Knowledge Resource Center for Ecological Environment in Arid Area
| DOI | 10.1117/12.857070 |
| The Very Large Telescope Interferometer: 2010 edition | |
| Haguenauer, Pierre1; Alonso, Jaime1; Bourget, Pierre1; Brillant, Stephane1; Gitton, Philippe1; Guisard, Stephane1; Poupar, Sebastien1; Schuhler, Nicolas1; Abuter, Roberto2; Andolfato, Luigi2; Blanchard, Guillaume1; Berger, Jean-Philippe1; Cortes, Angela1; Derie, Frederic2; Delplancke, Francoise2; Di Lieto, Nicola2; Dupuy, Christophe2; Gilli, Bruno1; Glindemann, Andreas2; Guniat, Serge1; Hudepohl, Gerhard1; Kaufer, Andreas1; Le Bouquin, Jean-Baptiste1; Leveque, Samuel2; Menardi, Serge2; Merand, Antoine1; Morel, Sebastien1; Percheron, Isabelle2; Duc, Than Phan2; Pino, Andres1; Ramirez, Andres1; Rengaswamy, Sridhar1; Richichi, Andrea2; Rivinius, Thomas1; Sahlmann, Johannes2; Schoeller, Markus2; Schmid, Christian2; Stefl, Stanislav1; Valdes, Guillermo1; Van Belle, Gerard2; Wehner, Stefan1; Wittkowski, Markus2 | |
| 通讯作者 | Haguenauer, Pierre |
| 会议名称 | Conference on Optical and Infrared Interferometry II |
| 会议日期 | JUN 27-JUL 02, 2010 |
| 会议地点 | San Diego, CA |
| 英文摘要 | The ESO Very Large Telescope Interferometer (VLTI) offers access to the four 8-m Unit Telescopes (UT) and the four 1.8-m Auxiliary Telescopes (AT) of the Paranal Observatory located in the Atacama Desert in northern Chile. The two VLTI instruments, MIDI and AMBER deliver regular scientific results. In parallel to the operation, the instruments developments are pursued, and new modes are studied and commissioned to offer a wider range of scientific possibilities to the community. New configurations of the ATs array are discussed with the science users of the VLTI and implemented to optimize the scientific return. The monitoring and improvement of the different systems of the VLTI is a continuous work. The PRIMA instrument, bringing astrometry capability to the VLTI and phase referencing to the instruments has been successfully installed and the commissioning is ongoing. The possibility for visiting instruments has been opened to the VLTI facility. The current status of the VLTI is described and prospects on future evolution presented. |
| 英文关键词 | Optical long baseline interferometry Very Large Telescope Interferometer |
| 来源出版物 | OPTICAL AND INFRARED INTERFEROMETRY II |
| ISSN | 0277-786X |
| 出版年 | 2010 |
| 卷号 | 7734 |
| EISBN | 978-0-8194-8224-2 |
| 出版者 | SPIE-INT SOC OPTICAL ENGINEERING |
| 类型 | Proceedings Paper |
| 语种 | 英语 |
| 国家 | Chile;Germany |
| 收录类别 | CPCI-S |
| WOS记录号 | WOS:000285505400003 |
| WOS类目 | Engineering, Electrical & Electronic ; Optics ; Physics, Applied |
| WOS研究方向 | Engineering ; Optics ; Physics |
| 资源类型 | 会议论文 |
| 条目标识符 | http://119.78.100.177/qdio/handle/2XILL650/299052 |
| 作者单位 | 1.European So Observ, Casilla 19001, Santiago 19, Chile; 2.European Southern Observ, D-85748 Garching, Germany |
| 推荐引用方式 GB/T 7714 | Haguenauer, Pierre,Alonso, Jaime,Bourget, Pierre,et al. The Very Large Telescope Interferometer: 2010 edition[C]:SPIE-INT SOC OPTICAL ENGINEERING,2010. |
| 条目包含的文件 | 条目无相关文件。 | |||||
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。
