The polarization of Rotating Radio Transients

Details The polarization of Rotating Radio Transients The polarization of Rotating Radio Transients

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop.1033k&link_type=abstract

ATNF proposal P584, Semester: October, 2007

Physics

Galactic, Parkes

Scientific paper

We propose to continue using the baseband recorder CPSR2 during the regular monitoring of Rotating Radio Transients at the Parkes telescope, to measure the polarization of as many of these sources as we can at the various monitoring frequencies (50, 20 and 10 cm). The purpose of our observations is to use the polarization measurements to better characterize the relationship of this type of object to the well known radio pulsars. We are in contact with the team proposing and carrying out the RRAT monitoring and therefore are requiring no additional telescope time.

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