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Diffstat (limited to 'sci-astronomy/zebra/metadata.xml')
| -rw-r--r-- | sci-astronomy/zebra/metadata.xml | 30 |
1 files changed, 15 insertions, 15 deletions
diff --git a/sci-astronomy/zebra/metadata.xml b/sci-astronomy/zebra/metadata.xml index ba10176c2..b9760ac17 100644 --- a/sci-astronomy/zebra/metadata.xml +++ b/sci-astronomy/zebra/metadata.xml @@ -6,20 +6,20 @@ <name>Gentoo Astronomy Project</name> </maintainer> <longdescription lang="en"> - The Zurich Extragalactic Bayesian Redshift Analyzer is a software to - compute and analyze photometric redshifts of galaxies. - ZEBRA combines and extends several of the classical approaches to - produce accurate photometric redshifts down to faint magnitudes. In - particular, ZEBRA uses the template-fitting approach to produce - Maximum Likelihood and Bayesian redshift estimates based on: - * An automatic iterative technique to correct the original set of - galaxy templates to best represent the SEDs of real galaxies at - different redshifts; - * A training set of spectroscopic redshifts for a small fraction of - the photometric sample, to improve the robustness of the - photometric redshift estimates; and - * An iterative technique for Bayesian redshift estimates, which - extracts the full two-dimensional redshift and template likelihood - function for each galaxy. +The Zurich Extragalactic Bayesian Redshift Analyzer is a software to +compute and analyze photometric redshifts of galaxies. +ZEBRA combines and extends several of the classical approaches to +produce accurate photometric redshifts down to faint magnitudes. In +particular, ZEBRA uses the template-fitting approach to produce +Maximum Likelihood and Bayesian redshift estimates based on: +* An automatic iterative technique to correct the original set of +galaxy templates to best represent the SEDs of real galaxies at +different redshifts; +* A training set of spectroscopic redshifts for a small fraction of +the photometric sample, to improve the robustness of the +photometric redshift estimates; and +* An iterative technique for Bayesian redshift estimates, which +extracts the full two-dimensional redshift and template likelihood +function for each galaxy. </longdescription> </pkgmetadata> |