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
3725.98 Pu I 285 -
3726.11 Pu II 285 -
3726.79 Pu II 285 -
3732.03 Pu II 285 -
3744.78 Pu I 285 -
3753.63 Pu I 3000 -
3755.94 Pu I 3000 -
3757.82 Pu I 285 -
3758.34 Pu I 3000 -
3774.38 Pu I 3000 -
3776.71 Pu I 285 -
3792.22 Pu I 3000 -
3799.37 Pu I 3000 3
3805.93 Pu I 3000 4
3811.4 Pu I 3000 4
3812.3 Pu II 285 -
3827.57 Pu I 285 -
3835.52 Pu I 3000 5
3836.96 Pu I 285 -
3838.92 Pu I 285 -
3842.1 Pu I 285 -
3851.01 Pu I 3000 5
3851.85 Pu I 2000 4
3878.54 Pu I 3000 7
3895.89 Pu I 2000 6
3928.53 Pu I 285 1
3975.43 Pu II 285 2
4097.12 Pu I 285 16
4101.96 Pu I 285 16
4105.95 Pu II 285 19
4111.07 Pu I 285 19
4114.91 Pu I 285 19
4128.12 Pu I 285 27
4129.93 Pu II 285 27
4133.01 Pu I 3000 267
4135.97 Pu I 285 32
4140.04 Pu I 3000 317
4141.2 Pu II 285 32
4151.09 Pu I 3000 375
4151.45 Pu I 3000 375
4155.46 Pu I 285 44
4159.39 Pu II 285 44
4167.77 Pu I 285 51
4170.95 Pu I 285 51
4178.28 Pu II 285 59
4189.9 Pu II 285 67
4190.06 Pu II 285 67
4196.2 Pu II 285 76
4206.48 Pu I 5500 1680
4208.23 Pu I 3000 840
  |««     ‹   Page:   ›     »»|  
4

Privacy Policy | Back to interactive spectra

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