Murriyang cryogenic phased array feed: Spectral-line results and noise-reduction methods

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Authors: Lister Staveley‐Smith, S. Barker, R. Berangi, A.B. Bolin, S. Broadhurst, J. D. Bunton, Nick Carter, Santiago Castillo, W. Chandler, A. P. Chippendale, J.R. Dawson, F. Di Dio
+16 more A.R. Dunning, Scott D. Gordon, J. Green, A. Hafner, DB Hayman, D. Humphrey, A. Jameson, S. Johnston, J.F. Kaczmarek, J. Ma, G. Perry, M. Pilawa, Jonghwan Rhee, Lawrence Toomey, J. van Aardt, N. Wang
Cited by: 1
References: 102

Abstract

Abstract Spectral-line results from a new cryogenic phased array feed (cryoPAF) on the Murriyang telescope at Parkes are presented. This array offers a significant improvement in field of view, aperture efficiency, bandwidth, chromaticity, and survey speed compared with conventional horn-fed receivers. We demonstrate this with measurements of sky calibrators and observations of 21-cm neutral hydrogen (HI) in the Large Magellanic Cloud (LMC) and the nearby galaxy NGC 6744. Within 0.3 deg of the optical axis, the ratio of system temperature to dish aperture efficiency ( $T_\mathrm{sys}/\eta_{d}$ ) is 25 K, and the ratio with beam efficiency ( $T_\mathrm{sys}/\eta_\mathrm{mb}$ ) is 21 K (at 1.4 GHz). For the previously measured $T_\mathrm{sys} = 17$ K, respective efficiency values $\eta_{d} \approx 0.7$ and $\eta_\mathrm{mb} \approx 0.8$ are derived. Our HI observational results are in good agreement with previous results, although detailed comparison with multibeam observations of the LMC suggests that the earlier observations may have missed an extended component of low-column-density gas ( $\sim$ $8\times 10^{18}$ cm $^{-2}$ ). We use the cryoPAF zoom-band and wideband data to make a preliminary investigation of whether the large number of simultaneous beams (72) permits the use of novel data reduction methods to reduce the effects of foreground/background continuum contamination and radio-frequency interference (RFI). We also investigate if these methods can better protect against signal loss for the detection of faint, extended cosmological signals such as HI intensity maps. Using robust higher-order singular value decomposition (SVD) techniques, we find encouraging results for the detection of both compact and extended sources, including challenging conditions with high RFI occupancy and significant sky continuum structure. Examples are shown that demonstrate that 3D SVD techniques offer a significant improvement in noise reduction and signal capture compared with more traditional layered 2D techniques.

Fields of Study & Subjects

Radio Astronomy Observations and Technology Superconducting and THz Device Technology Astronomy and Astrophysical Research

Publication details

Journal / source
Publications of the Astronomical Society of Australia
Publisher
Cambridge University Press (CUP)
Volume
43
Publication date
1 January 2026
Language
EN