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Table 1:

Log of the AMBER observations of WR 118 ( top) and the corresponding calibrators ( bottom).
Object
Date Time Name $B_{\rm p}$[*] PA[*] seeing
  [UTC]   [m] [ $\hbox{$^\circ$ }$] [ $\hbox{$^{\prime\prime}$ }$]
2007-10-08 02:18:53 WR 118 9.2 74.3 0.61
2008-03-28 08:43:43 WR 118 13.4-40.2 61.7 0.83
2008-03-31 06:51:05 WR 118 9.6-28.8 42.6 0.73
2008-03-31 07:09:33 WR 118 10.3-32.0 47.6 0.86
calibrators
Date Time HD UD[*] spectral seeing
  [UTC] number [mas] type[*] [ $^{\prime\prime}$]
2007-10-08 01:07:58 175583 $1.02\pm 0.01$ K2III 0.66
2008-03-28 09:33:52 175583 $1.02\pm 0.01$ K2III 0.60
2008-03-31 07:42:46 175583 $1.02\pm 0.01$ K2III 0.81
2008-03-31 08:20:04 165524 $1.11\pm 0.01$ K3III 0.80


Source LaTeX | All tables | In the text

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