Asmooth: a simple and efficient algorithm for adaptive kernel smoothing of two-dimensional imaging data

An efficient algorithm for adaptive kernel smoothing (AKS) of two-dimensional imaging data has been developed and implemented using the Interactive Data Language (idl). The functional form of the kernel can be varied (top-hat, Gaussian, etc.) to allow different weighting of the event counts registered within the smoothing region. For each individual pixel, the algorithm increases the smoothing scale until the signal-to-noise ratio (S/N) within the kernel reaches a pre-set value. Thus, noise is suppressed very efficiently, while at the same time real structure, that is, signal that is locally significant at the selected S/N level, is preserved on all scales. In particular, extended features in noise-dominated regions are visually enhanced. The asmooth algorithm differs from other AKS routines in that it allows a quantitative assessment of the goodness of the local signal estimation by producing adaptively smoothed images in which all pixel values share the same S/N above the background. We apply asmooth to both real observational data (an X-ray image of clusters of galaxies obtained with the Chandra X-ray Observatory) and to a simulated data set. We find the asmoothed images to be fair representations of the input data in the sense that the residuals are consistent with pure noise, that is, they possess Poissonian variance and a near-Gaussian distribution around a mean of zero, and are spatially uncorrelated.

[1]  THE WARPS SURVEY. III. THE DISCOVERY OF AN X-RAY LUMINOUS GALAXY CLUSTER AT z \ 0.833 AND THE IMPACT OF X-RAY SUBSTRUCTURE ON CLUSTER ABUNDANCE MEASUREMENTS , 1999, astro-ph/9905321.

[2]  P. Peebles,et al.  The Large-Scale Structure of the Universe , 1980 .

[3]  Galaxy and hot gas distributions in the z = 0.52 galaxy cluster RBS 380 from CHANDRA and NTT observations , 2003, astro-ph/0306499.

[4]  B. Silverman Density estimation for statistics and data analysis , 1986 .

[5]  R. Kraft,et al.  X-Ray Arc Structures in Chandra Images of NGC 5128 (Centaurus A) , 2002, astro-ph/0205493.

[6]  The Chandra Deep Field North Survey. IX. Extended X-Ray Sources* , 2001, astro-ph/0112002.

[7]  Robert K. Pina,et al.  INCORPORATION OF SPATIAL INFORMATION IN BAYESIAN IMAGE RECONSTRUCTION: THE MAXIMUM RESIDUAL LIKELIHOOD CRITERION , 1992 .

[8]  Harald Ebeling Improved approximations of Poissonian errors for high confidence levels , 2003 .

[9]  Discovery of a Large-Scale Filament Connected to the Massive Galaxy Cluster MACS J0717.5+3745 at z = 0.55* ** ** * , 2004, astro-ph/0406049.

[10]  M. Donahue,et al.  Chandra X-Ray Observatory Observation of the High-Redshift Cluster MS 1054–0321 , 2001, astro-ph/0107314.

[11]  Y. Lacasse,et al.  From the authors , 2005, European Respiratory Journal.

[12]  C. D. Kemp,et al.  Density Estimation for Statistics and Data Analysis , 1987 .

[13]  K. Weaver,et al.  Discovery of Bright Variable X-Ray Sources in NGC 1569 with Chandra , 2003, astro-ph/0305499.

[14]  Jean-Luc Starck,et al.  Structure Detection in Low Intensity X-Ray Images using the Wavelet Transfor M Applied to Galaxy Cluster Cores Analysis , 1997, astro-ph/9707305.

[15]  Astronomy,et al.  The Chandra view of NGC 1800 and the X‐ray scaling properties of dwarf starbursts , 2004, astro-ph/0407284.

[16]  Institute for Astronomy,et al.  Lensing Effects on the Protogalaxy Candidate cB58 and Their Implications for the Cosmological Constant , 1997, astro-ph/9703136.

[17]  A. Zezas,et al.  Chandra Observations of “The Antennae” Galaxies (NGC 4038/9) , 2001 .

[18]  A. C. Fabian,et al.  Adaptive binning of X-ray galaxy cluster images , 2000 .

[19]  W. Brandt,et al.  ROSAT PSPC and HRI observations of the composite starburst/Seyfert 2 galaxy NGC 1672 , 1995, astro-ph/9604162.

[20]  D. Merritt,et al.  NonParametric Estimation of Density Profiles , 1994 .

[21]  H Germany,et al.  XMM-Newton observations of three poor clusters: Similarity in dark matter and entropy profiles down to low mass , 2004, astro-ph/0406366.

[22]  Accepted for publication in The Astronomical Journal Observations of the core of the Pleiades with the Chandra X-ray Observatory , 2000 .

[23]  Michele Cappellari,et al.  Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations , 2003, astro-ph/0302262.