def __init__(self, root='sdssj1723+3411', filter='f140w', galfit_exec='galfit', catfile=None, segfile=None):
self.root = root
self.galfit_exec = galfit_exec
self.filter = filter
data = self.get_data(filter=filter, catfile=catfile, segfile=segfile)
self.sci, self.wht, self.seg, self.cat, self.wcs = data
self.flt_files = self.get_flt_files(sci_hdu=self.sci)
self.DPSF = DrizzlePSF(flt_files=self.flt_files, info=None, driz_image=self.sci.filename())
def __init__(self, root='sdssj1723+3411', filter='f140w', galfit_exec='galfit', catfile=None, segfile=None):
self.root = root
self.galfit_exec = galfit_exec
self.filter = filter
data = self.get_data(filter=filter, catfile=catfile, segfile=segfile)
self.sci, self.wht, self.seg, self.cat, self.wcs = data
self.flt_files = self.get_flt_files(sci_hdu=self.sci)
self.DPSF = DrizzlePSF(flt_files=self.flt_files, info=None, driz_image=self.sci.filename())
def drizzle_images(label='macs0647-jd1', ra=101.9822125, dec=70.24326667, pixscale=0.06, size=10, wcs=None, pixfrac=0.8, kernel='square', theta=0, half_optical_pixscale=False, filters=['f160w','f814w', 'f140w','f125w','f105w','f110w','f098m','f850lp', 'f775w', 'f606w','f475w','f555w','f600lp', 'f390w', 'f350lp'], remove=True, rgb_params=RGB_PARAMS, master='grizli-jan2019', aws_bucket='s3://grizli/CutoutProducts/', scale_ab=21, thumb_height=2.0, sync_fits=True, subtract_median=True, include_saturated=True, include_ir_psf=False):
"""
label='cp561356'; ra=150.208875; dec=1.850241667; size=40; filters=['f160w','f814w', 'f140w','f125w','f105w','f606w','f475w']
"""
import glob
import copy
import os
import numpy as np
import astropy.io.fits as pyfits
from astropy.coordinates import SkyCoord
import astropy.units as u
from drizzlepac.adrizzle import do_driz
import boto3
from grizli import prep, utils
from grizli.pipeline import auto_script
if isinstance(ra, str):
coo = SkyCoord('{0} {1}'.format(ra, dec), unit=(u.hour, u.deg))
ra, dec = coo.ra.value, coo.dec.value
if label is None:
try:
import mastquery.utils
label = mastquery.utils.radec_to_targname(ra=ra, dec=dec, round_arcsec=(1/15, 1), targstr='j{rah}{ram}{ras}{sign}{ded}{dem}{des}')
except:
label = 'grizli-cutout'
#master = 'cosmos'
#master = 'grizli-jan2019'
if master == 'grizli-jan2019':
parent = 's3://grizli/MosaicTools/'
s3 = boto3.resource('s3')
s3_client = boto3.client('s3')
bkt = s3.Bucket('grizli')
elif master == 'cosmos':
parent = 's3://grizli-preprocess/CosmosMosaic/'
s3 = boto3.resource('s3')
s3_client = boto3.client('s3')
bkt = s3.Bucket('grizli-preprocess')
else:
# Run on local files, e.g., "Prep" directory
parent = None
remove = False
for ext in ['_visits.fits', '_visits.npy', '_filter_groups.npy'][-1:]:
if (not os.path.exists('{0}{1}'.format(master, ext))) & (parent is not None):
s3_path = parent.split('/')[-2]
s3_file = '{0}{1}'.format(master, ext)
print('{0}{1}'.format(parent, s3_file))
bkt.download_file(s3_path+'/'+s3_file, s3_file,
ExtraArgs={"RequestPayer": "requester"})
#os.system('aws s3 cp {0}{1}{2} ./'.format(parent, master, ext))
#tab = utils.read_catalog('{0}_visits.fits'.format(master))
#all_visits = np.load('{0}_visits.npy'.format(master))[0]
if parent is not None:
groups = np.load('{0}_filter_groups.npy'.format(master), allow_pickle=True)[0]
else:
# Reformat local visits.npy into a groups file
groups_files = glob.glob('*filter_groups.npy')
if len(groups_files) == 0:
visit_file = glob.glob('*visits.npy')[0]
visits, groups, info = np.load(visit_file)
visit_root = visit_file.split('_visits')[0]
visit_filters = np.array([v['product'].split('-')[-1] for v in visits])
groups = {}
for filt in np.unique(visit_filters):
groups[filt] = {}
groups[filt]['filter'] = filt
groups[filt]['files'] = []
groups[filt]['footprints'] = []
groups[filt]['awspath'] = None
ix = np.where(visit_filters == filt)[0]
for i in ix:
groups[filt]['files'].extend(visits[i]['files'])
groups[filt]['footprints'].extend(visits[i]['footprints'])
np.save('{0}_filter_groups.npy'.format(visit_root), [groups])
else:
groups = np.load(groups_files[0])[0]
#filters = ['f160w','f814w', 'f110w', 'f098m', 'f140w','f125w','f105w','f606w', 'f475w']
has_filts = []
for filt in filters:
if filt not in groups:
continue
visits = [copy.deepcopy(groups[filt])]
#visits[0]['reference'] = 'CarlosGG/ak03_j1000p0228/Prep/ak03_j1000p0228-f160w_drz_sci.fits'
visits[0]['product'] = label+'-'+filt
if wcs is None:
hdu = utils.make_wcsheader(ra=ra, dec=dec, size=size, pixscale=pixscale, get_hdu=True, theta=theta)
h = hdu.header
else:
h = utils.to_header(wcs)
if (filt[:2] in ['f0', 'f1', 'g1']) | (not half_optical_pixscale):
#data = hdu.data
pass
else:
for k in ['NAXIS1','NAXIS2','CRPIX1','CRPIX2']:
h[k] *= 2
h['CRPIX1'] -= 0.5
h['CRPIX2'] -= 0.5
for k in ['CD1_1', 'CD1_2', 'CD2_1', 'CD2_2']:
h[k] /= 2
#data = np.zeros((h['NAXIS2'], h['NAXIS1']), dtype=np.int16)
#pyfits.PrimaryHDU(header=h, data=data).writeto('ref.fits', overwrite=True, output_verify='fix')
#visits[0]['reference'] = 'ref.fits'
print('\n\n###\nMake filter: {0}'.format(filt))
if (filt.upper() in ['F105W','F125W','F140W','F160W']) & include_ir_psf:
clean_i = False
else:
clean_i = remove
status = utils.drizzle_from_visit(visits[0], h, pixfrac=pixfrac, kernel=kernel, clean=clean_i, include_saturated=include_saturated)
if status is not None:
sci, wht, outh = status
if subtract_median:
med = np.median(sci[sci != 0])
print('\n\nMedian {0} = {1:.3f}\n\n'.format(filt, med))
sci -= med
outh['IMGMED'] = (med, 'Median subtracted from the image')
else:
med = 0.
