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...

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Bibliographic Details
Main Authors: Kennedy, Rebecca, Bamford, Steven P., Häußler, Boris, Baldry, Ivan, Bremer, Malcolm, Brough, Sarah, Brown, Michael J.I., Driver, Simon, Duncan, Kenneth, Graham, Alister W., Holwerda, Benne W., Hopkins, Andrew M., Kelvin, Lee S., Lange, Rebecca, Phillipps, Steven, Vika, Marina, Vulcani, Benedetta
Format: Article
Published: Oxford University Press 2016
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Online Access:https://eprints.nottingham.ac.uk/34950/