We report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO’s and Advanced Virgo’s third observing run (O3) combined with upper limits from the earlier O1 and O2 runs. Unlike in previous observing runs in the advanced detector era, we include Virgo in the search for the GWB. The results of the search are consistent with uncorrelated noise, and therefore we place upper limits on the strength of the GWB. We find that the dimensionless energy density Ω GW ≤ 5.8 × 10 − 9 at the 95% credible level for a flat (frequency-independent) GWB, using a prior which is uniform in the log of the strength of the GWB, with 99% of the sensitivity coming from the band 20–76.6 Hz; Ω GW ( f ) ...
We present cosmological parameter results from the final full-mission Planck measurements of the cosm...
To identify common alleles associated with different histotypes of epithelial ovarian cancer (EOC), ...
none243siThe process e+e-→π+π-π0γ is studied at a center-of-mass energy near the D(4S) resonance usi...
We report results of a search for an isotropic gravitational-wave background (GWB) using data from A...
We report results from searches for anisotropic stochastic gravitational-wave backgrounds using data...
We report on the population properties of compact binary mergers inferred from gravitational-wave ob...
This paper presents the results of a search for generic short-duration gravitational-wave transients...
We use 47 gravitational wave sources from the Third LIGO–Virgo–Kamioka Gravitational Wave Detector G...
The gravitational-wave signal GW190521 is consistent with a binary black hole (BBH) merger source at...
We search for signatures of gravitational lensing in the gravitational-wave signals from compact bin...
We present a search for continuous gravitational waves from five radio pulsars, comprising three rec...
We describe a directed search for continuous gravitational waves in data from the sixth initial LIGO...
We present cosmological parameter results from the final full-mission Planck measurements of the cosm...
To identify common alleles associated with different histotypes of epithelial ovarian cancer (EOC), ...
none243siThe process e+e-→π+π-π0γ is studied at a center-of-mass energy near the D(4S) resonance usi...
We report results of a search for an isotropic gravitational-wave background (GWB) using data from A...
We report results from searches for anisotropic stochastic gravitational-wave backgrounds using data...
We report on the population properties of compact binary mergers inferred from gravitational-wave ob...
This paper presents the results of a search for generic short-duration gravitational-wave transients...
We use 47 gravitational wave sources from the Third LIGO–Virgo–Kamioka Gravitational Wave Detector G...
The gravitational-wave signal GW190521 is consistent with a binary black hole (BBH) merger source at...
We search for signatures of gravitational lensing in the gravitational-wave signals from compact bin...
We present a search for continuous gravitational waves from five radio pulsars, comprising three rec...
We describe a directed search for continuous gravitational waves in data from the sixth initial LIGO...
We present cosmological parameter results from the final full-mission Planck measurements of the cosm...
To identify common alleles associated with different histotypes of epithelial ovarian cancer (EOC), ...
none243siThe process e+e-→π+π-π0γ is studied at a center-of-mass energy near the D(4S) resonance usi...