CaltechAUTHORS
Published January 2013 | Version Published
Book Section - Chapter Open

DACOTA: The dense array for cosmological transitions

Creators

  • 1. ROR icon University of California, Berkeley
  • 2. ROR icon Institute of Astronomy and Astrophysics, Academia Sinica
  • 3. ROR icon University of Arizona
  • 4. ROR icon California Institute of Technology

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.

Additional Information

© 2013 IEEE.

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Identifiers

Eprint ID
73728
Resolver ID
CaltechAUTHORS:20170125-142618678

Dates

Created
2017-01-30
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Updated
2021-11-11
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