\begin{table}%t1
\caption{\label{table:1}Our cluster sample sorted by class type.} 
%\centering
\par
\begin{tabular}{l l r r r r r r r}
\hline\hline \noalign{\smallskip}
Cluster & IAU number  & $\alpha_{J2000}$ & $\delta_{J2000}$ & $l(^{\circ})$ & $b(^{\circ})$ & Diam ($'$) & Class & Remarks\\
\hline                        
NGC 2682       & C 0847+120 & 08:51:18        & +11:48:00    & 215.696	& 31.896      & 25.0 & $A$ & \\
\hline                         
NGC 1663       & C 0445+130 & 04:48:58        & +13:08:54  	& 185.845	& --19.735      & 12.0 & $B$ & pocr \\
NGC 1817       & C 0509+166 & 05:12:15        & +16:41:24    & 186.156	& --13.096      & 16.0 & $B$ & \\
NGC 2169       & C 0605+139 & 06:08:24        & +13:57:54    & 195.608	& --2.935      &  5.0 & $B$ & \\
NGC 2194       & C 0611+128 & 06:13:45        & +12:48:24    & 197.250	& --2.350      &  9.0 & $B$ & \\
Berkeley 29*    & C 0650+169 & 06:53:04        & +16:55:41    & 197.948	& 7.980      &  6.0 & $B$ & \\
NGC 2304       & C 0652+180 & 06:55:11        & +17:59:18    & 197.207	& 8.897      &  3.0 & $B$ & \\
NGC 2355       & C 0714+138 & 07:16:59        & +13:45:00    & 203.390	& 11.803      &  7.0 & $B$ & \\
NGC 2395       & C 0724+136 & 07:27:12        & +13:36:30    & 204.605	& 13.988      & 14.0 & $B$ & \\
Chupina 1       &          & 08:50:07        & +11:56:42    & 215.399	& 31.694      &  5.0 & $B$ & \\
Chupina 2       &          & 08:50:30        & +12:17:42    & 215.070	& 31.925      &  2.1 & $B$ & \\
Chupina 3       &          & 08:51:27        & +11:23:42    & 216.147	& 31.759      &  2.9 & $B$ & \\
Chupina 4       &          & 08:52:00        & +12:22:42    & 215.159	& 32.293      &  5.0 & $B$ & \\
Chupina 5       &          & 08:53:01        & +11:51:42    & 215.837	& 32.304      &  4.5 & $B$ & \\
Berkeley 82     & C 1909+129 & 19:11:20        & +13:07:06    & 46.853	& 1.624      &  2.0 & $B$ & \\
Roslund 1       & C 1942+174 & 19:45:00        & +17:31:00    &  54.600	& --3.400      &  3.0 & $B$ & \\
NGC 7036       &          & 21:10:02        & +15:31:00    & 64.544	& --21.443      &  4.0 & $B$ & pocr \\
\hline                          
Skiff J0614+129  &          & 06:14:48        & +12:52:24    & 197.314	& --2.098      &  7.0 & $C$ & \\
Ivanov 2        &          & 06:15:53        & +14:16:00    & 196.213	& --1.198      &  2.0 & $C$ & \\
Berkeley 43*    & C 1913+111 & 19:15:32        & +11:16:31    & 45.696	& --0.140      &  5.0 & $C$ & \\
Berkeley 45*    & C 1916+156 & 19:19:07        & +15:43:07    & 50.033	& 1.146      &  2.0 & $C$ & \\
Alessi 57       &          & 19:20:54        & +15:40:36    & 50.197	& 0.765      &  2.5 & $C$ & \\
Berkeley 47*    & C 1926+173 & 19:28:30        & +17:21:52    & 52.546	& --0.039      &  3.0 & $C$ & \\
King 26         & C 1926+147 & 19:29:00        & +14:52:00    & 50.410	& --1.339      &  2.0 & $C$ & \\
Dias 8          &          & 19:52:07        & +11:37:54    & 50.335	& --7.826      &  2.3 & $C$ & \\
NGC 7772       & C 2349+159 & 23:51:46        & +16:14:48    & 102.739	& --44.273      &  3.0 & $C$ & pocr\\
\hline                          
