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20002024
most citedWALLABY -- An SKA Pathfinder HI Survey

230 citations · 1.4k across the 49 of their papers we have counts for

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Showing 2010 · astro-ph.IMShow all

9 papers · 2 filters

astro-ph.IM2010★ 2 cited

Distributed GPU Volume Rendering of ASKAP Spectral Data Cubes

A. H. Hassan, C. J. Fluke, D. G. Barnes

The Australian SKA Pathfinder (ASKAP) will be producing 2.2 terabyte HI spectral-line cubes for each 8 hours of observation by 2013. Global views of spectral data cubes are vital f…

astro-ph.IM2010★ 4 cited

Visualisation and Analysis Challenges for WALLABY

Christopher J. Fluke, David G. Barnes, Amr H. Hassan

Visualisation and analysis of terabyte-scale datacubes, as will be produced with the Australian Square Kilometre Array Pathfinder (ASKAP), will pose challenges for existing astrono…

astro-ph.IM2010★ 36 cited

Astrophysical Supercomputing with GPUs: Critical Decisions for Early Adopters

Christopher J. Fluke, David G. Barnes, Benjamin R. Barsdell +1

General purpose computing on graphics processing units (GPGPU) is dramatically changing the landscape of high performance computing in astronomy. In this paper, we identify and inv…

astro-ph.IM2010★ 14 cited

Interactive Visualization of the Largest Radioastronomy Cubes

A. H. Hassan, C. J. Fluke, D. G. Barnes

3D visualization is an important data analysis and knowledge discovery tool, however, interactive visualization of large 3D astronomical datasets poses a challenge for many existin…

astro-ph.IM2010★ 32 cited

Analysing Astronomy Algorithms for GPUs and Beyond

Benjamin R. Barsdell, David G. Barnes, Christopher J. Fluke

Astronomy depends on ever increasing computing power. Processor clock-rates have plateaued, and increased performance is now appearing in the form of additional processor cores on…

astro-ph.IM2010★ 51 cited

Computational advances in gravitational microlensing: a comparison of CPU, GPU, and parallel, large data codes

N. F. Bate, C. J. Fluke, B. R. Barsdell +2

To assess how future progress in gravitational microlensing computation at high optical depth will rely on both hardware and software solutions, we compare a direct inverse ray-sho…

astro-ph.IM2010

GPU-Based Volume Rendering of Noisy Multi-Spectral Astronomical Data

Amr H. Hassan, Christopher J. Fluke, David G. Barnes

Traditional analysis techniques may not be sufficient for astronomers to make the best use of the data sets that current and future instruments, such as the Square Kilometre Array…

astro-ph.IM2010

Advanced Architectures for Astrophysical Supercomputing

Benjamin R. Barsdell, David G. Barnes, Christopher J. Fluke

Astronomers have come to rely on the increasing performance of computers to reduce, analyze, simulate and visualize their data. In this environment, faster computation can mean mor…

astro-ph.IM2010★ 4 cited

Visualization-Directed Interactive Model-Fitting to Spectral Data Cubes

Christopher J. Fluke, Jayanne English, David G. Barnes

Spectral datasets obtained at radio frequencies and optical/IR wavelengths are increasing in complexity as new facilities and instruments come online, resulting in an increased nee…