Zusammenfassung
We present a method to infer the redshift distribution of an arbitrary
dataset based on spatial cross-correlation with a reference population and we
apply it to various datasets across the electromagnetic spectrum. Our approach
advocates the use of clustering measurements on all available scales, in
constrast to previous works focusing only on linear scales. We apply this
technique to infer the redshift distributions of luminous red galaxies and
emission line galaxies from the SDSS, infrared sources from WISE and radio
sources from FIRST. We show that consistent redshift distributions are found
using both quasars and absorber systems as reference populations. This
technique promises to be widely applicable to existing and upcoming sky
surveys. It provides us with the invaluable ability to deproject the inherently
2D observations of the extragalactic sky.
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