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
5588.417	Ag	II	4	4	4d9.(2D5/2).5d	2[7/2]4	127608.6762	4d9.(2D5/2).4f	2[9/2]°4	145497.86
5589.7828	Ag	II	9	9	4d9.(2D5/2).5d	2[5/2]2	127523.4831	4d9.(2D5/2).4f	2[7/2]°3	145408.3
5610.6066	Ag	II	20	18	4d9.(2D5/2).5d	2[7/2]3	127491.0946	4d9.(2D5/2).4f	2[5/2]°2	145309.528
5620.974	Ag	II	-	-	4d9.(2D5/2).5p	2[3/2]°2	80176.4601	4d8.5s2	3F3	97962.039
5622.4822	Ag	II	75	75	4d9.(2D5/2).5d	2[7/2]4	127608.6762	4d9.(2D5/2).4f	2[9/2]°5	145389.48
5667.34	Ag	I	-	-	4d9.5s.(3D).5p	4D°7/2	61773.12	4d9.5s.(3D).6s	4D7/2	79413
5734.226	Ag	II	-	-	4d9.(2D5/2).5p	2[7/2]°3	82171.732	4d8.5s2	3F2	99606.031
6083.78	Ag	I	-	-	4d9.5s.(3D).5p	2F°7/2	65637.75	4d9.5s.(3D).6s	2D5/2	82071.1
6255.896	Ag	II	15	7	4d9.(2D5/2).5p	2[3/2]°1	83625.5147	4d8.5s2	3F2	99606.031
6268.5	Ag	I	4	2	4d10.6s	2S1/2	42556.147	4d9.5s.(3D).5p	4P°3/2	58504.586
6279.154	Ag	II	60	31	4d9.(2D5/2).6s	2[5/2]2	120911.2048	4d9.(2D3/2).6p	2[1/2]°1	136832.527
6331.275	Ag	II	90	42	4d9.(2D5/2).5p	2[7/2]°3	82171.732	4d8.5s2	3F3	97962.039
6403.6	Ag	II	80	33	4d9.(2D5/2).6s	2[5/2]2	120911.2048	4d9.(2D3/2).6p	2[5/2]°2	136518.895
6505.747	Ag	II	85	26	4d9.(2D3/2).5p	2[3/2]°1	89895.5377	4d8.5s2	3P2	105262.2691
6621.17	Ag	I	45	11	4d9.5s.(3D).5p	2D°5/2	66972.3	4d9.5s.(3D).6s	2D5/2	82071.1
6697.223	Ag	II	95	16	4d9.(2D3/2).5p	2[1/2]°1	90334.8716	4d8.5s2	3P2	105262.2691
6717.36	Ag	II	120	19	4d9.(2D5/2).6s	2[5/2]3	120533.6058	4d8.(3F).5s.5p.(3P°)	5G°2	135415.323
6893.7	Ag	II	210	18	4d9.(2D5/2).6s	2[5/2]2	120911.2048	4d8.(3F).5s.5p.(3P°)	5G°2	135415.323
6939.988	Ag	II	135	10	4d9.(2D5/2).5p	2[5/2]°2	85200.7563	4d8.5s2	3F2	99606.031
6998.91	Ag	II	270	14	4d8.(3F).5s.5p.(3P°)	5D°1	134799.164	4d9.(2D3/2).7s	2[3/2]1	149082.86
7198.5	Ag	II	1	-	4d9.(2D5/2).6s	2[5/2]2	120911.2048	4d8.(3F).5s.5p.(3P°)	5D°1	134799.164
7239.376	Ag	II	1	-	4d9.(2D5/2).6s	2[5/2]3	120533.6058	4d8.(3F).5s.5p.(3P°)	5G°3	134343.135
7359.96	Ag	I	-	-	4d9.5s2	2D3/2	34714.22643	4d10.6p	2P°1/2	48297.406
7439.5	Ag	II	-	-	4d9.(2D5/2).6s	2[5/2]2	120911.2048	4d8.(3F).5s.5p.(3P°)	5G°3	134343.135

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