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.
| Date |
UT |
Exp.time |
Wavelength |
S/N |
| |
start |
(s) |
interval (Å) |
|
| VLT-UT2 + UVES |
| 2005-02-08 |
02:49 |
7200 |
4780-6808 |
70 |
|
2005-02-09 |
00:30 |
7200 |
3758-4983 |
40 |
|
2005-02-09 |
00:30 |
7200 |
6705-10084 |
80 |
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