AMBER on the VLTI: Data processing and calibration issues

被引：4

作者：

Millour, F. ^{[1
]}

Petrov, R. ^{[2
]}

Malbet, F.

Tatulli, E. ^{[4
]}

Duvert, G. ^{[3
]}

Zins, G. ^{[3
]}

Altariba, E. ^{[3
]}

Vannier, M. ^{[5
]}

Hernandez, O. ^{[3
]}

Causi, G. Li ^{[6
]}

机构：

[1] Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany

[2] Lab Univ Astrophys Nice, F-06108 Nice, France

[3] Lab AstrOphys Grenoble, F-38400 Grenoble, France

[4] Osservatorio Arcetr, I-50125 Florence, Italy

[5] ESO, Santiago, Chile

[6] Rome Astro Observ, I-00040 Rome, Italy

来源：

THE 2007 ESO INSTRUMENT CALIBRATION WORKSHOP | 2008年

关键词：

D O I：

10.1007/978-3-540-76963-7_63

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：461 / +

页数：3

共 50 条

[1] AMBER data structure, processing and calibration
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[J]. INTERFEROMETRY IN OPTICAL ASTRONOMY, PTS 1 AND 2, 2000, 4006 : 261 - 268
[2] Optimised data reduction for the AMBER/VLTI instrument
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[3] Color-differential interferometry with AMBER/VLTI.: Data processing and precision from early observations
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[4] Detecting Jupiters with AMBER on the VLTI
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Mege, P.
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Bresson, Y.
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[J]. ASTRONOMY & ASTROPHYSICS, 2007, 464 (01) : 29 - 42
[7] Interferometric data reduction with AMBER/VLTI. Principle, estimators, and illustration
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[J]. INTERFEROMETRY FOR OPTICAL ASTRONOMY II, PTS 1 AND 2, 2003, 4838 : 1163 - 1170

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