Figure 5.
Upper panel: Hubble diagram for the 740 SNe Ia in the JLA compilation for different cosmological models: best-fitting ellipsoidal model (Ωm, Σ0, w, δ) ≃ (0.314, 0.001, −0.774, −0.008) (blue dashed line), and wCDM model (Ωm, w) ≃ (0.281, −0.750) (black line). Lower panel: residuals (distance modulus minus distance modulus for the wCDM model) for the same models in the upper panel.

Upper panel: Hubble diagram for the 740 SNe Ia in the JLA compilation for different cosmological models: best-fitting ellipsoidal model (Ωm, Σ0, w, δ) ≃ (0.314, 0.001, −0.774, −0.008) (blue dashed line), and wCDM model (Ωm, w) ≃ (0.281, −0.750) (black line). Lower panel: residuals (distance modulus minus distance modulus for the wCDM model) for the same models in the upper panel.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close