no code implementations • 16 Feb 2024 • Ahab Isaac, Wesley Armour, Karel Adámek
Accurate modelling of spectra produced by X-ray sources requires the use of Monte-Carlo simulations.
no code implementations • 13 Sep 2020 • Karel Adámek, Jan Novotný, Jeyarajan Thiyagalingam, Wesley Armour
We demonstrate how these results can be used to lower the power consumption of existing data processing pipelines.
Performance C.4
4 code implementations • 6 Dec 2018 • Karel Adámek, Wesley Armour
Time-domain radio astronomy utilizes a harmonic sum algorithm as part of the Fourier domain periodicity search, this type of search is used to discover single pulsars.
Instrumentation and Methods for Astrophysics
4 code implementations • 29 Nov 2017 • Karel Adámek, Sofia Dimoudi, Mike Giles, Wesley Armour
Our new improved convolution code which uses our custom GPU FFT code is between 2. 5 and 3. 9 times faster the than our cuFFT-based implementation (on an NVIDIA P100) and allows for a wider range of filter sizes then our previous version.
Instrumentation and Methods for Astrophysics
3 code implementations • 29 Nov 2016 • Karel Adámek, Wesley Armour
This code is part of the AstroAccelerate project which is a many-core accelerated time-domain signal processing code for radio astronomy.
Instrumentation and Methods for Astrophysics
4 code implementations • 23 Nov 2015 • Sofia Dimoudi, Wesley Armour
Pulsar acceleration searches are methods for recovering signals from radio telescopes, that may otherwise be lost due to the effect of orbital acceleration in binary systems.
Instrumentation and Methods for Astrophysics