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. The data was obtained by imaging the source at 2s resolution using data from the NOEMA interferometer. The flare emission was 100 - 1000 times brighter than the quiescent emission. There are two tables for the 2 linear polarisation channels H and V.

The flux density, flux density errors and detection significance (sigma) are provided in the table.