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 800-8000 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
7991.43 Y III 480 -
7999.358 Y I 10 - 4d.5s.(3D).5p z 47/2 17116.156 4d3 b 4F7/2 29613.726
8171.41 Y III 390 -
8329.571 Y I 25 - 4d2.(3F).5p y 49/2 32188.075 5p2.(3P).4d 4F9/2 44190.205
8344.404 Y I 35 - 4d2.(1D).5s b 2D5/2 16158.865 4d.5s.(1D).5p x 23/2 28139.645
8365.551 Y I 10 - 4d.5s.(3D).5p y 23/2 24480.666 4d.5s.(3D).6s f 2D5/2 36431.165
8450.335 Y I 40 - 4d2.(1D).5s b 2D3/2 15994.045 4d.5s.(1D).5p x 21/2 27824.647
8528.788 Y I 20 - 4d.5s.(3D).5p y 21/2 24698.85 4d.5s.(3D).6s f 2D3/2 36420.611
8645.09 Y III 195 -
8796.21 Y III 480 -
8800.59 Y I 40 - 4d.5s2 a 2D3/2 0 5s2.5p z 23/2 11359.757
8835.875 Y II 10 - 4d2 b 1D2 14832.862 4d.5p z 12 26147.252
9116.59 Y III 390 -
17422.838 Y I 5 - 4d2.(3F).5s a 4F5/2 11078.614 4d.5s.(3D).5p z 45/2 16816.641
17903.209 Y I 5 - 4d2.(3F).5s a 4F9/2 11532.096 4d.5s.(3D).5p z 47/2 17116.156
18049.81 Y I 5 - 4d2.(3F).5s a 4F7/2 11277.928 4d.5s.(3D).5p z 45/2 16816.641
21266.247 Y I 5 - 4d2.(3F).5s a 4F9/2 11532.096 4d.5s.(3D).5p z 49/2 16234.382
22549.98 Y I 5 - 4d2.(3F).5s a 4F7/2 11277.928 4d.5s.(3D).5p z 47/2 15712.522
23996.996 Y I 5 - 4d2.(3F).5s a 4F5/2 11078.614 4d.5s.(3D).5p z 45/2 15245.803
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