Like the G430L
grating, the G430M
grating is used with the CCD and has a spectral range from 3020-5600 Å.
Since a single exposure taken with this grating covers only 286 Å the grating must be scanned, with a series of exposures taken at 10 distinct settings, to cover the full spectral range of the grating.
The G430M
grating mode is designed for observations where spatially resolved, long slit spectroscopy is desired at relatively high spectral resolution (R~6000) over a limited region of the near-ultraviolet or optical spectrum.
Point source sensitivity assumes full transmission (zero slit losses). Diffuse source sensitivity assumes a 0.1" wide slit. To convert point source sensitivities to diffuse source sensitivities multiply the point source values by the grating spatial (cross dispersion) plate scale in units of arcseconds per pixel and by the width of the desired slit in units of arcseconds.
The top axis displays constant F values corresponding to the STMAG units (V+STMAG) on the bottom axis. Recall that STMAG=0 is equivalent to F = 3.63E-9 erg cm-2 s-1 Å-1. The curves are labeled with exposure times in seconds.
Figure 13.16: Diffuse Source Signal-to-Noise as a Function of STMAG for G430M
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