Full description
This proposal consolidates and concentrates the timing observations ofbinary and millisecond pulsars discovered by us in the Parkes
Multibeam (PKSMB) and high-latitude (PH) surveys. In order to fully
exploit the scientific promises of our discoveries it is essential to
perform continued timing observations. It is crucial that the
observing sessions be spaced at three-to-five week intervals. The
pulsars will be visible during LST 08:30 -- 22:30 and the project
should be scheduled within this interval.
Available: 2013-08-30
Data time period: 2005-10-01 to 2006-09-30
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
Galactic |
Physical Sciences |
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Identifiers
- DOI : 10.4225/08/521FE1362C28B
- Handle : 102.100.100/7300
- URL : data.csiro.au/collection/csiro:P501-2006APRS
