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/* $Id: vmifusphotcalib.c,v 1.2 2013-03-25 11:43:04 cgarcia Exp $
*
* This file is part of the VIMOS Pipeline
* Copyright (C) 2002-2004 European Southern Observatory
*
* 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., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA
*/
/*
* $Author: cgarcia $
* $Date: 2013-03-25 11:43:04 $
* $Revision: 1.2 $
* $Name: not supported by cvs2svn $
*/
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include <stdlib.h>
#include <stdio.h>
#include <string.h>
#include <math.h>
#include <pilmessages.h>
#include "vmimage.h"
#include "vmimageset.h"
#include "vmmatrix.h"
#include "vmmath.h"
#include "vmfit.h"
#include "vmccdtable.h"
#include "vmifutable.h"
#include "vmobjecttable.h"
#include "vmifutypes.h"
#include "vmmossphotcalib.h"
#include "vmifusphotcalib.h"
#define NUMFIBS 6400
#define IFU_HEAD_SIZE 80
int
VmIfuCalPhot(VimosImageSet *imageSet, int fitOrd, float int_frac)
{
int i, k, right, got, quadNum, ngood;
int referenceL, referenceM, specLen, objNumber = 0;
int fibL[NUMFIBS], fibM[NUMFIBS], fibLS[NUMFIBS];
int fibMS[NUMFIBS], toSort[NUMFIBS];
int refSlitNo = 0, refFibNo = 0, refQuad = 0, stdRow = 0, xLen, yLen;
int jj, ll, ok;
float referenceFlux, refTotIntensity = 0, wLenInc;
float threshold, fraction;
float fibIntFlux[NUMFIBS], fibIntFluxS[NUMFIBS];
double dValue;
char comment[80];
char modName[] = "VmIfuCalPhot";
VimosFloatArray *spectrum;
VimosImage *ifuImage, *ifuMask, *stdImage = NULL;
VimosSingleImage *oneImage;
VimosObjectTable *objTable;
VimosObjectObject *imaObjs;
VimosTable *stdTable = NULL;
VimosIfuTable *ifuTable;
VimosIfuQuad *theQuads;
VimosIfuSlit *theIfuSlits = NULL;
VimosIfuFiber *theIfuFibers;
VimosPixelRegion *pixRegion;
VimosPixelList *thePixList;
VimosPixelData *thePixData;
pilMsgInfo (modName, "Start computing spectro-photometric calibration");
puts("TBD: numbering for L,M from 0 or 1 (below) - CHECK IT");
oneImage = imageSet->images;
/* this is the subsctript for fibM, fibL, fibIntFlux arrays */
got = 0;
while (oneImage)
{
/* take the object table and IFU table of this image */
objTable = oneImage->objectTable;
ifuTable = oneImage->ifuTable;
/* length of spectra in wavelength */
specLen = oneImage->theImage->xlen;
/* Allocate spectrum */
spectrum = newFloatArray(specLen);
/* CHECK wLenInc DOUBLE OR FLOAT! */
/* read wlen inc keyword: expected in nm (DRS Document) */
readDoubleDescriptor(objTable->descs, "ESO PRO WLEN INC",
&dValue, comment);
wLenInc = (float) dValue;
/* counter for all objects in image */
objNumber = 0;
/* read which quadrant this image refers */
readIntDescriptor(objTable->descs, "ESO PRO QUAD", &quadNum, comment);
theQuads = ifuTable->quads;
/* take from ifuTable only those slits in the quadrant corresponding */
/* to the image in use */
while (theQuads)
{
if (theQuads->quadNo == quadNum)
{
theIfuSlits = theQuads->ifuSlits;
}
theQuads = theQuads->next;
}
/* take objects in the image object table */
imaObjs = objTable->objs;
while (imaObjs)
{
/* loop on IFU slits for this quadrant to find L,M of each object */
while (theIfuSlits)
{
/* if this is the "right" slit go on to take fibers */
if (theIfuSlits->ifuSlitNo == imaObjs->IFUslitNo)
{
theIfuFibers = theIfuSlits->fibers;
/* loop on fibers of this slit until find the one */
/* corresponding to the object */
while (theIfuFibers)
{
if (theIfuFibers->fibNo == imaObjs->IFUfibNo)
{
/* take this spectrum, to integrate */
for (i = 0; i < specLen; i++ )
{
spectrum->data[i] =
oneImage->theImage->data[i + ((imaObjs->rowNum)*
specLen)];
}
fibIntFlux[got] = integrateSpectrum(spectrum, wLenInc);
fibL[got] = theIfuFibers->fiberL;
fibM[got] = theIfuFibers->fiberM;
got++;
}
theIfuFibers = theIfuFibers->next;
}
}
theIfuSlits = theIfuSlits->next;
}
imaObjs = imaObjs->next;
/* increment counter of objects done */
objNumber++;
}
oneImage = oneImage->next;
deleteFloatArray(spectrum);
}
if (got != NUMFIBS) printf("WRONG NUMBER of DETECTED OBJECTS: %d",got);
/* now retrieve array of subscripts to sort in flux */
Indexx(NUMFIBS, fibIntFlux, toSort);
/* actual sorting. This mantains correspondence between flux array and */
/* L,M coordinates of fibers */
for (i=0; i<NUMFIBS; i++)
{
fibIntFluxS[i] = fibIntFlux[toSort[i]];
fibLS[i] = fibL[toSort[i]];
fibMS[i] = fibM[toSort[i]];
}
/* WARNING! CHECK THE SORTING */
/* take the flux reference fiber, i.e. the one with the max. flux */
referenceFlux = fibIntFluxS[0];
referenceL = fibLS[0];
referenceM = fibMS[0];
