-
Notifications
You must be signed in to change notification settings - Fork 0
/
convolved.py
1518 lines (1166 loc) · 43 KB
/
convolved.py
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
311
312
313
314
315
316
317
318
319
320
321
322
323
324
325
326
327
328
329
330
331
332
333
334
335
336
337
338
339
340
341
342
343
344
345
346
347
348
349
350
351
352
353
354
355
356
357
358
359
360
361
362
363
364
365
366
367
368
369
370
371
372
373
374
375
376
377
378
379
380
381
382
383
384
385
386
387
388
389
390
391
392
393
394
395
396
397
398
399
400
401
402
403
404
405
406
407
408
409
410
411
412
413
414
415
416
417
418
419
420
421
422
423
424
425
426
427
428
429
430
431
432
433
434
435
436
437
438
439
440
441
442
443
444
445
446
447
448
449
450
451
452
453
454
455
456
457
458
459
460
461
462
463
464
465
466
467
468
469
470
471
472
473
474
475
476
477
478
479
480
481
482
483
484
485
486
487
488
489
490
491
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
518
519
520
521
522
523
524
525
526
527
528
529
530
531
532
533
534
535
536
537
538
539
540
541
542
543
544
545
546
547
548
549
550
551
552
553
554
555
556
557
558
559
560
561
562
563
564
565
566
567
568
569
570
571
572
573
574
575
576
577
578
579
580
581
582
583
584
585
586
587
588
589
590
591
592
593
594
595
596
597
598
599
600
601
602
603
604
605
606
607
608
609
610
611
612
613
614
615
616
617
618
619
620
621
622
623
624
625
626
627
628
629
630
631
632
633
634
635
636
637
638
639
640
641
642
643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
660
661
662
663
664
665
666
667
668
669
670
671
672
673
674
675
676
677
678
679
680
681
682
683
684
685
686
687
688
689
690
691
692
693
694
695
696
697
698
699
700
701
702
703
704
705
706
707
708
709
710
711
712
713
714
715
716
717
718
719
720
721
722
723
724
725
726
727
728
729
730
731
732
733
734
735
736
737
738
739
740
741
742
743
744
745
746
747
748
749
750
751
752
753
754
755
756
757
758
759
760
761
762
763
764
765
766
767
768
769
770
771
772
773
774
775
776
777
778
779
780
781
782
783
784
785
786
787
788
789
790
791
792
793
794
795
796
797
798
799
800
801
802
803
804
805
806
807
808
809
810
811
812
813
814
815
816
817
818
819
820
821
822
823
824
825
826
827
828
829
830
831
832
833
834
835
836
837
838
839
840
841
842
843
844
845
846
847
848
849
850
851
852
853
854
855
856
857
858
859
860
861
862
863
864
865
866
867
868
869
870
871
872
873
874
875
876
877
878
879
880
881
882
883
884
885
886
887
888
889
890
891
892
893
894
895
896
897
898
899
900
901
902
903
904
905
906
907
908
909
910
911
912
913
914
915
916
917
918
919
920
921
922
923
924
925
926
927
928
929
930
931
932
933
934
935
936
937
938
939
940
941
942
943
944
945
946
947
948
949
950
951
952
953
954
955
956
957
958
959
960
961
962
963
964
965
966
967
968
969
970
971
972
973
974
975
976
977
978
979
980
981
982
983
984
985
986
987
988
989
990
991
992
993
994
995
996
997
998
999
1000
from __future__ import print_function
from pprint import pprint
import numpy
from numpy import sqrt, exp, array, ceil, log2, pi, ogrid, zeros, where
from numpy.fft import fftshift
import images
from sys import stderr
from . import statistics as stat
from . import pixmodel
from . import fconv
from . import analytic
from . import conversions
from .conversions import mom2sigma, cov2sigma
from .noise import add_noise_uw, add_noise_matched, add_noise_admom, get_s2n_matched, get_s2n_uw, get_s2n_admom
from .transform import rebin
import time
import admom
try:
import scipy.signal
from scipy.fftpack import ifftn, fftn
have_scipy=True
except:
have_scipy=False
# sigma ~ fwhm/TURB_SIGMA_FAC
TURB_SIGMA_FAC=1.68
TURB_PADDING=10.0
GAUSS_PADDING=5.0
EXP_PADDING=7.0
DEV_PADDING=15.0
def wlog(*args):
narg = len(args)
for i,arg in enumerate(args):
stderr.write("%s" % arg)
if i < (narg-1):
stderr.write(" ")
stderr.write('\n')
def convolve_gauss(image, sigma, get_psf=False):
"""
Convolve with a round gaussian.
