Abstract. The long-term behaviours of the pulsation and Blazhko periods of RR Lyr are investigated by means of Kepler and ground-based observations. The difficulties in detecting additional modes in the Cepheids monitored with CoRoT are discussed.
RR LyrRR Lyr≡KIC7198959 was included in the field-of-view of the Kepler space telescope [2] and highprecision, continuous observations could be secured. Well before the launch of Kepler, we decided to devise small, autonomous, and transportable photometric instruments to make the ground-based survey of the modulations in amplitude and phase (Blazhko effect) of RR Lyr as effective as possible. The instruments are composed of a commercial equatorial mount (Sky-Watcher HEQ5 Pro Goto), an AUDINE CCD camera (512x768 kaf400 chip) and a photographic 135-mm focal, f/2.8 lens with a field of view of 2 • x3 • (Fig. 1). We gave them the nickname VTTs for "Very Tiny Telescopes".The GEOS (Groupe Européen d'Observations Stellaires) RR Lyr database [5] is continuously updated by inserting all the published maxima of RR Lyr variables. RR Lyr itself is among them 1 . Therefore, we could analyse [6] all the observed maxima since 1899 in order to have a clear picture of the behaviours of the pulsation period P 0 and of the Blazhko effect, noticed since 1916. We could identify two states defined as pulsation over a "long" primary period (P 0 >0.56684 d) and over a "short" one (P 0 <0.56682 d). These states alternate with intervals of 13-16 yr, and are well defined since 1943. We also provided homogeneous determinations of the Blazhko period P B in several time intervals and we studied how it changed while the two states alternated. We could clearly establish how the Blazhko period had just one sudden decrease from 40.8 d to 39.0 d in 1975. The variations of the pulsation and Blazhko periods are completely decoupled (Fig. 2).Moreover, the combination of Kepler and VTT data recorded the vanishing of the Blazhko effect. The space telescope continuously monitored the monotonic long-term decrease, proving that smallscale modulations, lasting from 2 to 4 P B , are also visible in the O-C (observed minus calculated times of maximum brightness) values. The VTT data are now securing the RR Lyr monitoring after that Kepler had to be pointed in another direction. In particular, Fig. 2 Article available at