Full description
We request time to observe 160 pulsars on a regular basis in\rorder to provide accurate ephemerides necessary for the detection\r
of gamma-ray pulsars with the GLAST and AGILE satellites.\r
The main science goals are to increase the number\r
of known gamma-ray pulsars (both radio loud and radio quiet), to determine\r
accurate pulse profiles, to characterise their high energy spectra and\r
phase resolved spectroscopy of the brightest pulsars.\r
In the radio, the observations will also allow us to find glitches, \r
characterise timing noise, investigate dispersion and rotation measure \r
variability and enhance our knowledge of single pulse phenomenology.\r
We expect this program to continue for the ~5 years of the\r
GLAST and AGILE missions.
Available: 2013-09-08
Data time period: 2008-10-01 to 2009-03-31
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
Galactic |
Physical Sciences |
Stellar |
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Identifiers
- DOI : 10.4225/08/522BC340BCFFE
- Handle : 102.100.100/7405
- URL : data.csiro.au/collection/csiro:P574-2008OCTS
