Fig. 1 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. 1.

Left: SHARC‐II 350 μm flux contours at [3.0, 3.5, 4.0, 4.5] σ overlaid on a ﹩30^{\prime \prime }\times 30^{\prime \prime }﹩ square NDWFS false‐color image of the field. Axes are aligned along cardinal directions, with north facing up. Bottom right: IRAC 3.6 μm image of a region around MIPS J142824.0+352619. Top right: Close‐up view of the I‐band image with VLA contours at [0.2, 0.3, 0.4] mJy levels. Although there at least three faint red sources in the vicinity of MIPS J142824.0+352619, the radio position clearly favors the central bright object.

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