4 pages, 3 figures, proceedings of the ADASS XXX (2020) conference, to appear in ASP Conference SeriesInternational audienceThe next generation of radio telescopes, such as the Square Kilometer Array (SKA), will need to process an incredible amount of data in real-time. In addition, the sensitivity of SKA will require a new generation of calibration and imaging software to exploit its full potential. The wide-field direction-dependent spectral deconvolution framework, called DDFacet, has already been successfully used in several existing SKA pathfinders like MeerKAT. DDFacet has been developed and optimized for single node HPC systems. DDFacet is a good candidate for being integrated in the SKA computing pipeline and should therefore be run...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
Imaging is considered the most compute-intensive and therefore most challenging part of a radio-astr...
Large collecting area single dish telescope such as ATLAST will be especially effective for medium (...
4 pages, 3 figures, proceedings of the ADASS XXX (2020) conference, to appear in ASP Conference Seri...
International audienceThe next generation of radio telescopes, such as the Square Kilometer Array (S...
International audienceThe next generation of radio telescopes, such as the Square Kilometer Array (S...
International audienceABSTRACT In the era of big data, radio astronomical image reconstruction algor...
A giant distributed radio telescope is an unusual kind of massive parallel computing system. The des...
The new generation of radio interferometers is characterized by high sensitivity, wide fields of vie...
tionizing the way remotely sensed data is collected, managed and analyzed. The incorporation of late...
The Square Kilometre Array (SKA) will be both the largest radio telescope ever constructed and the l...
The Square Kilometre Array (SKA) will be both the largest radio telescope ever constructed and the l...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
Imaging is considered the most compute-intensive and therefore most challenging part of a radio-astr...
Large collecting area single dish telescope such as ATLAST will be especially effective for medium (...
4 pages, 3 figures, proceedings of the ADASS XXX (2020) conference, to appear in ASP Conference Seri...
International audienceThe next generation of radio telescopes, such as the Square Kilometer Array (S...
International audienceThe next generation of radio telescopes, such as the Square Kilometer Array (S...
International audienceABSTRACT In the era of big data, radio astronomical image reconstruction algor...
A giant distributed radio telescope is an unusual kind of massive parallel computing system. The des...
The new generation of radio interferometers is characterized by high sensitivity, wide fields of vie...
tionizing the way remotely sensed data is collected, managed and analyzed. The incorporation of late...
The Square Kilometre Array (SKA) will be both the largest radio telescope ever constructed and the l...
The Square Kilometre Array (SKA) will be both the largest radio telescope ever constructed and the l...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
Imaging is considered the most compute-intensive and therefore most challenging part of a radio-astr...
Large collecting area single dish telescope such as ATLAST will be especially effective for medium (...