Cody Messick

TL;DR: After searching data from the first observation run of the advanced LIGO detectors for signals at twice the rotational frequency of 200 known pulsars, no evidence of gravitational waves of any polarization is found.

TL;DR: In this article, the authors presented a search for gravitational waves from 222 pulsars with rotation frequencies ≳10 Hz using advanced LIGO data from its first and second observing runs spanning 2015-2017, which provides the highest-sensitivity gravitational-wave data so far obtained.

TL;DR: In this article, the authors present results from a search for gravitational-wave bursts coincident with a set of two core-collapse supernovae observed between 2007 and 2011, and present the probability of detecting signals from both astrophysically well-motivated and more speculative gravitational wave emission mechanisms as a function of distance from Earth.

TL;DR: The results from an all-sky search for short-duration gravitational waves in the data of the first run of the Advanced LIGO detectors between September 2015 and January 2016 are presented in this article.

TL;DR: In this paper, the authors revisited the binary neutron star coalescence GW170817 and focused on longer signal durations, up until the end of the second Advanced LIGO-Virgo observing run, which was 8.5 days after the coalescence.