The spatially resolved stellar population and ionized gas properties in the merger LIRG NGC 2623

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The spatially resolved stellar population and ionized gas properties in the merger LIRG NGC 2623 | Astronomy & Astrophysics (A&A)

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Volume 606 (October 2017)

A&A, 606 (2017) A95

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Fig. C.2

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Radial profile of M/L₅₆₃₅ derived from the ratio between μ_⋆ and L₅₆₃₅ (the luminosity measured at the normalized wavelength corrected by the stellar extinction) obtained for GM (black) and CB (grey) bases. M/L at the observed 1.6 μm and at the synthetic 1.6 μm are shown as dashed-red and solid-red lines, respectively.

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