STIS has a complement of neutral-density (ND) filters, which can be used with the CCD, the NUV-MAMA, and the FUV-MAMA spanning from ND1 (attenuation of 10-1) to ND5. The ND5 filter appears to have a UV throughput of at most 10-6, substantially smaller than prelaunch estimates.
F25NDQ1
,
F25NDQ2
,
F25NDQ3
, and
F25NDQ4
are physically four separate quadrants of a single 25 x 25 arcsecond filter occupying a single position on the slit wheel. The target is put into the appropriate quadrant when one of these apertures is requested. However, it should be noted that all four quadrants project onto the detector, and each quadrant plus a 5" surrounding perimeter must be considered for bright-object limits. Thus, although one may request placement of a bright object centered in F25NDQ4
, no other objects in the surrounding region may violate the bright-object limits for the other quadrants. This includes a 5" restrictive border around the interior of the selected quadrant, effectively reducing its size. In addition, any object that would produce a global count rate exceeding 1.5x106 counts s-1 or a local count rate above 500 counts sec-1 pixel-1 in F25NDQ1
may not be observed using any of the other quadrants. To ensure accurate placement of a bright object in the selected quadrant, a CCD target acquisition must also be specified. Also note that the boundaries between the four quadrants are not well centered, and as a result the sizes of the quadrants vary. Figure 13.82: shows a lamp image of this aperture, and Table 13.33 gives the approximate dimensions of each quadrant and the default locations where targets are placed.
F25ND3
and F25ND5
are each individual 25 x 25 arcsecond filtered apertures, occupying unique locations on the slit wheel. Detailed information for F25ND3 and F25ND5 are given in F25ND3-NUV-MAMA, F25ND3-FUV-MAMA, F25ND5-NUV-MAMA, and F25ND5-FUV-MAMA.
Space Telescope Science Institute http://www.stsci.edu Voice: (410) 338-1082 help@stsci.edu |