ifuImage = newImageAndAlloc(IFU_HEAD_SIZE,IFU_HEAD_SIZE);
/* NOTE: pixel (0,0) correspond to (L,M) = (1,1) */
/* put the fiber (fibL, fibM) = (1,1) at the pixel (0,0) */
/* CHECK IF THIS WORKS CORRECTLY */
puts("Check renumbering of fibers -> pixels");
for (k=0; k<NUMFIBS; k++)
{
ifuImage->data[(fibL[k]-1) + (fibM[k]-1)*IFU_HEAD_SIZE] = fibIntFlux[k];
}
/* now we can use the image for thresholding & looking for adjacent pixels*/
ifuMask = newImageAndAlloc(IFU_HEAD_SIZE,IFU_HEAD_SIZE);
/* set the threshold value */
threshold = referenceFlux * int_frac;
ngood = 0;
thresholdImage(ifuImage, threshold, ifuMask, &ngood);
/* now detect adjacent pixels, i.e. regions */
pixRegion = newPixelRegion();
pixRegion = findRegionsOnPixelMap(ifuImage, ifuMask, pixRegion,
ngood);
/* if more than one blob, look for the one with reference fiber */
if (pixRegion->numRegions > 1)
{
puts("VmIfuCalPhot: number of regions above threshold > 1");
}
thePixList = pixRegion->pixelList;
right = 0;
while (thePixList)
{
thePixData = thePixList->pixelData;
while (thePixData)
{
if ( (thePixData->x == referenceL) &&
(thePixData->y == referenceM) ) right++;
thePixData = thePixData->next;
}
if (right > 1) puts("something wrong in detecting reference region");
if (right == 1) refTotIntensity = thePixList->totIntensity;
thePixList = thePixList->next;
}
if(right == 0) puts("something wrong in detecting reference region");
/* loop on IFU Table to find slit and fiber number of reference spectrum */
oneImage = imageSet->images;
ifuTable = oneImage->ifuTable;
theQuads = ifuTable->quads;
while (theQuads)
{
theIfuSlits = theQuads->ifuSlits;
while (theIfuSlits)
{
theIfuFibers = theIfuSlits->fibers;
while (theIfuFibers)
{
if ((theIfuFibers->fiberL == referenceL) &&
(theIfuFibers->fiberM == referenceM))
{
refFibNo = theIfuFibers->fibNo;
refSlitNo = theIfuSlits->ifuSlitNo;
refQuad = theQuads->quadNo;
}
theIfuFibers = theIfuFibers->next;
}
theIfuSlits = theIfuSlits->next;
}
theQuads = theQuads->next;
}
/* determine the fraction factor: fraction of light lost by the ref. fibre*/
fraction = refTotIntensity/referenceFlux;
/* now loop on imageSet and objectTables to find the image with reference
spectrumand relative spectro-phot table, find row number for the
reference spectrum, correct flux loss for reference spectrum, and evaluate
spectro-photometric calibration */
ok = 0;
oneImage = imageSet->images;
while (oneImage)
{
/* take the object table and IFU table of this image */
objTable = oneImage->objectTable;
/* read which quadrant this image refers to */
readIntDescriptor(objTable->descs, "ESO PRO QUAD", &quadNum, "");
/* if this image refers to the quadrant with reference spectrum, go on */
if (quadNum == refQuad)
{
/* take objects in the image object table */
imaObjs = objTable->objs;
while (imaObjs)
{
if ((imaObjs->IFUslitNo == refSlitNo) &&
(imaObjs->IFUfibNo == refFibNo))
{
if (ok > 1)
{
pilMsgError(modName, ": More than one image for reference spectrum. Exiting");
return EXIT_FAILURE;
}
/* take row number of the std spectrum in the image */
stdRow = imaObjs->rowNum;
xLen = oneImage->theImage->xlen;
yLen = oneImage->theImage->ylen;
/* correct the ref. fibre spectrum for flux loss
before deriving response function as for MOS */
/* CHECK if THIS IS OK! */
puts("Check flux correction!");
for (ll=0; ll<xLen; ll++)
oneImage->theImage->data[ll + stdRow*yLen] *= fraction;
stdImage = newImageAndAlloc(xLen, yLen);
/* take image for spectro-photometric calibration */
for (jj=0; jj<yLen; jj++)
{
for (ll=0; ll<xLen; ll++)
{
stdImage->data[ll +jj*yLen] =
oneImage->theImage->data[ll +jj*yLen];
}
}
/* take spectro-photometric table of this image */
stdTable = oneImage->sphotStdTable;
ok++;
} /* end if this object is the reference spectrum */
imaObjs = imaObjs->next;
} /* end loop on objects for this image */
} /* end if the image comes from the quadrant with reference spectrum */
oneImage = oneImage->next;
}
/* now call VmSpCalPhot for spectro-photometric calibration */
if (EXIT_FAILURE == VmSpCalPhot(stdImage, stdTable, stdRow, fitOrd))
{
pilMsgError(modName," Failure in deriving spectro-photom. calibration");
return EXIT_FAILURE;
}
/* NOTE: ifu table is NOT updated with refL and refM*/
deleteImage(ifuImage);
deleteImage(ifuMask);
deleteImage(stdImage);
deleteObjectTable(objTable);
deleteObjectObject(imaObjs);
deleteTable(stdTable);
deleteIfuTable(ifuTable);
deletePixelRegion(pixRegion);
return EXIT_SUCCESS;
}
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