Table 1: Journal of observations.
June, 16, 2003 night, B = 102 m, PA = 7 $\hbox {$^\circ $ }$
Star Template Time Frames
HD 165 135 tracking 00:36:11 15 000
HD 165 135 phot. UT1 00:42:33 2000
HD 165 135 phot. UT3 00:44:12 2000
HD 152 786 tracking 01:06:42 12 000
HD 152 786 phot. UT1 01:12:15 3000
HD 152 786 phot. UT3 01:14:33 3000
$\alpha $ Ara tracking 01:35:27 12 000
$\alpha $ Ara phot. UT1 01:40:55 3000
$\alpha $ Ara phot. UT3 01:43:12 3000
HD 165 135 tracking 02:46:05 12 000
HD 165 135 phot. UT1 02:51:32 3000
HD 165 135 phot. UT3 02:46:05 3000
$\alpha $ Aql tracking 06:44:35 12 000
$\alpha $ Aql phot. UT1 06:50:08 3000
$\alpha $ Aql phot. UT3 06:52:14 3000
June, 17, 2003 night, B=79 m, PA = 55 $\hbox {$^\circ $ }$
HD 139 997 tracking 05:31:17 10 000
HD 139 997 phot. UT1 05:35:38 2000
HD 139 997 phot. UT3 05:37:29 2000
HD 168 545 tracking 06:35:05 15 000
HD 168 545 phot. UT1 06:40:33 2000
HD 168 545 phot. UT3 06:42:21 2000
$\alpha $ Ara tracking 07:09:19 12 000
$\alpha $ Ara phot. UT1 07:14:47 3000
$\alpha $ Ara phot. UT3 07:17:05 3000


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations
3 The SIMECA code and the envelope parameters used for the modeling of alpha Ara
4 Results
5 Discussion
6 Conclusion
References
List of tables
List of figures