| 1 | //
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| 2 | // C++ Implementation: PKSFiller
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| 3 | //
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| 4 | // Description:
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| 5 | //
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| 6 | //
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| 7 | // Author: Malte Marquarding <asap@atnf.csiro.au>, (C) 2010
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| 8 | //
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| 9 | // Copyright: See COPYING file that comes with this distribution
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| 10 | //
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| 11 | //
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| 12 | #include <casa/iostream.h>
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| 13 | #include <casa/iomanip.h>
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| 14 |
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| 15 | #include <casa/Exceptions.h>
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| 16 | #include <casa/OS/Path.h>
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| 17 | #include <casa/OS/File.h>
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| 18 | #include <casa/Quanta/Unit.h>
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| 19 | #include <casa/Arrays/ArrayMath.h>
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| 20 | #include <casa/Arrays/ArrayLogical.h>
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| 21 | #include <casa/Utilities/Regex.h>
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| 22 | #include <casa/Utilities/DataType.h>
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| 23 | #include <casa/Logging/LogIO.h>
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| 24 |
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| 25 | #include <casa/Containers/Record.h>
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| 26 | #include <measures/Measures/MDirection.h>
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| 27 | #include <measures/Measures/MeasConvert.h>
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| 28 |
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| 29 | #include <atnf/PKSIO/PKSrecord.h>
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| 30 | #include <atnf/PKSIO/PKSreader.h>
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| 31 |
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| 32 | #ifdef HAS_ALMA
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| 33 | #include <casa/System/ProgressMeter.h>
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| 34 | #endif
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| 35 | #include <casa/Logging/LogIO.h>
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| 36 |
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| 37 | #include <time.h>
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| 38 | #include <sstream>
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| 39 |
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| 40 | #include "STDefs.h"
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| 41 | #include "STAttr.h"
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| 42 |
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| 43 | #include "PKSFiller.h"
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| 44 | #include "STHeader.h"
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| 45 |
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| 46 | using namespace casa;
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| 47 |
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| 48 | namespace asap {
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| 49 |
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| 50 |
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| 51 | PKSFiller::PKSFiller( CountedPtr< Scantable > stbl ) :
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| 52 | FillerBase(stbl),
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| 53 | reader_(0)
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| 54 | {
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| 55 | setReferenceRegex(".*(e|w|_R)$");
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| 56 | }
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| 57 |
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| 58 | PKSFiller::~PKSFiller()
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| 59 | {
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| 60 | close();
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| 61 | }
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| 62 |
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| 63 | bool PKSFiller::open( const std::string& filename, const Record& rec)
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| 64 | {
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| 65 | Bool haveBase, haveSpectra;
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| 66 |
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| 67 | String inName(filename);
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| 68 | Path path(inName);
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| 69 | inName = path.expandedName();
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| 70 |
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| 71 | File file(inName);
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| 72 | filename_ = inName;
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| 73 |
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| 74 | // Create reader and fill in values for arguments
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| 75 | String format;
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| 76 | Vector<Bool> beams, ifs;
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| 77 | Vector<uInt> nchans,npols;
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| 78 |
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| 79 | String antenna("");
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| 80 | Bool getPt = False;
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| 81 |
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| 82 | // parsing MS options
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| 83 | if ( rec.isDefined( "ms" ) ) {
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| 84 | Record msrec = rec.asRecord( "ms" ) ;
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| 85 | //msrec.print( cout ) ;
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| 86 | if ( msrec.isDefined( "getpt" ) ) {
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| 87 | getPt = msrec.asBool( "getpt" ) ;
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| 88 | }
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| 89 | if ( msrec.isDefined( "antenna" ) ) {
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| 90 | if ( msrec.type( msrec.fieldNumber( "antenna" ) ) == TpInt ) {
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| 91 | Int antInt = msrec.asInt( "antenna" ) ;
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| 92 | ostringstream oss ;
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| 93 | oss << antInt ;
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| 94 | antenna = String( oss ) ;
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| 95 | }
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| 96 | else {
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| 97 | antenna = msrec.asString( "antenna" ) ;
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| 98 | }
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| 99 | }
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| 100 | }
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| 101 |
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| 102 | reader_ = getPKSreader(inName, antenna, 0, 0, format, beams, ifs,
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| 103 | nchans, npols, haveXPol_, haveBase, haveSpectra);
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| 104 | if (reader_.null() == True) {
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| 105 | return False;
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| 106 | }
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| 107 |
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| 108 | if (!haveSpectra) {
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| 109 | reader_ = 0;
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| 110 | throw(AipsError("No spectral data in file."));
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| 111 | }
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| 112 |
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| 113 | LogIO os( LogOrigin( "PKSFiller", "open()", WHERE ) ) ;
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| 114 | nBeam_ = beams.nelements();
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| 115 | nIF_ = ifs.nelements();
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| 116 | // Get basic parameters.
