A new method for classifying galaxy SEDs from multiwavelength photometry

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A new method for classifying galaxy SEDs from multiwavelength photometry

We present a new method to classify the broad-band optical–near-infrared spectral energy distributions (SEDs) of galaxies using three shape parameters (super-colours) based on a principal component analysis of model SEDs. As well as providing a compact representation of the wide variety of SED shape...

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Bibliographic Details
Main Authors:	Wild, Vivienne, Almaini, Omar, Cirasuolo, Michele, Dunlop, Jim, McLure, Ross, Bowler, Rebecca, Ferreira, Joao, Bradshaw, Emma, Chuter, Robert, Hartley, Will
Format:	Article
Published:	Oxford University Press 2014
Online Access:	https://eprints.nottingham.ac.uk/47056/

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