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As qp shows, redshift posteriors and redshift density functions can be parameterized in many possible ways. chippr unfortunately was scoped out before I'd really thought about a catalog that might not use the piecewise constant parameterization of SDSS. KiDS has photo-z PDFs parameterized as Gaussians and wants n(z) with way more parameters than chippr can actually handle. This issue can be closed when:
chippr can accept Gaussian photo-z PDFs without forcing them onto a grid
chippr can yield n(z) in a different parameterization than the input photo-z PDFs
The text was updated successfully, but these errors were encountered:
As qp shows, redshift posteriors and redshift density functions can be parameterized in many possible ways.
chippr
unfortunately was scoped out before I'd really thought about a catalog that might not use the piecewise constant parameterization of SDSS. KiDS has photo-z PDFs parameterized as Gaussians and wants n(z) with way more parameters thanchippr
can actually handle. This issue can be closed when:chippr
can accept Gaussian photo-z PDFs without forcing them onto a gridchippr
can yield n(z) in a different parameterization than the input photo-z PDFsThe text was updated successfully, but these errors were encountered: