Subaru conducts latest population census of galaxy clusters
The total stellar mass in a cluster, plotted on the y-axis, is found to be proportional to the total mass of the cluster (shown on the x-axis). What is more
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The metrology camera optics under tests in ASIAA
The metrology camera optics under tests in ASIAA
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The first color image (M31) of HSC_zoomed
The first color image (M31) of HSC. (Picture Credit: National Astronomical Observatory of Japan)
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Mass Distribution in and around the Galaxy Cluster MACS J1206.2-0847
Subaru BVRIz composite color images centered on the galaxy cluster MACS1206 (z=0.439), overlaid with mass contours from our joint strong-and-weak lensing analysis of HST and Subaru observations. The image size
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Lensing galaxy cluster CL0024+1654 (z=0.395)
Subaru BRZ pseudo color image of the central 3'x3' region of the galaxy cluster CL0024+1654 (taken and modified from Umetsu et al. 2010, arXiv:0908.0069).
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