I. Dave

TL;DR: In this article, two analysis errors have been identified that affect the results for a handful of the high-value pulsars given in Table 1 of Abbott et al. (2019).

TL;DR: In this article , the authors extended the search for lensing signatures to all binary black hole events from the third observing run of the LIGO--Virgo network, and used the nondetection of gravitational-wave lensing to constrain the lensing rate based on the latest merger-rate estimates and the fraction of dark matter composed of compact objects.

TL;DR: In this paper, the PyCBC pipeline is used to search for gravitational wave signals from compact binary coalescences, and it is shown that the removal of noisy data from analysis time can improve the sensitivity of searches for binary coalescence.

TL;DR: In this paper , the authors present a directed search for continuous gravitational wave (CW) signals emitted by spinning neutron stars located in the inner parsecs of the Galactic Center (GC).

TL;DR: In this article, the authors used 47 gravitational-wave sources from the Third LIGO-Virgo-KAGRA Gravitational-Wave Transient Catalog (GWTC-3) to estimate the Hubble parameter $H(z), including its current value, the Hubble constant $H_0.