Photospheric Magnitude Diagrams for Type II Supernovae: A Promising Tool to Compute Distances
Authors: Ósmar Rodríguez, Alejandro Clocchiatti, and Mario Hamuy
Rodríguez, Clocchiatti, & Hamuy
2014 The Astronomical Journal148107.
Provider: AAS Journals
Caption: Figure 5.
Comparison of AV obtained with the spectrum-fitting method and those obtained with the C3(BVI) method. Solid line represents the one-to-one relation. Open squares correspond to the outliers of the correlation. The shaded regions contain data within 1σ of the perfect correlation: using all SNe in our SN set (light gray region) and discarding the outliers (dark gray region).