Epoch of reionization window. II. Statistical methods for foreground wedge reduction

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Epoch of reionization window. II. Statistical methods for foreground wedge reduction

For there to be a successful measurement of the 21 cm epoch of reionization (EoR) power spectrum, it is crucial that strong foreground contaminants be robustly suppressed. These foregrounds come from a variety of sources (such as Galactic synchrotron emission and extragalactic point sources), but al...

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Bibliographic Details
Main Authors:	Liu, A., Parsons, A., Trott, Cathryn
Format:	Journal Article
Published:	American Physical Society 2014
Online Access:	http://hdl.handle.net/20.500.11937/8395

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