This document discusses the fundamentals of radiometry and image formation in cameras. It explains that an image measures the amount of light captured at each pixel, and describes how the pinhole camera model projects points in 3D space to 2D image coordinates. It also discusses the relationship between scene radiance and image irradiance, and defines radiance as the radiant power travelling in a given direction per unit area and solid angle. Finally, it briefly mentions specular and Lambertian reflection models, as well as more complex lighting effects like global illumination and shadows.