Image Details
Caption: Figure 16.
Left: 870 μm LABOCA flux density as a function of 1.4 mm SPT flux density for the 26 sources discussed in this paper (red) compared to the full sample of SPT sources which have been observed with LABOCA and Herschel-SPIRE (black). Right: same as to the left but with 350 μm Herschel-SPIRE flux density as a function of 870 μm LABOCA flux density.
© 2013. The American Astronomical Society. All rights reserved.