a table of observational chromospheric emission lines

Here is a table of observational chromospheric emission lines for low-mass stars:

Emission lines	Wavelength (nm)	Transition terms	Landé factors	\(g_\mathrm{eff}\)
H I (Hα)	656.28	-	-	1
H I (Hβ)	486.13	-	-	1
H I (Hγ)	434.05	-	-	1
H I (Hδ)	410.17	-	-	1
H I (Hε)	397.01	-	-	1
H I (Hζ)	388.90	-	-	1
He I D3	587.56	\(^3P^{\circ}_{2}\;-\;{}^3D_{3}\)	\(\tfrac{3}{2}\;-\;\tfrac{4}{3}\)	7/6
He I	447.15	\(^3P^{\circ}_{2}\;-\;{}^3D_{2}\)	\(\tfrac{3}{2}\;-\;\tfrac{7}{6}\)	4/3
He I	402.62	\(^3P^{\circ}_{1}\;-\;{}^3D_{2}\)	\(\tfrac{3}{2}\;-\;\tfrac{6}{7}\)	1
He I	388.86	\(^3S_{1}\;-\;{}^3P_{2}\)	\(2\;-\;\tfrac{3}{2}\)	5/4
He II	468.57038	\(^2D_{3}\;-\;{}^2F^{\circ}_{6}\)	\(\tfrac{3}{2}\;-\;\tfrac{5}{2}\)	9/10
Na II D1	588.995	\(^2S_{1/2}\;-\;{}^2P^{\circ}_{3/2}\)	\(1\;-\;\tfrac{4}{3}\)	7/6
Na II D2	589.592	\(^2S_{1/2}\;-\;{}^2P^{\circ}_{1/2}\)	\(2\;-\;\tfrac{2}{3}\)	4/3
Ca II K	393.37	\(^2S_{1/2}\;-\;{}^2P^{\circ}_{3/2}\)	\(1\;-\;\tfrac{4}{3}\)	7/6
Ca II H	396.85	\(^2S_{1/2}\;-\;{}^2P^{\circ}_{1/2}\)	\(2\;-\;\tfrac{2}{3}\)	4/3
Ca II IRT − 1	849.80	\(^2D_{3/2}\;-\;{}^2P^{\circ}_{1/2}\)	\(0.8\;-\;\tfrac{4}{3}\)	1.07
Ca II IRT − 2	854.21	\(^2D_{5/2}\;-\;{}^2P^{\circ}_{3/2}\)	\(1.2\;-\;\tfrac{4}{3}\)	1.1
Ca II IRT − 3	866.21	\(^2D_{3/2}\;-\;{}^2P^{\circ}_{1/2}\)	\(0.8\;-\;\tfrac{2}{3}\)	5/6
Fe II?	390.56	?	?	?

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