Search
Now showing items 1-1 of 1
Implementation of a goodness-of-fit test for finding optimal concurrent radio and γ-ray pulsar light curves
(SAIP, 2015)
Since the launch of the Fermi Large Area Telescope in 2008 the number of known
γ-ray pulsars has increased immensely to over 200, many of which are also visible in the
radio and X-ray bands. Seyffert et al. (2011) ...