[1443] | 1 | //#---------------------------------------------------------------------------
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| 2 | //# STFITSImageWriter.cc: Class to write out single dish spectra as FITS images
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| 3 | //#---------------------------------------------------------------------------
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| 4 | //# Copyright (C) 2008
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| 5 | //# ATNF
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| 6 | //#
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| 7 | //# This program is free software; you can redistribute it and/or modify it
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| 8 | //# under the terms of the GNU General Public License as published by the Free
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| 9 | //# Software Foundation; either version 2 of the License, or (at your option)
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| 10 | //# any later version.
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| 11 | //#
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| 12 | //# This program is distributed in the hope that it will be useful, but
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| 13 | //# WITHOUT ANY WARRANTY; without even the implied warranty of
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| 14 | //# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General
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| 15 | //# Public License for more details.
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| 16 | //#
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| 17 | //# You should have received a copy of the GNU General Public License along
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| 18 | //# with this program; if not, write to the Free Software Foundation, Inc.,
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| 19 | //# 675 Massachusetts Ave, Cambridge, MA 02139, USA.
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| 20 | //#
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| 21 | //# Correspondence concerning this software should be addressed as follows:
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| 22 | //# Internet email: Malte.Marquarding@csiro.au
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| 23 | //# Postal address: Malte Marquarding,
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| 24 | //# Australia Telescope National Facility,
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| 25 | //# P.O. Box 76,
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| 26 | //# Epping, NSW, 2121,
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| 27 | //# AUSTRALIA
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| 28 | //#
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| 29 | //# $Id: $
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| 30 | //#---------------------------------------------------------------------------
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| 31 |
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[1444] | 32 | #include <fitsio.h>
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[1443] | 33 | #include <images/Images/TempImage.h>
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| 34 |
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| 35 | #include <lattices/Lattices/ArrayLattice.h>
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| 36 |
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| 37 | #include <measures/Measures/MEpoch.h>
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| 38 | #include <measures/Measures/Stokes.h>
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| 39 |
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| 40 | #include <tables/Tables/Table.h>
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| 41 | #include <tables/Tables/TableIter.h>
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| 42 | #include <tables/Tables/TableRecord.h>
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| 43 | #include <casa/Containers/RecordField.h>
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| 44 | #include <tables/Tables/TableRow.h>
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| 45 | #include <tables/Tables/ScalarColumn.h>
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| 46 | #include <tables/Tables/ArrayColumn.h>
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| 47 |
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| 48 |
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| 49 | #include <coordinates/Coordinates/CoordinateUtil.h>
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| 50 | #include <coordinates/Coordinates/CoordinateSystem.h>
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| 51 | #include <coordinates/Coordinates/SpectralCoordinate.h>
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| 52 | #include <coordinates/Coordinates/DirectionCoordinate.h>
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| 53 | #include <coordinates/Coordinates/StokesCoordinate.h>
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| 54 | #include <coordinates/Coordinates/ObsInfo.h>
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| 55 |
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| 56 | #include <images/Images/ImageFITSConverter.h>
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| 57 | #include <images/Images/TempImage.h>
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| 58 |
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| 59 | #include <lattices/Lattices/ArrayLattice.h>
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| 60 |
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| 61 |
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| 62 | //#include "STDefs.h"
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| 63 | #include "STHeader.h"
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| 64 | #include "Scantable.h"
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| 65 | #include "STFITSImageWriter.h"
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| 66 |
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| 67 | using namespace casa;
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| 68 | using namespace asap;
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| 69 |
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| 70 |
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| 71 | STFITSImageWriter::STFITSImageWriter() : isClass_(False)
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| 72 | {;}
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| 73 |
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| 74 | STFITSImageWriter::~STFITSImageWriter()
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| 75 | {;}
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| 76 |
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| 77 |
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| 78 | Bool STFITSImageWriter::write(const Scantable& stable,
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| 79 | const String& fileName)
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| 80 | {
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| 81 |
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| 82 | // Get global Header from Table
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| 83 |
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| 84 | STHeader hdr = stable.getHeader();
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| 85 |
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| 86 | // Column keywords
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| 87 |
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| 88 | Table tab = stable.table();
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| 89 |
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| 90 | // Temps
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| 91 |
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| 92 | const Unit RAD(String("rad"));
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| 93 |
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| 94 | // Open and write header file
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| 95 |
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| 96 | String rootName(fileName);
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| 97 | if (rootName.length()==0) rootName = String("fits");
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| 98 |
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| 99 | ObsInfo oi;
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| 100 | oi.setTelescope(String(hdr.antennaname));
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| 101 | oi.setObserver(String(hdr.observer));
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| 102 |
