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Cosmic Origins SpectrographInstrument Handbookfor Cycle 21 > Chapter 13: Spectroscopic Reference Material > NUV Grating G225M

NUV Grating G225M
Description
The G225M grating samples wavelengths between about 2100 and 2500 Å. The grating has 13 central wavelength settings.
Special Considerations
G225M spectra consist of three 35-Å stripes separated by two 64-Å gaps. To acquire a complete spectrum requires the use of six central-wavelength settings.
 
Resolving
Power
R = λ/Δλ
Dispersion
(mÅ pixel–1)
Spatial Resolution (milliarcsec pixel-1)
FP-POS
Step
(Å step-1)
Figure 13.19: Wavelength Ranges for the G225M Grating
Dark lines represent wavelengths sampled by all four FP-POS positions.
G225M Point-Source Sensitivity
Table 13.9: G225M Point-Source Sensitivity for PSA
Sensitivity
(counts pixel-1 sec-1 per
erg cm-2 sec-1 Å-1)
Figure 13.20: G225M Point-Source Sensitivity for PSA and BOA
G225M Signal-to-Noise Ratio
Figure 13.21: Point-Source Signal-to-Noise as a Function of STMAG for G225M
The top axis displays constant Fλ values corresponding to the STMAG units (V+STMAGλ) on the bottom axis. Recall that STMAG = 0 is equivalent to Fλ = 3.63E-9 erg cm-2 s-1 Å-1. Colors refer to exposure times in seconds. The edge of the shaded area corresponds to the bright-object screening limit. Use of the PSA is assumed.

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