Reducing Photometric Redshift Uncertainties Using Galaxy Clustering Information
In cosmology and astronomy, measuring the distances to galaxies is an important task. This is done by measuring the redshift of the spectra from these sources. Photometric redshifts are a quick way of estimating the true redshifts and are calculated using color band intensities. The errors on thes...
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| Language: | en_US |
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The University of Arizona.
2017
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| Online Access: | http://hdl.handle.net/10150/624981 http://arizona.openrepository.com/arizona/handle/10150/624981 |