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| 117 | if ( anyEQ(haveXPol_, True) ) {
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| 118 | os << "Cross polarization present" << LogIO::POST;
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| 119 | for (uInt i=0; i< npols.nelements();++i) {
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| 120 | if (npols[i] < 3) npols[i] += 2;// Convert Complex -> 2 Floats
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| 121 | }
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| 122 | }
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| 123 | STHeader header;
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| 124 | header.nchan = max(nchans);
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| 125 | header.npol = max(npols);
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| 126 | header.nbeam = nBeam_;
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| 127 |
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| 128 | Int status = reader_->getHeader(header.observer, header.project,
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| 129 | header.antennaname, header.antennaposition,
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| 130 | header.obstype,
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| 131 | header.fluxunit,
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| 132 | header.equinox,
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| 133 | header.freqref,
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| 134 | header.utc, header.reffreq,
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| 135 | header.bandwidth);
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| 136 |
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| 137 | if (status) {
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| 138 | reader_ = 0;
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| 139 | throw(AipsError("Failed to get header."));
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| 140 | }
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| 141 | os << "Found " << header.antennaname << " data." << LogIO::POST;
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| 142 | if ((header.obstype).matches("*SW*")) {
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| 143 | // need robust way here - probably read ahead of next timestamp
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| 144 | os << "Header indicates frequency switched observation.\n"
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| 145 | << "setting # of IFs = 1 " << LogIO::POST;
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| 146 |
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| 147 | nIF_ = 1;
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| 148 | header.obstype = String("fswitch");
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| 149 | }
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| 150 | // Determine Telescope and set brightness unit
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| 151 | Bool throwIt = False;
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| 152 | Instrument inst = STAttr::convertInstrument(header.antennaname, throwIt);
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| 153 |
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| 154 | if (inst==ATMOPRA || inst==TIDBINBILLA) {
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| 155 | header.fluxunit = "K";
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| 156 | } else {
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| 157 | // downcase for use with Quanta
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| 158 | if (header.fluxunit == "JY") {
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| 159 | header.fluxunit = "Jy";
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| 160 | }
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| 161 | }
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| 162 | STAttr stattr;
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| 163 | header.poltype = stattr.feedPolType(inst);
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| 164 | header.nif = nIF_;
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| 165 | header.epoch = "UTC";
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| 166 | // *** header.frequnit = "Hz"
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| 167 | // Apply selection criteria.
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| 168 | Vector<Int> ref;
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| 169 |
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| 170 | Vector<Int> start(nIF_, 1);
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| 171 | Vector<Int> end(nIF_, 0);
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| 172 | reader_->select(beams, ifs, start, end, ref, True, haveXPol_[0], False, getPt);
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| 173 | setHeader(header);
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| 174 | //For MS, add the location of POINTING of the input MS so one get
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| 175 | //pointing data from there, if necessary.
