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A 12.5 GHz-spaced optical frequency comb spanning >400 nm for near-infrared astronomical spectrograph calibration

机译:间隔> 400 nm的12.5 GHz间隔光频率梳,用于近红外天文光谱仪校准

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A 12.5 GHz-spaced optical frequency comb locked to a global positioning system disciplined oscillator for near-infrared (IR) spectrograph calibration is presented. The comb is generated via filtering a 250 MHz-spaced comb. Subsequent nonlinear broadening of the 12.5 GHz comb extends the wavelength range to cover 1380–1820 nm, providing complete coverage over the H-band transmission window of earth’s atmosphere. Finite suppression of spurious sidemodes, optical linewidth, and instability of the comb has been examined to estimate potential wavelength biases in spectrograph calibration. Sidemode suppression varies between 20 and 45 dB, and the optical linewidth is ∼350 kHz at 1550 nm. The comb frequency uncertainty is bounded by ±30 kHz (corresponding to a radial velocity of ±5 cm/s), limited by the global positioning system disciplined oscillator reference. These results indicate that this comb can readily support radial velocity measurements below 1 m/s in the near IR.
机译:提出了一个12.5 GHz间隔的光频率梳,该梳被锁定到全球定位系统自律振荡器上,用于近红外(IR)光谱仪校准。该梳是通过对250 MHz间隔的梳进行滤波而生成的。随后12.5 GHz梳状线的非线性加宽将波长范围扩展到了1380–1820 nm,从而完全覆盖了地球大气层的H波段传输窗口。已经检查了杂散副模,光学线宽和梳子的不稳定性的有限抑制,以估计光谱仪校准中的潜在波长偏差。旁模抑制在20至45 dB之间变化,并且在1550 nm处的光学线宽约为350 kHz。梳齿频率的不确定度以±30 kHz为界(对应于±5 cm / s的径向速度),受全局定位系统约束的振荡器参考限制。这些结果表明,这种梳子可以很容易地支持近红外下低于1 m / s的径向速度测量。

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