M. Kramer, B. Klein, D. R. Lorimer, P. Mueller, A. Jessner, R. Wielebinski
Abstract
We report the status of a search for pulsars in the Galactic Centre, using a completely revised and improved high-sensitivity double-horn system at 4.85-GHz. We also present calculations about the success rate of periodicity searches for such a survey, showing that in contrast to conclusions in recent literature pulsars can be indeed detected at the chosen search frequency.