TY - JOUR
T1 - The SKA particle array prototype
T2 - The first particle detector at the Murchison Radio-astronomy Observatory
AU - Bray, J. D.
AU - Williamson, A.
AU - Schelfhout, J.
AU - James, C. W.
AU - Spencer, R. E.
AU - Chen, H.
AU - Cropper, B. D.
AU - Emrich, D.
AU - Gould, K. M.L.
AU - Haungs, A.
AU - Hodder, W.
AU - Howland, T.
AU - Huege, T.
AU - Kenney, D.
AU - McPhail, A.
AU - Mitchell, S.
AU - Niţu, I. C.
AU - Roberts, P.
AU - Tawn, R.
AU - Tickner, J.
AU - Tingay, S. J.
PY - 2020/9/1
Y1 - 2020/9/1
N2 - We report on the design, deployment, and first results from a scintillation detector deployed at the Murchison Radio-astronomy Observatory (MRO). The detector is a prototype for a larger array – the Square Kilometre Array Particle Array (SKAPA) – planned to allow the radio-detection of cosmic rays with the Murchison Widefield Array and the low-frequency component of the Square Kilometre Array. The prototype design has been driven by stringent limits on radio emissions at the MRO, and to ensure survivability in a desert environment. Using data taken from Nov. 2018 to Feb. 2019, we characterize the detector response while accounting for the effects of temperature fluctuations, and calibrate the sensitivity of the prototype detector to through-going muons. This verifies the feasibility of cosmic ray detection at the MRO. We then estimate the required parameters of a planned array of eight such detectors to be used to trigger radio observations by the Murchison Widefield Array.
AB - We report on the design, deployment, and first results from a scintillation detector deployed at the Murchison Radio-astronomy Observatory (MRO). The detector is a prototype for a larger array – the Square Kilometre Array Particle Array (SKAPA) – planned to allow the radio-detection of cosmic rays with the Murchison Widefield Array and the low-frequency component of the Square Kilometre Array. The prototype design has been driven by stringent limits on radio emissions at the MRO, and to ensure survivability in a desert environment. Using data taken from Nov. 2018 to Feb. 2019, we characterize the detector response while accounting for the effects of temperature fluctuations, and calibrate the sensitivity of the prototype detector to through-going muons. This verifies the feasibility of cosmic ray detection at the MRO. We then estimate the required parameters of a planned array of eight such detectors to be used to trigger radio observations by the Murchison Widefield Array.
KW - Cosmic rays
KW - Murchison Radio-astronomy Observatory
KW - Murchison Widefield Array
KW - Scintillation detectors
KW - Square Kilometre Array
UR - http://www.scopus.com/inward/record.url?scp=85085275763&partnerID=8YFLogxK
U2 - 10.1016/j.nima.2020.164168
DO - 10.1016/j.nima.2020.164168
M3 - Article
AN - SCOPUS:85085275763
VL - 973
JO - Nuclear Instruments and Methods in Physics Research Section A
JF - Nuclear Instruments and Methods in Physics Research Section A
SN - 0168-9002
M1 - 164168
ER -