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STIS Instrument Handbook for Cycle 24 |
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The PRISM has two central wavelength settings optimized to cover the optical through the far-ultraviolet (FUV) tail down to 1150 е. It is used with the NUV-MAMA detector.The full dispersion spreads over ~450 pixels with dispersion as shown in Figure 13.64; thus if you have sources covering the field of view in the dispersion direction, the red tail will be lost for some targets with this setting. For a plot of wavelength vs. pixel no., see Figure 4.12.
Figure 13.62: Wavelength Range for the Prism SettingTable 13.17: PRISM Throughputs & Sensitivities for a Point Source