Figure: The variations of RR Lyrea over the Blazhko cycle in 2004. Note that the spread in magnitudes for individual images is caused by the fact that we superimposed light curved within a Blazhko phase bin of 0.1 (almost 4 days).
Through this page data gathered in the framework of the Blazhko project can be downloaded.
For now, we present the photometric PMT data (differential magnitude) in the Johnson B and V filters for 6 southern Blazhko stars. The B and V data are in separate files. The data were gathered by Elisabeth Guggenberger, Patrick Lenz, Lucas Schmitzberger, Paul Beck, Thebe Medupe and his students, and Katrien Kolenberg. The used comparison stars are the C1 stars published in Kolenberg, Guggenberger & Medupe (2008), CoAst 153, 67. Details on the data set of SS For are published in Kolenberg, Guggenberger, edupe et al. (2008), submitted to MNRAS.
(KK, October 30, 2008)
Stay tuned for more data.