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Embedding Inflation into larger models of particle physics or string theory has proven difficult. The wealth of new cosmological data expected in the short-term motivate a better understanding of how such ideas work together. We report on work showing that small-field models of inflation embed in a systematic way. Through examples, we discuss how these systematics give rise to scaling relations between physical quantities, particularly the scales of inflation and SUSY breaking. We review how such scaling can also impact the attractor properties of inflationary dynamics and anomalies in the power spectrum.