A new strategy for deep wide-field high-resolution optical imaging

We propose a new strategy for obtaining enhanced-resolution (FWHM similar o r equal to 0 ".12) deep optical images over a wide field of view. As is wel l known, this type of image quality can be obtained in principle simply by fast guiding on a small (D similar to 1.5 m) telescope at a good site, but only for target objects which lie within a limited angular distance around a suitably bright guide star. For high-altitude turbulence this isokinetic angle is approximately 1'. With a 1 degrees field say, one would need to tr ack and correct the motions of thousands of isokinetic patches, yet there a re typically too few sufficiently bright guide stars to provide the necessa ry guiding information. Our proposed solution to these problems has two nov el features. The first is to use orthogonal transfer CCD technology to effe ctively implement a wide-held rubber focal plane detector composed of an ar ray of cells which can be guided independently. The second is to combine me asured motions of a set of guide stars made with an array of telescopes to provide the extra information needed to fully determine the deflection fiel d. We discuss the performance, feasibility, and design constraints of a sys tem which would provide the collecting area equivalent to a single 9 m tele scope, a 1 degree square field, and FWHM similar or equal to 0 ".12 image q uality.