On-sky demonstration of the GMT dispersed fringe phasing sensor prototype on the Magellan Telescope
The GMT is an aplanatic Gregorian telescope consisting of 7 primary and secondary mirror segments that must be phased to within a fraction of an imaging wavelength to allow the 25.4 meter telescope to reach its diffraction limit. When operating in Laser Tomographic Adaptive Optics (LTAO) mode, on-ax...
Similar Items
-
New and improved technology for manufacture of GMT primary mirror segments
by: Kim, Dae Wook, et al.
Published: (2016) -
Status of mirror segment production for the Giant Magellan Telescope
by: Martin, H. M., et al.
Published: (2016) -
Vibrations in MagAO: frequency-based analysis of on-sky data, resonance sources identification, and future challenges in vibrations mitigation
by: Zúñiga, Sebastián, et al.
Published: (2016) -
Development of the fast steering secondary mirror assembly of GMT
by: Lee, Sungho, et al.
Published: (2016) -
PROPERTIES OF CEPHEID VARIABLES IN THE LARGE MAGELLANIC CLOUD
by: Connolly, Leo Paul, 1947-
Published: (1975)