EMBRACE@Nançay: An ultra wide field of view prototype for the SKA
Journal article, 2015
A revolution in radio receiving technology is underway with the development of densely packed phased arrays for radio astronomy. This technology can provide an exceptionally large field of view, while at the same time sampling the sky with high angular resolution. Such an instrument, with a field of view of over 100 square degrees, is ideal for performing fast, all-sky, surveys, such as the ''intensity mapping'' experiment to measure the signature of Baryonic Acoustic Oscillations in the HI mass distribution at cosmological redshifts. The SKA, built with this technology, will be able to do a billion galaxy survey. I will present a very brief introduction to radio interferometry, as well as an overview of the Square Kilometre Array project. This will be followed by a description of the EMBRACE prototype and a discussion of results and future plans.
Instrumental noise
Instrument optimization
Antennas
Author
S. A. Torchinsky
USN - Station de Radioastronomie de Nancay
Henrik Olofsson
Chalmers, Earth and Space Sciences, Onsala Space Observatory
B. Censier
USN - Station de Radioastronomie de Nancay
A. Karastergiou
Rhodes University
M. Serylak
Onsala Space Observatory
University of the Western Cape
Rhodes University
USN - Station de Radioastronomie de Nancay
University of Oxford
P. Renaud
USN - Station de Radioastronomie de Nancay
C. Taffoureau
USN - Station de Radioastronomie de Nancay
Journal of Instrumentation
1748-0221 (ISSN)
Vol. 10 7Subject Categories (SSIF 2011)
Fusion, Plasma and Space Physics
DOI
10.1088/1748-0221/10/07/C07002