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| 176 | //Also find nrow in MS
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| 177 | nInDataRow = 0;
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| 178 | if (format == "MS2") {
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| 179 | Path datapath(inName);
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| 180 | String ptTabPath = datapath.absoluteName();
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| 181 | Table inMS(ptTabPath);
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| 182 | nInDataRow = inMS.nrow();
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| 183 | ptTabPath.append("/POINTING");
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| 184 | table_->table().rwKeywordSet().define("POINTING", ptTabPath);
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| 185 | if (header.antennaname.matches("GBT")) {
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| 186 | String GOTabPath = datapath.absoluteName();
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| 187 | GOTabPath.append("/GBT_GO");
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| 188 | table_->table().rwKeywordSet().define("GBT_GO", GOTabPath);
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| 189 | }
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| 190 | }
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| 191 | String freqFrame = header.freqref;
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| 192 | //translate frequency reference frame back to
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| 193 | //MS style (as PKSMS2reader converts the original frame
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| 194 | //in FITS standard style)
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| 195 | if (freqFrame == "TOPOCENT") {
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| 196 | freqFrame = "TOPO";
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| 197 | } else if (freqFrame == "GEOCENER") {
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| 198 | freqFrame = "GEO";
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| 199 | } else if (freqFrame == "BARYCENT") {
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| 200 | freqFrame = "BARY";
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| 201 | } else if (freqFrame == "GALACTOC") {
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| 202 | freqFrame = "GALACTO";
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| 203 | } else if (freqFrame == "LOCALGRP") {
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| 204 | freqFrame = "LGROUP";
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| 205 | } else if (freqFrame == "CMBDIPOL") {
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| 206 | freqFrame = "CMB";
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| 207 | } else if (freqFrame == "SOURCE") {
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| 208 | freqFrame = "REST";
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| 209 | }
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| 210 | // set both "FRAME" and "BASEFRAME"
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| 211 | table_->frequencies().setFrame(freqFrame, false);
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| 212 | table_->frequencies().setFrame(freqFrame, true);
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| 213 |
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| 214 | return true;
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| 215 | }
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| 216 |
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| 217 | void PKSFiller::close( )
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| 218 | {
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| 219 | if (reader_.null() != False) {
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| 220 | reader_ = 0;
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| 221 | }
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| 222 | table_ = 0;
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| 223 | }
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| 224 |
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| 225 | void PKSFiller::fill( )
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| 226 | {
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| 227 | int status = 0;
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| 228 | LogIO os( LogOrigin( "PKSFiller", "fill()", WHERE ) ) ;
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| 229 |
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| 230 | /**
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| 231 | Int beamNo, IFno, refBeam, scanNo, cycleNo;
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| 232 | Float azimuth, elevation, focusAxi, focusRot, focusTan,
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| 233 | humidity, parAngle, pressure, temperature, windAz, windSpeed;
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| 234 | Double bandwidth, freqInc, interval, mjd, refFreq, srcVel;
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| 235 | String fieldName, srcName, tcalTime, obsType;
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| 236 | Vector<Float> calFctr, sigma, tcal, tsys;
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| 237 | Matrix<Float> baseLin, baseSub;
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| 238 | Vector<Double> direction(2), scanRate(2), srcDir(2), srcPM(2), restFreq(1);
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| 239 | Matrix<Float> spectra;
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| 240 | Matrix<uChar> flagtra;
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| 241 | Complex xCalFctr;
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| 242 | Vector<Complex> xPol;
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| 243 | **/
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| 244 |
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| 245 | Double min = 0.0;
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| 246 | Double max = nInDataRow;
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| 247 | #ifdef HAS_ALMA
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| 248 | ProgressMeter fillpm(min, max, "Data importing progress");
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| 249 | #endif
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| 250 | PKSrecord pksrec;
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| 251 | pksrec.srcType=-1;
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| 252 | int n = 0;
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| 253 | bool isGBTFITS = false ;
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| 254 | if ((table_->getAntennaName().find( "GBT" ) != String::npos)
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| 255 | && File(filename_).isRegular()) {
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| 256 | FILE *fp = fopen( filename_.c_str(), "r" ) ;
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| 257 | fseek( fp, 640, SEEK_SET ) ;
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| 258 | char buf[81] ;
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| 259 | fread( buf, 80, 1, fp ) ;
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| 260 | buf[80] = '\0' ;
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| 261 | if ( strstr( buf, "NRAO_GBT" ) != NULL ) {
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| 262 | isGBTFITS = true ;
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| 263 | }
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| 264 | fclose( fp ) ;
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| 265 | }
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| 266 |
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| 267 | while ( status == 0 ) {
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| 268 |
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| 269 | status = reader_->read(pksrec);
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| 270 | if ( status != 0 ) break;
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| 271 | n += 1;
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| 272 | Regex filterrx(".*[SL|PA]$");
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| 273 | Regex obsrx("^AT.+");
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| 274 | if ( table_->getAntennaName().matches(obsrx) &&
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| 275 | pksrec.obsType.matches(filterrx)) {
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| 276 | //cerr << "ignoring paddle scan" << endl;
