Near-Infrared Observing at MDM
Located on the southwest ridge of Kitt Peak, MDM Observatory is jointly
operated by Dartmouth College, Columbia University, Ohio-State University, and
the University of Michigan. The observatory operates two telescopes: the 1.3m
McGraw-Hill Telescope, and the 2.4m Hiltner Telescope. For Near-Infrared
observations, the Dartmouth Supernova Group uses the 2.4m Hiltner telescope with
TIFKAM (a.k.a ONIS). TIFKAM is a highly
configurable Near-Infrared camera which uses a 512x1024 ALLADIN InSb array. TIFKAM
is equipped with standard J,H, and K filters for broadband imaging, and a variety
of grisms and order blocking filters that allow for low resolution (R about 700)
and moderate resolution (R about 1400) spectroscopy in the 0.8 -- 2.5 micron
wavelength regime. For more information about MDM observatory check out the
MDM website. For more about
TIFKAM (a.k.a. "ONIS", a.k.a. "MOSAIC"), try the
ONIS homepage.
This is a picture of the 2.4m Hiltner telescope from inside the dome.
Here is a picture of TIFKAM mounted on the 2.4m Hiltner telescope.
Back