//# SpectralElement.h: Describes (a set of related) spectral lines //# Copyright (C) 2001,2003,2004 //# Associated Universities, Inc. Washington DC, USA. //# //# This library is free software; you can redistribute it and/or modify it //# under the terms of the GNU Library General Public License as published by //# the Free Software Foundation; either version 2 of the License, or (at your //# option) any later version. //# //# This library 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 Library General Public //# License for more details. //# //# You should have received a copy of the GNU Library General Public License //# along with this library; if not, write to the Free Software Foundation, //# Inc., 675 Massachusetts Ave, Cambridge, MA 02139, USA. //# //# Correspondence concerning AIPS++ should be addressed as follows: //# Internet email: aips2-request@nrao.edu. //# Postal address: AIPS++ Project Office //# National Radio Astronomy Observatory //# 520 Edgemont Road //# Charlottesville, VA 22903-2475 USA //# //# //# $Id: SpectralElement.h 20652 2009-07-06 05:04:32Z Malte.Marquarding $ #ifndef COMPONENTS_LOGTRANSFORMEDPOLYNOMIALSPECTRALELEMENT_H #define COMPONENTS_LOGTRANSFORMEDPOLYNOMIALSPECTRALELEMENT_H #include namespace casa { //# NAMESPACE CASA - BEGIN // // Describes the often used for determining spectral index plus higher order terms: // y = log (S_x) = ln(c_0) + c_1*ln(x) + c_2*ln(x)**2 + c_3*ln(x)**3 + ... // where c_1 is the traditional spectral index (alpha). // // // // // //
  • SpectralElement module // // // // From power law, logarithm, and polynomial and spectral line and element // // // // Describes a function that can be used to fit for spectral index and higher order terms. // The implementation simply subclasses PolynomialSpectralElement since that's all this function // really is, whicht the exception the the lhs is ln(y) not y. This means it's the fitter // configurator's responsibility to pass in the ln of the actual ordinate values and the ln // of the abscissa values, not the ordinate and abscissa values themselves. Essentially, this // class differs from PolynomialSpectralElement in its type and its stream operator. // // // // // // // To have a spectral element representing a spectral index function. // class LogTransformedPolynomialSpectralElement: public PolynomialSpectralElement { public: // Constructor. The n coefficients c_i to be solved for are // c_0 + c_1 * ln(x) + c_2 * ln(x)**2 + c_3 * ln(x)**3 + ... c_(n-1)*ln(x)**(n-1) // where x = nu/nu0. order is the polynomial, so the actual // function will have order+1 coefficients explicit LogTransformedPolynomialSpectralElement(uInt order); // Construct with the given parameters. See above constructor for // order in which the parameters should be supplied. LogTransformedPolynomialSpectralElement(const Vector ¶m); // Copy constructor (deep copy) LogTransformedPolynomialSpectralElement(const LogTransformedPolynomialSpectralElement &other); ~LogTransformedPolynomialSpectralElement(); LogTransformedPolynomialSpectralElement &operator=( const LogTransformedPolynomialSpectralElement& other ); SpectralElement* clone() const; }; ostream &operator<<( ostream &os, const LogTransformedPolynomialSpectralElement &elem ); } //# NAMESPACE CASA - END #endif