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
4333.97 Pr II 555 261 4f3.(4I°11/2).6s1/2 (11/2,1/2)°6 1649.01 4f3.(4I°).6p 5I5 24716.04
4344.3 Pr II 570 267 4f2.5d.6s? 5I4 7832.43 4f2.(3H).5d.6p? 5K°?5 30844.63
4347.49 Pr II 375 175 4f3.(4I°13/2).6s1/2 (13/2,1/2)°6 3403.21 4f3.(4I°).6p? 6 26398.52
4350.4 Pr II 255 120
4354.28 Pr III 2 1
4354.91 Pr II 285 133 4f2.(3H).5d.6s.(3D)? 5 7888.5 4f2.(3H).5d.6p? 5K°?5 30844.63
4359.79 Pr II 420 197 4f3.(4I°15/2).6s1/2 (15/2,1/2)°7 5079.35 4f3.(4I°).6p? 7 28009.8
4371.62 Pr II 825 392
4379.82 Pr III 7 3
4381.47 Pr III 120 53
4396.08 Pr II 555 264
4404.71 Pr III 150 68
4405.12 Pr II 135 67
4405.83 Pr II 555 263 4f3.(4I°15/2).6s1/2 (15/2,1/2)°8 4437.15 4f3.(4I°).6p 5K8 27128
4408.82 Pr II 630 297 4f3.(4I°9/2).6s1/2 (9/2,1/2)°4 0 4f3.(4I°).6p 5K5 22675.44
4419.04 Pr II 375 175
4421.1 Pr III 6 3
4424.58 Pr II 420 197
4429.25 Pr II 900 429 4f3.(4I°13/2).6s1/2 (13/2,1/2)°7 2998.36 4f3.(4I°).6p 5K7 25569.19
4431.85 Pr III 180 85
4432.28 Pr II 360 169
4447.93 Pr III 15 8
4449.83 Pr II 525 249 4f3.(4I°11/2).6s1/2 (11/2,1/2)°6 1649.01 4f3.(4I°).6p 5K6 24115.5
4450.14 Pr III 165 80
4451. Pr III 20 10
4451.9 Pr II 330 160
4454.68 Pr II 120 60
4461.02 Pr III 6 3
4461.81 Pr III 10 5
4468.66 Pr II 510 242 4f3.(4I°11/2).6s1/2 (11/2,1/2)°5 1743.72 4f3.(4I°).6p 5K6 24115.5
4496.46 Pr II 870 423 4f3.(4I°9/2).6s1/2 (9/2,1/2)°5 441.95 4f3.(4I°).6p 5K5 22675.44
4500.31 Pr III 15 7
4510.15 Pr II 870 428 4f3.(4I°13/2).6s1/2 (13/2,1/2)°6 3403.21 4f3.(4I°).6p 5K7 25569.19
4534.15 Pr II 795 391 4f3.(4I°15/2).6s1/2 (15/2,1/2)°7 5079.35 4f3.(4I°).6p 5K8 27128
4612.02 Pr III 20 11
4612.08 Pr II 285 150 4f3.(4I°9/2).6s1/2 (9/2,1/2)°4 0 4f2.5d.6s? 5 8197.8
4625.18 Pr III 25 13
4632.28 Pr I 255 135
4635.68 Pr I 240 133
4639.55 Pr I 345 188
4654.16 Pr III 40 22
4687.8 Pr I 285 161
4695.77 Pr I 315 181
4708.07 Pr II 210 120 4f3.(4I°9/2).6s1/2 (9/2,1/2)°5 441.95 4f2.5d.6s? 5 8197.8
4709.52 Pr I 165 94
4713.7 Pr III 25 14
4725.55 Pr III 10 6
4728.21 Pr III 9 6
4730.67 Pr I 195 121
4734.117 Pr II 330 203 4f3.(4I°13/2).6s1/2 (13/2,1/2)°7 2998.36 4f3.(4I°).6p 5K6 24115.5
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