G. M. Guidi

TL;DR: In this article, the authors describe directed searches for continuous gravitational waves from sixteen well localized candidate neutron stars assuming none of the stars has a binary companion, and set upper limits on intrinsic gravitational wave strain as strict as $1\times10^{-25}, on fiducial neutron star ellipticity as strong as $2\times 10^{-9}, and on fiducial $r$-mode amplitude as tight as $3 \times 10-8}.

TL;DR: In this paper, the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data are presented.

TL;DR: In this article, the authors present the results of a search for BBH mergers that inspiral in eccentric orbits using data from the first and second observing runs (O1 and O2) of Advanced LIGO and Advanced Virgo.

TL;DR: In this article, a search for continuous gravitational waves emitted by neutron stars in binary systems in early data from the third observing run of the Advanced LIGO and Advanced Virgo detectors using the semicoherent, GPU-accelerated, binaryskyhough pipeline is presented.

TL;DR: In this article, the authors presented a semi-coherent analysis of 10 days of LIGO S5 data ranging from 50-550 Hz, and performed an incoherent sum of coherent power distributed amongst frequency-modulated orbital sidebands.