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Our understanding of blazars has been greatly increased in recent years byextensive multi-wavelength observations, particularly in the radio, X-ray andgamma-ray regions. Over the past decade the Whipple 10m telescope hascontributed to this with the detection of 5 BL Lacertae objects at very highgamma-ray energies. The combination of multi-wavelength data has shown thatblazars follow a well-defined sequence in terms of their broadband spectralproperties. Together with providing constraints on emission models, thisinformation has yielded a means by which potential sources of TeV emission maybe identified and predictions made as to their possible gamma-ray flux. We haveused the Whipple telescope to search for TeV gamma-ray emission from eightobjects selected from a list of such candidates. No evidence has been found forVHE emission from the objects in our sample, and upper limits have been derivedfor the mean gamma-ray flux above 390GeV. These flux upper limits are comparedwith the model predictions and the implications of our results for futureobservations are discussed.Comment: 15 pages, 2 figures, Accepted for publication in Ap

Search for High‐Energy Gamma Rays from an X‐Ray–selected Blazar Sample