\begin{table}%t3
\par
\caption {\label{T-yso2}Main spectral characteristics of non-symbiotic
  stars and proposed classification. } 
%\centerline
 {\tiny\begin{tabular}{llllrrl} 
\hline\hline
Name (IPHASJ....)  & Spectral    &  Continuum and       & Main emission features                & \multicolumn{2}{c}\ha  & Classification \\
                   & range       &  absorption features &                                       & {\it EW}    &   {\it FWHM}         &       \\
                   &       [nm]  &                      &                                       & [\AA] &  [\kms]        &       \\
\hline        
000432.31+580854.0 & 370--750 & featureless             & HI, HeI, FeII, \cab                          & 195 & 350 & Not classified    \\
012544.66+613611.7 & 370--835 & negligible              & nebular$^\star$, OI8446, \car                & 950 & --  & young PN$^\star$\\
031704.34+601500.0 & 390--780 & TiO                     & HI, FeII, \cab                             & 122 & --  & CTT \\
032039.49+562358.2 & 370--870 & featureless, DIB, NaI D   & HI, FeII, OI7772, 8446, \car:                 & 210 & --  & YSO     \\
035823.95+522312.6 & 390--745 & featureless             & HI, FeII, HeI:                              & 200 & 250 & Not classified  \\
045625.15+434931.8 & 600--740 & featureless             &  \ha                                      & 60  & --  & Not classified \\ 
053018.12+313558.9 & 370--780 & featureless, DIB         & HI, HeI                                    & 45  & --  & Be/YSO      \\
053113.16+382006.6 & 535--745 & featureless, DIB+NaI     & \ha                                       & 63  & 500 & Be/YSO  \\
053440.77+254238.2 & 370--870 & featureless, DIB         & nebular$^\star$, OI8446, \cabr               & 200 & 300 & young PN$^\star$\\
055254.08+171424.7 & 350--900 & faint TiO               & HI, Balmer jump, HI, HeI, FeII, \cabr          & 240 & --  & CTT? \\
060515.15+204036.7 & 600--740 & featureless             & \ha                                       &  62 & 300 & Not classified        \\
060821.91+295255.7 & 384--855 & TiO                     & HI, HeI, FeII, faint OI8446, \cabr            & 110 & 230 & CTT    \\
183748.03-001617.2 & 370--900 & faint TiO               & HI, faint HeI                              & 40  & 280 & CTT   \\
183807.38+001113.6 & 390--900 & TiO                     & HI, HeI, \cabr                              & 500 & --  & CTT \\
183814.63-012213.8 & 370--820 & TiO                     & \ha, \hb, [OI], \cab                         & 175 & 250 & CTT \\
184222.67+025807.0 & 370--870 & faint TiO, strong NaI    & \ha                                       & 13  & --  & dMe \\
184431.46-001652.4 & 390--900 & featureless, HeI6678, NaI, DIB & HI, FeII, OI8446, \car                   &  78 & 400 & Be/YSO     \\
184635.85+005521.4 & 370--900 & Li I 6707, 6495, NaI, DIB  & HI, FeII, faint HeI, OI8446, [SII], [OI], \cabr &  95 & 230 & CTT     \\
185005.71--004041.2& 425--775 & featureless, DIB         & HI, FeII, [FeII], [NII], [NiII]6666, 7378, 7412 &  65 & 250 & ? (see text) \\
185349.55+052353.7 & 370--900 & featureless             & HI, HeI, FeII, \car                          & 215 & --  & YSO    \\
185424.82+041905.0 & 600--900 & weak TiO                & HI, strong \car                            &  38 & 350 & CTT \\
185448.29+005033.5 & 370--890 & TiO                     & HI, HeI, [OI]                               & 90  & --  & CTT         \\
190015.86+000517.3 & 370--900 & rising                  & dominated by strong broad C lines         & --  & --  & WC8      \\
190021.58+052001.1 & 430--773 & featureless             & HI, FeII, [FeII], [OI], [OII], [NII], [SII]     & 180 & 250 & Be/YSO   \\
190229.97--022757.0& 370--850 & faint continuum         & HI, HeI, FeII, [FeII], [OI], [OII], OI8446      & 1500& 250 & B[e]       \\
190441.53--005957.2& 370--900 & deep TiO                & HI, FeII, faint HeI                         &  70 & 250 & symbiotic?   \\
190832.31+051226.6 & 370--850 & TiO                     & HI, HeI, OI8446, [OIII]:                     & 250 & 280 & symbiotic?   \\
