Changeset 2865
- Timestamp:
- 11/07/13 18:42:23 (11 years ago)
- Location:
- trunk/src
- Files:
-
- 2 edited
Legend:
- Unmodified
- Added
- Removed
-
trunk/src/STSideBandSep.cpp
r2864 r2865 574 574 const int itp = (tp_ == Table::Memory ? 0 : 1); 575 575 ScantableWrapper gtab = gridder.getResultAsScantable(itp); 576 // WORKAROUND : Shift TIME for proper pointing resolution in future imaging. 577 shiftTimeInGriddedST(gtab.getCP()); 576 578 return gtab; 577 579 }; … … 601 603 ymin = min(ymin, bmin); 602 604 ymax = max(ymax, bmax); 605 } 606 }; 607 608 // STGrid sets the identical time for all rows in scantable 609 // which is reasonable thing to do in position based averaging. 610 // However, this prevents CASA from finding proper pointing 611 // per spectra once the gridded scantable is converted to 612 // measurement set (MS). It is because MS does not 613 // have ability to store per spectra pointing information. 614 // MS stores pointing information in a subtable, POINTING, 615 // with corresponding TIME when an antenna pointed the direction. 616 // The pointing direction corresponding to a spectra is resolved 617 // in MS by interpolating DIRECTION in POINTING subtable in TIME 618 // the spectra is observed. If there are multiple match, 619 // the first match is adopted. Therefore, gridded table (whose TIME 620 // is set to a single value) is misunderstood in MS that all data 621 // come from a single pointing. 622 // The function workarounds this defect by artificially shifting 623 // TIME by INTERVAL in each row. 624 void STSideBandSep::shiftTimeInGriddedST(const CountedPtr<Scantable> &stab) 625 { 626 LogIO os(LogOrigin("STSideBandSep", "shiftTimeInGriddedST()", WHERE)); 627 // Gridded table usually has an IF and a BEAM. 628 { 629 std::vector<uint> bmnos = stab->getBeamNos(); 630 if (bmnos.size() > 1) 631 throw( AipsError("Multiple BEAMNOs found in the scantable. This may not a gridded table") ); 632 std::vector<uint> ifnos = stab->getIFNos(); 633 if (ifnos.size() > 1) 634 throw( AipsError("Multiple IFNOs found in the scantable. This may not a gridded table") ); 635 } 636 // Rows in gridded table usually sorted by DIRECTION 637 const Table& tab = stab->table(); 638 ROScalarColumn<Double> mjdCol( tab, "TIME"); 639 ROScalarColumn<Double> intCol( tab, "INTERVAL"); 640 ROArrayColumn<Double> dirCol( tab, "DIRECTION"); 641 Matrix<Double> direction = dirCol.getColumn(); 642 Vector<Double> ra( direction.row(0) ); 643 Vector<Double> dec( direction.row(1) ); 644 Double prevTime, prevInt, prevRA(ra[0]), prevDec(dec[0]); 645 mjdCol.get(0, prevTime); 646 intCol.get(0, prevInt); 647 Double currInt, currRA, currDec; 648 Double dx(xtol_*0.95), dy(ytol_*0.95); 649 Double secToDay(1./24./3600.); 650 for (int irow = 0; irow < stab->nrow(); ++irow){ 651 currRA = ra[irow]; 652 currDec = dec[irow]; 653 if ((prevRA+dx-currRA)*(currRA-prevRA+dx)>=0 && 654 (prevDec+dy-currDec)*(currDec-prevDec+dy)>=0) { 655 // the same time stamp as the previous row 656 mjdCol.put(irow, prevTime); 657 // remember the longest interval 658 intCol.get(irow, currInt); 659 if (currInt > prevInt) prevInt = currInt; 660 } else { 661 // a new direction. need to set new time stamp. 662 prevTime += prevInt*secToDay; 663 mjdCol.put(irow, prevTime); 664 // new interval and direction 665 intCol.get(irow, prevInt); 666 prevRA = currRA; 667 prevDec = currDec; 668 } 603 669 } 604 670 }; -
trunk/src/STSideBandSep.h
r2853 r2865 114 114 Double &ymin, Double &ymax); 115 115 116 /** 117 * Shift TIME in gridded scantable for future imaging 118 * 119 * STGrid sets the identical time for all rows in scantable 120 * which is reasonable thing to do in position based averaging. 121 * However, this prevents CASA from finding proper pointing 122 * per spectra once the gridded scantable is converted to 123 * measurement set (MS). It is because MS does not 124 * have ability to store per spectra pointing information. 125 * MS stores pointing information in a subtable, POINTING, 126 * with corresponding TIME when an antenna pointed the direction. 127 * The pointing direction corresponding to a spectra is resolved 128 * in MS by interpolating DIRECTION in POINTING subtable in TIME 129 * the spectra is observed. If there are multiple match, 130 * the first match is adopted. Therefore, gridded table (whose TIME 131 * is set to a single value) is misunderstood in MS that all data 132 * come from a single pointing. 133 * The function workarounds this defect by artificially shifting 134 * TIME by INTERVAL in each row. 135 **/ 136 void shiftTimeInGriddedST(const CountedPtr<Scantable> &stab); 116 137 /** 117 138 * Actual calculation of frequencies of image sideband
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