Hello all, You can pick up the whole thing in ftp://ftp.astro.princeton.edu/strauss/LSST/DRM.(ps,pdf) You can also find the source (LaTeX files and postscript figures) in ftp://ftp.astro.princeton.edu/strauss/LSST/DRM/source I consider this essentially done. Lots of small changes from all of your many comments. The following are the substantive changes since the version I posted two weeks ago: Abstract: Note the modified last few sentences. Intro: End of intro has been rewritten, and now has a forward reference to Chapter 12 ("What lies ahead") where the comparison of surveys is now discussed. Gravitational Lensing (Section 7): Tony is planning to get me cleaner versions of Figures 11 and 12 (actually, as I write this, the new version of Fig 11 arrived; thanks, Tony!). You will notice a number of wording changes through 7.4 and 7.5; Tony and Gary, in particular, should see whether my interpretation of their discussion is correct. Supernovae (Section 8): Chris Smith promises a new draft of the first paragraph of Section 8.1.1. I added further caveats there about possible systematics. There is some modified text at the end of 8.1.2. Gary pointed out some inconsistencies between the text and figures at the end of 8.3 on parameter estimation; I think I straightened that out now. The Appendix on data distribution has now been moved up as Chapter 11, as we discussed yesterday. Chapter 12 ("What lies ahead") has been expanded in a number of places, as we discussed. Based on comments from John Tonry, I've strengthened the statements (under 'observatory location') about the need for good seeing. I've added a discussion of the desirability to have common filter systems between different telescopes. And there is a new subsection about comparison between facilities (the first draft of which you saw as the end to the introduction, which I sent around last night). The text now simply states that the definition of figures of merit is an involved one, and we'll tackle this down the road; the table now simply has various characteristics of the different programs. Three newly added ones are exposure times, etendue (yes, I suppose this is a FOM, but one used throughout the text), and program duration. As before, please, everyone check for correctness! 8.4m LSST (Appendix B) adds a 'note in proof' describing the increase in field of view from 3 to 3.5 degrees, together with a figure showing the image quality as a function of radius. And that's about it! I plan to send a formal note to Jeremy Mould and Sidney Wolff first thing Monday morning saying we're all done; please send any (hopefully minor) corrections before then! Thanks, Michael LSST LSST LSST LSST LSST Mailing List Server LSST LSST LSST LSST LSST LSST LSST LSST This is message 237 in the lsst-general archive, URL LSST http://www.astro.princeton.edu/~dss/LSST/lsst-general/msg.237.html LSST http://www.astro.princeton.edu/cgi-bin/LSSTmailinglists.pl/show_subscription?list=lsst-general LSST The index is at http://www.astro.princeton.edu/~dss/LSST/lsst-general/INDEX.html LSST To join/leave the list, send mail to lsst-request@astro.princeton.edu LSST To post a message, mail it to lsst-general@astro.princeton.edu LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST LSST