MAORY: the adaptive optics module for the Extremely Large Telescope (ELT)

MAORY is a post-focal adaptive optics module that forms part of the first light instrument suite for the ELT. The main function of MAORY is to relay the light beam from the ELT focal plane to the client instrument while compensating the effects of the atmospheric turbulence and other disturbances affecting the wavefront from the scientific sources of interest.

[1]  Nicholas Devaney,et al.  Design of a performance verification unit for the MAORY system , 2020, Astronomical Telescopes + Instrumentation.

[2]  Enrico Cascone,et al.  MAORY main structure design: general overview , 2020, Astronomical Telescopes + Instrumentation.

[3]  John R. Rogers,et al.  A Maxwellian "ideal imager" optical relay suitable for AO applications. , 2020, Astronomical Telescopes + Instrumentation.

[4]  Roberto Ragazzoni,et al.  MAORY RTC, a status update , 2020, Astronomical Telescopes + Instrumentation.

[5]  I. Di Antonio,et al.  MAORY calibration unit design status , 2020, Astronomical Telescopes + Instrumentation.

[6]  Enrico Cascone,et al.  MAORY Instrument Control Hardware: general overview , 2020 .