Adaptive spatial binning of integral-field spectroscopic data using voronoi tessellations
Feb, 200311 pages
Published in:
- Mon.Not.Roy.Astron.Soc. 342 (2003) 345
e-Print:
- astro-ph/0302262 [astro-ph]
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Abstract: (arXiv)
We present new techniques to perform adaptive spatial binning of Integral-Field Spectroscopic (IFS) data to reach a chosen constant signal-to-noise ratio per bin. These methods are required for the proper analysis of IFS observations, but can also be used for standard photometric imagery or any other two-dimensional data. Various schemes are tested and compared by binning and extracting the stellar kinematics of the Sa galaxy NGC2273 from spectra obtained with the panoramic IFS SAURON.- METHODS DATA ANALYSIS
- TECHNIQUES PHOTOMETRIC
- TECHNIQUES SPECTROSCOPIC
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