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The Primordial Inflation Polarization Explorer (PIPER): instrument description

Eimer, Joseph, Bennett, C., McCullagh, L., Zeng, L., Benford, D., Chuss, D., Fixsen, D., Hinderks, J., Jhabvala, C., Kogut, A., Mirel, P., Moseley, S., Staguhn, G., Voellmer, G., Wollack, E., Irwin, K., Hilton, G., Halpern, M., Ade, Peter A. R., Tucker, Carole and Dotson, J. 2010. The Primordial Inflation Polarization Explorer (PIPER): instrument description. Presented at: American Astronomical Society 215th Meeting, Washington, DC, January 4th 2010, Washigton, DC, 4 January, 2010.

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Abstract

We describe the PIPER balloon born instrument for observing the polarization of the cosmic microwave background. The experiment uses two co-aligned cold optic telescopes with variable-delay polarization modulators as their first optical element. Each telescope has two 32 x 40 arrays of backshort-under-grid(BUG) TES bolometers

Item Type: Conference or Workshop Item (Poster)
Date Type: Completion
Status: Unpublished
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Last Modified: 04 Jun 2017 04:09
URI: http://orca.cf.ac.uk/id/eprint/33530

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