Linear order shear power spectrum (thick solid line; Eq. (12)) and lensing bias and ellipticity estimator corrections. The short dashed (dashed) lines show the lensing bias corrections to the B-mode shear power spectrum (Eq. (61)) assuming q = 1 (q = 2). The dotted (dashed-dotted) lines show the lensing bias corrections to the E-mode shear power spectrum (Eq. (60)) assuming q = 1 (q = 2). The fine solid line illustrates the magnitude of the correction arising from the conversion between ellipticity and reduced shear Eq. (45) for the e ellipticity with  ⟨ e^(s)2 ⟩ ^1 / 2 = 0.6. This correction is negative and its normalization depends on the distribution of source galaxies (see Sect. 3.3 for details). This figure uses the same cosmology and source redshifts as Fig. 1.