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Fig. 4.

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2D distribution of the spectral index for all quasars in the study. The four quadrants represent different shapes of the radio spectra. The blue stars in the lower-right quadrant are the MPS samples discussed in this paper. Red dots indicate sources that meet 0 < α 54 144 < 0.1 $ 0 < \alpha^{144}_{54} < 0.1 $ and α 144 1400 < 0 $ \alpha^{1400}_{144} < 0 $ criteria, and light blue dots represent the remaining samples. The horizontal solid, vertical solid, vertical dashed, and horizontal dashed gray lines represent the α 144 1400 = 0 $ \alpha^{1400}_{144}=0 $, α 54 144 = 0.1 $ \alpha^{144}_{54}=0.1 $, α 54 144 = 0 , $ \alpha^{144}_{54}=0, $ and 1-to-1 lines. The typical median error of samples is represented by black lines in the bottom-right corner. The median errors are 0.09 and 0.03 for α 54 144 $ \alpha^{144}_{54} $ and α 144 1400 $ \alpha^{1400}_{144} $, respectively. Top and right: Histogram of the spectral index, with colors corresponding to those in the middle panel. The vertical lines represent the median values of each sample.

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