Table 1: Upper limits for w obtained for the assumed values of $\Omega _{{\rm m0}}$ and $t_{{\rm GC}}$ at 68% and 95% c.l. for globular cluster formation at z=3.
t₀ (Gyr) $\Omega _{{\rm m0}}$ $t_{{\rm GC}}$ (Gyr) w H₀ (km s^-1 kpc^-1)

13.53 0.295 11.45 -1.21 72

11.98 0.295 10.00 -0.56 72

13.66 0.260 11.45 -1.02 72

12.06 0.260 10.00 -0.52 72

13.73 0.295 11.45 -0.83 64

11.88 0.295 10.00 -0.25 64

13.82 0.260 11.45 -0.57 64

11.92 0.260 10.00 -0.23 64

**Table 1:** Upper limits for w obtained for the assumed values of $\Omega _{{\rm m0}}$ and $t_{{\rm GC}}$ at 68% and 95% c.l. for globular cluster formation at z=3.
t₀ (Gyr)	$\Omega _{{\rm m0}}$	$t_{{\rm GC}}$ (Gyr)	w	H₀ (km s^-1 kpc^-1)
13.53	0.295	11.45	-1.21	72
11.98	0.295	10.00	-0.56	72
13.66	0.260	11.45	-1.02	72
12.06	0.260	10.00	-0.52	72
13.73	0.295	11.45	-0.83	64
11.88	0.295	10.00	-0.25	64
13.82	0.260	11.45	-0.57	64
11.92	0.260	10.00	-0.23	64

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