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Cosmic Origins SpectrographInstrument Handbookfor Cycle 21 > Chapter 13: Spectroscopic Reference Material > NUV Grating G285M

NUV Grating G285M
Description
The G285M grating samples wavelengths between about 2500 and 3200 Å. The grating has 17 central wavelength settings.
Special Considerations
G285M spectra consist of three 41-Å stripes separated by two 74-Å gaps. To acquire a complete spectrum requires the use of eight central-wavelength settings.
 
Resolving
Power
R = λ/Δλ
Dispersion
(mÅ pixel–1)
Spatial Resolution (milliarcsec pixel-1)
FP-POS
Step
(Å step-1)
Figure 13.22: Wavelength Ranges for the G285M Grating
Dark lines represent wavelengths sampled by all four FP-POS positions.
G285M Point-Source Sensitivity
Table 13.10: G285M Point-Source Sensitivity for PSA
Sensitivity
(counts pixel-1 sec-1 per
erg cm-2 sec-1 Å-1)
Figure 13.23: G285M Point-Source Sensitivity for PSA and BOA
G285M Signal-to-Noise Ratio
Figure 13.24: Point-Source Signal-to-Noise as a Function of STMAG for G285M
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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