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The Yuan Tseh Lee Array (YTLA, formerly AMiBA)

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Combined with Subaru weak lensing measurements, the AMiBA SZE data can be used to derive gas mass fraction as a function of cluster radius

Image Credit: ASIAA

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$Combined with Subaru weak lensing measurements, the AMiBA SZE data can be used to derive gas mass fraction as a function of cluster radius$

Combined with Subaru weak lensing measurements, the AMiBA SZE data can be used to derive gas mass fraction as a function of cluster radius (Umetsu et al., 2009, ApJ, 694, 1643).