The PLANCK LFI flight model ortho-mode transducers
O. D'Arcangelo, A. Simonetto, L. Figini, E. Pagana, F.Villa, M., Pecora, P. Battaglia, M. Bersanelli, R.C. Butler, S. Garavaglia, P. Guzzi, N., Mandolesi, C. Sozzi

TL;DR
This paper details the design, development, and testing of the Ortho-Mode Transducers for the Planck LFI instrument, crucial for polarization measurements of the Cosmic Microwave Background.
Contribution
It presents the complete development process and performance evaluation of the eleven flight model OMTs, including design, manufacturing, and qualification testing.
Findings
All OMT units met flight acceptance criteria.
Electromagnetic performance was at least marginally compliant.
Units passed thermoelastic qualification tests.
Abstract
The Low Frequency Instrument (LFI) of the ESA Planck CMB mission is an array of 22 ultra sensitive pseudocorrelation radiometers working at 30, 44, and 70 GHz. LFI has been calibrated and delivered for integration with the satellite to the European Space Agency on November 2006. The aim of Planck is to measure the anisotropy and polarization of the Cosmic Background Radiation with a sensitivity and angular resolution never reached before over the full sky. LFI is intrinsically sensitive to polarization thanks to the use of Ortho-Mode Transducers (OMT) located between the feedhorns and the pseudo-correlation radiometers. The OMTs are microwave passive components that divide the incoming radiation into two linear orthogonal components. A set of 11 OMTs (2 at 30 GHz, 3 at 44 GHz, and 6 at 70 GHz) were produced and tested. This work describes the design, development and performance of the…
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