T-ReCS and Michelle: The Mid-Infrared Spectroscopic Capabilities of the   Gemini Observatory
  Gemini Observatory's northern and southern telescopes are both presently being outfitted with facility mid-infrared imagers/spectrometers. This will allow observers the unique opportunity to apply to one observatory for all-sky spectroscopic access in the mid-infrared with the light gathering power of 8-meter telescopes. Gemini South has recently commissioned the Thermal-Region Camera and Spectrograph (T-ReCS) and is now available to perform queue observations for the community. T-ReCS is capable of low-resolution long-slit spectroscopy of R~100 near 10 and 20 um, and medium-resolution long-slit spectroscopy of R~1000 near 10 um. Gemini North is presently commissioning Michelle, which will be capable of low-, medium-, and high-resolution long-slit spectroscopy of R~200, 1000, and 3000, respectively, near 10 um, as well as low-resolution long-slit spectroscopy of R~200 near 20 um. Michelle can also perform echelle spectroscopy of R~30000 at 10 and 20 um. The low-, medium-, and high-resolution spectroscopic modes of Michelle will be available to the public for the fall semester of 2004, and the echelle mode is expected to be available in 2005. 
James M. De Buizer (Gemini South Observatory) and R. Scott Fisher   (Gemini North Observatory)