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

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Name Grade Comm. Project Berger Jean-Philippe AA FOST IONIC, VITRUV, JMMC Beuzit Jean-Luc CR FOST MDM, VLTPF, MCAO, WIRCAM Chalabaev Almas CR FOST GRIF, VLTPF Charton Julien IR MDM, NAOS, VLTPF Chelli Alain A FOST AMBER, JMMC, EII Duvert Gilles AA FOST AMBER, JMMC, EII Feautrier Philippe IR (HDR) NAOS, WIRCAM, VLTPF Jocou Laurent AI MDM, IONIC, MAII, IODA, VITRUV Kern Pierre IR NAOS, MDM, AMBER, IONIC, MAII, IODA, VITRUV, EII Le Coarer Etienne IR (HDR) AMBER, IONIC, IODA, VITRUV Malbet Fabien CR FOST AMBER, IONIC, VITRUV, JMMC, PEGASE, EII Perraut Karine AA AMBER, IONIC, IODA, VITRUV Perrier Christian A FOST AMBER, MAII, VITRUV, EII, NACO, VLTPF, WIRCAM Puget Pascal IR (1) NAOS, AMBER, WIRCAM, VLTPF Rabou Patrick IR NAOS, VLTPF Stadler Eric IR MDM, NAOS, WIRCAM, VLTPF Zins Gérard IR AMBER, JMMC, EII Arezki Brahim IE AMBER, IONIC, MAII, IODA Delboulbé Alain AI AMBER, IONIC, MAII, IODA, VITRUV, WIRCAM Delfosse Xavier AA FOST JMMC Fraix-Burnet Didier CR SHERPAS AMBER Glück Laurence IE AMBER, JMMC Lagrange Anne-Marie DR FOST NACO, VLTPF Monin Jean-Louis PR FOST AMBER Petrucci Pierre-Olivier CR SHERPAS VITRUV Preis Olivier IE IONIC, VITRUV Note: 1 on leave from LAOG mid-2002 Table 14.1: GRIL permanent staff. 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. Note that 2 engineers are qualified to supervised PhDs (french ’HDR’). • MOEMS pour la correction de surface d’onde en optique adaptative, by Schwartz W., Beuzit J.-L., Kern P.; 2003 in Microsystèmes opto-électromécaniques, pp. 141-180 • See section on valorisation for results on MMD development (patents submission prevent publication) • Series ”Integrated optics for astronomical interferometry” in A&A • Planar integrated optics and astronomical interferometry, Kern, P.; Berger, J.-P.; Haguenauer, P.; Malbet, F.; Perraut, K.; 2001 ; C. R. Acad. Sci. Paris ; 2 ; 111-124 • First Results with the IOTA3 Imaging Interferometer: The Spectroscopic Binaries lambda Virginis and WR 140, Monnier, J. D.; Traub, W. A.; Schloerb, F. P.; Millan-Gabet, R.; Berger, J.-P.; Pedretti, E.; Carleton, N. P.; Kraus, S.; Lacasse, M. G.; Brewer, M.; Ragland, S.; Ahearn, A.; Coldwell, C.; Haguenauer, P.; Kern, P.; Labeye, P.; Lagny, L.; Malbet, F.; Malin, D.; Maymounkov, P.; Morel, S.; Papaliolios, C.; Perraut, K.; Pearlman, M.; Porro, I. L.; Schanen, I.; Souccar, K.; Torres, G.; Wallace, G.; 2004 ; Astrophysical Journal Letters ; 602 ; L57-L60 • First observations with an H-band integrated optics beam combiner at the VLTI, Le Bouquin, J. B.; Rousselet-Perraut, K.; Kern, P.; Malbet, F.; Haguenauer, P.; Kervella, P.; Schanen, I.; Berger, J. P.; Delboulbe, A.; Arezki, B.; Schöller, M.; 2004 ; Astronomy and Astrophysics ; 424 ; 719-726 • Infrared Imaging of Capella with the IOTA Closure Phase Interferometer, Kraus, S.; Schloerb, F. P.; Traub, W. A.; Carleton, N. P.; Lacasse, M.; Pearlman, M.; Monnier, J. D.; Millan-Gabet, R.; Berger, J.-P.; Haguenauer, P.; Perraut, K.; Kern, P.; Malbet, F.; Labeye, P.; 2005 ; The Astronomical Journal, Volume 130, Issue 1, 246-255 140
• Tantalum superconducting tunnel junctions for infrared photon counting, Jorel, C.; Villégier, J.-C.; Feautrier, P.; Benoit, A.; 2004 ; Nuclear Instruments and Methods in Physics Research A ; 520 ; 516-518 14.3 Industrial development 14.3.1 Patents Three applications have been filled regarding possible patents in the frame of our R&D activities on new deformable micro-mirrors. All three patents have now been issued. Details are given below: • ”Dispositif d’actionnement électrostatique miniature et installation comprenant de tels dispositifs”, European Patent, CNRS/CEA, FR0206293 from 23/05/2002. Patent holders: J. Charton and E. Stadler. • ”Composant MEMS électrostatique permettant un déplacement vertical important”, French patent, CNRS/CEA, FR0351211 from 26/12/2003. Patent holders: J. Charton and C. Divoux (CEA/LETI). • ”Miroir déformable magnétique”, French Patent, CNRS, FR0452342 from 12/10/2004. Patent Holders: J. Charton, Z. Hubert, L. Jocou, E. Stadler, P. Kern and J.-L. Beuzit. Two applications are currently processed in the frame of our activities on future detectors: • ”Détecteur et caméra spectroscopique interférentiels”, French Patent, UJF INPI 04/52992, applied December 15th 2004. Patent Holders: le Coarer, E., Benech, P. • ”Spectrographes à onde contra-propagative”, French Patent, UJF INPI 05/08429, applied August 8th 2005. Patent Holders: le Coarer, E., Benech, P., Blaize, S., Kern, P., Lérondel, G., Morand, A. 14.3.2 Technological transfer After the commercial license agreements signed for the distribution of our magnetic deformable mirrors, it is intended to extend this industrial development to other instrumental research results. 14.4 Highlights The main facts related to our activities since 2001 are summarized below: • The NAOS (Nasmyth Adaptive Optics System) instrument for the VLT is now offered to the ESO astronomical community after a successful commissioning and science verification between November 2001 and August 2002. • Magnetic Deformable Mirrors are now fully functional and available to all interested parties through our industrial partners. • The developments of electrostatic deformable mirrors between LAOG and CEA/LETI is underway with a first fully functional 19-actuators laboratory prototype being characterized. • The “Planet Finder” proposal for a second generation instrument for the VLT led by LAOG was selected by the ESO STC in April 2005 after a successfull 2-year phase A study, awaiting formal decision by the next ESO Council. • Development, Integration, Installation of the AMBER instrument to ESO. It is now offered to the ESO astronomical community for part of its modes and will be fully offered when the VLTI improvement plan is completed. 141
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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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Page 182 and 183: 20.13 Darwin ¡¢£¤¥¦§¨©�
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