Data

Parkes observations for project P1092 semester 2020OCTS_13

Commonwealth Scientific and Industrial Research Organisation
Xue, Mengyao ; Hobbs, George ; Li, Di ; Cameron, Andrew ; Wang, Jingbo ; Wang, Na ; Wang, Pei ; Zhu, Weiwei ; Miao, Chenchen ; Wang, Shuangqiang ; Luo, Rui ; Niu, Jiarui
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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:doi10.25919/4q1q-5794&rft.title=Parkes observations for project P1092 semester 2020OCTS_13&rft.identifier=https://doi.org/10.25919/4q1q-5794&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose to use the Parkes UWL receiver for confirmation and monitoring a sub-set of bright FAST-discovered pulsars, especially for those discoveries located outside the sky regions covered by the purchased PX-500 project. For special FAST discoveries that already confirmed by Parkes, such as MSPs or pulsars with interesting emission properties, we propose to do long-term monitoring for them as well. These monitoring aim to solve their parameters, binary orbit, and provide significant insight into the special emission properties of these new discoveries and facilitate science. The Parkes UWL system provides a unique capability for studying the pulsars over wide bandwidths, in term of both the timing precision and frequency-dependent observing properties.&rft.creator=Xue, Mengyao &rft.creator=Hobbs, George &rft.creator=Li, Di &rft.creator=Cameron, Andrew &rft.creator=Wang, Jingbo &rft.creator=Wang, Na &rft.creator=Wang, Pei &rft.creator=Zhu, Weiwei &rft.creator=Miao, Chenchen &rft.creator=Wang, Shuangqiang &rft.creator=Luo, Rui &rft.creator=Niu, Jiarui &rft.date=2021&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=P1092_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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Data is accessible online and may be reused in accordance with licence conditions

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We propose to use the Parkes UWL receiver for confirmation and monitoring a sub-set of bright FAST-discovered pulsars, especially for those discoveries located outside the sky regions covered by the purchased PX-500 project. For special FAST discoveries that already confirmed by Parkes, such as MSPs or pulsars with interesting emission properties, we propose to do long-term monitoring for them as well. These monitoring aim to solve their parameters, binary orbit, and provide significant insight into the special emission properties of these new discoveries and facilitate science. The Parkes UWL system provides a unique capability for studying the pulsars over wide bandwidths, in term of both the timing precision and frequency-dependent observing properties.

Available: 2021-03-12

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

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Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | P1092_2020OCTS | Physical Sciences | neutron stars | pulsars |

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