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
1955.14 Ir IV 1500 - 5d5.(4G).6s 3G4 71191.62 5d5.6p 122338°5 122338.65
1961.498 Ir IV 60 - 5d5.(4G).6s 3G3 69741.38 5d5.6p 120722°4 120722.59
1971.971 Ir IV 135 - 5d5.(4G).6s 3G4 71191.62 5d5.6p 121902°3 121902.29
1976.714 Ir II 330 - 5d8 3P2 3090.16 5d7.(4F3/2).6p (3/2,1/2)°2 53678.68
1987.989 Ir II 4500 - 5d7.(4F).6s 5F5 0 5d6.6s.(6D9/2).6p (9/2,1/2)°4 50302.01
1993.71 Ir II 1000 - 5d8 1D2 8974.95 5d7.(4P3/2).6p (3/2,1/2)°2 59132.98
1993.801 Ir IV 1000 - 5d5.(6S).6s 5S2 50417.92 5d5.(6S).6p 73 100573.47
1995.777 Ir II 1005 - 5d8 3P2 3090.16 5d7.(4P5/2).6p (5/2,1/2)°3 53196.15
1997.179 Ir II 2500 - 5d8 3P1 9062.22 5d7.(4P3/2).6p (3/2,1/2)°2 59132.98
1999.197 Ir IV 30 - 5d5.6s 840054 84005.15 5d5.6p 134025°4 134025.31
  |««     «     ‹   Page:

Privacy Policy | Back to interactive spectra

These tables are Public Domain/CC0 (