8 citations · 14 across the 7 of their papers we have counts for
8 papers
The Planck Low Frequency Instrument
N. Mandolesi, C. Burigana, R. C. Butler +14
Planck is the third generation of mm-wave instruments designed for space observations of the cosmic microwave background (CMB) anisotropies within the new Cosmic Vision 2020 ESA Sc…
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…