FinGraV reconstructs fine-grain GPU power profiles for sub-millisecond AI kernels by synchronizing CPU-GPU clocks, binning execution times, and separating steady-state execution from steady-state power.
Cutting the cost of pulsar astronomy: Saving time and energy when searching for binary pulsars using NVIDIA GPUs
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abstract
Using the Fourier Domain Acceleration Search (FDAS) method to search for binary pulsars is a computationally costly process. Next generation radio telescopes will have to perform FDAS in real time, as data volumes are too large to store. FDAS is a matched filtering approach for searching time-domain radio astronomy datasets for the signatures of binary pulsars with approximately linear acceleration. In this paper we will explore how we have reduced the energy cost of an SKA-like implementation of FDAS in AstroAccelerate, utilising a combination of mixed-precision computing and dynamic frequency scaling on NVIDIA GPUs. Combining the two approaches, we have managed to save 58% of the overall energy cost of FDAS with a (<3%) sacrifice in numerical sensitivity.
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FinGraV: Methodology for Fine-Grain GPU Power Visibility and Insights
FinGraV reconstructs fine-grain GPU power profiles for sub-millisecond AI kernels by synchronizing CPU-GPU clocks, binning execution times, and separating steady-state execution from steady-state power.