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A Mass Model for the Lensing Cluster SDSS J1004+4112: Constraints from the Third Time Delay

  • Authors: R. Forés-Toribio, J. A. Muñoz, C. S. Kochanek, E. Mediavilla

R. Forés-Toribio et al 2022 The Astrophysical Journal 937 .

  • Provider: AAS Journals

Caption: Figure 1.

χ 2 contours and profiles for the virial mass, concentration, and inner slope parameters of the generalized NFW model (Equation (1)). Red lines and points mark the values for which the χ 2 is minimized, orange lines delimiter the 1σ contours, and green lines the 2σ contours. The black (gray) shadow is the 1σ (2σ) region.

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