NGC 1807       & C 0507+164 & 05:10:43        & +16:31:18    & 186.088	& --13.495      & 15.0 & $D$ & (c.3)\\
DolDzim 2       &          & 05:23:54        & +11:28:00    & 192.240	& --13.560      & 10.0 & $D$ & (c.2)\\
Teutsch 11      &          & 06:25:24        & +13:51:59    & 197.654	& 0.649      &  2.3 & $D$ & (c.1) \\
Teutsch 12      &          & 06:25:40        & +13:36:25    & 197.914	& 0.585      &  4.2 & $D$ & (c.1)\\
NGC 2224       &          & 06:27:32        & +12:39:20    & 198.968	& 0.544      & 20.0 & $D$ & (c.2)\\
NGC 2234       &          & 06:29:29        & +16:43:08    & 195.584	& 2.846      & 35.0 & $D$ & (c.2)\\
NGC 2265       &          & 06:41:41        & +11:54:18    & 201.225	& 3.268      &  9.0 & $D$ & (c.2)\\
Dolidze 26      & C 0727+120 & 07:30:06        & +11:54:00    & 206.508	& 13.901      & 23.0 & $D$ & (c.2)\\
NGC 2678       &          & 08:50:02        & +11:20:18    & 216.035	& 31.421      & 10.0 & $D$ & (c.1)\\
DolDzim 7       &          & 17:10:36        & +15:32:00    & 36.294	& 29.166      &  5.0 & $D$ & (c.2)\\
NGC 6525       &          & 18:02:06        & +11:01:24    & 37.378	& 15.890      &  8.0 & $D$ & (c.2)\\
NGC 6738       & C 1859+115 & 19:01:21        & +11:36:54    & 44.398	& 3.102      & 15.0 & $D$ & (c.2) \\
Riddle 15       &          & 19:11:09        & +14:50:04    & 48.357	& 2.455      &  0.8 & $D$ & (c.1)\\
Juchert 1       &          & 19:22:32        & +12:40:00    & 47.727	& --1.001      &  3.2 & $D$ & (c.1)\\
Kronberger 13   &          & 19:25:15        & +13:56:42    & 49.167	& --0.979      &  1.5 & $D$ & (c.1)\\
Dolidze 35      & C 1924+115 & 19:25:24        & +11:39:30    & 47.170	& --2.095      &  7.0 & $D$ & (c.2)\\
NGC 6837       & C 1951+115 & 19:53:08        & +11:41:54    & 50.519	& --8.009	   &  3.0 & $D$ & (c.2)\\
NGC 6839       &          & 19:54:33        & +17:56:18    & 56.114	& --5.152      &  6.0 & $D$ & (c.2)\\
NGC 6840       &          & 19:55:18        & +12:07:36    & 51.162	& --8.253	   &  6.0 & $D$ & (c.2)\\
NGC 6843       &          & 19:56:06        & +12:09:48    & 51.293	& --8.404	   &  5.0 & $D$ & (c.2)\\
NGC 6858       &          & 20:02:56        & +11:15:30    & 51.360	& --10.304      & 10.0 & $D$ & (c.2)\\
NGC 6950       &          & 20:41:04        & +16:37:06    & 61.107	& --15.198      & 15.0 & $D$ & (c.2)\\
NGC 7084       &          & 21:32:33        & +17:30:30    & 69.963	& --24.302      & 16.0 & $D$ & (c.2)\\
\hline                                  
\end{tabular}
\tablefoot {The parameter values are taken from the D07 catalogue at Vizier \citep{Dias07}, apart from the coordinates of the clusters Berkeley~29, 43, 45, and~47 since they were re-centred by means of a detailed visual examination performed with Aladin~(*). The Galactic coordinates presented here were computed by VizieR. Classes:  $A$-{\it reference}, $B$-{\it known}, $C$-{\it known without proper-motion} and $D$-{\it others}. In~the remarks, pocr indicates the possible open cluster remnants while the~``c.'' indicates which condition of the Sect.~2.2 applies. Note: the~Chupina clusters are actually subclusters formed on the outskirts of NGC~2682 \citep{Chupina1998}.}
\end{table}