-
1
-
2
A gravitational-wave standard siren measurement of the Hubble constant
Published 2019Get full text
Article -
3
Effects of waveform model systematics on the interpretation of GW150914
Published 2019“…For signals with higher signal-to-noise ratio than GW150914, or in other regions of the binary parameter space (lower masses, larger mass ratios, or higher spins), we expect that systematic errors in current waveform models may impact gravitational-wave measurements, making more accurate models desirable for future observations.…”
Get full text
Article -
4
Calibration of the LIGO gravitational wave detectors in the fifth science run
Published 2015“…The Laser Interferometer Gravitational Wave Observatory (LIGO) is a network of three detectors built to detect local perturbations in the space–time metric from astrophysical sources. These detectors, two in Hanford, WA and one in Livingston, LA, are power-recycled Fabry-Perot Michelson interferometers. …”
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Article -
5
All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
Published 2022“…None of these searches has found clear evidence for a CW signal, so upper limits on the gravitational-wave strain amplitude are calculated, which for this broad range in parameter space are the most sensitive ever achieved.…”
Get full text
Article -
6
All-sky search for periodic gravitational waves in the full S5 LIGO data
Published 2012“…A new detection pipeline utilizing a loosely coherent algorithm was able to follow up weaker outliers, increasing the volume of space where signals can be detected by a factor of 10, but has not revealed any gravitational-wave signals. …”
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Article -
7
Search for Gravitational Waves from a Long-lived Remnant of the Binary Neutron Star Merger GW170817
Published 2022“…Through simulated signals, we quantify that with the current detector sensitivity, nowhere in the studied parameter space are we sensitive to a signal from more than 1 Mpc away, compared to the actual distance of 40 Mpc. …”
Get full text
Article -
8
All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems
Published 2022“…We estimate the sensitivity of the search using simulated continuous wave signals, achieving the most sensitive results to date across the analyzed parameter space.…”
Get full text
Article -
9
-
10
-
11
-
12
All-sky search for continuous gravitational waves from isolated neutron stars in the early O3 LIGO data
Published 2022“…These limits are the most constraining to date over most of the parameter space searched.…”
Get full text
Article -
13
-
14
-
15
-
16
-
17
Directed search for continuous gravitational waves from the Galactic center
Published 2014“…These upper limits are the most constraining to date for a large-parameter-space search for continuous gravitational wave signals.…”
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Article -
18
Constraints on Cosmic Strings from the LIGO-Virgo Gravitational-Wave Detectors
Published 2014“…In particular, if the size of loops is given by the gravitational backreaction scale, we place upper limits on the string tension Gμ below 10[superscript −8] in some regions of the cosmic string parameter space.…”
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Article -
19
-
20