Redshifts of quasi-stellar objects. Refer to the Journal of Astrophysics & Astronomy (Mar./Jun. 2003) study of red- shifts in quasi-stellar objects presented in Exercise 11.27 (p. 599). Recall that simple linear regression was used to model the magnitude (y) of a quasi-stellar object as a function of the redshift level (x). In addition to the least 10 12

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11.90 Redshifts of quasi-stellar objects. Refer to the Journal of
Astrophysics & Astronomy (Mar./Jun. 2003) study of red-
COLS shifts in quasi-stellar objects presented in Exercise 11.27
g (p. 599). Recall that simple linear regression was used
hsv to model the magnitude (y) of a quasi-stellar object as a
ol ( function of the redshift level (x). In addition to the least
aldet s
squares line, ŷ = 18.13 + 6.21x, the coefficient of correla-
%3D
19s tion was determined to be r =
sonsa. Interpret the value of rin the words of the problem.
b. What is the relationship between r and the estimated
alucelo slope of the line?
eon dmu hila
.84.
%3D
c. Find and interpret the value of r2.
Transcribed Image Text:11.90 Redshifts of quasi-stellar objects. Refer to the Journal of Astrophysics & Astronomy (Mar./Jun. 2003) study of red- COLS shifts in quasi-stellar objects presented in Exercise 11.27 g (p. 599). Recall that simple linear regression was used hsv to model the magnitude (y) of a quasi-stellar object as a ol ( function of the redshift level (x). In addition to the least aldet s squares line, ŷ = 18.13 + 6.21x, the coefficient of correla- %3D 19s tion was determined to be r = sonsa. Interpret the value of rin the words of the problem. b. What is the relationship between r and the estimated alucelo slope of the line? eon dmu hila .84. %3D c. Find and interpret the value of r2.
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