def redux_basic(self,path='./',nproc=12):
"""
This is a basic engine that performs redux of MUSE data using the eso pipeline in a basic
form, that is apply all the basic calibs but stop before sky subtraction and coaddition.
This can be done in a later step, after some post-processing of the cube for enhanced
data quality
path - the top level folder where data reduction has to be performed.
This includes a folder Raw where the data have been downloaded using the
eso shell script. It assumes that basic calibrations are also included, as
provided by eso archive.
nproc - the number of processors to use during the reduction
This code is designed to handle a single OB or groups of OBs that share the same sets of calibrations
"""
import muse_redux_basic as rdx
import os
print 'Starting reduction...'
#First, make sure the various folders exist as needed
if not os.path.exists(path+"Raw"):
print "Cannot find Raw data..."
exit()
if not os.path.exists(path+"Script"):
os.makedirs(path+"Script")
if not os.path.exists(path+"Proc"):
os.makedirs(path+"Proc")
#parse the xml file(s)
xml_info=rdx.parse_xml(path=path,nproc=nproc)
#now start reduction. Enter the proc folder
currdir=os.getcwd()
os.chdir(path+'Proc')
print 'Changing dir to proc...'
#First handle the bias
if not os.path.isfile("MASTER_BIAS.fits"):
print 'Creating bias...'
rdx.make_bias(xml_info,nproc=nproc)
print 'All done with the bias...'
else:
print 'Bias already exist'
#Next handle the dark
if not os.path.isfile("MASTER_DARK.fits"):
print 'Creating dark...'
rdx.make_dark(xml_info,nproc=nproc)
print 'All done with the dark...'
else:
print 'Dark already exist'
#Next handle the flats
if not os.path.isfile("MASTER_FLAT.fits"):
print 'Creating flat...'
rdx.make_flat(xml_info,nproc=nproc)
print 'All done with flat...'
else:
print 'Flat already exist'
#Next handle the arcs
if not os.path.isfile("WAVECAL_RESIDUALS.fits"):
print 'Processing the arcs...'
rdx.make_arcs(xml_info,nproc=nproc)
print 'All done with arcs...'
else:
print 'Arcs already processed'
#Next handle the twilight flat
if not os.path.isfile("DATACUBE_SKYFLAT.fits"):
print 'Processing the twiflat...'
rdx.make_twiflat(xml_info,nproc=nproc)
print 'All done with twiflat...'
else:
print 'Twiflat already processed'
#Next calibrate standard star
if not os.path.isfile("STD_RED_0001.fits"):
print 'Processing the standard star...'
rdx.make_stdstar(xml_info,nproc=nproc)
print 'All done with standard star...'
else:
print 'Standard star already processed'
#Next generate flux table
if not os.path.isfile("STD_FLUXES_0001.fits"):
print 'Processing the flux table...'
rdx.make_stdflux(xml_info,nproc=nproc)
print 'All done with flux table...'
else:
print 'Flux table already processed'
#Next calibrate objects
if not os.path.isfile("OBJECT_RED_0001.fits"):
print 'Processing the objects...'
rdx.make_objects(xml_info,nproc=nproc)
print 'All done with objects...'
else:
print 'Objects already processed'
#Finally, process science
print 'Preparing intermediate data cubes...'
rdx.make_cubes(xml_info,nproc=nproc)
#Done - back to original directory!
print 'All done with basic redux...'
os.chdir(currdir)
return xml_info
def redux_basic(self, path='./', nproc=12, pipecal=False):
"""
This is a basic engine that performs redux of MUSE data using the eso pipeline in a basic
form, that is apply all the basic calibs but stop before sky subtraction and coaddition.
This can be done in a later step, after some post-processing of the cube for enhanced
data quality
path - the top level folder where data reduction has to be performed.
