A spectroscopically confirmed excess of 24 μm sources in a super galaxy group at z = 0.37: Enhanced dusty star formation relative to the cluster and field environment

Kim Vy H. Tran, Amélie Saintonge, John Moustakas, Lei Bai, Anthony H. Gonzalez, Bradford P. Holden, Dennis Zaritsky, Stefan J. Kautsch

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