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Mining the SDSS Archive. I. Photometric Redshifts in the Nearby Universe
- Publication Year :
- 2007
-
Abstract
- We present a supervised neural network approach to the determination of photometric redshifts. The method was tuned to match the characteristics of the Sloan Digital Sky Survey and it exploits the spectroscopic redshifts provided by this unique survey. In order to train, validate and test the networks we used two galaxy samples drawn from the SDSS spectroscopic dataset: the general galaxy sample (GG) and the luminous red galaxies subsample (LRG). The method consists of a two steps approach. In the first step, objects are classified in nearby (z<br />Comment: 45 pages, 14 figures, accepted for publication is the Astrophysical Journal
- Subjects :
- media_common.quotation_subject
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Table (information)
photometric redshift
galaxies
Range (statistics)
Astrophysics::Solar and Stellar Astrophysics
Galaxies: Photometry
Astrophysics::Galaxy Astrophysics
media_common
Physics
Astrophysics (astro-ph)
Sigma
Astronomy and Astrophysics
Redshift
Galaxy
Universe
Cosmology: Large-Scale Structure of Universe
Space and Planetary Science
Sky
Hidden layer
cosmology
Galaxies: Distances and Redshift
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....37404d2efed66beb69017b1a7a8a073f