Differences between revisions 3 and 4

Targets for observation

In case you run out of targets during the night

GOWI

M31 Nova search Mosaic 2x2 central region each 5 x 1min L -Filter
Magnetic CVs eclipse lightcurve
- HU Aqr (21 07 58.188 -05 17 40.47) L-filter high time resolution 10 - 20 sec
calibration: If photometric observe field with spectrophotometric standard star at same airmass as field to calibrate
- GRB150309A (18h 28m 21.22s +86d 25' 47.6")

-  ⇤ ← Revision 3 as of 2014-11-14 18:30:39 → 
  Size: 370
  Editor: VadimBurwitz
  Comment:
+   ← Revision 4 as of 2015-03-12 13:43:21 → ⇥
  Size: 542
  Editor: TassiloSchweyer
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
 Line 11:
-  * HU Aqr    21 07 58.188 -05 17 40.47  L-filter high time resolution 10 - 20 sec
+  * HU Aqr (21 07 58.188 -05 17 40.47)  L-filter high time resolution 10 - 20 sec
 
 * calibration: If photometric observe field with spectrophotometric standard star at same airmass as field to calibrate
  * GRB150309A (18h 28m 21.22s +86d 25' 47.6")