P. J. Sutton
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View article: Evolution of human cognition required Einstein's gravitational waves
Evolution of human cognition required Einstein's gravitational waves Open
We describe an unexpected anthropic fine-tuning of gravity: human cognition arose on Earth only because the laws of gravity included gravitational waves. Their link is the heat from decays of the radioactive isotopes U-238 and Th-232, whic…
View article: Title Pending
Title Pending Open
View article: Toward real-time detection of unmodeled gravitational wave transients using convolutional neural networks
Toward real-time detection of unmodeled gravitational wave transients using convolutional neural networks Open
Convolutional neural networks (CNNs) have demonstrated potential for the real-time analysis of data from gravitational wave detector networks for the specific case of signals from coalescing compact-object binaries such as black-hole binar…
View article: GWSkyNet. II. A Refined Machine-learning Pipeline for Real-time Classification of Public Gravitational Wave Alerts
GWSkyNet. II. A Refined Machine-learning Pipeline for Real-time Classification of Public Gravitational Wave Alerts Open
Electromagnetic follow-up observations of gravitational wave events offer critical insights and provide significant scientific gain from this new class of astrophysical transients. Accurate identification of gravitational wave candidates a…
View article: GWSkyNet II : a refined machine learning pipeline for real-time classification of public gravitational wave alerts
GWSkyNet II : a refined machine learning pipeline for real-time classification of public gravitational wave alerts Open
Electromagnetic follow-up observations of gravitational wave events offer critical insights and provide significant scientific gain from this new class of astrophysical transients. Accurate identification of gravitational wave candidates a…
View article: Applications of Deep Learning to physics workflows
Applications of Deep Learning to physics workflows Open
Modern large-scale physics experiments create datasets with sizes and streaming rates that can exceed those from industry leaders such as Google Cloud and Netflix. Fully processing these datasets requires both sufficient compute power and …
View article: Real-Time Detection of Unmodeled Gravitational-Wave Transients UsingConvolutional Neural Networks
Real-Time Detection of Unmodeled Gravitational-Wave Transients UsingConvolutional Neural Networks Open
Convolutional Neural Networks (CNNs) have demonstrated potential for the real-time analysis of data from gravitational-wave detector networks for the specific case of signals from coalescing compact-object binaries such as black-hole binar…
View article: Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks
Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks Open
Convolutional Neural Networks (CNNs) have demonstrated potential for the real-time analysis of data from gravitational-wave detector networks for the specific case of signals from coalescing compact-object binaries such as black-hole binar…
View article: Real-Time Detection of Unmodelled Gravitational-Wave Transients Using\n Convolutional Neural Networks
Real-Time Detection of Unmodelled Gravitational-Wave Transients Using\n Convolutional Neural Networks Open
Convolutional Neural Networks (CNNs) have demonstrated potential for the\nreal-time analysis of data from gravitational-wave detector networks for the\nspecific case of signals from coalescing compact-object binaries such as\nblack-hole bi…
View article: The optical afterglow of the short gamma-ray burst associated with GW170817
The optical afterglow of the short gamma-ray burst associated with GW170817 Open
View article: The optical afterglow of the short gamma-ray burst associated with GW170817
The optical afterglow of the short gamma-ray burst associated with GW170817 Open
The binary neutron star merger GW170817 was the first multi-messenger event observed in both gravitational and electromagnetic waves. The electromagnetic signal began approximately 2 seconds post-merger with a weak, short burst of gamma-ra…
View article: The Environment of the Binary Neutron Star Merger GW170817
The Environment of the Binary Neutron Star Merger GW170817 Open
We present Hubble Space Telescope ( HST ) and Chandra imaging, combined with Very Large Telescope MUSE integral field spectroscopy of the counterpart and host galaxy of the first binary neutron star merger detected via gravitational-wave e…
View article: The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars
The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars Open
We report the discovery and monitoring of the near-infrared counterpart (AT2017gfo) of a binary neutron-star merger event detected as a gravitational wave source by Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo …
View article: Observing gravitational waves from core-collapse supernovae in the advanced detector era
Observing gravitational waves from core-collapse supernovae in the advanced detector era Open
The next galactic core-collapse supernova (CCSN) has already exploded, and its electromagnetic (EM)
\nwaves, neutrinos, and gravitational waves (GWs) may arrive at any moment. We present an extensive study
\non the potential sensitivity of…
View article: Cost–benefit analysis for commissioning decisions in GEO 600
Cost–benefit analysis for commissioning decisions in GEO 600 Open
Gravitational wave interferometers are complex instruments, requiring years\nof commissioning to achieve the required sensitivities for the detection of\ngravitational waves, of order 10^-21 in dimensionless detector strain, in the\ntens o…