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os << "Fractional Bandwidth is " << fbw*100 << " %. Please check that (a) the flux variation across the chosen frequency range (" << startfreq << " Hz to " << endfreq << " Hz) is at least twice the single-channel noise-level, and (b) a " << ntaylor_p << "-term Taylor-polynomial fit across this frequency range is appropriate. " << LogIO::WARN << LogIO::POST; //# WBCleanImageSkyModel.cc: Implementation of WBCleanImageSkyModel class//# Copyright (C) 1996,1997,1998,1999,2000,2001,2002,2003//# 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//#//# $Id: WBCleanImageSkyModel.cc 13615 2010-12-20 14:04:00 UrvashiRV$//# v2.6 : Added psf-patch support to reduce memory footprint.