The kernel is generated and applied in fourier space.
Note for more general convolutions, use the ConvolvedImageFFT class.
parameters
----------
image:
A two dimensional image.
sigma:
The sigma of the gaussian kernel.
get_psf:
If True, return an image of the psf as well.
(im, psf)
Dims should be even to get a psf that is centered
"""
dims = array(image.shape)
if dims[0] != dims[1]:
raise ValueError("only square images for now")
# padding for PSF
kdims = dims.copy()
kdims += 2.*4.*sigma
# Always use 2**n-sized FFT
kdims = 2**ceil(log2(kdims))
kcen = kdims/2.
imfft = fftn(image,kdims)
krow,kcol=ogrid[0:kdims[0], 0:kdims[1]]
kr = array(krow - kcen[0], dtype='f8')
kc = array(kcol - kcen[1], dtype='f8')
k2 = kr**2 + kc**2
ksigma = 1.0/sigma
# get into fft units
ksigma *= kdims[0]/(2.*pi)
ksigma2 = ksigma**2
gk = exp(-0.5*k2/ksigma2)
gk = fftshift(gk)
ckim = gk*imfft
cim = ifftn(ckim)[0:dims[0], 0:dims[1]]
cim = cim.real
if get_psf:
psf = ifftn(gk)
psf = fftshift(psf)
psf = sqrt(psf.real**2 + psf.imag**2)
psf = pixmodel._centered(psf, dims)
return cim, psf
else:
return cim
def convolve_turb(image, fwhm, get_psf=False):
"""
Convolve the input image with a turbulent psf
parameters
----------
image:
A numpy array
fwhm:
The FWHM of the turbulent psf.
get_psf:
If True, return a tuple (im,psf)
The images dimensions should be square, and even so the psf is
centered.
"""
dims = array(image.shape)
if dims[0] != dims[1]:
raise ValueError("only square images for now")
# add padding for PSF in real space
# sigma is approximate
kdims=dims.copy()
kdims += 2*4*fwhm/TURB_SIGMA_FAC
# Always use 2**n-sized FFT
kdims = 2**ceil(log2(kdims))
kcen = kdims/2.
imfft = fftn(image,kdims)
k0 = 2.92/fwhm
# in fft units
k0 *= kdims[0]/(2*pi)
otf = pixmodel.ogrid_turb_kimage(kdims, kcen, k0)
otf = fftshift(otf)
ckim = otf*imfft
cim = ifftn(ckim)[0:dims[0], 0:dims[1]]
cim = cim.real
if get_psf:
psf = ifftn(otf)
psf = fftshift(psf)
psf = sqrt(psf.real**2 + psf.imag**2)
psf = pixmodel._centered(psf, dims)
return cim, psf
else:
return cim
class ConvolverBase(dict):
def __init__(self, objpars, psfpars, **keys):
"""
Abstract base class
"""
self.objpars=objpars
self.psfpars=psfpars
self.center_offset=keys.get('center_offset',None)
if self.objpars['model'] not in ['gauss','exp','dev','gexp','gdev']:
raise ValueError("only support gauss/exp/dev objects")
if self.psfpars['model'] not in ['gauss','dgauss','turb','gturb']:
raise ValueError("only support gauss/dgauss/turb psf")
if 'cov' in self.objpars:
self.objpars['cov'] = array(self.objpars['cov'],dtype='f8')
if 'cov' in self.psfpars:
self.psfpars['cov'] = array(self.psfpars['cov'],dtype='f8')
# we want to try to let the expansion factor do the trick
# even for dev, we probably don't need a full nsub=16 here
defsub=1
self['image_nsub'] = keys.get('image_nsub', defsub)
self['expand_fac_min'] = keys.get('expand_fac_min', 1)
self['verbose'] = keys.get('verbose',False)
if self['verbose']:
wlog("image_nsub:",self['image_nsub'])
# for calculations we will demand sigma > minres pixels
# then sample back
if self.objpars['model'] == 'dev':
#minres_def = 24
minres_def = 20
else:
minres_def = 12
self['minres'] = keys.get('minres',minres_def)
self.set_default_padding(**keys)
self.image0=None
self.image=None
self.psf=None
def set_default_padding(self, **keys):
if 'psffac' in keys:
self['psffac'] = keys['psffac']
if 'objfac' in keys:
self['objfac'] = keys['objfac']
else:
# Hint for how large to make the base image
if self.objpars['model'] == 'exp':
self['objfac']=EXP_PADDING
elif self.objpars['model'] == 'dev':
self['objfac']=DEV_PADDING
else:
self['objfac']=GAUSS_PADDING
def make_images(self):
"""
Make an image convolved with the psf.
