![]() ![]() 1st May 2020: Updated Medusa search mode coherent dedispersion and DM parameters.20th Jun 2020: Updated information on accessing Medusa from outside the ATNF/CSIRO network.Updated information on DHAGU? release v0.10.0. 23rd Sep 2020: Included Tsys/Tcal plots for the 13MM receiver.28th Oct 2020: Added information on supported web browsers.19th Feb 2021: Added field_comment to CSV import in DHAGU?.1st March 2021: Lowered supported Firefox on Debian to v78.11th Mar 2021: Clarified definition of the output_tsubint parameter.4th Apr 2021: Updated text and figures associated with scanning modes as the scan type can now be defined as a small or great-circle scan.Removed H-OH receiver (superceeded by UWL.) 18th May 2021: Improved Moon Tsys/Tcal plots for some receivers.26th May 2021: Updated 13MM Tsys/Tcal plots.Removed option to select small/great circle scans. 31st May 2021: 'field_comment' in a CSV import file is now 'comment'.The joffrey command "makePSRCAT_backends" now pushes the current version of PSRCAT toĭHAGU?, but note a logout/login of DHAGU? is required to pick up the changes. This isĭone internally, with the condition lat1=lat2 for the endpoints results in a small-circle scan, great otherwise. 15th Jun 2021: It is no longer possible to select the mode of a scan as small or great-circle.28th Jun 2021: Removed 0407-658 as a continuum calibrator as there is no well-defined flux model.13th Jul 2021: Added 13MM gain-el curve at 22387 MHz.29th Jul 2021: Added 13mm gain-el curve at 23916 MHz.27th Aug 2021: Added gain-el curves for UWL at 1.38, 3.1 and 3.3 GHz.07th Mar 2022: Added info on Observing Queue being disabled if wind parked.17th Mar 2022: Added information on the NoDrive observing mode.20th Apr 2022: Added information on setting up MARS/13MM receivers and DHAGU? integration.16th May 2022: Remove TOS import, added information on observing with MARS/13MM receivers.10th Jun 2022: Added SPOT continuum mode for pointing purposes.13th Oct 2022: Updated Mars configuration on Medusa to an LO setting of 8457 MHz was 8500 MHz.03rd Nov 2022: Removed Galileo, SX and AT-Prototype as offered receivers.In any of our documentation, please email the Murriyang Users GuideĬomments on documentation are especially welcomed. If you find that any part of Murriyang doesn't work as described The presentation of the document on the webĪnd in print was improved, and the content was significantly updated.Ĭopies of this manual and other ATNF documentation can be obtained In 2019 April there was a major overhaul of this manual: Chapter 4 walks you through processes that occur once your observations are over, such as accessing your data and reporting your experiences. Chapter 3 is dedicated to observing procedures and systems and details how to actually do your observations. Chapter 2 can be read after being given observing time on Murriyang, as this chapter focuses on preparations needed to observe with Murriyang. This information can be used before proposing to use the telescope, the procedure for which is also detailed in this chapter. ![]() Chapter 1 describes the telescope system, including the characteristics of the available receivers and backends. This manual is a reference and you should not feel that you must read all of it in order to use Murriyang. Murriyang, the 64m CSIRO Parkes Radio Telescope. This manual describes how to apply for observing time, make an observing schedule and carry out observations with
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