WHAT LIES BENEATH: USING p ( z ) TO REDUCE SYSTEMATIC PHOTOMETRIC REDSHIFT ERRORS
- 17 July 2009
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 700 (2) , L174-L177
- https://doi.org/10.1088/0004-637x/700/2/l174
Abstract
No abstract availableAll Related Versions
This publication has 12 references indexed in Scilit:
- Photometric Redshifts and Signal‐to‐Noise RatiosThe Astrophysical Journal, 2008
- Precision photometric redshift calibration for galaxy–galaxy weak lensingMonthly Notices of the Royal Astronomical Society, 2008
- On estimating redshift and luminosity distributions in photometric redshift surveysMonthly Notices of the Royal Astronomical Society, 2007
- Effects of Photometric Redshift Uncertainties on Weak‐Lensing TomographyThe Astrophysical Journal, 2006
- Error analysis of the photometric redshift techniqueMonthly Notices of the Royal Astronomical Society, 2002
- Bayesian Photometric Redshift EstimationThe Astrophysical Journal, 2000
- A Maximum Likelihood Method to Improve Faint‐Source Flux and Color EstimatesPublications of the Astronomical Society of the Pacific, 1998
- A Blind Test of Photometric Redshift PredictionThe Astronomical Journal, 1998
- Slicing Through Multicolor Space: Galaxy Redshifts from Broadband PhotometryThe Astronomical Journal, 1995
- On a Formula for Correcting Statistics for the Effects of a known Probable Error of ObservationMonthly Notices of the Royal Astronomical Society, 1913