Astronomical spectrograph calibration with broad-spectrum frequency combs

被引：126

作者：

Braje, D. A. ^{[1
]}

Kirchner, M. S. ^{[1
]}

Osterman, S. ^{[2
]}

Fortier, T. ^{[1
]}

Diddams, S. A. ^{[1
]}

机构：

[1] Natl Inst Stand & Technol, Div Time & Frequency, Boulder, CO 80305 USA

[2] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA

来源：

EUROPEAN PHYSICAL JOURNAL D | 2008年 / 48卷 / 01期

基金：

欧盟地平线“2020”;

关键词：

D O I：

10.1140/epjd/e2008-00099-9

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

Broadband femtosecond-laser frequency combs are filtered to spectrographically resolvable frequency-mode spacing, and limitations of using cavities for spectral filtering are considered. Data and theory are used to show implications relevant to spectrographic calibration of high-resolution, astronomical spectrometers.

引用

页码：57 / 66

页数：10

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