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 employed at MITO telescope to search for calibration sources and investigate polarization near the CMB anisotropy peaks in the next campaign (Winter 2002-03).
Far infrared polarimeter with very low instrumental polarization / Battistelli, Elia Stefano; DE PETRIS, Marco; Lamagna, Luca; Maoli, Roberto; Melchiorri, F.; Palladino, E.; Savini, G.; Mauskopf, P. D.; Orlando, A.. - 4843:(2003), pp. 241-249. (Intervento presentato al convegno Polarimetry in Astronomy tenutosi a Waikoloa, Hawaii, USA) [10.1117/12.458224].
Far infrared polarimeter with very low instrumental polarization
BATTISTELLI, Elia Stefano
;DE PETRIS, Marco;LAMAGNA, Luca;MAOLI, Roberto;
2003
Abstract
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 employed at MITO telescope to search for calibration sources and investigate polarization near the CMB anisotropy peaks in the next campaign (Winter 2002-03).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
