We analyzed the luminosity-temperature (L-T) relation for 2 samples of galaxy clusters which have all been observed by the ASCA satellite. We used 32 high redshift clusters (0.3<z<0.6), 53 low redshift clusters (z<0.3), and also the combination of the low and high redshift datasets. We assumed a power law relation between the bolometric luminosity of the galaxy cluster and its integrated temperature and redshift (Lbol,44=C*T^alpha*(1+z)^A). The results are consistent, independent of cosmology, with previous estimates of L\~T³ found by other authors. We observed weak or zero evolution.
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Novicki et al. (2002) studied this question.
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