Space Telescope Science Institute  First-Order Line Spread Functions Spectral Purity, Order Confusion, and Peculiarities

Echelle Line Spread Functions



Table 13.39: Spectral Resolution for Echelle Medium-Resolution Modes (E230M, E140M)
Slit
Spectral Resolution (FWHM in pixels)
Point Source
Extended Source
1200
Å
1500
Å
1700
Å
2400
Å
0.1X0.03
0.9
0.9
1.0 1,1.6 2
1.6
~1
0.2X0.2
1.4
1.3
1.11, 2.02
1.9
~6
0.2X0.06
1.3
1.2
1.1 1, 1.8 2
1.7
~2
6X0.2
1.6
1.4
1.2 1, 2 2
1.9
~6
1 FWHM with FUV-MAMA (E140M).

2 FWHM with NUV-MAMA (E230M).

Figure 13.88: Echelle Line Spread Functions, E140M (top) and E230M (bottom)

 


Table 13.40: Spectral Resolution for Echelle High Resolution Modes (E140H, E230H)
Slit
1200
1500
1700
2400
Extended Source
0.1X0.03
0.8
0.8
1 1, 1.5 2
1.5
~1
0.2X0.2
1.3
1.1
11, 1.82
1.7
~6
0.2X0.09
1.2
1.1
1 1, 1.7 2
1.7
~2
6X0.2
1.4
1.2
1.2 1, 2 2
1.8
~5
1 FWHM with FUV-MAMA (E140M).

2 FWHM with NUV-MAMA (E230M).

Figure 13.89: Echelle Line Spread Functions, E140H (top) and E230H (bottom)

 

First-Order Line Spread Functions Spectral Purity, Order Confusion, and Peculiarities
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