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...
| Main Authors: | , , , , , , , , , |
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| Format: | Article |
| Published: |
Oxford University Press
2014
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| Online Access: | https://eprints.nottingham.ac.uk/47056/ |