A plan has been developed to incorporate the various projects I have worked on over the duration of my degree to complete an effective thesis useful for future work. Correlator design is a key component to modern radio astronomy. Large-N and large bandwidth designs are an important subject for SKA array development. A station correlator for the LOFAR station at Chilbolton Observatory is currently under going design and deployment is planned for the next year. Using this design as a model an FPGA based SKA Phase I correlator design will be examined and compared to competing technologies.
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
Figures 2-12 and 2-17 are re-used under CC BY-NC 4.0 International & CC 3.0 Unported Licences respec...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
Low frequency radio astronomy has entered a second golden age driven by the development of a new cla...
Low frequency radio astronomy has entered a second golden age driven by the development of a new cla...
Low frequency radio astronomy has entered a second golden age driven by the development of a new cla...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
Multi-element radio telescopes employ methods of indirect imaging to capture the image of the sky. T...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
Radio telescopes that employ arrays of many antennas are in operation, and ever larger ones are bein...
Radio astronomical imaging arrays comprising large numbers of antennas, O(102-103) have posed a sign...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
The maximum signal bandwidth on the Australia Telescope Compact Array (ATCA) is to expand from 128MH...
ISBN: 9780819491534International audienceTwo large correlators have been constructed to combine the ...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
Figures 2-12 and 2-17 are re-used under CC BY-NC 4.0 International & CC 3.0 Unported Licences respec...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
Low frequency radio astronomy has entered a second golden age driven by the development of a new cla...
Low frequency radio astronomy has entered a second golden age driven by the development of a new cla...
Low frequency radio astronomy has entered a second golden age driven by the development of a new cla...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
Multi-element radio telescopes employ methods of indirect imaging to capture the image of the sky. T...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
Radio telescopes that employ arrays of many antennas are in operation, and ever larger ones are bein...
Radio astronomical imaging arrays comprising large numbers of antennas, O(102-103) have posed a sign...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
The maximum signal bandwidth on the Australia Telescope Compact Array (ATCA) is to expand from 128MH...
ISBN: 9780819491534International audienceTwo large correlators have been constructed to combine the ...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...
Figures 2-12 and 2-17 are re-used under CC BY-NC 4.0 International & CC 3.0 Unported Licences respec...
A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Unit...