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1Caltech Optical Observatories,California Institute of Technology, 2Department of Astronomy,California Institute of Technology, 3Dunlap Institute for Astronomy and Astrophysics,University of Toronto, 4Inter-University Centre for Astronomy & Astrophysics, 5Observatories of the Carnegie Institution for Science, 6Benoziyo Center for Astrophysics,Weizmann Institute of Science
Chapitres
- 00:05Titre
- 02:45Pre-observing Procedures
- 03:52High-order Adaptive Optics Correction
- 05:40Observing in the Visible with Post-facto Registration Correction
- 06:56End of Night Procedures
- 08:01Results: Sample Images using Robo-AO
- 09:35Conclusion
Luz de objetos astronômicos deve viajar através da atmosfera turbulenta da terra antes de ser fotografada por telescópios terrestres. Para ativar imagens diretas na resolução teórica máxima angular, técnicas avançadas, como os empregados pelo Robo-AO sistema adaptativo óptica deve ser usado.
