Galaxy And Mass Assembly (GAMA): understanding the wavelength dependence of galaxy structure with bulge-disc decompositions
With a large sample of bright, low-redshift galaxies with optical–near-IR imaging from the GAMA survey we use bulge-disc decompositions to understand the wavelength-dependent behaviour of single-Sersic structural measurements. We denote the variation in single-Sersic index with wavelength as N, like...
| Main Authors: | , , , , , , , , , , , , , , , , |
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| Format: | Article |
| Published: |
Oxford University Press
2016
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| Subjects: | |
| Online Access: | https://eprints.nottingham.ac.uk/34950/ |