期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 433, 期 2, 页码 1344-1361出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stt822
关键词
methods: data analysis; methods: numerical; galaxies: evolution; galaxies: fundamental parameters; galaxies: photometry; galaxies: structure
资金
- NASA [ADP/NNX09AD02G, NSF/0908242]
- Alfred P. Sloan Foundation
- National Science Foundation
- US Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council for England
- American Museum of Natural History
- Astrophysical Institute Potsdam
- University of Basel
- University of Cambridge
- Case Western Reserve University
- University of Chicago
- Drexel University, Fermilab
- Institute for Advanced Study
- Japan Participation Group
- Johns Hopkins University
- Joint Institute for Nuclear Astrophysics
- Kavli Institute for Particle Astrophysics and Cosmology
- Korean Scientist Group
- Chinese Academy of Sciences (LAMOST)
- Los Alamos National Laboratory
- Max-Planck-Institute for Astronomy (MPIA)
- Max-Planck-Institute for Astrophysics (MPA)
- New Mexico State University
- Ohio State University
- University of Pittsburgh
- University of Portsmouth
- Princeton University
- United States Naval Observatory
- University of Washington
We present the results of fitting simulations of an unbiased sample of Sloan Digital Sky Survey (SDSS) galaxies utilizing the fitting routine galfit and analysis pipeline pymorph. These simulations are used to test the two-dimensional decompositions of SDSS galaxies. The simulations show that single Sersic models of SDSS data are recovered with Sigma(mag) approximate to 0.025 mag and Sigma(radius) approximate to 5 per cent. The global values (half-light radius and magnitude) are equally well constrained when a two-component model is used. Sub-components of two-component models present more scatter. SDSS resolution is the primary source of error in the recovery of models. We use a simple statistical correction of the biases in fitted parameters, providing an example using the Sersic index. Fitting a two-component Sersic + Exponential model to a single Sersic galaxy results in a noisier, but unbiased, recovery of the input parameters (Sigma(totalmag) approximate to 0.075 mag and Sigma(radius) approximate to 10 per cent); fitting a single Sersic profile to a two-component system results in biases of total magnitude and half-light radius of approximate to 0.05-0.10 mag and 5-10 per cent in radius. Using an F-test to select the best-fitting model from among the single- and two-component models is sufficient to remove this bias. We recommend fitting a two-component model to all galaxies when attempting to measure global parameters such as total magnitude and half-light radius.
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