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Indirect searches for dark matter using dwarf spheroidal galaxies are a promising technique that complements other indirect and direct dark matter detection strategies. In this short talk, I'll cover some interesting new tools developed as a Utah-Hawai'i collaboration that facilitate gamma-ray searches for new physics, including MADHAT and TweedleDEE. Searches for new physics are often limited by systematic uncertainties in modeling diffuse gamma-ray backgrounds. To this point I'll discuss a recent likelihood-based comparison of locally constructed empirical background models (such as those used by TweedleDEE) and theoretically-motivated models that incorporate the Fermi-LAT diffuse background.