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DACOTA: The dense array for cosmological transitions

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
Related URLs:
URLURL TypeDescription
https://doi.org/10.1109/USNC-URSI-NRSM.2013.6525026DOIArticle
ORCID:
AuthorORCID
Bower, Geoffrey C.0000-0003-4056-9982
Marrone, Daniel0000-0002-2367-1080
Readhead, Anthony0000-0001-9152-961X
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: Kristin Buxton
Deposited On:30 Jan 2017 22:58
Last Modified:11 Nov 2021 05:21

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