Bayesian Photometric redshift estimation

Details Bayesian Photometric redshift estimation Bayesian Photometric redshift estimation

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.596b&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

Bayesian inference is applied to photometric redshift estimation. The
resulting method offers a significant improvement over existing
techniques. There is an excellent agreement between the ~100 1 < z
< 6 HDF spectroscopic redshifts and the predictions of this method,
with a rms error Delta z = 0.18 and no outliers.

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