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SDSS IV MaNGA: stellar population gradients as a function of galaxy environment

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Figure

Figure 1. The left-hand plot shows a section of the SDSS footprint and the red circles highlight the positions of the observed MaNGA galaxies
Figure 2. An example early-type galaxy from the MaNGA survey (MaNGA ID 1-114998) that has been observed with the 61 fibre IFU
Figure 3. Distributions of stellar mass [log (M/M⊙)] for the four differentenvironmental bins that make up the sample used in this work
Figure 5. Light- and mass-weighted stellar population gradients in age (left-hand panels) and metallicity (right-hand panels) as a function of galaxy massfor different local environmental densities
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