Table 3
Summary of the parameters used in the recovery of the SFH of each tile in the Magellanic Bridge.
| Tile | Coordinates | Number of stars | E(B-V) | Distance Modulus (mag) | FWHM | Phot. error at g=22.8 mag (mag) | SHARPNESS | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| RA [h:m:s] | Dec | Mean | Dispersion | g(″) | i(″) | min | max | ||||
| 2_11 | 02:23:27 | −74° 24′ 29” | 16 227 | 0.050 | 0.005 | 18.82 | 0.99, 1.20 | 0.59, 1.03 | 0.03 | −0.4 | 0.5 |
| 2_12 | 02:37:39 | −74° 24′ 29” | 14 615 | 0.060 | 0.007 | 18.85 | 1.06, 1.47 | 0.95, 1.08 | 0.03 | −0.5 | 0.5 |
| 3_11 | 02:15:00 | −73° 24′ 59” | 20419 | 0.060 | 0.008 | 18.86 | 0.98, 1.13 | 1.03, 1.07 | 0.03 | −0.4 | 0.5 |
| 3_12 | 02:28:24 | −73° 24′ 59” | 11 398 | 0.040 | 0.007 | 18.84 | 1.07, 1.17 | 1.02, 0.99 | 0.04 | −0.3 | 0.4 |
| 3_13 | 02:41:47 | −73° 24′ 59” | 11 510 | 0.060 | 0.008 | 18.77 | 1.22, 1.23 | 1.06, 1.04 | 0.05 | −1.0 | 1.0 |
| 3_14 | 02:55:11 | −73° 24′ 59” | 14061 | 0.040 | 0.008 | 18.75 | 1.12, 1.17 | 0.95, 1.02 | 0.04 | −0.4 | 0.5 |
| 3_15 | 03:08:35 | −73° 24′ 59” | 14274 | 0.035 | 0.008 | 18.73 | 1.23, 1.25 | 0.99, 0.96 | 0.03 | −0.4 | 0.55 |
| 3_16 | 03:21:58 | −73° 24′ 59” | 17 664 | 0.055 | 0.010 | 18.66 | 1.29, 1.74 | 0.83, 0.96 | 0.02 | −0.4 | 0.5 |
| 3_17 | 03:35:22 | −73° 24′ 59” | 18 739 | 0.065 | 0.010 | 18.58 | 1.19, 1.15 | 0.95, 1.02 | 0.04 | −1.0 | 1.0 |
| 3_18 | 03:48:46 | −73° 24′ 59” | 21 277 | 0.075 | 0.020 | 18.55 | 1.23, 1.01 | 1.16, 1.12 | 0.03 | −1.0 | 1.0 |
| 3_19 | 04:02:10 | −73° 24′ 59” | 27 946 | 0.090 | 0.020 | 18.50 | 1.13, 1.22 | 0.96, 0.96 | 0.04 | −1.0 | 1.0 |
| 3_20 | 04:15:34 | −73° 24′ 59” | 68 022 | 0.104 | 0.020 | 18.45 | 1.37, 1.19 | 0.75, 0.73 | 0.03 | −0.5 | 0.6 |
| 3_21 | 04:28:58 | −73° 24′ 59” | 155 884 | 0.120 | 0.030 | 18.45 | 1.36, 1.41 | 0.63, 0.78 | 0.05 | −0.55 | 0.65 |
| 4_12 | 02:20:10 | −72° 25′ 27” | 11 670 | 0.045 | 0.008 | 18.86 | 1.05, 1.21 | 0.91, 1.00 | 0.03 | −0.45 | 0.45 |
Notes. Columns provide: (1) tile name; (2 and 3) J2000 equatorial coordinates; (4) total number of stars; (5 and 6) mean E(B-V) extinction and its dispersion; (7) distance modulus (m-M)0; (8 and 9) full width half maximum in the g and i filters; (10) photometric error at g = 22.8 mag; (11 and 12) sharpness range for source selection.
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