//#--------------------------------------------------------------------------- //# STFITSImageWriter.cc: Class to write out single dish spectra as FITS images //#--------------------------------------------------------------------------- //# Copyright (C) 2008 //# ATNF //# //# This program 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 2 of the License, or (at your option) //# any later version. //# //# This program 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 this program; if not, write to the Free Software Foundation, Inc., //# 675 Massachusetts Ave, Cambridge, MA 02139, USA. //# //# Correspondence concerning this software should be addressed as follows: //# Internet email: Malte.Marquarding@csiro.au //# Postal address: Malte Marquarding, //# Australia Telescope National Facility, //# P.O. Box 76, //# Epping, NSW, 2121, //# AUSTRALIA //# //# $Id: $ //#--------------------------------------------------------------------------- #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include #include //#include "STDefs.h" #include "STHeader.h" #include "Scantable.h" #include "STFITSImageWriter.h" using namespace casacore; using namespace asap; STFITSImageWriter::STFITSImageWriter() : isClass_(False) {;} STFITSImageWriter::~STFITSImageWriter() {;} Bool STFITSImageWriter::write(const Scantable& stable, const String& fileName) { // Get global Header from Table STHeader hdr = stable.getHeader(); // Column keywords Table tab = stable.table(); // Temps const Unit RAD(String("rad")); // Open and write header file String rootName(fileName); if (rootName.length()==0) rootName = String("fits"); ObsInfo oi; oi.setTelescope(String(hdr.antennaname)); oi.setObserver(String(hdr.observer)); uInt maxMem = 128; Bool preferVelocity = False; Bool opticalVelocity = False; Int bitPix = -32; // FLoating point Float minPix = 1.0; Float maxPix = -1.0; Bool overWrite = True; Bool degLast = False; Bool reallyVerbose = False; String errMsg; Block cols(5); cols[0] = String("SCANNO"); cols[1] = String("CYCLENO"); cols[2] = String("BEAMNO"); cols[3] = String("IFNO"); cols[4] = String("POLNO"); TableIterator iter(tab, cols); // Open data file while ( !iter.pastEnd() ) { Table t = iter.table(); ROTableRow row(t); const TableRecord& rec = row.get(0); String dirtype = stable.getDirectionRefString(); ostringstream onstr; if (rootName.length()==0) { rootName = "fits"; } if (tab.nrow() > 1) { if (stable.nscan() > 1) onstr << "_SCAN" << rec.asuInt("SCANNO"); if (stable.ncycle(rec.asuInt("SCANNO")) > 1) onstr << "_CYCLE" << rec.asuInt("CYCLENO"); if (stable.nbeam(rec.asuInt("SCANNO")) > 1) onstr << "_BEAM" << rec.asuInt("BEAMNO"); if (stable.nif(rec.asuInt("SCANNO")) > 1) onstr << "_IF" << rec.asuInt("IFNO"); if (stable.npol(rec.asuInt("SCANNO")) > 1) onstr << "_POL" << rec.asuInt("POLNO"); } String fileName = rootName + String(onstr) + String(".fits"); int row0 = t.rowNumbers(tab)[0]; const MPosition& mp = stable.getAntennaPosition(); const MDirection& md = stable.getDirection(row0); const MEpoch& me = stable.getEpoch(row0); oi.setObsDate(me); //const Double& rf = // stable.molecules().getRestFrequency(rec.asuInt("MOLECULE_ID") ); const std::vector& rf = stable.molecules().getRestFrequency(rec.asuInt("MOLECULE_ID") ); SpectralCoordinate sC = stable.frequencies().getSpectralCoordinate(md, mp, me, rf, rec.asuInt("FREQ_ID")); Int polno = rec.asuInt("POLNO"); Stokes::StokesTypes stokes = Stokes::type(stable.getPolarizationLabel(polno, stable.getPolType())); Vector whichStokes(1); whichStokes(0) = Int(stokes); StokesCoordinate stC(whichStokes); CoordinateSystem