Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts obtained in the Hubble Deep Field with the Keck Telescope are presented. The best photometric redshift schemes predict spectroscopic redshifts with a redshift accuracy of Δz < 0.1 for more than 68% of sources and with Δz < 0.3 for 100%, when single-feature spectroscopic redshifts are removed from consideration. This test shows that photometric redshift schemes work well, at least when the photometric data are of high quality and when the sources are at moderate redshifts
Context. In the next decade, the Large Synoptic Survey Telescope (LSST) will become a major facility...
With the availability of the huge amounts of data produced by current and future large multiband pho...
We use the deepest and most complete redshift catalog currently available (the Hubble Deep Field (HD...
Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts o...
Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts o...
This article describes the various photometric techniques currently being used, including some preli...
We present a study of photometric redshift accuracy in the 3D-HST photometric catalogs, using 3D-HST...
International audienceWe tested the performance of photometric redshifts for galaxies in the Hubble ...
We tested the performance of photometric redshifts for galaxies in the Hubble Ultra Deep field down ...
International audienceSince more than 70 years ago, the colours of galaxies derived from flux measur...
The aim of this paper is to investigate ways to optimize the accuracy of photometric redshifts for a...
Received???; accepted??? Context. In the next decade, the Large Synoptic Survey Telescope (LSST) wil...
We discuss the construction of a photometric redshift catalogue of luminous red galaxies (LRGs) from...
We use numerical simulations to characterize the performance of a clustering-based method to calibra...
We present photometric redshifts for the COSMOS survey derived from a new code, optimized to yield a...
Context. In the next decade, the Large Synoptic Survey Telescope (LSST) will become a major facility...
With the availability of the huge amounts of data produced by current and future large multiband pho...
We use the deepest and most complete redshift catalog currently available (the Hubble Deep Field (HD...
Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts o...
Results of a blind test of photometric redshift predictions against spectroscopic galaxy redshifts o...
This article describes the various photometric techniques currently being used, including some preli...
We present a study of photometric redshift accuracy in the 3D-HST photometric catalogs, using 3D-HST...
International audienceWe tested the performance of photometric redshifts for galaxies in the Hubble ...
We tested the performance of photometric redshifts for galaxies in the Hubble Ultra Deep field down ...
International audienceSince more than 70 years ago, the colours of galaxies derived from flux measur...
The aim of this paper is to investigate ways to optimize the accuracy of photometric redshifts for a...
Received???; accepted??? Context. In the next decade, the Large Synoptic Survey Telescope (LSST) wil...
We discuss the construction of a photometric redshift catalogue of luminous red galaxies (LRGs) from...
We use numerical simulations to characterize the performance of a clustering-based method to calibra...
We present photometric redshifts for the COSMOS survey derived from a new code, optimized to yield a...
Context. In the next decade, the Large Synoptic Survey Telescope (LSST) will become a major facility...
With the availability of the huge amounts of data produced by current and future large multiband pho...
We use the deepest and most complete redshift catalog currently available (the Hubble Deep Field (HD...