High-contrast imaging science with Adaptive Optics

被引：1

作者：

Brandner, W ^{[1
]}

Potter, D ^{[1
]}

机构：

[1] European So Observ, D-85748 Garching, Germany

来源：

SCIENTIFIC DRIVERS FOR ESO FUTURE VLT/VLTI INSTRUMENTATION, PROCEEDINGS | 2002年

关键词：

D O I：

10.1007/10857019_42

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Adaptive Optics (AO) has become an integral part of almost all present and future large telescope initiatives, and will be essential in exploiting the full potential of the large optical interferometers currently under construction. This contribution focuses on the limitations of AO with respect to dynamic range, and on the potential of high-contrast imaging techniques.

引用

页码：264 / 266

页数：3

共 7 条

[1] Achromatic interfere coronagraphy II. Effective performance on the sky
Baudoz, P
Rabbia, Y
Gay, J
Burg, R
Petro, L
Bely, P
Fleury, B
Madec, PY
Charbonnier, F
[J]. ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 2000, 145 (02): : 341 - 350
[2] GRAVES JE, 2000, SPIE, V4007, P126
[3] CONICA: The high resolution near-infrared camera for the ESO VLT
Lenzen, R
Hofmann, R
Bizenberger, P
Tusche, A
[J]. INFRARED ASTRONOMICAL INSTRUMENTATION, PTS 1-2, 1998, 3354 : 606 - 614
[4] Speckle noise and the detection of faint companions
Racine, R
Walker, GAH
Nadeau, D
Doyon, R
Marois, C
[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1999, 111 (759) : 587 - 594
[5] Stellar coronagraph with phase mask
Roddier, F
Roddier, C
[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1997, 109 (737) : 815 - 820
[6] Status of the VLT Nasmyth adaptive optics system (NAOS)
Rousset, G
Lacombe, F
Puget, P
Gendron, E
Arsenault, R
Kern, P
Rabaud, D
Madec, PY
Hubin, N
Zins, G
Stadler, E
Charton, J
Gigan, P
Feautrier, P
[J]. ADAPTIVE OPTICAL SYSTEMS TECHNOLOGY, PTS 1 AND 2, 2000, 4007 : 72 - 81
[7] Ground-based coronagraphy with high-order adaptive optics
Sivaramakrishnan, A
Koresko, CD
Makidon, RB
Berkefeld, T
Kuchner, MJ
[J]. ASTROPHYSICAL JOURNAL, 2001, 552 (01) : 397 - 408

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