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The blazar Mrk421 was observed independently, but contemporaneously, in 2005at TeV energies by MAGIC, the Whipple 10m telescope, and by a single VERITAStelescope during the construction phase of operations. A comparison of the timeaveraged spectra, in what was a relatively quiescent state, demonstrates thelevel of agreement between instruments. In addition, the increased sensitivityof the new generation instruments, and ever decreasing energy thresholds,questions how best to compare new observational data with archival results.

Time Averaged VHE Spectrum of Mrk 421 in 2005