190857.31+053620.6 & 370--900 & featureless, DIB, NaI D   & HI, [NII], OI8446                           & 90  & 350 & Be/YSO               \\
191017.43+065258.1 & 370--900 & featureless, HeI5876, DIB, NaI D & HI, HeI6678(PCyg), [OI], OI8446,\car   & 150 & 350 & YSO               \\
192033.79+231040.3 & 430--775 & TiO                     & HI                                        &  35 & 100 & CTT?      \\
192249.80+142236.3 & 430--775 & featureless, DIB         & \ha, [OI]                                  &  100& 330 & Be/YSO               \\
192400.05+230253.1 & 370--900 & featureless             & HI, faint \cab                             & 42  & 300 & Not classified     \\
192515.05+224720.3 & 390--900 & TiO                     & HI, HeI, \cab                               & 80  & --  & CTT \\
192841.27+174819.9 & 370--900 & featureless             & HI, HeI, FeII, complex \ha, OI8446, strong \car&  63 & 200 & YSO               \\
193038.84+183909.8 & 370--900 & featureless, DIB         & strong HeI, HeII                          &  120 & 700& WN8-9                 \\
193232.88+151711.5 & 370--900 & HI, HeI, strong DIB, NaI   & HI, FeII, OI8446,\car                       &   52 & 400& Be/YSO                \\
194609.56+225423.2 & 380--840 & featureless, DIB, NaI D   & \ha, \hb                                   &  55  & 250&  Be/YSO               \\
194907.23+211742.0 & 370--900 & faint                   & nebular$^\star$                            & 250 & --  & young PN$^\star$\\
195935.55+283830.3 & 360-835 & featureless, DIB         & strong HeI and HeII, HI, [NII], [NeIII], [OIII],& 80 & 350  & WR nebula? \\
                   &         &                         & [FeVII], [CaVII], [SIII], [ArIII], [ArIV], [ArV] &    &      &               \\
200514.59+322125.1 & 370--856 & negligible              & nebular$^\star$, OI8446                     & 4000& --  & young PN$^\star$\\
201057.51+343732.4 & 370--870 & featureless, strong DIB  & HI, FeII, OI7772, 8446, \car                  &  77 & --  & YSO?                 \\
201152.98+281517.0 & 370--870 & featureless             & HI, OI 8446, strong \car                  &  85 & 220 & YSO?                 \\
201708.12+410727.0 & 370--870 & featureless, DIB        & HI, broad strong HeI and HeII              &  95 & 700 & WN8-9              \\
201918.94+381448.5 & 370--880 & featureless             & HI, HeI, faint \cab                         & 380 & --  & YSO             \\
202834.25+355417.4 & 372--875 & featureless, HeI5876, Na ID, DIBS& HI, [OI], OI8446,\car                 & 370 & 200 & YSO                \\
202947.93+355926.5 & 370--870 & featureless, weak HeI    & HI, FeII, OI8446, \car:                      & 180 & 350 & YSO$^\dag$\\
203413.39+410157.9 & 510--870 & featureless             & \ha, [OI], OI8446                           & 370 & 300 & YSO       \\
203545.40+400332.6 & 370--900 & TiO                     & HI                                        & 105 & --  & CTT          \\
204134.22+393239.0 & 370--870 & faint TiO, LiI 6707      & HI, HeI, FeII, [SII], strong \cabr            & 160 & 200 & CTT   \\
205544.33+463313.2 & 373--875 & faint                   & rich FeII, [FeII], HI, faint HeI, OI8446, [Ni II], \car  &1500 & 180 & B[e] \\
210404.87+535124.4 & 370--860 & TiO                     & HI, HeI, OI8446                             & 350 & 180 & CTT          \\
222628.63+612049.0 & 370--900 & TiO                     & HI, HeI                                    & 260 & --  & CTT          \\
230342.17+611850.4 & 370--900 & featureless             & HI, FeII, \cab, [SII], strong \car, OI7772, 8446& 145 & --  & CTT          \\
231334.92+620944.1 & 390--780 & TiO, NaI D               & HI                                        &  80 & --  & CTT         \\
\hline
\end{tabular}}
\par
\smallskip
The spectral range covered by our
  spectra is indicated, for reference for future studies of the
  objects. For line identification, the symbol ``:'' indicates
  marginal or uncertain detection. The \ha\ {\it FWHM}, corrected for the
  instrumental profile, is given in all cases where the
  spectral resolution allowed us to resolve the line width.
$^\star$ Viironen et~al. (2009b).
$^\dag$  Krause et~al. (2003).
\end{table}