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Title: Characterizing and Modeling the Noise and Complex Impedance of Feedhorn-Coupled TES Polarimeters

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3292317· OSTI ID:21325793
; ; ; ; ; ;  [1]; ; ; ;  [2]; ; ; ; ; ; ;  [3]; ;  [4]
  1. Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University, Princeton, NJ, 08544 (United States)
  2. Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences and Department of Physics, University of Colorado, Boulder, CO 80309 (United States)
  3. NIST Quantum Devices Group, 325 Broadway Mailcode 817.03, Boulder, CO, USA 80305 (United States)
  4. Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States)

We present results from modeling the electrothermal performance of feedhorn-coupled transition edge sensor (TES) polarimeters under development for use in cosmic microwave background (CMB) polarization experiments. Each polarimeter couples radiation from a corrugated feedhorn through a planar orthomode transducer, which transmits power from orthogonal polarization modes to two TES bolometers. We model our TES with two- and three-block thermal architectures. We fit the complex impedance data at multiple points in the TES transition. From the fits, we predict the noise spectra. We present comparisons of these predictions to the data for two TESes on a prototype polarimeter.

OSTI ID:
21325793
Journal Information:
AIP Conference Proceedings, Vol. 1185, Issue 1; Conference: LTD13: 13. international workshop on low temperature detectors, Stanford, CA (United States), 20-24 Jul 2009; Other Information: DOI: 10.1063/1.3292317; (c) 2009 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English