Table 3: Empirical population synthesis results of the galaxies with asymptotic (young-star) metallicities [ $Z/Z_\odot ]=-0.5$ : percentage contribution to $F_{\lambda 5870}$ .
[ $Z/Z_{\odot}$ ] [ $Z/Z_\odot ]=-0.5$ -1.0 -1.5 -2.0 $EW_{\rm abs}$ (Å)

Age(yr) HII E7 5E7 E8 5E8 E9 5E9 E10

Name 35 34 30 26 22 18 13 7 A_V H $\delta$ H $\gamma$ H $\beta$ H $\alpha$

iiizw12 18.2 10.0 16.2 10.5 10.9 18.9 9.6 5.6 .07 4.62 3.50 4.09 1.51

haro15 23.3 5.7 19.8 20.8 13.5 9.8 4.0 3.2 .04 4.59 3.27 3.75 1.51

iiizw33 21.3 5.4 10.7 8.2 18.5 16.5 11.3 8.1 .08 3.78 2.44 3.56 1.38

iiizw43 1.0 1.6 4.6 6.1 21.4 43.0 16.4 6.0 .86 4.24 3.45 4.33 1.25

iizw23 14.1 6.0 14.4 10.2 8.4 18.0 19.6 9.3 .27 4.76 3.17 4.26 1.89

iizw28 28.1 6.3 10.6 7.8 19.8 14.4 7.6 5.5 .06 3.41 2.19 3.09 1.03

iizw33 27.3 3.5 5.1 3.0 6.4 24.0 22.6 8.1 .09 3.01 1.88 2.94 1.59

iizw40 52.4 1.8 11.9 13.1 13.5 4.8 1.4 1.2 .01 2.57 2.11 2.23 .66

mrk5 12.1 2.3 7.2 9.2 48.6 14.6 3.1 2.9 .02 3.57 3.20 4.43 .28

viizw153 9.2 5.1 14.8 11.3 24.1 23.6 7.3 4.6 .05 4.70 3.81 4.36 1.53

viizw156 2.6 2.8 16.3 15.8 17.5 16.4 17.8 10.9 .17 5.53 4.02 4.55 1.71

haro1 21.7 6.8 14.8 18.6 15.2 9.8 6.1 6.9 .09 4.37 3.12 4.76 1.82

mrk385 9.0 6.7 16.4 14.3 22.6 13.3 9.2 8.6 .10 5.03 2.48 4.60 1.39

mrk390 25.0 7.7 14.7 10.3 8.6 18.1 10.4 5.4 .11 4.08 2.84 3.81 1.93

mrk105 8.5 9.5 8.5 8.8 12.9 25.0 16.2 10.6 .41 4.69 3.34 4.25 1.50

izw18 47.8 1.1 6.9 10.5 26.9 4.5 1.2 1.1 .01 2.25 1.87 2.31 .29

mrk402 23.5 7.1 12.9 7.7 14.7 24.4 6.3 3.4 .04 3.80 3.10 3.49 1.63

haro22 27.0 3.9 20.1 15.5 9.0 11.0 7.7 5.9 .06 4.29 3.35 3.47 1.55

haro23 28.4 3.2 12.4 9.5 19.6 19.0 4.7 3.3 .03 3.39 2.64 3.35 1.01

haro2 32.6 5.5 15.0 13.5 14.2 13.0 3.6 2.6 .03 3.63 2.77 3.45 1.64

mrk148 16.6 4.3 12.5 9.2 8.7 10.1 21.0 17.6 .84 4.39 2.57 3.98 1.69

haro25 26.5 7.4 14.5 15.5 10.4 8.4 7.9 9.5 .10 4.11 3.27 3.84 1.30

mrk1267 20.6 4.3 15.8 16.3 26.0 9.9 3.8 3.3 .03 4.22 3.08 3.96 .89

haro4 45.6 3.6 18.9 14.5 8.0 5.6 2.1 1.7 .02 3.34 2.66 2.93 1.00

mrk169 16.3 9.2 10.2 6.6 7.7 14.8 22.9 12.2 .61 4.43 3.07 4.59 1.88

