Table 2
Results for the programme targets.
| Cluster | log t | (m − M)0 | E(B − V)a | Z | [Fe/H]DG | [Fe/H]specb | Phot. systemsc |
|
|
|||||||
| Berkeley 11 | 7.80 | 12.20 | 0.96(6) | 0.020(5) | +0.01(14) | UBVpe, UBVRIccd | |
| Collinder 140 | 7.55 | 8.05 | 0.04(4) | 0.021(3) | +0.04(7) | UBVpe, Strpe, G | |
| Collinder 272 | 7.30 | 11.75 | 0.43(3) | 0.021(4) | +0.06(9) | UBVRI ccd | |
| IC 2391 | 7.65 | 5.80 | 0.01(1) | 0.018(3) | −0.03(7) | −0.02(1)/2 | UBVpe, Strpe, G |
| IC 2602 | 7.85 | 5.85 | 0.03(2) | 0.019(3) | +0.00(8) | −0.03(4)/2 | UBVpe, Strpe, G |
| IC 4665 | 7.70 | 7.70 | 0.19(3) | 0.020(2) | +0.02(6) | −0.03(4)/1 | UBVpe, Strpe, G |
| IC 4725 | 7.85 | 9.00 | 0.45(5) | 0.020(3) | +0.03(8) | +0.02(2)/1 | UBVpe, Strpe |
| King 21 | 7.30 | 12.40 | 0.86(6) | 0.021(6) | +0.06(14) | UBVpe, Δa, 2M | |
| Lynga 1 | 8.10 | 11.40 | 0.45(4) | 0.021(4) | +0.04(10) | UBVpe, UBVRIccd | |
| Melotte 20 | 7.75 | 6.15 | 0.09(3) | 0.021(5) | +0.05(13) | +0.09(20)/2 | UBVpe, Strpe, G |
| Melotte 22 | 8.05 | 5.50 | 0.04(2) | 0.016(2) | −0.08(7) | +0.02(4)/5 | UBVpe, Strpe, G |
| Melotte 105 | 8.60 | 11.85 | 0.44(4) | 0.022(5) | +0.08(12) | UBVIccd, Strccd | |
| Melotte 111 | 8.85 | 4.70 | 0.00(1) | 0.018(2) | −0.04(5) | +0.01(8)/2 | UBVpe, Strpe, G |
| NGC 1039 | 8.25 | 8.35 | 0.08(2) | 0.021(4) | +0.05(10) | +0.07(4)/1 | UBVpe, BVccd, Strpe, G |
| NGC 1662 | 8.60 | 8.05 | 0.32(3) | 0.021(3) | +0.05(8) | UBVpe, Strpe, G | |
| NGC 1901 | 8.90 | 8.20 | 0.03(2) | 0.019(2) | +0.01(5) | −0.08(1)/1 | UBVpe, UBVccd, Strpe |
| NGC 2099 | 8.65 | 10.55 | 0.30(1) | 0.019(2) | +0.00(4) | +0.01(5)/1 | UBV pe |
| NGC 2232 | 7.70 | 7.65 | 0.03(2) | 0.025(6) | +0.14(12) | +0.22(9)/1 | UBVpe, Strpe, G |
| NGC 2287 | 8.40 | 9.10 | 0.02(2) | 0.014(3) | −0.16(9) | −0.23(2)/1 | UBVpe, Strpe, G |
| NGC 2343 | 8.05 | 9.90 | 0.20(2) | 0.021(6) | +0.05(14) | UBVpe, byccd | |
| NGC 2422 | 8.15 | 8.50 | 0.09(2) | 0.023(4) | +0.09(8) | UBVpe, UBVIccd, Strpe, G | |
| NGC 2423 | 9.00 | 9.80 | 0.10(1) | 0.024(5) | +0.11(10) | +0.14(6)/1 | Strpe, G, APASS |
| NGC 2447 | 8.75 | 10.13 | 0.01(1) | 0.020(3) | +0.03(7) | −0.03(6)/4 | Strpe, G |
| NGC 2451A | 7.70 | 6.35 | 0.01(1) | 0.017(4) | −0.06(11) | UBVpe, BVccd, Strpe, G | |
| NGC 2451B | 7.70 | 7.95 | 0.10(3) | 0.020(3) | +0.02(9) | UBVpe, Strpe, G | |
| NGC 2489 | 8.75 | 11.30 | 0.31 | 0.022(4) | +0.06(10) | UBVI ccd | |
| NGC 2516 | 8.25 | 8.05 | 0.11(3) | 0.020(5) | +0.03(12) | +0.01(7)/1 | UBVpe, Strpe, G |
| NGC 2546 | 8.15 | 9.75 | 0.14(3) | 0.020(4) | +0.01(9) | UBVpe, APASS, 2M | |
| NGC 2567 | 8.45 | 11.05 | 0.13(3) | 0.020(4) | +0.02(10) | +0.00(5)/1 | UBV pe |
| NGC 2632 | 8.80 | 6.30 | 0.01(1) | 0.027(5) | +0.17(9) | +0.14(10)/4 | UBVpe, Strpe, G |
| NGC 2658 | 8.50 | 13.05 | 0.36(3) | 0.020(5) | +0.02(12) | UBVRI ccd | |
| NGC 3114 | 8.20 | 9.85 | 0.07(2) | 0.022(5) | +0.07(11) | +0.04(2)/2 | UBVpe, Strpe, G |