outh['IMGMED'] = (med, 'Median subtracted from the image')
pyfits.writeto('{0}-{1}_drz_sci.fits'.format(label, filt),
data=sci, header=outh, overwrite=True,
output_verify='fix')
pyfits.writeto('{0}-{1}_drz_wht.fits'.format(label, filt),
data=wht, header=outh, overwrite=True,
output_verify='fix')
has_filts.append(filt)
if (filt.upper() in ['F105W','F125W','F140W','F160W']) & include_ir_psf:
from grizli.galfit.psf import DrizzlePSF
hdu = pyfits.open('{0}-{1}_drz_sci.fits'.format(label, filt),
mode='update')
flt_files = [] #visits[0]['files']
for i in range(1, 10000):
key = 'FLT{0:05d}'.format(i)
if key not in hdu[0].header:
break
flt_files.append(hdu[0].header[key])
dp = DrizzlePSF(flt_files=flt_files, driz_hdu=hdu[0])
psf = dp.get_psf(ra=dp.driz_wcs.wcs.crval[0],
dec=dp.driz_wcs.wcs.crval[1],
filter=filt.upper(),
pixfrac=dp.driz_header['PIXFRAC'],
kernel=dp.driz_header['KERNEL'],
wcs_slice=dp.driz_wcs, get_extended=True,
verbose=False, get_weight=False)
psf[1].header['EXTNAME'] = 'PSF'
#psf[1].header['EXTVER'] = filt
hdu.append(psf[1])
hdu.flush()
#psf.writeto('{0}-{1}_drz_sci.fits'.format(label, filt),
# overwrite=True, output_verify='fix')
#status = prep.drizzle_overlaps(visits, parse_visits=False, check_overlaps=True, pixfrac=pixfrac, skysub=False, final_wcs=True, final_wht_type='IVM', static=True, max_files=260, fix_wcs_system=True)
#
# if len(glob.glob('{0}-{1}*sci.fits'.format(label, filt))):
# has_filts.append(filt)
if remove:
os.system('rm *_fl*fits')
if len(has_filts) == 0:
return []
if rgb_params:
#auto_script.field_rgb(root=label, HOME_PATH=None, filters=has_filts, **rgb_params)
show_all_thumbnails(label=label, thumb_height=thumb_height, scale_ab=scale_ab, close=True, rgb_params=rgb_params)
if aws_bucket:
#aws_bucket = 's3://grizli-cosmos/CutoutProducts/'
#aws_bucket = 's3://grizli/CutoutProducts/'
s3 = boto3.resource('s3')
s3_client = boto3.client('s3')
bkt = s3.Bucket(aws_bucket.split("/")[2])
aws_path = '/'.join(aws_bucket.split("/")[3:])
if sync_fits:
files = glob.glob('{0}*'.format(label))
else:
files = glob.glob('{0}*png'.format(label))
for file in files:
print('{0} -> {1}'.format(file, aws_bucket))
bkt.upload_file(file, '{0}/{1}'.format(aws_path, file).replace('//','/'), ExtraArgs={'ACL': 'public-read'})
#os.system('aws s3 sync --exclude "*" --include "{0}*" ./ {1} --acl public-read'.format(label, aws_bucket))
#os.system("""echo "<pre>" > index.html; aws s3 ls AWSBUCKETX --human-readable | sort -k 1 -k 2 | grep -v index | awk '{printf("%s %s",$1, $2); printf(" %6s %s ", $3, $4); print "<a href="$5">"$5"</a>"}'>> index.html; aws s3 cp index.html AWSBUCKETX --acl public-read""".replace('AWSBUCKETX', aws_bucket))
return has_filts
class Galfitter(object):
def __init__(self,
root='sdssj1723+3411',
filter='f140w',
galfit_exec='galfit',
catfile=None,
segfile=None):
self.root = root
self.galfit_exec = galfit_exec
self.filter = filter
data = self.get_data(filter=filter, catfile=catfile, segfile=segfile)
self.sci, self.wht, self.seg, self.cat, self.wcs = data
self.flt_files = self.get_flt_files(sci_hdu=self.sci)
self.DPSF = DrizzlePSF(flt_files=self.flt_files,
info=None,
driz_image=self.sci.filename())
def get_data(self, filter='f140w', catfile=None, segfile=None):
import glob
sci_file = glob.glob('{0}-{1}_dr?_sci.fits'.format(self.root, filter))
sci = pyfits.open(sci_file[0])
wht = pyfits.open(sci_file[0].replace('sci', 'wht'))
if segfile is None:
segfile = sci_file[0].split('_dr')[0] + '_seg.fits'
seg = pyfits.open(segfile)
if catfile is None:
catfile = '{0}-{1}.cat.fits'.format(self.root, filter)
cat = utils.GTable.gread(catfile)
wcs = pywcs.WCS(sci[0].header, relax=True)
return sci, wht, seg, cat, wcs
def get_flt_files(self, sci_hdu=None):
flt_files = []
h = self.sci[0].header
for i in range(h['NDRIZIM']):
file = h['D{0:03d}DATA'.format(i + 1)].split('[sci')[0]
if file not in flt_files:
flt_files.append(file)
return flt_files
@staticmethod
def fit_arrays(sci,
wht,
seg,
psf,
id=None,
platescale=0.06,
exptime=0,
path='/tmp',
root='gf',
galfit_exec='galfit',
ab_zeropoint=26,
gaussian_guess=False,
components=[GalfitSersic()],
recenter=True,
psf_sample=1,
write_constraints=True):
"""
Fit array data with Galfit
"""
from astropy.coordinates import Angle
import astropy.units as u
rms = 1 / np.sqrt(wht) # *exptime
if exptime > 0:
rms = np.sqrt((rms * exptime)**2 + sci * exptime *
(sci > 0)) / exptime
rms[wht == 0] = 1e30
if id is not None:
mask = ((seg > 0) & (seg != id)) | (wht == 0)
else:
mask = wht == 0
sh = sci.shape[0]
fp = open('{0}/{1}.feedme'.format(path, root), 'w')
sci_file = '{0}/{1}_sci.fits'.format(path, root)
constraints_file = sci_file.replace('_sci.fits', '.constraints')
cmd = GALFIT_IMAGES.format(input=sci_file,
output=sci_file.replace('_sci', '_out'),
sigma=sci_file.replace('_sci', '_rms'),
psf=sci_file.replace('_sci', '_psf'),
mask=sci_file.replace('_sci', '_mask'),
constraints=constraints_file,
xmax=sh,
ymax=sh,
sh=sh,
ps=platescale,
psf_sample=psf_sample,
ab_zeropoint=ab_zeropoint)
fp.write(cmd)
if gaussian_guess:
fit, q, theta = fit_gauss(sci)
if (not os.path.exists(constraints_file)) & (write_constraints):
fpc = open(constraints_file, 'w')
else:
fpc = None
for i, comp in enumerate(components):
if recenter:
comp.set(pos=[sh / 2., sh / 2.])