haro27 13.9 4.1 6.8 4.5 14.7 35.8 13.2 7.0 .07 3.66 2.67 3.23 1.72

mrk201 24.5 4.2 12.8 15.1 11.6 11.6 9.4 10.7 .12 3.96 3.11 4.02 1.61

haro28 4.2 3.7 7.6 5.4 12.5 31.6 25.1 9.8 .09 4.69 2.03 3.94 1.44

haro8 11.7 2.0 8.3 8.3 30.6 36.2 1.8 1.2 .01 3.63 3.14 3.91 .80

haro29 37.4 2.0 12.4 11.9 25.3 7.7 1.8 1.4 .01 3.04 2.49 3.12 .78

mrk215 19.9 8.7 11.2 8.5 15.0 14.8 12.3 9.7 .10 4.09 3.11 4.39 1.67

haro32 36.9 5.2 12.9 9.2 8.2 16.2 6.9 4.4 .05 3.23 2.23 2.66 1.28

haro33 21.3 2.5 17.8 16.3 23.9 12.1 3.4 2.7 .03 4.23 3.20 3.18 1.24

haro36 7.8 2.8 8.4 6.7 43.3 23.6 4.2 3.2 .02 3.83 1.54 3.59 .52

haro35 19.7 4.4 17.2 17.8 14.6 14.5 6.3 5.4 .05 4.50 3.66 4.54 1.27

haro37 25.7 6.9 16.5 12.9 14.8 12.1 6.4 4.7 .05 4.12 3.23 3.39 1.30

mrk57 .6 1.0 3.1 3.7 29.0 37.5 20.0 5.2 .17 4.02 2.60 3.77 1.09

mrk235 15.2 4.4 7.4 5.8 10.4 20.2 23.0 13.6 .14 3.98 2.82 3.40 1.53

haro38 12.4 2.8 14.2 11.4 33.5 18.0 4.3 3.4 .03 4.25 2.88 3.31 1.19

mrk275 20.0 3.9 12.2 7.0 19.7 23.4 8.7 5.1 .05 3.77 2.60 3.42 1.25

haro42 23.3 3.1 9.8 7.9 9.7 22.6 14.3 9.3 .07 3.58 2.73 3.22 1.32

haro43 10.0 3.8 17.0 12.1 29.3 18.8 5.2 3.8 .03 4.69 3.30 4.23 1.32

haro44 25.9 4.4 20.8 15.7 18.5 9.6 3.0 2.1 .02 4.28 3.65 3.54 1.11

iizw70 38.2 4.1 13.1 10.5 19.4 9.9 2.8 2.1 .02 3.11 2.67 3.02 .84

izw117 22.3 7.0 13.1 11.2 8.8 11.4 14.0 12.1 .56 4.18 3.47 3.76 1.43

izw123 26.6 3.9 12.2 12.7 27.2 9.7 4.0 3.7 .03 3.58 1.58 3.82 1.10

mrk297 31.6 3.4 12.6 14.9 16.0 9.1 5.7 6.8 .06 3.52 2.51 3.63 1.51

izw159 22.0 6.8 11.7 10.3 23.1 17.4 5.2 3.7 .04 3.81 2.98 3.60 1.27

izw166 25.1 7.6 15.6 11.7 8.8 8.6 11.7 10.8 .27 4.21 2.23 4.03 1.85

mrk893 15.7 6.2 10.4 7.6 12.9 20.3 16.5 10.5 .16 4.19 2.83 3.51 1.98

izw191 5.0 8.8 7.5 7.1 14.6 33.6 15.3 8.0 .19 4.71 3.88 3.92 1.49

ivzw93 22.5 5.0 12.6 7.7 12.9 25.3 9.4 4.7 .05 3.79 2.56 3.51 1.82

mrk314 22.6 4.1 14.9 10.1 9.7 11.6 14.7 12.2 .16 4.13 2.22 2.78 1.57

ivzw149 16.0 4.9 16.6 14.8 23.7 16.0 4.5 3.5 .03 4.49 3.40 4.17 1.44

zw2335 16.5 4.9 11.1 9.2 11.3 13.4 19.3 14.4 .34 4.27 3.26 3.92 1.58

