In one last attempt to break Buckaroo, Lizardo has him do a magnitude estimation experiment where he must give his subjective ratings of light brightness vs. the objective luminance of the stimuli. Fitting Buckaroo's data with a power function, Lizardo finds that the best-fitting parameters are k = 3 and b = .5. What would we expect Buckaroo's subjective rating to be for a light of 36 cd/m^2?

MATLAB: An Introduction with Applications
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Author:Amos Gilat
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In one last attempt to break Buckaroo,
Lizardo has him do a magnitude estimation
experiment where he must give his
subjective ratings of light brightness vs. the
objective luminance of the stimuli. Fitting
Buckaroo's data with a power function,
Lizardo finds that the best-fitting
parameters are k = 3 and b = .5. What
would we expect Buckaroo's subjective
rating to be for a light of 36 cd/m^2?
Transcribed Image Text:In one last attempt to break Buckaroo, Lizardo has him do a magnitude estimation experiment where he must give his subjective ratings of light brightness vs. the objective luminance of the stimuli. Fitting Buckaroo's data with a power function, Lizardo finds that the best-fitting parameters are k = 3 and b = .5. What would we expect Buckaroo's subjective rating to be for a light of 36 cd/m^2?
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