head 1.1; access; symbols; locks http:1.1; strict; comment @# @; expand @b@; 1.1 date 2004.01.28.13.17.52; author TimoPrusti; state Exp; branches; next ; desc @none @ 1.1 log @Overheads from 28 Jan 2004 @ text @ࡱ>   !"#$%&'()*+,-./0Root EntrydO) GPowerPoint Document(HSummaryInformation( DocumentSummaryInformation83D ( / 0LDTimes New Roman詼t\ )0tY 0 ` .  @@n?" dd@@  @@@@`` X$  c $@@7uʚ;2Nʚ;g4@@d@@d )0hppp@@ <4!d!d 0$Ԫ<4dddd 0$Ԫ Stars, ISM and Solar System No SSOs Some simple image processing needed (subtraction e.g. for variable or moving objects or narrow band imaging) Data validation (outliers, cross-calibration) Proposal writing Science case Stars, ISM and Solar System Error propagation (e.g. J and H photometry has errors, when J-H is calculated, then J-H error is done as well automatically) Cloudy and dusty mentioned as examples of modeling tools which could be accessed through VO to compare with data  Science cases  Several identified Approach is to download demo version, start working and to estimate Additional tools needed Need to polish existing VO tools The availability of astronomer effort in time scales compatible with VO development&WWW  Projects Continuation of demo cases (Richards and Cambresy) AGB to PN transition (Garcia-Lario et al.) Discovery of new candidates Examination of spectra for classification Stellar variability (Ortiz) Contains an idea of temporal data examination which may also be applicable to SED analysisT^ZFZZ[Z^F[H)      Projects Luminosity functions of star forming regions (Prusti) Demo has already most of the tools Companions to PN central stars (Kerber et al,) Demo has already most of the tools Negative result would also have value `6#/I6#/I@@.   CR ` ` ̙33` 333MMM` ff3333f` f` f` 3>?" dd@@,|?" dd@@   " @@ ` n?" dd@@   @@@@``PR    @@ ` ` p>> f(    6ݼ P  T Click to edit Master title style! !  0`   RClick to edit Master text styles Second level Third level Fourth level Fifth level!     S  0 ``  >*  0 `   @@*  0< `   @@*H  0޽h ? ̙33 Default Design  P$(  r  S @@hP  h r  S h h H  0޽h ? ̙33  `$(  r  S \P  \ r  S i\ \ H  0޽h ? ̙33  p$(  r  S ~\P  \ r  S hh h H  0޽h ? ̙33   $(   r  S \P  \ r  S q\ \ H  0޽h ? ̙33  $$(  $r $ S \P  \ r $ S \ \ H $ 0޽h ? ̙33r$  PxdP , ( / 0LDTimes New Roman詼t\ )0tY 0 ` .  @@n?" dd@@  @@@@``   !"#$%&'()*+,-./012456789:;=Oh+'0 `h  PowerPoint Presentation Timo Prustitprusti8ruMicrosoft PowerPointon@@p@@s@@` GG~ g  E& &&#TNPP(2OMi & TNPP &&TNPP    --- !---&G&j}w@@ QwZw0- &Gy& --y@@H-- @@Times New RomanQwZw0- .02 Stars, ISM and Solar System!!4!!/.--yH-- @@Times New RomanQwZw0- . 2 R. .$2 vStars,some ISM, no     &  . . 2 SSOs. . 2 ;R. .=2 ;v$Some simple image processing needed !        . .E2 ov)(subtraction e.g. for variable or moving             . .62 vobjects or narrow band imaging)       . . 2 R. .72 v Data validation (outliers, cross       . . 2 -. .2  calibration)  . . 2 R. .2 vProposal writing  . . 2 ZR. .2 Zv Science case    .--"System 0-&TNPP &՜.+,0    On-screen ShowcESAH  Times New RomanDefault DesignStars, ISM and Solar SystemStars, ISM and Solar SystemScience cases Projects Projects Projects  Fonts UsedDesign Template Slide Titles_HtprustitprustiCurrent User<5X$  c $@@7uʚ;2Nʚ;g4@@d@@d )0hppp@@ <4!d!d 0$Ԫ<4dddd 0$Ԫ ? %Stars, ISM and Solar System Stars,some ISM, no SSOs Some simple image processing needed (subtraction e.g. for variable or moving objects or narrow band imaging) Data validation (outliers, cross-calibration) Proposal writing Science case Stars, ISM and Solar System Error propagation (e.g. J and H photometry has errors, when J-H is calculated, then J-H error is done as well automatically) Cloudy and dusty mentioned as examples of modeling tools which could be accessed through VO to compare with data  Science cases  Several identified Approach is to