The search for extrasolar giant planets using integral field spectroscopy: Simulations

被引：1

作者：

Berton, A ^{[1
]}

Feldt, M

Gratton, R

Hippler, S

Henning, T

机构：

[1] Max Planck Inst Astron, D-69117 Heidelberg, Germany

[2] Osserv Astron Padova, INAF, I-35122 Padua, Italy

来源：

NEW ASTRONOMY REVIEWS | 2006年 / 49卷 / 10-12期

关键词：

extrasolar planets; simulations; adaptive optics; integral field spectroscopy;

D O I：

10.1016/j.newar.2005.10.021

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present here simulations of extrasolar planets detections obtained using a combination of extreme adaptive optics and integral field spectroscopy. The simulation code, written for IDL, provides images and, in particular, spectra, taking into account realistic Speckle Noise, AO correction effects and specific instrumental features. A detailed study has been done for ESO VLT telescopes (8.2 m), within the Phase A of the CHEOPS project, but the code is particularly flexible and can be updated for larger telescope diameters (ELTs) in order to give a realistic estimate of the detection limits, for giant telescopes, in standard conditions of seeing. (c) 2005 Elsevier B.V. All rights reserved.

引用

页码：661 / 669

页数：9

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