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...
| Main Authors: | , , |
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| Format: | Journal Article |
| Published: |
American Physical Society
2014
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| Online Access: | http://hdl.handle.net/20.500.11937/8395 |