Overview of forecasted contributions to the detection significance as a function of lensing multipole L for the power spectrum (solid black), as well as for several other mass tracers, at the noise levels of our MV lens reconstruction. Our measurement of the power spectrum is presented in Sect. 6, The ISW-φ correlation believed to be induced by dark energy is studied in Sect. 6.2. The NVSS-φ correlation is studied (along with other galaxy correlations) in Sect. 6.3. The CIB-φ prediction (dashed cyan) uses the linear SSED model of Hall et al. (2010), assuming no noise or foreground contamination. A full analysis and interpretation of the CIB-φ correlation is performed in Planck Collaboration XVIII (2014).