A review of airborne observation data with particular respect to the observation of the Stardust, ATV-1, and Hayabusa is given. These re-entries were observed from the NASA Airborne Observatory (in case of ATV-1 in addition from a second airplane) and, if possible, through ground based observation. A variety of experiments were used to gather data over a spectral range from 300nm to 1.6 m with different spectral resolutions to create a spectral data base to support the validation of aerothermodynamic simulation codes. A motivation for such re-entry observation is given and the basic principles and constraints of airborne observations are explained. The theoretical simulation of observation data and the re-entry missions of concern are discussed and selected results are presented. Finally, future perspectives for even more effective observation campaigns are given.