The Mach number scaling of the individual azimuthal modes of jet mixing noise was studied for jets in flight conditions, i.e. with co-flow. The data were obtained via a series of Direct Numerical Simulations (DNS), performed of fully turbulent jets with a target Reynolds number, based on nozzle diameter, of Re jet = 8, 000. The DNS included a pipe 25 diameters in length in order to ensure that the flow developed to a fully turbulent state before exiting into a laminar co-flow, and to account for all possible noise generation mechanisms. To allow for a detailed study of the jet-mixing noise component of the combined pipe/jet configuration, acoustic liner boundary conditions on the inside of the pipe and a modification to the synthetic turbulent inlet boundary condition of the pipe were applied to minimize internal noise in the pipe. Despite these measures, the use of a phased array source breakdown technique was essential in order to isolate the sources associated with jet noise mechanisms from additional noise sources that could be attributed to internal noise or unsteady flow past the nozzle lip, in particular for the axisymmetric mode. Decomposing the sound radiation from the pipe/jet configuration into its azimuthal Fourier modes, and accounting for the co-flow effects, it was found † Email address for correspondence: richard.sandberg@unimelb.edu.au