def align_combine(fitsdir, myfilter, examine=True):
from pyraf import iraf
iraf.noao(_doprint=0)
iraf.digiphot(_doprint=0)
iraf.apphot(_doprint=0)
os.chdir(fitsdir)
listfiles = glob.glob(myfilter)
listfiles.sort()
if (examine):
print "Opening ",listfiles[0]," to examine."
iraf.imexamine(input=listfiles[0], \
logfile="coords.dat", \
keeplog="yes")
with open("align.list",'w') as f:
for i in listfiles:
f.write(i+"\n")
print "Aligning with reference:",listfiles[0]
iraf.imalign( input = "@align.list", referenc= listfiles[0], coords = "coords.dat", output = "*****@*****.**")
listfiles = glob.glob("a_"+myfilter)
listfiles.sort()
with open("comb.list",'w') as f:
for i in listfiles:
f.write(i+"\n")
print "Combining"
iraf.imcombine(input = "@comb.list",\
output = "out.fits",\
combine= "median")
def align_combine(fitsdir, myfilter, examine=True):
from pyraf import iraf
iraf.noao(_doprint=0)
iraf.digiphot(_doprint=0)
iraf.apphot(_doprint=0)
os.chdir(fitsdir)
listfiles = glob.glob(myfilter)
listfiles.sort()
if (examine):
print "Opening ",listfiles[0]," to examine."
iraf.imexamine(input=listfiles[0], \
logfile="coords.dat", \
keeplog="yes")
with open("align.list",'w') as f:
for i in listfiles:
f.write(i+"\n")
print "Aligning with reference:",listfiles[0]
iraf.imalign( input = "@align.list", referenc= listfiles[0], coords = "coords.dat", output = "*****@*****.**")
listfiles = glob.glob("a_"+myfilter)
listfiles.sort()
with open("comb.list",'w') as f:
for i in listfiles:
f.write(i+"\n")
print "Combining"
iraf.imcombine(input = "@comb.list",\
output = "out.fits",\
combine= "median")
def check():
lstlst = ['objlst']
if os.path.isfile('objlst'):
webbrowser.open('objlst')
webbrowser.open('../errfilelst')
iraf.imexamine(input='@objlst', frame=1)
print '<<<<<check the list>>>>>'
def checkfile(filename):
'''Print statistics and run open imexamine task'''
iraf.imstatistics.unlearn()
iraf.imexamine.unlearn()
print 'Check output file:'
iraf.imstatistics(filename)
print ' Running "imexamine" task..'
iraf.imexamine(filename, 1)
def checkfile(filename):
'''Print statistics and run open imexamine task'''
iraf.imstatistics.unlearn()
iraf.imexamine.unlearn()
print 'Check output file:'
iraf.imstatistics(filename)
print ' Running "imexamine" task..'
iraf.imexamine(filename, 1)
def check():
lstlst = [
'spec_bias.lst', 'halogen.lst', 'lamp.lst', 'std.lst', 'cor_std.lst'
]
for i in lstlst:
if os.path.isfile(i):
webbrowser.open(i)
iraf.imexamine(input='@%s' % i, frame=1)
if 'i' == 'cor_std.lst':
break
def check_bias():
biaspath = os.getcwd() + os.sep + 'bias'
if os.path.isfile(biaspath + os.sep + 'spec_bias.lst'):
os.chdir('bias')
webbrowser.open('spec_bias.lst')
iraf.imexamine(input='@spec_bias.lst[1]', frame=1)
dirname = os.path.dirname(os.getcwd())
os.chdir(dirname)
iraf.flpr()
else:
print('no bias dir in ' + os.getcwd())
def check_bias():
biaspath = os.getcwd() + os.sep + 'bias'
if os.path.isfile(biaspath + os.sep + 'spec_bias.lst'):
os.chdir('bias')
os.system('gedit spec_bias.lst &')
iraf.imexamine(input = '@spec_bias.lst[1]', frame = 1)
dirname, filename = os.path.split(os.getcwd())
os.chdir(dirname)
iraf.flpr()
else:
print('no bias dir in ' + os.getcwd())
def getfwhm(images='@imh.lis', coordlist='ref_stars', outfile='getfwhm.log',radius=4.0,buffer=7.0,width=5.0,rplot=15.0,center='no',verbose='no',imagelist=None,mode='al',DOLLARnargs=0,taskObj=None):
Vars = IrafParList('getfwhm')
Vars.addParam(makeIrafPar(images, datatype='string', name='images',mode='a',prompt='Input image(s)'))
Vars.addParam(makeIrafPar(coordlist, datatype='string', name='coordlist',mode='a',prompt='List of object positions'))
Vars.addParam(makeIrafPar(outfile, datatype='string', name='outfile',mode='a',prompt='Output file'))
Vars.addParam(makeIrafPar(radius, datatype='real', name='radius', mode='h',prompt='Object radius'))
Vars.addParam(makeIrafPar(buffer, datatype='real', name='buffer', mode='h',prompt='Background buffer width'))
Vars.addParam(makeIrafPar(width, datatype='real', name='width', mode='h',prompt='Background width'))
Vars.addParam(makeIrafPar(rplot, datatype='real', name='rplot', mode='h',prompt='Plotting radius'))
Vars.addParam(makeIrafPar(center, datatype='bool', name='center', mode='h',prompt='Center object in aperture?'))
Vars.addParam(makeIrafPar(verbose, datatype='bool', name='verbose',mode='h',prompt='Verbose output?'))
Vars.addParam(makeIrafPar(imagelist, datatype='struct', name='imagelist',list_flag=1,mode='h'))
Vars.addParam(makeIrafPar(mode, datatype='string', name='mode', mode='h'))
Vars.addParam(makeIrafPar(DOLLARnargs, datatype='int', name='$nargs',mode='h'))
Vars.addParam(makeIrafPar(None, datatype='int', name='len', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='image', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='imagefile',mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='imlist', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='coords', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='outputfile',mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='rad', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='buff', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='wid', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='rpl', mode='u'))
Vars.imlist = Vars.images
Vars.imagefile = iraf.mktemp('tmp$getfwhm')
iraf.sections(Vars.imlist, option = 'fullname', Stdout=Vars.imagefile)
Vars.imagelist = Vars.imagefile
Vars.coords = Vars.coordlist
Vars.outputfile = Vars.outfile
Vars.rad = Vars.radius
Vars.buff = Vars.buffer
Vars.wid = Vars.width
Vars.rpl = Vars.rplot
iraf.rimexam.radius = Vars.rad
iraf.rimexam.buffer = Vars.buff
iraf.rimexam.width = Vars.wid
iraf.rimexam.rplot = Vars.rpl
if (Vars.center == yes):
iraf.rimexam.center = yes
else:
iraf.rimexam.center = no
iraf.rimexam.fittype = 'gaussian'
iraf.rimexam.iterati = 1
iraf.clPrint('# RIMEXAM Parameter Settings: Radius=', Vars.rad,', Buffer=',Vars.buff,', Width=',Vars.wid,StdoutAppend=Vars.outputfile)
while (iraf.fscan(locals(), 'Vars.imagelist', 'Vars.image') != EOF):
Vars.len = iraf.strlen(Vars.image)
if (iraf.substr(Vars.image, Vars.len - 3, Vars.len) == '.imh'):
Vars.image = iraf.substr(Vars.image, 1, Vars.len - 4)
if (Vars.verbose):
iraf.clPrint('...processing ', Vars.image)
iraf.clPrint(Vars.image)
iraf.imexamine(Vars.image, logfile = Vars.outputfile, keeplog = yes,defkey = 'a',imagecur = Vars.coords,wcs = 'world',use_display = no)
def check_other(path):
if os.path.isdir(path):
os.chdir(path)
lstlst = ['halogen.lst', 'lamp.lst', 'cor_lamp.lst','std.lst','cor_std.lst']
for i in lstlst:
if os.path.isfile(i):
os.system('gedit %s &' % i)
iraf.imexamine(input = '@%s[1]'%i, frame = 1)
dirname, filename = os.path.split(os.getcwd())
os.chdir(dirname)
iraf.flpr()
else:
print('no dir ' + path + ' in ' + os.getcwd())
def check_other(path):
if os.path.isdir(path):
os.chdir(path)
lstlst = [
'halogen.lst', 'lamp.lst', 'cor_lamp.lst', 'std.lst', 'cor_std.lst'
]
for i in lstlst:
if os.path.isfile(i):
webbrowser.open(i)
iraf.imexamine(input='@%s[1]' % i, frame=1)
dirname, filename = os.path.split(os.getcwd())
os.chdir(dirname)
iraf.flpr()
else:
print('no dir ' + path + ' in ' + os.getcwd())
def check_bias():
print 'check bias...'
print '***please remove the bad bias from the list***'
f = open('bias.lst')
l = f.readlines()
f.close()
if len(l) != 0:
os.popen("gedit bias.lst &")
iraf.imexamine(input = '@bias.lst//[1]', frame = 1)
else:
os.remove('bias.lst')
label = raw_input('bias.lst has no fits files, do you want to use older bias?')
if label == 'y' or label == 'Y' or label == 'yes' or label == 'Yes':
path = raw_input('Please input the path of the file:')
print 'copying older flat ' + path + '...'
shutil.copy(path, './')
def check_obj():
print 'check object...'
print '***please correct the wrong fits in the list***'
name = os.popen('ls object*.lst').readlines()
name = [i.split('\n')[0] for i in name]
for i in name:
f = open(i)
l = f.readlines()
f.close()
l = [i2.split('\n')[0] for i2 in l if '.fits' in i2]
output = open('temp.lst', 'w')
for i2 in l:
output.write(i2 + '\n')
output.close()
os.popen("gedit " + i + " &")
iraf.imexamine(input = '@temp.lst//[1]', frame = 1)
os.remove("temp.lst")
def shift_align(filenames):
if len(filenames) == 0:
return ''
fno = 1
for i in filenames:
iraf.display(image = i, frame = fno)
fno += 1
print 'The fits number is', len(filenames)
if len(filenames) > 1:
print 'Please check the fits pic and determine whether you need to shift the pic'
print 'imexamine...'
iraf.imexamine()
valget = raw_input('Are you need to shift the fits picture?(y)')
if valget == 'y' or valget == 'Y':
nfilenames = [filenames[0]]
for i2 in filenames:
print 'implot ' + i2
iraf.implot(image = i2)
fno = 1
iraf.immatch()
while fno < len(filenames):
valget = raw_input('Please input ' + filenames[fno] + ' xshift, yshift: ')
valget = valget.split()
fxshift = float(valget[0])
fyshift = float(valget[1])
ims_key = 1
if os.path.isfile('shift_' + filenames[fno]):
valget = raw_input('shift_' + filenames[fno] + ' is already exist, are you want to delete the old one?(y):')
if valget == 'y' or valget == 'Y' or valget == 'yes' or valget == 'Yes':
os.remove('shift_' + filenames[fno])
else:
ims_key = 0
if ims_key == 1:
print 'what happend????????????????'
iraf.imshift(input = filenames[fno]
, output = 'shift_' + filenames[fno], xshift = fxshift
, yshift = fyshift, shifts_file = '', interp_type = 'linear'
, boundary_type = 'nearest', constant = 0.0)
nfilenames.append('shift_' + filenames[fno])
fno += 1
for i2 in xrange(len(nfilenames)):
iraf.display(image = nfilenames[i2], frame = i2 + 1)
iraf.imexamine()
return cos_clear(nfilenames)
return cos_clear(filenames)
def _profiler(self,coordfile,coord):
# deploy task to pyraf
results = iraf.imexamine(self.filename,image=self.filename,use_display='no',logfile='',defkey='r',imagecur=coordfile,frame=1,mode='h',StdoutG=self.tempradfile.name,Stdout=1)
try:
results = results[0].split()
# prad frad flux bgd mpeak ellip pa mbeta 2dfwhm mfwhm fwhm
except IndexError:
# some error
results = [np.nan]*len(self.R_COLMAP)
# first, process stdout
for idx,r in enumerate(results):
try:
results[idx] = np.float(r)
except ValueError:
results[idx] = np.nan
results = OrderedDict(zip(self.R_COLMAP,results))
tbl = Table([results])
tbl = tbl[self.R_COLMAP]
tbl['flux'].unit = u.ct
tbl['bgd'].unit = u.ct
tbl['mpeak'].unit = u.ct
tbl['pa'].unit = u.deg
#tbl['2dfwhm'].unit = u.pix
tbl['mfwhm'].unit = u.pix
tbl['fwhm'].unit = u.pix
# add xi,yi
xi,yi = (np.float(i) for i in coord)
tbl.add_column(Column([xi],name='xi',format='%.2f'),0)
tbl.add_column(Column([yi],name='yi',format='%.2f'),1)
#remove 2dfwhm cuz wut?
tbl.remove_column('2dfwhm')
#add arcsec columns
for fwhmcol in tbl.colnames[-2:]:
try:
val = tbl[fwhmcol]*self.pxscale
except TypeError:
val = [np.nan]
tbl.add_column(Column(val,name='%s_s'%fwhmcol,unit=u.arcsec,format='%.3f'),tbl.index_column(fwhmcol)+1)
# process profile graphics
gki = iraf.gkidecode(self.tempradfile.name,Stdout=1,verbose=True)
gki = '\n'.join(gki)
xr,yr,xf,yf = self.extract_gkidata(gki)
vals = [tbl[x][0] for x in tbl.colnames] + [xr,yr,xf,yf,tbl]
p = Profile(*vals)
return p
def label_objects(images, xfield, yfield):
'''Given a list of images, allow the user to pick an object in the
display and have the x and y coordinates saved as header keywords
xfield and yfield.'''
files = get_files(images)
print "Please use the 'a' key to select objects"
for file in files:
iraf.display(file, 1)
res = iraf.imexamine(file, Stdout=1)
#res = iraf.rimcursor(file, Stdout=1)
x, y = map(float, (string.split(res[2])[0:2]))
iraf.hedit(images=file, fields=xfield, value=x, add=1, verify=0)
iraf.hedit(images=file, fields=yfield, value=y, add=1, verify=0)
def check_flat():
print 'check flat...'
print '***please remove the bad flat from the list***'
name = os.popen('ls *flat.lst').readlines()
name1 = [i.split('\n')[0] for i in name if '_no_flat' not in i]
name2 = [i.split('\n')[0] for i in name if '_no_flat' in i]
for i in name1:
os.popen("gedit " + i + " &")
iraf.imexamine(input = '@' + i + '//[1]', frame = 1)
for i in name2:
if i.replace('_no','') not in name1:
label = raw_input(i + " has no flat fits, do you want use older flat?")
if label == 'y' or label == 'Y' or label == 'yes' or label == 'Yes':
path = raw_input('Please input the path of the lstfile:')
print 'coping older lstflat ' + path + ' as new name ' + i.replace('_no','') + '...'
shutil.copy(path, './' + i.replace('_no',''))
path = path[0:path.rfind('/')]
file1 = open(i.replace('_no',''))
file1_ctent = file1.readlines()
file1.close()
file1_ctent = [j.split('\n')[0] for j in file1_ctent]
for j in file1_ctent:
print 'coping ' + j + '...'