**Table 3:** Empirical population synthesis results of the galaxies with asymptotic (young-star) metallicities [ $Z/Z_\odot ]=-0.5$ : percentage contribution to $F_{\lambda 5870}$ .
[ $Z/Z_{\odot}$ ]	[ $Z/Z_\odot ]=-0.5$		-1.0		-1.5	-2.0		$EW_{\rm abs}$ (Å)
Age(yr)	HII	E7	5E7	E8	5E8	E9	5E9	E10
Name	35	34	30	26	22	18	13	7	A_V	H $\delta$	H $\gamma$	H $\beta$	H $\alpha$
iiizw12	18.2	10.0	16.2	10.5	10.9	18.9	9.6	5.6	.07	4.62	3.50	4.09	1.51
haro15	23.3	5.7	19.8	20.8	13.5	9.8	4.0	3.2	.04	4.59	3.27	3.75	1.51
iiizw33	21.3	5.4	10.7	8.2	18.5	16.5	11.3	8.1	.08	3.78	2.44	3.56	1.38
iiizw43	1.0	1.6	4.6	6.1	21.4	43.0	16.4	6.0	.86	4.24	3.45	4.33	1.25
iizw23	14.1	6.0	14.4	10.2	8.4	18.0	19.6	9.3	.27	4.76	3.17	4.26	1.89
iizw28	28.1	6.3	10.6	7.8	19.8	14.4	7.6	5.5	.06	3.41	2.19	3.09	1.03
iizw33	27.3	3.5	5.1	3.0	6.4	24.0	22.6	8.1	.09	3.01	1.88	2.94	1.59
iizw40	52.4	1.8	11.9	13.1	13.5	4.8	1.4	1.2	.01	2.57	2.11	2.23	.66
mrk5	12.1	2.3	7.2	9.2	48.6	14.6	3.1	2.9	.02	3.57	3.20	4.43	.28
viizw153	9.2	5.1	14.8	11.3	24.1	23.6	7.3	4.6	.05	4.70	3.81	4.36	1.53
viizw156	2.6	2.8	16.3	15.8	17.5	16.4	17.8	10.9	.17	5.53	4.02	4.55	1.71
haro1	21.7	6.8	14.8	18.6	15.2	9.8	6.1	6.9	.09	4.37	3.12	4.76	1.82
mrk385	9.0	6.7	16.4	14.3	22.6	13.3	9.2	8.6	.10	5.03	2.48	4.60	1.39
mrk390	25.0	7.7	14.7	10.3	8.6	18.1	10.4	5.4	.11	4.08	2.84	3.81	1.93
mrk105	8.5	9.5	8.5	8.8	12.9	25.0	16.2	10.6	.41	4.69	3.34	4.25	1.50
izw18	47.8	1.1	6.9	10.5	26.9	4.5	1.2	1.1	.01	2.25	1.87	2.31	.29
mrk402	23.5	7.1	12.9	7.7	14.7	24.4	6.3	3.4	.04	3.80	3.10	3.49	1.63
haro22	27.0	3.9	20.1	15.5	9.0	11.0	7.7	5.9	.06	4.29	3.35	3.47	1.55
haro23	28.4	3.2	12.4	9.5	19.6	19.0	4.7	3.3	.03	3.39	2.64	3.35	1.01
haro2	32.6	5.5	15.0	13.5	14.2	13.0	3.6	2.6	.03	3.63	2.77	3.45	1.64
mrk148	16.6	4.3	12.5	9.2	8.7	10.1	21.0	17.6	.84	4.39	2.57	3.98	1.69
haro25	26.5	7.4	14.5	15.5	10.4	8.4	7.9	9.5	.10	4.11	3.27	3.84	1.30
mrk1267	20.6	4.3	15.8	16.3	26.0	9.9	3.8	3.3	.03	4.22	3.08	3.96	.89
haro4	45.6	3.6	18.9	14.5	8.0	5.6	2.1	1.7	.02	3.34	2.66	2.93	1.00
mrk169	16.3	9.2	10.2	6.6	7.7	14.8	22.9	12.2	.61	4.43	3.07	4.59	1.88
