Data

Parkes observations for project P960 semester 2021APRS_03

Commonwealth Scientific and Industrial Research Organisation
Mader, Stacy ; Green, James ; Robishaw, Timothy
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.25919/p1aa-9305&rft.title=Parkes observations for project P960 semester 2021APRS_03&rft.identifier=10.25919/p1aa-9305&rft.publisher=Commonwealth Scientific and Industrial Research Organisation (CSIRO)&rft.description=We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS, SX, K/KU-BAND and 13MM packages. In addition to cross-referencing C007 for flux calibration via pointing, we aim to conduct gain-elevation and system temperature experiments using the Moon, to ensure users of the Parkes Observatory have the most accurate information available for calibration purposes. We also wish to fully characterise the spectro-polarimetry response of the UWL, by determining the Mueller Matrix of the receiver.&rft.creator=Mader, Stacy &rft.creator=Green, James &rft.creator=Robishaw, Timothy &rft.date=2021&rft.edition=v1&rft_rights=All Rights (including copyright) CSIRO 2021.&rft_rights=Creative Commons Attribution https://creativecommons.org/licenses/by/4.0/&rft_subject=interstellar medium in and around the Milky Way, magnetic fields, active galactic nuclei / quasars&rft_subject=Astronomical and Space Sciences not elsewhere classified&rft_subject=PHYSICAL SCIENCES&rft_subject=ASTRONOMICAL AND SPACE SCIENCES&rft.type=dataset&rft.language=English Access the data

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Creative Commons Attribution
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All Rights (including copyright) CSIRO 2021.

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Brief description

We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS, SX, K/KU-BAND and 13MM packages. In addition to cross-referencing C007 for flux calibration via pointing, we aim to conduct gain-elevation and system temperature experiments using the Moon, to ensure users of the Parkes Observatory have the most accurate information available for calibration purposes. We also wish to fully characterise the spectro-polarimetry response of the UWL, by determining the Mueller Matrix of the receiver.

Data time period: 2021-04-01 to 2021-09-30

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