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 most 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: 2009-04-01 to 2009-09-30
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
Galactic |
Physical Sciences |
Stellar |
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Identifiers
- DOI : 10.4225/08/51F4015458717
- Handle : 102.100.100/6748
- URL : data.csiro.au/collection/csiro:P140-2009APRS
