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arXiv 1605.09660astro-ph.IM
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FRIDA：用于GTC的衍射限制成像和积分场spectroscopy

FRIDA: diffraction-limited imaging and integral-field spectroscopy for the GTC

Alan M. Watson, José A. Acosta-Pulido, Luis C. Álvarez-Núñez, Vicente Bringas-Rico, Nicolás Cardiel, Salvador Cuevas, Oscar Chapa, José Javier Díaz García, Step… 展开作者

Alan M. Watson, José A. Acosta-Pulido, Luis C. Álvarez-Núñez, Vicente Bringas-Rico, Nicolás Cardiel, Salvador Cuevas, Oscar Chapa, José Javier Díaz García, Stephen S. Eikenberry, Carlos Espejo, Rubén A. Flores-Meza, Jorge Fuentes-Fernández, Jesús Gallego, José Leonardo Garcés Medina, Francisco Garzón López, Peter Hammersley, Carolina Keiman, Gerardo Lara, José Alberto López, Pablo L. López, Diana Lucero, Heidy Moreno Arce, Sergio Pascual Ramirez, Jesús Patrón Recio, Almudena Prieto, Alberto José Rodríguez, José Marco de la Rosa, Beatriz Sánchez, Jorge A. Uribe, Francisco Váldez Berriozabal

备注：
To appear in the proceedings of SPIE conference 9908 "Ground-based and Airborne Instrumentation for Astronomy VI". 8 pages
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摘要：

FRIDA是一个衍射限制成像仪和积分场光谱仪，正在为加那利大望远镜的自适应光学聚焦而建造。在成像模式下，FRIDA将提供0.010、0.020和0.040角秒/像素的标度，在IFS模式下，光谱分辨率为1500、4000和30，000。FRIDA正在开始系统集成，计划于2017年底在实验室完成完全集成的系统测试，并在此后不久交付给GTC。在这篇文章中，我们提出了一个总结，其设计，制造，目前的状况和潜在的科学应用。

英文摘要：

FRIDA is a diffraction-limited imager and integral-field spectrometer that is being built for the adaptive-optics focus of the Gran Telescopio Canarias. In imaging mode FRIDA will provide scales of 0.010, 0.020 and 0.040 arcsec/pixel and in IFS mode spectral resolutions of 1500, 4000 and 30,000. FRIDA is starting systems integration and is scheduled to complete fully integrated system tests at the laboratory by the end of 2017 and to be delivered to GTC shortly thereafter. In this contribution we present a summary of its design, fabrication, current status and potential scientific applications.

机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。

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