Collaborators : B. Cl ment (LAM), P. Hibon (KIAS) J.Willis (Univ. Victoria), C. ... as the change in the far-UV LF is much milder. Data for z=6.5 : ...
Gemini: Mathieu Bec, Celine d'Orgeville, ... CFHT, Gemini, Keck, Subaru, UH. URLs. How are they set at ... Gemini preliminary data. Data not automatically ...
MAMBO, CFHT, Bolocam and (future) others. COSMOS major components (in order of appearance) ... MAMBO, CFHT, TNG and others. November, 7 2006. CXC Extragalactic ...
compatible with a cosmological constant, WL~0.7. SNe: ... Produces calibrated star catalogs in the CFHTLS Deep fields, in natural Megacam magnitudes. ...
Christophe Alard (IAP), R mi Cabanac (CFHT), Bernard Fort (IAP) ... automated softwares. How to find them? Develop automated procedure to search the lenses ...
HST, Spitzer, VLA, GALEX, CFHT LS blah blah blah 'AEGIS' ApJL special issue (~20 ... AGN contribution to the total luminosity of the universe (c.f. stars) ...
La lunette de Galil e Objectif convergent Oculaire divergent Image droite Les premi res d couvertes de Galil e Quelques grandes lunettes T lescope de Newton ...
m me si les r sultats actuels marquants viennent plut t de la cosmologie (SNLS, ... les r percutions sur le fonctionnement actuel d'un CFH aujourd'hui tr s ...
My focus is on effects of photometric errors on photo-z measurement ... Not shown today, but z-band data, plus other fields, are also available for photo-z tests ...
Title: PowerPoint-Pr sentation Last modified by: Harald Kuntschner Document presentation format: Custom Company: Micaela Stumpf Other titles: Times New Roman HG ...
Title: SNe Ia and the effect of environment Author: Mark Sullivan Last modified by: Mark Sullivan Created Date: 2/20/2006 12:54:04 AM Document presentation format
Red galaxies are the ones with bulges. DEEP 1 galaxies with HST imaging (fits by L. Simard) ... brighter bulges. COMBO- 17 photometric survey. Large area, 17 ...
'Retooling' Data Centre Infrastructure to Support the ... e.g. adGet -a CGPS -s -op getData?cutout=[100:100,210:210,1:272,1:1] CGPS_MA2_HI_line -nocrc -o ...
Galactic archaeology. Rodrigo Ibata. Observatoire de Strasbourg. age in Gyr. mass fraction ... What was the role of accretion in the formation of the halo, disk, ...
Lyman Break Galaxies in Large Quasar Groups at z~1 G Williger (Louisville/JHU), R Clowes (Central Lancashire), L Campusano (U de Chile), L Haberzettl & J Lauroesch ...
AO Reveals Faint Companions to Bright Stars. Mike Brown (CalTech) Galactic Center ... Movie of the asteroid Kleopatra, observed during seven-hour period with ...
Gauss-Bonnet Lagrangian. Solution in static spherical. symmetry in a linearized. PPN metric with ... coupled Gauss-Bonnet. see L. A., C. Charmousis, S. Davis ...
Colloque ... Large-scale structure induces correlations between the observed shapes of ... Quintessence study underway , aiming to. constrain, for example, ...
Aggregating Metadata from Multiple Archives: a Non-VO Approach CADC Stephen Gwyn Canadian Astronomy Data Centre Stephen Gwyn Canadian Astronomy Data Centre
towards joint operation of VTT, Themis, DOT, SST ( Gregor eventually EST) ... THEMIS. 1.52m Telescope. Telescopio Carlos Sancez. 2m Telescope. Telescope ...
GALAXY EVOLUTION OPTICAL AND IR SURVEYS Lucia Pozzetti INAF Osservatorio Astronomico di Bologna PEOPLE INVOLVED IN BOLOGNA INAF-OAB: Bardelli, Cappi, Ciliegi ...
WP 6200.1 - Partecipazione alla Definizione dei KP in GT WP 6200.2 Partecipazione alla Preparazione dei KP in GT WP 6200.3 Sviluppo di algoritmi di riduzione ...
L1: The Cosmic Microwave Background & the Thermal History of the Universe. Dick Bond ... Non april fool. Is the universe like a soccer ball? The CMB data decides: ...
Accretion Channeling in CTTS. Scott Gregory, Moira Jardine. Classical T ... (e.g. Guenther et al. 1999). Electron-cyclotron maser emission (Smith et al. 2003) ...
PEGASE2 is used to fit SED templates to the optical data. ... No evidence for gross differences between light-curves in passive and active galaxies ...
... C-O WD systems (Nomoto et al astro-ph/9907386) WD red giant ... WD MS in common envelope. AGB with C O core. RG He core. Significant time delay ...
For a given quintessence potential V(f), we set the 'initial conditions' at z=0 ... Approximating Quintessence for Phenomenology Friedmann Equations DM B. 1 ...
43% of the galaxies show interaction signs. 32% of the groups ... Generated by stripped material from the galaxies. Material dispersed on the group potential ...
Broad-band filters: Y, J, H, Ks. Narrow band filters: Low OH-1 Low OH-2, CH4 On, CH4 Off, H2, K continuum. ... The H band is notoriously variable by /-0.5 mag. ...
Forms multiple images of the telescope pupil which are imaged through the grism spectrograph. ... A simple fibre re-formatter from sky to spectrograph slit ...
A universal force in 4D mediated by a massless tensor field. What is ... coupled Gauss-Bonnet. see L. A., C. Charmousis, S. Davis 2006. Boisseau et al. 2000 ...
MERCURY OBSERVATIONS -- JUNE 2006 DATA REVIEW MEETING -- 20-21 November 2006 ... 19:00: Group Dinner at The Castle at Boston University, 225 Bay State Road ...
LCROSS Video. 4. Wireless Access ... on the experience of Deep Impact ... Satellite (LCROSS) lunar swingby calibration and LCROSS impact, and support of ...