a. The figure shows normal quantile plots of beetle orientation errors in the two groups of beetles. Each dot is the orientation error of a single beetle. Which frequency distribution of orientation errors deviated most from the normal distribution? Explain how you mined this. b. The data below are measurements for 10 ran- domly selected beetles from each group. Use to h the data and the Mann–Whitney U-test to test dee whether the distribution of orientation errors differs between beetle groups under simulated Milky Way and equal-intensity illumination conditions. Optional: Instead, use a computer to analyze the full data set available at whitlockschluter3e.zoology.ubc.ca. Equal intensity: 35, 50, 55, 65, 80, 80, 95, 120, limob160, 165 Milky Way: 5, 5, 10, 20, 20, 30, 40, 50, 70, 90

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question 32

a. The figure shows normal quantile plots of
beetle orientation errors in the two groups of
beetles. Each dot is the orientation error of a
single beetle. Which frequency distribution
of orientation errors deviated most from the
normal distribution? Explain how you
mined this.
b. The data below are measurements for 10 ran-
domly selected beetles from each group. Use
to h
the data and the Mann–Whitney U-test to test
dee
whether the distribution of orientation errors
differs between beetle groups under simulated
Milky Way and equal-intensity illumination
conditions. Optional: Instead, use a computer
to analyze the full data set available at
whitlockschluter3e.zoology.ubc.ca.
Equal intensity: 35, 50, 55, 65, 80, 80, 95, 120,
limob160, 165
Milky Way: 5, 5, 10, 20, 20, 30, 40, 50, 70, 90
Transcribed Image Text:a. The figure shows normal quantile plots of beetle orientation errors in the two groups of beetles. Each dot is the orientation error of a single beetle. Which frequency distribution of orientation errors deviated most from the normal distribution? Explain how you mined this. b. The data below are measurements for 10 ran- domly selected beetles from each group. Use to h the data and the Mann–Whitney U-test to test dee whether the distribution of orientation errors differs between beetle groups under simulated Milky Way and equal-intensity illumination conditions. Optional: Instead, use a computer to analyze the full data set available at whitlockschluter3e.zoology.ubc.ca. Equal intensity: 35, 50, 55, 65, 80, 80, 95, 120, limob160, 165 Milky Way: 5, 5, 10, 20, 20, 30, 40, 50, 70, 90
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