download demo version, start working and to estimate Additional tools needed Need to polish existing VO tools The availability of astronomer effort in time scales compatible with VO development&WWW  Projects Continuation of demo cases (Richards and Cambresy) AGB to PN transition (Garcia-Lario et al.) Discovery of new candidates Examination of spectra for classification Stellar variability (Ortiz) Contains an idea of temporal data examination which may also be applicable to SED analysisT^ZFZZ[Z^F[H)      Projects Luminosity functions of star forming regions (Prusti) Demo has already most of the tools Companions to PN central stars (Kerber et al,) Demo has already most of the tools Negative result would also have value `6#/I6#/I@@.   CR  P$(  r  S @@hP  h r  S h h H  0޽h ? ̙33r*|, , ( / 0LDTimes New Roman詼t\ )0tY 0 ` .  @@n?" dd@@  @@@@`` X$  c $@@7uʚ;2Nʚ;g4@@d@@d )0hppp@@ <4!d!d 0$Ԫ<4dddd 0$Ԫ ? %Stars, ISM and Solar System Stars,some ISM, no SSOs Some simple image processing needed (subtraction e.g. for variable or moving objects or narrow band imaging) Data validation (outliers, cross-calibration) Proposal writing Science case Stars, ISM and Solar System Error propagation (e.g. J and H photometry has errors, when J-H is calculated, then J-H error is done as well automatically) Cloudy and dusty mentioned as examples of modeling tools which could be accessed through VO to compare with data  Science cases  Several identified Approach is to download demo version, start working and to estimate Additional tools needed Need to polish existing VO tools The availability of astronomer effort in time scales compatible with VO development&WWW  Projects Continuation of demo cases (Richards and Cambresy) AGB to PN transition (Garcia-Lario et al.) Discovery of new candidates Examination of spectra for classification Stellar variability (Ortiz) Contains an idea of temporal data examination which may also be applicable to SED analysisT^ZFZZ[Z^F[H)      Projects Luminosity functions of star forming regions (Prusti) Demo has already most of the tools Companions to PN central stars (Kerber et al,) Demo has already most of the tools Negative result would also have value `6#/I6#/I@@.   CRr,,09 D ( / 0LDTimes New Roman詼t\ )0tY 0 ` .  @@n?" dd@@  @@@@`` `(   c $@@7uʚ;2Nʚ;g4@@d@@d )0hppp@@ <4!d!d 0$Ԫ<4dddd 0$Ԫ ? % Stars, ISM and Solar System Stars,some ISM, no SSOs Some simple image processing needed (subtraction e.g. for variable or moving objects or narrow band imaging) Data validation (outliers, cross-calibration) Proposal writing Science case Stars, ISM and Solar System Error propagation (e.g. J and H photometry has errors, when J-H is calculated, then J-H error is done as well automatically) Cloudy and dusty mentioned as examples of modeling tools which could be accessed through VO to compare with data  Science cases  Several identified Approach is to download demo version, start working and to estimate Additional tools needed Need to polish existing VO tools The availability of astronomer effort in time scales compatible with VO development&WWW  Projects Continuation of demo cases (Richards and Cambresy) AGB to PN transition (Garcia-Lario et al.) Discovery of new candidates Examination of spectra for classification Stellar variability (Ortiz) Contains an idea of temporal data examination which may also be applicable to SED analysisT^ZFZZ[Z^F[H)      Projects Luminosity functions of star forming regions (Prusti) Demo has already most of the tools Companions to PN central stars (Kerber et al,) Demo has already most of the tools Negative result would also have value `6#/I6#/I@@.   CR Projects ^Abundance gradients from PN and HII regions (Walton) Link to modelling tools Image subtraction&5*5*5 *  ($(  (r ( S .\P  \ r ( S \ \ H ( 0޽h ? ̙33rd9 F@@9H @