\begin{table}%T1
\caption{\label{t-targets} Properties of the five new dwarf novae.}  
%\centerline
 {\small
\begin{tabular}{lccccc}
\hline\hline\noalign{\smallskip}
    & 
HS~0417+7445 & 
HS~1016+3412 & 
HS~1340+1524 & 
HS~1857+7127 &
HS~2214+2845 \\
\hline\noalign{\smallskip}
Right ascension {(J2000)} & 
$04^{\rm h}23^{\rm m}32.8^{\rm s}$ &
$10^{\rm h}19^{\rm m}47.3^{\rm s}$ &
$13^{\rm h}43^{\rm m}23.2^{\rm s}$ &
$18^{\rm h}57^{\rm m}20.4^{\rm s}$ &
$22^{\rm h}16^{\rm m}31.2^{\rm s}$ \\
%
Declination {(J2000)} &
$+74\degr52\arcmin50.30\arcsec$ &
$+33\degr57\arcmin53.9\arcsec$ &
$+15\degr09\arcmin16.9\arcsec$ &
$+71\degr31\arcmin19.2\arcsec$ &
$+29\degr00\arcmin20.6\arcsec$ \\
%
Period (min) &
$\simeq$105.1/$\simeq$109.9 &
$114.3\pm2.7$ & 
$92.66\pm0.17$ &
$272.317\pm0.001$ &
$258.02\pm0.56$ \\
%
Magnitude range & 
$18.0{-}13.5$ & %$18.0-13.7$ &
$18.6{-}15.4$: & %$17.5-15.5:$ &
$18.5{-}14.2$ & %$18.5-14.7$ &
$17.2{-}13.9$ &
$16.5{-}12.3$ \\
%
\Ha\ {\it EW} [\AA]/{\it FHWM} [\AA] &
172/43 &
184/27 &
121/28 &
39/32 &
53/33 \\
%
\Hb\ {\it EW} [\AA]/{\it FHWM} [\AA] &
98/43 &
125/25 &
88/23 &
33/32 &
42/31 \\
%
\Hg\ {\it EW} [\AA]/{\it FHWM} [\AA] & 
73/38 &
85/24 &
59/22 & 
27/33 & 
30/32 \\
%
\Line{He}{I}{5876} {\it EW} [\AA]/{\it FHWM} [\AA] & 
40/43 &
52/31 & 
36/30 & 
7/34 & 
7/25 \\
%
\Line{He}{I}{6678} {\it EW} [\AA]/{\it FHWM} [\AA] &  
7/30 &
26/35 &
18/32 &
3/46 &
5/39 \\
%
RASS source (1RXS~J) &
042332.8+745300 &
101946.7+335811 &
134323.1+150916 &
185722.6+713126 &
221631.2+290025 \\
%
RASS count rate ${\rm (0.01~cts~s^{-1})}$ &
$6.0\pm1.3$ &
$2.5\pm1.0$ &
$7.3\pm1.7$ &
$3.4\pm4.5$ &
$9.9\pm1.5$ \\
%
Hardness ratio HR1 &
$1.00\pm0.09$ &
$1.00\pm0.91$ &
$0.18\pm0.23$ &
$1.00\pm0.04$ &
$0.92\pm0.06$ \\
%
Hardness ratio HR2 &
$0.21\pm0.20$ &
$-0.32\pm0.38$ &
$-0.05\pm0.27$ &
$0.69\pm0.10$ &
$0.10\pm0.14$ \\
%
\hline
\end{tabular}}
\smallskip
Notes. The coordinates are taken from the USNO-B
  catalogue \citep{monetetal03-1}; the ROSAT PSPC count rates and
  hardness ratios HR1 and HR2 have been obtained from the ROSAT All
  Sky Survey (RASS) Bright Source Catalogue \citep{vogesetal99-1} and
  from the RASS Faint Source Catalogue \citep{vogesetal00-1}; the
  \Ha--\Hg\ and \Line{He}{I}{5876, 6678} equivalent widths ({\it EW}) and
  full width at half maximum ({\it FWHM}) were measured from the Calar Alto
  average spectra (Fig.~\ref{f-spectra}) using the
  \texttt{integrate/line} task in \texttt{MIDAS}; the outburst of
  HS~1016 is uncertain (marked by a colon), as only one outburst
  was observed.
\par
\end{table}