Table 1.1: Overall Physical and Optical Characteristics

FunctionValue
LocationRight Nasmyth platform, Keck II; removable from focus
LayoutTwo cameras fed from common collimator
Rotator540 degrees rotation
User accessSlit masks, all gratings and 2 user filters/side
Guiding systemTwo guiders; ~5 arcmin2 field in each
Telescope focusGuiders allow continuous monitoring
FlexureGoal is <0.1 px over typical integrations
Spectrograph flexure controlActive optic with closed loop feedback
Focal plane flexure controlRigidly attached reticles for guiders
Slit masks10 per side; matched to focal plane curvature
Slitlet optionsSlitlets of arbitrary shape, size and orientation
Dispersive elements6-in x 8-in and 8-in x 12-in gratings
Imaging optionSilvered flat mirror replaces grating
Filters for each camera6.5 x 6.5-in glass filters; 7 slots for B,V,R,I, "clear," and 2 user
Collimator focal length86.50-in
Camera focal length15.00-in
Beam diameter6.33-in for 10.95 m primary; 5.79-in for 10.02 m vignetting radius1
Monochromatic f/ratiof/2.358 11.00 m primary; f/2.586 for 10.02 vignetting radius1
Polychromatic f/ratiof/ 1.29
Scale at detector0".00759 um^-1 ; 0".1193 per 15um px
Angular field radius of camera 11.40 degrees
Typical camera image quality B band imaging: 30 um RMS (0".20 FWHM)
........V-->I band imaging: 20 um RMS (0".13 FWHM)
........Spectroscopy2 : 20um RMS (0".13 FWHM)
Camera glass transmission 91% for l> 5200 A
........(in blue) 50% at 3900 A; 82% at 4400 A
Total camera throughput 83% at l > 5200 A (inc. coatings and transmission)

1 The vignetting radius of the primary mirror is that circle that contains all tips of the primary mirror segments except the 6 outermost ones. It is 10.02 m in diameter. The light beyond the vignetting radius is 4.5% of the total area of the unobscured primary, or 0.75% per tip. The vignetting radius has been used to simplify various vignetting calculations.

2 Averaged over all field angles for an object at the middle of the slit and for A 4400-11000 A.