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Phase 2 Proposal Instructions for Cycle 10 | |||
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10.1 Introduction to STIS
The Instrument Configurations and Operating Modes described here are used to specify exposures on the RPS2 Visit and Exposure Specifications. The legal Visit and Exposure Specifications are discussed in a summary fashion in the following sections. More complete descriptions of Instrument Configurations, Modes, Apertures, Spectral Elements, etc. are available in the STIS Instrument Handbook.
Note that many of the Optional Parameters have default values; in such cases, an entry as an Optional Parameter in the Visit and Exposure Specifications is necessary only if it is desired to override the default value. In the STScI proposal system, the physical units of Optional Parameter quantities are always implicit and should never be entered by the observer.
STIS has a lot of apertures, and keeping track of them is difficult. To simplify matters somewhat, and to avoid typographical errors, a complete list of them is provided at the end of this chapter (see Table10.4: Supported STIS Apertures). That table should be taken as definitive if any additional information in this chapter appears to conflict.
The following table lists the permitted Instrument Configurations, Operating Modes, Spectral Elements, and Optional Parameters for the STIS.
Note also that in addition to the automatic wavelength calibrations added by the system, the following observer-added contemporaneous calibrations may also be made:
- CCDFLAT (fringe flats) for G750L and G750M observations longward of 7000 .
- WAVE calibrations for added wavelength precision.
See the STIS Instrument Handbook for more information.
STIS Optional Parameters
Table 10.1: Supported Optional Parameters for STIS Instrument Modes
The following sections provide further details of the entries to be made on the Visit and Exposure Specifications when a particular STIS/CCD, STIS/FUVŠMAMA, or STIS/NUVŠMAMA Mode/Configuration is chosen.
Note: the AXIS1 and AXIS2 coordinate system is as defined in the discussion of the STIS coordinate system, which is in the STIS Instrument Handbook. Array sizes are given as AXIS1 x AXIS2. For CCD and MAMA first-order grating and MAMA echelle spectroscopic modes, AXIS1 is in the dispersion direction and AXIS2 is in the cross-dispersion direction.
Space Telescope Science Institute http://www.stsci.edu Voice: (410) 338-1082 help@stsci.edu |
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