Space Telescope Science Institute  A.3 NICMOS A.5 WFPC2

A.4 STIS


Suppose that you wish to use the STIS to observe a target at a declination of +15 degrees, so that there are 52 minutes of visibility time per orbit (see Table 6.1). Your desired exposures are listed in Table A.10, and the associated overheads are listed in Table A.11. In Table A.12 you can see how this fits into a total of 2 orbits.


Table A.10: STIS Example: Planned Exposures
Config
Mode
Spectral
Element
Number of Exp
Time per Exp [m]
Notes
STIS/CCD
ACQ



target acquisition
STIS/CCD
ACQ/PEAK



peakup acquisition (necessary because of use of 0.1" wide slit for subsequent spectra)
STIS/CCD
IMAGING
F28X50OII
2
2

STIS/NUV
IMAGING
F25QTZ
1
19

STIS/NUV
SPECTROSCOPIC
G230L
1
13
with 52X0.1 slit
STIS/FUV
SPECTROSCOPIC
G140L
1
17
with 52X0.1 slit

Table A.11: STIS Example: Incurred Overheads
Overhead
Overhead Time [m]
Notes
see Table
Guide star acquisition
6
first orbit in new visit
Guide star re-acquisition
5
per orbit after first orbit
ACQ
6
target acquisition
ACQ/PEAK
6
peakup target acquisition
CCD imaging
5
but only 1m if no change from previous exposure
MAMA imaging
5
but only 1m if no change from previous exposure
MAMA spectroscopy
8
but only 1m if no change from previous exposure

Table A.12: STIS Example: Orbit Planning
Activity
Duration [m]
Elapsed Time [m]
Orbit 1


Guide star acquisition
6
6
ACQ
6
12
ACQ/PEAK
6
18
F28X50OII Exp Time
2x2
22
F28X50OII Overhead
5+1
28
F25QTZ Exp Time
19
47
F25QTZ Overhead
5
52
Orbit 2


Guide star re-acquisition
5
5
G230L Exp Time
13
18
G230L Overhead
8
26
G140L Exp Time
17
43
G140L Overhead
8
51
Unused
1
52

A.3 NICMOS A.5 WFPC2
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