Observations of selected AGN with HESS

A sample of selected active galactic nuclei (AGN) was observed in 2003 and 2004 with the High Energy Stereoscopic System (HESS), an array of imaging atmospheric-Cherenkov telescopes in Namibia. The redshifts of these candidate very-high-energy (VHE, > 100 GeV) gamma-ray emitters range from z = 0.00183 to z = 0.333. Significant detections were already reported for some of these objects, such as PKS 2155-304 and Markarian 421. Marginal evidence (3.1 sigma) for a signal is found from large-zenith-angle observations of Markarian 501, corresponding to an integral flux of I(> 1.65 TeV) = (1.5 +/- 0.6(stat)+/- 0.3(syst)) x 10(-12) cm(-2) s(-1) or similar to 15% of the Crab Nebula flux. Integral flux upper limits for 19 other AGN, based on exposures of similar to 1 to similar to 8 h live time, and with average energy thresholds between 160 GeV and 610 GeV, range from 0.4% to 5.1% of the Crab Nebula flux. All the upper limits are the most constraining ever reported for these objects.