"""
raise RuntimeError("over-ride this")
def set_cov_and_etrue(self):
cov = self.objpars['cov']
T=(cov[2]+cov[0])
self['covtrue'] = self.objpars['cov']
self['e1true'] = (cov[2]-cov[0])/T
self['e2true'] = 2*cov[1]/T
self['etrue'] = sqrt( self['e1true']**2 + self['e2true']**2 )
def get_image0(self, verify=False, expand=False):
"""
Create the pre-psf model
run these first
self.set_cov_and_etrue()
self.set_dims()
"""
pars = self.objpars
objmodel = pars['model']
if expand:
cen = self['ecen']
dims = self['edims']
cov = pars['ecov']
else:
cen = self['cen']
dims = self['dims']
cov = pars['cov']
image0 = pixmodel.model_image(objmodel,dims,cen,cov,
nsub=self['image_nsub'])
if verify:
self.verify_image(image0, cov)
return image0
def add_image0_stats(self):
"""
mom = stat.fmom(self.image0)
cov_meas = mom['cov']
cen_meas = mom['cen']
res = admom.admom(self.image0, cen_meas[0],cen_meas[1],
guess=(cov_meas[0]+cov_meas[1])/2 )
cov_meas_admom = array([res['Irr'],res['Irc'],res['Icc']])
"""
pars = self.objpars
mom = stat.fmom(self.image0)
cov_uw = mom['cov']
cen_uw = mom['cen']
res = admom.admom(self.image0, cen_uw[0],cen_uw[1],
guess=(cov_uw[0]+cov_uw[2])/2)
cov_admom = array([res['Irr'],res['Irc'],res['Icc']])
cen_admom = array([res['wrow'], res['wcol']])
pars['cov_uw'] = cov_uw
pars['cen_uw'] = cen_uw
pars['cov_admom'] = cov_admom
pars['cen_admom'] = cen_admom
self['cov_image0_uw'] = cov_uw
self['cen_image0_uw'] = cen_uw
e1_uw = (cov_uw[2]-cov_uw[0])/(cov_uw[2]+cov_uw[0])
e2_uw = 2*cov_uw[1]/(cov_uw[2]+cov_uw[0])
self['e1_image0_uw'] = e1_uw
self['e2_image0_uw'] = e2_uw
self['e_image0_uw'] = sqrt(e1_uw**2 + e2_uw**2)
def add_psf_stats(self):
mom = stat.fmom(self.psf)
cov_uw = mom['cov']
cen_uw = mom['cen']
res = admom.admom(self.psf,cen_uw[0],cen_uw[1],
guess=(cov_uw[0]+cov_uw[2])/2)
cov_admom = array([res['Irr'],res['Irc'],res['Icc']])
cen_admom = array([res['wrow'], res['wcol']])
self.psfpars['cov_uw'] = cov_uw
self.psfpars['cen_uw'] = cen_uw
self.psfpars['cov_admom'] = cov_admom
self.psfpars['cen_admom'] = cen_admom
self['cov_psf_uw'] = cov_uw
self['cen_psf_uw'] = cen_uw
self['cov_psf_admom'] = cov_admom
self['cen_psf_admom'] = cen_admom
self['a4_psf'] = res['a4']
def add_image_stats(self):
mom_uw = stat.fmom(self.image)
cov_uw = mom_uw['cov']
cen_uw = mom_uw['cen']
res = admom.admom(self.image, cen_uw[0], cen_uw[1],
guess=(cov_uw[0]+cov_uw[2])/2)
if res['whyflag'] != 0:
raise ValueError("admom failure: '%s'" % res['whystr'])
cov_admom = array([res['Irr'],res['Irc'],res['Icc']])
cen_admom = array([res['wrow'], res['wcol']])
self['cov_uw'] = cov_uw
self['cen_uw'] = cen_uw
self['cov_admom'] = cov_admom
self['cen_admom'] = cen_admom
self['a4'] = res['a4']
self['e1_admom'] = res['e1']
self['e2_admom'] = res['e2']
def verify_image(self, image, cov, eps=2.e-3):
'''
Ensure that the *unweighted* moments are equal to input moments
This is only useful for expanded images since unweighted moments don't
include sub-pixel effects
'''
mom = stat.fmom(image)
mcov = mom['cov']
rowrel = abs(mcov[0]/cov[0]-1)
colrel = abs(mcov[2]/cov[2]-1)
pdiff = max(rowrel,colrel)
