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Non-classified objects

Thirteen non emission-line objects are hard to classify at all. Their continua have too low signal-to-noise ratio to detect trustworthy absorption features, or the EW of the emission lines is too small. Six of them are certainly non-stellar on DSS images, and classified as well as non-stellar in the APM database. From our spectra in the range $\approx$ 4000 to $\approx$ 7300-8000 Å, we can exclude the presence of strong H$\alpha$. The remaining 7 objects are indistinguishable from stellar ones, and we suggest that most of them are galactic stars. One of the galaxies - namely HS 1232+3609, was presented after our observations in the paper by Popescu et al. ([1998]) as ELG with z=0.2529. Our spectrum is too noisy, and we could not identify any significant emission with this redshift.