S. J. Chamberlin

TL;DR: In this paper, the authors presented the results of a search for gravitational wave bursts with memory (BWMs) using the first five years of NANOGrav observations, and set upper limits on the rate at which BWMs of various amplitudes could have occurred during the time spanned by their data.

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.