NEWS
RSS feed
Comments
YouTube channel
Facebook
OBSERVING CAMPAIGNS NEW
Expired Campaigns
OBSERVING PROJECTS
B.R.N.O. - eclipsing binaries
MEDUZA - intrinsic variables
TRESCA - exoplanets
HERO - high energy objects
OBSERVERS LOG
User-defined objects
ABOUT US
Leadership
Actions
Perseus Bulletin
J. Silhan price "The Observer of the year"
Membership conditions
List of members
DATABASES & TOOLS
General Search Gateway
Open European Journal on Variable stars
O-C Gateway
CzeV Catalogue
SvkV Catalogue
RafV Catalogue
MEDUZA light curves & data
Known eclipsing binaries
Data statistics
Exoplanet Transit Database
CAS - Czech Astronomical Society
> Light curve and airmass <
> Global light curve (MOOZ) <
> Close vicinity of the variable <
> Show source data <
> B A C K > All observations:
> Add comment for object or page ...
No records
RSS feed
Comments
Facebook
OBSERVERS LOG
> Add comment for object or page ...
Comment
object EQ UMa
Primary minimum for 2017-03-16 occurs about 2 hours later than predicted (for elements 48706.7253+0.3581435*E.
2014-04-06.Sekundární minimum nastalo o 1h 10 min později oproti předpovědi pro orbitální elementy 51422.719+0.360224*E
2014-04-06.Sekundární minimum nastalo o 1h 10 min později oproti předpovědi pro orbitální elementy 51422.719+0.360224*E
page
No records