Here we describe the key modes of GMOS to be tested as part of System Verification
(SV). The pool from which verification observations will be drawn is described in the
GMOS-North SV plan and GMOS-South
SV plan. These plan contains details of individual observations
and describes other aspects of the system which will be tested.
GMOS has six SV modes:
Direct imaging
Plate scale: 0.072 arcsec/pixel
FOV: 5.5 x 5.5 arcmin2
It is likely that all spectroscopic masks will be designed with the aid of direct images
taken with GMOS.
Long-slit spectroscopy
Spectral resolution: 670 - 4400 (0.5 arcsec slit)
Slit width: custom slits >= 0.25 arcsec width
Slit length: up to 5.5 arcmin
Multi aperture spectroscopy
Up to 600 slitlets over a 5.5 x 5.5 arcmin2 FOV
Spectral resolution: 670 - 4400 (0.5 arcsec slit)
Slit width: custom slits >= 0.25 arcsec width
Slit length: up to 5.5 arcmin
Nod-and-Shuffle
May be used with long-slit or MOS to improve sky subtraction
Integral field spectroscopy
Spectral resolution: 670 - 4400
Integral field unit configuration: two-dimensional spectroscopy over a contiguous field
of ~50 arcsec2 with 0.2 arcsec sampling. A small background field will be
available at fixed separation (>1 arcmin) from the main object field for accurate
background subtraction.
Effective slit width: ~0.27 arcsec
Spectrum length: up to 3000 pixels long and up to 900 spectral resolution elements per
spatial sample