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The Bolocam Galactic Plane Survey has laid the grounds for an extensive study  of dense gas within our Galaxy.  I examined the brightest sources within the BGPS, discovering 18 with masses  $M>10^4$ \msun, large enough to form bound clusters. These sources are all  actively star-forming and can now be used for unbiased proto-cluster population  studies.  I performed follow-up studies with \formaldehyde observations from the Green  Bank Telescope and Arecibo Observatory.  \input{solobib}