Application of Multicore Optical Fibers in Astronomy

被引:0
|
作者
Jovanovici, Nemanja [1 ,2 ]
Cuyon, Olivier [1 ,3 ,4 ,5 ]
Kawahara, Hajime [6 ,7 ]
Kotani, Takayuki [8 ]
机构
[1] NINS, Subaru Telescope, Natl Astron Observ Japan, 650 North AOhoku Pl, Hilo, HI 96720 USA
[2] Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia
[3] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[4] Univ Arizona, Coll Opt Sci, Tucson, AZ 85721 USA
[5] NINS, Astrobiol Ctr, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[6] Univ Tokyo, Dept Earth & Planetary Sci, Tokyo 1130033, Japan
[7] Univ Tokyo, Res Ctr Early Universe, Sch Sci, Tokyo, Japan
[8] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan
来源
2017 OPTICAL FIBER COMMUNICATIONS CONFERENCE AND EXHIBITION (OFC) | 2017年
关键词
PHOTONIC LANTERN; REDSHIFT SURVEY;
D O I
暂无
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
Multicore fibers are gaining growing attention in astronomy. The two main attributes which make them attractive for astronomy are that they reduce the distance between cores and hence have a superior fill factor to other approaches and they offer the possibility to transport light in many channels with the overhead of only having to handle a single fiber. These properties are being exploited to realize miniature integral field units that can transport light from different regions in a focal plane to a spectrograph for example. here we offer an overview of several applications where multicore fibers are now being considered and applied to astronomical observations to enhance scientific yield.
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页数:3
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