cSys; Vector lonlat = md.getAngle().getValue(); DirectionCoordinate dC = getDirectionCoordinate(stable.getDirectionRefString(), lonlat[0], lonlat[1]); cSys.addCoordinate(sC); cSys.addCoordinate(dC); cSys.addCoordinate(stC); cSys.setObsInfo(oi); Vector spec = rec.asArrayFloat("SPECTRA"); Vector flag = rec.asArrayuChar("FLAGTRA"); Vector bflag(flag.shape()); convertArray(bflag, flag); // Create casacore Image IPosition shp(4, 1); shp(0)= spec.nelements(); TempImage tIm(shp, cSys); tIm.put(spec); ArrayLattice latMask(shp); IPosition where(4,0); IPosition stride(4,1); latMask.putSlice(!bflag, where, stride); tIm.attachMask(latMask); if (isClass_) { preferVelocity = True; } Bool ok = ImageFITSConverter::ImageToFITS(errMsg, tIm, fileName, maxMem, preferVelocity, opticalVelocity, bitPix, minPix, maxPix, overWrite, degLast, reallyVerbose); if (!ok) { throw(AipsError(errMsg)); } int status = 0; fitsfile *fptr; if( fits_open_file(&fptr, fileName.c_str(), READWRITE, &status) ) throw AipsError("Coudn't open fits file for modification"); if (isClass_) { // Add CLASS specific information // Apply hacks to fits file so it can be read by class // modifications are // CTYPE1 : FREQ-XYZ -> FREQ // CRVAL1 : -> CRVAL1-RESTFREQ // Use preferVelocity which seems to work. // When no restfrequency is given this will set up the correct // frequency axis. Otherwise it uses a velocity axis char ctyp[84]; fits_read_key(fptr, TSTRING, "CTYPE1", ctyp, NULL, &status); if (String(ctyp).contains("FREQ", 0)) { float restf,refval; fits_read_key(fptr, TFLOAT, "CRVAL1", &refval, NULL, &status); restf = 0.0; if ( fits_update_key(fptr, TFLOAT, "CRVAL1", &restf, NULL, &status) ) { throw AipsError("Couldn't modify CRVAL1"); } if ( fits_update_key(fptr, TFLOAT, "RESTFREQ", &refval, NULL, &status) ) { throw AipsError("Couldn't modify RESTFREQ"); } } else { float refval = sC.referenceValue()[0]; if ( fits_update_key(fptr, TFLOAT, "RESTFREQ", &refval, NULL, &status) ) { throw AipsError("Couldn't modify RESTFREQ"); } } } Float tsys = stable.getTsys(row0); if ( fits_update_key(fptr, TFLOAT, "TSYS", &tsys, "System temperature", &status) ) { throw AipsError("Couldn't modify TSYS"); } Float otime = Float(stable.getIntTime(row0)); if ( fits_update_key(fptr, TFLOAT, "OBSTIME", &otime, "Integration time", &status) ) { throw AipsError("Couldn't modify OBSTIME"); } const char* oname = stable.getSourceName(row0).c_str(); if ( fits_update_key(fptr, TSTRING, "OBJECT", (char *)oname, NULL, &status) ) { throw AipsError("Couldn't modify OBJECT"); } Float elev = stable.getElevation(row0)/C::pi*180.0; if ( fits_update_key(fptr, TFLOAT, "ELEVATIO", &elev, "Telescope elevation (degrees)", &status) ) { throw AipsError("Couldn't modify ELEVATIO"); } Float azi = stable.getAzimuth(row0)/C::pi*180.0; if ( fits_update_key(fptr, TFLOAT, "AZIMUTH", &azi, "Telescope azimuth (degrees)", &status) ) { throw AipsError("Couldn't modify AZIMUTH"); } fits_close_file(fptr, &status); LogIO os( casacore::LogOrigin("STFITSImageWriter")); os << "Wrote " << fileName << LogIO::POST; ++iter; } return True; } DirectionCoordinate STFITSImageWriter::getDirectionCoordinate(const String& reff, Double lon, Double lat) { Projection proj(Projection::SIN); // What should we use ? Matrix xForm(2,2); xForm = 0.0; xForm.diagonal() = 1.0; Vector incLonLat(2,0.0); Vector refPixLonLat(2,0.0); MDirection::Types mdt; if (!MDirection::getType(mdt, reff)) { throw(AipsError("Illegal Direction frame.")); } return DirectionCoordinate(mdt, proj, lon, lat, incLonLat[0], incLonLat[1], xForm, refPixLonLat[0], refPixLonLat[1]); }