The Low Frequency Instrument (LFI) is one of the two instrument onboard the ESA Planck Mission. LFI will image the Cosmic Microwave Background anisotropies in four different bands, from 30 GHz to 100 GHz, with an array of 54 radiometers. The instrument characteristics and expected performances are presented, with particular attention to the control of systematic effects.
Planck low frequency instrument / N. Mandolesi, M. Bersanelli, R.C. Butler, C. Burigana, D. Maino, A. Mennella, G. Morgante, L. Valenziano, F. Villa - In: Experimental cosmology at millimetre wavelengths : 2K1BC workshop, Breuil-Cervinia (AO), Valle d'Aosta, Italy, 9-13 July 2001 / [a cura di] M. De Petris, M. Gervasi. - Melville : American institute of physics, 2002. - ISBN 0-7354-0062-8. - pp. 193-201 (( convegno Workshop on experimental cosmology at millimetre wavelengths tenutosi a Breuil-Cervinia (Italia) nel 2001 [10.1063/1.1475627].
Planck low frequency instrument
M. BersanelliSecondo
;D. Maino;A. Mennella;F. VillaUltimo
2002
Abstract
The Low Frequency Instrument (LFI) is one of the two instrument onboard the ESA Planck Mission. LFI will image the Cosmic Microwave Background anisotropies in four different bands, from 30 GHz to 100 GHz, with an array of 54 radiometers. The instrument characteristics and expected performances are presented, with particular attention to the control of systematic effects.
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