shutil.copy(path + '/' + j, './')
def ecpsf(img, ofwhm, threshold, psfstars, distance, interactive, psffun='gauss', fixaperture=False, _catalog='', _datamax=None, show=False):
try:
import lsc, string
hdr = lsc.util.readhdr(img + '.fits')
instrument = lsc.util.readkey3(hdr, 'instrume')
print 'INSTRUMENT:', instrument
if 'PIXSCALE' in hdr:
scale = lsc.util.readkey3(hdr, 'PIXSCALE')
elif 'CCDSCALE' in hdr:
if 'CCDXBIN' in hdr:
scale = lsc.util.readkey3(hdr, 'CCDSCALE') * lsc.util.readkey3(hdr, 'CCDXBIN')
elif 'CCDSUM' in hdr:
scale = lsc.util.readkey3(hdr, 'CCDSCALE') * int(string.split(lsc.util.readkey3(hdr, 'CCDSUM'))[0])
if _datamax is None:
_datamax = lsc.util.readkey3(hdr, 'datamax')
_wcserr = lsc.util.readkey3(hdr, 'wcserr')
print _wcserr
if float(_wcserr) == 0:
if 'L1FWHM' in hdr:
seeing = float(lsc.util.readkey3(hdr, 'L1FWHM'))
elif 'L1SEEING' in hdr:
seeing = float(lsc.util.readkey3(hdr, 'L1SEEING')) * scale
else:
seeing = 3
else:
seeing = 3
if 'PSF_FWHM' in hdr:
seeing = float(lsc.util.readkey3(hdr, 'PSF_FWHM'))
else:
sys.exit('astrometry not good')
#except: sys.exit('astrometry not good')
fwhm = seeing / scale
print 'FWHM[header] ', fwhm, ' in pixel'
if ofwhm: fwhm = float(ofwhm)
print ' FWHM[input] ', fwhm, ' in pixel'
xdim, ydim = iraf.hselect(img+'[0]', 'i_naxis1,i_naxis2', 'yes', Stdout=1)[0].split()
print img, fwhm, threshold, scale,xdim
#################################################################################
################### write file to compute psf _psf.coo ############
#################################################################################
if _catalog:
print '\n#### use catalog to measure the psf'
ddd=iraf.wcsctran(input=_catalog,output='STDOUT',Stdout=1,image=img + '[0]',inwcs='world',outwcs='logical',
units='degrees degrees',columns='1 2',formats='%10.1f %10.1f',verbose='no')
ddd=[i for i in ddd if i[0]!='#']
ddd=[' '.join(i.split()[0:3]) for i in ddd]
line=''
for i in ddd:
a,b,c = string.split(i)
if float(a) < float(xdim) and float(b) < float(ydim) and float(b) > 0:
line = line + '%10s %10s %10s \n' % (a, b, c)
if line:
ff = open('_psf.coo', 'w')
ff.write(line)
ff.close()
else:
sys.exit('error: no catalog objects are in the field')
elif interactive:
iraf.display(img + '[0]', 1, fill=True)
iraf.delete('tmp.lo?', verify=False)
print '_' * 80
print '>>> Mark reference stars with "a". Then "q"'
print '-' * 80
iraf.imexamine(img, 1, wcs='logical', logfile='tmp.log', keeplog=True)
xyrefer = iraf.fields('tmp.log', '1,2,6,15', Stdout=1)
xns, yns, _fws = [], [], []
############# write file for PSF #########################
ff = open('_psf.coo', 'w')
for i in range(len(xyrefer)):
xns.append(float(xyrefer[i].split()[0]))
yns.append(float(xyrefer[i].split()[1]))
_fws.append(float(xyrefer[i].split()[3]))
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
ff.close()
fwhm = np.median(_fws)
else:
############ run sextractor #####################################
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
tot = np.compress(abs(np.array(fluxrad) * 1.6 - fwhm) / fwhm < .5, fluxrad)
if len(tot) < 5:
print 'warning: fwhm from sexractor different from fwhm computed during pre-reduction'
print 'try using option --fwhm xxx'
ff = open('tmp.cursor', 'w')
image_hdu = fits.open(img + '.fits')
for i in range(len(xs)):
_xs = np.delete(xs, i)
_ys = np.delete(ys, i)
dist2 = np.sqrt((_xs - xs[i]) ** 2 + (_ys - ys[i]) ** 2)
########### cut star, not near other object ##########################
if abs(fluxrad[i] * 1.6 - fwhm) / fwhm < .5 and min(dist2) > distance * fwhm:
x1, x2 = int(xs[i] - fwhm * 3), int(xs[i] + fwhm * 3)
y1, y2 = int(ys[i] - fwhm * 3), int(ys[i] + fwhm * 3)
if x1 < 1: x1 = 1
if y1 < 1: y1 = 1
if x2 > int(xdim):
x2 = int(xdim)
if y2 > int(ydim):
y2 = int(ydim)
fmax = np.max(image_hdu[0].data[y1-1:y2, x1-1:x2])
########## cut saturated object ########################
if float(fmax) < _datamax: # not saturated
ff.write('%10.3f %10.3f 1 m \n' % (xs[i], ys[i]))
ff.close()
image_hdu.close()
iraf.delete('tmp.lo?,tmp.sta?,tmp.gk?', verify=False)
iraf.psfmeasure(img+'[0]', imagecur='tmp.cursor', logfile='tmp.log', radius=int(fwhm), iter=3,
display=False, StdoutG='tmp.gki')
ff = open('tmp.log')
righe = ff.readlines()
xn = [float(righe[3].split()[1])]
yn = [float(righe[3].split()[2])]
_fw = [float(righe[3].split()[4])]
for r in righe[4:-2]:
if len(r) > 0:
xn.append(float(r.split()[0]))
yn.append(float(r.split()[1]))
_fw.append(float(r.split()[3]))
print 'FWHM: ', righe[-1].split()[-1]
print 80 * "#"
######
############## eliminate double object identification ###########################
xns, yns, _fws = [xn[0]], [yn[0]], [_fw[0]]
for i in range(1, len(xn)):
if abs(xn[i] - xn[i - 1]) > .2 and abs(yn[i] - yn[i - 1]) > .2:
xns.append(xn[i])
yns.append(yn[i])
_fws.append(_fw[i])
######### write clean file for PSF #########################
fw = []
ff = open('_psf.coo', 'w')
for i in range(len(xns)):
if abs(_fws[i] - fwhm) / fwhm < .3:
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
fw.append(_fws[i])
ff.close() ## End automatic selection
######################################################################################
################### write file of object to store in fits table #############
######################################################################################
if _catalog:
ddd=iraf.wcsctran(input=_catalog,output='STDOUT',Stdout=1,image=img + '[0]',inwcs='world',outwcs='logical',
units='degrees degrees',columns='1 2',formats='%10.1f %10.1f',verbose='no')
ddd=[i for i in ddd if i[0]!='#']
ddd=[' '.join(i.split()[0:3]) for i in ddd]
ff = open('_psf2.coo', 'w')
for i in ddd:
a,b,c = string.split(i)
ff.write('%10s %10s %10s \n' % (a, b, c))
ff.close()
elif interactive:
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
ff = open('_psf2.coo', 'w')
for i in range(len(xs)):
ff.write('%10s %10s %10s \n' % (xs[i], ys[i], fluxrad[i]))
ff.close()
else:
os.system('cp _psf.coo _psf2.coo')
# dflux = fluxrad - np.median(fluxrad)
# fstar = np.compress(dflux < np.std(fluxrad), fluxrad)
#################################################################################################################
print 80 * "#"
photmag, pst, fitmag = psffit(img, fwhm, psfstars, hdr, interactive, _datamax, psffun, fixaperture)
photmag2, fitmag2 = psffit2(img, fwhm, psfstars, hdr, _datamax, psffun, fixaperture)
radec = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag,
Stdout=1, image=img + '[0]', inwcs='logical', outwcs='world', columns="1 2",
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
radec2 = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag2,
Stdout=1, image=img + '[0]', inwcs='logical', outwcs='world', columns="1 2",
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
if interactive or show:
iraf.set(stdimage='imt1024')
iraf.display(img + '[0]', 1, fill=True, Stdout=1)
iraf.tvmark(1, coords='STDIN', mark='circle', radii=15, label=True, Stdin=photmag, nxoffset=5, nyoffset=5, txsize=2)
iraf.tvmark(1, coords='STDIN', mark='circle', radii=35, label=False, Stdin=pst, color=208)
# iraf.tvmark(1, coords='STDIN', mark='cross', length=35, label=False, Stdin=fitmag2, color=204)
idpsf = []
for i in range(len(pst)):
idpsf.append(pst[i].split()[2])
dmag = []
for i in range(len(radec)):
ra, dec, idph, magp2, magp3, magp4, merrp2, merrp3, merrp4 = radec[i].split()
dmag.append(9.99)
for j in range(len(fitmag)):
raf, decf, idf, magf, magerrf = fitmag[j].split()
if idph == idf and idph in idpsf and \
magp3 != 'INDEF' and magf != 'INDEF':
dmag[i] = float(magp3) - float(magf)
break
_dmag = np.compress(np.array(dmag) < 9.99, np.array(dmag))
print '>>> Aperture correction (phot) %6.3f +/- %5.3f %3d ' % \
(np.mean(_dmag), np.std(_dmag), len(_dmag))
if len(_dmag) > 3:
_dmag = np.compress(np.abs(_dmag - np.median(_dmag)) < 2 * np.std(_dmag), _dmag)
print '>>> 2 sigma rejection) %6.3f +/- %5.3f %3d [default]' \
% (np.mean(_dmag), np.std(_dmag), len(_dmag))
print '>>> fwhm %s ' % (str(fwhm))
for i in range(len(dmag)):
if dmag[i] == 9.99:
dmag[i] = ''
else:
dmag[i] = '%6.3f' % (dmag[i])
exptime = lsc.util.readkey3(hdr, 'exptime')
object = lsc.util.readkey3(hdr, 'object').replace(' ', '')
filtro = lsc.util.readkey3(hdr, 'filter')
#######################################
rap, decp, magp2, magp3, magp4, smagf, merrp3, smagerrf = [], [], [], [], [], [], [], []
rap0, decp0 = [], []
for i in range(len(radec2)):
aa = radec2[i].split()
rap.append(aa[0])
decp.append(aa[1])
rap0.append(lsc.lscabsphotdef.deg2HMS(ra=aa[0]))
decp0.append(lsc.lscabsphotdef.deg2HMS(dec=aa[1]))
idp = aa[2]
magp2.append(aa[3])
magp3.append(aa[4])
magp4.append(aa[5])
merrp3.append(aa[7])
_smagf, _smagerrf = 9999, 9999
for j in range(len(fitmag2)):
raf, decf, idf, magf, magerrf = fitmag2[j].split()
if idf == idp:
_smagf = magf
_smagerrf = magerrf
break
smagf.append(_smagf)
smagerrf.append(_smagerrf)
tbhdu = fits.BinTableHDU.from_columns(fits.ColDefs([fits.Column(name='ra', format='20A', array=np.array(rap)),
fits.Column(name='dec', format='20A', array=np.array(decp)),
fits.Column(name='ra0', format='E', array=np.array(rap0)),
fits.Column(name='dec0', format='E', array=np.array(decp0)),
fits.Column(name='magp2', format='E',
array=np.array(np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
fits.Column(name='magp3', format='E',
array=np.array(np.where((np.array(magp3) != 'INDEF'),
np.array(magp3), 9999), float)),
fits.Column(name='merrp3', format='E',
array=np.array(np.where((np.array(merrp3) != 'INDEF'),
np.array(merrp3), 9999), float)),
fits.Column(name='magp4', format='E',
array=np.array(np.where((np.array(magp4) != 'INDEF'),
np.array(magp4), 9999), float)),
fits.Column(name='smagf', format='E',
array=np.array(np.where((np.array(smagf) != 'INDEF'),
np.array(smagf), 9999), float)),
fits.Column(name='smagerrf', format='E',
array=np.array(np.where((np.array(smagerrf) != 'INDEF'),
np.array(smagerrf), 9999),
float)),
]))
hdu = fits.PrimaryHDU(header=hdr)
thdulist = fits.HDUList([hdu, tbhdu])
lsc.util.delete(img + '.sn2.fits')
thdulist.writeto(img + '.sn2.fits')
lsc.util.updateheader(img + '.sn2.fits', 0, {'APCO': [np.mean(_dmag), 'Aperture correction']})
lsc.util.updateheader(img + '.sn2.fits', 0, {'APCOERR': [np.std(_dmag), 'Aperture correction error']})
lsc.util.updateheader(img + '.sn2.fits', 0, {'XDIM': [lsc.util.readkey3(hdr, 'naxis1'), 'x number of pixels']})
lsc.util.updateheader(img + '.sn2.fits', 0, {'YDIM': [lsc.util.readkey3(hdr, 'naxis2'), 'y number of pixels']})
lsc.util.updateheader(img + '.sn2.fits', 0,
{'PSF_FWHM': [fwhm * scale, 'FWHM (arcsec) - computed with daophot']})
os.chmod(img + '.sn2.fits', 0664)
os.chmod(img + '.psf.fits', 0664)
result = 1
except:
result = 0
fwhm = 0.0
traceback.print_exc()
return result, fwhm * scale
if not os.path.isdir('flat_files'):
os.mkdir('flat_files')
allfiles = flatlist
for file in allfiles:
shutil.copy(file, 'flat_files/')
# combine flat images
print 'Combining flat images ...'
iraf.ccdred.flatcombine.ccdtype = ''
iraf.ccdred.flatcombine.process = 'no'
iraf.ccdred.flatcombine.reject = 'ccdclip'
iraf.ccdred.flatcombine.rdnoise = 'rdnoise'
iraf.ccdred.flatcombine.gain = 'gain'
iraf.ccdred.flatcombine.output = 'Flat'
iraf.ccdred.flatcombine(input=flatin)
for file in flatlist:
os.remove(file)
print 'openning a ds9 window if not already openned...'
ds9.ds9()
# check output flat image
print 'Check output file:'
iraf.imstatistics('Flat')
print ' Running "imexamine" task..'