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| 277 | continue;
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| 278 | }
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| 279 |
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| 280 | Vector<Double> sratedbl(pksrec.scanRate.nelements());
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| 281 | convertArray(sratedbl, pksrec.scanRate);
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| 282 | setScanRate(sratedbl);
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| 283 |
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| 284 | Regex rx(getReferenceRegex());
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| 285 | Regex rx2("_S$");
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| 286 | Int match = pksrec.srcName.matches(rx);
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| 287 | std::string srcname;
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| 288 | Int srctype = Int(SrcType::NOTYPE);
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| 289 | if (match) {
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| 290 | srcname = pksrec.srcName;
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| 291 | srctype = Int(SrcType::PSOFF);
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| 292 | } else {
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| 293 | srcname = pksrec.srcName.before(rx2);
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| 294 | srctype = Int(SrcType::PSON);
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| 295 | }
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| 296 | if ( pksrec.srcType != Int(SrcType::NOTYPE)) {
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| 297 | srctype = pksrec.srcType ;
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| 298 | }
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| 299 | setTime(pksrec.mjd, pksrec.interval);
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| 300 | setSource(srcname, srctype, pksrec.fieldName,
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| 301 | pksrec.srcDir, pksrec.srcPM, pksrec.srcVel);
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| 302 |
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| 303 | if (nBeam_ > 1 ) {
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| 304 | setReferenceBeam(pksrec.refBeam-1);
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| 305 | }
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| 306 |
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| 307 | setMolecule(pksrec.restFreq);
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| 308 | setTcal(pksrec.tcalTime, pksrec.tcal);
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| 309 | setWeather(pksrec.temperature, pksrec.pressure,
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| 310 | pksrec.humidity, pksrec.windSpeed,
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| 311 | pksrec.windAz);
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| 312 | setFocus(pksrec.parAngle, pksrec.focusAxi, pksrec.focusTan,
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| 313 | pksrec.focusRot);
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| 314 | setDirection(pksrec.direction, pksrec.azimuth, pksrec.elevation);
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| 315 |
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| 316 | setFrequency(Double(pksrec.spectra.nrow()/2),
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| 317 | pksrec.refFreq, pksrec.freqInc);
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| 318 |
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| 319 | // Note: this is only one value for all polarisations!
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| 320 | setFlagrow(pksrec.flagrow);
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| 321 | // Turn the (nchan,npol) matrix and possible complex xPol vector
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| 322 | // into 2-4 rows in the scantable
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| 323 | Vector<Float> tsysvec(1);
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| 324 | // Why is spectra.ncolumn() == 3 for haveXPol_ == True
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| 325 | uInt npol = (pksrec.spectra.ncolumn()==1 ? 1: 2);
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| 326 | uInt polno =0;
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| 327 | for ( uInt i=0; i< npol; ++i ) {
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| 328 | tsysvec = pksrec.tsys(i);
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| 329 | if (isGBTFITS) {
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| 330 | polno = pksrec.polNo ;
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| 331 | } else {
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| 332 | polno = i;
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| 333 | }
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| 334 | setIndex(pksrec.scanNo-1, pksrec.cycleNo-1, pksrec.IFno-1, polno,
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| 335 | pksrec.beamNo-1);
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| 336 | setSpectrum(pksrec.spectra.column(i), pksrec.flagged.column(i), tsysvec);
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| 337 | commitRow();
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| 338 | }
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| 339 | if ( haveXPol_[0] ) {
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| 340 | // no tsys given for xpol, so emulate it
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| 341 | tsysvec = sqrt(pksrec.tsys[0]*pksrec.tsys[1]);
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| 342 | // add real part of cross pol
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| 343 | polno = 2;
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| 344 | Vector<Float> r(real(pksrec.xPol));
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| 345 | // make up flags from linears
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| 346 | /// @fixme this has to be a bitwise or of both pols
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| 347 | /// pksrec.flagged.column(0) | pksrec.flagged.column(1);
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| 348 |
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| 349 | setIndex(pksrec.scanNo-1, pksrec.cycleNo-1, pksrec.IFno-1, polno,
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| 350 | pksrec.beamNo-1);
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| 351 | setSpectrum(r, pksrec.flagged.column(0), tsysvec);
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| 352 | commitRow();
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| 353 |
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| 354 | // ad imaginary part of cross pol
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| 355 | polno = 3;
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| 356 | Vector<Float> im(imag(pksrec.xPol));
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| 357 | setIndex(pksrec.scanNo-1, pksrec.cycleNo-1, pksrec.IFno-1, polno,
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| 358 | pksrec.beamNo-1);
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| 359 | setSpectrum(im, pksrec.flagged.column(0), tsysvec);
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| 360 | commitRow();
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| 361 | }
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| 362 | #ifdef HAS_ALMA
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| 363 | fillpm._update(n);
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| 364 | #endif
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| 365 | }
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| 366 | if (status > 0) {
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| 367 | close();
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| 368 | throw(AipsError("Reading error occured, data possibly corrupted."));
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| 369 | }
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| 370 | #ifdef HAS_ALMA
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| 371 | fillpm.done();
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| 372 | #endif
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| 373 | }
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| 374 |
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| 375 | }//namespace asap
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