137 citations · 391 across the 12 of their papers we have counts for
12 papers · 1 filter
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…
Primordial Resonant Lines and Observational Strategy for ODIN and HERSCHEL
R. Maoli, P. Chambaud, J. Y. Daniel +8
The presence of a primordial molecular or atomic medium can give us the possibility to investigate the first phases of the structure formation. The lines produced by resonant scatt…
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…
MAD-4-MITO, a Multi Array of Detectors for ground-based mm/submm SZ observations
L. Lamagna, M. De Petris, F. Melchiorri +5
The last few years have seen a large development of mm technology and ultra-sensitive detectors devoted to microwave astronomy and astrophysics. The possibility to deal with large…
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.…
The Sunyaev-Zeldovich MITO Project
Livia D'Alba, Francesco Melchiorri, Marco De Petris +6
Compton scattering of the cosmic microwave background radiation by electrons in the hot gas in clusters of galaxies - the Sunyaev-Zeldovich effect - has long been recognized as a u…
BOOMERanG: a scanning telescope for 10 arcminutes resolution CMB maps
S. Masi, P. A. R. Ade, R. Artusa +24
The BOOMERanG experiment is a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales between a few degrees and ten arcminu…
Mapping the CMB Sky: The BOOMERANG experiment
P. de Bernardis, P. A. R. Ade, R. Artusa +23
We describe the BOOMERanG experiment, a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales between a few degrees and t…
Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American test flight of BOOMERANG
P. D. Mauskopf, P. A. R. Ade, P. de Bernardis +31
We describe a measurement of the angular power spectrum of anisotropies in the Cosmic Microwave Background (CMB) from 0.3 degrees to ~10 degrees from the North American test flight…
Molecular signals from primordial clouds at high redshift
R. Maoli, V. Ferrucci, F. Melchiorri +2
The possibility to detect cosmological signals from the post-recombination Universe is one of the main aims of modern cosmology. In a previous paper we emphasized the role that ela…