We present a total of 57 days of contiguous , high-cadence photometry ( 14 days in 2004 and 43 in 2005 ) of the star BD+18 4914 obtained with the MOST MOST 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 .
We detect 16 frequencies down to a signal-to-noise of 3.6 ( amplitude \sim 0.5 mmag ) .
Six of these are less than 3 cycles/day , and the other ten are between 7 and 16 cycles/day .
We intrepret the low frequencies as g-mode \gamma Doradus-type pulsations and the others as \delta 
Scuti-type p-modes , making BD+18 4914 one of the few known hybrid pulsators of its class .
If the g-mode pulsations are high-overtone non-radial modes with identical low degree \ell , we can assign a unique mode classification of n = { 12 , 20 , 21 , 22 , 31 , 38 } based on the frequency ratio method .