Age – metallicity relation in the Magellanic Clouds clusters

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Volume 554 (June 2013)

A&A, 554 (2013) A16

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Table 1

Observing log.

Name	RA	Dec	Exp. time/frame	Frames	Date
	hms	dms	ybv	ybv

KMK1	5 03 48	−69 09 44	153030	222	Dec. 8, 9 2002
KMK3	5 03 45	−69 05 33	153030	222	Dec. 8, 9 2002
KMK8	5 04 29	−69 09 21	153030	222	Dec. 8, 9 2002
KMK32	5 10 20	−68 52 45	152530	222	Dec. 28 1997
HS153	5 10 30	−68 52 21	152530	222	Dec. 28 1997
KMK49	5 21 10	−69 56 25	203030	222	Jan. 3 1998
KMK50	5 21 23	−69 54 34	203030	222	Jan. 3 1998
SL36	4 46 09	−74 53 19	153030	222	Dec. 14, 15 1998
SL620	5 36 29	−74 24 18	153030	222	Dec. 16 1998
KMHK81	4 45 13	−75 07 00	153030	222	Dec. 8, 9 2002
KMHK1042	5 31 00	−74 40 18	153030	222	Dec. 10 2002
KMHK1278	5 43 28	−63 24 47	153030	222	Dec. 28 1997
KMHK1381	5 48 21	−63 35 50	153030	222	Jan. 1 1998
KMHK1399	5 45 06	−70 14 30	153030	222	Dec. 9 2002
KMHK1640	6 04 48	−75 06 09	153030	222	Dec. 10 2002

L11 (K7)	0 27 45	−72 46 53	200300650	333	Aug. 22−23 2001
L17 (K13)	0 35 42	−73 35 51	200300650	333	Aug. 22−23 2001
L113	1 49 29	−73 43 42	200300650	333	Aug. 22−23 2001
NGC 376	1 03 50	−72 49 34	200300650	333	Aug. 22−23 2001
NGC 419 (L85)	1 08 29	−72 53 12	200300650	333	Aug. 22−23 2001
NGC 330	0 56 19	−72 27 50	7090140	111	Aug. 22 2001
L80	1 07 28	−72 46 10	7090200	111	Aug. 23 2001
NGC 361	1 02 11	−71 36 21	7090140	111	Aug. 22 2001

Notes.The KMHK clusters are named from Kontizas et al. (1990), whereas KMK clusters are named from Kontizas et al. (1988).

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