Developing arrayed waveguide grating spectrographs for multi-object astronomical spectroscopy

被引:71
作者
Cvetojevic, Nick [1 ,2 ]
Jovanovic, Nemanja [1 ,2 ,3 ]
Lawrence, Jon [1 ,2 ,3 ]
Withford, Michael [1 ,2 ]
Bland-Hawthorn, Joss [4 ,5 ]
机构
[1] Macquarie Univ, Dept Phys & Astron, MQ Photon Res Ctr, N Ryde, NSW 2109, Australia
[2] Macquarie Univ, Ctr Astron Astrophys & Astrophoton, N Ryde, NSW 2109, Australia
[3] Anglo Australian Observ, Epping, NSW 2121, Australia
[4] Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia
[5] Univ Sydney, Sch Phys, Inst Photon & Opt Sci, Sydney, NSW 2006, Australia
关键词
FLAT SPECTRAL RESPONSE; PHOTONIC LANTERN; MULTIMODE; DESIGN; MULTIPLEXER; DEVICES; OPTICS;
D O I
10.1364/OE.20.002062
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
With the aim of utilizing arrayed waveguide gratings for multi-object spectroscopy in the field of astronomy, we outline several ways in which standard telecommunications grade chips should be modified. In particular, by removing the parabolic-horn taper or multimode interference coupler, and injecting with an optical fiber directly, the resolving power was increased threefold from 2400 +/- 200 (spectral resolution of 0.63 +/- 0.2 nm) to 7000 +/- 700 (0.22 +/- 0.02 nm) while attaining a throughput of 77 +/- 5%. More importantly, the removal of the taper enabled simultaneous off-axis injection from multiple fibers, significantly increasing the number of spectra that can be obtained at once (i.e. the observing efficiency). Here we report that similar to 12 fibers can be injected simultaneously within the free spectral range of our device, with a 20% reduction in resolving power for fibers placed at 0.8 mm off-centre. (C)2012 Optical Society of America
引用
收藏
页码:2062 / 2072
页数:11
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