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We present observations performed with the Green Bank Telescope at 1.4 and 5 GHz of three strips coincident with the anomalous microwave emission features previously identified in the Perseus molecular cloud at 33 GHz with the Very Small Array. With these observations we determine the level of the low frequency (~1 - 5 GHz) emission. We do not detect any significant extended emission in these regions and we compute conservative 3\sigma upper limits on the fraction of free-free emission at 33doi:10.1088/0004-637x/770/2/122 fatcat:uflskomvcrbgzf3vwvlgjj2aje