R. W. P. Drever

TL;DR: In this article, the first low frequency all-sky search of continuous gravitational wave signals was conducted on Virgo VSR2 and VSR4 data and the results of the search covered the full sky, a frequency range between 20 and 128 Hz with a range of spin-down between -1.0×10-10 and +1.5×10 -11 Hz/s.

TL;DR: In this paper, a search for gravitational-wave bursts in data from the three LIGO interferometric detectors during their third science run was reported. But no gravitational-warp signals were detected in the eight days of analysed data.

TL;DR: In this article, the authors apply correlated noise identification and mitigation techniques to data taken by the two LIGO Hanford detectors, H1 and H2, during the fifth science run, and demonstrate techniques that will be useful for future searches using advanced detectors, where correlated noise from global magnetic fields may affect even widely separated detectors.

TL;DR: In this paper, it was shown that pulses of gravitational radiation of less than a few milliseconds duration are too infrequent to account for the signals reported by Weber in 1970, and that the frequency of these pulses is not large enough to explain the signal.

TL;DR: In this paper, the authors present a high-energy neutrino follow-up search for the second GW event, GW151226, as well as for gravitational wave candidate LVT151012.