Software and algorithms of Subaru AO

被引：3

作者：

Gaessler, W ^{[1
]}

Takami, H ^{[1
]}

Takato, N ^{[1
]}

Hayano, Y ^{[1
]}

Kamata, Y ^{[1
]}

Saint-Jacques, D ^{[1
]}

Minowa, Y ^{[1
]}

Iye, M ^{[1
]}

机构：

[1] Subaru Telescope, Hilo, HI 96720 USA

来源：

ADAPTIVE OPTICAL SYSTEM TECHNOLOGIES II, PTS 1 AND 2 | 2003年 / 4839卷

关键词：

adaptive optics; software; algorithm; curvature sensor; real-time;

D O I：

10.1117/12.457144

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

Subaru AO a 36 element Curvature Sensor was developed for the 8.2m Subaru Telescope operated by the National Astronomical Observatory of Japan. The system is already over one year on sky and now offered for open use observation. During the time from first light to open use we did major changes in software to operate the instrument more easy and efficient and also improved the performance by tuning the control loop. We will discuss the software model and show what we learned and how we managed the crucial points of this implementation. After this we will have a look at how we can improve the system further.

引用

页码：954 / 963

页数：10

共 12 条

[1]

Gaessler W, 2001, PROC SPIE, V4494, P30

[2] Near-infrared adaptive optics spectroscopy of binary brown dwarfs HD 130948B and HD 130948C [J].

Goto, M ;

Kobayashi, N ;

Terada, H ;

Gaessler, W ;

Kanzawa, T ;

Takami, H ;

Takato, N ;

Hayano, Y ;

Kamata, Y ;

Iye, M ;

Saint-Jacques, DJ ;

Tokunaga, AT ;

Potter, D ;

Cushing, M .

ASTROPHYSICAL JOURNAL, 2002, 567 (01) :L59-L62

[3] First light for Hokupa'a 36 on Gemini North [J].

Graves, JE ;

Northcott, M ;

Roddier, F ;

Roddier, C ;

Potter, D ;

O'Connor, D .

ADAPTIVE OPTICAL SYSTEMS TECHNOLOGY, PTS 1 AND 2, 2000, 4007 :26-30

[4]

Madec P, 1999, ADAPTIVE OPTICS ASTR, P131

[5] Test, debug and development environment of Subaru Observation Software System [J].

Noumaru, J ;

Mizumoto, Y ;

Sasaki, T ;

Kosugi, G ;

Kawai, JA ;

Morita, Y ;

Akiyama, I ;

Kusama, Y ;

Imai, S .

TELESCOPE CONTROL SYSTEMS II, 1997, 3112 :52-59

[6] Performance of the Canada-France-Hawaii Telescope adaptive optics bonnette [J].

Rigaut, F ;

Salmon, D ;

Arsenault, R ;

Thomas, J ;

Lai, O ;

Rouan, D ;

Veran, JP ;

Gigan, P ;

Crampton, D ;

Fletcher, JM ;

Stilburn, J ;

Boyer, C ;

Jagourel, P .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1998, 110 (744) :152-164

[7] ERROR PROPAGATION IN A CLOSED-LOOP ADAPTIVE OPTICS SYSTEM - A COMPARISON BETWEEN SHACK-HARTMANN AND CURVATURE WAVE-FRONT SENSORS [J].

RODDIER, F .

OPTICS COMMUNICATIONS, 1995, 113 (4-6) :357-359

[8]

RODDIER FJ, 1991, P SOC PHOTO-OPT INS, V1524, P248

[9] Adaptive optics system for Cassegrain focus of Subaru 8.2 m telescope [J].

Takami, H ;

Takato, N ;

Otsubo, M ;

Kanzawa, T ;

Kamata, Y ;

Nakashima, K ;

Iye, M .

ADAPTIVE OPTICAL SYSTEM TECHNOLOGIES, PARTS 1 AND 2, 1998, 3353 :500-507

[10]

TAKAMI H, 2001, IN PRESS EUROPEAN SO

← 1 2 →