Data

Long-term project observations for project P1101 semester 2025OCTS_05

Commonwealth Scientific and Industrial Research Organisation
Dai, Shi ; Hobbs, George ; Li, Di ; Wang, Pei ; Zhang, Lei ; Zhu, Weiwei ; Feng, Yi ; Xue, Mengyao ; Yang, Yuanpei ; Zhang, YongKun ; Niu, Chenhui ; Xu, Jiaying ; Zhu, Yuhao ; Zhang, Jiaheng
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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/fqy0-4137&rft.title=Long-term project observations for project P1101 semester 2025OCTS_05&rft.identifier=https://doi.org/10.25919/fqy0-4137&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose a long-term project to monitor a very active repeater, FRB 20190520B, with Murriyang's UWL system. Our previous observations show that FRB 20190520B is not only among the most active FRBs that can be observed with Murriyang, but also shows extreme rotation measure (RM) and dispersion measure (DM) evolution, along with distinctive behavior at 3GHz frequency. This makes the UWL receiver uniquely suited for detailed studies and long-term monitoring of this repeating FRB. Through this program, we anticipate detecting a large sample of bursts from this FRB. In collaboration with FAST, we aim to investigate the time evolution of various properties of FRB 20190520B, enhance our understanding of polarisation across an extremely wide bandwidth with high sensitivity, and gain deeper insights into the local environment and emission mechanisms of FRBs.&rft.creator=Dai, Shi &rft.creator=Hobbs, George &rft.creator=Li, Di &rft.creator=Wang, Pei &rft.creator=Zhang, Lei &rft.creator=Zhu, Weiwei &rft.creator=Feng, Yi &rft.creator=Xue, Mengyao &rft.creator=Yang, Yuanpei &rft.creator=Zhang, YongKun &rft.creator=Niu, Chenhui &rft.creator=Xu, Jiaying &rft.creator=Zhu, Yuhao &rft.creator=Zhang, Jiaheng &rft.date=2025&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 2025.&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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Creative Commons Attribution 4.0 International Licence
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Data is accessible online and may be reused in accordance with licence conditions

All Rights (including copyright) CSIRO 2025.

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We propose a long-term project to monitor a very active repeater, FRB 20190520B, with Murriyang's UWL system. Our previous observations show that FRB 20190520B is not only among the most active FRBs that can be observed with Murriyang, but also shows extreme rotation measure (RM) and dispersion measure (DM) evolution, along with distinctive behavior at 3GHz frequency. This makes the UWL receiver uniquely suited for detailed studies and long-term monitoring of this repeating FRB. Through this program, we anticipate detecting a large sample of bursts from this FRB. In collaboration with FAST, we aim to investigate the time evolution of various properties of FRB 20190520B, enhance our understanding of polarisation across an extremely wide bandwidth with high sensitivity, and gain deeper insights into the local environment and emission mechanisms of FRBs.

Available: 2025-12-21

Data time period: 2025-10-01 to 2026-03-31

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ACN 633 798 857