PDS_VERSION_ID                     = PDS3
RECORD_TYPE                        = "STREAM"
LABEL_REVISION_NOTE                = "2004-09-07: Information loaded into OLAF
        by Gordon Bjoraker;
        2007-02-23: Additional information contributed by Bobby Bus"

OBJECT                             = INSTRUMENT
 INSTRUMENT_ID                     = "I0046"
 INSTRUMENT_HOST_ID                = "OBS376T3"

 OBJECT                            = INSTRUMENT_INFORMATION
  INSTRUMENT_NAME                  = "SPEX"
  INSTRUMENT_TYPE                  = {"SPECTROMETER", "IMAGER"}
  INSTRUMENT_DESC                  = "


  Instrument Overview
  ===================
    Low- to medium-resolution near-IR spectrograph and imager at the NASA IRTF
    on Mauna Kea.  The spectrograph employs a 1024x1024 Aladdin 3 InSb array
    along with various slits, gratings and prism cross-dispersers to produce
    spectra with resolving powers up to R ~ 2000 across the wavelength
    intervals 0.8 to 2.5 microns and 2 to 5.5 microns.   The slit-viewing
    imager uses a 512x512 Aladdin 2 InSb array that covers a 60x60 arcsec
    field of view at a image scale of 0.12 arcsec per pixel.  In addition to
    object acquisition and scientific imaging, the imaging array is used as an
    infrared auto-guider for the spectrograph."
 END_OBJECT                        = INSTRUMENT_INFORMATION

 OBJECT                            = INSTRUMENT_REFERENCE_INFO
  REFERENCE_KEY_ID                 = "RAYNERETAL2003"
 END_OBJECT                        = INSTRUMENT_REFERENCE_INFO

 OBJECT                            = INSTRUMENT_REFERENCE_INFO
  REFERENCE_KEY_ID                 = "RAYNERETAL2004"
 END_OBJECT                        = INSTRUMENT_REFERENCE_INFO

END_OBJECT                         = INSTRUMENT
END