All Tables

Table 1: Basic parameters of MACHO 47.2496.8.
Table 2: Optical Geneva and near-IR photometry of MACHO 47.2496.8, together with their JD and phase. The Geneva R and I are from the Gunn resp. Cousins photometric systems.
Table 3: Log of the high-resolution VLT-UVES observations. Small spectral gaps occur between 5757 Å and 5833 Å and between 8521 Å and 8660 Å due to the spatial gap between the two UVES CCDs. Since continuum spectral intervals are hardly found in the spectrum, the signal-to-noise ratios S/N given in the rightmost column, are only indicative, and should be interpreted more as lower limits than as fixed values.
Table 4: The abundance results for MACHO 47.2496.8. The atmospheric parameters of the model atmosphere are given in Sect. 4.2. The adopted carbon-oxygen difference in the syntheses is $\log(\epsilon({\rm C})-\epsilon({\rm O}))$ = 7.98. The explanation of the different columns is given in the text (Sect. 4.3). At the bottom, the usual s-process indices, together with metallicity, are given. More information on the calculation of these indices is found in the Sect. 4.7. The elements C and O are not separately included in the table due to the specific difficulties for these elements that are discussed in Sect. 4.4.