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Calibration of an echelle spectrograph with an astro-comb: a laser frequency comb with very high repetition rate

机译:用天体梳校准阶梯光谱仪:具有很高重复率的激光频率梳

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Searches for extrasolar planets using precision radial velocity (PRV) techniques are approaching Earth-like planet sensitivity, however require an improvement of one order of magnitude to identify earth-mass planets in the habitable zone of sun-like stars. A key limitation is spectrograph calibration. An astro-comb, an octave-spanning laser frequency comb and a Fabry-Pérot cavity, producing evenly spaced frequencies with large wavelength coverage, is a promising tool for improved wavelength calibration. We demonstrate the calibration of a high-resolution astrophysical spectrograph below the 1 m/s level in the 8000-9000 Å and 4200 Å spectral bands.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:使用精密径向速度(PRV)技术寻找太阳系外行星的方法正接近类地行星的灵敏度,但是,需要将识别太阳类恒星的宜居地带中的行星质量提高一个数量级。关键限制是光谱仪校准。 astrocomb,跨度为八度的激光频率梳和Fabry-Pérot腔可产生均匀间隔的频率并具有较大的波长覆盖范围,是改善波长校准的有前途的工具。我们在8000-9000&Aring中演示了1 m / s以下的高分辨率天体光谱仪的校准。和4200Å光谱带。©(2012)版权所有。摘要的下载仅允许个人使用。

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