8 citations · 14 across the 7 of their papers we have counts for
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The CMB Power Spectrum from the Background Emission Anisotropy Scanning Telescope (BEAST) Experiment
Ian J. O'Dwyer, Marco Bersanelli, Jeffrey Childers +19
The Background Emission Anisotropy Scanning Telescope (BEAST) is a 2.2m off-axis telescope with an 8 element mixed Q (38-45GHz) and Ka (26-36GHz) band focal plane, designed for bal…
Signature of HDM clustering at Planck angular scales
L. A. Popa, C. Burigana, N. Mandolesi
We present the CMB anisotropy induced by the non-linear perturbations in the massive neutrino density associated to the non-linear gravitational clustering. We show that the non-li…
Advanced pseudo-correlation radiometers for the Planck-LFI instrument
A. Mennella, M. Bersanelli, R. C. Butler +34
The LFI (Low Frequency Instrument) on board the ESA Planck satellite is constituted by an array of radiometric detectors actively cooled at 20 K in the 30-70 GHz frequency range in…
Advanced simulation techniques for straylight prediction of high performance mm-wave reflecting telescope
M. Sandri, F. Villa, M. Bersanelli +3
The prediction of the antenna radiation pattern can be extremely complex for antenna system composed of several reflector surfaces. Typically, at mm-wavelengths, telescopes are com…
PLANCK/LFI: an Advanced Multi-beam High Performance mm-wave Optics for Space Applications
F. Villa, M. Sandri, M. Bersanelli +5
The Low Frequency Instrument (LFI) is one of the two instruments onboard the ESA PLANCK satellite foreseen to be launched in 2007. The LFI will image the Cosmic Microwave Backgroun…
A Map of the Cosmic Microwave Background from the BEAST Experiment
Peter R. Meinhold, Marco Bersanelli, Jeffrey Childers +24
We present the first sky maps from the BEAST (Background Emission Anisotropy Scanning Telescope) experiment. BEAST consists of a 2.2 meter off axis Gregorian telescope fed by a cry…