I. Dave

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: Abbott et al. as mentioned in this paper compared the four probability sky maps produced for the gravitational-wave transient GW150914, and provided additional details of the EM follow-up observations that were performed in the different bands.

TL;DR: In this paper, the results from a search for gravitational-wave transients associated with core-collapse supernovae observed within a source distance of approximately 20 Mpc during the first and second observing runs of Advanced LIGO and Advanced Virgo were presented.

TL;DR: In this paper, an all-sky search for gravitational waves (GWs) from merging intermediate mass black hole binaries (IMBHBs) was performed. But no GWs from IMBHB were detected; therefore, the most stringent limit was obtained for black holes of individual mass 100 ǫ m⊙, with spins aligned with the binary orbital angular momentum.

TL;DR: In this article, the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo were presented.