A Schmidt camera (or Schmidt telescope) is a reflector telescope with a spherical primary mirror and a lens to correct the spherical aberration (called the Schmidt corrector plate). For a given a size, a spherical mirror is easier to grind than a non-spherical mirror and produces little of the other aberrations usually associated with a short focal length, allowing Schmidt cameras to be made with a wide field of view, which is especially suitable for surveys. However, the focal plane is not planar, but curved, thus requiring unique design of the image recording mechanism, such as curved photographic paper in the photography age. The general design of the Schmidt camera was developed by Bernardt Schmidt in 1930. Variants of the Schmidt camera combine it with other telescope designs, e.g., the Schmidt-Newton telescope (SNT) or Schmidt-Cassegrain telescope (SCT).