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This is usually referred to in astronomy as the "drift scan" technique, and has actually been used with ground-based telescopes since the early 1980s (e.g., McGraw, Angel, & Sargent 1980, Wright & Mackay 1981). Gibson & Hickson (1992) have a summary of work done in the 1980s and early 1990s in the Introduction section of their paper; ...


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