Fig. 3 from MIPS J142824.0+352619: A Hyperluminous Starburst Galaxy at z = 1.325

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MIPS J142824.0+352619: A Hyperluminous Starburst Galaxy at z = 1.325

Authors: C. Borys, A. W. Blain, A. Dey, E. Le Floc'h, B. T. Jannuzi, V. Barnard, C. Bian, M. Brodwin, K. Menéndez-Delmestre, D. Thompson, K. Brand, M. J. I. Brown, C. D. Dowell, P. Eisenhardt, D. Farrah, D. T. Frayer, J. Higdon, S. Higdon, T. Phillips, B. T. Soifer, D. Stern, and D. Weedman

Borys et al. 2006 The Astrophysical Journal 636 134.

Provider: AAS Journals

Caption: Fig. 3.

SED of MIPS J142824.0+352619, shifted to the rest frame at ﹩z=1.325﹩. Overlaid on the MIPS+submillimeter points is the best‐fit graybody. The radio portion of the SED assumes a spectral index of 0.7, which is commonly used to describe starburst galaxies (Condon 1992). Squares and upper limits represent the rest‐frame SED of HR10.

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