if gaussian_guess:
comp.set(q=q,
pa=Angle.wrap_at(theta * u.rad,
360 * u.deg).to(u.deg).value)
fp.write(str(comp))
if fpc is not None:
fpc.write(SERSIC_CONSTRAINTS.format(comp=i + 1))
fp.close()
if fpc is not None:
fpc.close()
pyfits.writeto(sci_file, data=sci, overwrite=True)
pyfits.writeto(sci_file.replace('_sci', '_rms'),
data=rms,
overwrite=True)
pyfits.writeto(sci_file.replace('_sci', '_mask'),
data=mask * 1,
overwrite=True)
pyfits.writeto(sci_file.replace('_sci', '_psf'),
data=psf,
overwrite=True)
for ext in ['out', 'model']:
fi = sci_file.replace('_sci', '_' + ext)
if os.path.exists(fi):
os.remove(fi)
os.system('{0} {1}/{2}.feedme'.format(galfit_exec, path, root))
# Move galfit.[latest] to output file
gf_files = glob.glob('galfit.[0-9]*')
gf_files.sort()
gf_log = sci_file.replace('_sci.fits', '.gfmodel')
os.system('mv {0} {1}'.format(gf_files[-1], gf_log))
lines = open(gf_log).readlines()
# Results dictionary
res = {}
res['rms'] = rms
res['mask'] = mask * 1
im = pyfits.open(sci_file.replace('_sci', '_out'))
res['model'] = im[2]
res['resid'] = im[3]
res['ascii'] = lines
return res
def fit_object(self,
id=449,
radec=(None, None),
size=40,
components=[GalfitSersic()],
recenter=True,
get_mosaic=True,
gaussian_guess=False,
get_extended=True):
"""
Fit an object
"""
if id is not None:
rd = self.cat['X_WORLD', 'Y_WORLD'][self.cat['NUMBER'] == id][0]
radec = tuple(rd)
xy = self.wcs.all_world2pix([radec[0]], [radec[1]], 0)
xy = np.array(xy).flatten()
xp = np.cast[int](np.round(xy))
slx, sly, wcs_slice = self.DPSF.get_driz_cutout(ra=radec[0],
dec=radec[1],
get_cutout=False,
size=size)
#drz_cutout = self.get_driz_cutout(ra=ra, dec=dec, get_cutout=True)
h = self.sci[0].header
psf = self.DPSF.get_psf(ra=radec[0],
dec=radec[1],
filter=self.filter.upper(),
wcs_slice=wcs_slice,
pixfrac=h['D001PIXF'],
kernel=h['D001KERN'],
get_extended=get_extended)
exptime = h['EXPTIME']
sci = self.sci[0].data[sly, slx] # *exptime
wht = self.wht[0].data[sly, slx]
rms = 1 / np.sqrt(wht) # *exptime
rms = np.sqrt((rms * exptime)**2 + sci * exptime * (sci > 0)) / exptime
rms[wht == 0] = 1e30
seg = self.seg[0].data[sly, slx]
if id is not None:
mask = ((seg > 0) & (seg != id)) | (wht == 0)
else:
mask = wht == 0
sh = sci.shape[0]
path = '/tmp/'
psf_file = '{0}-{1}_psf_{2:05d}.fits'.format(self.root, self.filter,
id)
fp = open(path + 'galfit.feedme', 'w')
fp.write(
GALFIT_IMAGES.format(input=path + 'gf_sci.fits',
output=path + 'gf_out.fits',
sigma=path + 'gf_rms.fits',
psf=psf_file,
mask=path + 'gf_mask.fits',
xmax=sh,
ymax=sh,
sh=sh,
ps=self.DPSF.driz_pscale,
psf_sample=1,
constraints='none',
ab_zeropoint=26))
if gaussian_guess:
fit, q, theta = fit_gauss(sci)
from astropy.coordinates import Angle
import astropy.units as u
for comp in components:
if recenter:
comp.set(pos=[sh / 2., sh / 2.])
