The Swift Gamma-Ray Burst Mission, Swift XRT, contains a grazing incidence Wolter I telescope to focus X-rays onto a state-of-the-art CCD. The complete mirror module for the XRT consists of the X-ray mirrors, thermal baffle, a mirror collar, and an electron deflector. To prevent on-orbit degradation of the mirror module's performance, it is maintained at 20 ± 5 °C, with gradients of <1 °C by an actively controlled thermal baffle (purple, in the schematic) similar to the one used for JET-X. A composite telescope tube holds the focal plane camera (red), containing a single CCD-22 detector. Credit: Swift PI: Neil Gehrels, Responsible NASA Official: Phil Newman, Web Curator: J.D. Myers, PAO Contact: Francis Reddy.
