redMaGiC: Selecting luminous red galaxies from the DES Science Verification data
- Univ. of Arizona, Tucson, AZ (United States)
- Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Univ. Autonoma de Barcelona, Barcelona (Spain)
- Institut de Ciencies de l'Espai, Barcelona (Spain)
- Stanford Univ., Stanford, CA (United States); ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), Redfern, NSW (Australia); Univ. of Queensland (Australia)
- Ludwig-Maximilians Univ. Munchen, Munchen (Germany)
- Univ. College London, London (United Kingdom)
- National Optical Astronomy Observatory, La Serena (Chile)
- Univ. of Cambridge, Cambridge (United Kingdom)
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Institut d'Astrophysique de Paris, Paris (France)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Univ. of Portsmouth, Portsmouth (United Kingdom)
- Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Observatorio Nacional, Rio de Janeiro (Brazil)
- Univ. of Notre Dame, Notre Dame, IN (United States)
- Univ. of Illinois, Urbana, IL (United States); National Center for Supercomputing Applications, Urbana, IL (United States)
- Univ. Autonoma de Barcelona, Barcelona (Spain); Institut de Ciencies de l'Espai, Barcelona (Spain)
- Australian National Univ., Canberra, ACT (Australia)
- Stanford Univ., Stanford, CA (United States)
- Stanford Univ., Stanford, CA (United States); ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), Redfern, NSW (Australia); Univ. of Queensland, Queensland (Australia)
- Texas A & M Univ., College Station, TX (United States)
- Excellence Cluster Universe, Garching (Germany); Ludwig-Maximilians Univ., Munich (Germany)
- Ludwig-Maximilians Univ. Munchen, Munchen (Germany); Excellence Cluster Universe, Garching (Germany)
- Univ. of Pennsylvania, Philadelphia, PA (United States); California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Lab. Interinstitucional de e-Astonomia - LIneA, Rio de Janeiro (Brazil)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
- Swinburne Univ. of Technology (Australia)
- Ludwig-Maximilians Univ. Munchen, Munchen (Germany); Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
- The Ohio State Univ., Columbus, OH (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Australian Astronomical Observatory, North Ryde, NSW (Australia)
- ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), Redfern, NSW (Australia); Australian Astronomical Observatory, North Ryde, NSW (Australia)
- Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Univ. de Sao Paulo, Sao Paulo (Brazil)
- Univ. Autonoma de Barcelona, Barcelona (Spain); Institucio Catalana de Recerca i Estudis Avancats, Barcelona (Spain)
- Excellence Cluster Univ., Garching (Germany); Ludwig-Maximilians Univ., Munich (Germany); Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
- Univ. of Queensland, Queensland (Australia)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ. of Sussex, Brighton (United Kingdom)
- Centro de Investigaciones Energeticas Medioambientales y Tecnologicas (CIEMAT), Madrid (Spain)
- Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil)
- Univ. of Illinois, Urbana, IL (United States); Centro de Investigaciones Energeticas, Madrid (Spain)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil)
- National Center for Supercomputing Applications, Urbana, IL (United States)
- Univ. of Illinois, Urbana, IL (United States)
- ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), Redfern, NSW (Australia); Swineburne Univ. of Technology, VIC (Australia)
- Argonne National Lab. (ANL), Lemont, IL (United States)
Here, we introduce redMaGiC, an automated algorithm for selecting luminous red galaxies (LRGs). The algorithm was specifically developed to minimize photometric redshift uncertainties in photometric large-scale structure studies. redMaGiC achieves this by self-training the colour cuts necessary to produce a luminosity-thresholded LRG sample of constant comoving density. We demonstrate that redMaGiC photo-zs are very nearly as accurate as the best machine learning-based methods, yet they require minimal spectroscopic training, do not suffer from extrapolation biases, and are very nearly Gaussian. We apply our algorithm to Dark Energy Survey (DES) Science Verification (SV) data to produce a redMaGiC catalogue sampling the redshift range z ϵ [0.2, 0.8]. Our fiducial sample has a comoving space density of 10–3 (h–1 Mpc)–3, and a median photo-z bias (zspec – zphoto) and scatter (σz/(1 + z)) of 0.005 and 0.017, respectively. The corresponding 5σ outlier fraction is 1.4 per cent. We also test our algorithm with Sloan Digital Sky Survey Data Release 8 and Stripe 82 data, and discuss how spectroscopic training can be used to control photo-z biases at the 0.1 per cent level.
- Research Organization:
- Argonne National Lab. (ANL), Argonne, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), Basic Energy Sciences (BES); National Science Foundation (NSF); University of Chicago - Kavli Institute for Cosmological Physics; Ohio State University
- Grant/Contract Number:
- AC02-06CH11357
- OSTI ID:
- 1371551
- Journal Information:
- Monthly Notices of the Royal Astronomical Society, Vol. 461, Issue 2; ISSN 0035-8711
- Publisher:
- Royal Astronomical SocietyCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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