MAORY calibration unit design status

I. Di Antonio; G. Di Rico; A. Valentini; G. Rodeghiero; M. Dolci; A. Goncharov; N. Devaney; V. Cianniello; V. De Caprio; E. Redaelli; M. Riva; C. Eredia; E. Cascone; L. Busoni; P. Ciliegi; S. Oberti

doi:10.1117/12.2561429

MAORY calibration unit design status

I. Di Antonio, G. Di Rico, A. Valentini, G. Rodeghiero, M. Dolci, A. Goncharov, N. Devaney, V. Cianniello, V. De Caprio, E. Redaelli, M. Riva, C. Eredia, E. Cascone, L. Busoni, P. Ciliegi, S. Oberti

Physics

Research output: Chapter in Book or Conference Publication/Proceeding › Conference Publication › peer-review

3 Citations (Scopus)

Abstract

MAORY (Multi-conjugate Adaptive Optics RelaY) is one of the first light instruments for the ESO Extremely Large Telescope (ELT). It will be firstly used by MICADO (Multi-AO Imaging CamerA for Deep Observations), a near-infrared high-angular resolution imager, to compensate aberrations and provide highStrehl images within a 53"×53"Field of View (FoV). The complexity of MAORY requires calibration functionalities for both the AIV (Assembly-Integration-Verification) and the operational phase. The Calibration Unit (CU), providing suitable light sources, both Natural Guide Stars (NGS) and Laser Guide Stars (LGS), will enable MAORY to run calibration templates as well as verification and test procedures, in standalone mode, drastically reducing the amount of required night-time for such operations. An overview of the instrument, the current status of the design and the main challenges to face in the future are here presented.

Original language	English
Title of host publication	Adaptive Optics Systems VII
Editors	Laura Schreiber, Dirk Schmidt, Elise Vernet
Publisher	SPIE
ISBN (Electronic)	9781510636835
DOIs	https://doi.org/10.1117/12.2561429
Publication status	Published - 2020
Event	Adaptive Optics Systems VII 2020 - Virtual, Online, United States Duration: 14 Dec 2020 → 22 Dec 2020

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11448
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Adaptive Optics Systems VII 2020
Country/Territory	United States
City	Virtual, Online
Period	14/12/20 → 22/12/20

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10.1117/12.2561429

Cite this

Di Antonio, I., Di Rico, G., Valentini, A., Rodeghiero, G., Dolci, M., Goncharov, A., Devaney, N., Cianniello, V., De Caprio, V., Redaelli, E., Riva, M., Eredia, C., Cascone, E., Busoni, L., Ciliegi, P., & Oberti, S. (2020). MAORY calibration unit design status. In L. Schreiber, D. Schmidt, & E. Vernet (Eds.), Adaptive Optics Systems VII Article 1144830 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11448). SPIE. https://doi.org/10.1117/12.2561429

@inproceedings{0dbb82e632d34344a0e061791f70f44a,

title = "MAORY calibration unit design status",

abstract = "MAORY (Multi-conjugate Adaptive Optics RelaY) is one of the first light instruments for the ESO Extremely Large Telescope (ELT). It will be firstly used by MICADO (Multi-AO Imaging CamerA for Deep Observations), a near-infrared high-angular resolution imager, to compensate aberrations and provide highStrehl images within a 53{"}×53{"}Field of View (FoV). The complexity of MAORY requires calibration functionalities for both the AIV (Assembly-Integration-Verification) and the operational phase. The Calibration Unit (CU), providing suitable light sources, both Natural Guide Stars (NGS) and Laser Guide Stars (LGS), will enable MAORY to run calibration templates as well as verification and test procedures, in standalone mode, drastically reducing the amount of required night-time for such operations. An overview of the instrument, the current status of the design and the main challenges to face in the future are here presented.",

author = "\{Di Antonio\}, I. and \{Di Rico\}, G. and A. Valentini and G. Rodeghiero and M. Dolci and A. Goncharov and N. Devaney and V. Cianniello and \{De Caprio\}, V. and E. Redaelli and M. Riva and C. Eredia and E. Cascone and L. Busoni and P. Ciliegi and S. Oberti",

