Table 5: Stellar populations for the cluster galaxies in terms of the six stellar components defined (see text): main sequence (luminosity class V) young, intermediate and old populations; giant (luminosity class III) young and intermediate populations; young supergiant (luminosity class I) populations. All values are in percentage and give the contribution of each population component to the total light at  Å. The distance D, the number of features () (see Sect. 5.1) used for each solution found and the value of E(B-V), when applicable, are also given. The relative position of each galaxy within the cluster (see Fig. 6 is indicated in the second row ("ct'' stands for centre or core; "it'' denotes the intermediate region and "p'' identifies peripheral galaxies).

CL0048	position	V young	V int.	V old	III young	III int.	I young	D		E(B-V)
218	ct.			25		25	50	193	36	0.0
235	ct.			32		45	23	63	33	0.0
189	ct.		11	40		9	40	106	30	0.0
213	ct.		16	20	14	45	5	75	37	0.0
216	ct.		16	17	4	53	10	125	43	0.0
231	it.			15	1	17	67	50	18	0.0
102	it.					42	58	582	33	0.0
128	it.			40		7	53	96	32	0.0
184	it.		17	17	3	41	22	56	35	0.0
322	it.	18	22	27	13	18	2	36	33	0.0
343	it.		11	27		26	36	117	41	0.0
391	it.					41	59	75	19	0.0
396	p.			40			60	52	19	0.0
404	p.		10	4	21	49	16	60	32	0.15
421	p.			12			88	164	26	0.0
443	p.	6		13	1	60	20	66	28	0.0
451	p.		7	29		43	21	280	31	0.0
902	p.		20	13		35	32	156	35	0.0
37	p.	6			3	33	58	17	19	0.0