if gaussian_guess:
comp.set(q=q,
pa=Angle.wrap_at(theta * u.rad,
360 * u.deg).to(u.deg).value)
fp.write(str(comp))
fp.close()
pyfits.writeto(path + 'gf_sci.fits', data=sci, overwrite=True)
pyfits.writeto(path + 'gf_rms.fits', data=rms, overwrite=True)
pyfits.writeto(path + 'gf_mask.fits', data=mask * 1, overwrite=True)
#pyfits.writeto(path+'gf_psf.fits', data=psf[1].data, overwrite=True)
pyfits.writeto(psf_file, data=psf[1].data, overwrite=True)
for ext in ['out', 'model']:
if os.path.exists(path + 'gf_{0}.fits'.format(ext)):
os.remove(path + 'gf_{0}.fits'.format(ext))
os.system('{0} {1}/galfit.feedme'.format(self.galfit_exec, path))
#out = pyfits.open('/tmp/gf_out.fits')
# Get in DRZ frame
gf_file = glob.glob('galfit.[0-9]*')[-1]
lines = open(gf_file).readlines()
for il, line in enumerate(lines):
if line.startswith('A)'):
lines[
il] = 'A) {0} # Input data image (FITS file)\n'.format(
self.sci.filename())
if line.startswith('B)'):
lines[
il] = 'B) {0}-{1}_galfit_{2:05d}.fits # Output data image block\n'.format(
self.root, self.filter, id)
if line.startswith('P) 0'):
lines[
il] = "P) 1 # Choose: 0=optimize, 1=model, 2=imgblock, 3=subcomps\n"
if line.startswith('H)'):
out_sh = self.sci[0].data.shape
lines[
il] = "H) 1 {0} 1 {1} # Image region to fit (xmin xmax ymin ymax)\n".format(
out_sh[1], out_sh[0])
if line.startswith(' 1)'):
xy = np.cast[float](line.split()[1:3])
lines[il] = ' 1) {0} {1} 1 1 # Position x, y\n'.format(
xy[0] + slx.start, xy[1] + sly.start)
fp = open('galfit.{0}.{1:05d}'.format(self.filter, id), 'w')
fp.writelines(lines)
fp.close()
os.system('{0} galfit.{1}.{2:05d}'.format(self.galfit_exec,
self.filter, id))
model = pyfits.open('{0}-{1}_galfit_{2:05d}.fits'.format(
self.root, self.filter, id),
mode='update')
model[0].data /= self.sci[0].header['EXPTIME']
model.flush()
return (lines, model)
model = pyfits.open('/tmp/gf_model.fits')
if False:
full_model = self.sci[0].data * 0
full_model += model[0].data
pyfits.writeto('{0}-{1}_galfit.fits'.format(self.root, self.filter),
data=full_model,
header=self.sci[0].header,
overwrite=True)
def drizzle_images(label='macs0647-jd1', ra=101.9822125, dec=70.24326667, pixscale=0.1, size=10, wcs=None, pixfrac=0.33, kernel='square', theta=0, half_optical_pixscale=True, filters=['f160w', 'f140w', 'f125w', 'f105w', 'f110w', 'f098m', 'f850lp', 'f814w', 'f775w', 'f606w', 'f475w', 'f555w', 'f600lp', 'f390w', 'f350lp'], skip=None, remove=True, rgb_params=RGB_PARAMS, master='grizli-jan2019', aws_bucket='s3://grizli/CutoutProducts/', scale_ab=21, thumb_height=2.0, sync_fits=True, subtract_median=True, include_saturated=True, include_ir_psf=False, show_filters=['visb', 'visr', 'y', 'j', 'h'], combine_similar_filters=True, single_output=True, aws_prep_dir=None, make_segmentation_figure=False, get_dict=False, dryrun=False, **kwargs):
"""
label='cp561356'; ra=150.208875; dec=1.850241667; size=40; filters=['f160w','f814w', 'f140w','f125w','f105w','f606w','f475w']
master: These are sets of large lists of available exposures
'cosmos': deprecated
'grizli-cosmos-v2': All imaging covering the COSMOS field
'candels-july2019': CANDELS fields other than COSMOS
'grizli-v1': First processing of the Grizli CHArGE dataset
'grizli-v1-19.12.04': Updated CHArGE fields
"""
import glob
import copy
import os
import numpy as np
import astropy.io.fits as pyfits
from astropy.coordinates import SkyCoord
import astropy.units as u
from drizzlepac.adrizzle import do_driz
import boto3
from grizli import prep, utils
from grizli.pipeline import auto_script
# Function arguments
if get_dict:
frame = inspect.currentframe()
args = inspect.getargvalues(frame).locals
pop_args = ['get_dict', 'frame', 'kwargs']
pop_classes = (np.__class__, do_driz.__class__, SkyCoord.__class__)
for k in kwargs:
args[k] = kwargs[k]
for k in args:
if isinstance(args[k], pop_classes):
pop_args.append(k)
for k in pop_args:
if k in args:
args.pop(k)
return args
# Boto objects
s3 = boto3.resource('s3')
s3_client = boto3.client('s3')
if isinstance(ra, str):
coo = SkyCoord('{0} {1}'.format(ra, dec), unit=(u.hour, u.deg))
ra, dec = coo.ra.value, coo.dec.value
if label is None:
try:
import mastquery.utils
label = mastquery.utils.radec_to_targname(ra=ra, dec=dec, round_arcsec=(1/15, 1), targstr='j{rah}{ram}{ras}{sign}{ded}{dem}{des}')
except:
label = 'grizli-cutout'
#master = 'cosmos'
#master = 'grizli-jan2019'
if master == 'grizli-jan2019':
parent = 's3://grizli/MosaicTools/'
bkt = s3.Bucket('grizli')
elif master == 'cosmos':
parent = 's3://grizli-preprocess/CosmosMosaic/'
bkt = s3.Bucket('grizli-preprocess')
elif master == 'grizli-cosmos-v2':
parent = 's3://grizli-cosmos-v2/Mosaics/'
bkt = s3.Bucket('grizli-cosmos-v2')
elif master == 'candels-july2019':
parent = 's3://grizli-v1/Mosaics/'
bkt = s3.Bucket('grizli-v1')
elif master == 'grizli-v1-19.12.04':
