Pushing the Limits
STIS has observing modes which are unsupported but are
"available",
upon consultation with a STIS Instrument Scientist and after approval of
Phase II proposal. Usage of these modes requires
justification and entails certain
responsibilities and
risks.
Some modes and methods of observing are inherently challenging or push the limits of
what can be done with STIS. These include:
Coronographic spectroscopy
Slitless first-order spectroscopy
Long-slit echelle spectroscopy
Spectroscopy with the highest spectral resolution
Precise
slit orientation requiring accurate
offset angles.
Solar system observations
High signal-to-noise observations
HST has the ability to do simultaneous
parallel
observations. STIS can be used in combination with another instrument, as either
the primary instrument pointing at the target position or the parallel instrument
pointing at an offset position determined by the spacecraft geometry. Restrictions
on parallel observations are given in the
HST Call for Proposals.
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