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Optical design of the EPIC-IM crossed Dragone telescope

Authors :
Chao-Lin Kuo
James J. Bock
Talso Chui
Elena Pierpaoli
Daniel Bauman
Paul L. Richards
Charles R. Lawrence
M. D. Seiffert
Andrew E. Lange
Celeste Satter
Shaul Hanany
Meir Shimon
Peter Day
Abdullah S. Aljabri
Huan Tran
Adrian T. Lee
Hien Nguyen
Jonas Zmuidzinas
S. S. Meyer
Nate Miller
Clive Dickenson
Brad Johnson
M. Betoule
A. Amblard
Asantha Cooray
Brian Keating
Brett Williams
Sunil Golwala
Kent D. Irwin
Nicolas Ponthieu
Dustin Crumb
Jeff Raab
L. P. L. Colombo
Krzysztof M. Gorski
Warren Holmes
Jean Loup Puget
Darren Dowell
M. Dragovan
Oschmann, Jacobus M., Jr.
Clampin, Mark C.
MacEwen, Howard A.
Source :
SPIE Proceedings.
Publication Year :
2010
Publisher :
SPIE, 2010.

Abstract

The Experimental Probe of Inflationary Cosmology - Intermediate Mission (EPIC-IM) is a concept for the NASA Einstein Inflation Probe satellite. EPIC-IM is designed to characterize the polarization properties of the Cosmic Microwave Background to search for the B-mode polarization signal characteristic of gravitational waves generated during the epoch of Inflation in the early universe. EPIC-IM employs a large focal plane with 11,000 detectors operating in 9 wavelength bands to provide 30 times higher sensitivity than the currently operating Planck satellite. The optical design is based on a wide-field 1.4 m crossed-Dragone telescope, an aperture that allows not only comprehensive measurements of Inflationary B-mode polarization, but also measurements of the E-mode and lensing polarization signals to cosmological limits, as well as all-sky maps of Galactic polarization with unmatched sensitivity and angular resolution. The optics are critical to measuring these extremely faint polarization signals, and any design must meet demanding requirements on systematic error control. We describe the EPIC-IM crossed Dragone optical design, its polarization properties, and far-sidelobe response.

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
SPIE Proceedings
Accession number :
edsair.doi.dedup.....ff67bc2a44b182f72f587ef22883b9be
Full Text :
https://doi.org/10.1117/12.857423