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| 103 | uInt maxMem = 128;
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| 104 | Bool preferVelocity = False;
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| 105 | Bool opticalVelocity = False;
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| 106 | Int bitPix = -32; // FLoating point
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| 107 | Float minPix = 1.0;
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| 108 | Float maxPix = -1.0;
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| 109 | Bool overWrite = True;
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| 110 | Bool degLast = False;
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| 111 | Bool reallyVerbose = False;
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| 112 | String errMsg;
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| 113 |
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| 114 |
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| 115 | Block<String> cols(5);
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| 116 | cols[0] = String("SCANNO");
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| 117 | cols[1] = String("CYCLENO");
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| 118 | cols[2] = String("BEAMNO");
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| 119 | cols[3] = String("IFNO");
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| 120 | cols[4] = String("POLNO");
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| 121 | TableIterator iter(tab, cols);
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| 122 | // Open data file
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| 123 | while ( !iter.pastEnd() ) {
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| 124 | Table t = iter.table();
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| 125 | ROTableRow row(t);
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| 126 | const TableRecord& rec = row.get(0);
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| 127 | String dirtype = stable.getDirectionRefString();
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| 128 | ostringstream onstr;
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| 129 | onstr << "SCAN" << rec.asuInt("SCANNO")
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| 130 | << "_CYCLE" << rec.asuInt("CYCLENO")
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| 131 | << "_BEAM" << rec.asuInt("BEAMNO")
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| 132 | << "_IF" << rec.asuInt("IFNO")
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| 133 | << "_POL" << rec.asuInt("POLNO");
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| 134 | String fileName = rootName + String(onstr) + String(".fits");
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| 135 | int row0 = t.rowNumbers(tab)[0];
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| 136 |
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| 137 | const MPosition& mp = stable.getAntennaPosition();
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| 138 | const MDirection& md = stable.getDirection(row0);
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| 139 | const MEpoch& me = stable.getEpoch(row0);
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| 140 | oi.setObsDate(me);
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| 141 |
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| 142 | const Double& rf =
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| 143 | stable.molecules().getRestFrequency(rec.asuInt("MOLECULE_ID") );
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| 144 | SpectralCoordinate sC =
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| 145 | stable.frequencies().getSpectralCoordinate(md, mp, me, rf,
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| 146 | rec.asuInt("FREQ_ID"));
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| 147 |
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| 148 | Int polno = rec.asuInt("POLNO");
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| 149 | Stokes::StokesTypes stokes =
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| 150 | Stokes::type(stable.getPolarizationLabel(polno, stable.getPolType()));
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| 151 | Vector<Int> whichStokes(1);
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| 152 | whichStokes(0) = Int(stokes);
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| 153 | StokesCoordinate stC(whichStokes);
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| 154 |
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| 155 |
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| 156 | CoordinateSystem cSys;
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| 157 | Vector<Double> lonlat = md.getAngle().getValue();
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| 158 | DirectionCoordinate dC =
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| 159 | getDirectionCoordinate(stable.getDirectionRefString(),
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| 160 | lonlat[0], lonlat[1]);
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| 161 | cSys.addCoordinate(sC);
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| 162 | cSys.addCoordinate(dC);
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| 163 | cSys.addCoordinate(stC);
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| 164 | cSys.setObsInfo(oi);
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| 165 |
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| 166 | Vector<Float> spec = rec.asArrayFloat("SPECTRA");
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| 167 | Vector<uChar> flag = rec.asArrayuChar("FLAGTRA");
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| 168 | Vector<Bool> bflag(flag.shape());
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| 169 | convertArray(bflag, flag);
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| 170 |
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| 171 | // Create casacore Image
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| 172 | IPosition shp(4, 1);
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| 173 | shp(0)= spec.nelements();
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| 174 | TempImage<Float> tIm(shp, cSys);
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| 175 | tIm.put(spec);
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| 176 | ArrayLattice<Bool> latMask(shp);
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| 177 | IPosition where(4,0);
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| 178 | IPosition stride(4,1);
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| 179 | latMask.putSlice(!bflag, where, stride);
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| 180 | tIm.attachMask(latMask);
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[1500] | 181 | if (isClass_) {
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| 182 | preferVelocity = True;
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| 183 | }
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[1443] | 184 | Bool ok = ImageFITSConverter::ImageToFITS(errMsg, tIm, fileName,
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| 185 | maxMem, preferVelocity,
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| 186 | opticalVelocity, bitPix,
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| 187 | minPix, maxPix, overWrite,
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| 188 | degLast, reallyVerbose);
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| 189 | if (!ok) {
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| 190 | throw(AipsError(errMsg));
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| 191 | }
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| 192 | if (isClass_) {
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[1500] | 193 | // Add CLASS specific information
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| 194 | // Apply hacks to fits file so it can be read by class
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| 195 | // modifications are
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| 196 | // CTYPE1 : FREQ-XYZ -> FREQ
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| 197 | // CRVAL1 : -> CRVAL1-RESTFREQ
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| 198 | int status = 0;
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| 199 | fitsfile *fptr;
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| 200 | if( fits_open_file(&fptr, fileName.c_str(), READWRITE, &status) )
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| 201 | throw AipsError("Coudn't open fits file for CLASS modification");
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| 202 |
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| 203 | // Use preferVelocity which seems to work.
