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

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8.1.3 Graduate Students . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105 8.2 Awards and Prizes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105 V Team GRIL 107 9 Presentation of the team 109 9.1 Foundation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109 9.2 A specific expertise . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 109 9.3 Organization . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 9.4 Related activities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 10 Scientific rationale 111 10.1 Background . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111 10.1.1 Key astrophysical questions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111 10.1.2 Related instrumental evolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111 10.1.3 Current trend of large equipments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112 10.1.4 Increasing networking process . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112 10.2 Strategy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112 10.2.1 Well defined priorities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112 10.2.2 Focusing on three complementary axii . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113 10.2.3 The principles of our involvement . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 114 10.2.4 A logical sequence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 114 11 Results 116 11.1 Towards high dynamic with Adaptive Optics (AO) . . . . . . . . . . . . . . . . . . . . . . . . . . 116 11.1.1 The first generation: NAOS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 116 11.1.2 The high contrast imaging: VLTPF . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 116 11.1.3 Instrumental Research and development activities . . . . . . . . . . . . . . . . . . . . . . 118 11.2 Bringing optical interferometry into mainstream astronomy . . . . . . . . . . . . . . . . . . . . . 120 11.2.1 The classical approach: AMBER . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120 11.2.2 The innovative integrated optics: IONIC on the IOTA and VLTI interferometers . . . . . 122 11.2.3 Combining up to eight telescopes of the VLTI array: VITRUV . . . . . . . . . . . . . . . 122 11.2.4 Instrumental Research and development activities . . . . . . . . . . . . . . . . . . . . . . 123 11.2.5 JMMC and European Interferometry Initiative . . . . . . . . . . . . . . . . . . . . . . . . 125 8
11.3 Cameras and detectors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 126 11.3.1 Towards wide-field cameras: WIRCam . . . . . . . . . . . . . . . . . . . . . . . . . . . . 126 11.3.2 Research and development activities in photon counting superconducting detectors . . . 126 12 Perspectives 129 12.1 Adaptive optics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129 12.1.1 Instruments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129 12.1.2 R&D activities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131 12.1.3 Means and methods . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131 12.2 Optical interferometry . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132 12.2.1 Instruments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132 12.2.2 Software development for interferometry . . . . . . . . . . . . . . . . . . . . . . . . . . . 133 12.2.3 R&D activities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 133 12.2.4 Means and methods . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 134 12.3 Cameras and detectors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 134 12.3.1 Instrument support technology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 135 12.3.2 R&D activities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 135 12.3.3 Means and methods . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 135 13 Recruitment plan 137 14 Appendix 139 14.1 Staff . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 14.1.1 Permanent staff . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 14.1.2 PhD students . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 14.1.3 Other contributors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 14.2 Main publications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139 14.3 Industrial development . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141 14.3.1 Patents . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141 14.3.2 Technological transfer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141 14.4 Highlights . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141 14.5 Awards . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142 14.6 Acronyms . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142 9
Page 3: LABORATOIRE D’ASTROPHYSIQUE DE GR
Page 6 and 7: III Team ASTROMOL 41 2 Presentation
Page 10 and 11: VI Team SHERPA 145 15 Results 147 1
Page 13: Part I Foreword: Presentation of th
Page 17: Part II Executive Summary A 18th ce
Page 20 and 21: of CNRS for technicians and enginee
Page 22 and 23: Figure 1.3: New LAOG organigram (20
Page 24 and 25: heart attack. Manuel went back to t
Page 26 and 27: Figure 1.6: PhD student repartition
Page 28 and 29: • LAOG researchers (and publishin
Page 30 and 31: and published 95 papers in four yea
Page 32 and 33: • National astronomy programs. 4
Page 34 and 35: 1.5 From dreams to reality: Human r
Page 36 and 37: and accretion disks with heavy nume
Page 38 and 39: emphasis on the chemistry of planet
Page 41: Part III TEAM ASTROMOL Sub-arcsecon
Page 44 and 45: • we develop quantum and classica
Page 46 and 47: Table shows not only the volume of
Page 48 and 49: • Herschel-HIFI: Astromol is invo
Page 50 and 51: particular, we calculated a 9D H2O-
Page 52 and 53: • The hot corinos. More spectacul
Page 54 and 55: the massive deeply embedded protost
Page 56 and 57: tens of visual magnitudes, hence pr
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quantum VCC-IOS approximation may f
Page 60 and 61:
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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et al. 2002; 2003). We have found t
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Figure 6.8: Distribution of separat
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with only three known to date. Most
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300 objects, a size sufficient for
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therefore no surprise that vast eff
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data to verify the predictions we a
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Chapter 8 Appendices 8.1 Members of
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106
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108
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equipments for these tasks, from de
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10.1.3 Current trend of large equip
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• Improving High Angular Resoluti
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Chapter 11 Results 11.1 Towards hig
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Figure 11.2: NAOS-CONICA image of t
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on PUEO at CFHT. The IFS experts (A
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Figure 11.5: Image of the binary st
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Figure 11.7: PICNIC low noise infra
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have taken responsibilities: A. Che
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Figure 11.10: thermal modeling of W
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Figure 12.1: All the GRIL projects
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12.2 Optical interferometry As for
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the VLTI. CHARA is equipped with an
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• ANR Alterdetect, with IMEP : si
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Mixed GRIL-other team profiles 1. A
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Name Grade Comm. Project Berger Jea
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• First fringes in the H band wit
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144
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146
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Table 15.1: List of the permanent S
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15.4 Transport phenomena in accreti
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Figure 15.2: Spectral energy distri
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states, combining a still powerful
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Excitation of turbulence by Cosmic
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Table 15.2: Former PhD students of
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Chapter 16 Perspectives The distinc
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Ray background. The second project
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164
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- Ceccarelli Cecilia (AT) - Delfoss
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Among the various areas of expertis
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-responsable du groupe ”logiciel
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Chef de l’ Equipe ASTROMOL du LAO
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jury de concours: 1 concours IR CNR
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Chapter 20 Appendix 4: The Jean Mar
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20.7 Production informatique ¡¢£
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20.10 Formation des utilisateurs La
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20.13 Darwin ¡¢£¤¥¦§¨©�
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Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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