Fig. 6

Simulation showing convergence of the gain solution for one year of observations of one 30GHz detector. The simulations include CMB dipole(s), CMB anisotropies, and Galactic emission. The input gain was 12.86 K/V and the sky included all diffuse components as well as nominal instrument noise. The first iteration shows large errors caused by Galactic and CMB anisotropy emissions; however, after one hundred iterations, convergence is achieved with an overall deviation from the input value of less than 0.01%. The various curves show the solution after 1, 30, 60 and 100 iterations.
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