GeminiFocus 2017 Year in Review | Page 58

APRIL 2017 GHOST Taking Shape Development of Gemini’s high-resolution optical spectrograph GHOST — a joint effort by the Australian Astronomical Observatory, the National Research Council Canada-Herz- berg, and the Australian National University — continues to progress. As of the end of 2016, most of the Cassegrain unit’s mechani- cal parts have been manufactured, received, Figure 15. GHOST integral field unit positioner frame. Figure 16). GHOST Slit Viewer mechanical assembly. test fitted (as shown in Figures 15-17), and partially disassembled for anodizing. The Cassegrain unit’s mechanical assembly is close to being completed. Most of its op- tics have also been received, and they have passed Acceptance Testing; optics integra- tion will start at the end of March, followed by electronics integration. The final mechanical elements for the Guide Camera assembly, Slit Viewer assembly, and Calibration unit, have also been completed, and we are now ready to integrate their op- tical elements and electronics. The Guide Camera assembly and Calibration unit are on target for Instrument Control Software integration in mid-May. — David Henderson Figure 17. FLAMINGOS-2 Capabilities GHOST IFU positioner mounted in its frame on the tilt table. Multi-Object Spectroscopy Progress Credits: All AAO The FLAMINGOS-2 (F-2) near-infrared (NIR) imager and spectrograph was designed with multi-object spectroscopy (MOS) in mind, but we could not commission this important feature until now. F-2 MOS is achieved by cutting aluminum plates (“masks”) with the desired slitlets’ width, length, and target po- sitions in the 6 x 2 arcminutes field-of-view on the sky. The masks are located on the “MOS wheel,” which locates each mask on the telescope’s focal plane and has slots for nine different masks. One critical capability for MOS observations is the ability to change masks while the in- strument is installed on the telescope. By addressing this important function (as we did with this work) we minimize the impact on the instrument-telescope alignment and keep the camera cryogenic dewar cold, with the detector stabilized at its working tem- 56 GeminiFocus January 2018 / 2017 Year in Review