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 3800-8000 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
6554.25 W I 165 45 5d4.6s.(6D).6p 51 28198.9 5d4.6s.(6D).7s 7D1 43451.98
6562.26 W I 8 2
6579.77 W I 10 3
6599.98 W I 15 4 5d4.6s.(6D).6p 54 32828.12 5d4.6s.(6D).7s 7D4 47975.54
6609.05 W I 120 29 5d4.6s2 3D3 15460.01 5d4.6s.(6D).6p 53 30586.64
6616.19 W I 15 4
6626. W I 55 12
6634.54 W I 40 8
6636.02 W I 120 25
6636.68 W I 195 42 5d4.6s.(6D).6p 54 31432.91 5d4.6s.(6D).7s 7D3 46496.62
6639.56 W I 20 4
6645.27 W I 25 5
6651.91 W I 25 5
6652.37 W I 25 5
6659.36 W I 20 4
6663.18 W I 15 3
6663.61 W I 15 3
6664.16 W I 210 43 5d4.6s2 3G4 16431.31 5d4.6s.(6D).6p 54 31432.91
6666.75 W I 25 5
6674.12 W I 8 2
6679.79 W I 7 1
6693.08 W I 45 8 5d4.6s2 3D2 14976.18 5d4.6s.(6D).6p 53 29912.85
6705.68 W I 35 6
6708.6 W I 15 2
6710.57 W I 20 3
6713.28 W I 105 18 5d4.6s2 3P21 13307.1 5d4.6s.(6D).6p 51 28198.9
6713.96 W I 30 5
6744.36 W I 45 7
6745.47 W I 345 50
6750.19 W I 50 7
6755.75 W I 180 26
6756.38 W I 90 13
6766.04 W I 30 4
6782.78 W I 50 6
6787.69 W I 30 4
6795.56 W I 70 9
6796.34 W I 225 27
6799.3 W I 450 55 5d4.6s2 3H5 15069.93 5d4.6s.(6D).6p 75 29773.34
6812.58 W I 30 3
6816.24 W I 330 38
6817.7 W I 30 3
6819.89 W I 105 12
6844.88 W I 360 37 5d4.6s.(6D).6p 55 33370.04 5d4.6s.(6D).7s 7D4 47975.54
6861.16 W I 30 3
6871.13 W I 35 3
6875.16 W I 120 11 5d4.6s2 3G3 13348.56 5d5.(6S).6p 74 27889.68
6876.73 W I 90 8
6887.81 W I 390 33 5d4.6s2 3H4 12161.96 5d4.6s.(6D).6p 75 26676.48
6893.2 W I 55 5
6903.8 W I 30 2
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