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
4540.19 Sm II 780 390
4542.06 Sm II 810 406
4543.95 Sm II 1500 675
4544.83 Sm II 135 64
4552.66 Sm II 900 451
4554.45 Sm II 645 320
4560.43 Sm II 405 202
4566.21 Sm II 795 405
4577.69 Sm II 1500 767
4581.58 Sm I 240 123
4581.73 Sm I 1000 623
4584.83 Sm II 1500 764
4591.82 Sm II 990 512
4593.54 Sm II 465 236
4595.29 Sm II 945 490
4596.74 Sm I 210 108
4604.18 Sm II 780 411
4606.51 Sm II 420 222
4615.44 Sm II 210 110
4615.69 Sm II 405 220
4630.21 Sm II 390 212
4642.24 Sm II 990 542
4645.4 Sm I 405 224
4646.68 Sm II 510 284
4648.16 Sm II 120 69
4649.49 Sm I 270 146
4655.13 Sm II 180 103
4663.56 Sm I 1000 581
4669.4 Sm II 600 336
4669.65 Sm II 735 416
4670.75 Sm I 420 237
4674.6 Sm II 930 524
4676.91 Sm II 1000 599
4681.55 Sm I 420 239
4687.18 Sm II 600 344
4688.73 Sm I 270 159
4693.63 Sm II 210 119
4699.34 Sm II 165 98
4704.4 Sm II 615 360
4713.06 Sm II 285 170
4715.26 Sm II 300 178
4716.1 Sm I 450 271 4f6.6s2 7F5 3125.46 4f6.(7F).6s.6p.(1P°) 75 24323.51
4717.07 Sm I 240 147
4717.72 Sm II 315 186
4718.33 Sm II 315 188
4719.84 Sm II 405 242
4726.02 Sm II 360 216
4728.42 Sm I 555 333 4f6.6s2 7F3 1489.55 4f6.(7F).6s.6p.(1P°) 73 22632.3
4745.68 Sm II 480 298
4750.72 Sm I 195 124
  |««     ‹   Page:   ›     »»|  
4

Privacy Policy | Back to interactive spectra

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