Role of corona in the quiescent and active millimeter emission in young M dwarfs: Results from AD Leo.

The AD Leo flare dateset. Millimeter spectral data of the flare around 100GHz is provided using data from the NOEMA interferometer. The flare emission was 100 - 1000 times brighter than the quiescent emission. There are 3 tables for the 2 linear polarisation channels H and V, and STOKES I. The flux density, flux density errors and detection significance (sigma) are provided in the table. Movies of flare period are also provided with contours at -0.8,-0.6,-0.4,0.4,0.6,0.8 times the peak flux.