Dear colleagues, we have some good news for those who use MuniDOS (DOS/Windows part of CCD photometry package called MuniPack) for their reductions Maybe some of you know about the bug in FITS conversion, that too bright stars (brighter than Word/2 ~32000 counts) are converted to 0 intensity. We did today bug fix on this and right now we test it. This fault was also reason for troubles using flat-fields with intensity more than 32000 (often case). New conversion program wrote by Filip, tested under Linux and also compiled and tested for DOS is done. The update (in microsoft's term "service pack" :))) will be available at the web-site in a few days. It will be also a date when you would be able to download also Windows NT version of MuniDOS which will be available (just made some changes due to different DOS/Win95 and NT OS strategy). Right now I'm trying to prepare completely new WINDOWS distribution (advanced but also free of charge) with command-line based system of photometry (stability, stability,...) and mainly with more precise differential photometry methods. Probalby first statistical search for variables in long runs. [[[ It is based on the fact that the brightness of star have distribution seems like normal (not tested yet in fact) with mean value and uncertainyty sigma. Stars which brightness is changing during night (eclipses, humps,...) have very different sigma than stars with same brightness and constant brightness. The tendecny f(mean magnitude,sigma) is exponential (logarithmic) for magnitude distribution so if the distance from the fitted curve will be larger than normal scatter than it is possible that the star is variable. I made some preliminary test on this with known variable stars and I got quite good results. Of course, the algorithm should be more robust and everyone who would like to help me to build it is welcome. ]]] have a nice day and stay tuned. If you want to be informed about MuniPack updates, register. It's free and will bring you news. Right now we have couple of tenths of registered users :) Rudolf Novak N. Copernicus Observatory Brno CR