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
9487.2	Hg	I	-	-	5d10.6s.6d	3D1	71336.005	5d10.6s.11p	3P°2	81873.704
9495.9	Hg	I	7	-	5d10.6s.6d	3D2	71396.073	5d10.6s.8f	3F°3	81923.9
9520.198	Hg	II	40	-	5d10.5f	2F°7/2	123153.775	5d10.5g	2G9/2	133654.879
9526.3	Hg	I	5	-	5d10.6s.6d	3D3	71431.18	5d10.6s.8f	3F°4	81925.7
9544.7	Hg	I	-	-	5d10.6s.6d	1D2	71333.053	5d10.6s.11p	3P°1	81807.95
9547.3	Hg	I	-	-	5d10.6s.6d	3D1	71336.005	5d10.6s.11p	3P°1	81807.95
9554.1	Hg	I	1	-	5d10.6s.6d	3D1	71336.005	5d10.6s.11p	3P°0	81800.43
9574.3	Hg	I	2	-	5d10.6s.6d	3D3	71431.18	5d10.6s.11p	3P°2	81873.704
9602.	Hg	I	-	-	5d10.6s.16s	3S1	83324.7	5d9.6s2.(2D3/2).6p	2[3/2]°1	93736.4
9639.06	Hg	II	4	-	5d10.7s	2S1/2	95714.406	5d9.6s.6p	(2D<5/2>,1P<1>)°3/2	106086.013
9759.557	Hg	II	1	-	5d10.5f	2F°5/2	123411.351	5d10.5g	2G7/2	133654.913
9775.3	Hg	I	2	-	5d10.6s.7p	3P°0	69516.576	5d10.6s.6f	3F°2	79743.7
9792.9	Hg	I	1	-	5d10.6s.7p	3P°2	71207.296	5d10.6s.11s	3S1	81416.17
9808.	Hg	I	-	-	5d9.6s2.(2D5/2).6p	2[7/2]°3	70932.2	5d10.6s.6g	3G4	81125
9821.8	Hg	I	2	-	5d10.6s.7p	1P°1	71294.86	5d10.6s.11s	1S0	81473.4
9832.3	Hg	I	-	-	5d10.6s.18s	1S0	83569	5d9.6s2.(2D3/2).6p	2[3/2]°1	93736.4
9838.1	Hg	I	7	-	5d10.6s.7p	3P°0	69516.576	5d10.6s.8d	3D1	79678.57
9969.3	Hg	I	7	-	5d10.6s.7p	3P°1	69661.803	5d10.6s.8d	3D2	79690.16
9980.9	Hg	I	7	-	5d10.6s.7p	3P°1	69661.803	5d10.6s.8d	3D1	79678.57
9999.	Hg	I	6	-	5d10.6s.7p	3P°1	69661.803	5d10.6s.8d	1D2	79660.56

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