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
4293.535 W I - -
4294.606 W I 225 101 5d5.(6S).6s 7S3 2951.29 5d5.(6S).6p 72 26229.77
4302.11 W I 210 98 5d5.(6S).6s 7S3 2951.29 5d4.6s.(6D).6p 73 26189.2
4302.897 W I - - 5d5.(6S).6p 74 27889.68 5d4.6s.(6D).7s 5D4 51123.14
4305.318 W I - -
4306.87 W I 180 82 5d4.6s.(6D).6p 74 24763.39 5d4.6s.(6D).7s 7D4 47975.54
4311.29 W I - -
4315.486 W I - -
4316.574 W I - -
4317.65 W I - -
4318.76 W I - -
4319.865 W I - -
4320.985 W I - -
4322.124 W I - -
4323.28 W I 1 1
4328.782 W I - -
4331.62 W I 165 75
4333.76 W I - -
4336.326 W I 2 1
4337.63 W I 1 1
4340.27 W I - -
4341.124 W I 180 86
4341.61 W I 1 1
4342.781 W I 270 128
4344.634 W I 225 106
4351.097 W I - -
4353.1 W I 330 155
4361.814 W I 555 263 5d4.6s2 5D4 6219.33 5d4.6s.(6D).6p 53 29139.12
4362.228 W I - -
4364.778 W I 570 269 5d4.6s2 5D2 3325.53 5d5.(6S).6p 72 26229.77
4372.522 W I 465 219 5d4.6s2 5D2 3325.53 5d4.6s.(6D).6p 73 26189.2
4373.063 W I - -
4378.484 W I 375 176 5d4.6s2 5D3 4830 5d4.6s.(6D).6p 52 27662.52
4391.115 W I 3 2
4398.698 W I - -
4400.85 W I 225 106
4401.316 W I - -
4403.947 W I 570 271 5d4.6s2 3H6 17008.5 5d4.6s.(4H).6p 57 39709.04
4406.88 W I - -
4408.282 W I 600 287 5d4.6s.(6D).6p 75 26676.48 5d4.6s.(6D).7s 7D5 49354.68
4409.946 W I 150 71
4412.188 W I 555 266 5d4.6s2 5D2 3325.53 5d4.6s.(6D).6p 51 25983.6
4431.963 W I 1 1
4433.634 W I 105 52
4436.898 W I 855 407 5d4.6s.(6D).6p 72 23964.67 5d4.6s.(6D).7s 7D3 46496.62
4444.44 W I 435 209 5d4.6s.(6D).6p 72 23964.67 5d4.6s.(6D).7s 5D1 46458.3
4466.742 W I 690 329
4469.714 W I 150 71
4477.824 W I 150 74 5d4.6s.(6D).6p 74 28797.24 5d4.6s.(6D).7s 5D4 51123.14
4496.228 W I 405 199
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