**Table 3:** Comparison of our results (indicated by bold face) to already published cluster parameters.
Cluster	log t	E(B-V)	d [kpc]	Ref
King 21	7.20(1)^a	0.85(5)	3.41(56)
		0.89	1.91	Mohan & Pandey (1984)
	7.16	0.89	2.10	Dias et al. (2002)
N 3293	7.00(1)	0.29(5)	2.76(45)
	6.70	0.33	2.50	Turner et al. (1980)
	7.00	0.31	2.60	Feinstein & Marraco (1980)
	7.00	0.25^b	2.75	Balona (1994)
	6.90	0.29	2.75	Baume et al. (2003)
	6.94	0.25	2.47	Kharchenko et al. (2005)
	7.01	0.26	2.33	Dias et al. (2002)
N 5999	8.50(1)	0.48(5)	2.20(36)
	8.00	0.44		Santos & Bica (1993)
	8.60	0.45	2.20	Piatti et al. (1999)
	8.60	0.45	2.05	Dias et al. (2002)
N 6802	8.70(1)	0.89(5)	2.13(35)
		0.83	0.91	Hoag & Applequist (1965)
		0.80	0.82:^c	Becker & Fenkart (1971)
	9.18:	0.80	1.84	Kaluzny & Shara (1988)
	9.00	0.94	1.43	Sirbaugh et al. (1995)
	8.87	0.85	1.12	Dias et al. (2002)
N 6830	8.30(1)	0.48(5)	1.92(31)
			1.68	Barkhatova (1957)
		0.51	1.38	Hoag & Applequist (1965)
		0.58	1.47	Becker & Fenkart (1971)
	8.00	0.56	1.70	Moffat (1972)
	7.52	0.50	1.64	Kharchenko et al. (2005)
	7.57	0.50	1.64	Dias et al. (2002)
Ru 44	6.80(1)	0.58(5)	4.79(79)
		0.64	4.60	Turner (1981)
		0.68	6.80	FitzGerald & Moffat (1976)
	6.00	0.70	6.60	Moffat & Fitzgerald (1974)
	7.33	0.62	4.66	Kharchenko et al. (2005)
	6.94	0.62	4.73	Dias et al. (2002)
Ru 115	8.60(1)	0.74(5)	2.00(33)
	8.70	0.60	2.50	Piatti et al. (1999)
	8.78	0.65	2.16	Dias et al. (2002)
Ru 120	8.00(1)	0.65(5)	1.98(33)
	8.00	0.65	2.30	Piatti et al. (1999)
	8.18	0.70	2.00	Dias et al. (2002)

^a The errors of the last digits are always given in parenthesis.
^b Interstellar reddening was transformed according E(b-y) = 0.74E(B-V) (Crawford 1978).
^c Indicates an uncertain result in the respective reference.

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