Far-infrared polarimeter with very low instrumental polarization

Elia Stefano Battistelli; Marco DePetris; Luca Lamagna; Roberto Maoli; Francesco Melchiorri; Emilia Palladino; Giorgio Savini; Philip D. Mauskopf; Angiola Orlando

doi:10.1117/12.458224

14 February 2003 Far-infrared polarimeter with very low instrumental polarization

Elia Stefano Battistelli, Marco DePetris, Luca Lamagna, Roberto Maoli, Francesco Melchiorri, Emilia Palladino, Giorgio Savini, Philip D. Mauskopf, Angiola Orlando

Author Affiliations +

Proceedings Volume 4843, Polarimetry in Astronomy; (2003) https://doi.org/10.1117/12.458224
Event: Astronomical Telescopes and Instrumentation, 2002, Waikoloa, Hawai'i, United States

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).

Citation Download Citation

Elia Stefano Battistelli, Marco DePetris, Luca Lamagna, Roberto Maoli, Francesco Melchiorri, Emilia Palladino, Giorgio Savini, Philip D. Mauskopf, and Angiola Orlando "Far-infrared polarimeter with very low instrumental polarization", Proc. SPIE 4843, Polarimetry in Astronomy, (14 February 2003); https://doi.org/10.1117/12.458224

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