Data reduction for the MATISSE instrument

被引：2

作者：

Millour, F. ^{[1
]}

Berio, P. ^{[1
]}

Heininger, M. ^{[2
]}

Hofmann, K. -H. ^{[2
]}

Schertl, D. ^{[2
]}

Weigelt, G. ^{[2
]}

Guitton, F. ^{[1
]}

Jaffe, W. ^{[3
]}

Beckmann, U. ^{[2
]}

Petrov, R. ^{[1
]}

Allouche, F. ^{[1
]}

Robbe-Dubois, S. ^{[1
]}

Lagarde, S. ^{[1
]}

Soulain, A. ^{[1
]}

Meilland, A. ^{[1
]}

Matter, A. ^{[1
]}

Cruzalebes, P. ^{[1
]}

Lopez, B. ^{[1
]}

机构：

[1] Univ Cote Azur, CNRS, OCA, Lagrange, France

[2] Max Planck Inst Radioastron, Bonn, Germany

[3] Huygens Lab, Leiden, Netherlands

来源：

OPTICAL AND INFRARED INTERFEROMETRY AND IMAGING V | 2016年 / 9907卷

关键词：

ATISSE; Interferometry; Data Reduction Software; REFRACTIVE-INDEX; INTERFEROMETRY; AMBER/VLTI; AIR;

D O I：

10.1117/12.2232283

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

We present in this paper the general formalism and data processing steps used in the MATISSE data reduction software, as it has been developed by the MATISSE consortium. The MATISSE instrument is the mid-infrared new generation interferometric instrument of the Very Large Telescope Interferometer (VLTI). It is a 2-in-1 instrument with 2 cryostats and 2 detectors: one 2k x 2k Rockwell Hawaii 2RG detector for L&M-bands, and one 1k x 1k Raytheon Aquarius detector for N-band, both read at high framerates, up to 30 frames per second. MATISSE is undergoing its first tests in laboratory today.

引用

页数：14

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