Table 2: Measurements for the emission lines of the LSB candidate sample. All entries which are marked with a were not used for the estimation of the mean redshift $\langle z\rangle $ and therefore also not for the estimation of the standard deviation $\sigma _z$. All lines which were either influenced by night sky emission lines or which had only upper limits were also not used for the determination of the mean redshift. It was not possible to resolve the two component of the [S II]-doublet. Therefore [S II] was not used in order to estimate redshifts. The redshift of LSB J22324-60520 (marked with b) was estimated measuring the wavelength of the Ca II-K absorption line.
NAME [O II] H$\beta$ [O III] [O III] H$\alpha$ [N II] [S II] z $\sigma _z$
  $\lambda$3727 $\lambda$4861 $\lambda$4959 $\lambda$5007 $\lambda$6563 $\lambda$6584 $\lambda$$\lambda$6717,6731    
  [Å] [Å] [Å] [Å] [Å] [Å] [Å]    
LSB J22311-60503 4172 - - - 7351 - - 0.1198 0.0004
LSB J22325-60155 3924 5118 5219 5270 6907 - 7077a 0.0526 0.0002
LSB J22330-60543 3936 5133 5236 5287 6929 - 7096a 0.0559 0.0001
LSB J22343-60222 3903 5089 5190 5242 6866 6888a 7037a 0.0467 0.0005
LSB J22352-60420 4170 5439 5550a 5603a 7347 - - 0.1191 0.0003
LSB J22353-60311 3946 5146 5250 5297 6943 6968a - 0.0584 0.0004
LSB J22354-60122 4329 5647 5758 5816 - - - 0.1615 0.0002
LSB J22355-60183 4194 5468 5584a 5632 7381 - - 0.1249 0.0003

LSB J22324-60520
- - - - - - - 0.1723b -


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