Design and Commissioning of a Hi-Resolution Visible/Near-IR Echelle Spectrograph (HI-VIS) for the AEOS Telescope

摘要

The Institute for Astronomy has developed and recently installed a high-resolution cross-dispersed echelle spectrograph for use at one of the coude foci of the AEOS 3.7-meter telescope, operated by the Air Force Space Command atop Mt. Haleakala on the island of Maui. The spectrograph features an optical arm for the wavelength range 0.5-1.0 urn and an infrared arm for the range 1.0 - 2.5 microns We review the spectrograph design and present commissioning results obtained with both the visible and infrared arms. Both channels use a white- pupil collimator design to maximize grating efficiency and to limit the size of the camera optics. The visible arm of the spectrograph uses deep-depletion CCDs optimized for operation near 1.0 urn. The infrared detector is a 2048 x 2048 HGCdTe array (HAWAII-2) that has been developed by Rockwell Science Center for this project. Both channels are equipped with slit-viewing cameras for object acquisition and control of a fast guiding tip-tilt mirror located in a pupil image in the spectrograph fore optics.