iraf.imexamine('Flat', 1)
print '--- DONE ---'
def main():
print '=' * 20 + ' check wcal2d ' + '=' * 20
iraf.imexamine('wftbo//@cor_halogen.lst', frame=1)
def ecpsf(img, ofwhm, threshold, interactive, ds9, fixaperture=False,_catalog=''):
try:
import agnkey
import string
hdr = agnkey.util.readhdr(img + '.fits')
instrument = agnkey.util.readkey3(hdr, 'instrume')
print 'INSTRUMENT:', instrument
if 'PIXSCALE' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'PIXSCALE')
elif 'CCDSCALE' in hdr:
if 'CCDXBIN' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'CCDSCALE') * agnkey.util.readkey3(hdr, 'CCDXBIN')
elif 'CCDSUM' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'CCDSCALE') * int(
string.split(agnkey.util.readkey3(hdr, 'CCDSUM'))[0])
if instrument in ['kb05', 'kb70', 'kb71', 'kb73', 'kb74', 'kb75', 'kb76', 'kb77', 'kb78', 'kb79']:
scale = pixelscale
_datamax = 45000
elif instrument in ['fl02', 'fl03', 'fl04']:
scale = pixelscale
_datamax = 120000
elif instrument in ['fs01', 'em03']:
scale = pixelscale
_datamax = 65000
elif instrument in ['fs02', 'fs03']:
scale = pixelscale
_datamax = 65000
elif instrument in ['em01']:
scale = pixelscale
_datamax = 65000
try:
_wcserr = agnkey.util.readkey3(hdr, 'wcserr')
if float(_wcserr) == 0:
if instrument in ['kb05', 'kb70', 'kb71', 'kb73', 'kb74', 'kb75', 'kb76', 'kb77', 'kb78', 'kb79']:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif instrument in ['fl02', 'fl03', 'fl04']:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif instrument in ['fs01', 'fs02', 'fs03', 'em03', 'em01']:
if 'L1FWHM' in hdr:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'L1SEEING' in hdr:
seeing = float(agnkey.util.readkey3(hdr, 'L1SEEING')) * scale
else:
seeing = 3
else:
seeing = 3
else:
seeing = float(agnkey.util.readkey3(hdr, 'PSF_FWHM'))
sys.exit('astrometry not good')
except:
sys.exit('astrometry not good')
fwhm = seeing / scale
print 'FWHM[header] ', fwhm, ' in pixel'
if ofwhm:
fwhm = float(ofwhm)
print ' FWHM[input] ', fwhm, ' in pixel'
if interactive:
iraf.display(img, 1, fill=True)
iraf.delete('tmp.lo?', verify=False)
print '_' * 80
print '>>> Mark reference stars with "a". Then "q"'
print '-' * 80
iraf.imexamine(img, 1, wcs='logical', logfile='tmp.log', keeplog=True)
xyrefer = iraf.fields('tmp.log', '1,2,6,15', Stdout=1)
xns, yns, _fws = [], [], []
ff = open('_ap.coo', 'w')
for i in range(len(xyrefer)):
xns.append(float(xyrefer[i].split()[0]))
yns.append(float(xyrefer[i].split()[1]))
_fws.append(float(xyrefer[i].split()[3]))
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
ff.close()
elif _catalog:
# cat1=agnkey.agnastrodef.readtxt(_catalog)
# cat1['ra'],cat1['dec']
ddd=iraf.wcsctran(input=_catalog,output='STDOUT',Stdout=1,image=img,inwcs='world',outwcs='logical',
units='degrees degrees',columns='1 2',formats='%10.1f %10.1f',verbose='no')
ddd=[i for i in ddd if i[0]!='#']
ddd=[' '.join(i.split()[0:3]) for i in ddd]
ff = open('_ap.coo', 'w')
for i in ddd:
a,b,c = string.split(i)
#print a,b,c
ff.write('%10s %10s %10s \n' % (a, b, c))
ff.close()
print 'use catalog'
else:
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
ff = open('_ap.coo', 'w')
for i in range(len(xs)):
ff.write('%10.3f %10.3f %7.2f \n' % (xs[i], ys[i], float(fluxrad[i])))
ff.close() ## End automatic selection
print 80 * "#"
photmag = apfit(img, fwhm, hdr, interactive, _datamax, fixaperture)
radec = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag, \
Stdout=1, image=img, inwcs='logical', outwcs='world', columns="1 2", \
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
exptime = agnkey.util.readkey3(hdr, 'exptime')
object = agnkey.util.readkey3(hdr, 'object').replace(' ', '')
filtro = agnkey.util.readkey3(hdr, 'filter')
#######################################
rap, decp, magp2, magp3, magp4, smagf = [], [], [], [], [], []
merrp2, merrp3, merrp4, smagerrf = [], [], [], []
rap0, decp0 = [], []
for i in range(len(radec)):
aa = radec[i].split()
rap.append(aa[0])
decp.append(aa[1])
rap0.append(agnkey.agnabsphotdef.deg2HMS(ra=aa[0]))
decp0.append(agnkey.agnabsphotdef.deg2HMS(dec=aa[1]))
idp = aa[2]
magp2.append(aa[3])
magp3.append(aa[4])
magp4.append(aa[5])
merrp2.append(aa[6])
merrp3.append(aa[7])
merrp4.append(aa[8])
tbhdu = pyfits.new_table(pyfits.ColDefs([
pyfits.Column(name='ra', format='20A', array=np.array(rap)),
pyfits.Column(name='dec', format='20A', array=np.array(decp)),
pyfits.Column(name='ra0', format='E', array=np.array(rap0)),
pyfits.Column(name='dec0', format='E', array=np.array(decp0)),
pyfits.Column(name='magp2', format='E', array=np.array(np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
pyfits.Column(name='magp3', format='E', array=np.array(np.where((np.array(magp3) != 'INDEF'),
np.array(magp3), 9999), float)),
pyfits.Column(name='magp4', format='E', array=np.array(np.where((np.array(magp4) != 'INDEF'),
np.array(magp4), 9999), float)),
pyfits.Column(name='merrp2', format='E', array=np.array(np.where((np.array(merrp2) != 'INDEF'),
np.array(merrp2), 9999), float)),
pyfits.Column(name='merrp3', format='E', array=np.array(np.where((np.array(merrp3) != 'INDEF'),
np.array(merrp3), 9999), float)),
pyfits.Column(name='merrp4', format='E', array=np.array(np.where((np.array(merrp4) != 'INDEF'),
np.array(merrp4), 9999), float)),
pyfits.Column(name='smagf', format='E', array=np.array(np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
pyfits.Column(name='smagerrf', format='E', array=np.array(np.where((np.array(merrp2) != 'INDEF'),
np.array(merrp2), 9999), float)),
]))
hdu = pyfits.PrimaryHDU(header=hdr)
thdulist = pyfits.HDUList([hdu, tbhdu])
agnkey.util.delete(img + '.sn2.fits')
thdulist.writeto(img + '.sn2.fits')
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'XDIM': [agnkey.util.readkey3(hdr, 'naxis1'), 'x number of pixels']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'YDIM': [agnkey.util.readkey3(hdr, 'naxis2'), 'y number of pixels']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'PSF_FWHM': [fwhm * scale, 'FWHM (arcsec) - computed with daophot']})
os.chmod(img + '.sn2.fits', 0664)
os.chmod(img + '.psf.fits', 0664)
result = 1
except:
result = 0
fwhm = 0.0
traceback.print_exc()
return result, fwhm * scale
_xpos, _ypos = pix1[0][0], pix1[0][1]
else:
_xpos, _ypos = '', ''
if _xpos and _ypos:
print 'use xpos and ypos from fits table'
print _xpos, _ypos
else:
print 'no xpos and ypos define, do that interactively'
jj = 0
while not _xpos or not _ypos:
print " MARK SN REGION WITH - x -, EXIT - q -"
try:
agnkey.util.delete('tmp.log')
zz1, zz2, goon = agnkey.util.display_image(img, 1, '', '', True)
# iraf.display(img,1,fill=True,Stdout=1)
iraf.imexamine(img, 1, wcs='logical', logfile='tmp.log', keeplog=True)
xytargets = iraf.fields('tmp.log', '1,2', Stdout=1)
_xpos, _ypos = string.split(xytargets[0])[0], string.split(xytargets[0])[1]
except:
_xpos, _ypos = '', ''
jj = jj + 1
if jj > 10:
goon = False
break
if goon:
print _xpos, _ypos, _mag
print img0, psfimg, _xpos, _ypos, _mag
imgout = re.sub('.fits', '.temp.fits', string.split(img0, '/')[-1])
agnkey.util.delete('_tmp.fits,_tmp2.fits,_tmp2.fits.art,' + imgout)
xpa('catalog symbol shape text')
if environ == 'mac':
xpa('catalog save sb "' + userPath + '/tmp.catsel"')
elif environ == 'linux':
xpa('catalog save sb "' + userPath + '/tmp.catsel"')
xpa('raise')
iraf.fields('tmp.catsel', '1,2', Stdout='tmp.tv')
answ = 'no'
while answ != 'yes':
print '>> Identify (minimum 2, preferably 3) reference stars (mark with "a") in your image'
iraf.imexamine(img, 1, logfile='tmp.coo', keeplog='yes')
iraf.tvmark(1,
'tmp.coo',
mark="circle",
number='yes',
radii=10,
nxoffse=10,
nyoffse=10,
color=214,
txsize=2)
xycoo = iraf.fields('tmp.coo', '1,2,13', Stdout=1)
print '>> Identify reference stars'
idcat = []
for i in range(len(xycoo)):
idcat.append(int(raw_input('Star ' + str(i + 1) + '= ? ')))
def register_module(img, _system, coordinatelist, interactive, logincl,
_filter):
from snoopy2 import src
import snoopy2
import string, os
# logincl=src.open_program()
from pyraf import iraf
iraf.astcat(_doprint=0)
iraf.imcoords(_doprint=0)
iraf.set(stdimage='imt1024')
iraf.tv.rimexam.backgrou = 'yes'
subdirectory = ['optical/', 'infrared/', 'sloan/']
iraf.delete(coordinatelist + ".tv", verify='no')
iraf.delete(coordinatelist + "_templ.coo", verify='no')
iraf.delete("_templ.*", verify='no')
try:
dir_system = subdirectory[_system]
iraf.fields('home$coordinate_std/' + dir_system + coordinatelist +
'.list',
'2,3,1',
Stdout=coordinatelist + '.tv')
iraf.fields('home$coordinate_std/' + dir_system + coordinatelist +
'.list',
'1',
Stdout='_templ.coo')
iraf.wcsctran(coordinatelist + '.tv',
'_templ.coo2',
'home$coordinate_std/' + dir_system + coordinatelist +
'_templ.fits',
inwcs='world',
units='degrees degrees',
outwcs='logical',
columns='1 2',
formats='%10.1f %10.1f')
a = iraf.fields('_templ.coo', '1', Stdout=1)
b = iraf.fields('_templ.coo2', '1,2', Stdout=1)[2:]
ff = open(coordinatelist + '_templ.coo', 'w')
for i in range(len(a)):
ff.write(b[i] + '\t' + a[i] + ' \n')
ff.close()
if _system == 0 or _system == 2:
standard = iraf.fields('home$coordinate_std/' + dir_system +
coordinatelist + '.list',
'1,4,5,6,7,8',
Stdout=1)
else:
standard = iraf.fields('home$coordinate_std/' + dir_system +
coordinatelist + '.list',
'1,4,5,6',
Stdout=1)
except Exception as e:
print e
print "WARNING: no coordinate " + coordinatelist + " file found in " + snoopy2.__path__[
0] + '/coordinate_std/' + dir_system + ' !!! '
src.close_program(logincl)
stars = []
for i in standard:
nome = string.split(i)
stars.append(nome[0])
# _filter='XXX'
src.delete("tmp." + img + ".coo")
iraf.wcsctran(coordinatelist + '.tv',
'tmp.' + img + '.coo',
img,
inwcs='world',
units='degrees degrees',
outwcs='logical',
columns='1 2',
formats='%10.1f %10.1f')
if interactive:
print '######### Select FRAME TILE on your DS9 !!!!!'
_z1, _z2, goon = src.display_image(
snoopy2.__path__[0] + '/coordinate_std/' + dir_system +
coordinatelist + '_templ.fits', 2, '', '', False)
if not goon: src.close_program(logincl)
iraf.tvmark(2,
coordinatelist + '_templ.coo',
mark="circle",
number='no',
label='yes',
radii=20,
nxoffse=15,
nyoffse=15,
color=214,
txsize=4)
_z1, _z2, goon = src.display_image(img, 1, '', '', False)
if not goon: src.close_program(logincl)
iraf.tvmark(1,
'tmp.' + img + '.coo',
mark="circle",
number='no',
label='yes',
radii=20,
nxoffse=15,
nyoffse=15,
color=205,
txsize=2)
answ = raw_input(
'is the astrometry of the field good ? \n [y/n] ? [y] ')
if not answ: answ = 'y'
if answ == 'n':
try:
src.delete('tmp.' + img + '.coo')
src.delete('tmp.ccdb')
iraf.ccmap('_first.ccmap',
'tmp.ccdb',
images=img,
fitgeome='rscale',
lngunit='degrees',
update='yes',
interact=False)
iraf.wcsctran('_first_image.tv',
'tmp.' + img + '.coo',
img,
inwcs='world',
units='degrees degrees',
outwcs='logical',
columns='1 2',
formats='%10.1f %10.1f')
iraf.tvmark(1,
'tmp.' + img + '.coo',
mark="circle",
number='no',
label='yes',
radii=20,
nxoffse=15,
nyoffse=15,
color=206,
txsize=4)
answ = raw_input(
'AND NOW, is the astrometry of the field good [y/n] ? [y] '
)
if not answ: answ = 'y'
except:
pass
while answ == 'n':
_z1, _z2, goon = src.display_image(img, 1, '', '', False)
if not goon: src.close_program(logincl)
print '>> Identify (minimum 2, preferably 3) reference stars (mark with "a")'
iraf.delete('tmp.coo', verify='no')
iraf.imexamine(img, 1, logfile='tmp.coo', keeplog='yes')
iraf.tvmark(1,
'tmp.coo',
mark="circle",
number='yes',
label='no',
radii=15,
nxoffse=15,
nyoffse=15,
color=214,
txsize=4)
xycoo = iraf.fields('tmp.coo', '1,2,13', Stdout=1)
print '>> Identify reference stars'
idcat = []
for i in range(len(xycoo)):
idcat.append(raw_input('Star ' + str(i + 1) + '= ? '))
ff = open(coordinatelist + '.tv', 'r')
rr = ff.readlines()
ff.close()
gg = open('tmp.ccmap', 'w')
fw = []
for i in range(len(idcat)):
idpos = stars.index(idcat[i])
_rr = string.split(rr[idpos])
_x, _y, _fw = string.split(xycoo[i])
gg.write(_x + ' ' + _y + ' ' + _rr[0] + ' ' + _rr[1] + ' \n')
fw.append(float(_fw))
gg.close()
iraf.delete('_first_image.tv', verify='no')
iraf.delete('_first.ccmap', verify='no')
os.system('cp ' + coordinatelist + '.tv _first_image.tv')
os.system('cp tmp.ccmap _first.ccmap')
iraf.ccmap('tmp.ccmap',
'tmp.ccdb',
images=img,
fitgeome='rscale',
lngunit='degrees',
update='yes',
interact=False)
_z1, _z2, goon = src.display_image(img, 1, '', '', False)
if not goon: src.close_program(logincl)
iraf.delete('tmp.' + img + '.coo', verify='no')
iraf.wcsctran(coordinatelist + '.tv',
'tmp.' + img + '.coo',
img,
inwcs='world',
units='degrees degrees',
outwcs='logical',
columns='1 2',
formats='%10.1f %10.1f')
iraf.tvmark(1,
'tmp.' + img + '.coo',
mark="circle",
number='yes',
label='no',
radii=20,
nxoffse=15,
nyoffse=15,
color=205,
