F. Clara

TL;DR: In this article, the authors presented the results of a weakly modeled burst search for gravitational waves from mergers of non-spinning intermediate mass black holes (IMBH) in the total mass range 100--450 solar masses and with the component mass ratios between 1:1 and 4:1.

TL;DR: In this article, the authors used a linear search grid to analyse GRB events with large sky localisation uncertainties such as the localisations provided by the Fermi Gamma-ray Burst Monitor (GBM).

TL;DR: In this article, the authors describe directed searches for continuous gravitational waves (GWs) from 16 well-localized candidate neutron stars, assuming none of the stars has a binary companion.

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.