  The outer Galactic disc contains some features such as the warp and flare,
whose origin is still debated. The Gaia data provide an excellent opportunity
to probe the Galactic disc at large distances and study these features. We
derive the density distributions of the average (old) whole population and the
supergiants (representative of a young population), and we use them to
constrain their warp and flare. By comparing the results, we study how the
properties of these phenomena depend on the studied population. We used Lucy's
deconvolution method to recover corrected star counts as a function of
distance, from which we derive the density distribution. We find that
supergiants have an asymmetric warp, reaching a maximum amplitude of
$z_w=0.658$ kpc and minimum amplitude of $z_w=-0.717$ kpc at a distance of
$R=[19.5,20]$ kpc, which is almost twice as high as the amplitude of the whole
population of the disc. We find a significant flare of the whole population,
especially in the thick disc. The scale height increases from
$h_{z,thick}\approx 0.8$ kpc and $h_{z,thin}\approx 0.3$ kpc in the solar
neighbourhood, to $h_{z,thick} \approx 3$ kpc and $h_{z,thin}\approx 0.7$ kpc
in the remote regions of the Milky Way ($R\approx 18$ kpc). The supergiants'
population has only a small flare.