haro27	13.9	4.1	6.8	4.5	14.7	35.8	13.2	7.0	.07	3.66	2.67	3.23	1.72
mrk201	24.5	4.2	12.8	15.1	11.6	11.6	9.4	10.7	.12	3.96	3.11	4.02	1.61
haro28	4.2	3.7	7.6	5.4	12.5	31.6	25.1	9.8	.09	4.69	2.03	3.94	1.44
haro8	11.7	2.0	8.3	8.3	30.6	36.2	1.8	1.2	.01	3.63	3.14	3.91	.80
haro29	37.4	2.0	12.4	11.9	25.3	7.7	1.8	1.4	.01	3.04	2.49	3.12	.78
mrk215	19.9	8.7	11.2	8.5	15.0	14.8	12.3	9.7	.10	4.09	3.11	4.39	1.67
haro32	36.9	5.2	12.9	9.2	8.2	16.2	6.9	4.4	.05	3.23	2.23	2.66	1.28
haro33	21.3	2.5	17.8	16.3	23.9	12.1	3.4	2.7	.03	4.23	3.20	3.18	1.24
haro36	7.8	2.8	8.4	6.7	43.3	23.6	4.2	3.2	.02	3.83	1.54	3.59	.52
haro35	19.7	4.4	17.2	17.8	14.6	14.5	6.3	5.4	.05	4.50	3.66	4.54	1.27
haro37	25.7	6.9	16.5	12.9	14.8	12.1	6.4	4.7	.05	4.12	3.23	3.39	1.30
mrk57	.6	1.0	3.1	3.7	29.0	37.5	20.0	5.2	.17	4.02	2.60	3.77	1.09
mrk235	15.2	4.4	7.4	5.8	10.4	20.2	23.0	13.6	.14	3.98	2.82	3.40	1.53
haro38	12.4	2.8	14.2	11.4	33.5	18.0	4.3	3.4	.03	4.25	2.88	3.31	1.19
mrk275	20.0	3.9	12.2	7.0	19.7	23.4	8.7	5.1	.05	3.77	2.60	3.42	1.25
haro42	23.3	3.1	9.8	7.9	9.7	22.6	14.3	9.3	.07	3.58	2.73	3.22	1.32
haro43	10.0	3.8	17.0	12.1	29.3	18.8	5.2	3.8	.03	4.69	3.30	4.23	1.32
haro44	25.9	4.4	20.8	15.7	18.5	9.6	3.0	2.1	.02	4.28	3.65	3.54	1.11
iizw70	38.2	4.1	13.1	10.5	19.4	9.9	2.8	2.1	.02	3.11	2.67	3.02	.84
izw117	22.3	7.0	13.1	11.2	8.8	11.4	14.0	12.1	.56	4.18	3.47	3.76	1.43
izw123	26.6	3.9	12.2	12.7	27.2	9.7	4.0	3.7	.03	3.58	1.58	3.82	1.10
mrk297	31.6	3.4	12.6	14.9	16.0	9.1	5.7	6.8	.06	3.52	2.51	3.63	1.51
izw159	22.0	6.8	11.7	10.3	23.1	17.4	5.2	3.7	.04	3.81	2.98	3.60	1.27
izw166	25.1	7.6	15.6	11.7	8.8	8.6	11.7	10.8	.27	4.21	2.23	4.03	1.85
mrk893	15.7	6.2	10.4	7.6	12.9	20.3	16.5	10.5	.16	4.19	2.83	3.51	1.98
izw191	5.0	8.8	7.5	7.1	14.6	33.6	15.3	8.0	.19	4.71	3.88	3.92	1.49
ivzw93	22.5	5.0	12.6	7.7	12.9	25.3	9.4	4.7	.05	3.79	2.56	3.51	1.82
mrk314	22.6	4.1	14.9	10.1	9.7	11.6	14.7	12.2	.16	4.13	2.22	2.78	1.57
ivzw149	16.0	4.9	16.6	14.8	23.7	16.0	4.5	3.5	.03	4.49	3.40	4.17	1.44
zw2335	16.5	4.9	11.1	9.2	11.3	13.4	19.3	14.4	.34	4.27	3.26	3.92	1.58

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