AFOEV - Light curves

The light curves are plotted after our data. Their formatting is due to François Ochsenbein (CDS - Strasbourg Observatory) whom we thank for his kind help.
Click on the abbreviated name of the constellation then on the Argelander name of the star.

The light curve displayed for each star is based on the data collected during the last 12 months or the last 5 years or the curve using the whole dataset. Visual observations are plotted in green, mpg, pep(B) and CCD(B) observations in blue, pep(R) or CCD(R) measurements in red and I measurements in black. At the bottom of the page, a panel allows zooming on a selected part of the curve. To that effect, input the date and end of the interval (for instance 50000 and 51000) in the "x cuts" boxes. The amplitude can be reduced by inputting your choice of values for the magnitudes. Lastly, click on "Adapt Plot".

The home page of each variable allows access to the information contained in the Simbad and VizieR databases. Since the update of the tool, the link to Aladin is dead.

Simbad supplies basic information on the star, its names in different catalogues as well as bibliographical references.

VizieR reproduces data from the General Catalogue of Variable Stars (GCVS).


Constellations   :

And
Ant
Aps
Aqr
Aql
Ara
Ari
Aur
Boo
Cae
Cam
Cnc
CVn
CMa
CMi
Cap
Car
Cas
Cen
Cep
Cet
Cir
Col
Com
CrB
Crv
Crt
Cru
Cyg
Del
Dor
Dra
Equ
Eri
For
Gem
Gru
Her
Hor
Hya
Hyi
Ind
Lac
Leo
LMi
Lep
Lib
Lyn
Lyr
Mic
Mon
Mus
Oph
Ori
Pav
Peg
Per
Phe
Pic
PsA
Psc
Pup
Pyx
Ret
Sge
Sgr
Sco
Scl
Sct
Ser
Sex
Tau
Tel
Tri
TrA
UMa
UMi
Vel
Vir
Vul
  
NSV stars
SN (supernovae)
  
Misc (divers)


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