We present 10.27 ~ { } hrs of photometry of the roAp star HD 134214 obtained by the \it { MOST } \it { MOST } ( Microvariability and Oscillations of STars ) is a Canadian Space Agency mission , operated jointly by Dynacon , Inc. , and the Universities of Toronto and British Columbia , with assistance from the University of Vienna . satellite .
The star is shown to be monoperiodic and oscillating at a frequency of 2948.97 ~ { } \pm~ { } 0.55 ~ { } \muHz .
This is consistent with earlier ground based photometric campaigns ( e.g .
Kreidl et al .
1994 ) .
We do not detect any of the additional frequencies identified in the recent spectroscopic study by Kurtz et al .
( 2006 ) down to an amplitude limit of 0.36 ~ { } mmag ( 2 \sigma significance limit ) .