4.7 Article

MegaMorph - multiwavelength measurement of galaxy structure. Sersic profile fits to galaxies near and far

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stt1320

关键词

methods: data analysis; techniques: image processing; galaxies: fundamental parameters; galaxies: photometry; galaxies: structure

资金

  1. NPRP grant Qatar National Research Fund [08-643-1-112]
  2. NPRP grant
  3. STFC Advanced Fellowship
  4. Alfred P. Sloan Foundation
  5. National Science Foundation
  6. US Department of Energy
  7. National Aeronautics and Space Administration
  8. Japanese Monbukagakusho
  9. Max Planck Society
  10. Higher Education Funding Council for England
  11. American Museum of Natural History
  12. Astrophysical Institute Potsdam
  13. University of Basel
  14. University of Cambridge
  15. Case-Western Reserve University
  16. University of Chicago
  17. Drexel University
  18. Fermilab
  19. Institute for Advanced Study
  20. Johns Hopkins University
  21. Joint Institute for Nuclear Astrophysics
  22. Kavli Institute for Particle Astrophysics and Cosmology
  23. Chinese Academy of Sciences (LAMOST)
  24. Los Alamos National Laboratory
  25. Max-Planck-Institute for Astronomy (MPIA)
  26. Max-Planck-Institute for Astrophysics (MPA)
  27. New Mexico State University
  28. Ohio State University
  29. University of Pittsburgh
  30. University of Portsmouth
  31. Princeton University
  32. United States Naval Observatory
  33. University of Washington
  34. STFC [ST/H007156/1, ST/K00090X/1, ST/I001212/1] Funding Source: UKRI
  35. Science and Technology Facilities Council [ST/K00090X/1, ST/H007156/1, ST/I001212/1] Funding Source: researchfish

向作者/读者索取更多资源

We demonstrate a new multiwavelength technique for two-dimensional parametric modelling of galaxy surface-brightness profiles, which we have incorporated into the widely used software GALFIT. Our new method, named GALFITM, extends GALFIT3's current single-band fitting process by simultaneously using multiple images of the same galaxy to constrain a wavelength-dependent model. Each standard profile parameter may vary as a function of wavelength, with a user-definable degree of smoothness, from constant to fully free. The performance of GALFITM is evaluated by fitting elliptical Sersic profiles to ugriz imaging data for 4026 galaxies, comprising the original Sloan Digital Sky Survey (SDSS) imaging for 163 low-redshift (v less than or similar to 7000 km s(-1)) galaxies and 3863 artificially redshifted (0.01 less than or similar to z less than or similar to 0.25) images of the same galaxies. Comparing results from single-band and multiband techniques, we show that GALFITM significantly improves the extraction of information, particularly from bands with low signal-to-noise ratio (e. g. u and z SDSS bands) when combined with higher signal-to noise images. We also study systematic trends in the recovered parameters, particularly Sersic index, that appear when one performs measurements of the same galaxies at successively higher redshifts. We argue that it is vital that studies investigating the evolution of galaxy structure are careful to avoid or correct for these biases. The resulting multiband photometric structural parameters for our sample of 163 galaxies are provided. We demonstrate the importance of considering multiband measurements by showing that the Sersic indices of spiral galaxies increase to redder wavelengths, as expected for composite bulge-disc systems. Finally, for the ellipticals in our sample, which should be well represented by single-Sersic models, we compare our measured parameters to those from previous studies.

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