Subject: Re: Shared software development Hello Peter (and the rest of gang): You are right that more communication would be desirable. But something is actually happening behind the scene. At least I can comment on the projects in which I am involved: 1) Catalog update: I think you have all received information about the updated JEM-X source catalog "cat_combine_02.txt". When working on that I communicated a lot with Ken Ebisawa and Arash Bodaghee at ISDC. The catalog update was needed in connection with my light curve work. 2) Source detection. Only minor updates to midisky has happened since the introduction of the mask support structure in the detector illumination model. The main effort over the last months have actually happened in Valencia where Paul Connell have taken midisky and transformed it into an ISDC compatible version "JEMIROS". Just before Christmas Paul sent me back his first version of JEMIROS which I had hoped to update with the small changes I made since Paul started his work. Unfortunately, first family problems (my mother died on January 1st) and later troubles getting the light curve program to behave have kept me off JEMIROS until now. However, Jerome have installed Paul software here, so we are ready to go. Specifically on the mask support structure modelling: one of Stefans students, Cecilia Kozma, has been working in Stockholm with the subroutines I developed, so I believe they are now also part of Stefans source extraction software. 3) Mosaics. Right now I am in daily contact with Roland Walter on how to produce the best looking global mosaics showing the whole Galactic plane. Fortunately ,we have recently acquired a very fast multi CPU PC here running linux, and it can create images from all the 3000 "Survey" science windows in about 8 hours. We are now in the sixth such cycle of cleaning iterations. 4) Light curves. Stefan circulated in early December a description of his source extraction software. And for my part I have been working with a light curve program based on the midisky source illuminaton model for the last couple of months. In a mail later today shall report in more detail on the status of this software which is just now beginning to give results. Many of the contributions we have planned for the Munich workshop will depend on getting decent lightcurves and the time pressure to get something out is very high. Right now I am optimistic about producing acceptable light curves for weak sources, but for strong sources the vignetting errors are still quite noticeable. My main worry now is that for several of the most interesting projects much of the data are in restricted imaging format, which my program cannot handle today. with best regards niels