GeMS first on-sky results

被引：28

作者：

Rigaut, Francois ^{[1
,2
]}

Neichel, Benoit ^{[1
]}

Boccas, Maxime ^{[1
]}

d'Orgeville, Celine ^{[1
,2
]}

Arriagada, Gustavo ^{[1
]}

Fesquet, Vincent ^{[1
]}

Diggs, Sarah J. ^{[1
]}

Marchand, Claudio ^{[1
]}

Gausachs, Gaston ^{[1
]}

Rambold, William N. ^{[1
]}

Lurhs, Javier ^{[1
]}

Walker, Shane ^{[1
]}

Rodrigo Carrasco-Damele, Eleazar ^{[1
]}

Edwards, Michelle L. ^{[1
]}

Pessev, Peter ^{[1
]}

Galvez, Ramon L. ^{[1
]}

Vucina, Tomislav B. ^{[1
]}

Araya, Claudio ^{[1
]}

Gutierrez, Alejandro ^{[1
]}

Ebbers, Angelic W. ^{[1
]}

Serio, Andrew ^{[1
]}

Moreno, Cristian ^{[1
]}

Urrutia, Cristian ^{[1
]}

Rogers, Rolando ^{[1
]}

Rojas, Roberto ^{[1
]}

Trujillo, Chadwick ^{[1
]}

Miller, Brian ^{[1
]}

Simons, Douglas A. ^{[1
]}

Lopez, Ariel ^{[1
]}

Montes, Vanesa ^{[1
]}

Diaz, Herman ^{[1
]}

Daruich, Felipe ^{[1
]}

Colazo, Felipe ^{[1
]}

Bec, Matthieu ^{[3
]}

Trancho, Gelys ^{[3
]}

Sheehan, Michael ^{[3
]}

McGregor, Peter ^{[2
]}

Young, Peter J. ^{[2
]}

Doolan, Matthew C. ^{[2
]}

van Harmelen, Jan ^{[2
]}

Ellerbroek, Brent L. ^{[4
]}

Gratadour, Damien ^{[5
]}

Garcia-Rissmann, Aurea ^{[6
]}

机构：

[1] AURA, Gemini Observ, Casilla 603, La Serena, Chile

[2] Australian Natl Univ, Res Sch Astron & Astrophys, Mt Stromlo Observ, Weston, ACT 2611, Australia

[3] Giant Magellan Telescope Org Corp, Pasadena, CA 91109 USA

[4] Thirty Meter Telescope, Pasadena, CA 91125 USA

[5] Observatoire Paris Meudon, LESIA, F-92190 Meudon, France

[6] European Southern Observ, D-85748 Garching, Germany

来源：

ADAPTIVE OPTICS SYSTEMS III | 2012年 / 8447卷

关键词：

Multi-Conjugated Adaptive Optics; Adaptive Optics performance; astrometry; ADAPTIVE-OPTICS; PERFORMANCE; TELESCOPES;

D O I：

10.1117/12.927061

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

GeMS, the Gemini Laser Guide Star Multi-Conjugate Adaptive Optics facility system, has seen first light in December 2011, and has already produced images with H band Strehl ratio in excess of 35% over fields of view of 85x85 arcsec, fulfilling the MCAO promise. In this paper, we report on these early results, analyze trends in performance, and concentrate on key or novel aspects of the system, like centroid gain estimation, on-sky non-common path aberration estimation. We also present the first astrometric analysis, showing very encouraging results.

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页数：15

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