Galaxy And Mass Assembly (GAMA): the wavelength dependence of galaxy structure versus redshift and luminosity

We study how the sizes and radial profiles of galaxies vary with wavelength, by fitting Sersic functions simultaneously to imaging in nine optical and near-infrared bands. To quantify the wavelength dependence of effective radius we use the ratio, R, of measurements in two rest-frame bands. The depe...

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Bibliographic Details
Main Authors: Kennedy, Rebecca, Bamford, Steven P., Baldry, Ivan, Häußler, Boris, Holwerda, Benne W., Hopkins, Andrew M., Kelvin, Lee S., Lange, Rebecca, Moffett, Amanda J., Popescu, Cristina C., Taylor, Edward N., Tuffs, Richard J., Vika, Marina, Vulcani, Benedetta
Format: Article
Published: Oxford University Press 2015
Subjects:
Online Access:https://eprints.nottingham.ac.uk/34969/