Table 1:
Log of the UVES observations. The S/N ratio per pixel is
given for
three representative wavelengths. (Due to the large number of pixels
in each resolution element, the S/N ratios of the table need to be
multiplied by a factor of 1.3 in order to compare them to the values
available in the literature).
Star name |
|
|
Slit |
Total exposure time |
|
|
|
|
|
Date of |
width |
Blue |
Yellow |
Red |
S/N |
S/N |
S/N |
|
V |
observation |
'' |
396 nm |
573 nm |
850 nm |
400 nm |
510 nm |
630 nm |
1 HD 2796 |
8.51 |
Oct. 2000 |
1.0 |
1800 |
1300 |
400 |
250 |
390 |
550 |
2 HD 122563 |
6.20 |
Jul. 2000 |
1.0 |
|
|
|
250 |
430 |
670 |
3 HD 186478 |
9.18 |
Oct. 2000 |
1.0 |
800 |
400 |
400 |
|
|
|
4 BD +17:3248 |
9.37 |
Oct. 2000 |
1.0 |
2700 |
2700 |
1200 |
160 |
290 |
310 |
- |
|
Jun. 2001 |
|
|
|
|
|
|
|
- |
|
Sep. 2001 |
|
|
|
|
|
|
|
5 BD -18:5550 |
9.35 |
Oct. 2000 |
1.0 |
1800 |
1200 |
600 |
220 |
410 |
630 |
- |
|
Sep. 2001 |
|
|
|
|
|
|
|
6 CD -38:245 |
12.01 |
Jul. 2000 |
1.0 |
7200 |
3600 |
3600 |
150 |
150 |
200 |
- |
|
Aug. 2000 |
|
|
|
|
|
|
|
7 BS 16467-062 |
14.09 |
Jun. 2001 |
1.0 |
3600 |
3600 |
|
90 |
140 |
170 |
- |
|
Jul. 2001 |
|
7200 |
3600 |
3600 |
|
|
|
8 BS 16477-003 |
14.22 |
Jun. 2001 |
1.0 |
14 400 |
7200 |
7200 |
90 |
130 |
170 |
9 BS 17569-049 |
13.36 |
Jun. 2001 |
1.0 |
9600 |
6600 |
3000 |
120 |
170 |
260 |
10 CS 22169-035 |
12.88 |
Oct. 2000 |
1.0 |
7200 |
3600 |
3600 |
150 |
210 |
280 |
11 CS 22172-002 |
12.73 |
Oct. 2000 |
1.0 |
7494 |
3600 |
3900 |
130 |
200 |
330 |
12 CS 22186-025 |
14.24 |
Oct. 2001 |
1.0 |
10 800 |
7200 |
3600 |
95 |
140 |
190 |
13 CS 22189-009 |
14.04 |
Oct. 2000 |
1.0 |
7200 |
3600 |
3600 |
90 |
150 |
120 |
14 CS 22873-055 |
12.65 |
May 2001 |
1.0 |
7200 |
3600 |
3600 |
140 |
150 |
200 |
- |
|
Sep. 2001 |
|
|
|
|
|
|
|
15 CS 22873-166 |
11.82 |
Oct. 2000 |
1.0 |
5400 |
2700 |
2700 |
160 |
240 |
300 |
16 CS 22878-101 |
13.73 |
Jul. 2000 |
1.0 |
14 400 |
7200 |
7200 |
85 |
100 |
120 |
17 CS 22885-096 |
13.33 |
Jul. 2000 |
1.0 |
15 835 |
9184 |
6600 |
160 |
250 |
410 |
- |
|
Aug. 2000 |
|
|
|
|
|
|
|
18 CS 22891-209 |
12.17 |
Oct. 2000 |
1.0 |
5400 |
2700 |
2700 |
160 |
200 |
350 |
19 CS 22892-052 |
13.18 |
Sep. 2001 |
1.0 |
7200 |
3600 |
3600 |
140 |
130 |
190 |
20 CS 22896-154 |
13.64 |
Oct. 2000 |
1.0 |
12 600 |
7200 |
5400 |
110 |
230 |
200 |
21 CS 22897-008 |
13.33 |
Oct. 2000 |
1.0 |
10 800 |
5400 |
5400 |
100 |
170 |
180 |
22 CS 22948-066 |
13.47 |
Sep. 2001 |
1.0 |
7200 |
3600 |
3600 |
100 |
130 |
130 |
23 CS 22949-037 |
14.36 |
Aug. 2000 |
1.0 |
30 000 |
19 200 |
10 800 |
110 |
180 |
170 |
- |
|
Sep. 2001 |
|
|
|
|
|
|
|
24 CS 22952-015 |
13.28 |
Oct. 2000 |
1.0 |
10 200 |
4800 |
5400 |
150 |
220 |
250 |
25 CS 22953-003 |
13.72 |
Sep. 2001 |
1.0 |
13 500 |
9900 |
3600 |
140 |
160 |
210 |
26 CS 22956-050 |
14.27 |
Sep. 2001 |
1.0 |
9000 |
5400 |
3600 |
75 |
95 |
130 |
27 CS 22966-057 |
14.32 |
Sep. 2001 |
1.0 |
9000 |
5400 |
3600 |
80 |
105 |
120 |
28 CS 22968-014 |
13.72 |
Oct. 2000 |
1.0 |
14 100 |
8700 |
5400 |
150 |
220 |
240 |
29 CS 29491-053 |
12.92 |
Oct. 2001 |
1.0 |
5800 |
2900 |
2900 |
140 |
205 |
230 |
30 CS 29495-041 |
13.34 |
Jun. 2001 |
1.0 |
7200 |
3600 |
3600 |
115 |
130 |
170 |
- |
|
Sep. 2001 |
|
|
|
|
|
|
|
31 CS 29502-042 |
12.71 |
Oct. 2000 |
1.0 |
13 500 |
9900 |
3600 |
290 |
310 |
330 |
- |
|
Sep. 2001 |
|
|
|
|
|
|
|
32 CS-29516-024 |
13.59 |
Jun. 2001 |
1.0 |
3600 |
3600 |
|
140 |
205 |
230 |
33 CS 29518-051 |
13.02 |
Oct. 2000 |
1.0 |
7200 |
3600 |
3600 |
100 |
150 |
190 |
34 CS 30325-094 |
12.33 |
Jul. 2000 |
1.0 |
7200 |
6300 |
3600 |
110 |
220 |
280 |
- |
|
Aug. 2000 |
|
|
|
|
|
|
|
35 CS 31082-001 |
11.70 |
Aug. 2000 |
1.0 |
2400 |
1200 |
1200 |
-* |
-* |
-* |
- |
|
Aug. 2000 |
0.45 |
6000 |
3000 |
3000 |
|
|
|
- |
|
Oct. 2000 |
0.45 |
25 200 |
10 800 |
14 400 |
|
|
|
* For CS 31082-001 the details of the
observations are given in Hill et al. (
2002).
Source LaTeX |
All tables |
In the text