Brief 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.Available: 2021-01-26
Data time period: 2020-10-01 to 2021-03-31
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
P1092_2020OCTS |
Physical Sciences |
neutron stars |
pulsars |
User Contributed Tags
Login to tag this record with meaningful keywords to make it easier to discover
Identifiers
- DOI : 10.25919/A93Q-A322
- Handle : 102.100.100/388689
- URL : data.csiro.au/collection/csiro:48594