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| Some template libraries (the one
below is the UIST
library) use folders to group template MSBs into categories. Click on
the
lever next to a folder to open it. |
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| The UFTI templates are shown below. Full MSBs
are at
the top, and utility sequences are at the bottom. You will not need to
include utility sequences in your program, since they are independently
accessible through the Query Tool at the summit. (A possible
exception: if observing bright targets where persistence may be a
problem, you might want to copy "Flush Array"s in your MSBs as a
reminder to the observer.) |
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| The UIST templates are shown below. Spectroscopy
has been
expanded in the figure. The notes at the top are informative -
make sure you read them before copying MSBs into your program. |
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| The CGS4 templates. As with UFTI, you will not
need to include any utility sequences in your program. |
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| Polarimetry. In this case, skyflat utilities are
not accessible via the QT calibrations menu and should be included in
your MSBs (the MSBs presented do include them). |
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| Fabry-Perot library. Again, the sky flat
utilities will
need to be included explicitly in your program MSBs. |
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