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Table 1: Photon energy spectra and luminosity (0.2 to 10 TeV) of the VHE $\gamma$ -ray emission of LS 5039 for different orbital phase intervals. The broad phase intervals INFC and SUPC encompass the inferior and superior conjunction epochs. The orbital phase $\phi$ is calculated from the ephemeris of Casares et al. (2005). The best-fit function is indicated for each phase interval. The errors quoted are statistical with systematic errors in the 10 to 15% range.