if pdiff > eps:
raise ValueError("row pdiff %f not within "
"tolerance %f" % (pdiff,eps))
T = mcov[2] + mcov[0]
e1 = (mcov[2]-mcov[1])/T
e2 = 2*mcov[1]/T
e = sqrt(e1**2 + e2**2)
Ttrue = cov[2] + cov[0]
e1true = (cov[2]-cov[1])/T
e2true = 2*cov[1]/T
etrue = sqrt(e1true**2 + e2true**2)
erel = abs(e/etrue-1)
if erel > eps:
raise ValueError("moments pdiff %f not within "
"tolerance %f" % (erel,eps))
def write_fits(self, fits_file, extra_keys=None):
"""
Write the images and metadata to a fits file
The images are in separate extensions 'image','psf','image0' and the
metadata are in a binary table 'table'
parameters
----------
fits_file: string
Name of the file to write
ci: child of ConvolverBase
"""
import fitsio
dt=[]
for k,v in self.iteritems():
if isinstance(v,int) or isinstance(v,long):
dt.append( (k, 'i8') )
elif isinstance(v,float):
dt.append( (k, 'f8') )
elif isinstance(v,numpy.ndarray):
this_t = v.dtype.descr[0][1]
this_n = v.size
if this_n > 1:
this_dt = (k,this_t,this_n)
else:
this_dt = (k,this_t)
dt.append(this_dt)
else:
raise ValueError("unsupported type: %s" % type(v))
table = numpy.zeros(1, dtype=dt)
for k,v in self.iteritems():
table[k][0] = v
with fitsio.FITS(fits_file,mode='rw',clobber=True) as fitsobj:
h={}
# note not all items will be written, only basic types,
# so this is not for feeding to the sim code. The full
# metadata are in the table
for k,v in self.iteritems():
h[k] = v
if extra_keys:
for k,v in extra_keys.iteritems():
h[k] = v
fitsobj.write(self.image, header=h, extname='image')
fitsobj.write(self.psf, extname='psf')
fitsobj.write(self.image0, extname='image0')
fitsobj.write(table, extname='table')
class NoisyConvolvedImage(dict):
def __init__(self, ci, s2n, s2n_psf, s2n_method='matched',
fluxfrac=None):
self.ci = ci
self.image = ci.image
self.image0 = ci.image0
self.psf = ci.psf
if hasattr(ci,'objpars'):
self.objpars=ci.objpars
if hasattr(ci,'psfpars'):
self.psfpars=ci.psfpars
self.s2n_method=s2n_method
self.fluxfrac=fluxfrac
self['verbose'] = ci.get('verbose',False)
for k,v in ci.iteritems():
self[k] = v
if s2n > 0:
self.image_nonoise = ci.image
(self.image,
self['skysig'],
self['s2n_uw'],
self['s2n_matched'],
self['s2n_admom']) = self.add_noise(ci.image,s2n)
if s2n_psf > 0:
self.psf_nonoise = ci.psf
(self.psf,
self['skysig_psf'],
self['s2n_uw_psf'],
self['s2n_matched_psf'],
self['s2n_admom_psf']) = self.add_noise(ci.psf,s2n_psf)
def add_noise(self, image, s2n):
if self.s2n_method == 'matched':
if self.fluxfrac is not None and self['verbose']:
wlog("implementing fluxfrac:",self.fluxfrac)
noisy_image, skysig = add_noise_matched(image, s2n,
fluxfrac=self.fluxfrac,
cen=self.ci['cen'],)
s2n_uw = get_s2n_uw(image, skysig)
s2n_matched = s2n
s2n_admom = get_s2n_admom(image, self.ci['cen_admom'], skysig)
elif self.s2n_method=='uw':
if self.fluxfrac is not None:
raise ValueError("fluxfrac not implemented for uw yet")
noisy_image, skysig = add_noise_uw(image, s2n)
s2n_matched = get_s2n_matched(image, skysig)
s2n_uw = s2n
s2n_admom = get_s2n_admom(image, self.ci['cen_admom'], skysig)
elif self.s2n_method=='admom':
