Unnormalized thick velocity slice power spectra for MBM 16, integrating over −1.1 <v_LSR< 15.6 km s^-1 and spectral indices from least squares fits. High spatial frequency limits k_m< 0.06 arcmin^-1, corresponding to a linear size of 0.39 pc were applied and are indicated by the vertical black line. Black dots represent data derived after apodization, beam correction, and noise subtraction. In this case we fit γ = −3.63 ± 0.04. The red triangles show results obtained without apodization and beam correction by fitting the median power distribution. Here we fit γ = −3.88 ± 0.04.