  The comprehensive statistical analysis of Swift X-ray light-curves,
collecting data from six years of operation, revealed the existence of a
universal scaling among the isotropic energy emitted in the rest frame 10-10^4
keV energy band during the prompt emission (E_{gamma,iso}), the peak of the
prompt emission energy spectrum (E_{pk}), and the X-ray energy emitted in the
0.3-10 keV observed energy band (E_{X,iso}). In this paper we show that this
three-parameter correlation is robust and does not depend on our definition of
E_{X,iso}. It is shared by long, short, and low-energetic GRBs, differently
from the well-known E_{gamma,iso}-E_{pk} correlation. We speculate that the
ultimate physical property that regulates the GRB properties is the outflow
Lorentz factor.
