arXiv · astro-ph/0302262
Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations
Abstract
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.
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Michele Cappellari, Yannick Copin. 2003-02-13. Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations. https://doi.org/10.1046/j.1365-8711.2003.06541.x
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