activity
19952006
most citedMeasurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American test flight of BOOMERANG

137 citations · 391 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph2006★ 15 cited

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…

astro-ph2004★ 2 cited

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…

astro-ph2003★ 37 cited

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…

astro-ph2002★ 5 cited

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…

astro-ph2002★ 66 cited

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…

astro-ph2002★ 2 cited

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…