  We examine simultaneous X-ray and UV light curves from multi-epoch 8 day XMM
Newton observations of the narrow line Seyfert 1 galaxy 1H 0707-495. The
simultaneous observations reveal that both X-ray and UV emission are variable
and that the amplitude of the X-ray variations is significantly greater than
that of the UV variations in both epochs. Using a discrete correlation function
(DCF) the X-ray and UV light curves were examined for correlation on timescales
up to 7.0 d. Low significance (~ 95 percent confidence) correlations with the
UV leading the X-ray variations are observed. The lack of a significant
correlation between the UV and X-ray bands seems consistent with the X-ray
source being centrally compact and dominated by light bending close to the
black hole. In addition, multi-band X-ray light curves were examined for
correlations on similar timescales. Highly significant (> 99.9 per cent
confidence) correlations were observed at zero lag consistent with previous
studies of this AGN.
