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SUMMARY:2012 Fall Physics Colloquium Series:  Dr. Jennifer Marshall
DESCRIPTION;ENCODING=QUOTED-PRINTABLE:Dr. Jennifer Marshall=0D=0A=
Associate Research Scientist, Department of Physics and Astronomy=0D=0A=
Texas A&M University - College Station, Texas=0D=0A=
The GMACS Spectrograph for the Giant Magellan Telescope=0D=0A=
GMACS is a wide-field, multi-object, moderate-resolution optical spectrograph being built at Texas A&M that has been selected as a first light instrument for the Giant Magellan Telescope (GMT). The primary design drivers are high=0D=0A=
throughput, simultaneous wide wavelength coverage, and a very wide field. GMACS will be able to study some of the faintest objects in the Universe, from the highest redshift=0D=0A=
galaxies, to nearby low surface brightness objects, to KBOs in our solar system. I will describe the telescope, the instrument,=0D=0A=
and the science drivers that led us to the design of the instrument.=0D=0A=
For more information contact: Dr. Anzhong Wang 254-710-2276=0D=0A=
=0D=0A=

LOCATION:Baylor Sciences Building, Room D.109
DTSTART;TZID=US_Central:20121017T160000
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