Determining the Hubble constant without the sound horizon: A <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>3.6</mml:mn><mml:mo>%</mml:mo></mml:mrow></mml:math> constraint on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math> from galaxy surveys, CMB lensing, and supernovae
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