Preserving Structure in Multi-wavelength Images of Extended Objects

Details Preserving Structure in Multi-wavelength Images of Extended Objects Preserving Structure in Multi-wavelength Images of Extended Objects

2011-01-09

arxiv.org/abs/1101.1679v1

Astronomy and Astrophysics

Astrophysics

Instrumentation and Methods for Astrophysics

22 pages, 11 figures

Scientific paper

A non-parametric smoothing method is presented that reduces noise in multi-wavelength imaging data sets. Using Principle Component Analysis (hereafter PCA) to associate pixels according to their $ugriz$-band colors, smoothing is done over pixels with a similar location in PCA space. This method smoothes over pixels with similar color, which reduces the amount of mixing of different colors within the smoothing region. The method is tested using a mock galaxy with signal-to-noise levels and color characteristics of SDSS data. When comparing this method to smoothing methods using a fixed radial profile or an adaptive radial profile, the chi^2-like statistic for the method presented here is smaller. The method shows a small dependence on input parameters. Running this method on SDSS data and fitting theoretical stellar population models to the smoothed data of the mock galaxy and SDSS data, shows that the method reduces scatter in the best-fit stellar population analysis parameters, when compared to cases where no smoothing is done. For an area centered on the star forming region of the mock galaxy, the median and standard deviation of the PCA-smoothed data is 7 Myr (+/- 3 Myr), as compared to 10 Myr (+/- 1 Myr) for a simple radial average, where the noise-free true value is 7.5 Myr (+/- 3.7 Myr).

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