Table 1:

Our cluster sample sorted by class type.

Cluster	IAU number					Diam (')	Class	Remarks
NGC 2682	C 0847+120	08:51:18	+11:48:00	215.696	31.896	25.0	A
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
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
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)

Notes. The parameter values are taken from the D07 catalogue at Vizier (Dias et al. 2002a), 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-reference, B-known, C-known without proper-motion and D-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 (Chupina & Vereshchagin 1998).