txsize=4)
iraf.delete("tmp.ccmap", verify='no')
iraf.delete("tmp.coo", verify='no')
iraf.delete("tmp.ccdb", verify='no')
answ = raw_input(
'is the astrometry of the field good [y/n] ? [y]')
if not answ: answ = 'y'
iraf.delete("tmp.star", verify='no')
iraf.ccfind('home$coordinate_std/' + dir_system + coordinatelist + '.list',
'tmp.star',
img,
lngcolu=2,
latcolu=3,
lngunit='degrees',
usewcs='yes')
iraf.ccmap('tmp.star',
'tmp.ccdb',
images=img,
fitgeome='rscale',
xcolum=9,
ycolum=10,
lngcolum=2,
latcolumn=3,
lngunit='degrees',
update='yes',
interact=False)
iraf.delete('tmp.' + img + '.coo', verify='no')
iraf.wcsctran(coordinatelist + '.tv',
'tmp.' + img + '.coo',
img,
inwcs='world',
units='degrees degrees',
outwcs='logical',
columns='1 2',
formats='%10.1f %10.1f')
iraf.delete("tmp.ccdb", verify='no')
iraf.delete("tmp.star", verify='no')
iraf.delete("tmp.coo", verify='no')
return stars, 'tmp.' + img + '.coo'
def ecpsf(img, ofwhm, threshold, psfstars, distance, interactive, ds9, psffun='gauss', fixaperture=False,_catalog='',_datamax=''):
try:
import agnkey
hdr = agnkey.util.readhdr(img + '.fits')
instrument = agnkey.util.readkey3(hdr, 'instrume')
print 'INSTRUMENT:', instrument
if 'PIXSCALE' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'PIXSCALE')
elif 'CCDSCALE' in hdr:
if 'CCDXBIN' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'CCDSCALE') * agnkey.util.readkey3(hdr, 'CCDXBIN')
elif 'CCDSUM' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'CCDSCALE') * int(
string.split(agnkey.util.readkey3(hdr, 'CCDSUM'))[0])
if 'kb' in instrument:
scale = pixelscale
if not _datamax:
_datamax = 45000
elif 'fl' in instrument:
scale = pixelscale
if not _datamax:
_datamax = 60000
elif 'fs' in instrument:
scale = pixelscale
if not _datamax:
_datamax = 65000
try:
#if 1==1:
if 'WCSERR' in hdr:
_wcserr = hdr['WCSERR']
elif 'WCS_ERR' in hdr:
_wcserr = hdr['WCS_ERR']
print _wcserr
if float(_wcserr) == 0:
if 'kb' in instrument:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'fl' in instrument:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'fs' in instrument:
if 'L1FWHM' in hdr:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'L1SEEING' in hdr:
seeing = float(agnkey.util.readkey3(hdr, 'L1SEEING')) * scale
else:
seeing = 3
else:
seeing = 3
else:
seeing = float(agnkey.util.readkey3(hdr, 'PSF_FWHM'))
sys.exit('astrometry not good')
except ValueError:
# except:
sys.exit('astrometry not good')
fwhm = seeing / scale
print 'FWHM[header] ', fwhm, ' in pixel'
if ofwhm: fwhm = float(ofwhm)
print ' FWHM[input] ', fwhm, ' in pixel'
xdim, ydim = iraf.hselect(img+'.fits[0]', 'i_naxis1,i_naxis2', 'yes', Stdout=1)[0].split()
print img, fwhm, threshold, scale
#################################################################################
################### write file to compute psf _psf.coo ############
#################################################################################
if interactive:
iraf.set(stdimage='imt1024')
iraf.display(img+'.fits[0]', 1, fill=True)
iraf.delete('tmp.lo?', verify=False)
print '_' * 80
print '>>> Mark reference stars with "a". Then "q"'
print '-' * 80
iraf.imexamine(img+'[0]', 1, wcs='logical', logfile='tmp.log', keeplog=True)
xyrefer = iraf.fields('tmp.log', '1,2,6,15', Stdout=1)
xns, yns, _fws = [], [], []
############# write file for PSF #########################
ff = open('_psf.coo', 'w')
for i in range(len(xyrefer)):
xns.append(float(xyrefer[i].split()[0]))
yns.append(float(xyrefer[i].split()[1]))
_fws.append(float(xyrefer[i].split()[3]))
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
ff.close()
fwhm = np.median(_fws)
else:
############ run sextractor #####################################
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
_ra1,_dec1,xx11,yy11,_mag,_dist = agnkey.agnastrodef.starsfields(img+'.fits',20,19)
if len(_ra1):
dist,pos0,pos1 = agnkey.agnastrodef.crossmatchxy(xs,ys,xx11,yy11,10)
if len(pos0):
xs = xs[pos0]
ys = ys[pos0]
ran = ran[pos0]
decn = decn[pos0]
magbest = magbest[pos0]
classstar = classstar[pos0]
fluxrad = fluxrad[pos0]
bkg = bkg[pos0]
ff = open('tmp.cursor', 'w')
for i in range(len(xs)):
x1, x2 = int(xs[i] - fwhm * 3), int(xs[i] + fwhm * 3)
y1, y2 = int(ys[i] - fwhm * 3), int(ys[i] + fwhm * 3)
sect = '[' + str(x1) + ':' + str(x2) + ',' + str(y1) + ':' + str(y2) + ']'
try:
fmax = iraf.imstat(img+'.fits[0]' + sect, fields='max', Stdout=1)[1]
########## cut saturated object ########################
if float(fmax) < _datamax: # not saturated
ff.write('%10.3f %10.3f 1 m \n' % (xs[i], ys[i]))
except:
print sect
# print 'problem here'
# pass
ff.close()
iraf.delete('tmp.lo?,tmp.sta?,tmp.gk?', verify=False)
iraf.psfmeasure(img+'[0]', imagecur='tmp.cursor', logfile='tmp.log', radius=int(fwhm), iter=3,
display=False, StdoutG='tmp.gki')
ff = open('tmp.log')
righe = ff.readlines()
xn = [float(righe[3].split()[1])]
yn = [float(righe[3].split()[2])]
_fw = [float(righe[3].split()[4])]
for r in righe[4:-2]:
if len(r) > 0:
xn.append(float(r.split()[0]))
yn.append(float(r.split()[1]))
_fw.append(float(r.split()[3]))
print 'FWHM: ', righe[-1].split()[-1]
print 80 * "#"
######
############## eliminate double object identification ###########################
xns, yns, _fws = [xn[0]], [yn[0]], [_fw[0]]
for i in range(1, len(xn)):
if abs(xn[i] - xn[i - 1]) > .2 and abs(yn[i] - yn[i - 1]) > .2:
xns.append(xn[i])
yns.append(yn[i])
_fws.append(_fw[i])
######### write clean file for PSF #########################
fw = []
ff = open('_psf.coo', 'w')
for i in range(len(xns)):
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
fw.append(_fws[i])
ff.close() ## End automatic selection
######################################################################################
################### write file of object to store in fits table #############
######################################################################################
if interactive:
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
ff = open('_psf2.coo', 'w')
for i in range(len(xs)):
ff.write('%10s %10s %10s \n' % (xs[i], ys[i], fluxrad[i]))
ff.close()
elif _catalog:
print '\n#### use catalog '
ddd=iraf.wcsctran(input=_catalog,output='STDOUT',Stdout=1,image=img,inwcs='world',outwcs='logical',
units='degrees degrees',columns='1 2',formats='%10.1f %10.1f',verbose='no')
ddd=[i for i in ddd if i[0]!='#']
ddd=[' '.join(i.split()[0:3]) for i in ddd]
ff = open('_psf2.coo', 'w')
for i in ddd:
a,b,c = string.split(i)
ff.write('%10s %10s %10s \n' % (a, b, c))
ff.close()
print 'use catalog'
else:
os.system('cp _psf.coo _psf2.coo')
# print '\n### use sextractor'
# xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
# ff = open('_psf2.coo', 'w')
# for i in range(len(xs)):
# ff.write('%10s %10s %10s \n' % (xs[i], ys[i], fluxrad[i]))
# ff.close()
###################################################################################
print 80 * "#"
photmag, pst, fitmag = psffit(img, fwhm, psfstars, hdr, interactive, _datamax, psffun, fixaperture)
photmag2, fitmag2 = psffit2(img, fwhm, psfstars, hdr, _datamax, psffun, fixaperture)
radec = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag, \
Stdout=1, image=img+'.fits[0]', inwcs='logical', outwcs='world', columns="1 2", \
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
radec2 = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag2, \
Stdout=1, image=img+'.fits[0]', inwcs='logical', outwcs='world', columns="1 2", \
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
if ds9 == 0 and interactive:
iraf.set(stdimage='imt1024')
iraf.display(img, 1, fill=True, Stdout=1)
iraf.tvmark(1, coords='STDIN', mark='circle', radii=15, label=False, Stdin=photmag)
iraf.tvmark(1, coords='STDIN', mark='rectangle', length=35, label=False, Stdin=pst)
iraf.tvmark(1, coords='STDIN', mark='cross', length=35, label=False, Stdin=fitmag2, color=204)
idpsf = []
for i in range(len(pst)):
idpsf.append(pst[i].split()[2])
dmag = []
for i in range(len(radec)):
ra, dec, idph, magp2, magp3, magp4, merrp2, merrp3, merrp4 = radec[i].split()
dmag.append(9.99)
for j in range(len(fitmag)):
raf, decf, idf, magf, magerrf = fitmag[j].split()
if idph == idf and idph in idpsf and \
magp3 != 'INDEF' and magf != 'INDEF':
dmag[i] = float(magp3) - float(magf)
break
_dmag = np.compress(np.array(dmag) < 9.99, np.array(dmag))
print '>>> Aperture correction (phot) %6.3f +/- %5.3f %3d ' % \
(np.mean(_dmag), np.std(_dmag), len(_dmag))
if len(_dmag) > 3:
_dmag = np.compress(abs(_dmag - np.median(_dmag)) < 2 * np.std(_dmag), _dmag)
print '>>> 2 sigma rejection) %6.3f +/- %5.3f %3d [default]' \
% (np.mean(_dmag), np.std(_dmag), len(_dmag))
print '>>> fwhm %s ' % (str(fwhm))
for i in range(len(dmag)):
if dmag[i] == 9.99:
dmag[i] = ''
else:
dmag[i] = '%6.3f' % (dmag[i])
exptime = agnkey.util.readkey3(hdr, 'exptime')
object = agnkey.util.readkey3(hdr, 'object').replace(' ', '')
filtro = agnkey.util.readkey3(hdr, 'filter')
#######################################
rap, decp, magp2, magp3, magp4, smagf = [], [], [], [], [], []
merrp2, merrp3, merrp4, smagerrf = [], [], [], []
rap0, decp0 = [], []
for i in range(len(radec2)):
aa = radec2[i].split()
rap.append(aa[0])
decp.append(aa[1])
rap0.append(agnkey.agnabsphotdef.deg2HMS(ra=aa[0]))
decp0.append(agnkey.agnabsphotdef.deg2HMS(dec=aa[1]))
idp = aa[2]
magp2.append(aa[3])
magp3.append(aa[4])
magp4.append(aa[5])
merrp2.append(aa[6])
merrp3.append(aa[7])
merrp4.append(aa[8])
_smagf, _smagerrf = 9999, 9999
for j in range(len(fitmag2)):
raf, decf, idf, magf, magerrf = fitmag2[j].split()
if idf == idp:
_smagf = magf
_smagerrf = magerrf
break
smagf.append(_smagf)
smagerrf.append(_smagerrf)
new_cols = pyfits.ColDefs([
pyfits.Column(name='ra', format='20A', array=np.array(rap)),
pyfits.Column(name='dec', format='20A', array=np.array(decp)),
pyfits.Column(name='ra0', format='E', array=np.array(rap0)),
pyfits.Column(name='dec0', format='E', array=np.array(decp0)),
pyfits.Column(name='magp2', format='E', array=np.array(np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
pyfits.Column(name='magp3', format='E', array=np.array(np.where((np.array(magp3) != 'INDEF'),
np.array(magp3), 9999), float)),
pyfits.Column(name='magp4', format='E', array=np.array(np.where((np.array(magp4) != 'INDEF'),
np.array(magp4), 9999), float)),
pyfits.Column(name='merrp2', format='E', array=np.array(np.where((np.array(merrp2) != 'INDEF'),
np.array(merrp2), 9999), float)),
pyfits.Column(name='merrp3', format='E', array=np.array(np.where((np.array(merrp3) != 'INDEF'),
np.array(merrp3), 9999), float)),
pyfits.Column(name='merrp4', format='E', array=np.array(np.where((np.array(merrp4) != 'INDEF'),
np.array(merrp4), 9999), float)),
pyfits.Column(name='smagf', format='E', array=np.array(np.where((np.array(smagf) != 'INDEF'),
np.array(smagf), 9999), float)),
pyfits.Column(name='smagerrf', format='E', array=np.array(np.where((np.array(smagerrf) != 'INDEF'),
np.array(smagerrf), 9999), float)),
])
tbhdu = pyfits.BinTableHDU.from_columns(new_cols)
hdu = pyfits.PrimaryHDU(header=hdr)
thdulist = pyfits.HDUList([hdu, tbhdu])
agnkey.util.delete(img + '.sn2.fits')
thdulist.writeto(img + '.sn2.fits')
agnkey.util.updateheader(img + '.sn2.fits', 0, {'APCO': [np.mean(_dmag), 'Aperture correction']})
agnkey.util.updateheader(img + '.sn2.fits', 0, {'APCOERR': [np.std(_dmag), 'Aperture correction error']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'XDIM': [agnkey.util.readkey3(hdr, 'naxis1'), 'x number of pixels']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'YDIM': [agnkey.util.readkey3(hdr, 'naxis2'), 'y number of pixels']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'PSF_FWHM': [fwhm * scale, 'FWHM (arcsec) - computed with daophot']})
os.chmod(img + '.sn2.fits', 0664)
os.chmod(img + '.psf.fits', 0664)
result = 1
except IOError as e:
print e
result = 0
fwhm = 0.0
traceback.print_exc()
return result, fwhm * scale
def ecpsf(img, ofwhm, threshold, psfstars, distance, interactive, ds9, psffun='gauss', fixaperture=False,_catalog='',_datamax=''):
try:
import agnkey
hdr = agnkey.util.readhdr(img + '.fits')
instrument = agnkey.util.readkey3(hdr, 'instrume')
print ('INSTRUMENT:', instrument)
if 'PIXSCALE' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'PIXSCALE')
elif 'CCDSCALE' in hdr:
if 'CCDXBIN' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'CCDSCALE') * agnkey.util.readkey3(hdr, 'CCDXBIN')
elif 'CCDSUM' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'CCDSCALE') * int(
string.split(agnkey.util.readkey3(hdr, 'CCDSUM'))[0])
if 'kb' in instrument:
scale = pixelscale
if not _datamax:
_datamax = 45000
elif 'fl' in instrument:
scale = pixelscale
if not _datamax:
_datamax = 60000
elif 'fa' in instrument:
scale = pixelscale
if not _datamax:
_datamax = 60000
elif 'fs' in instrument:
