Full description
By continuing our brief but intense observations of PSR J0437-4715, we intend to further increase our sensitivity to long-term effects such as the structure of the ISM, receiver stability and orbital period variations (which translate into a precise kinematic distance). At the same time, these campaigns will help improve calibration methods and debug new observing systems.Available: 2013-07-28
Data time period: 2009-10-01 to 2010-03-31
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
Physical Sciences |
neutron stars |
pulsars |
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Identifiers
- DOI : 10.4225/08/51F4225532C8A
- Handle : 102.100.100/6747
- URL : data.csiro.au/collection/csiro:P140-2009OCTS
