Fig. 9.
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For nonsaturated VVV-PSF stars, the intrinsic extinction 
(top panel) and 
(bottom panel) is shown as a function of 
, according to the indicated extinction laws (see Table 4). The same 
values are shown in both panels, obtained from E(J − Ks) reddenings using a Surot et al. (2020) extinction law, which is also used to obtain 
values. The dashed gray line indicates a perfect correlation.
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