scale = pixelscale
if not _datamax:
_datamax = 65000
try:
#if 1==1:
if 'WCSERR' in hdr:
_wcserr = hdr['WCSERR']
elif 'WCS_ERR' in hdr:
_wcserr = hdr['WCS_ERR']
print _wcserr
if float(_wcserr) == 0:
if 'kb' in instrument:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'fl' in instrument:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'fa' in instrument:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'fs' in instrument:
if 'L1FWHM' in hdr:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif 'L1SEEING' in hdr:
seeing = float(agnkey.util.readkey3(hdr, 'L1SEEING')) * scale
else:
seeing = 3
else:
seeing = 3
else:
seeing = float(agnkey.util.readkey3(hdr, 'PSF_FWHM'))
sys.exit('astrometry not good')
except ValueError:
# except:
sys.exit('astrometry not good')
fwhm = seeing / scale
print 'FWHM[header] ', fwhm, ' in pixel'
if ofwhm: fwhm = float(ofwhm)
print ' FWHM[input] ', fwhm, ' in pixel'
xdim, ydim = iraf.hselect(img+'.fits[0]', 'i_naxis1,i_naxis2', 'yes', Stdout=1)[0].split()
print img, fwhm, threshold, scale
#################################################################################
################### write file to compute psf _psf.coo ############
#################################################################################
if interactive:
iraf.set(stdimage='imt1024')
iraf.display(img+'.fits[0]', 1, fill=True)
iraf.delete('tmp.lo?', verify=False)
print '_' * 80
print '>>> Mark reference stars with "a". Then "q"'
print '-' * 80
iraf.imexamine(img+'[0]', 1, wcs='logical', logfile='tmp.log', keeplog=True)
xyrefer = iraf.fields('tmp.log', '1,2,6,15', Stdout=1)
xns, yns, _fws = [], [], []
############# write file for PSF #########################
ff = open('_psf.coo', 'w')
for i in range(len(xyrefer)):
xns.append(float(xyrefer[i].split()[0]))
yns.append(float(xyrefer[i].split()[1]))
_fws.append(float(xyrefer[i].split()[3]))
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
ff.close()
fwhm = np.median(_fws)
else:
############ run sextractor #####################################
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
_ra1,_dec1,xx11,yy11,_mag,_dist = agnkey.agnastrodef.starsfields(img+'.fits',20,19)
if len(_ra1):
dist,pos0,pos1 = agnkey.agnastrodef.crossmatchxy(xs,ys,xx11,yy11,10)
if len(pos0):
xs = xs[pos0]
ys = ys[pos0]
ran = ran[pos0]
decn = decn[pos0]
magbest = magbest[pos0]
classstar = classstar[pos0]
fluxrad = fluxrad[pos0]
bkg = bkg[pos0]
ff = open('tmp.cursor', 'w')
for i in range(len(xs)):
x1, x2 = int(xs[i] - fwhm * 3), int(xs[i] + fwhm * 3)
y1, y2 = int(ys[i] - fwhm * 3), int(ys[i] + fwhm * 3)
sect = '[' + str(x1) + ':' + str(x2) + ',' + str(y1) + ':' + str(y2) + ']'
try:
fmax = iraf.imstat(img+'.fits[0]' + sect, fields='max', Stdout=1)[1]
########## cut saturated object ########################
if float(fmax) < _datamax: # not saturated
ff.write('%10.3f %10.3f 1 m \n' % (xs[i], ys[i]))
except:
print sect
# print 'problem here'
# pass
ff.close()
iraf.delete('tmp.lo?,tmp.sta?,tmp.gk?', verify=False)
iraf.psfmeasure(img+'[0]', imagecur='tmp.cursor', logfile='tmp.log', radius=int(fwhm), iter=3,
display=False, StdoutG='tmp.gki')
ff = open('tmp.log')
righe = ff.readlines()
xn = [float(righe[3].split()[1])]
yn = [float(righe[3].split()[2])]
_fw = [float(righe[3].split()[4])]
for r in righe[4:-2]:
if len(r) > 0:
xn.append(float(r.split()[0]))
yn.append(float(r.split()[1]))
_fw.append(float(r.split()[3]))
print 'FWHM: ', righe[-1].split()[-1]
print 80 * "#"
######
############## eliminate double object identification ###########################
xns, yns, _fws = [xn[0]], [yn[0]], [_fw[0]]
for i in range(1, len(xn)):
if abs(xn[i] - xn[i - 1]) > .2 and abs(yn[i] - yn[i - 1]) > .2:
xns.append(xn[i])
yns.append(yn[i])
_fws.append(_fw[i])
######### write clean file for PSF #########################
fw = []
ff = open('_psf.coo', 'w')
for i in range(len(xns)):
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
fw.append(_fws[i])
ff.close() ## End automatic selection
######################################################################################
################### write file of object to store in fits table #############
######################################################################################
if interactive:
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
ff = open('_psf2.coo', 'w')
for i in range(len(xs)):
ff.write('%10s %10s %10s \n' % (xs[i], ys[i], fluxrad[i]))
ff.close()
elif _catalog:
print '\n#### use catalog '
ddd=iraf.wcsctran(input=_catalog,output='STDOUT',Stdout=1,image=img,inwcs='world',outwcs='logical',
units='degrees degrees',columns='1 2',formats='%10.1f %10.1f',verbose='no')
ddd=[i for i in ddd if i[0]!='#']
ddd=[' '.join(i.split()[0:3]) for i in ddd]
ff = open('_psf2.coo', 'w')
for i in ddd:
a,b,c = string.split(i)
ff.write('%10s %10s %10s \n' % (a, b, c))
ff.close()
print 'use catalog'
else:
os.system('cp _psf.coo _psf2.coo')
# print '\n### use sextractor'
# xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
# ff = open('_psf2.coo', 'w')
# for i in range(len(xs)):
# ff.write('%10s %10s %10s \n' % (xs[i], ys[i], fluxrad[i]))
# ff.close()
###################################################################################
print 80 * "#"
photmag, pst, fitmag = psffit(img, fwhm, psfstars, hdr, interactive, _datamax, psffun, fixaperture)
photmag2, fitmag2 = psffit2(img, fwhm, psfstars, hdr, _datamax, psffun, fixaperture)
radec = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag, \
Stdout=1, image=img+'.fits[0]', inwcs='logical', outwcs='world', columns="1 2", \
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
radec2 = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag2, \
Stdout=1, image=img+'.fits[0]', inwcs='logical', outwcs='world', columns="1 2", \
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
if ds9 == 0 and interactive:
iraf.set(stdimage='imt1024')
iraf.display(img, 1, fill=True, Stdout=1)
iraf.tvmark(1, coords='STDIN', mark='circle', radii=15, label=False, Stdin=photmag)
iraf.tvmark(1, coords='STDIN', mark='rectangle', length=35, label=False, Stdin=pst)
iraf.tvmark(1, coords='STDIN', mark='cross', length=35, label=False, Stdin=fitmag2, color=204)
idpsf = []
for i in range(len(pst)):
idpsf.append(pst[i].split()[2])
dmag = []
for i in range(len(radec)):
ra, dec, idph, magp2, magp3, magp4, merrp2, merrp3, merrp4 = radec[i].split()
dmag.append(9.99)
for j in range(len(fitmag)):
raf, decf, idf, magf, magerrf = fitmag[j].split()
if idph == idf and idph in idpsf and \
magp3 != 'INDEF' and magf != 'INDEF':
dmag[i] = float(magp3) - float(magf)
break
_dmag = np.compress(np.array(dmag) < 9.99, np.array(dmag))
print '>>> Aperture correction (phot) %6.3f +/- %5.3f %3d ' % \
(np.mean(_dmag), np.std(_dmag), len(_dmag))
if len(_dmag) > 3:
_dmag = np.compress(abs(_dmag - np.median(_dmag)) < 2 * np.std(_dmag), _dmag)
print '>>> 2 sigma rejection) %6.3f +/- %5.3f %3d [default]' \
% (np.mean(_dmag), np.std(_dmag), len(_dmag))
print '>>> fwhm %s ' % (str(fwhm))
for i in range(len(dmag)):
if dmag[i] == 9.99:
dmag[i] = ''
else:
dmag[i] = '%6.3f' % (dmag[i])
exptime = agnkey.util.readkey3(hdr, 'exptime')
object = agnkey.util.readkey3(hdr, 'object').replace(' ', '')
filtro = agnkey.util.readkey3(hdr, 'filter')
#######################################
rap, decp, magp2, magp3, magp4, smagf = [], [], [], [], [], []
merrp2, merrp3, merrp4, smagerrf = [], [], [], []
rap0, decp0 = [], []
for i in range(len(radec2)):
aa = radec2[i].split()
rap.append(aa[0])
decp.append(aa[1])
rap0.append(agnkey.agnabsphotdef.deg2HMS(ra=aa[0]))
decp0.append(agnkey.agnabsphotdef.deg2HMS(dec=aa[1]))
idp = aa[2]
magp2.append(aa[3])
magp3.append(aa[4])
magp4.append(aa[5])
merrp2.append(aa[6])
merrp3.append(aa[7])
merrp4.append(aa[8])
_smagf, _smagerrf = 9999, 9999
for j in range(len(fitmag2)):
raf, decf, idf, magf, magerrf = fitmag2[j].split()
if idf == idp:
_smagf = magf
_smagerrf = magerrf
break
smagf.append(_smagf)
smagerrf.append(_smagerrf)
new_cols = pyfits.ColDefs([
pyfits.Column(name='ra', format='20A', array=np.array(rap)),
pyfits.Column(name='dec', format='20A', array=np.array(decp)),
pyfits.Column(name='ra0', format='E', array=np.array(rap0)),
pyfits.Column(name='dec0', format='E', array=np.array(decp0)),
pyfits.Column(name='magp2', format='E', array=np.array(np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
pyfits.Column(name='magp3', format='E', array=np.array(np.where((np.array(magp3) != 'INDEF'),
np.array(magp3), 9999), float)),
pyfits.Column(name='magp4', format='E', array=np.array(np.where((np.array(magp4) != 'INDEF'),
np.array(magp4), 9999), float)),
pyfits.Column(name='merrp2', format='E', array=np.array(np.where((np.array(merrp2) != 'INDEF'),
np.array(merrp2), 9999), float)),
pyfits.Column(name='merrp3', format='E', array=np.array(np.where((np.array(merrp3) != 'INDEF'),
np.array(merrp3), 9999), float)),
pyfits.Column(name='merrp4', format='E', array=np.array(np.where((np.array(merrp4) != 'INDEF'),
np.array(merrp4), 9999), float)),
pyfits.Column(name='smagf', format='E', array=np.array(np.where((np.array(smagf) != 'INDEF'),
np.array(smagf), 9999), float)),
pyfits.Column(name='smagerrf', format='E', array=np.array(np.where((np.array(smagerrf) != 'INDEF'),
np.array(smagerrf), 9999), float)),
])
tbhdu = pyfits.BinTableHDU.from_columns(new_cols)
hdu = pyfits.PrimaryHDU(header=hdr)
thdulist = pyfits.HDUList([hdu, tbhdu])
agnkey.util.delete(img + '.sn2.fits')
thdulist.writeto(img + '.sn2.fits')
agnkey.util.updateheader(img + '.sn2.fits', 0, {'APCO': [np.mean(_dmag), 'Aperture correction']})
agnkey.util.updateheader(img + '.sn2.fits', 0, {'APCOERR': [np.std(_dmag), 'Aperture correction error']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'XDIM': [agnkey.util.readkey3(hdr, 'naxis1'), 'x number of pixels']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'YDIM': [agnkey.util.readkey3(hdr, 'naxis2'), 'y number of pixels']})
agnkey.util.updateheader(img + '.sn2.fits', 0,
{'PSF_FWHM': [fwhm * scale, 'FWHM (arcsec) - computed with daophot']})
os.chmod(img + '.sn2.fits', 0664)
os.chmod(img + '.psf.fits', 0664)
result = 1
except IOError as e:
print e
result = 0
fwhm = 0.0
traceback.print_exc()
return result, fwhm * scale
_mag0 = raw_input(
'which mag do you want to subtract ' + str(_mag) +
' ? ')
if _mag0:
_mag = float(_mag0)
print 'magnitude to be subtracted:', _mag
####################### Chose Ra and Dec ##############
if chosepos:
print 'choose xpos, ypos interactively'
lsc.util.delete('tmp.log')
zz1, zz2, goon = lsc.util.display_image(
img, 1, '', '', True)
iraf.imexamine(img,
1,
wcs='logical',
logfile='tmp.log',
keeplog=True)
xytargets = iraf.fields('tmp.log', '1,2', Stdout=1)
_xpos, _ypos = string.split(xytargets[0])[0], string.split(
xytargets[0])[1]
elif not _ra or not _dec:
print 'use ra and dec from input database !!! '
_ra, _dec, _SN0, _type = lsc.util.checksndb(
img0, 'targets')
if _ra and _dec:
print 'convert RA, dec to xpos, ypos using header'
hdr0 = lsc.util.readhdr(img0)
wcs = WCS(hdr0)
pix1 = wcs.wcs_world2pix([(_ra, _dec)], 1)
op1 = cordatals[i].split('_')[3]
op2 = cordatals[i + 1].split('_')[3]
print "\tnormal step:"
print ' subtracting', rname + '_' + op1 + '_cor.fit' + '-' + rname + '_' + op2 + '_cor.fit', 'to create:', rname + '_' + op1 + '-' + op2 + '_df.fit'
iraf.imarith(operand1=rname + '_' + op1 + '_cor.fit',
op="-",
operand2=rname + '_' + op2 + '_cor.fit',
result=rname + '_' + op1 + '-' + op2 + '_df.fit')
imimlst.write(rname + '_' + op1 + '-' + op2 + '_df.fit' + '\n')
imimlst.close()
# setting display parameters and imexamine (<<< select star to align)
print "> displaying images to select the star used for alignment"
iraf.set(stdimage="imt1024")
iraf.imexamine("@imexamine_image.irafl",
frame=1,
logfile="imexamine.irafl",
keeplog="yes")
# preparation and manipulation of lists and align/shift processes
shimlst1 = open('images_to_shift.irafl', 'w')
shimlst22 = open('shifted_images.irafl', 'w')
imlog = open("imexamine.irafl", "r") # selecting the x,y values only
lines = imlog.readlines()
imlog.close()
x = []
y = []
for lin in lines:
lin.split(' ')
if lin.split()[0] != "#":
print lin.split()[0], lin.split()[1]
def Main(obj, obstime_kw=None, iraf_display_mode='display'):
"""
Given a list of images in a specified folder, will display
them using iraf.display (if iraf_display_mode=='display') or iraf.imexamine
(if iraf_display_mode=='imexamine') in blocks of 10. For first pass inspection,
the point is to see whether there are any significant pointing
drifts between frames that will cause the source tracking
algorithm to fail. For second pass inspection, the point is
to make a quick comparison between the absolute photometry
output from the pipeline and manual imexam photometry values.
