Line Tables

These tables give observed air wavelengths for the 2000-20000 Å range for spectra other than Fr I. Outside of the 2000-20000 Å range, the wavelengths are vacuum wavelengths. Lines of Fr I are extrapolated vacuum wavelengths from known energy levels. All observed lines are from NIST ASD. All energy level information is from NIST ASD. Wavelengths from MIT Wavelength Tables have been omitted as this publication appears to still be under copyright. However, in some cases, the exact same wavelength is given by NIST and MIT; in that case, the line is included.

Line intensities have been adjusted in the visible region to match photographed visible spectra. Line intensities of Rn have been adjusted to match the Grotrian diagram of Rn I. Line intensities in the infrared and ultraviolet are less reliable, but every effort was made to estimate them as accurately as possible. The elements He, O, Cl, Ar, Kr, and Xe have had their NIR lines photographed out to roughly 11000 Å. The intensities of the "brightest" several IR lines of each of these elements, in the 7000-10000 Å range, can be trusted. For the range of 800-8000 Å, estimated visual brightnesses (EVB) are given. A dash in either of the intensity columns means the line intensity would be less than one relative to other lines of the same spectrum.

All Spectra

H   He
Li Be   B C N O F Ne
Na Mg   Al Si P S Cl Ar
K Ca   Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr
Rb Sr   Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe
Cs Ba La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn
Fr Ra Ac Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr Rf Db Sg Bh Hs Mt Ds Rg Cn Nh Fl Mc Lv Ts Og

Entire Range | 2000-10000 Å | Visible Region | Si CCD/CMOS Region | Thermal IR | Vacuum UV
Specific Wavelength (rounded):  Å  nm

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λ, Å E. Sp.# Rel.Int. EVB Lower Config Lower Term+J Lower Level Upper Config Upper Term+J Upper Level
4002.59 Ho II 75 1
4003.39 Ho I 100 1
4013.5 Ho I 1000 15
4014.2 Ho II 40 1
4018.09 Ho II 25 -
4022.76 Ho II 1000 18
4023.94 Ho II 30 -
4025.39 Ho I 25 -
4027.21 Ho I 40 1
4028.86 Ho I 30 -
4031.8 Ho I 25 -
4037.62 Ho I 15 -
4038.87 Ho II 25 -
4040.81 Ho I 900 18 4f11.6s2 415/2 0 4f10.5d.6s2 13/2 24740.52
4047.52 Ho I 15 -
4053.93 Ho I 945 23 4f11.6s2 415/2 0 4f11.(4I°15/2).6s.6p.(1P°1) (15/2,1)15/2 24660.8
4054.48 Ho II 7 -
4057.55 Ho I 4 -
4060.31 Ho I 6 -
4065.09 Ho II 20 1
4067.57 Ho I 465 15
4068.05 Ho I 15 1
4071.83 Ho I 810 27
4073.13 Ho I 8 -
4073.51 Ho I 765 26
4080.23 Ho II 150 6
4083.67 Ho I 4 -
4085.09 Ho I 180 8
4087.35 Ho I 5 -
4087.59 Ho I 5 -
4091.64 Ho I 135 6
4094.78 Ho I 135 6
4100.22 Ho I 5 -
4103.84 Ho I 495 28 4f11.6s2 415/2 0 4f11.(4I°15/2).6s.6p.(1P°1) (15/2,1)17/2 24360.81
4105.04 Ho I 150 10
4106.5 Ho I 5 -
4107.36 Ho I 120 8
4108.62 Ho I 135 9 4f11.6s2 413/2 5419.7 4f11.(4I°13/2).6s.6p.(1P°1) (13/2,1)13/2 29751.91
4112. Ho I 6 -
4112.72 Ho I 3 -
4116.73 Ho I 8 1
4120.2 Ho I 195 16
4125.65 Ho I 100 9
4127.16 Ho I 735 71 4f11.6s2 413/2 5419.7 4f11.(4I°13/2).6s.6p.(1P°1) (13/2,1)15/2 29642.6
4134.54 Ho I 25 3
4136.22 Ho I 210 24
4139.34 Ho I 690 78
4142.19 Ho I 10 1
4148.97 Ho I 15 2
4152.61 Ho II 120 16
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