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Cosmic Origins SpectrographInstrument Handbookfor Cycle 21 > Chapter 13: Spectroscopic Reference Material > FUV Grating G160M

FUV Grating G160M
Description
The G160M grating samples wavelengths between about 1405 and 1775 Å. It offers higher resolution and effective area than the G140L grating, but less spectral coverage.
Special Considerations
The gap between segments A and B spans 18.1 Å. To fill this gap requires exposures separated by two central-wavelength settings.
Resolving
Power
R = λ/Δλ
Dispersion
(mÅ pixel–1)
FP-POS
Step
(Å step-1)
Figure 13.10: Wavelength Ranges for the G160M Grating
G160M Point-Source Sensitivity
Table 13.6: G160M Point-Source Sensitivity for PSA
Sensitivity
(counts pixel-1 sec-1 per
erg cm-2 sec-1 Å-1)
Figure 13.11: G160M Point-Source Sensitivity for PSA and BOA
G160M Signal-to-Noise Ratio
Figure 13.12: Point-Source Signal-to-Noise as a Function of STMAG for G160M at 1610 Å
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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