MEGARA: THE NEW MULTI-OBJECT AND INTEGRAL FIELD SPECTROGRAPH FOR GTC

被引：0

作者：

Carrasco, E. ^{[1
]}

Paez, G. ^{[2
]}

Izazaga-Perez, R. ^{[1
]}

de Paz, A. Gil ^{[3
]}

Gallego, J. ^{[3
]}

Iglesias-Paramo, J. ^{[4
]}

机构：

[1] Inst Nacl Astrofis Opt & Electr, Luis Enrique Erro 1, Puebla 72840, Mexico

[2] Ctr Invest Opt, Loma Bosque 115, Guanajuato 37150, Mexico

[3] Univ Complutense Madrid, Ave Complutense S-N, E-28040 Madrid, Spain

[4] Inst Astrofis Andalucia CSIC, Glorieta Astron S-N, Granada 18008, Spain

来源：

XV LATIN AMERICAN REGIONAL IAU MEETING, 2016 | 2017年 / 49卷

关键词：

instrumentation:; spectrographs;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

MEGARA is an optical integral-field unit and multi-object spectrograph for the 10.4m Gran Telescopio Canarias. Both observational modes will provide identical spectral resolutions R-fwhm similar to 6,000, 12,000 and 18,700. The spectrograph is a collimator-camera system. The unique characteristics of MEGARA in terms of throughput and versatility make this instrument the most efficient tool to date to analyze astrophysical objects at intermediate spectral resolutions. The instrument is currently at the telescope for on-sky commissioning. Here we describe the as-built main characteristics the instrument.

引用

页码：39 / 40

页数：2

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