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
Download CSV

  |««     ‹   Page:
λ, Å E. Sp.# Rel.Int. EVB Lower Config Lower Term+J Lower Level Upper Config Upper Term+J Upper Level
7927.72 Ce I 30 - 4f.(2F°) .5d2.(3F).6s (4F) 56 4455.756 4f.5d.(3H°).6s.6p.(3P°) 5I6 17066.246
7934.5 Ce II - - 4f.(2F°).5d2.(1G) 213/2 15517.772 4f2.(1I).5d 2K15/2 28117.519
7948.64 Ce III 20 -
7960.31 Ce III 30 -
7991.01 Ce III 30 -
8025.56 Ce II 45 - 4f.(2F°).5d2.(3F) 47/2 0 4f2.(3F).5d 4H7/2 12456.746
8030.8 Ce III 25 -
8070.71 Ce I - - 4f.5d.6s2 35 4199.367 4f.5d.(1G°).6s.6p.(3P°) 5 13784.151
8084.12 Ce III 20 -
8094.43 Ce I - - 4f.(2F°) .5d2.(3F).6s (4F) °5 3210.583 4f.5d.(3H°).6s.6p.(3P°) 5I5 15561.346
8120.36 Ce I 30 - 4f.(2F°) .5d2.(3F).6s (4F) 54 2437.629 4f.5d.(1G°).6s.6p.(3P°) 4 14748.945
8177.33 Ce III 25 -
8186.03 Ce III 20 -
8222.16 Ce III 20 -
8241.55 Ce II - - 4f.(2F°).5d2.(3F) °9/2 6638.258 4f2.(3F).5d 4H9/2 13117.922
8261.09 Ce I 50 - 4f.(2F°) .5d2.(3F).6s (4F) 54 2437.629 4f.5d.(3F°).6s.6p.(3P°) 3 16384.741
8418.23 Ce II - - 4f.5d.(3F°).6s °5/2 2634.666 4f2.(3F).5d 7/2 18393.327
8495.82 Ce I 20 - 4f.(2F°) .5d2.(3F).6s (4F) 53 2369.068 4f.5d.(3H°).6s.6p.(3P°) 3 14136.322
8539.08 Ce II - - 4f.(2F°).5d2.(3F) 49/2 1410.304 4f2.(3F).5d 4H9/2 13117.922
8612.64 Ce I 30 - 4f.(2F°) .5d2.(3F).6s (4F) 55 3764.008 4f.5d.(3H°).6s.6p.(3P°) 4 15371.647
8647.66 Ce I 30 - 4f.(2F°) .5d2.(3F).6s (4F) 56 4455.756 4f.5d.(3H°).6s.6p.(3P°) 5 21581.408
8702.38 Ce II - - 4f.(2F°).5d2.(3F) 413/2 3793.634 4f2.(3F).5d 4H13/2 15281.602
8772.14 Ce II 55 - 4f.(2F°).5d2.(3F) 411/2 2879.695 4f2.(3F).5d 4H11/2 14276.298
8810.84 Ce I - - 4f.(2F°) .5d2.(3F).6s (4F) 54 2437.629 4f.5d.(1G°).6s.6p.(3P°) 5 13784.151
8891.2 Ce II 2 - 4f.(2F°).5d2.(3F) °7/2 3703.594 4f2.(3F).5d 4H9/2 13117.922
9056.53 Ce III 20 -
9079.58 Ce III 20 -
9328.2 Ce III 25 -
9367.03 Ce III 20 -
9567.37 Ce III 20 -
10458.37 Ce III 25 -
10494.42 Ce III 25 -
10534.36 Ce III 20 -
10684.46 Ce III 25 -
  |««     ‹   Page:
10

Privacy Policy | Back to interactive spectra

These tables are Public Domain/CC0 (https://creativecommons.org/publicdomain/zero/1.0/).