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EBEX: The E and B Experiment

Abstract : The E and B experiment (EBEX) is a balloon-borne telescope designed to measure the polar- ization of the cosmic microwave background radiation as well as that from Galactic dust. The instrument is equipped with a 1.5 meter aperture Gregorian-Dragone telescope, providing an 8' beam at three frequency bands centered on 150, 250 and 410 GHz. Polarimetry is achieved by rotating an achromatic half-wave plate on a superconducting magnetic bearing. In January 2013, EBEX completed 11 days of observations in a ight over Antarctica covering 6000 square degrees of the sky. This marks the rst time that arrays with about 1000 transition-edge sensor bolometers have made science observations on a balloon-borne platform. These proceedings describe the EBEX instrument, the science ight and the status of the data analysis. 1 I
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Submitted on : Thursday, February 19, 2015 - 5:06:46 PM
Last modification on : Friday, December 18, 2020 - 6:46:05 PM

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  • HAL Id : in2p3-01118723, version 1

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Joy Didier, Asad M. Aboobaker, Peter Ade, Francois Aubin, Carlo Baccigalupi, et al.. EBEX: The E and B Experiment. XLIXth Rencontres de Moriond – Cosmology, Mar 2014, La Thuile, Italy. pp.41-44. ⟨in2p3-01118723⟩

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