F. Clara

TL;DR: In this paper, the authors proposed a 3G detector for the LIGO and Virgo observatories, which would have a 10-fold improvement in strain sensitivity over the current generation of instruments, yielding signal-to-noise ratios of 1000 for events like those already seen.

TL;DR: In this article, the expected surface deformation from point absorbers and the impact on power build-up in second generation GW detectors (dual-recycled Fabry-Perot Michelson interferometers) was analyzed and it was shown that the power-dependent reduction in interferometer performance will significantly degrade maximum stored power by up to 50%.

TL;DR: In this article, the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015 are presented.

TL;DR: In this article, the Weave semi-coherent method was used to search for continuous gravitational waves from the neutron stars in the Cassiopeia A (Cas A) and Vela Jr. supernova remnants.

TL;DR: In this article , the authors presented results of an all-sky search for continuous gravitational waves which can be produced by spinning neutron stars with an asymmetry around their rotation axis, using data from the third observing run of the Advanced LIGO and Advanced Virgo detectors.