FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA

FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA

Detection of 21 cm emission of H i from the epoch of reionization, at redshifts z > 6, is limited primarily by foreground emission. We investigate the signatures of wide-field measurements and an all-sky foreground model using the delay spectrum technique that maps the measurements to foreground...

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Bibliographic Details
Main Authors: Cappallo, Roger J. (Contributor), Corey, Brian E. (Contributor), de Oliveira-Costa, Angelica (Contributor), Dillon, Joshua Shane (Contributor), Ewall-Wice, Aaron Michael (Contributor), Feng, L. (Contributor), Goeke, Robert F. (Contributor), Hewitt, Jacqueline N. (Contributor), Kratzenberg, Eric W. (Contributor), Lonsdale, Colin John (Contributor), McWhirter, Stephen R. (Contributor), Morgan, Edward H. (Contributor), Neben, Abraham Richard (Contributor), Rogers, Alan E. E. (Contributor), Tegmark, Max Erik (Contributor), Whitney, Alan R. (Contributor), Williams, Christopher Leigh (Contributor)
Other Authors: Haystack Observatory (Contributor), Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-05-28T17:43:35Z.
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