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MIRMOS is a multi-object + integral field near-infrared R~3700 spectrograph
MIRMOS is a multi-object + integral field near-infrared R~3700 spectrograph
optimized for
optimized for
faint-object spectroscopy of galaxies and diffuse emission
faint-object spectroscopy of galaxies and diffuse emission
&
&
high spectrophotometric precision observations of exoatmospheres
high spectrophotometric precision observations of exoatmospheres
on
on
the Magellan Telescopes.
the Magellan Telescopes.
MIRMOS will be built at Carnegie Observatories
MIRMOS will be built at Carnegie Observatories
in collaboration with the
in collaboration with the
Instrument Development Group (IDG)
Instrument Development Group (IDG)
at Johns Hopkins University.
at Johns Hopkins University.
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