Kernel density functions for the seeing, coherence time, turbulence velocity, and guide star magnitude (r band) showing the conditions under which the VLT/SPHERE telemetry was taken. The first three panels are measurements closest to the time of the observation output by the MASS-DIMM (accessed via ESO Paranal query form). The corresponding targets were found at the VLT/SPHERE ESO archive and their r-band magnitudes were found in the VizieR catalog. The kernel density functions are a nonparametric estimation of the probability functions.