Data

Parkes observations for project P885 semester 2022APRS_03

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/zmt1-8s32&rft.title=Parkes observations for project P885 semester 2022APRS_03&rft.identifier=10.25919/zmt1-8s32&rft.publisher=Commonwealth Scientific and Industrial Research Organisation (CSIRO)&rft.description=We request a continued reduced monitoring cadence for the magnetars 1E 1547.0-5408 and Swift J1818.0-1607 at once every 10 days, to track their rotation, flux density, and polarisation. Swift J1818.0-1607 remains very dynamic, and the unique UWL capabilities promise new opportunities to probe still mysterious radio emission mechanisms in magnetars. Our timing results indicate that 1E 1547.0-5408 is currently a more stable rotator, supporting the diminished cadence. We will observe XTE J1810-197 and PSR J1622-4950 less frequently, to complement monitoring elsewhere. The overall request is 18 hours.&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=2022&rft.edition=v1&rft_rights=All Rights (including copyright) CSIRO 2022.&rft_rights=Creative Commons Attribution https://creativecommons.org/licenses/by/4.0/&rft_subject=pulsars, neutron stars&rft_subject=Astronomical and Space Sciences not elsewhere classified&rft_subject=PHYSICAL SCIENCES&rft_subject=ASTRONOMICAL AND SPACE SCIENCES&rft.type=dataset&rft.language=English Access the data

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Creative Commons Attribution
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All Rights (including copyright) CSIRO 2022.

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Brief description

We request a continued reduced monitoring cadence for the magnetars 1E 1547.0-5408 and Swift J1818.0-1607 at once every 10 days, to track their rotation, flux density, and polarisation. Swift J1818.0-1607 remains very dynamic, and the unique UWL capabilities promise new opportunities to probe still mysterious radio emission mechanisms in magnetars. Our timing results indicate that 1E 1547.0-5408 is currently a more stable rotator, supporting the diminished cadence. We will observe XTE J1810-197 and PSR J1622-4950 less frequently, to complement monitoring elsewhere. The overall request is 18 hours.

Data time period: 2022-04-01 to 2022-09-30

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