The FP-SPLIT slits consist of two sets of five slits-in each set the slits are all the same size. They are for use with the MAMA echelle gratings. It is possible to achieve high S/N data for bright targets, independently of the quality of the flat-field, by means of a special observing strategy wherein multiple spectrograms are obtained through these slits.
See Chapter 12 for more details on obtaining high S/N spectral data.
| Aperture |
Projected Length (arcsec) |
Width (arcsec) |
|---|---|---|
0.2X0.2FPA |
0.2 |
0.2 |
0.2X0.2FPB |
0.2 |
0.2 |
0.2X0.2FPC |
0.2 |
0.2 |
0.2X0.2FPD |
0.2 |
0.2 |
0.2X0.2FPE |
0.2 |
0.2 |
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% Throughput |
|---|---|
| 1200 |
54.7 |
| 1800 |
67.4 |
| 2400 |
73.9 |
| 3000 |
77.3 |
| 3600 |
79.7 |
| 6000 |
82.0 |
|
Space Telescope Science Institute http://www.stsci.edu Voice: (410) 338-1082 help@stsci.edu |