parent = 's3://grizli-v1/Mosaics/'
bkt = s3.Bucket('grizli-v1')
elif master == 'grizli-v1-19.12.05':
parent = 's3://grizli-v1/Mosaics/'
bkt = s3.Bucket('grizli-v1')
else:
# Run on local files, e.g., "Prep" directory
parent = None
bkt = None
#remove = False
# Download summary files from S3
for ext in ['_visits.fits', '_visits.npy', '_filter_groups.npy'][-1:]:
newfile = '{0}{1}'.format(master, ext)
if (not os.path.exists(newfile)) & (parent is not None):
s3_path = parent.split('/')[-2]
s3_file = '{0}{1}'.format(master, ext)
print('{0}{1}'.format(parent, s3_file))
bkt.download_file(s3_path+'/'+s3_file, s3_file,
ExtraArgs={"RequestPayer": "requester"})
#os.system('aws s3 cp {0}{1}{2} ./'.format(parent, master, ext))
#tab = utils.read_catalog('{0}_visits.fits'.format(master))
#all_visits = np.load('{0}_visits.npy'.format(master))[0]
if parent is not None:
groups = np.load('{0}_filter_groups.npy'.format(master), allow_pickle=True)[0]
else:
if aws_prep_dir is not None:
spl = aws_prep_dir.replace('s3://', '').split('/')
prep_bucket = spl[0]
prep_root = spl[2]
prep_bkt = s3.Bucket(prep_bucket)
s3_prep_path = 'Pipeline/{0}/Prep/'.format(prep_root)
s3_full_path = '{0}/{1}'.format(prep_bucket, s3_prep_path)
s3_file = '{0}_visits.npy'.format(prep_root)
# Make output path Prep/../Thumbnails/
if aws_bucket is not None:
aws_bucket = ('s3://' +
s3_full_path.replace('/Prep/', '/Thumbnails/'))
print('{0}{1}'.format(s3_prep_path, s3_file))
if not os.path.exists(s3_file):
prep_bkt.download_file(os.path.join(s3_prep_path, s3_file),
s3_file, ExtraArgs={"RequestPayer": "requester"})
groups_files = glob.glob('{0}_filter_groups.npy'.format(prep_root))
visit_query = prep_root+'_'
else:
groups_files = glob.glob('*filter_groups.npy')
visit_query = '*'
# Reformat local visits.npy into a groups file
if (len(groups_files) == 0):
visit_file = glob.glob(visit_query+'visits.npy')[0]
visits, groups, info = np.load(visit_file, allow_pickle=True)
visit_root = visit_file.split('_visits')[0]
visit_filters = np.array([v['product'].split('-')[-1] for v in visits])
groups = {}
for filt in np.unique(visit_filters):
groups[filt] = {}
groups[filt]['filter'] = filt
groups[filt]['files'] = []
groups[filt]['footprints'] = []
groups[filt]['awspath'] = []
ix = np.where(visit_filters == filt)[0]
for i in ix:
groups[filt]['files'].extend(visits[i]['files'])
groups[filt]['footprints'].extend(visits[i]['footprints'])
Nf = len(groups[filt]['files'])
print('{0:>6}: {1:>3} exposures'.format(filt, Nf))
if aws_prep_dir is not None:
groups[filt]['awspath'] = [s3_full_path
for file in range(Nf)]
np.save('{0}_filter_groups.npy'.format(visit_root), [groups])
else:
print('Use groups file: {0}'.format(groups_files[0]))
groups = np.load(groups_files[0], allow_pickle=True)[0]
#filters = ['f160w','f814w', 'f110w', 'f098m', 'f140w','f125w','f105w','f606w', 'f475w']
filt_dict = FilterDict()
filt_dict.meta['label'] = label
filt_dict.meta['ra'] = ra
filt_dict.meta['dec'] = dec
filt_dict.meta['size'] = size
filt_dict.meta['master'] = master
filt_dict.meta['parent'] = parent
if filters is None:
filters = list(groups.keys())
has_filts = []
lower_filters = [f.lower() for f in filters]
for filt in lower_filters:
if filt not in groups:
continue
visits = [copy.deepcopy(groups[filt])]
#visits[0]['reference'] = 'CarlosGG/ak03_j1000p0228/Prep/ak03_j1000p0228-f160w_drz_sci.fits'
visits[0]['product'] = label+'-'+filt
if wcs is None:
hdu = utils.make_wcsheader(ra=ra, dec=dec, size=size, pixscale=pixscale, get_hdu=True, theta=theta)
h = hdu.header
else:
h = utils.to_header(wcs)
if (filt[:2] in ['f0', 'f1', 'g1']) | (not half_optical_pixscale):
#data = hdu.data
pass
else:
for k in ['NAXIS1', 'NAXIS2', 'CRPIX1', 'CRPIX2']:
h[k] *= 2
h['CRPIX1'] -= 0.5
h['CRPIX2'] -= 0.5
for k in ['CD1_1', 'CD1_2', 'CD2_1', 'CD2_2']:
if k in h:
h[k] /= 2
#data = np.zeros((h['NAXIS2'], h['NAXIS1']), dtype=np.int16)
#pyfits.PrimaryHDU(header=h, data=data).writeto('ref.fits', overwrite=True, output_verify='fix')
#visits[0]['reference'] = 'ref.fits'
print('\n\n###\nMake filter: {0}'.format(filt))
if (filt.upper() in ['F105W', 'F110W', 'F125W', 'F140W', 'F160W']) & include_ir_psf:
clean_i = False
else:
clean_i = remove
status = utils.drizzle_from_visit(visits[0], h, pixfrac=pixfrac, kernel=kernel, clean=clean_i, include_saturated=include_saturated, skip=skip, dryrun=dryrun)
if dryrun:
filt_dict[filt] = status
continue
elif status is not None:
sci, wht, outh, filt_dict[filt] = status
if subtract_median:
#med = np.median(sci[sci != 0])
try:
un_data = np.unique(sci[(sci != 0) & np.isfinite(sci)])
med = utils.mode_statistic(un_data)
except:
med = 0.
if not np.isfinite(med):
med = 0.
print('\n\nMedian {0} = {1:.3f}\n\n'.format(filt, med))
outh['IMGMED'] = (med, 'Median subtracted from the image')
else:
med = 0.
