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We perform a cosmological parameter analysis of the 75 square degree CTIO lensing survey in conjunction with CMB and Type Ia supernovae data. For Lambda CDM cosmologies, we find that the amplitude of the power spectrum at low redshift is given by sigma₈ = 0. 812+0. 146, -0. 100 (95% c. l. ), where the error bar includes both statistical and systematic errors. The total of all systematic errors is smaller than the statistical errors, but they do make up a significant fraction of the error budget. We find that weak lensing improves the constraints on dark energy as well. The (constant) dark energy equation of state paremeter, w, is measured to be -0. 894+0. 156, -0. 208 (95% c. l. ). Marginalizing over a constant w slightly changes the estimate of sigma₈ to 0. 790+0. 170, -0. 141 (95% c. l. ). We also investigate variable w cosmologies, but find that the constraints weaken considerably; the next generation surveys are needed to obtain meaningful constraints on the possible time evolution of dark energy.
Jarvis et al. (Sat,) studied this question.