  We use data from the ARGO cosmic microwave background (CMB) anisotropy
experiment to constrain cosmogonies. We account for the ARGO beamwidth and
calibration uncertainties, and marginalize over the offset removed from the
data. Our derived amplitudes of the CMB anisotropy detected by the ARGO
experiment are smaller than those derived previously.
  We consider open and spatially-flat-Lambda cold dark matter cosmogonies, with
clustered-mass density parameter Omega_0 in the range 0.1-1, baryonic-mass
density parameter Omega_B in the range (0.005-0.029)h^{-2}, and age of the
universe t_0 in the range (10--20) Gyr. Marginalizing over all parameters but
Omega_0, the ARGO data favors an open (spatially-flat-Lambda) model with
Omega_0= 0.23 (0.1). However, these numerical values are model dependent.
  At the 2 sigma confidence level model normalizations deduced from the ARGO
data are consistent with those drawn from the UCSB South Pole 1994, MAX 4+5,
White Dish, and SuZIE data sets. The ARGO open model normalizations are also
consistent with those deduced from the DMR data. However, for most
spatially-flat-Lambda models the DMR normalizations are more than 2 sigma above
the ARGO ones.
