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
80251.41 V I 4 - 3d4.(5D).4s a 4D5/2 8578.542 3d3.4s2 a 4P5/2 9824.626
81697.34 V I 4 - 3d4.(5D).4s a 4D1/2 8413.009 3d3.4s2 a 4P3/2 9637.039
85666.35 V II 4 - 3d3.(2G).4s b 1G4 19112.9298 3d3.(2H).4s b 3H5 20280.2493
86147.11 V I 4 - 3d4.(5D).4s a 4D3/2 8476.234 3d3.4s2 a 4P3/2 9637.039
88368.42 V I 4 - 3d4.(5D).4s a 4D1/2 8413.009 3d3.4s2 a 4P1/2 9544.635
88538.3 V II 4 - 3d3.(2G).4s b 1G4 19112.9298 3d3.(2H).4s b 3H4 20242.385
89290. V X 4 - 3s.3p3 31 220984 3s.3p3 33 222104
90181.16 V I 4 - 3d4.(5D).4s a 4D7/2 8715.747 3d3.4s2 a 4P5/2 9824.626
93999.37 V II 4 - 3d4 a 3H4 12545.1024 3d4 b 3F24 13608.9393
95541.2 V II 4 - 3d4 b 3F24 13608.9393 3d4 a 3G5 14655.6082
96800. V XVI 4 - 2s2.2p4 3P1 48937 2s2.2p4 3P0 49970
96900. V X 4 - 3s.3p3 32 221072 3s.3p3 33 222104
100973.9 V II 4 - 3d3.(2P).4s b 3P1 19166.315 3d3.(4P).4s c 3P0 20156.67
103000.91 V II 4 - 3d4 b 3F22 13490.8843 3d4 a 3G3 14461.7495
105582.17 V II 4 - 3d4 b 3F24 13608.9393 3d4 a 3G4 14556.0689
108801.69 V II 4 - 3d4 b 3F23 13542.6461 3d4 a 3G3 14461.7495
111507.6 V II 4 - 3d4 a 3D1 18269.515 3d3.(2P).4s b 3P1 19166.315
115837.7 V II 4 - 3d4 a 3D1 18269.515 3d3.(2P).4s b 3P2 19132.792
119200.9 V II 4 - 3d4 a 3D2 18293.8723 3d3.(2P).4s b 3P2 19132.792
128376. V II 4 - 3d4 a 3D3 18353.83 3d3.(2P).4s b 3P2 19132.792
133821.3 V I 4 - 3d3.4s2 a 2P3/2 13801.551 3d3.4s2 2D25/2 14548.816

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