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Parkes observations for project P885 semester 2020OCTS_16

Commonwealth Scientific and Industrial Research Organisation
Camilo, Fernando ; Johnston, Simon ; Sarkissian, John ; Reynolds, John ; Scholz, Paul ; Lower, Marcus
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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/qv2f-hd25&rft.title=Parkes observations for project P885 semester 2020OCTS_16&rft.identifier=https://doi.org/10.25919/qv2f-hd25&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose to continue observing the magnetars 1E 1547.0?5408 and PSR J1622?4950 weekly, to track their rotation, flux density, and polarisation. The revolutionary UWL capabilities promise new opportunities to disentangle still mysterious radio emission mechanisms in magnetars. This promise is supported by the recent follow up of XTE J1810?197, again a radio magnetar after 10 years dormant, and of the hot-off-the-press magnetar Swift J1818.0?1607, for which our observations with the UWL receiver are providing unique and tantalizing measurements of radio spectrum and polarisation.&rft.creator=Camilo, Fernando &rft.creator=Johnston, Simon &rft.creator=Sarkissian, John &rft.creator=Reynolds, John &rft.creator=Scholz, Paul &rft.creator=Lower, Marcus &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=P885_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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Brief description

We propose to continue observing the magnetars 1E 1547.0?5408 and PSR J1622?4950 weekly, to track their rotation, flux density, and polarisation. The revolutionary UWL capabilities promise new opportunities to disentangle still mysterious radio emission mechanisms in magnetars. This promise is supported by the recent follow up of XTE J1810?197, again a radio magnetar after 10 years dormant, and of the hot-off-the-press magnetar Swift J1818.0?1607, for which our observations with the UWL receiver are providing unique and tantalizing measurements of radio spectrum and polarisation.

Available: 2021-03-03

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

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Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | P885_2020OCTS | Physical Sciences | neutron stars | pulsars |

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