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Research

Group Membership

Grants & Funding

Research Facilities

Planetary Systems

McDonald Laser Ranging Station

Stars

Space Astrometry

White Dwarf Stars and the Age of the Galaxy

Whole Earth Telescope

Extragalactic

Interstellar

Star Formation

EXES: mid-IR Spectrograph for SOFIA

Spitzer Legacy Project - c2d

Theory
EXES

Estimated Capabilities


The following are estimates of EXES performance. Certain parameters, particularly the low spectral resolution, are not constrained at this time. We welcome your comments on the capabilities most important to your science.

  • Detector: 256 x 256 pixel Si:As BIB

  • Wavelength range: 5.5 to 28.5 µm

  • High Resolution Mode:
    R ~ 100,000; cross-dispersed; ~10 orders (0.5 cm-1 per order)

  • Medium Resolution Mode:
    R ~ 10,000; long slit; wavelength coverage ~5 cm-1

  • Low Resolution Mode:
    R ~ 2,000; long slit; wavelength coverage ~lambda/30 µm


Typical EXES Modes and Estimated Sensitivities


Lambda

[µm]


R

[lam/D_lam]


Slit Width

["/pixels]


Slit Length

["]


Bandwidth

[µm/kms-1]


NEFDa

[Jy]


NELBb

[Wm-2sr-1]

6
120,000

14,000

4200
1.3/3.4

1.8/4.8

1.8/4.8
10

95

95
0.023/1200

0.023/1200

0.07/3800
1.7

0.5

0.2
1.7x10-7

2.7x10-7

4.0x10-7
13.5
120,000

14,000

3700c
1.3/3.4

1.8/4.8

1.8/4.8
25

95

50c
0.038d/850

0.053/1200

0.19/4300
4.4

1.2

0.6
2.0x10-7

3.3x10-7

6.4x10-7
18
80,000

10,000

3800
1.8/4.8

2.6/6.7

2.6/6.7c
30

95

50c
0.038d/630

0.07/1200

0.18/3000
5.2

1.4

1.1
1.3x10-7

2.2x10-7

4.3x10-7
27
60,000

6800

1800
2.6/6.7

3.7/9.6

3.7/9.6
44

95

40c
0.038d/420

0.10/1200

0.39/4300
10.7

2.8

1.4
1.0x10-7

1.7x10-7

3.3x10-7

aIncludes nodding along the slit (10sigma:100 s).
bIncludes nodding off the slit (10sigma:100 s).
cAllows for 15 Hz maximum frame rate.
dOrder extends beyond size of detector giving incomplete wavelength coverage at this wavelength.



 




24 April 2003
Astronomy Program · The University of Texas at Austin · Austin, Texas 78712
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