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We present results of very-high-energy gamma-ray observations (E > 160 GeV)of two high-frequency-peaked BL Lac (HBL) objects, 1ES 1218+304 and H 1426+428,with the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). Bothsources are very-high-energy gamma-ray emitters above 100 GeV, detected usingground-based Cherenkov telescopes. STACEE observations of 1ES 1218+304 and H1426+428 did not produce detections; we present 99% CL flux upper limits forboth sources, assuming spectral indices measured mostly at higher energies.

Very high-energy observations of the two high-frequency peaked BL Lac objects 1ES 1218+304 and H 1426+428