Scaling relations of z~0.25-1.5 galaxies in various environments from
  the morpho-kinematic analysis of the MAGIC sample
  The evolution of galaxies is influenced by many physical processes which may
vary depending on their environment. We combine Hubble Space Telescope (HST)
and Multi-Unit Spectroscopic Explorer (MUSE) data of galaxies at 0.25<z<1.5 to
probe the impact of environment on the size-mass relation, the Main Sequence
(MS) and the Tully-Fisher relation (TFR).
  We perform a morpho-kinematic modelling of 593 [Oii] emitters in various
environments in the COSMOS area from the MUSE-gAlaxy Groups In Cosmos (MAGIC)
survey. The HST F814W images are modelled with a bulge-disk decomposition to
estimate their bulge-disk ratio, effective radius and disk inclination. We use
the [Oii]{\lambda}{\lambda}3727, 3729 doublet to extract the ionised gas
kinematic maps from the MUSE cubes, and we model them for a sample of 146 [Oii]
emitters, with bulge and disk components constrained from morphology and a dark
matter halo.
  We find an offset of 0.03 dex on the size-mass relation zero point between
the field and the large structure subsamples, with a richness threshold of N=10
to separate between small and large structures, and of 0.06 dex with N=20.
Similarly, we find a 0.1 dex difference on the MS with N=10 and 0.15 dex with
N=20. These results suggest that galaxies in massive structures are smaller by
14% and have star formation rates reduced by a factor of 1.3-1.5 with respect
to field galaxies at z=0.7. Finally, we do not find any impact of the
environment on the TFR, except when using N=20 with an offset of 0.04 dex. We
discard the effect of quenching for the largest structures that would lead to
an offset in the opposite direction. We find that, at z=0.7, if quenching
impacts the mass budget of galaxies in structures, these galaxies would have
been affected quite recently, for roughly 0.7-1.5 Gyr. This result holds when
including the gas mass, but vanishes once we include the asymmetric drift
correction.
