Short-wavelength (SWP) and long-wavelength (LWP, LWR) cameras.
Low and high dispersion modes
Ranked Observing Configurations
Rank
Far-UV
Mid-UV
First choice:
SWP - low
LWP - low
Second:
SWP - hi
LWR - low
Third:
LWP - hi
Fourth:
LWR - hi
Problems:
Limited dynamic range, so both under & overexposures can be a problem.
Possible excessive cosmic ray contamination
Specifications for selected representative dataset:
Second observation after 1986.0 (if applicable). If observations are
available only before this date, rank the preference in reverse time
order before 1986.0.
Comments:
Low dynamic range means relatively high rate of under/over exposures to
be culled out when encountered.
Include high-dispersion observations only for subsequent versions.
Exclusions:
'Engineering' (nulls, flatfields, emission-comparison) and solar system
spectra. These correspond to IUE object classes .lt. 10 and .gt. 90.