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20102026
most citedSensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run

415 citations · 3.2k across the 69 of their papers we have counts for

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Showing 2021Show all

16 papers · 1 filter

astro-ph.IM2021★ 3 cited

The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science

D. Steeghs, D. K. Galloway, K. Ackley +50

The Gravitational-wave Optical Transient Observer (GOTO) is an array of wide-field optical telescopes, designed to exploit new discoveries from the next generation of gravitational…

gr-qc2021★ 29 cited

Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors

Gregory Ashton, Sarah Thiele, Yannick Lecoeuche +2

The two interferometric LIGO gravitational-wave observatories provide the most sensitive data to date to study the gravitational-wave Universe. As part of a global network, they ha…

astro-ph.CO2021★ 20 cited

Does non-stationary noise in LIGO and Virgo affect the estimation of ?

Simone Mozzon, Gregory Ashton, Laura K. Nuttall +1

Gravitational-wave observations of binary neutron star mergers and their electromagnetic counterparts provide an independent measurement of the Hubble constant, , through the…

physics.ins-det2021★ 6 cited

Point Absorber Limits to Future Gravitational-Wave Detectors

W. Jia, H. Yamamoto, K. Kuns +198

High-quality optical resonant cavities require low optical loss, typically on the scale of parts per million. However, unintended micron-scale contaminants on the resonator mirrors…

astro-ph.IM2021

SkyPy: A package for modelling the Universe

Adam Amara, Lucia F. de la Bella, Simon Birrer +18

SkyPy is an open-source Python package for simulating the astrophysical sky. It comprises a library of physical and empirical models across a range of observables and a command-lin…

astro-ph.HE2021★ 10 cited

Searching For Fermi GRB Optical Counterparts With The Prototype Gravitational-Wave Optical Transient Observer (GOTO)

Y. -L. Mong, K. Ackley, D. K. Galloway +45

The typical detection rate of gamma-ray burst (GRB) per day by the \emph{Fermi} Gamma-ray Burst Monitor (GBM) provides a valuable opportunity to further our understanding o…

physics.ins-det2021★ 53 cited

LIGOs Quantum Response to Squeezed States

L. McCuller, S. E. Dwyer, A. C. Green +194

Gravitational Wave interferometers achieve their profound sensitivity by combining a Michelson interferometer with optical cavities, suspended masses, and now, squeezed quantum sta…

astro-ph.IM2021★ 30 cited

Light curve classification with recurrent neural networks for GOTO: dealing with imbalanced data

U. F. Burhanudin, J. R. Maund, T. Killestein +42

The advent of wide-field sky surveys has led to the growth of transient and variable source discoveries. The data deluge produced by these surveys has necessitated the use of machi…

astro-ph.IM2021★ 3 cited

Processing GOTO data with the Rubin Observatory LSST Science Pipelines II: Forced Photometry and light curves

L. Makrygianni, J. Mullaney, V. Dhillon +45

We have adapted the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Science Pipelines to process data from the Gravitational-Wave Optical Transient Observer (GOTO)…

astro-ph.IM2021★ 40 cited

Transient-optimised real-bogus classification with Bayesian Convolutional Neural Networks -- sifting the GOTO candidate stream

T. L. Killestein, J. Lyman, D. Steeghs +45

Large-scale sky surveys have played a transformative role in our understanding of astrophysical transients, only made possible by increasingly powerful machine learning-based filte…

astro-ph.SR2021★ 21 cited

Evidence that short period AM CVn systems are diverse in outburst behaviour

C. Duffy, G. Ramsay, D. Steeghs +12

We present results of our analysis of up to 15 years of photometric data from eight AM CVn systems with orbital periods between 22.5 and 26.8 min. Our data has been collected from…

quant-ph2021★ 96 cited

Approaching the motional ground state of a 10 kg object

Chris Whittle, Evan D. Hall, Sheila Dwyer +197

The motion of a mechanical object -- even a human-sized object -- should be governed by the rules of quantum mechanics. Coaxing them into a quantum state is, however, difficult: th…

astro-ph.IM2021★ 233 cited

LIGO Detector Characterization in the Second and Third Observing Runs

D. Davis, J. S. Areeda, B. K. Berger +284

The characterization of the Advanced LIGO detectors in the second and third observing runs has increased the sensitivity of the instruments, allowing for a higher number of detecta…

astro-ph.IM2021★ 72 cited

Environmental Noise in Advanced LIGO Detectors

P. Nguyen, R. M. S. Schofield, A. Effler +215

The sensitivity of the Advanced LIGO detectors to gravitational waves can be affected by environmental disturbances external to the detectors themselves. Since the transition from…

astro-ph.IM2021★ 26 cited

The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation

O Edy, A. Lundgren, L. K. Nuttall

Bayesian inference is used to extract unknown parameters from gravitational wave signals. Detector noise is typically modelled as stationary, although data from the LIGO and Virgo…

physics.ins-det2021★ 49 cited

Point absorbers in Advanced LIGO

Aidan F. Brooks, Gabriele Vajente, Hiro Yamamoto +198

Small, highly absorbing points are randomly present on the surfaces of the main interferometer optics in Advanced LIGO. The resulting nano-meter scale thermo-elastic deformations a…