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Paper detail

Layer Oriented Wavefront sensor for MAD on Sky operations

The Multiconjugate Adaptive optics Demonstrator (MAD) has successfully demonstrated on sky both Star Oriented (SO) and Layer Oriented (LO) multiconjugate adaptive optics techniques. While SO has been realized using 3 Shack-Hartmann wavefront sensors (WFS), we designed a multi-pyramid WFS for the LO. The MAD bench accommodates both WFSs and a selecting mirror allows choosing which sensor to use. In the LO approach up to 8 pyramids can be placed on as many reference stars and their light is co-added optically on two different CCDs conjugated at ground and to an high layer. In this paper we discuss LO commissioning phase and on sky operations.

preprint2009arXivOpen access
Carmelo ArcidiaconoMatteo LombiniRoberto RagazzoniJacopo FarinatoEmiliano DiolaitiAndrea BaruffoloPaolo BagnaraGiorgia GentileLaura SchreiberEnrico MarchettiJohann KolbSebastien TordoRobert DonaldsonChristian SoenkeSylvain ObertiEnrico FedrigoElise VernetNorbert Hubin
astro-ph.IM
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Carmelo ArcidiaconoMatteo LombiniRoberto RagazzoniJacopo FarinatoEmiliano DiolaitiAndrea BaruffoloPaolo BagnaraGiorgia GentileLaura SchreiberEnrico MarchettiJohann KolbSebastien TordoRobert DonaldsonChristian SoenkeSylvain ObertiEnrico FedrigoElise VernetNorbert Hubin

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