outh['IMGMED'] = (0., 'Median subtracted from the image')
pyfits.writeto('{0}-{1}_drz_sci.fits'.format(label, filt),
data=sci, header=outh, overwrite=True,
output_verify='fix')
pyfits.writeto('{0}-{1}_drz_wht.fits'.format(label, filt),
data=wht, header=outh, overwrite=True,
output_verify='fix')
has_filts.append(filt)
if (filt.upper() in ['F105W', 'F110W', 'F125W', 'F140W', 'F160W']) & include_ir_psf:
from grizli.galfit.psf import DrizzlePSF
hdu = pyfits.open('{0}-{1}_drz_sci.fits'.format(label, filt),
mode='update')
flt_files = [] # visits[0]['files']
for i in range(1, 10000):
key = 'FLT{0:05d}'.format(i)
if key not in hdu[0].header:
break
flt_files.append(hdu[0].header[key])
try:
dp = DrizzlePSF(flt_files=flt_files, driz_hdu=hdu[0])
psf = dp.get_psf(ra=dp.driz_wcs.wcs.crval[0],
dec=dp.driz_wcs.wcs.crval[1],
filter=filt.upper(),
pixfrac=dp.driz_header['PIXFRAC'],
kernel=dp.driz_header['KERNEL'],
wcs_slice=dp.driz_wcs, get_extended=True,
verbose=False, get_weight=False)
psf[1].header['EXTNAME'] = 'PSF'
#psf[1].header['EXTVER'] = filt
hdu.append(psf[1])
hdu.flush()
except:
pass
if remove:
os.system('rm *_fl*fits')
# Dry run, just return dictionary of the found exposure files
if dryrun:
return filt_dict
# Nothing found
if len(has_filts) == 0:
return []
if combine_similar_filters:
combine_filters(label=label)
if rgb_params:
#auto_script.field_rgb(root=label, HOME_PATH=None, filters=has_filts, **rgb_params)
show_all_thumbnails(label=label, thumb_height=thumb_height, scale_ab=scale_ab, close=True, rgb_params=rgb_params, filters=show_filters)
if (single_output != 0):
# Concatenate into a single FITS file
files = glob.glob('{0}-f*_dr[cz]_sci.fits'.format(label))
files.sort()
if combine_similar_filters:
comb_files = glob.glob('{0}-[a-eg-z]*_dr[cz]_sci.fits'.format(label))
comb_files.sort()
files += comb_files
hdul = None
for file in files:
hdu_i = pyfits.open(file)
hdu_i[0].header['EXTNAME'] = 'SCI'
if 'NCOMBINE' in hdu_i[0].header:
if hdu_i[0].header['NCOMBINE'] <= single_output:
continue
filt_i = file.split('-')[-1].split('_dr')[0]
else:
filt_i = utils.get_hst_filter(hdu_i[0].header)
for h in hdu_i:
h.header['EXTVER'] = filt_i
if hdul is None:
hdul = pyfits.HDUList([h])
else:
hdul.append(h)
print('Add to {0}.thumb.fits: {1}'.format(label, file))
# Weight
hdu_i = pyfits.open(file.replace('_sci', '_wht'))
hdu_i[0].header['EXTNAME'] = 'WHT'
for h in hdu_i:
h.header['EXTVER'] = filt_i
if hdul is None:
hdul = pyfits.HDUList([h])
else:
hdul.append(h)
hdul.writeto('{0}.thumb.fits'.format(label), overwrite=True,
output_verify='fix')
for file in files:
for f in [file, file.replace('_sci', '_wht')]:
if os.path.exists(f):
print('Remove {0}'.format(f))
os.remove(f)
# Segmentation figure
thumb_file = '{0}.thumb.fits'.format(label)
if (make_segmentation_figure) & (os.path.exists(thumb_file)) & (aws_prep_dir is not None):
print('Make segmentation figure')
# Fetch segmentation image and catalog
s3_prep_path = 'Pipeline/{0}/Prep/'.format(prep_root)
s3_full_path = '{0}/{1}'.format(prep_bucket, s3_prep_path)
s3_file = '{0}_visits.npy'.format(prep_root)
has_seg_files = True
seg_files = ['{0}-ir_seg.fits.gz'.format(prep_root),
'{0}_phot.fits'.format(prep_root)]
for s3_file in seg_files:
if not os.path.exists(s3_file):
remote_file = os.path.join(s3_prep_path, s3_file)
try:
print('Fetch {0}'.format(remote_file))
prep_bkt.download_file(remote_file, s3_file,
ExtraArgs={"RequestPayer": "requester"})
except:
has_seg_files = False
print('Make segmentation figure failed: {0}'.format(remote_file))
break
if has_seg_files:
s3_cat = utils.read_catalog(seg_files[1])
segmentation_figure(label, s3_cat, seg_files[0])
if aws_bucket:
#aws_bucket = 's3://grizli-cosmos/CutoutProducts/'
#aws_bucket = 's3://grizli/CutoutProducts/'
s3 = boto3.resource('s3')
s3_client = boto3.client('s3')
bkt = s3.Bucket(aws_bucket.split("/")[2])
aws_path = '/'.join(aws_bucket.split("/")[3:])
if sync_fits:
files = glob.glob('{0}*'.format(label))
else:
files = glob.glob('{0}*png'.format(label))
for file in files:
print('{0} -> {1}'.format(file, aws_bucket))
bkt.upload_file(file, '{0}/{1}'.format(aws_path, file).replace('//', '/'), ExtraArgs={'ACL': 'public-read'})
#os.system('aws s3 sync --exclude "*" --include "{0}*" ./ {1} --acl public-read'.format(label, aws_bucket))
#os.system("""echo "<pre>" > index.html; aws s3 ls AWSBUCKETX --human-readable | sort -k 1 -k 2 | grep -v index | awk '{printf("%s %s",$1, $2); printf(" %6s %s ", $3, $4); print "<a href="$5">"$5"</a>"}'>> index.html; aws s3 cp index.html AWSBUCKETX --acl public-read""".replace('AWSBUCKETX', aws_bucket))
return has_filts
class Galfitter(object):
def __init__(self, root='sdssj1723+3411', filter='f140w', galfit_exec='galfit', catfile=None, segfile=None):
self.root = root
self.galfit_exec = galfit_exec
self.filter = filter
data = self.get_data(filter=filter, catfile=catfile, segfile=segfile)
self.sci, self.wht, self.seg, self.cat, self.wcs = data
self.flt_files = self.get_flt_files(sci_hdu=self.sci)
self.DPSF = DrizzlePSF(flt_files=self.flt_files, info=None, driz_image=self.sci.filename())
def get_data(self, filter='f140w', catfile=None, segfile=None):
import glob
sci_file = glob.glob('{0}-{1}_dr?_sci.fits'.format(self.root, filter))
sci = pyfits.open(sci_file[0])
wht = pyfits.open(sci_file[0].replace('sci','wht'))
if segfile is None:
segfile = sci_file[0].split('_dr')[0]+'_seg.fits'
seg = pyfits.open(segfile)
if catfile is None:
catfile = '{0}-{1}.cat.fits'.format(self.root, filter)
cat = utils.GTable.gread(catfile)
wcs = pywcs.WCS(sci[0].header, relax=True)
return sci, wht, seg, cat, wcs
def get_flt_files(self, sci_hdu=None):
flt_files = []
h = self.sci[0].header
for i in range(h['NDRIZIM']):
file = h['D{0:03d}DATA'.format(i+1)].split('[sci')[0]
if file not in flt_files:
flt_files.append(file)
return flt_files
@staticmethod
def fit_arrays(sci, wht, seg, psf, id=None, platescale=0.06, exptime=0, path='/tmp/', galfit_exec='galfit', gaussian_guess=False, components=[GalfitSersic()], recenter=True, psf_sample=1):
rms = 1/np.sqrt(wht)#*exptime
if exptime > 0:
rms = np.sqrt((rms*exptime)**2+sci*exptime*(sci > 0))/exptime
rms[wht == 0] = 1e30
if id is not None:
mask = ((seg > 0) & (seg != id)) | (wht == 0)
else:
mask = wht == 0
sh = sci.shape[0]
fp = open(path+'galfit.feedme','w')
fp.write(GALFIT_IMAGES.format(input=path+'gf_sci.fits', output=path+'gf_out.fits', sigma=path+'gf_rms.fits', psf=path+'gf_psf.fits', mask=path+'gf_mask.fits', xmax=sh, ymax=sh, sh=sh, ps=platescale, psf_sample=psf_sample))
if gaussian_guess:
fit, q, theta = fit_gauss(sci)
from astropy.coordinates import Angle
import astropy.units as u
for comp in components:
if recenter:
comp.set(pos=[sh/2., sh/2.])
