首页> 外文会议>Conference on Future Giant Telescopes, Aug 26-28, 2002, Waikoloa, Hawaii, USA >THE LARGE PETAL TELESCOPE FOR THE NEXT GENERATION CANADA-FRANCE-HAWAII TELESCOPE
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THE LARGE PETAL TELESCOPE FOR THE NEXT GENERATION CANADA-FRANCE-HAWAII TELESCOPE

机译:适用于下一代加拿大-法国-夏威夷电视台的大型电视

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Considered until recently one of the best telescopes in the world, the Canada-France-Hawaii Telescope (CFHT) is now bypassed by larger telescopes. Aware of this problem, the CFHT Science Advisory Council (SAC) solicited proposals from the CFH community groups to replace the present telescope by a world-class research facility before the end of the decade. A report describing our proposal is available on our web site (www.astrsp-mrs.fr/denisgcfhtgcfht.html). The motivation to design and build a new telescope is often driven by the astronomers need to observe fainter and fainter sources. The basis of the next generation CFHT (NG-CFHT) is therefore to increase the size of the primary mirror to reach fainter and more remote objects in the luminosity functions. But beyond this photon quest, the way we use the photons is also very important. The development of new technologies will permit an optimization of performances and a better image quality thanks to state-of-the-art instruments on state-of-the-art telescopes.
机译:直到最近,加拿大-法国-夏威夷望远镜(CFHT)才被认为是世界上最好的望远镜之一,而现在却被大型望远镜绕开了。意识到这一问题,CFHT科学顾问委员会(SAC)征求了CFH社区团体的建议,以在本世纪末之前用世界一流的研究机构替代目前的望远镜。可在我们的网站(www.astrsp-mrs.fr/denis/ngcfht/ngcfht.html)上找到描述我们建议的报告。天文学家需要观察微弱和微弱的源头,通常是设计和建造新望远镜的动力。因此,下一代CFHT(NG-CFHT)的基础是增加主镜的尺寸,以达到发光功能中较暗且较远的物体。但是,除了追求光子以外,我们使用光子的方式也非常重要。由于采用了最先进的望远镜上的最新仪器,因此新技术的发展将使性能得到优化,并获得更好的图像质量。

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