Space Telescope Science Institute   6.7 Exposure Time Examples Chapter 7:  Feasibility and Detector Performance

6.8 Tabular Sky Backgrounds


We provide a table of the high sky background numbers as plotted in Figure 6.1:, for easy reference. See the text and the caption in Figure 6.1 for more details. The high sky values are defined as the earthshine at 24° from the limb and by the typical zodiacal light of mV = 22.7. Table 6.1 lists the average value of the zodiacal and earthshine backgrounds (excluding the contributions from geocoronal emission lines) in each wavelength interval. The contributions of the geocoronal emission lines are tabulated separately in Table 6.7.

Table 6.6: High Sky Background (excluding geocoronal emission lines)
Wavelength
Earthshine
Zodiacal Light
Total Background
Å
erg sec-1 cm-2
Å-1 arcsec-2
erg sec-1 cm-2
Å-1 arcsec-2
erg sec-1 cm-2
Å-1 arcsec-2
1000
1.32E-22
2.56E-28
1.32E-22
1100
3.38E-22
1.37E-26
3.38E-22
1200
8.25E-23
1.27E-25
8.26E-23
1300
5.41E-24
6.88E-25
6.10E-24
1400
4.65E-25
2.68E-24
3.14E-24
1500
3.97E-25
4.60E-23
4.64E-23
1600
3.42E-25
2.32E-22
2.33E-22
1700
1.24E-23
6.49E-21
6.50E-21
1800
1.26E-22
1.35E-20
1.37E-20
1900
4.69E-22
2.13E-20
2.18E-20
2000
1.02E-21
4.22E-20
4.32E-20
2100
1.42E-21
1.21E-19
1.22E-19
2200
8.02E-22
2.00E-19
2.01E-19
2300
3.73E-22
1.97E-19
1.97E-19
2400
2.59E-22
2.14E-19
2.14E-19
2500
2.80E-22
2.05E-19
2.06E-19
2600
1.29E-21
4.73E-19
4.75E-19
2700
5.42E-21
8.26E-19
8.31E-19
2800
7.72E-21
7.48E-19
7.56E-19
2900
4.43E-20
1.52E-18
1.56E-18
3000
1.01E-19
1.72E-18
1.82E-18
3100
2.12E-19
1.92E-18
2.14E-18
3200
3.50E-19
2.24E-18
2.59E-18
3300
4.45E-19
2.72E-18
3.17E-18
3400
6.36E-19
2.65E-18
3.28E-18
3500
8.28E-19
2.67E-18
3.50E-18
3600
1.05E-18
2.53E-18
3.58E-18
3700
1.20E-18
3.03E-18
4.23E-18
3800
1.26E-18
2.87E-18
4.13E-18
3900
1.59E-18
2.83E-18
4.42E-18
4000
2.33E-18
4.22E-18
6.55E-18
4250
2.31E-18
4.42E-18
6.73E-18
4500
2.70E-18
5.16E-18
7.86E-18
4750
2.75E-18
5.23E-18
7.98E-18
5000
2.65E-18
5.10E-18
7.75E-18
5250
2.56E-18
5.02E-18
7.58E-18
5500
2.55E-18
5.16E-18
7.71E-18
5750
2.53E-18
5.25E-18
7.78E-18
6000
2.43E-18
5.14E-18
7.57E-18
6250
2.31E-18
5.00E-18
7.31E-18
6500
2.18E-18
4.80E-18
6.98E-18
6750
2.08E-18
4.69E-18
6.77E-18
7000
1.94E-18
4.48E-18
6.42E-18
7250
1.83E-18
4.30E-18
6.13E-18
7500
1.74E-18
4.13E-18
5.87E-18
7750
1.64E-18
3.97E-18
5.62E-18
8000
1.56E-18
3.83E-18
5.39E-18
8250
1.48E-18
3.68E-18
5.15E-18
8500
1.38E-18
3.47E-18
4.84E-18
8750
1.30E-18
3.31E-18
4.61E-18
9000
1.22E-18
3.17E-18
4.40E-18
9250
1.15E-18
3.03E-18
4.18E-18
9500
1.10E-18
2.92E-18
4.02E-18
9750
1.05E-18
2.81E-18
3.86E-18
10000
9.99E-19
2.70E-18
3.70E-18
10250
9.48E-19
2.60E-18
3.55E-18
10500
8.99E-19
2.49E-18
3.39E-18
10750
8.42E-19
2.36E-18
3.20E-18
11000
8.02E-19
2.24E-18
3.04E-18


Table 6.7: Geocoronal Emission Lines
Wavelength
(Å)
ID
Line Width (Å)
Intensity
Day
Night
kilo-
Rayleighs
erg s-1 cm-2 arcsec-2
kilo-
Rayleighs
erg s-1 cm-2 arcsec-2
1216
Ly
0.04
~20
6.1 x 10-13
2
6.1 x 10-14
1304
O I
0.013
~2
5.7 x 10-14
0.013
3.8 x 10-16
1356
O I]
0.013
~0.2
~5 x 10-15
~ 0.001
~3 x 10-17
2471
[O I]
0.023
< 0.2
<3  x 10-15
< 0.001
<1.5 x 10-17


 6.7 Exposure Time Examples Chapter 7:  Feasibility and Detector Performance
Space Telescope Science Institute
http://www.stsci.edu
Voice: (410) 338-1082
help@stsci.edu