Figure 2 from VLT/MUSE Observations of SDSS J1029+2623: Toward a High-precision Strong Lensing Model

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VLT/MUSE Observations of SDSS J1029+2623: Toward a High-precision Strong Lensing Model

Authors: Ana Acebron, Claudio Grillo, Pietro Bergamini, Amata Mercurio, Piero Rosati, Gabriel Bartosch Caminha, Paolo Tozzi, Gabriel B. Brammer, Massimo Meneghetti, Andrea Morelli, Mario Nonino, and Eros Vanzella

2022 The Astrophysical Journal 926 86.

Provider: AAS Journals

Caption: Figure 2.

Color–magnitude relation of SDSS1029 spectroscopic members (blue dots). Red dots mark the photometrically selected cluster members, according to the red sequence, and the magenta dots are the spectroscopic members with QF = 1. The best fit of the spectroscopic red sequence is indicated in black, and the dashed lines represent the 68% confidence limits.

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