head 1.1; access; symbols; locks http:1.1; strict; comment @# @; expand @b@; 1.1 date 2004.06.12.19.15.46; author MarkusDolensky; state Exp; branches; next ; desc @none @ 1.1 log @cosmology group summary by Leibundgut @ text @ࡱ> mdlI( ./ 0DTimes New Roman0:A 0DArialNew Roman0:A 0 DWingdingsRoman0:A 0 B).  @@n?" dd@@  @@@@`` H(\   )"                 L%  $    .,B ii' 33 + + i9          ! %            '+          6<6J  #0 3 ++2#    <  -./0123456789; 0e0e     A@@  A5% 8c8c     ?1 d0u0@@Ty2 NP'p<'pA)BCD|E||s " 0e@@        @@ABC DEEFGHIJK5%LMNOPQRSTUWYZ[ \]^_ `abN E5%  N E5%  N F   5%    !"?N@@ABC DEFFGHIJK5%LMNOPQRSTUWYZ[ \]^_ `ab fPPff3f@@AN ʚ;Tu8ʚ;g42d2d :A 0ppp <4!d!dL$ 0s<4ddddL$ 0s <4!d!dL # 00___PPT10 pp~___PPT9`X@@? %+9AVO SWG: cosmology f  I Possible SRMs&    Fcosmic shear (to measure w) build-up of black holes high-z QSOs galaxy clusters M, dark matter, LSS, power spectrum, SZ, correlation with CMB (ISW) detection through multi-spectral comparisons morphology-density relation look for rare objects SEDs, search multi-dimensional parameter space4 /4 &.&&/&r;   D I   + JPossible SRMs (cont.)&     llook for objects with parameters not fitting the known SEDs, search multi-dimensional parameter space build-up of stellar mass with cosmic time multi-wavelength, multiple surveys, modelling chemical evolution over cosmic time star light, QSO absorption correlation of CMB, radio and optical/NIR galaxy surveys DM-haloes galaxy-galaxy lensing epoch of re-ionisation7P/P*P.P$PPCPPP7&/&*.$C      r7  *      KComing datasets  APEX, ALMA (Southern), SCUBA-2 AMI, AMOEBA, etc. LOFAR (Northern) Pan-Stars (2008/9), LSST (2011), JDEM/SNAP Astro-F (IR survey) UKIDSS, VISTA/VST Herschel Planck SWIFT GLAST eMerlin, eVLAZ~  =  !      LOngoing surveys  SDSS, 2MASS, Combo-17(+4), HDFs, UDF, CDF-S 2dF, 6dF XMM, Chandra XMM-LSS, XMM serendipitous sky survey CFHT-LS Spitzer SWIRE, GOODS COSMOS, GEMS GALEX 22 GHz (ATCA) WMAP, COBE FIRST, NVSS, SUMSS, WENSSBZ&ZZ ZFZB& FV     4 b  MExisting (imaging) archive  Radio NRAO, Merlin, E-VLBI, ATCA, JCMT, UMRAO IR Spitzer, ISO, IRAS Optical ESO, UK-ADC, CFHT, NOAO, Gemini, AAT, HST, WFI-Astrowise UV Galex, IUE everything MASTZ(ZZZZ9ZZ Z ZZ(9     L{       N Weak shear   dcosmological parameters (especially  and w) determine LSS need large area photometric redshifts image quality COSMOS, CFHT-LS, JDEM/SNAP Yannick Mellier knows all about this & <5B$$,$$$'$      f$ = )     OBuild-up of black holes  ^census of black holes as a function of z QSO 1 and QSO 2 (Padovani) correlating radio, X-ray and optical/NIR point sources need field of view GOODS only good for z>3 photometric redshifts SED  identifications high-z QSOs (McMahon) sky area, Lyman-break ( SED ) XMM serendipitous survey and FIRST/SUMSS)KFF,FG" P)K,       G@@:    R PGalaxy clusters  M, 8, dark matter, LSS, power spectrum, SZ, correlation with CMB (ISW) (Maccacaro, Hopp, Cimatti, Voges, Rosati) detection through multi-spectral comparisons red sequence in optical/NIR diffuse X-rays galaxy clustering SZ signal lensing signal (add spectral search) Large-scale galaxy evolution (Valentijn) morphology-density relation sites of morphological transitions automatic morphological classification statistics: identification of LSS and outside s-PlF)Pf<.F$,$,C$&'&&-$l$$ $$ $  E            t  <    Q6Rare or unknown objects (Leahy, Valentijn, Leibundgut)P7$&&&2       search multi-dimensional parameter space time-variability SEDs,  two-colour diagrams beware of false-positives (uncertainties!)2)X)$X$2)   C R)Build-up of stellar mass with cosmic time** * SEDs (Cimatti) optical, NIR (UKIDSS/VISTA), infrared (Spitzer-SWIRE/GOODS) fitting to population synthesis models (e.g. GISSEL) Gas masses (?) HI DLAs and IGMqPFq N       S#Chemical evolution over cosmic time$$ $ ostar light (Cimatti, De Young) massive spectroscopy surveys (e.g. VIMOS, GALEX, SDSS, 2dF, CIRPASS, FMOS, KMOS)FQ Q&   ] TUCorrelation of CMB, radio/mm and optical/NIR galaxy surveys (Banday, Leahy, da Costa)JV<(@@=      ^ all sky surveys Sunyaev-Zeldovich clusters (AMI, AMOEBA, Planck) integrated Sachs-Wolfe effect (WMAP, Planck) gravitational lensing of CMB polarisation (BICEP, CLOVER, etc.)