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diff --git a/cuda/2d/fbp.h b/cuda/2d/fbp.h
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+/*
+-----------------------------------------------------------------------
+Copyright: 2010-2015, iMinds-Vision Lab, University of Antwerp
+           2014-2015, CWI, Amsterdam
+
+Contact: astra@uantwerpen.be
+Website: http://sf.net/projects/astra-toolbox
+
+This file is part of the ASTRA Toolbox.
+
+
+The ASTRA Toolbox is free software: you can redistribute it and/or modify
+it under the terms of the GNU General Public License as published by
+the Free Software Foundation, either version 3 of the License, or
+(at your option) any later version.
+
+The ASTRA Toolbox is distributed in the hope that it will be useful,
+but WITHOUT ANY WARRANTY; without even the implied warranty of
+MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
+GNU General Public License for more details.
+
+You should have received a copy of the GNU General Public License
+along with the ASTRA Toolbox. If not, see <http://www.gnu.org/licenses/>.
+
+-----------------------------------------------------------------------
+$Id$
+*/
+
+#include "algo.h"
+#include "fbp_filters.h"
+
+namespace astraCUDA {
+
+class _AstraExport FBP : public ReconAlgo {
+public:
+	FBP();
+	~FBP();
+
+	virtual bool useSinogramMask() { return false; }
+	virtual bool useVolumeMask() { return false; }
+
+	// Returns the required size of a filter in the fourier domain
+	// when multiplying it with the fft of the projection data.
+	// Its value is equal to the smallest power of two larger than
+	// or equal to twice the number of detectors in the spatial domain.
+	//
+	// _iDetectorCount is the number of detectors in the spatial domain.
+	static int calcFourierFilterSize(int _iDetectorCount);
+
+	// Sets the filter type. Some filter types require the user to supply an
+	// array containing the filter.
+	// The number of elements in a filter in the fourier domain should be equal
+	// to the value returned by calcFourierFilterSize().
+	// The following types require a filter:
+	//
+	// - FILTER_PROJECTION:
+	// The filter size should be equal to the output of
+	// calcFourierFilterSize(). The filtered sinogram is
+	// multiplied with the supplied filter.
+	//
+	// - FILTER_SINOGRAM:
+	// Same as FILTER_PROJECTION, but now the filter should contain a row for
+	// every projection direction.
+	//
+	// - FILTER_RPROJECTION:
+	// The filter should now contain one kernel (= ifft of filter), with the
+	// peak in the center. The filter width
+	// can be any value. If odd, the peak is assumed to be in the center, if
+	// even, it is assumed to be at floor(filter-width/2).
+	//
+	// - FILTER_RSINOGRAM
+	// Same as FILTER_RPROJECTION, but now the supplied filter should contain a
+	// row for every projection direction.
+	//
+	// A large number of other filters (FILTER_RAMLAK, FILTER_SHEPPLOGAN,
+	// FILTER_COSINE, FILTER_HAMMING, and FILTER_HANN)
+	// have a D variable, which gives the cutoff point in the frequency domain.
+	// Setting this value to 1.0 will include the whole filter
+	bool setFilter(astra::E_FBPFILTER _eFilter,
+                   const float * _pfHostFilter = NULL,
+                   int _iFilterWidth = 0, float _fD = 1.0f, float _fFilterParameter = -1.0f);
+
+	bool setShortScan(bool ss) { m_bShortScan = ss; return true; }
+
+	virtual bool init();
+
+	virtual bool iterate(unsigned int iterations);
+
+	virtual float computeDiffNorm() { return 0.0f; } // TODO
+
+protected:
+	void reset();
+
+	void* D_filter; // cufftComplex*
+	bool m_bShortScan;
+};
+
+}