MAVIS update: WFSing and control
Jesse Cranney  1, 2, @  , Cedric Plantet  3  , Guido Agapito  3  , Olivier Beltramo-Martin  4  , Maria Bergomi  5  , Jean-Claude Bouret  4  , David Brodrick  1, 2  , Giovanni Cresci  3  , Nicolas Doucet  1, 2  , Damien Gratadour  1, 2, 6  , Pierre Haguenauer  7  , Dionne Haynes  2, 1  , Richard Mcdermid  8, 2  , Enrico Pinna  3  , Kalyan Radhakrishnan Santhakumari  5  , Francois Rigaut  2, 1  , Valentina Viotto  5  , Hao Zhang  2, 1  
1 : Advanced Instrumentation Technology Centre, Research School of Astronomy and Astrophysics, Australian National University, Canberra
2 : Astralis Instrumentation Consortium
3 : INAF - Osservatorio Astrofisico di Arcetri
4 : Laboratoire d'Astrophysique de Marseille
Le Laboratoire D'Astrophysique De Marseille
5 : INAF - Osservatorio Astronomico di Padova
6 : Laboratoire d'études spatiales et d'instrumentation en astrophysique  (LESIA)
Observatoire de Paris, Observatoire de Paris
7 : European Southern Observatory
8 : Australian Astronomical Optics, Macquarie University, Sydney

The MCAO Assisted Visible Imager and Spectrograph (MAVIS) is approaching PDR, and will begin the final design phase in 2023. In order for MAVIS to satisfy the tight error budget for V-band wide-field imaging, novel WFSing and control concepts have been employed. We present a status update on various aspects of the MAVIS WFSing and control design.

Subject : : oral
Topics : WFSensing & Reconstruction Methods
PDF version :  PDF version
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