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GMOS

The two Gemini Multi-Object Spectrographs (GMOS), one on each telescope, provide 0.36-1.10 µm long-slit and multi-slit spectroscopy and imaging over a 5.5 arcmin field of view. Each GMOS is also equipped with an Integral Field Unit (IFU) making it possible to obtain spectra of an area of about 35 square arcsec with a sampling of 0.2 arcsec. The Nod-and-Shuffle mode, enabling superior sky subtraction, is available with both GMOSs in most spectroscopic modes.

The GMOSs were built by a collaboration of the Astronomy Technology Centre at the ROE and the University of Durham in the UK and the Herzberg Institute of Astrophysics in Canada. GMOS-N was delivered in July 2001 with GMOS-S following in December 2002.

The Instrument Scientists for GMOS are Rodrigo Carrasco (GMOS-S) and Kathy Roth (GMOS-N).

Announcements

GMOS-N B600 grating unavailable. See the Status and Availability page for current instrument configurations.

GMOS science highlights

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How to use these pages

The GMOS pages are organized as follows.