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Magellan Planet Search Program
The Magellan Planet Search Program is a ground based extrasolar planet search device which began gathering data in December 2002. It utilizes the MIKE echelle spectrograph mounted on the Magellan Telescopes which are twin, 6.5m Magellan II (Clay) telescope located within the Las Campanas Observatory in Chile.〔
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== Specifications==
The MIKE echelle spectrograph works at a resolution of R ~ 50,000 when gathering spectra that covers a wavelength 3900 to 6200 Å. MIKE is divided into a red and blue CCD. The blue CCD captures stellar activities while the red CCD falls into a temperature controlled Iodine absorption cell is mounted in front of the MIKE entrance slit, this imprints iodine spectrum referencing directly to starlight.〔
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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