if gaussian_guess:
comp.set(q=q, pa=Angle.wrap_at(theta*u.rad, 360*u.deg).to(u.deg).value)
fp.write(str(comp))
fp.close()
pyfits.writeto(path+'gf_sci.fits', data=sci, overwrite=True)
pyfits.writeto(path+'gf_rms.fits', data=rms, overwrite=True)
pyfits.writeto(path+'gf_mask.fits', data=mask*1, overwrite=True)
pyfits.writeto(path+'gf_psf.fits', data=psf, overwrite=True)
for ext in ['out', 'model']:
if os.path.exists(path+'gf_{0}.fits'.format(ext)):
os.remove(path+'gf_{0}.fits'.format(ext))
os.system('{0} {1}/galfit.feedme'.format(galfit_exec, path))
def fit_object(self, id=449, radec=(None, None), size=40, components=[GalfitSersic()], recenter=True, get_mosaic=True, gaussian_guess=False, get_extended=True):
"""
Fit an object
"""
if id is not None:
rd = self.cat['X_WORLD', 'Y_WORLD'][self.cat['NUMBER'] == id][0]
radec = tuple(rd)
xy = self.wcs.all_world2pix([radec[0]], [radec[1]], 0)
xy = np.array(xy).flatten()
xp = np.cast[int](np.round(xy))
slx, sly, wcs_slice = self.DPSF.get_driz_cutout(ra=radec[0], dec=radec[1], get_cutout=False, size=size)
#drz_cutout = self.get_driz_cutout(ra=ra, dec=dec, get_cutout=True)
h = self.sci[0].header
psf = self.DPSF.get_psf(ra=radec[0], dec=radec[1], filter=self.filter.upper(), wcs_slice=wcs_slice, pixfrac=h['D001PIXF'], kernel=h['D001KERN'], get_extended=get_extended)
exptime = h['EXPTIME']
sci = self.sci[0].data[sly, slx]#*exptime
wht = self.wht[0].data[sly, slx]
rms = 1/np.sqrt(wht)#*exptime
rms = np.sqrt((rms*exptime)**2+sci*exptime*(sci > 0))/exptime
rms[wht == 0] = 1e30
seg = self.seg[0].data[sly, slx]
if id is not None:
mask = ((seg > 0) & (seg != id)) | (wht == 0)
else:
mask = wht == 0
sh = sci.shape[0]
path = '/tmp/'
psf_file = '{0}-{1}_psf_{2:05d}.fits'.format(self.root, self.filter, id)
fp = open(path+'galfit.feedme','w')
fp.write(GALFIT_IMAGES.format(input=path+'gf_sci.fits', output=path+'gf_out.fits', sigma=path+'gf_rms.fits', psf=psf_file, mask=path+'gf_mask.fits', xmax=sh, ymax=sh, sh=sh, ps=self.DPSF.driz_pscale, psf_sample=1))
if gaussian_guess:
fit, q, theta = fit_gauss(sci)
from astropy.coordinates import Angle
import astropy.units as u
for comp in components:
if recenter:
comp.set(pos=[sh/2., sh/2.])
if gaussian_guess:
comp.set(q=q, pa=Angle.wrap_at(theta*u.rad, 360*u.deg).to(u.deg).value)
fp.write(str(comp))
fp.close()
pyfits.writeto(path+'gf_sci.fits', data=sci, overwrite=True)
pyfits.writeto(path+'gf_rms.fits', data=rms, overwrite=True)
pyfits.writeto(path+'gf_mask.fits', data=mask*1, overwrite=True)
#pyfits.writeto(path+'gf_psf.fits', data=psf[1].data, overwrite=True)
pyfits.writeto(psf_file, data=psf[1].data, overwrite=True)
for ext in ['out', 'model']:
if os.path.exists(path+'gf_{0}.fits'.format(ext)):
os.remove(path+'gf_{0}.fits'.format(ext))
os.system('{0} {1}/galfit.feedme'.format(self.galfit_exec, path))
#out = pyfits.open('/tmp/gf_out.fits')
# Get in DRZ frame
gf_file = glob.glob('galfit.[0-9]*')[-1]
lines = open(gf_file).readlines()
for il, line in enumerate(lines):
if line.startswith('A)'):
lines[il] = 'A) {0} # Input data image (FITS file)\n'.format(self.sci.filename())
if line.startswith('B)'):
lines[il] = 'B) {0}-{1}_galfit_{2:05d}.fits # Output data image block\n'.format(self.root, self.filter, id)
if line.startswith('P) 0'):
lines[il] = "P) 1 # Choose: 0=optimize, 1=model, 2=imgblock, 3=subcomps\n"
if line.startswith('H)'):
out_sh = self.sci[0].data.shape
lines[il] = "H) 1 {0} 1 {1} # Image region to fit (xmin xmax ymin ymax)\n".format(out_sh[1], out_sh[0])
if line.startswith(' 1)'):
xy = np.cast[float](line.split()[1:3])
lines[il] = ' 1) {0} {1} 1 1 # Position x, y\n'.format(xy[0]+slx.start, xy[1]+sly.start)
fp = open('galfit.{0}.{1:05d}'.format(self.filter, id),'w')
fp.writelines(lines)
fp.close()
os.system('{0} galfit.{1}.{2:05d}'.format(self.galfit_exec, self.filter, id))
model = pyfits.open('{0}-{1}_galfit_{2:05d}.fits'.format(self.root, self.filter, id), mode='update')
model[0].data /= self.sci[0].header['EXPTIME']
model.flush()
return(lines, model)
model = pyfits.open('/tmp/gf_model.fits')
if False:
full_model = self.sci[0].data*0
full_model += model[0].data
pyfits.writeto('{0}-{1}_galfit.fits'.format(self.root, self.filter), data=full_model, header=self.sci[0].header, overwrite=True)
class Galfitter(object):
def __init__(self,
root='sdssj1723+3411',
filter='f140w',
galfit_exec='galfit'):
self.root = root