This includes a folder Raw where the data have been downloaded using the
eso shell script. It assumes that basic calibrations are also included, as
provided by eso archive.
nproc - the number of processors to use during the reduction
pipecal - if set to true, static calibrations provided with the pipeline
will be used. This pplies to ALL static calibrations
This code is designed to handle a single OB or groups of OBs that share the same sets of calibrations
"""
import muse_redux_basic as rdx
import os
print 'Starting reduction...'
#First, make sure the various folders exist as needed
if not os.path.exists(path + "Raw"):
print "Cannot find Raw data..."
exit()
if not os.path.exists(path + "Script"):
os.makedirs(path + "Script")
if not os.path.exists(path + "Proc"):
os.makedirs(path + "Proc")
#parse the xml file(s)
xml_info = rdx.parse_xml(path=path, nproc=nproc, pipecal=pipecal)
#now start reduction. Enter the proc folder
currdir = os.getcwd()
os.chdir(path + 'Proc')
print 'Changing dir to proc...'
#First handle the bias
if not os.path.isfile("MASTER_BIAS.fits"):
print 'Creating bias...'
rdx.make_bias(xml_info, nproc=nproc)
print 'All done with the bias...'
else:
print 'Bias already exist'
#Next handle the dark
if not os.path.isfile("MASTER_DARK.fits"):
print 'Creating dark...'
rdx.make_dark(xml_info, nproc=nproc)
print 'All done with the dark...'
else:
print 'Dark already exist'
#Next handle the flats
if not os.path.isfile("MASTER_FLAT.fits"):
print 'Creating flat...'
rdx.make_flat(xml_info, nproc=nproc)
print 'All done with flat...'
else:
print 'Flat already exist'
#Next handle the arcs
if not os.path.isfile("WAVECAL_RESIDUALS.fits"):
print 'Processing the arcs...'
rdx.make_arcs(xml_info, nproc=nproc)
print 'All done with arcs...'
else:
print 'Arcs already processed'
#Next handle the twilight flat
if not os.path.isfile("DATACUBE_SKYFLAT.fits"):
print 'Processing the twiflat...'
rdx.make_twiflat(xml_info, nproc=nproc)
print 'All done with twiflat...'
else:
print 'Twiflat already processed'
#Next calibrate standard star
if not os.path.isfile("STD_RED_0001.fits"):
print 'Processing the standard star...'
rdx.make_stdstar(xml_info, nproc=nproc)
print 'All done with standard star...'
else:
print 'Standard star already processed'
#Next generate flux table
if not os.path.isfile("STD_FLUXES_0001.fits"):
print 'Processing the flux table...'
rdx.make_stdflux(xml_info, nproc=nproc)
print 'All done with flux table...'
else:
print 'Flux table already processed'
#Next calibrate objects
if not os.path.isfile("OBJECT_RED_0001.fits"):
print 'Processing the objects...'
rdx.make_objects(xml_info, nproc=nproc)
print 'All done with objects...'
else:
print 'Objects already processed'
#Finally, process science
print('Preparing intermediate data cubes...')
rdx.make_cubes(xml_info, nproc=nproc)
#In the end, handle sky offsets if present
print('Checking if sky offsets are present and preparing sky model')
rdx.make_skymodel(xml_info, nproc=nproc)
#Done - back to original directory!
print('All done with basic redux...')
os.chdir(currdir)
return xml_info
def cubex_process(self,catalogue,xml_info,path='./',refcube=None,highsn=None):
"""
Take individual cubes and process them with CubEx to tweak the illumination and perform sky subtraction
Needs a catalogue of sources in the field, (ra, dec) one per line, so as to realign the WCS to
absolute references
CubEx is a privite code by S. Cantalupo and cannot be redistributed. Contact the author directly.
path - the top level folder where data reduction has to be performed.