noisy_image, skysig = add_noise_admom(image, s2n)
s2n_admom=s2n
s2n_matched = get_s2n_matched(image, skysig)
s2n_uw = get_s2n_uw(image, skysig)
else:
raise ValueError("bad s2n_method: '%s'" % self.s2n_method)
return noisy_image, skysig, s2n_uw, s2n_matched, s2n_admom
class TrimmedConvolvedImage(ConvolverBase):
def __init__(self, ci, fluxfrac=0.999937):
"""
"3-sigma" corresponds to 0.9973
"4-sigma" corresponds to 0.999937 of the flux
"""
for k,v in ci.iteritems():
self[k] = v
self.ci = ci
#self.objpars=ci.objpars
#self.psfpars=ci.psfpars
self.objpars={}
self.psfpars={}
self.fluxfrac=fluxfrac
self.trim()
self.add_image0_stats()
self.add_psf_stats()
self.add_image_stats()
self['cen'] = self['cen_uw']
def trim(self):
im = self.ci.image
row,col=ogrid[0:im.shape[0],
0:im.shape[1]]
rm = array(row - self.ci['cen'][0], dtype='f8')
cm = array(col - self.ci['cen'][1], dtype='f8')
radm = sqrt(rm**2 + cm**2)
radii = numpy.arange(1,im.shape[0]/2)
cnts=numpy.zeros(radii.size)
for ir,r in enumerate(radii):
w=where(radm <= r)
if w[0].size > 0:
cnts[ir] = im[w].sum()
cnts /= cnts.max()
w,=where(cnts > self.fluxfrac)
if w.size > 0:
rad = radii[w[0]]
rmin = self.ci['cen'][0]-rad
rmax = self.ci['cen'][0]+rad
cmin = self.ci['cen'][1]-rad
cmax = self.ci['cen'][1]+rad
if rmin < 0:
rmin=0
if rmax > (im.shape[0]-1):
rmax = (im.shape[0]-1)
if cmin < 0:
cmin=0
if cmax > (im.shape[1]-1):
cmax = (im.shape[1]-1)
self.image = self.ci.image[rmin:rmax, cmin:cmax]
self.image0 = self.ci.image0[rmin:rmax, cmin:cmax]
self.psf = self.ci.psf[rmin:rmax, cmin:cmax]
else:
raise ValueError("no radii found, that might be a bug!")
self.image = self.ci.image[rmin:rmax, cmin:cmax]
self.image0 = self.ci.image0[rmin:rmax, cmin:cmax]
self.psf = self.ci.psf[rmin:rmax, cmin:cmax]
class ConvolverGaussFFT(ConvolverBase):
"""
Convolve models with a gaussian or double gaussian psf
"""
def __init__(self, objpars, psfpars, **keys):
"""
Gaussian fft with some model
"""
super(ConvolverGaussFFT,self).__init__(objpars,psfpars,**keys)
if 'psffac' not in self:
self['psffac'] = GAUSS_PADDING
# inherited
self.set_cov_and_etrue()
# these implemented in this class
self.set_dims_and_expansion()
self.make_images()
# these inherited
self.add_image0_stats()
self.add_psf_stats()
self.add_image_stats()
def set_dims_and_expansion(self):
"""
All images are created in reall space, so want odd
"""
psffac = self['psffac']
objfac = self['objfac']
obj_cov = self.objpars['cov']
if self.psfpars['model'] == 'gauss':
psf_cov=self.psfpars['cov']
elif self.psfpars['model'] == 'dgauss':
psf_cov1 = self.psfpars['cov1']
psf_cov2 = self.psfpars['cov2']
psf_cov = zeros(3)
psf_cov[0] = max(psf_cov1[0], psf_cov2[0])
psf_cov[2] = max(psf_cov1[2], psf_cov2[2])
else:
raise ValueError("model should be gauss or dgauss")
# assume ellip=0.8. This will equalize the image
# sizes for different ellipticities
sigma_psf = cov2sigma(psf_cov,maxe=0.8)
sigma_obj = cov2sigma(obj_cov,maxe=0.8)
imsize = 2*sqrt( psffac**2*sigma_psf**2 + objfac**2*sigma_obj**2)
dims = array([imsize]*2,dtype='i8')
self['dims'] = dims
if (dims[0] % 2) != 0:
dims += 1
self['cen'] = (dims-1.)/2.
