WASP 13b exoplanet transit (Feb. 22,2012)


HAT P10 / WASP 11b exoplanet transit (Sept. 30,2011)

V 368 Sge summer 2011 campaign, concluded

MMARCH
2011
Started GM UMa observing campaign
I’ll try to
determinate some TOM of GM Uma, a shortly followed eclipsing variable star
First
photometric run made on March 23, 2011 (duration about 2 hours), very difficult
observing conditions with bad seeing
A TOM
was expected at 19:59 UT
An
elaboration (little forced for great points dispersion for seeing) with Kwee
and van Woerden alghorithm shows the
minimum
possible at about the same hour (only 0.1 mag magnitude down)
corresponding
to HJD = 2455644.335768

(great
dispersion for terrible seeing!)
Used a B-Block
Custom Scientific filter
Parabolic fit of points, elaboration by KW alghoritm and O-C position
of my observation (blue point) in O-C gateway ( only one observation between
1991-today !)
I NEED TO OBSERVE MUCH MORE TOM!, THE FIRST IN
UNCERTAIN !
HERE WE GO!

(L. Kohoutek - R. Wehmeyer)