Subject: Re: SDSS Filter Responses for USNO40?
From: jeg@astro.Princeton.EDU
Submitted: Mon, 17 Aug 1998 14:22:44 -0400 (EDT)
Message number: 1592 (previous: 1591, next: 1593 up: Index)
Attached is the extinction table for PALOMAR (1700m). You can scale
this to other altitudes assuming that the scale height of the atmosphere
is about 7000 m and multiplying the entries (magnitudes) in the table by
airmass*exp((1700-alt)/7000). This is not quite correct, because there
are contributions to the extinction (primarily ozone) which are
independent of altitude, but the major contribution is molecular
Rayleigh scattering, which scales in the indicated manner. The onset of
ozone is so sudden that treating it the same way is not a problem.
There is contribution from water in the red which is highly variable
anyway, so no simple treatment is very good.
ATMOSPHERIC EXTINCTION (MAGNITUDES) AT AIRMASS 1.00 at Palomar
2900 15.000
3000 9.000
3150 1.450
3160 1.345
3170 1.282
3180 1.225
3190 1.173
3200 1.125
3210 1.085
3220 1.050
3230 1.020
3240 0.993
3250 0.967
3260 0.945
3270 0.926
3280 0.905
3290 0.885
3300 0.867
3320 0.833
3340 0.804
3360 0.780
3380 0.763
3400 0.746
3450 0.715
3500 0.650
3600 0.585
3700 0.526
3800 0.485
3900 0.440
4000 0.385
4100 0.347
4200 0.316
4300 0.291
4400 0.267
4500 0.244
4600 0.225
4700 0.209
4800 0.197
4900 0.186
5000 0.178
5200 0.167
5400 0.156
5600 0.150
5800 0.145
6000 0.127
6100 0.113
6200 0.102
6500 0.085
6820 0.078
6880 0.158
6980 0.074
7000 0.073
7140 0.070
7180 0.160
7220 0.120
7300 0.110
7340 0.068
7360 0.067
7560 0.065
7570 0.065
7588 0.118
7594 0.379
7607 0.943
7620 0.481
7633 0.601
7646 0.477
7653 0.331
7660 0.256
7673 0.146
7680 0.063
7690 0.062
7700 0.061
7900 0.059
8100 0.058
8140 0.110
8300 0.110
8350 0.055
8360 0.055
8625 0.053
8890 0.052
8900 0.052
8980 0.190
9060 0.140
9260 0.140
9350 0.559
9420 0.420
9460 0.490
9500 0.430
9540 0.440
9580 0.360
9620 0.270
9700 0.100
9740 0.140
9860 0.045
9870 0.045
11200 0.043
12500 0.041
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