Brief description
We request a reduced monitoring cadence for the magnetars 1E 1547.0-5408 and Swift J1818.0-1607 to 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: 2021-10-01 to 2022-03-31
Subjects
Astronomical and Space Sciences |
Astronomical and Space Sciences Not Elsewhere Classified |
Physical Sciences |
pulsars, neutron stars |
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Identifiers
- Local : 102.100.100/433949
- DOI : 10.25919/h1jb-b741