1. INTRODUCTION
2. $\mathrm{NH_{3}}$ AND $\mathrm{H_{2}O}$ MASER SURVEY OF BGPS SOURCES
2.1. New $GBT NH_{3}$ Observations
2.2. New GBT $H_{2}O$ Maser Observations
3. DEVELOPING A STAR FORMATION INDICATOR CATALOG
3.1. Catalog Cross-Matching
3.2. Infrared Surveys
3.3.2. $\mathrm{CH_{3}OH}$ Masers
3.5. Star Formation Indicator Catalog Summary
4. DETERMINING HELIOCENTRIC DISTANCE
4.1. Distance Probability Density Functions
4.2. Distance Resolution Broadcasting
4.3. Distance Comparisons
5. ANALYSIS OF PHYSICAL PROPERTIES WITH STAR FORMATION INDICATORS
5.1. Monte Carlo Sampling
5.2. Flux Density, Flux Concentration, and Size
5.3. Gas Kinetic Temperature and Linewidth
5.4.2. Clump Mass
5.4.3. Virial Parameter
6. DISCUSSION
6.1. Massive Star-forming Potential of Clumps
6.2. Clump Timescales
6.3. Origin of Starless vs. Protostellar Clump Mass Difference