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HESS J0632+057 has been recently identified as a new gamma-ray binary system.The source, located in the Monoceros region and associated with the massive Bestar MWC 148, shows variability from radio to very high energy (VHE)gamma-rays, displaying a maximum of its non-thermal emission about 100 daysafter periastron passage (at orbital phases close to 0.3). We present here theresults obtained with the VERITAS and H.E.S.S Cherenkov telescopes spanning awide time interval from 2004 to 2012. The source is detected at TeV gamma-raysat a high significance level at orbital phase 0.3. We also report for the firsttime TeV observations belonging to orbital phases never explored so far. TheVHE gamma-ray results are discussed in a multiwavelength context, focusing oncontemporaneous observations obtained with the Swift-XRT.

VERITAS and H.E.S.S. observations of the gamma-ray binary HESS J0632+057