Japanese "Variable Stars" 1997 Vol. 28 No.1 has been recently published by "Nihon Henkousei Kenkyuukai" (Reserch Group for Variable Stars in Japan?). Titles from this monthly-to-bimonthly issue (text in Japanese). * From the recent observations (Y. Maehara): visual observations of little observed or poorly studied eclipsing binaries. ZZ Aur, V523 Cas, V432 Per, AM Tau * Report on the "Variable Star Festival", Nagano division (M. Momose) Unfortunate clouds with some breaks. The target star X Tri was not observed. Demonstration of CCD observation. * February stars (M. Watanabe) Recommended Mira stars, RV Tau stars, bright CVs * Prediction of Mira-type maxima dates for 1997 (M. Watanabe) * Inivitation to the Februrary "Variable Star Party" (Sorry again for my very _iikagen_ English summary > Watanabe-san) By the way, present Japanese eclipsing binary observers often use what is called "Krakow's table" (SAC) or GCVS 4 for predicting minima times -- prediction sometimes too unreliable. Does anyone know other up-to-date and comprehensive eclipsing binary ephemeris table? Regards, Taichi Kato