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Untitled - ESO

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The activities within the EU FP6-supported<br />

ELT Design Studies programme,<br />

led by <strong>ESO</strong> but largely executed in<br />

industry and academia outside the<br />

organisation, are aligned with the<br />

activities of the E-ELT programme and in<br />

all areas much progress is being made.<br />

Actuator prototypes, edge sensors, phasing<br />

techniques, wind evaluation systems,<br />

dome designs, site testing and many<br />

other such activities are all contributing to<br />

the knowledge we require to advance the<br />

project into the next phase. Integral to<br />

this planning is the membership of Spain<br />

in <strong>ESO</strong> and the expertise that the Spanish<br />

community will bring. Spain has just<br />

completed the segmented 10.4-m Gran<br />

Telescopio Canarias (GTC) telescope<br />

and, with Spain’s membership, <strong>ESO</strong><br />

engineers will gain technical access to<br />

that system.<br />

Participants to the E-ELT conference in Marseille.<br />

46<br />

<strong>ESO</strong> Annual Report 006<br />

The baseline reference design selected<br />

and approved by the <strong>ESO</strong> Council to<br />

move into the Phase B of the project is<br />

the five-mirror design. While the Gregorian<br />

design had advantages in a better<br />

theoretical performance in adaptive optics,<br />

a smaller mirror count and smaller<br />

central obstruction, the five-mirror design<br />

was considered to have advantages in<br />

the image quality across the focal plane,<br />

the control of the wavefront using laser<br />

guide stars, the flexibility of the focal stations,<br />

the deployment of atmospheric<br />

dispersion compensators, the smaller<br />

dome and the relative ease with which it<br />

could be upgraded to follow the development<br />

of technology in the future. Most<br />

critically however, the five-mirror design<br />

was considered to have much lower risk<br />

in the area of adaptive optics by virtue<br />

of the separation of the field-stabilisation<br />

and adaptive-optics functions, a key recommendation<br />

of the OWL review.<br />

Into Phase B<br />

The results of this burst of activity came<br />

together during November 006 in preparation<br />

for a series of presentations of<br />

the Project Office conclusions to ESE,<br />

ESRC, STC, to 50 astronomers at the<br />

Marseilles meeting on the E-ELT and, finally,<br />

to the <strong>ESO</strong> Council. The endorsement<br />

of the Project Office proposal by<br />

this broad spectrum of the community<br />

and decision makers reflects not only the<br />

good progress <strong>ESO</strong> made during 006<br />

in the elaboration of the design but also<br />

the clear scientific need to advance<br />

rapidly and effectively in the area of E-<br />

ELTs and the commitment of the user<br />

community.

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