Table 1: Broadband colors in stellar magnitudes for pure hydrogen atmospheres. Models are computed with nonideal EOS and Los Alamos (TOPS) opacities. Temperatures $T_{\rm eff}$ are given in thousands K and $\log g$ are in cgs units.
Z $T_{\rm eff}$ $\log g$ U-B B-V V-R V-I

1 20 7 -0.895 -0.057 -0.098 -0.206

1 20 8 -0.965 -0.012 -0.103 -0.202

1 20 9 -1.017 0.014 -0.109 -0.199

1 20 10 -1.076 0.026 -0.112 -0.180

1 30 7 -1.121 -0.193 -0.135 -0.290

1 30 8 -1.157 -0.171 -0.139 -0.288

1 30 9 -1.186 -0.163 -0.142 -0.288

1 30 10 -1.211 -0.168 -0.145 -0.275

1 50 7 -1.238 -0.284 -0.146 -0.325

1 50 8 -1.244 -0.277 -0.147 -0.325

1 50 9 -1.251 -0.275 -0.148 -0.323

1 50 10 -1.256 -0.275 -0.149 -0.320

1 70 7 -1.257 -0.313 -0.145 -0.338

1 70 8 -1.262 -0.308 -0.150 -0.339

1 70 9 -1.268 -0.304 -0.150 -0.336

1 70 10 -1.271 -0.304 -0.152 -0.336

1 100 7 -1.279 -0.329 -0.142 -0.348

1 100 8 -1.280 -0.327 -0.145 -0.350

1 100 9 -1.282 -0.324 -0.146 -0.349

1 100 10 -1.282 -0.324 -0.150 -0.349

**Table 1:** Broadband colors in stellar magnitudes for pure hydrogen atmospheres. Models are computed with nonideal EOS and Los Alamos (TOPS) opacities. Temperatures $T_{\rm eff}$ are given in thousands K and $\log g$ are in cgs units.
Z	$T_{\rm eff}$	$\log g$	U-B	B-V	V-R	V-I
1	20	7	-0.895	-0.057	-0.098	-0.206
1	20	8	-0.965	-0.012	-0.103	-0.202
1	20	9	-1.017	0.014	-0.109	-0.199
1	20	10	-1.076	0.026	-0.112	-0.180
1	30	7	-1.121	-0.193	-0.135	-0.290
1	30	8	-1.157	-0.171	-0.139	-0.288
1	30	9	-1.186	-0.163	-0.142	-0.288
1	30	10	-1.211	-0.168	-0.145	-0.275
1	50	7	-1.238	-0.284	-0.146	-0.325
1	50	8	-1.244	-0.277	-0.147	-0.325
1	50	9	-1.251	-0.275	-0.148	-0.323
1	50	10	-1.256	-0.275	-0.149	-0.320
1	70	7	-1.257	-0.313	-0.145	-0.338
1	70	8	-1.262	-0.308	-0.150	-0.339
1	70	9	-1.268	-0.304	-0.150	-0.336
1	70	10	-1.271	-0.304	-0.152	-0.336
1	100	7	-1.279	-0.329	-0.142	-0.348
1	100	8	-1.280	-0.327	-0.145	-0.350
1	100	9	-1.282	-0.324	-0.146	-0.349
1	100	10	-1.282	-0.324	-0.150	-0.349

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