DeBoer, David R. and Bower, Geoffrey C. and Keating, Garrett and Plambeck, Richard and Chang, Tzu-Ching and Ho, Paul T. P. and Marrone, Daniel and Readhead, Anthony (2013) DACOTA: The dense array for cosmological transitions. In: 2013 US National Committee of URSI National Radio Science Meeting (USNC-URSI NRSM). IEEE , Piscataway, NJ. ISBN 978-1-4673-4778-5. https://resolver.caltech.edu/CaltechAUTHORS:20170125-142618678
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Abstract
The Epoch of Reionization (EoR) heralded the advent of the Universe we recognize today, containing stars, galaxies and super-massive black holes. A number of experiments to detect the red-shifted hydrogen signature of the atomic component of the intergalactic medium (IGM) are on-going (e.g. PAPER, MWA, LOFAR). Due to the faintness of the signal, the bright foregrounds, and the challenge of instrumental systematics, multiple techniques are essential to create a more robust detection and to provide the complete picture on the evolution of early galaxies.
| Item Type: | Book Section | ||||||||
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| Additional Information: | © 2013 IEEE. | ||||||||
| DOI: | 10.1109/USNC-URSI-NRSM.2013.6525026 | ||||||||
| Record Number: | CaltechAUTHORS:20170125-142618678 | ||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20170125-142618678 | ||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||
| ID Code: | 73728 | ||||||||
| Collection: | CaltechAUTHORS | ||||||||
| Deposited By: | INVALID USER | ||||||||
| Deposited On: | 30 Jan 2017 22:58 | ||||||||
| Last Modified: | 11 Nov 2021 05:21 |
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