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PRL Advanced Radial-velocity All-sky Search : ウィキペディア英語版 | PRL Advanced Radial-velocity All-sky Search PARAS〔(First Light results from PARAS: The PRL Echelle Spectrograph ), Abhijit Chakraborty et al., 2010.〕 is a ground based extrasolar planet search device. Based at 1.2m telescope is located at Mt. Abu, India.The project is funded by Physical Research Laboratory, India. The spectrograph works at a resolution of 67000. With the help of simultaneous calibration technique, PARAS has achieved an RV accuracy of 1.3 m/s for bright sun like quiet stars. Thorium-Argon lamp is used for calibration. New calibration techniques are also being explored by the project team. PARAS can detect planet in the habitable zone around M type stars. ==References==
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「PRL Advanced Radial-velocity All-sky Search」の詳細全文を読む
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