Table A.1: Bands of ${\rm N_{2}}$ ( ${\rm B^{3}\Pi _g - A^{3}\Sigma ^{+}_{u}}$), with the wavelength $\lambda $, and Einstein coefficient Av'v'' (Forrest et al. 1992).

Band(v', v'')		 $\lambda $ [$\mu$m] Av'v'' [s-1]
$\Delta v=+4$    
10, 6 0.5842 8.13e+4
9, 5 0.5894 6.4e+4
8, 4 0.5974 4.6e+4
7, 3 0.6001 2.93e+4
6, 2 0.6057 1.59e+4
5, 1 0.6114 6.59e+3
$\Delta v$ = +3    
17,14 0.5857 8.0e+3
16,13 0.5917 1.48e+3
15,12 0.5979 3.0e+2
14,11 0.6042 5.68e+3
13,10 0.6106 1.77e+4
12, 9 0.6172 3.52e+4
11, 8 0.6239 5.58e+4
10, 7 0.6309 7.59e+4
8, 5 0.6454 9.91e+4
7, 4 0.6530 9.61e+4
6, 3 0.6608 8.21e+4
5, 2 0.6689 5.95e+4
4, 1 0.6772 3.35e+4
3, 0 0.6858 1.16e+4
$\Delta v$ = +2    
21,19 0.5916 4.79e+2
19,17 0.6072 5.84e+3
18,16 0.6150 1.47e+4
17,15 0.6230 2.52e+4
16,14 0.6312 3.48e+4
15,13 0.6394 4.10e+4
8, 6 0.7042 5.71e+3
7, 5 0.7147$\dagger$ 2.2e+4
6, 4 0.7255$\dagger$ 4.60e+4
5, 3 0.7368$\dagger$ 7.03e+4
4, 2 0.7484$\dagger$ 8.4e+4
3, 1 0.7606$\dagger$ 7.61e+4
2, 0 0.7732$\dagger$ 4.29e+4
$\dagger$ With the increase of K, their rotational line
come into our wavelength range.

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