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
1661.478 Be I 5 - 1s2.2s2 1S0 0 1s2.2s.3p 11 60187.4434
1754.69 Be III 5 - 1s.3s 3S1 1121184 1s.4p 31 1178174
1776.1 Be II 5 - 1s2.2p 21/2 31928.744 1s2.3s 2S1/2 88231.915
1776.307 Be II 5 - 1s2.2p 23/2 31935.32 1s2.3s 2S1/2 88231.915
1907.12 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.12d 3D1 74414.6
1912.49 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.11d 3D1 74267.4
1917.03 Be III 5 -
1919.76 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.10d 3D1 74069.3
1929.67 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.9d 3D1 73801
1943.68 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.8d 3D3 73429.34
1954.97 Be III 5 - 1s.3p 30 1128300 1s.4d 3D1 1179451
1956.63 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.8s 3S1 73088.4
1964.59 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.7d 3D3 72880.92
1985.13 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.7s 3S1 72354.7
1998.01 Be I 5 - 1s2.2s.2p 32 21981.26 1s2.2s.6d 3D1 72029.49
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