40 
XV 
XIX Asymptote 53986. 13 | 54354.11 | 54905.34 | 55696.37 | 57039.02 
x=1 | 2719.00 | 2602.35 | 2652.70 | 2598.16 | 2510.60 
x=2 | 2220.85 2203.13 | 2175.99 | 2139.89 | 2079.55 
EE 2060.25 | 2044.78 | 2021.96 | 1990.20 | 1938.83 
} 
The valnes for z==3 lie all in the not investigated region. 
Further I have found a third group of translation series in the 
spectrum of Antimony, the first member of which has as formula: 
109675.0 
10° 1-1 = 44790.00 -— ae bes Bei 
(@ + 1.269826 + 1757,48 A1)? 
p= 
XX ; Bin ; 
| A | x Limit of 1 
x | dy db | Ap anaes Intensity 
i | 
| | | 
1 | 3232. 61 3232.61 | 0.00 | (03. Ate 
| | 
2 | 2652.70 2652.70 0.00 688604 4 
| | | 
3 | 2478.401)| 2477.45 | 40.95 | 2 | 2 
4 | 2395.31 2395.31 | 0.00 0.03 1 
5 n.0. DAD) aje | = a 
22349.50 has not been observed any more, which tallies with the 
course of the intensity, as 1 indicates the faintest lines according to 
Exner and HAsCHEK. 
The following form was found as corresponding translation series: 
109675.0 
(z + 1,269826 4- 1757,48 A—})? 
10° A —! = 52099.97 — 
eal oe 
are . Limit of ; 
x Me dy | — 4 Errors Intensity 
1 2614.74 261414 1 De DE 
2 | 2022.10 | 2001.88 | 40.22 0.10 = 
3 | 2098.47 | 2097.76 | +40.7r | 0.30 = 
4 | oro, | 2038.40 | a = Ss 
1) Exner and HascHeK loc. cit. p. 232. 