"""
images = np.loadtxt(obj.image_list, dtype='str')
if obstime_kw!=None:
obstimes = np.zeros(len(images))
for i in range(len(obstimes)):
h = pyfits.getheader(images[i])
obstimes[i] = h[obstime_kw]
ixs = np.argsort(obstimes)
images = images[ixs]
blockids = np.zeros(len(images))
nperblock = 10
nimages = len(images)
nblocks = int(np.ceil(float(nimages)/nperblock))
record_outcome = np.ones(nblocks)
block_counter = 0
for i in range(nblocks):
n = min([nperblock, nimages-i*nperblock])
print '\nBlock %i of %i' % (i+1,nblocks)
for j in range(n):
ix = i*nperblock+j
blockids[ix] = i
try:
print 'Loading %s...' % images[ix]
if iraf_display_mode=='display':
iraf.display(images[ix],j+1)
elif iraf_display_mode=='imexamine':
iraf.imexamine(images[ix],j+1)
else:
pdb.set_trace()
except:
pass
print '\nEnter 1 for OK, 0 if not:\n'
outcome = ''
while outcome=='':
outcome = raw_input('')
record_outcome[i] = outcome
ixs = np.arange(nblocks)[record_outcome==0]
ncloser = len(ixs)
print '\nYou identified %i blocks to look at again closely.' % ncloser
print 'Enter y to go through them again now, or n to exit:'
outcome = ''
while outcome=='':
outcome = raw_input('')
if outcome=='y':
for i in range(ncloser):
closer_images = images[blockids==ixs[i]]
print '\n Block %i:' % (ixs[i]+1)
for j in range(len(closer_images)):
print closer_images[j]
iraf.display(closer_images[j],j+1)
print ' (enter c to continue)'
outcome = ''
while outcome=='':
outcome = raw_input('')
else:
print '\nFor future reference, the identified blocks were:'
for i in range(ncloser):
print '\n Block %i, containing:' % ixs[i]
closer_images = images[blockids==ixs[i]]
for j in range(len(closer_images)):
print ' - %s' % closer_images[j]
return None
print '\ncreating a zero_files/ dir to store original data'
if not os.path.isdir('zero_files'):
os.mkdir('zero_files')
allfiles = zerolist
for file in allfiles:
shutil.copy(file, 'zero_files/')
# combine bias images
print 'Combining zero level images...'
iraf.ccdred.zerocombine.ccdtype = ''
iraf.ccdred.zerocombine.reject = 'ccdclip'
iraf.ccdred.zerocombine.rdnoise = 'rdnoise'
iraf.ccdred.zerocombine.gain = 'gain'
iraf.ccdred.zerocombine(input=zeroin)
for zero in zerolist:
os.remove(zero)
print 'openning a ds9 window if not already openned...'
ds9.ds9()
# check output image
print 'Check output file:'
iraf.imstatistics('Zero')
print ' Running "imexamine" task..'
iraf.imexamine('Zero', 1)
print '--- DONE ---'
def radprof_iraf(image,
coords,
radius,
step=0.1,
output='STDOUT',
plotfile=None,
verbose=False,
test=False,
pxscale=None):
iraf.apphot.centerpars.setParam('maxshift', radius) # search radius
if test:
results = iraf.imexamine(image,
image=image,
use_display='no',
logfile='',
defkey='r',
imagecur=coords,
frame=1,
mode='h',
StdoutG=plotfile,
Stdout=1)
results = [np.float(x) for x in results[0].split()]
# prad frad flux bgd mpeak ellip pa mbeta 2dfwhm mfwhm fwhm
results = OrderedDict(zip(R_COLMAP, results))
tbl = Table([results])
tbl = tbl[R_COLMAP]
tbl['flux'].unit = u.ct
tbl['bgd'].unit = u.ct
tbl['mpeak'].unit = u.ct
tbl['pa'].unit = u.deg
#tbl['2dfwhm'].unit = u.pix
tbl['mfwhm'].unit = u.pix
tbl['fwhm'].unit = u.pix
#remove 2dfwhm cuz wut?
tbl.remove_column('2dfwhm')
if pxscale:
#add arcsec columns
for fwhmcol in tbl.colnames[-2:]:
tbl.add_column(
Column(tbl[fwhmcol] * pxscale,
name='%s_s' % fwhmcol,
unit=u.arcsec,
format='%.3f'),
tbl.index_column(fwhmcol) + 1)
gki = iraf.gkidecode(plotfile, Stdout=1, verbose=True)
gki = '\n'.join(gki)
xr, yr, xf, yf = extract_gkidata(gki)
#plt.scatter(xr,yr)
#plt.plot(xf,yf)
#plt.show()
return tbl, xr, yr, xf, yf
results = iraf.apphot.radprof(image,
radius=radius,
step=step,
coords=coords,
output=output,
verbose=verbose,
verify=False,
interactive=False,
Stdout=1)
#remove datalines
data = []
pradline = None
for idx, line in enumerate(results):
if '*\\' in line:
line = line.split()[0:3]
line = [np.float(x) for x in line]
data.append((idx, line))
#remove pradius line descriptors
elif 'PRADIUS' in line:
pradline = idx
idx, data = zip(*data)
#print data
#remove from min idx onward
ridx = np.min(idx)
del results[ridx:]
del results[pradline:pradline + 4]
# remove '\' from last line
results[-1] = results[-1][0:-1]
results = '\n'.join(results[1:])
rtbl = Table.read(results, format='ascii.daophot')
#print rtbl['PFWHM']/2.0
ptbl = Table(rows=data, names=('radius', 'intensity', 'tintensity'))
ptbl['intensity'] *= rtbl['INORM']
#tbl.pprint()
#plt.plot(tbl['radius'],tbl['intensity']*ptbl['INORM'])
return ptbl
color=206,
txsize=4)
answ = raw_input(
'AND NOW, is the astrometry of the field good [y/n] ? [y] '
)
if not answ: answ = 'y'
except:
pass
while answ == 'n':
_z1, _z2, goon = src.display_image(img, 1, '', '', False)
if not goon: src.close_program(logincl)
print '>> Identify (minimum 2, preferably 3) reference stars (mark with "a")'
iraf.imexamine(img, 1, logfile='tmp.coo', keeplog='yes')
iraf.tvmark(1,
'tmp.coo',
mark="circle",
number='yes',
label='no',
radii=5,
nxoffse=5,
nyoffse=5,
color=214,
txsize=4)
xycoo = iraf.fields('tmp.coo', '1,2,13', Stdout=1)
print '>> Identify reference stars'
idcat = []
for i in range(len(xycoo)):
idcat.append(raw_input('Star ' + str(i + 1) + '= ? '))
@author: jlee
"""
import numpy as np
import os
from time import sleep
from pyraf import iraf
iraf.images()
iraf.tv()
import init_cfg as ic
com_ds9 = 'ds9 -scalemode zscale -scale lock yes -frame lock image '
# ----- Enter an image list (manually!) ----- #
# imglist = ' '
# for i in np.arange(len(ic.nfits)):
# imglist += ic.nfits[i]+' '
imgs = ['B.fits', 'mB.fits', 'V.fits']
imglist = ' '
for i in np.arange(len(imgs)):
imglist += imgs[i] + ' '
# ------------------------------------------- #
os.system(com_ds9 + imglist + '&')
sleep(float(len(ic.nfits)))
iraf.imexamine()
fin = open('alginput.list', 'w+')
fout = open('algoutput.list', 'w+')
for afile in files:
print >> fin, afile
print >> fout, 'alg' + afile
fin.close()
fout.close()
print green("\nUse imexam to mark stars in your reference image.")
print green(
"Use keystroke 'a' to measure a point source, and keystroke 'q' to quit."
)
print green("The reference image is: %s\n" % reference)
#Imexam
output = iraf.imexamine(Stdout=1)
#make coordinate file
f = open('images.coord', 'w+')
for i in range(1, len(output)):
splt = output[i].split()
if len(splt) == 4:
print >> f, splt[0] + ' ' + splt[1]
f.close()
print green(
"\nUse imexam to mark a star in all images that are to be aligned, starting with your"
)
print green("reference image. Mark the same star in all images.")
print green(
"Use keystroke 'a' to measure a point source, and keystroke 'q' to quit."
def ntrim_flat(filename):
flatname = get_flatlst_name(filename)
f = open(filename)
l = f.readlines()
f.close()
l = [i.split()[0] for i in l]
objfitsnames = []
for i in l:
if '.fits' in i:
objfitsnames.append(i)
f = open(flatname)
l = f.readlines()
f.close()
l = [i.split()[0] for i in l]
flatfitsnames = []
for i in l:
if '.fits' in i:
flatfitsnames.append(i)
fitsnames = objfitsnames + flatfitsnames
tempfile = 'temp.lst'
f = open(tempfile,'w')
for i in fitsnames:
f.write(i + '\n')
f.close()
temppath = sys.argv[0]
tempindex = temppath.rfind(os.sep)
temppath = temppath[:tempindex]
trimfile = temppath + os.sep + 'trim.lst'
print 'get trimlst'
f = open(trimfile)
l = f.readlines()
f.close()
trimseclist = []
for i in l:
trimseclist.append(i.split())
trimsec = ''
for i in trimseclist:
if i[0] == filename:
trimsec = i[1]
break
if trimsec == '':
print 'trim.lst not have the object'
print 'Please check the fits image and determine the size to trim...'
os.popen('gedit ' + tempfile +' &')
iraf.imexamine(input = 'bo//@' + tempfile, frame = 1)
xy = raw_input("Please input x1, x2, y1, y2 to trim: ")
xy = xy.split()
trimsec = '[' + xy[0] + ':' + xy[1] + ',' + xy[2] + ':' + xy[3] +']'
f = open(trimfile,'a')
f.write(filename + ' ' + trimsec + '\n')
f.close()
print '=' * 20, 'correct trim', '=' * 20
correct_trim(tempfile, trimsec)
print '=' * 20, 'cimbine flat', '=' * 20
dtempname = combine_flat(flatname)
f = open(tempfile, 'w')
for i in objfitsnames:
f.write(i + '\n')
f.close()
print '=' * 20, 'correct flat', '=' * 20
correct_flat(tempfile, dtempname[-1])
print 'delete useless file...'
print 'delete ' + tempfile
os.remove(tempfile)
for i in dtempname:
print 'delete ' + i
os.remove(i)
for i in flatfitsnames:
print 'delete ' + 'tbo' + i
os.remove('tbo' + i)
print 'correct standard file name...'
objname = filename.split('_')[1]
f = open(filename)
l = f.readlines()
f.close()
l = [i.split()[0] for i in l]
sindex = l.index('standard') + 1
while sindex < len(l):
if '.fits' in l[sindex]:
nname = l[sindex].replace('.fits', objname + '.fits')
print 'ftbo' + l[sindex], 'rename', 'ftbo' + nname
os.rename('ftbo' + l[sindex], 'ftbo' + nname)
print 'delete tbo' + l[sindex]
os.remove('tbo' + l[sindex])
l[sindex] = nname
sindex += 1
else:
break
f = open(filename, 'w')
for i in l:
f.write(i + '\n')
f.close()
def ecpsf(img,
ofwhm,
threshold,
interactive,
ds9,
fixaperture=False,
_catalog=''):
try:
import agnkey
import string
hdr = agnkey.util.readhdr(img + '.fits')
instrument = agnkey.util.readkey3(hdr, 'instrume')
print 'INSTRUMENT:', instrument
if 'PIXSCALE' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'PIXSCALE')
elif 'CCDSCALE' in hdr:
if 'CCDXBIN' in hdr:
pixelscale = agnkey.util.readkey3(
hdr, 'CCDSCALE') * agnkey.util.readkey3(hdr, 'CCDXBIN')
elif 'CCDSUM' in hdr:
pixelscale = agnkey.util.readkey3(hdr, 'CCDSCALE') * int(
string.split(agnkey.util.readkey3(hdr, 'CCDSUM'))[0])
if instrument in [
'kb05', 'kb70', 'kb71', 'kb73', 'kb74', 'kb75', 'kb76', 'kb77',
'kb78', 'kb79'
]:
scale = pixelscale
_datamax = 45000
elif instrument in ['fl02', 'fl03', 'fl04']:
scale = pixelscale
_datamax = 120000
elif instrument in ['fs01', 'em03']:
scale = pixelscale
_datamax = 65000
elif instrument in ['fs02', 'fs03']:
scale = pixelscale
_datamax = 65000
elif instrument in ['em01']:
scale = pixelscale
_datamax = 65000
try:
_wcserr = agnkey.util.readkey3(hdr, 'wcserr')
if float(_wcserr) == 0:
if instrument in [
'kb05', 'kb70', 'kb71', 'kb73', 'kb74', 'kb75', 'kb76',
'kb77', 'kb78', 'kb79'
]:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif instrument in ['fl02', 'fl03', 'fl04']:
seeing = float(agnkey.util.readkey3(hdr, 'L1FWHM')) * .75
elif instrument in ['fs01', 'fs02', 'fs03', 'em03', 'em01']:
if 'L1FWHM' in hdr:
seeing = float(agnkey.util.readkey3(hdr,
'L1FWHM')) * .75
elif 'L1SEEING' in hdr:
seeing = float(agnkey.util.readkey3(
hdr, 'L1SEEING')) * scale
else:
seeing = 3
else:
seeing = 3
else:
seeing = float(agnkey.util.readkey3(hdr, 'PSF_FWHM'))
sys.exit('astrometry not good')
except:
sys.exit('astrometry not good')
fwhm = seeing / scale
print 'FWHM[header] ', fwhm, ' in pixel'
if ofwhm:
fwhm = float(ofwhm)
print ' FWHM[input] ', fwhm, ' in pixel'
if interactive:
iraf.display(img, 1, fill=True)
iraf.delete('tmp.lo?', verify=False)
print '_' * 80
print '>>> Mark reference stars with "a". Then "q"'
print '-' * 80
iraf.imexamine(img,
1,
wcs='logical',
logfile='tmp.log',
keeplog=True)
xyrefer = iraf.fields('tmp.log', '1,2,6,15', Stdout=1)
xns, yns, _fws = [], [], []
ff = open('_ap.coo', 'w')
for i in range(len(xyrefer)):
xns.append(float(xyrefer[i].split()[0]))
yns.append(float(xyrefer[i].split()[1]))
_fws.append(float(xyrefer[i].split()[3]))
ff.write('%10.3f %10.3f %7.2f \n' %
(xns[i], yns[i], float(_fws[i])))
ff.close()
elif _catalog:
# cat1=agnkey.agnastrodef.readtxt(_catalog)
# cat1['ra'],cat1['dec']
ddd = iraf.wcsctran(input=_catalog,
output='STDOUT',
Stdout=1,
image=img,
inwcs='world',
outwcs='logical',
units='degrees degrees',
columns='1 2',
formats='%10.1f %10.1f',
verbose='no')
ddd = [i for i in ddd if i[0] != '#']
ddd = [' '.join(i.split()[0:3]) for i in ddd]
ff = open('_ap.coo', 'w')
for i in ddd:
a, b, c = string.split(i)
#print a,b,c
ff.write('%10s %10s %10s \n' % (a, b, c))
ff.close()
print 'use catalog'
else:
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(
img, fwhm, threshold, scale)
ff = open('_ap.coo', 'w')
for i in range(len(xs)):
ff.write('%10.3f %10.3f %7.2f \n' %
(xs[i], ys[i], float(fluxrad[i])))
ff.close() ## End automatic selection
print 80 * "#"
photmag = apfit(img, fwhm, hdr, interactive, _datamax, fixaperture)
radec = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag, \
Stdout=1, image=img, inwcs='logical', outwcs='world', columns="1 2", \
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
exptime = agnkey.util.readkey3(hdr, 'exptime')
object = agnkey.util.readkey3(hdr, 'object').replace(' ', '')
filtro = agnkey.util.readkey3(hdr, 'filter')
#######################################
rap, decp, magp2, magp3, magp4, smagf = [], [], [], [], [], []
merrp2, merrp3, merrp4, smagerrf = [], [], [], []
rap0, decp0 = [], []
for i in range(len(radec)):
aa = radec[i].split()
rap.append(aa[0])
decp.append(aa[1])
rap0.append(agnkey.agnabsphotdef.deg2HMS(ra=aa[0]))
decp0.append(agnkey.agnabsphotdef.deg2HMS(dec=aa[1]))
idp = aa[2]
magp2.append(aa[3])
magp3.append(aa[4])
magp4.append(aa[5])
merrp2.append(aa[6])
merrp3.append(aa[7])
merrp4.append(aa[8])
tbhdu = pyfits.new_table(
pyfits.ColDefs([
pyfits.Column(name='ra', format='20A', array=np.array(rap)),
pyfits.Column(name='dec', format='20A', array=np.array(decp)),
pyfits.Column(name='ra0', format='E', array=np.array(rap0)),
pyfits.Column(name='dec0', format='E', array=np.array(decp0)),
pyfits.Column(name='magp2',
format='E',
array=np.array(
np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
pyfits.Column(name='magp3',
format='E',
array=np.array(
np.where((np.array(magp3) != 'INDEF'),
np.array(magp3), 9999), float)),
pyfits.Column(name='magp4',
format='E',
array=np.array(
np.where((np.array(magp4) != 'INDEF'),
np.array(magp4), 9999), float)),
pyfits.Column(name='merrp2',
format='E',
array=np.array(
np.where((np.array(merrp2) != 'INDEF'),
np.array(merrp2), 9999), float)),
pyfits.Column(name='merrp3',
format='E',
array=np.array(
np.where((np.array(merrp3) != 'INDEF'),
np.array(merrp3), 9999), float)),
pyfits.Column(name='merrp4',
format='E',
array=np.array(
np.where((np.array(merrp4) != 'INDEF'),
np.array(merrp4), 9999), float)),
pyfits.Column(name='smagf',
format='E',
array=np.array(
np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
pyfits.Column(name='smagerrf',
format='E',
array=np.array(
np.where((np.array(merrp2) != 'INDEF'),
np.array(merrp2), 9999), float)),
]))
hdu = pyfits.PrimaryHDU(header=hdr)
thdulist = pyfits.HDUList([hdu, tbhdu])
agnkey.util.delete(img + '.sn2.fits')
thdulist.writeto(img + '.sn2.fits')
agnkey.util.updateheader(img + '.sn2.fits', 0, {
'XDIM':
[agnkey.util.readkey3(hdr, 'naxis1'), 'x number of pixels']
})
agnkey.util.updateheader(img + '.sn2.fits', 0, {
'YDIM':
[agnkey.util.readkey3(hdr, 'naxis2'), 'y number of pixels']
})
agnkey.util.updateheader(img + '.sn2.fits', 0, {
'PSF_FWHM':
[fwhm * scale, 'FWHM (arcsec) - computed with daophot']
})
os.chmod(img + '.sn2.fits', 0664)
os.chmod(img + '.psf.fits', 0664)
result = 1
except:
result = 0
fwhm = 0.0
traceback.print_exc()
return result, fwhm * scale
def continuum_imexamine(setup, frame, sample_ext, cursor_file): iraf.imexamine(input='%s[%d]' % (frame,sample_ext), logfile='%s_ext%s_continuum_fit' % (setup, sample_ext), keeplog='yes', imagecur='%s_%s_cursor_file.dat' % (setup, frame))
print '\ncreating a zero_files/ dir to store original data'
if not os.path.isdir('zero_files'):
os.mkdir('zero_files')
allfiles = zerolist
for file in allfiles:
shutil.copy(file, 'zero_files/')
# combine bias images
print 'Combining zero level images...'
