Table 1:
Basic data for the observations and the pulsation properties of the program stars.
| HD |
HJD |
 |
Spectral type |
SNR |
Exp. time |
log P |
Q |
Remarks |
| |
|
[mag] |
|
|
[s] |
|
[d] |
|
| 127929 |
2 454 170.650 |
6.27 |
F0III |
238 |
550 |
-1.06 |
0.018 |
|
| 138918 |
2 454 170.693 |
3.80 |
F0IV |
286 |
550 |
-0.81 |
0.032 |
binary |
| 143466 |
2 454 171.703 |
4.97 |
F0IV |
465 |
550 |
-1.12 |
0.029 |
|
| 124675 |
2 454 170.598 |
4.74 |
A8IV |
390 |
600 |
-1.19 |
0.015 |
binary |
| 124953 |
2 454 170.614 |
5.97 |
A8III |
257 |
550 |
|
|
binary? |
| 125161 |
2 454 170.626 |
4.75 |
A9V |
295 |
550 |
-1.58 |
0.013 |
|
| 127762 |
2 454 170.686 |
3.00 |
A7III |
334 |
550 |
-1.14 |
0.017 |
binary |
The SNR is calculated at  5500 Å in a bin of 0.5 Å. The exposure time is in
seconds. The HJD indicates the Heliocentric Julian Date at the end of the
exposure. The analysed spectrum of HD 127929 is the sum of two spectra with the
same exposure time. Periods and Q values are taken from Rodríguez et al. (2000) and
López de Coca et al. (1990).
|
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