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
1849.723 Nb IV 255 - 4d.5s 3D3 53810.47 4d.5p 13 107872.61
1859.982 Nb IV 90 - 4d.5s 3D1 52064.67 4d.5p 32 105828.53
1863.13 Nb III - -
1877.34 Nb V - -
1879.355 Nb IV 390 - 4d.5s 3D1 52064.67 4d.5p 30 105274.38
1879.601 Nb IV 6 - 4d.4f 35 181809.42 4d.(2D5/2).5g 2[13/2]6 235012.29
1879.749 Nb IV 390 - 4d.5s 3D2 52629.96 4d.5p 32 105828.53
1880.387 Nb IV - - 4d.4f 33 181535.98 4d.(2D5/2).5g 2[5/2]3 234716.68
1883.881 Nb IV 5 - 4d.4f 14 179838.54 4d.(2D3/2).5g 2[11/2]5 232920.41
1890.276 Nb IV 480 - 4d.5s 3D1 52064.67 4d.5p 31 104967.04
1892.92 Nb III - -
1894.439 Nb IV - - 4d.4f 33 181535.98 4d.(2D5/2).5g 2[9/2]4 234322.02
1896.802 Nb IV - - 4d.5d 1G4 174061.29 4d.5f 34 226781.46
1901.586 Nb IV - - 4d.4f 35 181809.42 4d.(2D5/2).5g 2[11/2]6 234397.1
1902.85 Nb IV 10 - 4d.4f 14 179838.54 4d.(2D3/2).5g 2[9/2]5 232391.22
1909.97 Nb IV 2 - 4d.4f 34 182170.31 4d.(2D5/2).5g 2[7/2]4 234527.04
1910.693 Nb IV 300 - 4d.5s 3D2 52629.96 4d.5p 31 104967.04
1916.589 Nb IV 60 - 4d.4f 36 182746.93 4d.(2D5/2).5g 2[13/2]7 234922.96
1918.576 Nb IV 9 - 4d.4f 34 182170.31 4d.(2D5/2).5g 2[9/2]5 234292.25
1922.408 Nb IV 555 - 4d.5s 3D3 53810.47 4d.5p 32 105828.53
1935.893 Nb IV 9 - 4d.4f 34 181264.62 4d.(2D3/2).5g 2[11/2]5 232920.41
1936.104 Nb IV - - 4d.4f 36 182746.93 4d.(2D5/2).5g 2[11/2]6 234397.1
1938.84 Nb III - -
1944.882 Nb IV 6 - 4d.4f 32 181171.43 4d.(2D3/2).5g 2[7/2]3 232588.26
1950.5 Nb IV 2 - 4d.4f 12 183241.63 4d.(2D5/2).5g 2[7/2]3 234510.41
1954.252 Nb IV 15 - 4d.4f 35 181809.42 4d.(2D3/2).5g 2[11/2]6 232980.02
1955.931 Nb IV - - 4d.4f 34 181264.62 4d.(2D3/2).5g 2[9/2]5 232391.22
1958.105 Nb IV 4 - 4d.4f 33 181535.98 4d.(2D3/2).5g 2[7/2]4 232605.89
1962.804 Nb IV - - 4d.5d 1G4 174061.29 4d.5f 14 225008.83
1965.254 Nb IV - - 4d.4f 33 181535.98 4d.(2D3/2).5g 2[9/2]4 232420.05
1978.196 Nb IV 660 - 4d.5s 1D2 58566.68 4d.5p 11 109117.91
1979.07 Nb III - -
1985.15 Nb III - -
1991.208 Nb IV - - 4d.4f 34 182170.31 4d.(2D3/2).5g 2[9/2]5 232391.22
1997.11 Nb III - -
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