D. C. Vander-Hyde

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 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: This work analyzes the impact of a proposed tidal instability coupling p modes and g modes within neutron stars on GW170817 and finds that the observed signal is consistent with waveform models that neglect p-g effects, with lnB_{!pg}^{pg}=0.03_{-0.58}^{+0.70} (maximum a posteriori and 90% credible region).