Implementation of PhotoZ under Astro-WISE - A photometric redshift code for large datasets
arXiv:1110.1201 · doi:10.1007/s10686-011-9265-y
Abstract
We describe the implementation of the PhotoZ code in the framework of the Astro-WISE package and as part of the Photometric Classification Server of the PanSTARRS pipeline. Both systems allow the automatic measurement of photometric redshifts for the millions of objects being observed in the PanSTARRS project or expected to be observed by future surveys like KIDS, DES or EUCLID.
Accepted for publication in topical issue of Experimental Astronomy on Astro-WISE information system, references updated
References in corpus (12)
- The Seventh Data Release of the Sloan Digital Sky Survey
- Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
- ANNz: estimating photometric redshifts using artificial neural networks
- PHAT: PHoto-z Accuracy Testing
- Photometric Redshifts for the SDSS Early Data Release
- The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands
- Specific star formation rates to redshift 5 from the FORS Deep Field and the GOODS-S Field
- Photometric Redshifts of Galaxies in COSMOS
- Euclid Assessment Study Report for the ESA Cosmic Visions
- The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: II. The red bands
- Photometric redshifts and cluster tomography in the ESO Distant Cluster Survey
- A deep i-selected multi-waveband galaxy catalogue in the COSMOS field