Differences between revisions 15 and 16

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
- RX J0953+1458 --> 09 53 08.1 +14 58 36 NL AM 17.3 P_orb=0.072049 days = 1.729176 hrs = 103.75056
  - 2min exposures in L-filter cover at least 2.25 orbits = 3.8-4.0 hrs
- HU Aqr (21 07 58.188 -05 17 40.47) L-filter high time resolution 10 - 20 sec
- Ritter & Kolb cataclysmic varible catalog
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)
Several variables in a field in Cygnus, best pointing direction: 20h 49m 56s +34d 20' 30" (RGB photometry)
V404 Cyg (x-ray binary - BH + G-type star)
OJ 287 (Blazar; Vmag ~ 13..16) integrate for a few minutes; cycle through all filters; at least one epoch per night
HD 164595 (RATAN-600 radio detection; Vmag ~ 7mag)

-  ⇤ ← Revision 15 as of 2015-11-21 04:56:12 → 
  Size: 1354
  Editor: TassiloSchweyer
  Comment:
+   ← Revision 16 as of 2016-08-27 20:58:57 → ⇥
  Size: 1432
  Editor: TassiloSchweyer
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
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+ * [[Targets/HD164595|HD 164595]] (RATAN-600 radio detection; Vmag ~ 7mag)