In this study, we selected only data of high quality using the criteria described in Aharonian et al. (2006A&A...457..899A) and the quality cut on atmospheric transparency conditions developed by Hahn et al. (2014, Astropart. Phys., 54, 25). The observation live time of the analysed regions, corrected by the H.E.S.S. γ-ray acceptance, spans a range from ~10min to ~80h with a median value of 14.5h. The majority of data ( ~80%) have been recorded at average zenith angles smaller than 40°. Table A.1 lists the analysed source sample and the corrected observation live time, the averaged zenith angle for the observations of each source, and the closest H.E.S.S. source. (1 data file).