I. Dave

TL;DR: In this paper, the authors describe the online identification of gravitational wave transients and the distribution of gravitational-wave alerts by the LIGO and Virgo collaborations during O2 and give an overview of the online candidate alerts shared with observing partners.

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 effects of possible systematic errors in the waveform models on estimates of its source parameters were investigated and no evidence for a systematic bias relative to the statistical error of the original parameter recovery of GW150914 due to modeling approximations or modeling inaccuracies was found.

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.