at 8.4 GHz, 13.5 GHz, and 18.6 GHz and in polaris…
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…
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…
New radio observations of anomalous microwave emission in the HII region RCW175
E. S. Battistelli, E. Carretti, A. Cruciani +9
We have observed the HII region RCW175 with the 64m Parkes telescope at 8.4GHz and 13.5GHz in total intensity, and at 21.5GHz in both total intensity and polarization. High angular…
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…
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…