2014/07/09 by M. Brescia, S. Cavuoti, G. Longo +1 · 1 citation
Physics and Astronomy · #Apparent magnitude #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Galaxy #Luminous infrared galaxy #Photometry (optics) #Red shift #Redshift #Sky #Stellar, planetary, and galactic studies #astro-ph.CO #astro-ph.IM #sort
paper · pdf · doi:10.1051/0004-6361/201424383
published as A&A 568, A126 (2014) · 10 pages, To appear on section 14 (Catalogs and data) of Astronomy and Astrophysics
arxiv created 2014/07/09 · openalex publication_date 2014/07/22 · arxiv updated 2014/09/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. Accurate photometric redshifts for large samples of galaxies are among the main products of modern multiband digital surveys. Over the last decade, the Sloan Digital Sky Survey (SDSS) has become a sort of benchmark against which to test the various methods.