Image Details
Caption: Figure 5.
1D probability distributions and 2D regions with the 1–﹩3\sigma ﹩ contours corresponding to the parameters ﹩{{{\Omega }}_{{\rm m}}}﹩, ﹩{{w}_{{\rm de}}}﹩, α, and Υ in the best-fit wCDM model, using the simulated sample with 240 SLSNe Ic, assuming ΛCDM as the background cosmology.
© 2015. The American Astronomical Society. All rights reserved.