MAD about the Large Magellanic Cloud - Preparing for the era of Extremely Large Telescopes

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Table 3

Number of stars falling in the boxes outlined in Fig. 5, for different combination of filters.

N	MS	RGB	RC	MS	RGB	RC	MS	RGB	RC	MS	RGB	RC	MS	RGB	RC	RGB	RC
	(V − I)	(V − I)	(V − I)	(V − K)	(V − K)	(V − K)	(I − K)	(I − K)	(I − K)	(I − H)	(I − H)	(I − H)	(J − K)	(J − K)	(J − K)	(H − K)	(H − K)

0BS	183	52	195	175	53	190	151	46	197	86	26	111	83	24	100	26	113
1	2055	291	1176	2053	325	1176	1609	270	1297	1624	252	1292	1740	266	1298	294	1382
2	2265	319	1195	2260	367	1195	1803	306	1337	1821	289	1335	1970	300	1337	317	1433
3	5656	387	1093	5656	464	1092	4370	319	1330	4353	269	1364	4375	310	1333	362	1546
4	54	209	1245	52	208	1245	130	196	1324	158	183	1321	310	196	1324	196	1324
5	865	168	565	995	250	562	477	192	744	506	159	654	529	169	906	251	1075
6	360	150	652	406	218	651	196	172	810	206	156	699	243	137	921	190	1011
7	2156	210	1165	2140	172	1002	1746	171	1176	1757	258	1350	1947	309	1396	326	1503
8	853	248	993	853	205	934	625	191	1110	632	221	1141	703	235	1165	245	1194
9	891	113	980	882	86	801	763	85	965	776	157	1195	907	226	1302	232	1341

Notes. These boxes represent: Young (MS) and intermediate-old (RC and RGB) stellar populations.

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