- ...I
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``Dashboard: a Knowledge-Based Control System Interface" by De Clarke,
to be presented at the 1997 TCL Conference.)
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- ...dashboard
- See Part I, chapter 3.3.
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- ...observing
- Certain types of data will have to be protected, to
preserve the privacy of observers' projects and observing plans. Observers
will have access to all public data, and all private data pertaining to their own
research.
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- ...spectra
- Of course, we do not plan to store actual binary image data
in the database, only header information and the URL of the actual
image, in this case a FITS image file on local disk.
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- ...sketch.
- The attribute
``context" is available for each major entity in the DEIMOS database,
and it means whatever the software engineers want it to mean; it is
used merely to ``label" or associate entities for practical
purposes. During prototyping and schema development, this
generic attribute provides a certain flexibility in coding,
and latitude for invention and improvisation. As the schema and
applications settle into their final form, the ``context" attribute
usually turns out to mean something more concrete. In
the case of Paths, this attribute became useful for grouping
Paths into ``drawings" of related agents and their function. Each
Path context now has an author, title, and so forth. When the
great nomenclature
cleanup arrives, this attribute of Paths will probably be
renamed ``drawing".
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- ...elements
- Except for the analytical mappings in
Section 2.2. However, the analytical mappings could be used to
generate mappings in the same form described here
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- ...starlight
-
Aberration of starlight is maximum in directions tangential to motion.
However, the differential aberration is greatest in direction of
motion, reaching a maximum of 89#89, where 90#90 is the
edge-to-edge angle of the field. For DEIMOS, considering both beams and the
radius of the FOV, 91#91 and the differential aberration
can reach 92#92 arcsec in virtually any orientation. On the other hand,
differential mask alignment between beams A and B can remove a large
portion of the effect in the important cross-slit direction.
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- ...mask
- This procedure only works
if the mask surface closely approximates the spherical image surface of
the telesope. For differences h between the two surfaces, translational
errors can reach 100#100. At the extreme ends of the mask, the
curvature reaches a difference of 1.3 mm (88#88 = 0.034 arcsec);
the amplitude of the deviation between the cylindrical and spherical surfaces
is 30#301.4 mm (88#88 = 0.037 arcsec) along the ``flat'' axis. This latter
is the more critical, as it is in the ``cross-slit'' direction.
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- ...ray-tracing
-
This ray-tracing depends on the telescope focal length, 116#116,
and thus is only valid for one value of the focus. However,
116#116 appears to be quite stable - the primary's focal length cannot
be changed simply by tilting the segments, and the segments and secondary
are all in ``zerodur'' and so should not change shape (T. Mast, priv. comm.)
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- ...reflectance
- Reflectance for a given material depends not only
on the wavelength of light, but also the angle of incidence. However,
for small variations in incidence angle there is little variation in
reflectance, and we ignore this slight dependency throughout this discussion.
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- ...slope
- The slope itself will contain a pitch error for each grating.
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- ...throughput
- from above the atmosphere, as defined.
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- ...x
- If the mapping of 245#245 changes (for
example, by resetting the grating in its cell or adjusting pitch angle)
then either a new calibration set must be acquired for that grating or
the existing one must be corrected.
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