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
4845.38 Ir I 420 292 5d8.(3F).6s b 4F3/2 11831.09 5d7.6s.(5F).6p z 63/2 32463.58
4938.09 Ir I 510 380 5d8.(3F).6s a 2F5/2 12218.47 5d7.6s.(5F).6p z 63/2 32463.58
4939.173 Ir I 195 143 5d7.6s2 a 2G9/2 13939.8 5d7.6s.(5F).6p z 611/2 34180.48
4970.48 Ir I 435 327 5d8.(3P).6s a 4P5/2 12951.67 5d7.6s.(5F).6p z 65/2 33064.83
4999.74 Ir I 255 198 5d7.6s.(5F).6p z 69/2 32513.43 5d7.6s.(5F).7s e 6F9/2 52508.89
5002.74 Ir I 300 239 5d7.6s2 a 4F7/2 6323.91 5d7.6s.(5F).6p z 69/2 26307.5
5009.17 Ir I 165 132 5d8.(3P).6s a 2P1/2 12505.68 5d7.6s.(5F).6p z 63/2 32463.58
5014.98 Ir I 345 276 5d7.6s2 a 2G9/2 13939.8 5d7.6s.(5F).6p z 67/2 33874.43
5123.66 Ir I 795 670 5d8.(3P).6s a 4P5/2 12951.67 5d7.6s.(5F).6p z 63/2 32463.58
5177.95 Ir I 690 603 5d7.6s2 b 4P5/2 16103.32 5d7.6s.(5F).6p z 67/2 35410.63
5238.92 Ir I 450 405 5d8.(3P).6s a 4P3/2 16565.35 5d7.6s.(5F).6p z 61/2 35647.94
5449.5 Ir I 450 450 5d7.6s.(5F).6p z 613/2 32830.78 5d7.6s.(5F).7s e 6F11/2 51175.94
5454.5 Ir I 180 178 5d7.6s.(5F).6p z 611/2 34180.48 5d7.6s.(5F).7s e 6F9/2 52508.89
5469.4 Ir I 55 54 5d7.6s2 a 2H11/2 19593.25 5d7.6s.(5F).6p z 49/2 37871.69
5625.55 Ir I 135 137 5d7.6s2 b 4P5/2 16103.32 5d7.6s.(5F).6p z 67/2 33874.43
5882.3 Ir I 65 56 5d7.6s.(5F).6p z 611/2 34180.48 5d7.6s.(5F).7s e 6F11/2 51175.94
5894.06 Ir I 120 99 5d7.6s2 b 4P5/2 16103.32 5d7.6s.(5F).6p z 65/2 33064.83
6026.1 Ir I 120 87 5d7.6s2 a 2G9/2 13939.8 5d7.6s.(5F).6p z 67/2 30529.66
6110.67 Ir I 120 86 5d7.6s2 b 4P5/2 16103.32 5d7.6s.(5F).6p z 63/2 32463.58
6288.28 Ir I 70 36 5d8.(3P).6s a 4P3/2 16565.35 5d7.6s.(5F).6p z 63/2 32463.58
6334.44 Ir I 120 55 5d8.(3P).6s a 4P1/2 16681.2 5d7.6s.(5F).6p z 63/2 32463.58
6830.01 Ir I 1500 190 5d7.6s.(5F).6p z 49/2 37871.69 5d7.6s.(5F).7s e 6F9/2 52508.89
6929.88 Ir I 1500 124 5d7.6s2 b 4P5/2 16103.32 5d7.6s.(5F).6p z 67/2 30529.66
7183.71 Ir I 1500 32 5d7.6s2 b 4P3/2 18547.04 5d7.6s.(5F).6p z 63/2 32463.58
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