| NGC 3228 | 7.85 | 8.35 | 0.04(1) | 0.020(4) | +0.03(10) | UBVpe, Genf | |
| NGC 3532 | 8.55 | 8.35 | 0.04(2) | 0.021(3) | +0.04(7) | +0.05(4)/3 | UBVpe, Strpe, G |
| NGC 3960 | 9.00 | 11.65 | 0.29 | 0.020(4) | +0.03(9) | +0.02(4)/1 | BVpe, UBVIccd |
| NGC 5281 | 7.90 | 10.70 | 0.22(1) | 0.019(4) | +0.00(11) | UBVpe, BVIccd | |
| NGC 5460 | 8.20 | 9.20 | 0.13(1) | 0.021(4) | +0.06(9) | +0.05(24)/1 | UBVpe, Strpe, G |
| NGC 5662 | 8.05 | 9.30 | 0.30(4) | 0.022(4) | +0.06(9) | UBVpe, Strpe | |
| NGC 5999 | 8.70 | 11.75 | 0.46 | 0.019(3) | +0.00(8) | BVpe, BVIccd | |
| NGC 6031 | 8.40 | 11.00 | 0.44(3) | 0.020(4) | +0.02(9) | UBVpe, BVIccd | |
| NGC 6087 | 7.95 | 9.60 | 0.19(2) | 0.022(5) | +0.06(12) | +0.06(20)/1 | UBVpe, Strpe |
| NGC 6134 | 9.00 | 10.00 | 0.40(3) | 0.026(5) | +0.16(9) | +0.14(2)/3 | UBVpe, BVccd, Strccd |
| NGC 6192 | 8.20 | 11.05 | 0.63(4) | 0.026(7) | +0.16(13) | +0.12(4)/1 | UBVpe, BVccd, 2M |
| NGC 6204 | 8.05 | 10.25 | 0.47(1) | 0.021(5) | +0.05(12) | UBVpe, BVIccd, byccd | |
| NGC 6281 | 8.40 | 8.65 | 0.17(3) | 0.021(3) | +0.04(7) | +0.05(6)/1 | UBVpe, Strpe, G |
| NGC 6405 | 7.90 | 8.45 | 0.17(2) | 0.023(5) | +0.09(11) | UBVpe, Strpe, G | |
| NGC 6451 | 8.00 | 11.75 | 0.75 | 0.021(4) | +0.04(10) | BV I ccd | |
| NGC 6475 | 8.40 | 7.15 | 0.07(3) | 0.024(5) | +0.11(11) | +0.09(8)/2 | UBVpe, Strpe, G |
| NGC 6705 | 8.40 | 11.60 | 0.39(3) | 0.027(5) | +0.18(8) | +0.17(9)/2 | UBVI ccd |
| NGC 6756 | 8.10 | 12.30 | 1.03(5) | 0.023(6) | +0.10(14) | Strccd | |
| NGC 6802 | 9.00 | 11.65 | 0.79 | 0.020(5) | +0.03(13) | BV I ccd | |
| NGC 6830 | 8.10 | 11.90 | 0.54(4) | 0.031(3) | +0.24(5) | UBVpe, Δa, 2M | |
| NGC 7092 | 8.55 | 7.45 | 0.03(2) | 0.020(3) | +0.02(9) | UBVpe, Strpe, G | |
| NGC 7243 | 8.00 | 9.45 | 0.24(3) | 0.021(6) | +0.06(13) | UBVpe, Strpe, G | |
| NGC 7296 | 8.55 | 12.15 | 0.20 | 0.019(5) | +0.00(13) | BVR I ccd | |
| Ruprecht 115 | 8.65 | 11.35 | 0.74 | 0.021(3) | +0.04(7) | BV I ccd | |
| Ruprecht 130 | 8.75 | 11.50 | 1.00 | 0.020(5) | +0.03(14) | BVIccd, 2M/UKIDSS | |
| Trumpler 10 | 7.80 | 8.05 | 0.03(1) | 0.016(3) | −0.07(10) | UBVpe, APASS, Strpe, G | |
Notes.
The standard deviation of reddening is given in parentheses, if reddening was determined via photometric calibrations (e.g. UBV − Q method).
The mean spectroscopic [Fe/H] ratio and the standard deviation in parentheses. The number of studies used (listed by Carrera & Pancino 2011, and additional literature) is given by /#.
Photometric systems or surveys used for the analysis, e.g. G (Geneva), Str (Strömgren), 2M (2MASS), whereas pe/ccd stands for photoelectric and CCD data, respectively. For some clusters, V/(b − y) data by McSwain & Gies (2008) were included (byccd), or Δa photometry transformed to V/(B − V) as discussed in Sect. 4.
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