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Millimetric observation of the SZ effect in the Corona Borealis supercluster
E. S. Battistelli, M. De Petris, L. Lamagna +13
We have observed the Corona Borealis Supercluster with the Millimeter and Infrared Testa grigia Observatory (MITO), located in the Italian Alps, at 143, 214, 272, and 353 GHz. We p…
Absolute calibration and beam reconstruction of MITO (a ground-based instrument in the millimetric region)
G. Savini, A. Orlando, E. S. Battistelli +4
An efficient sky data reconstruction derives from a precise characterization of the observing instrument. Here we describe the reconstruction of performances of a single-pixel 4-ba…
Triple Experiment Spectrum of the Sunyaev-Zeldovich Effect in the Coma Cluster: H_0
E. S. Battistelli, M. De Petris, L. Lamagna +11
The Sunyaev-Zeldovich (SZ) effect was previously measured in the Coma cluster by the Owens Valley Radio Observatory and Millimeter and IR Testa Grigia Observatory experiments and r…
Far infrared polarimeter with very low instrumental polarization
E. S. Battistelli, M. De Petris, L. Lamagna +6
After a short analysis of the main problems involved in the construction of a Far Infrared polarimeter with very low instrumental noise, we describe the instrument that will be emp…
Cosmic Microwave Background Temperature at Galaxy Clusters
E. S. Battistelli, M. De Petris, L. Lamagna +7
We have deduced the cosmic microwave background (CMB) temperature in the Coma cluster (A1656, ), and in A2163 () from spectral measurements of the Sunyaev-Zel'do…
MITO measurements of the Sunyaev-Zeldovich Effect in the Coma cluster of galaxies
M. De Petris, L. D'Alba, L. Lamagna +7
We have measured the Sunyaev-Zeldovich effect towards the Coma cluster (A1656) with the MITO experiment, a 2.6-m telescope equipped with a 4-channel 17 arcminute (FWHM) photometer.…