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
4002.782	W	I	40	-
4002.956	W	I	-	-
4005.404	W	I	85	1	5d4.6s2	5D1	1670.29	5d4.6s.(6D).6p	5D°0	26629.46
4005.688	W	I	-	-
4008.7506	W	I	180	2	5d5.(6S).6s	7S3	2951.29	5d5.(6S).6p	7P°4	27889.68
4009.454	W	I	-	-	5d4.6s.(6D).6p	7D°3	26189.2	5d4.6s.(6D).7s	5D4	51123.14
4010.377	W	I	80	1	5d4.6s.(6D).6p	7F°3	23047.31	5d4.6s.(6D).7s	7D4	47975.54
4012.492	W	I	-	-
4012.988	W	I	-	-
4013.44	W	I	-	-
4016.108	W	I	60	1	5d4.6s.(6D).6p	7F°4	24763.39	5d4.6s.(6D).7s	5D3	49656.04
4018.898	W	I	-	-
4019.123	W	I	-	-
4019.227	W	I	180	3	5d4.6s2	5D2	3325.53	5d4.6s.(6D).6p	5P°1	28198.9
4022.115	W	I	120	2	5d4.6s.(6D).6p	7F°1	20064.3	5d4.6s.(6D).7s	7D2	44919.84
4022.83	W	I	40	1
4022.994	W	I	-	-
4023.492	W	I	-	-
4029.922	W	I	80	1
4032.382	W	I	85	1
4032.622	W	I	-	-
4034.898	W	I	-	-
4043.526	W	I	-	-
4045.594	W	I	195	5	5d5.(6S).6s	7S3	2951.29	5d4.6s.(6D).6p	5F°2	27662.52
4046.701	W	II	150	4	5d5	4G9/2	26158.581	5d4.(5D).6p	6F°9/2	50863.106
4065.32	W	I	105	3	5d4.6s.(6D).6p	7F°4	24763.39	5d4.6s.(6D).7s	7D5	49354.68
4069.95	W	I	10	-	5d4.6s2	5D3	4830	5d4.6s.(6D).6p	5P°2	29393.4
4070.608	W	I	225	8	5d4.6s2	5D1	1670.29	5d5.(6S).6p	7P°2	26229.77
4070.89	W	I	-	-
4074.358	W	I	390	13	5d5.(6S).6s	7S3	2951.29	5d5.(6S).6p	7P°3	27488.11
4076.124	W	I	-	-
4080.166	W	I	-	-
4081.2927	W	II	495	20	5d4.(5D).6s	4D3/2	14634.336	5d4.(5D).6p	6F°3/2	39129.46
4085.044	W	I	-	-
4086.525	W	I	-	-
4088.33	W	I	300	14	5d4.6s2	5D2	3325.53	5d4.6s.(6D).6p	5D°1	27778.5
4089.38	W	I	150	7	5d4.6s.(6D).6p	7F°5	26676.48	5d4.6s.(6D).7s	5D4	51123.14
4090.3	W	I	95	5
4091.04	W	I	120	5
4091.212	W	I	90	4
4093.134	W	I	105	5
4094.747	W	I	-	-
4096.756	W	I	-	-
4101.845	W	I	60	3
4102.702	W	I	255	15	5d4.6s2	5D4	6219.33	5d4.6s.(6D).6p	5P°3	30586.64
4102.942	W	I	-	-	5d4.6s2	5D3	4830	5d4.6s.(6D).6p	5D°2	29195.84
4107.816	W	I	120	8	5d4.6s2	5D2	3325.53	5d4.6s.(6D).6p	5F°2	27662.52
4111.815	W	I	165	11	5d4.6s2	5D1	1670.29	5d4.6s.(6D).6p	5F°1	25983.6
4118.976	W	I	75	6
4120.356	W	I	45	4

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