Design and characterization of the Large-Aperture Experiment to Detect the Dark Age (LEDA) radiometer systems
D.C. Price, L.J. Greenhill, A. Fialkov, G. Bernardi, H. Garsden, B.R., Barsdell, J. Kocz, M.M. Anderson, S.A. Bourke, J. Craig, M.R. Dexter, J., Dowell, M.W. Eastwood, T. Eftekhari, S.W. Ellingson, G. Hallinan, J.M., Hartman, R. Kimberk, T.J.W. Lazio, S. Leiker, D. MacMahon

TL;DR
LEDA is a radiometer system designed to detect the cosmic hydrogen absorption signature during the Dark Age, aiming to verify previous claims of a large absorption feature around 78 MHz.
Contribution
This paper details the design, calibration, and initial characterization of the LEDA radiometer systems for detecting the cosmic Dark Age signal.
Findings
Radiometer systems operate in 30-85 MHz band with dual polarization.
Calibration and characterization progress as of January 2016.
Modifications underway to improve performance near 78 MHz.
Abstract
The Large-Aperture Experiment to Detect the Dark Age (LEDA) was designed to detect the predicted O(100)mK sky-averaged absorption of the Cosmic Microwave Background by Hydrogen in the neutral pre- and intergalactic medium just after the cosmological Dark Age. The spectral signature would be associated with emergence of a diffuse Ly background from starlight during 'Cosmic Dawn'. Recently, Bowman et al. (2018) have reported detection of this predicted absorption feature, with an unexpectedly large amplitude of 530 mK, centered at 78 MHz. Verification of this result by an independent experiment, such as LEDA, is pressing. In this paper, we detail design and characterization of the LEDA radiometer systems, and a first-generation pipeline that instantiates a signal path model. Sited at the Owens Valley Radio Observatory Long Wavelength Array, LEDA systems include the station…
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