Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
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Chapter 13<br />
Recruitment plan<br />
GRIL needs are two-fold: researchers with instrumental skills able to fullfill key responsabilities in large projects<br />
or with research programs in specific technological fields that are at the heart of our R&D projects; engineers with<br />
a strong motivation in R&D activities and expertise in the fields that are of importance for our <strong>de</strong>velopments.<br />
Because of the strong commitment the LAOG has towards the VLT Planet Fin<strong>de</strong>r realisation and that of<br />
the VLTI 2µm imager, very likely to be scheduled soon, it is essential to increase our resources in some very<br />
specific fields of expertise in or<strong>de</strong>r to maintain and consolidate our R&D capabilities. For this reason, during<br />
the next quadrennal period, GRIL should either recruit or welcome external persons on the various profiles<br />
<strong>de</strong>scribed below according to the two categories, pure instrumental profiles (GRIL recruitments) and mixed<br />
astrophysical-instrumental profiles (thematic team recruitement with participation to GRIL activities).<br />
GRIL profiles<br />
1. Adaptive optics R&D and system<br />
Goal: Increase the LAOG capabilities in AO instrumentation. Because of our major involvement in the<br />
large PF project, most of our capabilities connected to AO expertise will be focused on the realisation<br />
of this instrument. In or<strong>de</strong>r to succeed in this whole pursuing our innovative R&D activities in AO, we<br />
need to increase our global capabilities in AO components R&D and/or system <strong>de</strong>finition by recruiting<br />
an AO-oriented instrumentalist researcher accompaning the recruitment of an AO-<strong>de</strong>dicated project manager/system<br />
engineer (IR1). This should occur in the fall of 2006.<br />
Target: 2007 or 2008<br />
2. Nulling interferometry at thermal IR wavelengths<br />
Goal: Preparation studies for Darwin. In parallel and support to R&D on thermal IR guiding optics,<br />
such as IODA and other possible studies in preparation for DARWIN, we have i<strong>de</strong>ntified the need for<br />
a researcher strongly <strong>de</strong>dicated to the search for planets in MIR in general and personally involved in<br />
the preparation of DARWIN or precursor missions. He would have to pilot the preparatory studies that<br />
LAOG is performing and possibly going to enlarge in the frame of its pluriannual commitment to ESA<br />
and ALCATEL ALENIA partnership.<br />
Target: 2007<br />
3. JMMC support for 4-6T exploitation<br />
Goal: Participation to the JMMC <strong>de</strong>velopments supporting the VLTI evolution toward more than 3 beams.<br />
LAOG has a special role in the JMMC since it harbors the coordination center and some key members<br />
of the working groups. Because of its probable involvement in a second generation instrument, it should<br />
also help in <strong>de</strong>veloping the <strong>de</strong>dicated tools for the VLTI exploitation.<br />
Target: 2008<br />
It should be noted that these profiles might evolve according to the actual profile of the MdC who should<br />
be recruited in section 34 or any other recruitment possibly achieved in 2006.<br />
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