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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 Journal 148 107.

  • 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).

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