BIGHORNS - Broadband Instrument for Global HydrOgen ReioNisation Signal
M. Sokolowski, S. E. Tremblay, R. B. Wayth, S. J. Tingay, N. Clarke,, P. Roberts, M. Waterson, R. D. Ekers, P. Hall, M. Lewis, M. Mossammaparast,, S. Padhi, F. Schlagenhaufer, A. Sutinjo, J. Tickner

TL;DR
The BIGHORNS experiment aims to detect the faint global hydrogen reionization signal from the Epoch of Reionisation using a highly stable, calibrated radiometer deployed in radio-quiet remote locations, addressing calibration and interference challenges.
Contribution
This paper introduces the design, deployment, and initial data collection of the BIGHORNS radiometer system for detecting the global 21cm signal from the Epoch of Reionisation, highlighting key calibration and interference mitigation strategies.
Findings
Deployment in radio-quiet locations yielded low RFI data
Identification of calibration challenges led to system improvements
Initial data collection demonstrates system stability and potential for EoR detection
Abstract
The redshifted 21cm line of neutral hydrogen (HI), potentially observable at low radio frequencies (~50-200 MHz), should be a powerful probe of the physical conditions of the inter-galactic medium during Cosmic Dawn and the Epoch of Reionisation (EoR). The sky-averaged HI signal is expected to be extremely weak (~100 mK) in comparison to the foreground of up to 10000 K at the lowest frequencies of interest. The detection of such a weak signal requires an extremely stable, well characterised system and a good understanding of the foregrounds. Development of a nearly perfectly (~mK accuracy) calibrated total power radiometer system is essential for this type of experiment. We present the BIGHORNS (Broadband Instrument for Global HydrOgen ReioNisation Signal) experiment which was designed and built to detect the sky-averaged HI signal from the EoR at low radio frequencies. The BIGHORNS…
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