Data

Parkes observations for project P1059 semester 2020APRS_08

Commonwealth Scientific and Industrial Research Organisation
Dai, Shi ; Lenc, Emil ; Hobbs, George ; Zhang, Lei ; Joshi, Bhal Chandra ; Achamveedu, Gopakumar ; Thyagarajan, Nithyanandan
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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:doi10.25919/5f69755c9994f&rft.title=Parkes observations for project P1059 semester 2020APRS_08&rft.identifier=https://doi.org/10.25919/5f69755c9994f&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose to observe a sample of 22 pulsars at high Galactic latitudes with the Parkes Ultra-Wideband Low (UWL) receiver. This sample of pulsars does not have flux densities nor polarisation measured before. The goal is to characterise their wideband properties in polarisation, spectrum and interstellar scintillation. Such properties will help us develop imaging pulsar search techniques for future radio continuum surveys, such as with the Australian SKA Pathfinder (ASKAP). Wideband spectrum, polarisation and scintillation of pulsars will also be useful for studies of pulsar radiation mechanism and interstellar medium at high Galactic latitudes.&rft.creator=Dai, Shi &rft.creator=Lenc, Emil &rft.creator=Hobbs, George &rft.creator=Zhang, Lei &rft.creator=Joshi, Bhal Chandra &rft.creator=Achamveedu, Gopakumar &rft.creator=Thyagarajan, Nithyanandan &rft.date=2020&rft.edition=v1&rft_rights=Creative Commons Attribution 4.0 International Licence https://creativecommons.org/licenses/by/4.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO 2020.&rft_subject=pulsars&rft_subject=neutron stars&rft_subject=P1059_2020APRS&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data
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We propose to observe a sample of 22 pulsars at high Galactic latitudes with the Parkes Ultra-Wideband Low (UWL) receiver. This sample of pulsars does not have flux densities nor polarisation measured before. The goal is to characterise their wideband properties in polarisation, spectrum and interstellar scintillation. Such properties will help us develop imaging pulsar search techniques for future radio continuum surveys, such as with the Australian SKA Pathfinder (ASKAP). Wideband spectrum, polarisation and scintillation of pulsars will also be useful for studies of pulsar radiation mechanism and interstellar medium at high Galactic latitudes.

Available: 2020-09-23

Data time period: 2020-04-01 to 2020-09-30

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Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | P1059_2020APRS | Physical Sciences | neutron stars | pulsars |

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Identifiers
ACN 633 798 857