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

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Mixed GRIL-other team profiles 1. Adaptive optics instrumental development Goal: Increase the LAOG capabilities in AO instrumentation. Because of our major involvement in the large PF project, we need to increase our capabilities of integration of AO-based instrumentation by recruiting an astrophysicist with experience in the final tests and performance analysis as well as in the operation and exploitation of AO imagers. Such a profile, with instrumentation as a secondary motivation (ideally CNAP ”services d’observation”), should appear both in GRIL and in a thematic team. Target: 2007 or 2008 2. NIR interferometric spectro-imaging Goal: Exploitation of the new imaging capabilities of the VLTI. Second generation instruments, such as VITRUV, will provide unprecedented imaging capabilities to the VLTI. The need is to prepare adequately the LAOG to the optimized exploitation of this mode by recruting a researcher directly involved in the VLTI 2nd generation instrumentation realisation. Such a profile, with instrumentation as additional competence and motivation, could appear both in GRIL and in a thematic team. Target: 2009 138
Chapter 14 Appendix 14.1 Staff 14.1.1 Permanent staff People involved in the instrumental activities at LAOG over the 2001-2005 period are listed in the table 14.1 below. Some members of GRIL being also active in another team, their other team is also indicated. Those mostly involved in prospective and/or publishing in instrumental research are in the upper part of the list. Other are contributors at various levels in the GRIL activities. 14.1.2 PhD students • Adaptive optics projects: Gael Chauvin (NAOS), Guillaume Montagnier (VLTPF), Jean-François Sauvage (VLTPF), Wilfrid Schwartz (DM). • Interferometric projects: Myriam Benisty (IONIC, VITRUV), Carla Gil (AMBER), Pierre Haguenauer (IONIC, MAII), Oscar Hernandez (AMBER), Lucas Labadie (IODA, IONIC), Emmanuel Laurent (IONIC, IODA), Jean-Baptiste Le Bouquin (IONIC, VITRUV), Laure Lagny (IONIC), Pierre Mège (AMBER), Florentin Millour (AMBER), Eric Tatulli (AMBER, JMMC). 14.1.3 Other contributors • Adaptive optics projects: Amandine Blanc (NAOS, MCAO, 2year CDD), Rodolphe Conan (VLTPF, 3year post-doctoral fellow), Zoltan Hubert (DM, 1year CDD). • Interferometric projects: Swain Mark (API, IONIC - Visitor), Guillaume Mella (JMMC, JRA4 - CDD), Sylvain Cètre (JMMC, JRA4 - CDD), Willem-Jan de Wit (AMBER - postdoc), Emilie Herwats (VIT- RUV, PEGASE - Master 2 student), Pierre Demolon (IONIC - INSA Rennes student), Fatemeh Zabihian (IONIC-VLTI - Master Pro Optique student), Pierre Gratier (VITRUV - ENS Lyon student), Bram Acke (AMBER - external PhD student - Univ. Louvain), Frédéric Rooms (IONIC - external PhD student - IMEP), Elena Dufour (IODA - ENSI Caen), Coralie Aubert (VITRUV - Master 1 student), Laurianne Pichon (VITRUV), Axel Chetail (VITRUV), Benoit Neichel (VITRUV). 14.2 Main publications • NAOS on-line characterization of turbulence parameters and adaptive optics performance, Fusco T., Rousset G., Rabaud D., Gendron E., Mouillet D., Lacombe F., Zins G., Madec P.-Y., Lagrange A.-M., Charton J., Rouan D., Hubin N., Ageorges N.; 2004; Journal of Optics A: Pure and Applied Optics; 6; 585-595 139
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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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Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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