Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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• First fringes in the H band with 3 telescopes of IOTA by means of an integrated optics beam combiner (Monnier et al. 2004, Kraus et al. 2005) • Nulling of 10 −4 achieved on the ALCATEL Space MAII bench by using an integrated optics beam combiner developed under ESA contract. • First formal demonstration of single mode guiding at 10 µm in the IODA project (Labadie et al. 2005) • Creation and development of the Centre Jean-Marie Mariotti (JMMC) with partners. Consecutive creation of the European interferometry Initiative (EII) coupling interferometry networks of the OPTICON EC I3. • Development, Integration, Installation of the WIRCAM instrument to CFHT. It is now offered to the CFH community. 14.5 Awards • The 52-actuator magnetic mirror has won the Photon d’Argent award of the Vitrine de l’innovation (second most innovative project) during the OPTO 2005 exhibition in September 2005 • Pierre Kern received the Cristal du CNRS in 2005 for the quality and scope of his personal contribution to a number of R&D as well as large projects • Fabien Malbet received the COMPAQ/SF2A price in 2004 for his pioneering contribution in long-baseline near-infrared interferometry and its application to the study of young stars 14.6 Acronyms • AMBER: near-infrared spectrograph for the VLTI • ANR Agence nationale de la recherche • ADONIS AO system installed on the ESO 3.6m telescope • API Antarctic Planet Interferometer • ARENA Antarctic Research, a European Network for Astronomy • AT VLTI auxiliary telescopes • CEA Atomic studies agency • CHARA Center for High Angular Resolution Astronomy Array • CNAP Conseil National des Astronomes et Physiciens • CNES Centre National d’Etudes Spatiales • CRTBT Centre de recherche des très basses températures (CNRS) • MDM: Micro Deformable Mirrors • DRFMC (CEA) Département de Recherche Fondamentale de la Matière Condensée • EC European Community • EII European Interferometry Initiative • FALCON Fiber-spectrograph with Adaptive optics on Large fields to Correct at Optical and Near-infrared wavelengths • FLUOR Fiber-Linked Unit for Optical Recombination • FP Framework Programme (of EC) • GdR Groupement de recherche (CNRS) • GeeO : Groupement d’Electromagnétisme Expérimental et d’Optoélectronique - Grenoble • GENIE Ground-based European Nulling Interferometer Experiment • GLAO Ground Layer Adaptive Optics • GTO Guarantee time observing • HRA High angular resolution • HARPS High Accuracy Radial velocity Planetary Search 142
• I3 IInternational Integrating Infrastructure (of EC FP) • IMEP Institut de Microélectronique, Electromagnétisme et Photonique (INPG) • INPG Institut National Polytechnique de Grenoble • IODA Integrated Optics for DArwin • IONIC Integrated Optics Near-Infrared Camera • IOTA Infrared Optical Telescope Array • JMMC: Jean-Marie Mariotti Center • JRA Joint research activity • KEOPS Kiloparsec Explorer for Optical Planet Search • LETI : Laboratoire d’Electronique de Technologie de l’Information (CEA) • LGGE Laboratoire de géologie et glaciologie (OSUG) • LPMC Laboratoire de Physicochimie de la Matière Condensée • MAII Multi-aperture Imaging Interferometer • MCAO Multi-Conjugate Adaptive Optics • NAOS: Nasmyth Adaptive Optics System • OCA Observatoire de la Côte d’Azur • ONERA Office national d’étude et recherches aérospatiales • OSUG Observatoire des sciences de l’Univers de Grenoble • PdB Plateau de Bure (IRAM interferometer site) • PNPS Programme National de Physique Stellaire (CNRS) • STC Scientific and Technical Committee (of ESO) • STJ Super conducting jonctions • TGE Very large equipments • VITRUV: near-infrared imager for the VLTI • WIRCAM: Wide-field InfraRed CAMera • XAO EXtreme AO 143
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LABORATOIRE D’ASTROPHYSIQUE DE GR
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III Team ASTROMOL 41 2 Presentation
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8.1.3 Graduate Students . . . . . .
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VI Team SHERPA 145 15 Results 147 1
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Part I Foreword: Presentation of th
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Part II Executive Summary A 18th ce
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of CNRS for technicians and enginee
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Figure 1.3: New LAOG organigram (20
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heart attack. Manuel went back to t
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Figure 1.6: PhD student repartition
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• LAOG researchers (and publishin
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and published 95 papers in four yea
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• National astronomy programs. 4
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1.5 From dreams to reality: Human r
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and accretion disks with heavy nume
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emphasis on the chemistry of planet
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Part III TEAM ASTROMOL Sub-arcsecon
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• we develop quantum and classica
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Table shows not only the volume of
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• Herschel-HIFI: Astromol is invo
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particular, we calculated a 9D H2O-
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• The hot corinos. More spectacul
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the massive deeply embedded protost
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tens of visual magnitudes, hence pr
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quantum VCC-IOS approximation may f
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Rate constant (cm 3 s -1 ) 1e-09 1e
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• One of us (PV) is strongly invo
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sublimation of water ice trapped ei
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If the chemistry in the first phase
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4.2.2 Molecular Physics The theoret
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Source Herschel Time Astromol Class
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several important studies that anti
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Chapter 5 Selected Publications •
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Part IV TEAM FOST The first image o
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393254 (5MJup at 55 AU) & AB Pic (1
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2.2 µ m 0.5" 11.7 µ m Figure 6.1:
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Figure 6.3: Contribution of heating
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such mid-term (several weeks) magne
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systems: HD 141569, HD 32297, HD 18
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C2D Spitzer/IRAC and MIPS data of s
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Page 178 and 179: 20.7 Production informatique ¡¢£
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Page 182 and 183: 20.13 Darwin ¡¢£¤¥¦§¨©�
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Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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