if self.center_offset is not None:
self['cen'] += self.center_offset
#
# do we need to expand before convolving?
#
sigma_obj_min = sqrt(min(obj_cov[0],obj_cov[2]))
sigma_min = min(sigma_psf,sigma_obj_min)
fac = 1
if sigma_min < self['minres']:
# find the odd integer expansion that will get sigma > minres
fac = int(self['minres']/sigma_min)
fac_min = self['expand_fac_min']
if fac < fac_min:
fac=fac_min
if (fac % 2) == 0:
fac += 1
self['expand_fac'] = fac
if fac > 1:
self['edims'] = fac*self['dims']
self['ecen'] = (self['edims']-1.)/2.
self.objpars['ecov'] = self.objpars['cov']*fac**2
else:
self['edims'] = self['dims']
self['ecen'] = self['cen']
self.objpars['ecov'] = self.objpars['cov']
def make_images(self):
"""
Make an image in real space, go to fourier space and multiply by
the psf, then fft back.
If we are expanding, we create an expanded pre-psf image and convolve
it. The convolved image and psf are rebinned back.
"""
nsub = self['image_nsub']
if self['expand_fac'] < 1:
raise ValueError("expected expansion >= 1")
fac = self['expand_fac']
if fac == 1:
dims = self['dims']
cen = self['cen']
expand=False
else:
expand=True
dims = self['edims']
cen = self['ecen']
stderr.write("image_nsub(again): %d expand_fac: %d\n" % (nsub,fac))
verify=False
image0 = self.get_image0(expand=expand,verify=verify)
if self.psfpars['model'] == 'dgauss':
b=self.psfpars['cenrat']
psf_cov1=self.psfpars['cov1']*fac**2
psf_cov2=self.psfpars['cov2']*fac**2
psf1 = pixmodel.model_image('gauss', dims, cen,
psf_cov1,nsub=nsub)
psf2 = pixmodel.model_image('gauss', dims, cen,
psf_cov2,nsub=nsub)
eim1 = scipy.signal.fftconvolve(image0, psf1, mode='same')
eim2 = scipy.signal.fftconvolve(image0, psf2, mode='same')
image = (eim1 + b*eim2)/(1.+b)
psf = (psf1 + b*psf2)/(1.+b)
else:
psf_cov=self.psfpars['cov']*fac**2
psf = pixmodel.model_image('gauss', dims, cen,
psf_cov,nsub=nsub)
image = scipy.signal.fftconvolve(image0, psf, mode='same')
if fac > 1:
image0 = rebin(image0, fac)
image = rebin(image, fac)
psf = rebin(psf, fac)
self.image0 = image0
self.image = image
self.psf = psf
class ConvolverAllGauss(ConvolverBase):
"""
Convolve gauss models with a gaussian or double gaussian psf
"""
def __init__(self, objpars, psfpars, **keys):
"""
all gaussians all the time
"""
super(ConvolverAllGauss,self).__init__(objpars,psfpars,**keys)
if 'psffac' not in self:
self['psffac'] = GAUSS_PADDING
# these inherited
self.set_cov_and_etrue()
# these implemented in this class
self.set_dims()
self.make_images()
# these inherited
self.add_image0_stats()
self.add_psf_stats()
self.add_image_stats()
def set_dims(self):
"""
Simple for analytic convolutions
"""
fac = self['psffac']
obj_cov = self.objpars['cov']
if self.psfpars['model'] == 'gauss':
psf_cov=self.psfpars['cov']
elif self.psfpars['model'] == 'dgauss':
psf_cov1 = self.psfpars['cov1']
psf_cov2 = self.psfpars['cov2']
psf_cov = zeros(3)
psf_cov[0] = max(psf_cov1[0], psf_cov2[0])
psf_cov[2] = max(psf_cov1[2], psf_cov2[2])
else:
raise ValueError("model should be gauss or dgauss")
cov = obj_cov + psf_cov
sigma = cov2sigma(cov,maxe=0.8)
imsize = fac*2*sigma
dims = array([imsize]*2,dtype='i8')
if (dims[0] % 2) == 0:
dims += 1
#cen=(dims-1)/2
cen=(dims-1.)/2.
