Table 5
Comparison of E(B–V) values of stars in sample considering different approaches.
| SPIPS(a) | DDOD(b) (n) | Stilism 3D map | SFD98 2D map(c) | |
|---|---|---|---|---|
| RS Pup |  |
 |
 |
 |
| ζ Gem |  |
 |
 |
 |
| η Aql |  |
 |
 |
 |
| V Cen(d) |  |
 |
 |
 |
| SU Cyg |  |
 |
 |
 |
Notes. (a) E(B–V) values are calculated from the SPIPS algorithm. (b)David Dunlap Observatory Database. Standard error is the deviation of the number (n) of measurements present in the literature. (c)Values were corrected by taking into account the star location using three-dimensional model for the Milky Way. (d) Extinction values are in agreement with extinction of others members of the open cluster NGC 5662 giving in average E(B–V) = 0.31 ± 0.04 (Claria et al. 1991).
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