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The new space telescope Kepler and its asteroseismological targets . We present primary and secondary asteroseismological targets for Kepler,the new NASA space mission. We derive log  T_eff and logL/Lȯ values for the selected stars and we put the starsin the log  L/Lȯ - log  T_eff diagram. Then, we presentour program of ground-based spectroscopic and photometric observationsof the selected targets and we show first results obtained from theseobservations.
 
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Observation and Astrometry data
| Constellation: | Cygnus |  
    | Right ascension: | 19h14m44.98s |  
    | Declination: | +51°08'42.3" |  
    | Apparent magnitude: | 9.272 |  
    
    
    | Proper motion RA: | -20.7 |  
    | Proper motion Dec: | -2.8 |  
    | B-T magnitude: | 9.993 |  
    | V-T magnitude: | 9.332 |  
    
 
 
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