Search Results for author: Huihuo Zheng

Found 5 papers, 2 papers with code

AI ensemble for signal detection of higher order gravitational wave modes of quasi-circular, spinning, non-precessing binary black hole mergers

1 code implementation29 Sep 2023 Minyang Tian, E. A. Huerta, Huihuo Zheng

We used this ensemble, 3 classifiers for signal detection and 2 total mass predictors, to process a year-long test set in which we injected 300, 000 signals.

Transfer Learning

Physics-inspired spatiotemporal-graph AI ensemble for gravitational wave detection

no code implementations27 Jun 2023 Minyang Tian, E. A. Huerta, Huihuo Zheng

Finally, when we distributed AI inference over 128 GPUs in the Polaris supercomputer and 128 nodes in the Theta supercomputer, our AI ensemble is capable of processing a decade of gravitational wave data from a three detector network within 3. 5 hours.

Gravitational Wave Detection

Inference-optimized AI and high performance computing for gravitational wave detection at scale

no code implementations26 Jan 2022 Pranshu Chaturvedi, Asad Khan, Minyang Tian, E. A. Huerta, Huihuo Zheng

We introduce an ensemble of artificial intelligence models for gravitational wave detection that we trained in the Summit supercomputer using 32 nodes, equivalent to 192 NVIDIA V100 GPUs, within 2 hours.

Gravitational Wave Detection

Interpretable AI forecasting for numerical relativity waveforms of quasi-circular, spinning, non-precessing binary black hole mergers

no code implementations13 Oct 2021 Asad Khan, E. A. Huerta, Huihuo Zheng

Our findings show that artificial intelligence can accurately forecast the dynamical evolution of numerical relativity waveforms in the time range $t\in[-100\textrm{M}, 130\textrm{M}]$.

Deep Learning at Scale for the Construction of Galaxy Catalogs in the Dark Energy Survey

2 code implementations5 Dec 2018 Asad Khan, E. A. Huerta, Sibo Wang, Robert Gruendl, Elise Jennings, Huihuo Zheng

Furthermore, we use our neural network model as a feature extractor for unsupervised clustering and find that unlabeled DES images can be grouped together in two distinct galaxy classes based on their morphology, which provides a heuristic check that the learning is successfully transferred to the classification of unlabelled DES images.

Clustering

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