370 citations · 1.6k across the 27 of their papers we have counts for
8 papers · 1 filter
Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
Nancy Aggarwal, Odylio D. Aguiar, Diego Blas +34
The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges…
The Virgo O3 run and the impact of the environment
F. Acernese, M. Agathos, A. Ain +486
Sources of geophysical noise (such as wind, sea waves and earthquakes) or of anthropogenic noise impact ground-based gravitational-wave interferometric detectors, causing transient…
Direct limits for scalar field dark matter from a gravitational-wave detector
Sander M. Vermeulen, Philip Relton, Hartmut Grote +20
The nature of dark matter remains unknown to date; several candidate particles are being considered in a dynamically changing research landscape. Scalar field dark matter is a prom…
Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
N. Aggarwal, O. D. Aguiar, A. Bauswein +22
The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges…
Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
Shreejit Jadhav, Nikhil Mukund, Bhooshan Gadre +2
We present a novel Machine Learning (ML) based strategy to search for binary black hole (BBH) mergers in data from ground-based gravitational wave (GW) observatories. This is the f…
Bilinear noise subtraction at the GEO 600 observatory
Nikhil Mukund, James Lough, Christoph Affeldt +8
Longitudinal control signals used to keep gravitational wave detectors at a stable operating point are often affected by modulations from test mass misalignments leading to an elev…
Limiting the effects of earthquakes on gravitational-wave interferometers
Michael Coughlin, Paul Earle, Jan Harms +9
Ground-based gravitational wave interferometers such as the Laser Interferometer Gravitational-wave Observatory (LIGO) are susceptible to high-magnitude teleseismic events, which c…
Towards a first design of a Newtonian-noise cancellation system for Advanced LIGO
Michael Coughlin, Nikhil Mukund, Jan Harms +3
Newtonian gravitational noise from seismic fields is predicted to be a limiting noise source at low frequency for second generation gravitational-wave detectors. Mitigation of this…