Table 1
Characterization of the observed fields.
| Field | l | b |
|
E(J−K)G11 | E(J−K)fit | NG/Nfld |
| name | ||||||
|
|
||||||
| p1m4 | 1.00 | –3.97 | 364 | 0.26 | 0.20 | 359/369 |
| p0m6 | 0.18 | –6.03 | 254 | 0.14 | 0.17 | 180/204 |
| m1m10 | –0.74 | –9.45 | 340 | 0.03 | 0.06 | 131/187 |
| p7m9 | 6.85 | –8.87 | 244 | 0.10 | 0.11 | 200/221 |
| m10m8 | –9.78 | –8.09 | 347 | 0.03 | 0.08 | 234/310 |
| m4m5 | –3.72 | –5.18 | 192 | 0.19 | 0.18 | 89/94 |
| m6m6 | –6.57 | –6.18 | 168 | 0.13 | 0.13 | 189/206 |
| p0m8 | 0.03 | –8.06 | 310 | 0.06 | 0.07 | 81/98 |
| p2m9 | 1.71 | –9.22 | 362 | 0.08 | 0.08 | 81/105 |
| p8m6 | 7.63 | –5.86 | 250 | 0.22 | 0.20 | 284/302 |
| p6m9 | 6.01 | –9.62 | 279 | 0.09 | 0.08 | 159/196 |
Notes. Signal-to-noise ratios are the field average. E(J−K)G11 corresponds to the reddening as computed from the extinction maps of Gonzalez et al. (2011) in a box of 30 arcmin per side centered in the respective (l, b) coordinates. E(J−K)fit values are those estimated in Sect. 3 from isochrone fitting. Finally, NG/Nfld provides the ratio between giant (log (g) < 3.5) and the total number of stars per field.
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