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| 204 | // When no restfrequency is given this will set up the correct
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| 205 | // frequency axis. Otherwise it uses a velocity axis
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| 206 | // if ( fits_update_key(fptr, TSTRING, "CTYPE1", (char *)"FREQ",
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| 207 | // NULL, &status) )
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| 208 | // throw AipsError("Couldn't modify CTYPE1.");
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| 209 | // float restf,refval,newfreq;
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| 210 | // fits_read_key(fptr, TFLOAT, "CRVAL1",
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| 211 | // &refval, NULL, &status);
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| 212 | // fits_read_key(fptr, TFLOAT, "RESTFREQ",
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| 213 | // &restf, NULL, &status);
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| 214 | // newfreq = refval - restf;
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| 215 | // if ( fits_update_key(fptr, TFLOAT, "CRVAL1", &newfreq, NULL, &status) )
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| 216 | // throw AipsError("Couldn't modify CRVAL1");
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| 217 |
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| 218 |
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| 219 | Float tsys = stable.getTsys(row0);
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| 220 | if ( fits_update_key(fptr, TFLOAT, "TSYS", &tsys,
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| 221 | "System temperature", &status) ) {
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| 222 | throw AipsError("Couldn't modify TSYS");
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| 223 | }
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| 224 | Float otime = Float(stable.getIntTime(row0));
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| 225 | if ( fits_update_key(fptr, TFLOAT, "OBSTIME", &otime,
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| 226 | "Integration time", &status) ) {
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| 227 | throw AipsError("Couldn't modify OBSTIME");
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| 228 | }
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| 229 |
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| 230 | const char* oname = stable.getSourceName(row0).c_str();
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| 231 | if ( fits_update_key(fptr, TSTRING, "OBJECT", (char *)oname,
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| 232 | NULL, &status) ) {
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| 233 | throw AipsError("Couldn't modify OBJECT");
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| 234 | }
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| 235 | fits_close_file(fptr, &status);
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[1443] | 236 | }
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| 237 | //pushLog(String(oss));
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| 238 | ++iter;
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| 239 | }
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| 240 | return True;
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| 241 | }
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| 242 |
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| 243 | DirectionCoordinate
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| 244 | STFITSImageWriter::getDirectionCoordinate(const String& reff,
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| 245 | Double lon, Double lat)
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| 246 | {
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| 247 |
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| 248 | Projection proj(Projection::SIN); // What should we use ?
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| 249 | Matrix<Double> xForm(2,2);
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| 250 | xForm = 0.0; xForm.diagonal() = 1.0;
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| 251 | Vector<Double> incLonLat(2,0.0);
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| 252 | Vector<Double> refPixLonLat(2,0.0);
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| 253 | MDirection::Types mdt;
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| 254 | if (!MDirection::getType(mdt, reff)) {
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| 255 | throw(AipsError("Illegal Direction frame."));
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| 256 | }
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| 257 | return DirectionCoordinate(mdt, proj, lon, lat,
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| 258 | incLonLat[0], incLonLat[1], xForm,
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| 259 | refPixLonLat[0], refPixLonLat[1]);
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| 260 |
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| 261 | }
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| 262 |
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