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
3941.87 Sm II 465 2
3943.24 Sm II 360 2
3946.51 Sm II 330 2
3948.11 Sm II 405 2
3951.89 Sm I 75 -
3959.53 Sm II 315 2
3963. Sm II 300 2
3966.04 Sm II 345 2
3967.68 Sm II 45 -
3970.53 Sm II 80 1
3971.4 Sm II 270 2
3974.66 Sm I 75 1
3976.27 Sm II 195 2
3976.43 Sm II 120 1
3979.2 Sm II 240 2
3983.14 Sm II 420 3
3986.68 Sm II 1000 11
3987.43 Sm II 20 -
3990. Sm II 60 1
3990.02 Sm I 2 - 4f6.6s2 7F5 3125.46 4f5.(6F°).5d.6s2 74 28180.95
3993.31 Sm II 150 1
4003.46 Sm II 435 5
4007.48 Sm II 885 11
4019.98 Sm II 300 4
4023.23 Sm II 285 4
4035.11 Sm II 375 7
4041.68 Sm II 150 3
4042.72 Sm II 55 1
4042.9 Sm II 55 1
4044.11 Sm II 20 -
4045.05 Sm II 50 1
4046.16 Sm II 40 1
4047.16 Sm II 1000 26
4048.62 Sm II 10 -
4049.81 Sm II 85 2
4058.87 Sm II 360 10
4063.54 Sm II 135 4
4064.32 Sm II 195 6
4064.58 Sm II 195 6
4066.74 Sm II 255 8
4068.33 Sm II 450 15
4075.84 Sm II 240 10
4076.65 Sm II 150 6
4080.56 Sm II 75 3
4082.6 Sm II 65 3
4083.58 Sm II 420 17
4084.4 Sm II 150 6
4092.27 Sm II 210 10
4094.05 Sm II 90 4
4104.13 Sm II 105 6
  ‹   Page:   ›     »»|  
2

Privacy Policy | Back to interactive spectra

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