note = "Publisher Copyright: {\textcopyright} 2020 SPIE.; Adaptive Optics Systems VII 2020 ; Conference date: 14-12-2020 Through 22-12-2020",

year = "2020",

doi = "10.1117/12.2561429",

language = "English",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Laura Schreiber and Dirk Schmidt and Elise Vernet",

booktitle = "Adaptive Optics Systems VII",

}

Di Antonio, I, Di Rico, G, Valentini, A, Rodeghiero, G, Dolci, M, Goncharov, A , Devaney, N, Cianniello, V, De Caprio, V, Redaelli, E, Riva, M, Eredia, C, Cascone, E, Busoni, L, Ciliegi, P & Oberti, S 2020, MAORY calibration unit design status. in L Schreiber, D Schmidt & E Vernet (eds), Adaptive Optics Systems VII., 1144830, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11448, SPIE, Adaptive Optics Systems VII 2020, Virtual, Online, United States, 14/12/20. https://doi.org/10.1117/12.2561429

MAORY calibration unit design status. / Di Antonio, I.; Di Rico, G.; Valentini, A. et al.
Adaptive Optics Systems VII. ed. / Laura Schreiber; Dirk Schmidt; Elise Vernet. SPIE, 2020. 1144830 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11448).

Research output: Chapter in Book or Conference Publication/Proceeding › Conference Publication › peer-review

TY - GEN

T1 - MAORY calibration unit design status

AU - Di Antonio, I.

AU - Di Rico, G.

AU - Valentini, A.

AU - Rodeghiero, G.

AU - Dolci, M.

AU - Goncharov, A.

AU - Devaney, N.

AU - Cianniello, V.

AU - De Caprio, V.

AU - Redaelli, E.

AU - Riva, M.

AU - Eredia, C.

AU - Cascone, E.

AU - Busoni, L.

AU - Ciliegi, P.

AU - Oberti, S.

PY - 2020

Y1 - 2020

N2 - MAORY (Multi-conjugate Adaptive Optics RelaY) is one of the first light instruments for the ESO Extremely Large Telescope (ELT). It will be firstly used by MICADO (Multi-AO Imaging CamerA for Deep Observations), a near-infrared high-angular resolution imager, to compensate aberrations and provide highStrehl images within a 53"×53"Field of View (FoV). The complexity of MAORY requires calibration functionalities for both the AIV (Assembly-Integration-Verification) and the operational phase. The Calibration Unit (CU), providing suitable light sources, both Natural Guide Stars (NGS) and Laser Guide Stars (LGS), will enable MAORY to run calibration templates as well as verification and test procedures, in standalone mode, drastically reducing the amount of required night-time for such operations. An overview of the instrument, the current status of the design and the main challenges to face in the future are here presented.

AB - MAORY (Multi-conjugate Adaptive Optics RelaY) is one of the first light instruments for the ESO Extremely Large Telescope (ELT). It will be firstly used by MICADO (Multi-AO Imaging CamerA for Deep Observations), a near-infrared high-angular resolution imager, to compensate aberrations and provide highStrehl images within a 53"×53"Field of View (FoV). The complexity of MAORY requires calibration functionalities for both the AIV (Assembly-Integration-Verification) and the operational phase. The Calibration Unit (CU), providing suitable light sources, both Natural Guide Stars (NGS) and Laser Guide Stars (LGS), will enable MAORY to run calibration templates as well as verification and test procedures, in standalone mode, drastically reducing the amount of required night-time for such operations. An overview of the instrument, the current status of the design and the main challenges to face in the future are here presented.

UR - https://www.scopus.com/pages/publications/85100035244

U2 - 10.1117/12.2561429

DO - 10.1117/12.2561429

M3 - Conference Publication

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Adaptive Optics Systems VII

A2 - Schreiber, Laura

A2 - Schmidt, Dirk

A2 - Vernet, Elise

PB - SPIE

T2 - Adaptive Optics Systems VII 2020

Y2 - 14 December 2020 through 22 December 2020

ER -

MAORY calibration unit design status

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