  In this work we complete a model independent analysis of dark matter
constraining its mass and interaction strengths with data from astro- and
particle physics experiments. We use the effective field theory framework to
describe interactions of thermal dark matter particles of the following types:
real and complex scalars, Dirac and Majorana fermions, and vector bosons. Using
Bayesian inference we calculate posterior probability distributions for the
mass and interaction strengths for the various spin particles. The
observationally favoured dark matter particle mass region is 10-100 GeV with
effective interactions that have a cut-off at 0.1-1 TeV. This mostly comes from
the requirement that the thermal abundance of dark matter not exceed the
observed value. Thus thermal dark matter coupled with present data implies new
physics most likely under 10 TeV.
