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
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Tran, Kim-Vy H.; Saintonge, Amélie; Moustakas, John; Bai, Lei; Gonzalez, Anthony H.; Holden, Bradford P.; Zaritsky, Dennis; Kautsch, Stefan J. (2009). 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. The Astrophysical Journal. Available electronically from https : / /hdl .handle .net /1969 .1 /184254.