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Parkes observations for project P1101 semester 2021OCTS_14

Commonwealth Scientific and Industrial Research Organisation
Dai, Shi ; Hobbs, George ; Li, Di ; Zhu, Weiwei ; Feng, Yi ; Niu, Chenhui
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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/yk5c-3s33&rft.title=Parkes observations for project P1101 semester 2021OCTS_14&rft.identifier=https://doi.org/10.25919/yk5c-3s33&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose to carry out fortnightly monitoring of a very active repeater, FRB~190520, with the Parkes UWL system. Our current observations show that FRB~190520 is not only the most active FRB that can be observed with Parkes, but also shows unique behaviour at 2 to 3 GHz frequency. This makes UWL the ideal instrument to carry out in-depth studies of this repeating FRB. With this program, we expect to detect a large sample of bursts from FRB~190520, and in collaboration with the FAST telescope we will study emission properties, fluence distributions and polarisation properties over an extremely wide bandwidth with high sensitivity.&rft.creator=Dai, Shi &rft.creator=Hobbs, George &rft.creator=Li, Di &rft.creator=Zhu, Weiwei &rft.creator=Feng, Yi &rft.creator=Niu, Chenhui &rft.date=2022&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 2021.&rft_subject=transients&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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Brief description

We propose to carry out fortnightly monitoring of a very active repeater, FRB~190520, with the Parkes UWL system. Our current observations show that FRB~190520 is not only the most active FRB that can be observed with Parkes, but also shows unique behaviour at 2 to 3 GHz frequency. This makes UWL the ideal instrument to carry out in-depth studies of this repeating FRB. With this program, we expect to detect a large sample of bursts from FRB~190520, and in collaboration with the FAST telescope we will study emission properties, fluence distributions and polarisation properties over an extremely wide bandwidth with high sensitivity.

Available: 2022-03-03

Data time period: 2021-10-01 to 2022-03-31

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Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Physical Sciences | transients |

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