14 February 2003 Far-infrared polarimeter with very low instrumental polarization
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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).
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Elia Stefano Battistelli, Elia Stefano Battistelli, Marco DePetris, Marco DePetris, Luca Lamagna, Luca Lamagna, Roberto Maoli, Roberto Maoli, Francesco Melchiorri, Francesco Melchiorri, Emilia Palladino, Emilia Palladino, Giorgio Savini, Giorgio Savini, Philip D. Mauskopf, Philip D. Mauskopf, Angiola Orlando, Angiola Orlando, "Far-infrared polarimeter with very low instrumental polarization", Proc. SPIE 4843, Polarimetry in Astronomy, (14 February 2003); doi: 10.1117/12.458224; https://doi.org/10.1117/12.458224


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