Abstract
We present a Bayesian technique, which uses a luminosity function prior, to calculate photometric redshifts for optically-obscured starburst galaxies. An example is compared with previous Monte Carlo simulations.
Partial funding for this work was provided by NSERC grant PGSB-253705-2002, CONACyT grants 39953-F and 39548-F, INAOE, and the conference local organizing committee.
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References
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© 2004 Kluwer Academic Publishers
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Chapin, E.L., Hughes, D.H., Aretxaga, I. (2004). A Bayesian Photometric Redshift Technique for Mm-Selected Galaxies. In: Plionis, M. (eds) Multiwavelength Cosmology. Astrophysics and Space Science Library, vol 301. Springer, Dordrecht. https://doi.org/10.1007/0-306-48570-2_25
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DOI: https://doi.org/10.1007/0-306-48570-2_25
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-1971-5
Online ISBN: 978-0-306-48570-1
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