IGI DESCRIPTION


Description:
A high efficiency, low resolution grism spectrograph and focal reducer (5:1). IGI uses the TK4 CCD as a detector. On the 2.7-m in imaging mode it can reach mv = 22 mag in 3 minutes with a 7 arcminute field. In the spectroscopy mode it can reach mv = 20 mag in 30 minutes and cover a wavelength range from 0.4 to 1.0 micron at a resolution of 12 - 20 Å. Multi-slit (up to 25 object) capability is available. IGI with TK4 gives a 3.5 to 1 reduction of the platescale at native cass, but only covers a 48 mm x 48 mm field of view at the cass focus (roughly 7x7 arcmin on the 2.7-m at f/9). Only one filter can be used at once and they are located at the telescope focus so can suffer from dust build up. It is designed primarily as a fast spectrograph rather than an imager. STAR-1 and PIXEL CCD acquisition and guiding are available.
Contact person:
Scientist: Dr. Gary Hill, 512/471-1477, <hill@astro.as.utexas.edu>
Available telescope positions:
2.7-m (cass f/9)
2.1-m (cass)
Available CCD's:
TK4