M. Steinke

TL;DR: In this article, the authors reported results of a deep all-sky search for periodic gravitational waves from isolated neutron stars in data from the first Advanced LIGO observing run, where they found no significant signal candidate and set the most stringent upper limits to date on the amplitude of gravitational wave signals from the target population.

TL;DR: In this article, a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSRJ0737-3039A), was presented.

TL;DR: In this article, the authors describe directed searches for continuous gravitational waves in data from the sixth LIGO science data run, where the targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars.

TL;DR: In this article, the authors derived the first constraints on the progenitor of GW170817 at the time of the second supernova (SN) and found these constraints to be comparable to those for Galactic BNS progenitors.

TL;DR: In this paper, the PyCBC pipeline was used to search for gravitational wave signals from compact binary coalescences, and the output of PyCBC was used as a metric for improvement.