Abstract
For next-generation radio telescopes such as the Square Kilometre Array, seemingly minor changes in scientific constraints can easily push computing requirements into the exascale domain. The authors propose a model for engineers and astronomers to understand these relations and make tradeoffs in future instrument designs.
| Original language | English |
|---|---|
| Pages (from-to) | 48-54 |
| Journal | Computer |
| Volume | 47 |
| Issue number | 9 |
| DOIs | |
| Publication status | Published - 2014 |
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