This includes a folder Proc with the processed datacube
catalogue is catalogue used for ra dec alignement
xml_info is xml_info used in reduction
refcube a reference cube used to resample WCS
highsn a combined, sky subtracted, high signal to noise cube used for the last pass
of sky subtraction
"""
#now start reduction. Enter the proc folder
import os
import glob
import subprocess
import muse_redux_cubex as cx
import muse_utils as utl
import muse_redux_basic as rdx
import multiprocessing
import numpy as np
currdir=os.getcwd()
os.chdir(path+'Proc')
print 'Changing dir to proc...'
########################################
# do a first loop of cubex fix and sky #
########################################
#Search how many exposures are there
scils=glob.glob("OBJECT_RED_0*.fits*")
nsci=len(scils)
#do it in parallel on exposures
workers=[]
for dd in range(nsci):
#reconstruct the name
pixtab="PIXTABLE_REDUCED_EXP{0:d}.fits".format(dd+1)
cube="DATACUBE_FINAL_EXP{0:d}.fits".format(dd+1)
#now launch the task
p = multiprocessing.Process(target=cx.fixandsky_firstpass,args=(cube,pixtab,True,))
workers.append(p)
p.start()
#wait for completion of all of them
for p in workers:
if(p.is_alive()):
p.join()
########################################
# compute offsets and re-project cubes #
########################################
#space
ra_off=[]
dec_off=[]
if not os.path.isfile('radecoffsets.txt'):
print 'Compute offsets to reference...'
for dd in range(nsci):
#reconstruct the name
cube="DATACUBE_FINAL_EXP{0:d}_skysub.fits".format(dd+1)
#Compute the offsets
offra,offdec=utl.aligntocat(cube,currdir+'/'+catalogue)
ra_off.append(offra)
dec_off.append(offdec)
#write to disk offsets
np.savetxt('radecoffsets.txt',(ra_off,dec_off))
else:
print 'Offsets file exists.. loading'
off=open('radecoffsets.txt','r')
ra_off=[float(ii) for ii in off.readline().strip().split()]
dec_off=[float(ii) for ii in off.readline().strip().split()]
off.close()
#now reproject cubes with offsets
if(refcube):
print 'Using reference cube for wcs...'
rdx.make_cubes(xml_info,nproc=12,wcsoff=[ra_off,dec_off],refcube=currdir+'/'+refcube)
else:
print 'Computing reference WCS on data themselves...'
rdx.make_cubes(xml_info,nproc=12,wcsoff=[ra_off,dec_off])
######################################################
# run a second iter of cubex fix and sky #
# with realigned images mostly to find sources for #
# masking #
######################################################
#do it in parallel on exposures
workers=[]
for dd in range(nsci):
#reconstruct the name
pixtab="PIXTABLE_REDUCED_EXP{0:d}_off.fits".format(dd+1)
cube="DATACUBE_FINAL_EXP{0:d}_off.fits".format(dd+1)
#now launch the task
p = multiprocessing.Process(target=cx.fixandsky_firstpass,args=(cube,pixtab,True,))
workers.append(p)
p.start()
#wait for completion of all of them
for p in workers:
if(p.is_alive()):
p.join()
##########################################
# run a third iter of cubex fix and sky #
# with better masking on sources #
##########################################
if(highsn):
#run the loop
print 'Do third pass of cubex..'
#do it in parallel on exposures
workers=[]
for dd in range(nsci):
#reconstruct the name
pixtab="PIXTABLE_REDUCED_EXP{0:d}_off.fits".format(dd+1)
cube="DATACUBE_FINAL_EXP{0:d}_off.fits".format(dd+1)
#now launch the task
p = multiprocessing.Process(target=cx.fixandsky_secondpass,args=(cube,pixtab,True,currdir+'/'+highsn))
workers.append(p)
p.start()
#wait for completion of all of them
for p in workers:
if(p.is_alive()):
p.join()
else:
print 'High SN cube not provided.. skip step 3'
#Done - back to original directory!
print 'All done with fancy redux... Ready to coadd'
os.chdir(currdir)