iraf.ccdred.zerocombine.ccdtype = ''
iraf.ccdred.zerocombine.reject = 'ccdclip'
iraf.ccdred.zerocombine.rdnoise = 'rdnoise'
iraf.ccdred.zerocombine.gain = 'gain'
iraf.ccdred.zerocombine(input=zeroin)
for zero in zerolist:
os.remove(zero)
print 'openning a ds9 window if not already openned...'
ds9.ds9()
# check output image
print 'Check output file:'
iraf.imstatistics('Zero')
print ' Running "imexamine" task..'
iraf.imexamine('Zero', 1)
print '--- DONE ---'
iraf.ccdred.combine.unlearn()
iraf.ccdred.zerocombine.unlearn()
iraf.ccdred.flatcombine.unlearn()
iraf.specred.response.unlearn()
# regular expression of files (e.g bias_00*.fits, flat-2000jan01_?.*)
theflat = str(raw_input('Enter flat image: '))
iraf.specred.extinction = ''
iraf.specred.caldir = ''
iraf.specred.observatory = 'lna'
print 'Create a response for flat...'
iraf.specred.response.interactive = True
iraf.specred.response.high_reject = 3.0
iraf.specred.response.low_reject = 3.0
iraf.specred.response(calibration=theflat,
normalization=theflat,
response='nFlat')
# check output flat image
print 'openning a ds9 window if not already openned...'
ds9.ds9()
print 'Check output file:'
iraf.imstatistics('nFlat')
print ' Running "imexamine" task..'
iraf.imexamine('nFlat', 1)
print '--- DONE ---'
def skynoise(image,path=None):
'''
Calcula el ruido del cielo de una imagen.
Toma una moda de la imagen total con \verb|imstat|. Luego genera una lista
de n puntos aleatorios entre los límites de la imagen, con
$n=\frac{anchoCCD^2}{10}$, y corre \verb|imexa| sobre cada punto, sacando
la estadística. Descarta los puntos que superen en cuentas 3 veces la moda
y toma la media de la desviación estandar del cielo de los puntos
restantes. Este valor es el que devuelve como aproximación del skynoise.
INPUT
image : una imagen
(path): camino a imagen
'''
if path is not None:
originalpath=aux.chdir(path,save=True)
stat= iraf.imstat(image,fields='mode',Stdout=1) #get the mode of the image
moda=float(stat[1]) # reads the mode as a float variable
binn=aux.hselect(image,'CCDSUM') # gets binning of the image
binn=binn[0] # access element 0 of the array
binn=binn[1] # access first character
binn=int(binn) # converts string to integer
#------------------------------------------------------------------
ccdsec=aux.hselect(image,'CCDSEC') # para agarrar imagenes con trim
if ccdsec[0]=='':
limits=aux.hselect(image,'CCDSIZE') # gets ccd pixel size
else:
limits=aux.hselect(image,'BIASSEC')
limit=limits[0] # gets element 0 of the array
limit=limit.strip() # removes white space
dd=[] # stores position of double dot
c=[] # stores position of comma
i=0
for x in limit: # for every character
if x==':': # if character is :
dd.append(i) #stores index
elif x==',': # if character is ,
c.append(i) #stores index
i=i+1
#-----------------------------------------------------------------
#
# x1=int(limit[1:dd[0]]) # saves first limit
# y1=int(limit[c[0]+1:dd[1]]) #saves las limit
x2=int(limit[dd[0]+1:c[0]])
y2=int(limit[dd[1]+1:-1])
l1=x2/binn # limit one
l2=y2/binn # limit two
# set random numbers aux file
aux.rm('ruidoceleste.coo') #delete if already exists
output='ruidoceleste.coo'
coords=[]
nrandom=int((l1**2)/100.) #quadratic growth
f=open(output,'a+') # creates outfile
for i in range(nrandom): # creates l1/10 random coordinates
x=random.randint(1,l1) # random x coord, from x1 to l1
y=random.randint(1,l2) # random y coord, from y1 to l2
coords.append([x,y])
print >> f,x,y # writes coords in file
f.close()
iraf.unlearn(iraf.imexamine) #unlearns imexamine first
# tuve que mandar estos comandos para que no me cambie el z1yz2 cada vez
# que calculaba todo. Cosa de como tenia mi seteado mi iraf ( o no?)
iraf.imexamine.autoredraw='no' #noredraw of the image
# iraf.display.zscale='no'
iraf.imexamine.allframes='no'
iraf.imexamine.use_display='no'
iraf.imexamine.imagecur=output # sets imexa infile
iraf.imexamine.defkey='m' # sets key to use in imexa
imst=iraf.imexamine(image,frame=1,Stdout=1) # calls imexa
stdev=[]
maxi=[]
for lin in imst[1:]:
stdev.append(float(lin.split()[4]))
maxi.append(float(lin.split()[6]))
# criterio de seleccion <3*moda no es estrella
validos=[]
for j in range(nrandom):
if maxi[j] < 3*moda:
validos.append(stdev[j])
sigmasky=mode(validos) # toma la moda
sigmasky=sigmasky[0][0]
# tomo la media de la disperción
# sigmasky=np.mean(validos)
# print validos
aux.rm(output) # mata el archivo auxiliar
if path is not None:
aux.chdir(originalpath)
return(sigmasky)
def getfwhm(images='@imh.lis',
coordlist='ref_stars',
outfile='getfwhm.log',
radius=4.0,
buffer=7.0,
width=5.0,
rplot=15.0,
center='no',
verbose='no',
imagelist=None,
mode='al',
DOLLARnargs=0,
taskObj=None):
Vars = IrafParList('getfwhm')
Vars.addParam(
makeIrafPar(images,
datatype='string',
name='images',
mode='a',
prompt='Input image(s)'))
Vars.addParam(
makeIrafPar(coordlist,
datatype='string',
name='coordlist',
mode='a',
prompt='List of object positions'))
Vars.addParam(
makeIrafPar(outfile,
datatype='string',
name='outfile',
mode='a',
prompt='Output file'))
Vars.addParam(
makeIrafPar(radius,
datatype='real',
name='radius',
mode='h',
prompt='Object radius'))
Vars.addParam(
makeIrafPar(buffer,
datatype='real',
name='buffer',
mode='h',
prompt='Background buffer width'))
Vars.addParam(
makeIrafPar(width,
datatype='real',
name='width',
mode='h',
prompt='Background width'))
Vars.addParam(
makeIrafPar(rplot,
datatype='real',
name='rplot',
mode='h',
prompt='Plotting radius'))
Vars.addParam(
makeIrafPar(center,
datatype='bool',
name='center',
mode='h',
prompt='Center object in aperture?'))
Vars.addParam(
makeIrafPar(verbose,
datatype='bool',
name='verbose',
mode='h',
prompt='Verbose output?'))
Vars.addParam(
makeIrafPar(imagelist,
datatype='struct',
name='imagelist',
list_flag=1,
mode='h'))
Vars.addParam(makeIrafPar(mode, datatype='string', name='mode', mode='h'))
Vars.addParam(
makeIrafPar(DOLLARnargs, datatype='int', name='$nargs', mode='h'))
Vars.addParam(makeIrafPar(None, datatype='int', name='len', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='image', mode='u'))
Vars.addParam(
makeIrafPar(None, datatype='string', name='imagefile', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='imlist',
mode='u'))
Vars.addParam(makeIrafPar(None, datatype='string', name='coords',
mode='u'))
Vars.addParam(
makeIrafPar(None, datatype='string', name='outputfile', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='rad', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='buff', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='wid', mode='u'))
Vars.addParam(makeIrafPar(None, datatype='real', name='rpl', mode='u'))
Vars.imlist = Vars.images
Vars.imagefile = iraf.mktemp('tmp$getfwhm')
iraf.sections(Vars.imlist, option='fullname', Stdout=Vars.imagefile)
Vars.imagelist = Vars.imagefile
Vars.coords = Vars.coordlist
Vars.outputfile = Vars.outfile
Vars.rad = Vars.radius
Vars.buff = Vars.buffer
Vars.wid = Vars.width
Vars.rpl = Vars.rplot
iraf.rimexam.radius = Vars.rad
iraf.rimexam.buffer = Vars.buff
iraf.rimexam.width = Vars.wid
iraf.rimexam.rplot = Vars.rpl
if (Vars.center == yes):
iraf.rimexam.center = yes
else:
iraf.rimexam.center = no
iraf.rimexam.fittype = 'gaussian'
iraf.rimexam.iterati = 1
iraf.clPrint('# RIMEXAM Parameter Settings: Radius=',
Vars.rad,
', Buffer=',
Vars.buff,
', Width=',
Vars.wid,
StdoutAppend=Vars.outputfile)
while (iraf.fscan(locals(), 'Vars.imagelist', 'Vars.image') != EOF):
Vars.len = iraf.strlen(Vars.image)
if (iraf.substr(Vars.image, Vars.len - 3, Vars.len) == '.imh'):
Vars.image = iraf.substr(Vars.image, 1, Vars.len - 4)
if (Vars.verbose):
iraf.clPrint('...processing ', Vars.image)
iraf.clPrint(Vars.image)
iraf.imexamine(Vars.image,
logfile=Vars.outputfile,
keeplog=yes,
defkey='a',
imagecur=Vars.coords,
wcs='world',
use_display=no)
def calc_upperlimit( self, skysigfits ):
skysigpath = os.path.join(self.dir,skysigfits)
hd = pyfits.open(skysigpath)[0].header
#set region range
one_side = round(0.5*self.aperture*np.sqrt(np.pi),0)
iraf.imexam.ncstat = one_side
iraf.imexam.nlstat = one_side
area_unit = one_side*one_side
#logical coord range
log_xmin = 1
log_xmax = float(hd["NAXIS1"])
log_ymin = 1
log_ymax = float(hd["NAXIS2"])
bias = 65 #np.sqrt((maxfwhm=20*1.75)**2*np.pi)
xmin = log_xmin + bias
xmax = log_xmax - bias
ymin = log_ymin + bias
ymax = log_ymax - bias
length_x = xmax - xmin
length_y = ymax - ymin
print length_x,length_y
sample_num = 1000
x = np.random.rand(sample_num)*length_x + bias
y = np.random.rand(sample_num)*length_y + bias
print len(x),len(y)
coords = SkyCoord(x,y,0,representation="cartesian")
print coords
idx,d2d,d3d = coords.match_to_catalog_3d(coords,nthneighbor=2)
required_d = one_side*np.sqrt(2)
print required_d
select = np.where(required_d < d3d)
print d3d
print select
survived = coords[select]
points = np.c_[x,y][select][:len(survived)]
ap_reg = os.path.join(self.dir,"aperture.reg") #random apertures
ap_tmp = os.path.join(self.dir,"aperture.tmp") #imexam m aperture template
with open(ap_reg,"w") as f, open(ap_tmp,"w") as g:
frame = 1
command = "m"
for i,xy in enumerate(points):
if i ==0:
f.write("global color=green dashlist=8 3 width=1 font=\"helvetica 10 normal roman\" select=1 highlite=1 dash=0 fixed=0 edit=1 move=1 delete=1 include=1 source=1\nimage\n")
x = round(xy[0],3)
y = round(xy[1],3)
tmp = "%s %s %s %s\n" % (x,y,frame,command)
g.write(tmp)
reg = "circle(%s,%s,10)\n" % (x,y)
f.write(reg)
output = os.path.join(self.dir,"aperture0.log")
iraf.imexamine(input=skysigpath,imagecur=ap_tmp,use_display="no",keeplog="yes",logfile=output,Stdout=True,frame=1)
log = os.path.join(self.dir,"aperture.log")
if os.path.exists(log):os.remove(log)
else:pass
os.system("sed -e \"1d\" %s > %s" % (output,log))
os.remove(output)
data = ascii.read(log)
print data.keys()
select = np.where(-200000. < data["MIN"])
print select
S = (0.5*self.aperture)**2*np.pi
mean_ls = np.array(data["MEAN"][select]*S)
clipper3 = ~sigma_clip(mean_ls,sigma=3).mask
mean_clip = mean_ls[clipper3]
self.random_ap_num = len(mean_clip)
print mean_clip
self.sigma = np.std(mean_clip)
print self.sigma
self.upperlimit = -2.5*np.log10(5*self.sigma) + self.Zmag
def ecpsf(img, ofwhm, threshold, psfstars, distance, interactive, ds9, psffun='gauss', fixaperture=False, _catalog='', _datamax=None, show=False):
try:
import lsc, string
hdr = lsc.util.readhdr(img + '.fits')
instrument = lsc.util.readkey3(hdr, 'instrume')
print 'INSTRUMENT:', instrument
if 'PIXSCALE' in hdr:
scale = lsc.util.readkey3(hdr, 'PIXSCALE')
elif 'CCDSCALE' in hdr:
if 'CCDXBIN' in hdr:
scale = lsc.util.readkey3(hdr, 'CCDSCALE') * lsc.util.readkey3(hdr, 'CCDXBIN')
elif 'CCDSUM' in hdr:
scale = lsc.util.readkey3(hdr, 'CCDSCALE') * int(string.split(lsc.util.readkey3(hdr, 'CCDSUM'))[0])
if _datamax is None and 'kb' in instrument:
_datamax = 45000
elif _datamax is None:
_datamax = 65000
_wcserr = lsc.util.readkey3(hdr, 'wcserr')
print _wcserr
if float(_wcserr) == 0:
if 'L1FWHM' in hdr:
seeing = float(lsc.util.readkey3(hdr, 'L1FWHM'))
elif 'L1SEEING' in hdr:
seeing = float(lsc.util.readkey3(hdr, 'L1SEEING')) * scale
else:
seeing = 3
else:
seeing = 3
if 'PSF_FWHM' in hdr:
seeing = float(lsc.util.readkey3(hdr, 'PSF_FWHM'))
else:
sys.exit('astrometry not good')
#except: sys.exit('astrometry not good')
fwhm = seeing / scale
print 'FWHM[header] ', fwhm, ' in pixel'
if ofwhm: fwhm = float(ofwhm)
print ' FWHM[input] ', fwhm, ' in pixel'
xdim, ydim = iraf.hselect(img+'[0]', 'i_naxis1,i_naxis2', 'yes', Stdout=1)[0].split()
print img, fwhm, threshold, scale,xdim
#################################################################################
