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Three dimensional interstellar extinction map toward the Galactic bulge

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Figure

Fig. 2. Star counts of VVV-survey data of two example fields for the 2MASS bands. Each field is 15  × 15  .
Fig. 4. a): log T e ff vs. log g grid in the Besançon model. Black trian- trian-gles indicate the coverage of the Besançon model (Robin et al
Fig. 5. Comparison of the Ks–[4.5] vs. [4.5] diagram of Baade window (left panel) with the old (middle panel) and the new temperature vs
Table 1. Extinction as a function of Galactic longitude, latitude, and distance based on VVV data.
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