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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
Chapters
- 00:05Title
- 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
Lys fra astronomiske objekter skal rejse gennem jordens turbulente atmosfære, før det kan afbildes ved jordbaserede teleskoper. For at aktivere direkte billeddannelse ved maksimal teoretisk kantede opløsning, skal avancerede teknikker såsom de ansat af Robo-AO adaptive-optik-systemet anvendes.
