  The Microchannel X-ray Telescope (MXT) is an innovative compact X-ray
instrument on board the SVOM astronomical mission dedicated to the study of
transient phenomena such as gamma-ray bursts. During 3 weeks, we have tested
the MXT flight model at the Panter X-ray test facility under the nominal
temperature and vacuum conditions that MXT will undergo in-flight. We collected
data at series of characteristic energies probing the entire MXT energy range,
from 0.28 keV up to 9 keV, for multiple source positions with the center of the
point spread function (PSF) inside and outside the detector field of view
(FOV). We stacked the data of the positions with the PSF outside the FOV to
obtain a uniformly illuminated matrix and reduced all data sets using a
dedicated pipeline. We determined the best spectral performance of MXT using an
optimized data processing, especially for the energy calibration and the charge
sharing effect induced by the pixel low energy thresholding. Our results
demonstrate that MXT is compliant with the instrument requirement regarding the
energy resolution (<80 eV at 1.5 keV), the low and high energy threshold, and
the accuracy of the energy calibration ($\pm$20 eV). We also determined the
charge transfer inefficiency (~$10^{-5}$) of the detector and modeled its
evolution with energy prior to the irradiation that MXT will undergo during its
in-orbit lifetime. Finally, we measured the relation of the energy resolution
as function of the photon energy. We determined an equivalent noise charge of
4.9 $\pm$ 0.2 e- rms for the MXT detection chain and a Fano factor of 0.131
$\pm$ 0.003 in silicon at 208 K, in agreement with previous works. This
campaign confirmed the promising scientific performance that MXT will be able
to deliver during the mission lifetime.
