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Optimisation of galaxy identification methods on large interferometric surveys
The astronomical size of spectral data cubes that will result from the SKA pathfinders planned large HI surveys such as LADUMA; Fornax HI survey; DINGO; WALLABY; etc. necessitate fully automated three-dimensional (3D) source finding and parametrization tools. A fraction of the percentage difference...
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| Language: | English |
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Department of Astronomy
2019
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