The third version of the AMBER data reduction software.

被引：0

作者：

Malbet, Fabien ^{[1
]}

Duvert, Gilles ^{[1
]}

Millour, Florentin ^{[2
]}

Le Bouquin, Jean-Baptiste ^{[1
]}

Mella, Guillaume ^{[1
]}

Halipre, Luc ^{[1
]}

Chelli, Alain ^{[1
]}

Lafrasse, Sylvain ^{[1
]}

Altariba, Evelyne ^{[1
]}

Zins, Gerard ^{[1
]}

机构：

[1] Univ Grenoble 1, UMR 5571, Lab Astrophys Grenoble LAOG, CNRS, BP 53, F-38051 Grenoble 9, France

[2] Max Planck Inst Radioastron, D-53121 Bonn, Germany

来源：

OPTICAL AND INFRARED INTERFEROMETRY II | 2010年 / 7734卷

关键词：

AMBER Instrument; Data Reduction; Visibility Calibration; Optical Interferometry; Multiaxial Recombination; Transfer Function; CALIBRATOR STARS; CATALOG;

D O I：

10.1117/12.857527

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

We present the third release of the AMBER data reduction software by the JMMC. This software is based on core algorithms optimized after several years of operation. An optional graphic interface in a high level language allows the user to control the process step by step or in a completely automatic manner. Ongoing improvement is the implementation of a robust calibration scheme, making use of the full calibration sets available during the night. The output products are standard OI-FITS files, which can be used directly in high level software like model fitting or image reconstruction tools. The software performances are illustrated on a full data set of calibrators observed with AMBER during 5 years taken in various instrumental setup.

引用

页数：12

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