Differences between revisions 4 and 5

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")
GSC 2135 420 (11.09 mag): 19h09m42.98s +29 09' 07.1" DSCT star with very short period (0.0800568 d) and with long term trend
- in amplitude, sequence of short (< 60 s) exposures with 'suitable' filter(s)

-  ⇤ ← Revision 4 as of 2015-03-12 13:43:21 → 
  Size: 542
  Editor: TassiloSchweyer
  Comment:
+   ← Revision 5 as of 2015-03-17 14:28:04 → ⇥
  Size: 754
  Editor: KonradDennerl
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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+ * GSC 2135 420 (11.09 mag): 19h09m42.98s  +29 09' 07.1"  DSCT star with very short period (0.0800568 d) and with long term trend
   in amplitude, sequence of short (< 60 s) exposures with 'suitable' filter(s)