self.galfit_exec = galfit_exec
self.filter = filter
data = self.get_data(filter=filter)
self.sci, self.wht, self.seg, self.cat, self.wcs = data
self.flt_files = self.get_flt_files(sci_hdu=self.sci)
self.DPSF = DrizzlePSF(flt_files=self.flt_files,
info=None,
driz_image=self.sci.filename())
def get_data(self, filter='f140w'):
sci = pyfits.open('{0}-{1}_drz_sci.fits'.format(self.root, filter))
wht = pyfits.open('{0}-{1}_drz_wht.fits'.format(self.root, filter))
seg = pyfits.open('{0}-{1}_seg.fits'.format(self.root, filter))
cat = grizli.utils.GTable.gread('{0}-{1}.cat'.format(
self.root, filter))
wcs = pywcs.WCS(sci[0].header, relax=True)
return sci, wht, seg, cat, wcs
def get_flt_files(self, sci_hdu=None):
flt_files = []
h = self.sci[0].header
for i in range(h['NDRIZIM']):
flt_files.append(h['D{0:03d}DATA'.format(i + 1)].split('[sci')[0])
return flt_files
def fit_object(self,
id=449,
radec=(None, None),
size=40,
components=[GalfitSersic()],
recenter=True,
get_mosaic=True,
gaussian_guess=False):
"""
Fit an object
"""
if id is not None:
rd = self.cat['X_WORLD', 'Y_WORLD'][self.cat['NUMBER'] == id][0]
radec = tuple(rd)
xy = self.wcs.all_world2pix([radec[0]], [radec[1]], 0)
xy = np.array(xy).flatten()
xp = np.cast[int](np.round(xy))
slx, sly, wcs_slice = self.DPSF.get_driz_cutout(ra=radec[0],
dec=radec[1],
get_cutout=False,
size=size)
#drz_cutout = self.get_driz_cutout(ra=ra, dec=dec, get_cutout=True)
h = self.sci[0].header
psf = self.DPSF.get_psf(ra=radec[0],
dec=radec[1],
filter=self.filter.upper(),
wcs_slice=wcs_slice,
pixfrac=h['D001PIXF'],
kernel=h['D001KERN'],
get_extended=True)
exptime = h['EXPTIME']
sci = self.sci[0].data[sly, slx] #*exptime
wht = self.wht[0].data[sly, slx]
rms = 1 / np.sqrt(wht) #*exptime
rms = np.sqrt((rms * exptime)**2 + sci * exptime * (sci > 0)) / exptime
rms[wht == 0] = 1e30
seg = self.seg[0].data[sly, slx]
if id is not None:
mask = ((seg > 0) & (seg != id)) | (wht == 0)
else:
mask = wht == 0
sh = sci.shape[0]
path = '/tmp/'
psf_file = '{0}-{1}_psf_{2:05d}.fits'.format(self.root, self.filter,
id)
fp = open(path + 'galfit.feedme', 'w')
fp.write(
GALFIT_IMAGES.format(input=path + 'gf_sci.fits',
output=path + 'gf_out.fits',
sigma=path + 'gf_rms.fits',
psf=psf_file,
mask=path + 'gf_mask.fits',
xmax=sh,
ymax=sh,
sh=sh))
if gaussian_guess:
fit, q, theta = fit_gauss(sci)
from astropy.coordinates import Angle
import astropy.units as u
for comp in components:
if recenter:
comp.set(pos=[sh / 2., sh / 2.])
if gaussian_guess:
comp.set(q=q,
pa=Angle.wrap_at(theta * u.rad,
360 * u.deg).to(u.deg).value)
fp.write(str(comp))
fp.close()
pyfits.writeto(path + 'gf_sci.fits', data=sci, overwrite=True)
pyfits.writeto(path + 'gf_rms.fits', data=rms, overwrite=True)
pyfits.writeto(path + 'gf_mask.fits', data=mask * 1, overwrite=True)
#pyfits.writeto(path+'gf_psf.fits', data=psf[1].data, overwrite=True)
pyfits.writeto(psf_file, data=psf[1].data, overwrite=True)
for ext in ['out', 'model']:
if os.path.exists(path + 'gf_{0}.fits'.format(ext)):
os.remove(path + 'gf_{0}.fits'.format(ext))
os.system('{0} {1}/galfit.feedme'.format(self.galfit_exec, path))
#out = pyfits.open('/tmp/gf_out.fits')
# Get in DRZ frame
gf_file = glob.glob('galfit.[0-9]*')[-1]
lines = open(gf_file).readlines()
for il, line in enumerate(lines):
if line.startswith('A)'):
lines[
il] = 'A) {0} # Input data image (FITS file)\n'.format(
self.sci.filename())
if line.startswith('B)'):
lines[
il] = 'B) {0}-{1}_galfit_{2:05d}.fits # Output data image block\n'.format(
self.root, self.filter, id)
if line.startswith('P) 0'):
lines[
il] = "P) 1 # Choose: 0=optimize, 1=model, 2=imgblock, 3=subcomps\n"
if line.startswith('H)'):
out_sh = self.sci[0].data.shape
lines[
il] = "H) 1 {0} 1 {1} # Image region to fit (xmin xmax ymin ymax)\n".format(
out_sh[1], out_sh[0])
if line.startswith(' 1)'):
xy = np.cast[float](line.split()[1:3])
lines[il] = ' 1) {0} {1} 1 1 # Position x, y\n'.format(
xy[0] + slx.start, xy[1] + sly.start)
fp = open('galfit.{0}.{1:05d}'.format(self.filter, id), 'w')
fp.writelines(lines)
fp.close()
os.system('{0} galfit.{1}.{2:05d}'.format(self.galfit_exec,
self.filter, id))
return (lines)
model = pyfits.open('/tmp/gf_model.fits')
if False:
full_model = self.sci[0].data * 0
full_model += model[0].data
pyfits.writeto('{0}-{1}_galfit.fits'.format(self.root, self.filter),
data=full_model,
header=self.sci[0].header,
overwrite=True)
