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![]() Date: 2009-04-07 14:10:35Interferometry Optical interferometry Very Large Telescope CHARA array Closure phase Radio telescope W. M. Keck Observatory Angular resolution Adaptive optics Observational astronomy Astronomy Telescopes | Source URL: usic.wikispaces.comDownload Document from Source WebsiteFile Size: 182,05 KBShare Document on Facebook |
![]() | Oscar A. Gonzalez Curriculum Vitae !DocID: 1qtfT - View Document |
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![]() | Fernando ComerĂ³n With thanks to Paul Vreeswijk and the team who implemented the RRM at the VLT The ESO Very Large Telescope 4 Unit Telescopes, each 8.2m diameter, on Cerro Paranal (Chile), at 2635m over seaDocID: 1jVM6 - View Document |
![]() | CHAPTER 1: INTRODUCTION This chapter starts by giving a brief history of the FriOWL project and details the project objectives and motivations. Then we discuss the atmospheric constraints on astronomical observation, befDocID: 1gxKE - View Document |