Description
The search for continuous and persistent gravitational waves emitted by isolated and rotating neutron stars is a top priority for current and future ground-based detectors. However, those searches are typically bounded in sensitivity by their high computational costs. In this work, we will show the optimization work done on the Frequency-Hough algorithm, which performs a blind search for unknown sources from any position in the sky. We will also show the status of the extensive testing of the computing infrastructures provided by ICSC.
Author
Lorenzo Pierini
(Istituto Nazionale di Fisica Nucleare)
Co-authors
Pia Astone
(Istituto Nazionale di Fisica Nucleare)
Stefano Dal Pra
(Istituto Nazionale di Fisica Nucleare)
Marco Serra
(Istituto Nazionale di Fisica Nucleare)
Cristiano Palomba
(Istituto Nazionale di Fisica Nucleare)