Dear all, > About the recent discussion on overobservations for mira > stars, I agree with the notion of not making estimates every night. > It's no use because of the long periods= the star is not going to vary in > just one day. The star is going to stay the same and maybe observational > error on our part will ruin a pretty nice lightcurve filling it with noise > that could have been avoided if we were patient enough to wait for the star > to actually vary. I'm of an just opposite opininon. Lets assume model Mira variable with period 300 days and amplitude 6 mag - star will change with rate 0.04 mag/day (assuming sinusoidal variation - lightcurve of Miras is similar), which can single observer catch (of cource, only if magnitudes are not rounded on tenths). And sometimes, the star varies quicker: in August I caught ascending branch of R UMi. This semiregular variable changed about 1 mag in eleven days! Rate 0.1 mag per day can be easily observed with eyes. Concerning the noise in lightcurve I have another example: during August the semiregular variable AY Dra has faded by 1,5 mag. I covered this variation with 17 estimates: 3 estimates deviates from mean lightcurve by 0,3 mag. What should I think if I instead of 17 estimates made only 6 (one est. in 5 days) and 3 of them were wrong? Thus, I think that large number of points in lightcurve can do very good job in filtering deviating estimates. And if lightcurve has stabile noise, some averaging might help. Best regards, Ondrej Pejcha