Data

Parkes observations for project P1061 semester 2020OCTS_05

Commonwealth Scientific and Industrial Research Organisation
Luo, Rui ; Hobbs, George ; Dai, Shi ; Deng, Xinping ; Zhang, Songbo ; Wang, Shuangqiang
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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/vc7z-ab33&rft.title=Parkes observations for project P1061 semester 2020OCTS_05&rft.identifier=https://doi.org/10.25919/vc7z-ab33&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Fast Radio Bursts (FRBs) have extremely high brightness temperature, owing to their short-duration and prominent flux from the distant universe. The studies on emission mechanism of FRBs have met bottleneck for a long time unless a complete spectrum is measured. We propose to observe a new repeating FRB source, FRB 180301, using the Parkes ultra-wide-bandwidth receiver (UWL). This source was initially found by Parkes multibeam receivers and confirmed repetition by the FAST telescope. The source is still active until Jun 2020 from FAST follow-ups. It’s an ideal opportunity to capture comprehensive spectral information using the Parkes UWL. We demonstrate that the beam coverage is feasible and 30-hr observations are required for at least one detection.&rft.creator=Luo, Rui &rft.creator=Hobbs, George &rft.creator=Dai, Shi &rft.creator=Deng, Xinping &rft.creator=Zhang, Songbo &rft.creator=Wang, Shuangqiang &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=P1061_2020OCTS&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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Fast Radio Bursts (FRBs) have extremely high brightness temperature, owing to their short-duration and prominent flux from the distant universe. The studies on emission mechanism of FRBs have met bottleneck for a long time unless a complete spectrum is measured. We propose to observe a new repeating FRB source, FRB 180301, using the Parkes ultra-wide-bandwidth receiver (UWL). This source was initially found by Parkes multibeam receivers and confirmed repetition by the FAST telescope. The source is still active until Jun 2020 from FAST follow-ups. It’s an ideal opportunity to capture comprehensive spectral information using the Parkes UWL. We demonstrate that the beam coverage is feasible and 30-hr observations are required for at least one detection.

Available: 2020-12-30

Data time period: 2020-10-01 to 2021-03-31

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Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | P1061_2020OCTS | Physical Sciences | neutron stars | pulsars |

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Identifiers
ACN 633 798 857