A Curvature‐compensated Corrector for Drift‐Scan Observations

Images obtained by drift‐scanning with a stationary telescope are affected by the declination‐dependent curvature of star trails. The image displacement due to curvature and drift‐rate variation increases with the angular field of view and can lead to significant loss of resolution with modern large‐format CCD arrays. We show that these effects can be essentially eliminated by means of an optical corrector design in which individual lenses are tilted and decentered. A specific example is presented of a four‐element corrector designed for the Large‐Zenith Telescope. The design reduces curvature errors to less than 0 074 over a 10 ' × 20 ' field of view centered at 49° declination. By changing the positions and tilts of the lenses, the same design can also be used for any field centers between 0° and ±49°.