AVO Science Telecon: Oct. 8, 03 present: MA Mark Allen TB Thomas Boch LC Laurent Cambresy PF Pepi Fabbiano FG Francoise Genova PP Paolo Padovani TP Timo Prusti AR Anita Richards chair: NW Nicholas Walton minutes: MD Markus Dolensky, revised by PP excused: DD Dave DeYoung PR Piero Rosati action items: [LC+AR+TP] write down ideas for a galactic case [PP+PR] write down ideas for extragalactic case [MD] prepare wiki page for SWG [PP] contact SWG and point them to the wiki page [ALL] next telecon: Oct 23, 2003, 4pm CET notes: NW reported on an email received from DD, who suggested to integrate the extragalactic case with numerical simulations and to stress for the Galactic one nulti-band IR data. 1.) galactic case PP: very little data for SIRTF in January, main release in Spring 2004 PF: the Galaxy Structure and Evolution SWG sub-group had indicated the importance of a tool for registering and mosaicing images; MONTAGE (IRSA) might do that, but not clear when available MA/MD: "bring in your own data to the VO" should be addressed by the demo, as users appear to be very interested in this AR: spectral energy distribution; compact objects TP: Is there a group doing it (combining spectra in multiple bands) already that could set requirements? Right now we approach from technical point of view, not from an existing scientific research project. PP: galactic case ISO/XMM star forming region: ISO spectra (SWS, LWS) + XMM data strong interest from ISO and XMM to work on overlapping fields; will discuss this in Strasbourg Consensus that Galactic case still weak; LC & AR will work on a draft on a short time-scale, TP will help as well. MD will then upload it to the Wiki. 2.) extra galactic case PP: GOODS field: FORS2 spectra available for a few hundred sources, XMM spectra available; one idea could be to look for type II AGN, for which one needs the X-ray spectrum to see the hard, absorbed component and the optical spectrum, which should show only narrow lines; nobody in the GOODS/AGN team (PP is a member) currently working on this. Discussion on cross-correlation tools to match sources from different catalogs; there are tools available (e.g. W3Browse (http://heasarc.gsfc.nasa.gov/db-perl/W3Browse/w3browse.pl) but require expert users. NW: suggests to create postage stamps of a list of sources, extracting cut-outs from available images Consensus that extragalactic case is stronger; PP will write a short draft and get PR's input. MD will then upload it to the Wiki. Once both drafts are there, PP will contact SWG members to point them to the Wiki and ask for comments/input. 3.) tools MD: brief discussion on SpecView, which can handle HST and FORS2 spectra, plus any ASCII file; Spexter is more a pipeline than a display tool Discussion will continue next week in Strasbourg.