The WEAVE prime focus correction: from design to integration
The WEAVE prime focus correction: from design to integration
复制标题
WEAVE 主焦校正:从设计到集成
DOI:
10.1117/12.2313718
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发表时间:
2018
期刊:
影响因子:
--
通讯作者:
Casalta J
中科院分区:
文献类型:
--
作者:
Casalta J
WEAVE is a new wide-field multi-object spectroscopy (MOS) facility proposed for the prime focus of the 4.2m William Herschel Telescope (WHT), situated on the island of La Palma, Canary Islands, Spain. To allow for the compensation of the effects of temperature-induced and gravity-induced image degradation, the WEAVE prime focus assembly will be translated along the telescope optical axis. The assembly comprises the prime focus corrector (PFC), a central mount for the corrector known as FTS[1], an instrument rotator and a twin-focal-plane fibre positioner. SENER, that manufactured and delivered the FTS, is also responsible for the final design, manufacturing, integration, alignment and testing of the PFC and its ancillary equipment. This manuscript describes the final design of the PFC along with the analyses and simulations performed and presents the procedures for the integration and alignment of the lenses in the corrector.
影响因子:
3.5
作者:
D. Brooks;P. Doel;R. Besuner;B. Flaugher;G. Gallo;G. Gutiérrez;S. Kent;M. Lampton;M. Levi;M. Liang;T. Miller;D. Sprayberry;A. Stefanik
通讯作者:
A. Stefanik
DOI:
10.1117/12.926590
发表时间:
2012
期刊:
--
影响因子:
--
作者:
Doel P
通讯作者:
Doel P
DOI:
--
发表时间:
2002
期刊:
SPIE Optics + Photonics
影响因子:
--
作者:
K. Doyle;Gregory J. Michels;V. Genberg
通讯作者:
V. Genberg