@@  [  + UDark matter haloes(  galaxy-galaxy lensing (Quinn) deep imaging surveys (SDSS, VST, GEMS, COSMOS) stacking of galaxy images and measuring galaxy shapes (similar to weak shear Mellier) (galaxy case?  tidal streams, dwarf companions/satellites, background galaxies)|RL    R  VEpoch of re-ionisation(  cross-correlate HI holes (LOFAR) with Lyman-break objects (Valentijn, Cimatti, Hopp) redshift known from LOFAR observations find high-z quasars (McMahon) see build-up of black holes V'<'  Z<       e  ` ` ̙33` 333MMM` ff3333f` f` f` 3>?" dd@@,|?" dd@@   " @@ ` n?" dd@@   @@@@``PR    @@ ` ` p>> f(    6Ƙ P  T Click to edit Master title style! !  0ɘ   RClick to edit Master text styles Second level Third level Fourth level Fifth level!     S  0Ϙ ``  >*  0Ԙ `   @@*  0T٘ `   @@*B  s *޽h ? ff3333f Default Design 0  *(     0O P   O X*   0܈O    O Z* d  c $ ?  O  0O  @@ O RClick to edit Master text styles Second level Third level Fourth level Fifth level!     S  6`O `P  O X*   6`O `  O Z* H  0޽h ? ̙3380___PPT10.? 8(    0TO P   O >*   0O    O @@*   6HO `P  O >*   6O `  O @@* H  0޽h ? ̙3380___PPT10.H?M   t l 0$ (  $r $ S 0    $ BP ?"oU 8 Geometry, LSS and early universe: Angular and luminosity distances: SNIa, cosmic shear, CMB power spectrum: amplitude, spectral index, running spectral index, growth rate: clustering of galaxies (z survey), cosmic shear topology: CMB anisotropy Extragalactic medium and history of building blocks: re-ionisation: survey of high-z QSOs , CMB LSS and super clusters of galaxies: M/L; early vs ate type contribution to mass and light, biasing linearity, stochasticity Clusters of galaxies: coupling X-ray,SZ, WL, redshifts: number density as function of redshift, mass function, mass profile Star formation and chemical history Morphological type formation history Fundamental physics: Large scale gravity: weak lensing Time variation of fundamental constant: QSOs Dark energy (topic 1): SNIa, cosmic shear, CMBX#1 1 71 q1 1 1 #f t 5f "[if7f      &        F    7  =   #    *     : $ H ?"6@@ NNN?N Mellier Jan  04 f   H $ 0޽h ? ff3333fy___PPT10Y+D=' = @@B +  dJ(  d d  6Hr"`  r d S sP   H d 0޽h ? ff3333f___PPT10i.N_+D=' = @@B + -K0 h$(  hr h S P   r h S P  H h 0޽h ? ff3333f___PPT10i.Np/X+D=' = @@B +< -K0 l$(  lr l S pP   r l S D  H l 0޽h ? ff3333f80___PPT10.N65< -K0 p$(  pr p S ,{P   r p S SNIa.-@@Arial-. $2 vH, cosmic shear, CMB1.-@@Times New Roman-. f2 vMellier.-@@Times New Roman-. f2 vJan 04.-՜.+,0    =On-screen ShowyanoffeNJ{ Times New RomanArial WingdingsDefault DesignAVO SWG: cosmologyPossible SRMsPossible SRMs (cont.)Coming datasetsOngoing surveysExisting (imaging) archive Weak shearBuild-up of black holesGalaxy clusters7Rare or unknown objects (Leahy, Valentijn, Leibundgut)*Build-up of stellar mass with cosmic time$Chemical evolution over cosmic timeVCorrelation of CMB, radio/mm and optical/NIR galaxy surveys (Banday, Leahy, da Costa)Dark matter haloesEpoch of re-ionisation  Fonts UsedDesign Template Slide Titles'_㣊Markus Dolensky  !"#$%&'()*+,-./0123456789:;<=>?@@ABCDEGHIJKLMNOPQRSTUVWXYZ[]^_`abcnRoot EntrydO)1'Oe@@Current User/SummaryInformation(F*PowerPoint Document(NJDocumentSummaryInformation8\@