################### write file to compute psf _psf.coo ############
#################################################################################
if interactive:
iraf.display(img, 1, fill=True)
iraf.delete('tmp.lo?', verify=False)
print '_' * 80
print '>>> Mark reference stars with "a". Then "q"'
print '-' * 80
iraf.imexamine(img, 1, wcs='logical', logfile='tmp.log', keeplog=True)
xyrefer = iraf.fields('tmp.log', '1,2,6,15', Stdout=1)
xns, yns, _fws = [], [], []
############# write file for PSF #########################
ff = open('_psf.coo', 'w')
for i in range(len(xyrefer)):
xns.append(float(xyrefer[i].split()[0]))
yns.append(float(xyrefer[i].split()[1]))
_fws.append(float(xyrefer[i].split()[3]))
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
ff.close()
fwhm = np.median(_fws)
elif _catalog:
print '\n#### use catalog to measure the psf'
ddd=iraf.wcsctran(input=_catalog,output='STDOUT',Stdout=1,image=img + '[0]',inwcs='world',outwcs='logical',
units='degrees degrees',columns='1 2',formats='%10.1f %10.1f',verbose='no')
ddd=[i for i in ddd if i[0]!='#']
ddd=[' '.join(i.split()[0:3]) for i in ddd]
line=''
for i in ddd:
a,b,c = string.split(i)
if float(a) < float(xdim) and float(b) < float(ydim) and float(b) > 0:
line = line + '%10s %10s %10s \n' % (a, b, c)
if line:
ff = open('_psf.coo', 'w')
ff.write(line)
ff.close()
else:
sys.exit('error: no catalog objects are in the field')
else:
############ run sextractor #####################################
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
tot = np.compress(abs(np.array(fluxrad) * 1.6 - fwhm) / fwhm < .5, fluxrad)
if len(tot) < 5:
print 'warning: fwhm from sexractor different from fwhm computed during pre-reduction'
print 'try using option --fwhm xxx'
ff = open('tmp.cursor', 'w')
image_hdu = fits.open(img + '.fits')
for i in range(len(xs)):
_xs = np.delete(xs, i)
_ys = np.delete(ys, i)
dist2 = np.sqrt((_xs - xs[i]) ** 2 + (_ys - ys[i]) ** 2)
########### cut star, not near other object ##########################
if abs(fluxrad[i] * 1.6 - fwhm) / fwhm < .5 and min(dist2) > distance * fwhm:
x1, x2 = int(xs[i] - fwhm * 3), int(xs[i] + fwhm * 3)
y1, y2 = int(ys[i] - fwhm * 3), int(ys[i] + fwhm * 3)
if x1 < 1: x1 = 1
if y1 < 1: y1 = 1
if x2 > int(xdim):
x2 = int(xdim)
if y2 > int(ydim):
y2 = int(ydim)
fmax = np.max(image_hdu[0].data[y1-1:y2, x1-1:x2])
########## cut saturated object ########################
if float(fmax) < _datamax: # not saturated
ff.write('%10.3f %10.3f 1 m \n' % (xs[i], ys[i]))
ff.close()
image_hdu.close()
iraf.delete('tmp.lo?,tmp.sta?,tmp.gk?', verify=False)
iraf.psfmeasure(img+'[0]', imagecur='tmp.cursor', logfile='tmp.log', radius=int(fwhm), iter=3,
display=False, StdoutG='tmp.gki')
ff = open('tmp.log')
righe = ff.readlines()
xn = [float(righe[3].split()[1])]
yn = [float(righe[3].split()[2])]
_fw = [float(righe[3].split()[4])]
for r in righe[4:-2]:
if len(r) > 0:
xn.append(float(r.split()[0]))
yn.append(float(r.split()[1]))
_fw.append(float(r.split()[3]))
print 'FWHM: ', righe[-1].split()[-1]
print 80 * "#"
######
############## eliminate double object identification ###########################
xns, yns, _fws = [xn[0]], [yn[0]], [_fw[0]]
for i in range(1, len(xn)):
if abs(xn[i] - xn[i - 1]) > .2 and abs(yn[i] - yn[i - 1]) > .2:
xns.append(xn[i])
yns.append(yn[i])
_fws.append(_fw[i])
######### write clean file for PSF #########################
fw = []
ff = open('_psf.coo', 'w')
for i in range(len(xns)):
if abs(_fws[i] - fwhm) / fwhm < .3:
ff.write('%10.3f %10.3f %7.2f \n' % (xns[i], yns[i], float(_fws[i])))
fw.append(_fws[i])
ff.close() ## End automatic selection
######################################################################################
################### write file of object to store in fits table #############
######################################################################################
if interactive:
xs, ys, ran, decn, magbest, classstar, fluxrad, bkg = runsex(img, fwhm, threshold, scale)
ff = open('_psf2.coo', 'w')
for i in range(len(xs)):
ff.write('%10s %10s %10s \n' % (xs[i], ys[i], fluxrad[i]))
ff.close()
elif _catalog:
ddd=iraf.wcsctran(input=_catalog,output='STDOUT',Stdout=1,image=img + '[0]',inwcs='world',outwcs='logical',
units='degrees degrees',columns='1 2',formats='%10.1f %10.1f',verbose='no')
ddd=[i for i in ddd if i[0]!='#']
ddd=[' '.join(i.split()[0:3]) for i in ddd]
ff = open('_psf2.coo', 'w')
for i in ddd:
a,b,c = string.split(i)
ff.write('%10s %10s %10s \n' % (a, b, c))
ff.close()
else:
os.system('cp _psf.coo _psf2.coo')
# dflux = fluxrad - np.median(fluxrad)
# fstar = np.compress(dflux < np.std(fluxrad), fluxrad)
#################################################################################################################
print 80 * "#"
photmag, pst, fitmag = psffit(img, fwhm, psfstars, hdr, interactive, _datamax, psffun, fixaperture)
photmag2, fitmag2 = psffit2(img, fwhm, psfstars, hdr, _datamax, psffun, fixaperture)
radec = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag,
Stdout=1, image=img + '[0]', inwcs='logical', outwcs='world', columns="1 2",
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
radec2 = iraf.wcsctran(input='STDIN', output='STDOUT', Stdin=photmag2,
Stdout=1, image=img + '[0]', inwcs='logical', outwcs='world', columns="1 2",
format='%13.3H %12.2h', min_sig=9, mode='h')[3:]
if ds9 == 0 and (interactive or show):
iraf.set(stdimage='imt1024')
iraf.display(img, 1, fill=True, Stdout=1)
iraf.tvmark(1, coords='STDIN', mark='circle', radii=15, label=True, Stdin=photmag, nxoffset=5, nyoffset=5, txsize=2)
iraf.tvmark(1, coords='STDIN', mark='circle', radii=35, label=False, Stdin=pst, color=208)
# iraf.tvmark(1, coords='STDIN', mark='cross', length=35, label=False, Stdin=fitmag2, color=204)
idpsf = []
for i in range(len(pst)):
idpsf.append(pst[i].split()[2])
dmag = []
for i in range(len(radec)):
ra, dec, idph, magp2, magp3, magp4, merrp2, merrp3, merrp4 = radec[i].split()
dmag.append(9.99)
for j in range(len(fitmag)):
raf, decf, idf, magf, magerrf = fitmag[j].split()
if idph == idf and idph in idpsf and \
magp3 != 'INDEF' and magf != 'INDEF':
dmag[i] = float(magp3) - float(magf)
break
_dmag = np.compress(np.array(dmag) < 9.99, np.array(dmag))
print '>>> Aperture correction (phot) %6.3f +/- %5.3f %3d ' % \
(np.mean(_dmag), np.std(_dmag), len(_dmag))
if len(_dmag) > 3:
_dmag = np.compress(np.abs(_dmag - np.median(_dmag)) < 2 * np.std(_dmag), _dmag)
print '>>> 2 sigma rejection) %6.3f +/- %5.3f %3d [default]' \
% (np.mean(_dmag), np.std(_dmag), len(_dmag))
print '>>> fwhm %s ' % (str(fwhm))
for i in range(len(dmag)):
if dmag[i] == 9.99:
dmag[i] = ''
else:
dmag[i] = '%6.3f' % (dmag[i])
exptime = lsc.util.readkey3(hdr, 'exptime')
object = lsc.util.readkey3(hdr, 'object').replace(' ', '')
filtro = lsc.util.readkey3(hdr, 'filter')
#######################################
rap, decp, magp2, magp3, magp4, smagf, merrp3, smagerrf = [], [], [], [], [], [], [], []
rap0, decp0 = [], []
for i in range(len(radec2)):
aa = radec2[i].split()
rap.append(aa[0])
decp.append(aa[1])
rap0.append(lsc.lscabsphotdef.deg2HMS(ra=aa[0]))
decp0.append(lsc.lscabsphotdef.deg2HMS(dec=aa[1]))
idp = aa[2]
magp2.append(aa[3])
magp3.append(aa[4])
magp4.append(aa[5])
merrp3.append(aa[7])
_smagf, _smagerrf = 9999, 9999
for j in range(len(fitmag2)):
raf, decf, idf, magf, magerrf = fitmag2[j].split()
if idf == idp:
_smagf = magf
_smagerrf = magerrf
break
smagf.append(_smagf)
smagerrf.append(_smagerrf)
tbhdu = fits.BinTableHDU.from_columns(fits.ColDefs([fits.Column(name='ra', format='20A', array=np.array(rap)),
fits.Column(name='dec', format='20A', array=np.array(decp)),
fits.Column(name='ra0', format='E', array=np.array(rap0)),
fits.Column(name='dec0', format='E', array=np.array(decp0)),
fits.Column(name='magp2', format='E',
array=np.array(np.where((np.array(magp2) != 'INDEF'),
np.array(magp2), 9999), float)),
fits.Column(name='magp3', format='E',
array=np.array(np.where((np.array(magp3) != 'INDEF'),
np.array(magp3), 9999), float)),
fits.Column(name='merrp3', format='E',
array=np.array(np.where((np.array(merrp3) != 'INDEF'),
np.array(merrp3), 9999), float)),
fits.Column(name='magp4', format='E',
array=np.array(np.where((np.array(magp4) != 'INDEF'),
np.array(magp4), 9999), float)),
fits.Column(name='smagf', format='E',
array=np.array(np.where((np.array(smagf) != 'INDEF'),
np.array(smagf), 9999), float)),
fits.Column(name='smagerrf', format='E',
array=np.array(np.where((np.array(smagerrf) != 'INDEF'),
np.array(smagerrf), 9999),
float)),
]))
hdu = fits.PrimaryHDU(header=hdr)
thdulist = fits.HDUList([hdu, tbhdu])
lsc.util.delete(img + '.sn2.fits')
thdulist.writeto(img + '.sn2.fits')
lsc.util.updateheader(img + '.sn2.fits', 0, {'APCO': [np.mean(_dmag), 'Aperture correction']})
lsc.util.updateheader(img + '.sn2.fits', 0, {'APCOERR': [np.std(_dmag), 'Aperture correction error']})
lsc.util.updateheader(img + '.sn2.fits', 0, {'XDIM': [lsc.util.readkey3(hdr, 'naxis1'), 'x number of pixels']})
lsc.util.updateheader(img + '.sn2.fits', 0, {'YDIM': [lsc.util.readkey3(hdr, 'naxis2'), 'y number of pixels']})
lsc.util.updateheader(img + '.sn2.fits', 0,
{'PSF_FWHM': [fwhm * scale, 'FWHM (arcsec) - computed with daophot']})
os.chmod(img + '.sn2.fits', 0664)
os.chmod(img + '.psf.fits', 0664)
result = 1
except:
result = 0
fwhm = 0.0
traceback.print_exc()
return result, fwhm * scale
xx0, yy0 = string.split(iraf.fields('tmp.pix', '1,2', Stdout=1)[2])
print 'box coordinate ',xx0, yy0
os.system('rm -rf tmp.*')
else:
xx0, yy0 = '', ''
if xx0 == '' and not _interactive:
sys.exit('coordinate of the object not found, reduction not possible')
if _interactive:
repeat = 'y'
while repeat == 'y':
print "_____________________________________________"
print " MARK SN REGION WITH - x -, EXIT - q -"
try:
iraf.imexamine(img + '.fits', 1, wcs='logical', logfile='tmp.log', keeplog=True)
xytargets = iraf.fields('tmp.log', '1,2', Stdout=1)
xx0 = xytargets[0].split()[0]
yy0 = xytargets[0].split()[1]
lsc.util.delete("tmplabel")
ff = open('tmplabel', 'w')
ff.write(str(xx0) + ' ' + str(yy0) + ' -1' + ' \n')
ff.close()
iraf.tvmark(1, 'tmplabel', autol='no', mark="cross", inter='no', label='no', txsize=4)
repeat = raw_input('### repeat selection ? [y/n] ? [n] ')
if not repeat:
repeat = 'n'
elif repeat == 'yes':
repeat = 'y'
elif repeat == 'YES':
repeat = 'y'
if _interactive: xx0 = ''
_z1, _z2 = '', ''
z11, z22 = 0, 0
if xx0 == '':
#print '\n### coordinate not found, reduction should be interactive'
_interactive = True
_show = True
###################### POINT TO SN #######################################
repeat = 'y'
while repeat == 'y':
print "_____________________________________________"
print " MARK SN REGION WITH - x -, EXIT - q -"
try:
iraf.imexamine(img + '.fits',
1,
wcs='logical',
logfile='tmp.log',
keeplog=True)
xytargets = iraf.fields('tmp.log', '1,2', Stdout=1)
x = xytargets[0].split()[0]
y = xytargets[0].split()[1]
agnkey.util.delete("tmplabel")
ff = open('tmplabel', 'w')
ff.write(str(x) + ' ' + str(y) + ' -1' + ' \n')
ff.close()
iraf.tvmark(1,
'tmplabel',
autol='no',
mark="cross",
inter='no',
label='no',
iraf.imred()
iraf.ccdred()
iraf.specred()
ds9()
iraf.zerocombine.unlearn()
iraf.zerocombine(input=bias,
reject='avsigclip',
ccdtype='',
rdnoise='rdnoise',
gain='gain')
iraf.imstat('bias*')
iraf.imstat('Zero')
iraf.imexamine('Zero')
iraf.flatcombine.unlearn()
iraf.flatcombine(input=flatcup,
output='Flat',
ccdtype='',
process=False,
subsets=False,
rdnoise='rdnoise',
gain='gain')
iraf.flatcombine(input=flati,
output='iFlat',
ccdtype='',
process=False,
subsets=False,