Data

Parkes observations for project P1306 semester 2023OCTS_01

Commonwealth Scientific and Industrial Research Organisation
Zhou, lu ; Liu, Xiaojin
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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:doi10.25919/96mg-1e43&rft.title=Parkes observations for project P1306 semester 2023OCTS_01&rft.identifier=https://doi.org/10.25919/96mg-1e43&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Magnetars are neutron stars with intense magnetic fields that undergo rapid rotation. The observation of their radio pulses carries great scientific significance. With the high sensitivity and wide frequency coverage of the Parkes telescope, we propose to search for radio pulse signals of the magnetar SGR J1833-0832 and (if detected) conduct a detailed analysis of its pulse characteristics, radio flux density, and polarization. This project will contribute significantly to advancing our understanding of magnetars' magnetic field structure, radiation mechanisms, and polarization phenomena.&rft.creator=Zhou, lu &rft.creator=Liu, Xiaojin &rft.date=2024&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 2024.&rft_subject=pulsars&rft_subject=neutron stars&rft_subject=magnetic fields&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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Magnetars are neutron stars with intense magnetic fields that undergo rapid rotation. The observation of their radio pulses carries great scientific significance. With the high sensitivity and wide frequency coverage of the Parkes telescope, we propose to search for radio pulse signals of the magnetar SGR J1833-0832 and (if detected) conduct a detailed analysis of its pulse characteristics, radio flux density, and polarization. This project will contribute significantly to advancing our understanding of magnetars' magnetic field structure, radiation mechanisms, and polarization phenomena.

Available: 2024-01-10

Data time period: 2023-10-01 to 2024-03-31

Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Physical Sciences | magnetic fields | neutron stars | pulsars |

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Identifiers
ACN 633 798 857