Table 1: Log of observations.

Date
UT Filter/ Mag. Exp. frames
    Grating   (s)  

2.2 m Calar Alto
 
2000 Sep. 20 22:26-22:40 ${\displaystyle B-200\atop
\displaystyle R-200}$ $V\simeq17.3$ 600 1/1

1.2 m Kryoneri Observatory
 
2002 Sep. 17 00:36-03:16 R $\simeq$17.6 90 97
2002 Sep. 17 22:40-23:11 R $\simeq$17.5 60 25
2002 Sep. 18 19:04-23:41 R $\simeq$17.6 60 210

1 m OGS
 
2003 Jul. 08 03:27-05:24 Clear $\simeq$15.7 15 390
2003 Jul. 10 01:21-03:47 Clear $\simeq$12.2 15 515
2003 Jul. 11 02:47-04:06 Clear $\simeq$12.2 12 37
2003 Jul. 14 01:21-03:59 Clear $\simeq$12.5 12 548
2003 Jul. 16 02:20-05:31 Clear $\simeq$12.8 12 617

0.82 m IAC80
 
2003 Sep. 25 00:19-03:14 Clear $\simeq$17.4 70 74
2003 Sep. 26 00:32-03:14 Clear $\simeq$17.5 70 119
2003 Sep. 27 23:31-03:10 Clear $\simeq$17.5 70 160
2003 Sep. 28 20:01-23:35 Clear $\simeq$17.5 70 147

4.2 m WHT
 
2003 Oct. 19 19:35-22:58 ${\displaystyle R600B\atop
\displaystyle R316R}$   400 28


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