The achievable image quality and the reliability of amplitudes in Kirchhoff migration strongly depend on the selection of the migration aperture. Optimal amplitudes are obtained if the migration aperture is restricted to the constructively contributing part of the reflection event which is related to the size of the projected Fresnel zone. The Common-Reflection-Surface (CRS) stack provides kinematic wavefield attributes that allow to address this problem together with a straightforward time migration velocity model building. The approach is applied to a complex onshore data set and compared to conventional Kirchhoff migration. We observe an improved continuity of the reflection events as well as more stable amplitudes in regions with reliably detected CRS attributes. Moreover, the computational costs of the prestack migration are significantly reduced. Related presentations B044 CRS stacking: a simplified explanation, J. Mann, J. Schleicher, and T. Hertweck P058 Automatic tracking of reflection events in 3D ZO volumes using CRS attributes, N.-A. Müller H015 2D CO CRS poststack imaging for walkaway VSP data, M. von Steht