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We report on the observation of the region around supernova remnant G65.1+0.6with the stand-alone MAGIC-I telescope. This region hosts the two bright GeVgamma-ray sources 1FGL J1954.3+2836 and 1FGL J1958.6+2845. They are identifiedas GeV pulsars and both have a possible counterpart detected at about 35 TeV bythe Milagro observatory. MAGIC collected 25.5 hours of good quality data, andfound no significant emission in the range around 1 TeV. We therefore reportdifferential flux upper limits, assuming the emission to be point-like (<0.1deg) or within a radius of 0.3 deg. In the point-like scenario, the flux limitsaround 1 TeV are at the level of 3 % and 2 % of the Crab Nebula flux, for thetwo sources respectively. This implies that the Milagro emission is eitherextended over a much larger area than our point spread function, or it must bepeaked at energies beyond 1 TeV, resulting in a photon index harder than 2.2 inthe TeV band.

MAGIC Upper Limits for two Milagro-detected, Bright Fermi Sources in the Region of SNR G65.1+0.6