GeminiFocus July, 2015 | Page 19

ficiency, the team recoated some key optics and redesigned one element that was vignetting the optical path). As a result, GRACES’s efficiency is improved by an average of roughly 20 percent towards the red part of the spectrum. (See Figures 1 and 2.) Small Projects Initiative Gemini’s instrumentation Department is also continuing with the Small Project initiative to leverage community interest and talent in keeping our current instruments competitive. We discussed ideas for these projects during the Toronto users meeting in June. A Request for Proposals will go out later this year. GeMS Laser Procurement Accepted In April, we completed a set of feasibility studies to explore the possibility of replacing the current Gemini Multi-congugate adaptive optics System (GeMS) laser with one we could operate more often with reduced staff requirements. The results of these studies, using both internal and external resources, were positive, and the Gemini Board agreed at its last meeting that we should proceed to procure a new laser. We have started the contracting work and have made this effort a high priority project. July 2015 Gemini Instrument Feasibility Study (GIFS) Update In April 2015, Gemini launched four independent instrument feasibility studies to help determine requirements for the next new Gemini instrument (also known as Generation 4#3, or Gen4#3) after GHOST. Each team’s study will provide Gemini with a collection of science cases, top-level science and instrument requirements, and corresponding feasible instrument designs. The team’s efforts are guided by a set of principles provided by the Science and Technology Advisory Committee (STAC) [viewable here] that describe very highlevel requirements for the Gen4#3 instrument. Once completed, the four studies will aid Gemini in creating the requirements for Gen4#3. We expect to release a Request for Proposals to design and build the instrument in the first half of 2016. Figure 2. Greg Barrick (Canada-FranceHawaii Telescope) installing the GRACES receiver module in the ESPaDOnS spectrograph, incorporating some of the recently improved optics. Each of the four feasibility study teams presented their ideas and work in progress at the recent Toronto 2015 Future & Science of Gemini Observatory meeting. The meeting also allowed each team to interact with many Gemini users and included a panel discussion that reflected on the coming needs for Gemini’s next new instrument. The teams will provide Gemini with draft study reports in mid-August 2015 and present their work in person a month later. Look for more detailed information shortly thereafter, both on the Gemini web pages (view here) and in future editions of GeminiFocus. The teams will submit the final reports in mid-October.  Summaries of the four team instrument studies follow:  GeminiFocus 17