An ultra-wide bandwidth (704 to 4 032 MHz) receiver for the Parkes radio telescope

2019/11/02 by George Hobbs, G. Hobbs, R. N. Manchester +140 · 1 voice · 13 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #astro-ph.IM

paper · pdf · doi:10.1017/pasa.2020.2

openalex created_date 2019/11/22 · openalex publication_date 2020/01/01 · openalex updated_date 2026/07/30

Abstract

Abstract We describe an ultra-wide-bandwidth, low-frequency receiver recently installed on the Parkes radio telescope. The receiver system provides continuous frequency coverage from 704 to 4032 MHz. For much of the band ( ∼60% ), the system temperature is approximately 22 K and the receiver system remains in a linear regime even in the presence of strong mobile phone transmissions. We discuss the scientific and technical aspects of the new receiver, including its astronomical objectives, as well as the feed, receiver, digitiser, and signal processor design. We describe the pipeline routines that form the archive-ready data products and how those data files can be accessed from the archives. The system performance is quantified, including the system noise and linearity, beam shape, antenna efficiency, polarisation calibration, and timing stability.

Citations

• A two-solar-mass neutron star measured using Shapiro delay

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Discussions

• The biggest bandwidth telescope and instrument in that plot is "PKS UWL" - which is the Parkes radio telescope (Murriyang) Ultra-Wideband Low-frequency receiver. That's the instrument we use! 📡 It's [bsky, 7 points, 0 comments]

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