Table 3
Temperatures derived from photometric data by using the final metallicity found for each star.
| Star | [Fe/H] | T BV | T VR | T VI | T VK | T JK | T JH |
|
|
|||||||
| DMA subsample | |||||||
| BS 15621-047 | –2.29 | 4730 | 4860 | 4870 | 4770 | 4620 | 4740 |
| –2.35 | 4730 | 4870 | 4860 | 4780 | 4620 | 4740 | |
| BS 16033-081 | –2.20 | 5170 | 5020 | 5020 | 5140 | 5090 | 5040 |
| –2.07 | 5180 | 5020 | 5010 | 5130 | 5090 | 5060 | |
| BS 16077-077 | –2.05 | 5440X | ... | ... | 4220X | 5890 | 5830 |
| –2.00 | 5450X | ... | ... | 4220X | 5890 | 5830 | |
| BS 16082-129 | –2.65 | 5090 | 4980 | 5010 | 5100 | 5050 | 4970 |
| –2.59 | 5100 | 4980 | 5010 | 5090 | 5050 | 4970 | |
| BS 16543-097 | –2.48 | 5170 | 5000 | 5030 | 5090 | 4990 | 5040 |
| –2.36 | 5170 | 5000 | 5020 | 5090 | 4990 | 5050 | |
| BS 16929-005 | –3.15 | 5400 | 5190 | 5350 | 5360 | 5180 | 4990 |
| –3.02 | 5390 | 5190 | 5340 | 5350 | 5180 | 5020 | |
| CS 22949-008 | –2.45 | 5740 | 5950 | 5920 | 5990 | 5960 | 5750 |
| –2.61 | 5740 | 5960 | 5920 | 6000 | 5960 | 5750 | |
| CS 29503-010 | –1.69 | 5990 | 5950 | 5840 | 6260 | 6220 | 6050 |
| –1.70 | 5990 | 5950 | 5840 | 6260 | 6220 | 6050 | |
| CS 29512-073 | –2.06 | 5680 | 5520 | 5460 | 5850 | 5750 | 5560 |
| –1.88 | 5690 | 5520 | 5460 | 5840 | 5750 | 5580 | |
| CS 29526-110 | –2.19 | 6600 | 6390 | 6470 | 7100 | 6790 | 6320 |
| –2.29 | 6600 | 6390 | 6480 | 7110 | 6790 | 6300 | |
| CS 29528-028 | –2.12 | 6500 | 6690 | 6790 | 6960 | 6840 | 6350 |
| –2.17 | 6500 | 6690 | 6790 | 6970 | 6840 | 6350 | |
| CS 31070-073 | –2.55 | 6020 | 5750 | 5800 | 6200 | 5950 | 5820 |
| –2.64 | 6020 | 5750 | 5810 | 6210 | 5950 | 5800 | |
|
|
|||||||
| SAT subsample | |||||||
| BS 16080-175 | –1.36 | 5942 | 6329 | 6247 | ... | 6328 | 5970 |
| BS 17436-058 | –1.90 | 4986 | 5246 | 5209 | ... | 5416 | 5467 |
| CS 22183-015 | –2.85 | 5291 | 5416 | 5468 | ... | 5600 | 5588 |
| CS 22887-048 | –1.70 | ... | ... | ... | ... | 6508 | 6581 |
| CS 22898-027 | –2.30 | 6039 | 6562 | ... | ... | 6477 | 6363 |
| CS 29502-092 | –3.05 | 5224 | 5064 | 5068 | ... | 4978 | 5060 |
Notes. For the DMA subsample, the first and second lines show the results for stellar parameters using [FeI/H] and [FeII/H], respectively. For the SAT subsample only one [Fe/H] value is given since ionisation balance was forced in determining log g. A suffix “X” indicates that the value was not used.
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