Space Telescope Science Institute  Echelle Grating E230H Echelle Grating E140H

Echelle Grating E140M


Description

The E140M grating is used with the FUV-MAMA and provides echelle spectra at a resolving power of 45,800 from 1123-1710 Å.

Special Considerations

A single E140M echellogram covers ~600 Å, however at wavelengths longward of 1649 Å, the echelle orders overrun the width of the detector in the dispersion direction, so there will be three small gaps in the wavelength coverage. One gap of ~0.2 Å, one of ~0.4 Å, and one of ~0.7 Å occur between 1649 and 1700 Å.

The separation between orders is ~15 pixels (or 0.44 arcseconds) at 1150 Å and ~33 (0.96 arcseconds) at 1700 Å.

Grating
Spectral Range
Average Dispersion
(Å per Pixel)
Dispersion, Cross Dispersion
Plate Scale
(arcsec / pixel)
Tilts
Central
Wavelengths
Complete
Per Tilt
E140M
1123-1710
620
/91,700
0.036,0.029
Prime
1425

Figure 13.54: Wavelength Range for the E140M Grating Setting

 

E140M Sensitivity

Table 13.15: E140M Throughputs & Sensitivities for a Point Source
Sensitivity
% Throughput
1200
1.2E11
0.3
1250
2.4E11
0.6
1300
3.0E11
0.7
1350
3.2E11
0.7
1400
3.0E11
0.6
1450
2.6E11
0.5
1500
2.2E11
0.4
1550
1.7E11
0.3
1600
1.2E11
0.2
1650
9.1E10
0.1
1700
5.9E10
0.1

Figure 13.55: E140M Point Source (left axis), and Diffuse Source (right axis) Sensitivities.

 

Note

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.

E140M Signal-to-Noise

Note:

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 13.56: Diffuse Source Signal-to-Noise as a Function of STMAG for E140M

 
Figure 13.57: Point Source Signal-to-Noise as a Function of STMAG for E140M

 

Echelle Grating E230H Echelle Grating E140H
Space Telescope Science Institute
http://www.stsci.edu
Voice: (410) 338-1082
help@stsci.edu