Abstract: An optical head for attachment to an optical system, such as a telescope, is shown. The optical head in a housing includes a first sensor for imaging an object in a field of view and a second sensor for tracking a star or other celestial body which is off axis to the field of view of the first sensor. The second sensor is rigidly supported and positioned a selected distance from and adjacent to the first sensor and is adapted to generate correction signals which are used to control a drive system of the optical system or telescope. The correction signals are representative of desired changes in the relative position of the optical system or telescope to the star being tracked. The correction signals are applied to the drive system to maintain, during imaging, optical alignment of the first sensor with an object in the field of view. In the preferred embodiment, the optical head is used for astronomical imaging and tracking wherein the first sensor is an imaging CCD and the second sensor is a tracking CCD.

Abstract: This invention is a scanning probe microscope which uses three separate motorized legs to adjust the distance between the probe and sample and to adjust the tilt between the probe and the sample. The microscope is shown configured in various ways. One form is a scanner on a base in which the base contains the sample and legs. Another is a scanner which contains the legs and rests on the sample, or may also rest on a support that spans a larger sample allowing translation of the sample independent of the scanner. Another is a scanner which contains the legs and is mounted so that a sample holder sits on the legs. The latter configuration allows for easy access to the sample. One variation of this configuration has provision for the mounting of several samples which can be sequenced for probing automatically.