#cen[0] = cen[0] + 0.223423
#cen[1] = cen[0] - 0.15234
self['dims'] = dims
self['cen'] = cen
if self.center_offset is not None:
self['cen'] += self.center_offset
def make_images(self):
"""
This is easy! We also force nsub=16 since there is no expansion crap
to deal with
"""
nsub=16
objcov = self.objpars['cov']
self.image0 = pixmodel.model_image('gauss',
self['dims'],
self['cen'],
objcov,nsub=nsub)
if self.psfpars['model'] == 'dgauss':
psf_cov1 = self.psfpars['cov1']
psf_cov2 = self.psfpars['cov2']
cov1 = objcov + psf_cov1
cov2 = objcov + psf_cov2
b = self.psfpars['cenrat']
im1 = pixmodel.model_image('gauss', self['dims'], self['cen'],
cov1,nsub=nsub)
im2 = pixmodel.model_image('gauss', self['dims'], self['cen'],
cov2,nsub=nsub)
self.image = (im1 + b*im2)/(1+b)
psf1 = pixmodel.model_image('gauss', self['dims'], self['cen'],
psf_cov1,nsub=nsub)
psf2 = pixmodel.model_image('gauss', self['dims'], self['cen'],
psf_cov2,nsub=nsub)
self.psf = (psf1 + b*psf2)/(1+b)
else:
psf_cov = self.psfpars['cov']
cov = objcov + psf_cov
self.image = \
pixmodel.model_image('gauss', self['dims'], self['cen'],
cov,nsub=nsub)
self.psf = pixmodel.model_image('gauss', self['dims'], self['cen'],
psf_cov,nsub=nsub)
class ConvolverGMix(ConvolverBase):
"""
Use gaussian mixture models for everything
The center is re-set based on internal algorithms
"""
def __init__(self, obj_gmix, psf_gmix, **keys):
"""
pars are GMix objects
"""
import gmix_image
self.update(keys)
if (not isinstance(obj_gmix,gmix_image.GMix) or
not isinstance(psf_gmix,gmix_image.GMix)):
raise ValueError("send GMix objects")
self.obj0_gmix=obj_gmix
self.psf_gmix=psf_gmix
self.obj_gmix = self.obj0_gmix.convolve(self.psf_gmix)
self.nsub=16
self.center_offset=keys.get('center_offset',None)
self.set_etrue_T()
self.set_dims_and_cen()
self.make_images()
self.add_psf_stats()
self.add_image_stats()
def set_etrue_T(self):
e1,e2,T = self.obj0_gmix.get_e1e2T()
e1conv,e2conv,Tconv = self.obj_gmix.get_e1e2T()
e1_psf,e2_psf,T_psf = self.psf_gmix.get_e1e2T()
counts = self.obj_gmix.get_psum()
self['Ttrue'] = T
self['counts_true'] = counts
self['e1true'] = e1
self['e2true'] = e2
self['etrue'] = sqrt(e1**2 + e2**2)
self['Ttrue_conv'] = Tconv
self['Ttrue_psf'] = T_psf
self['e1true_psf'] = e1_psf
self['e2true_psf'] = e2_psf
self['etrue_psf'] = sqrt(e1_psf**2 + e2_psf**2)
def set_dims_and_cen(self):
"""
Simple for analytic convolutions
"""
sigma=mom2sigma(self['Ttrue_conv'])
fac=GAUSS_PADDING
if 'pad_mult' in self:
fac *= self['pad_mult']
imsize = fac*2*sigma
dims = array([imsize]*2,dtype='i8')
if (dims[0] % 2) == 0:
dims += 1
cen=(dims-1.0)/2.0
if self.center_offset is not None:
cen += self.center_offset
self['dims'] = dims
self['cen'] = cen
self.psf_gmix.set_cen(cen[0],cen[1])
self.obj_gmix.set_cen(cen[0],cen[1])
self.obj0_gmix.set_cen(cen[0],cen[1])
def make_images(self):
import gmix_image
self.psf = gmix_image.gmix2image(self.psf_gmix,self['dims'],
nsub=self.nsub)
self.image = gmix_image.gmix2image(self.obj_gmix,self['dims'],
nsub=self.nsub)
#self.image0 = gmix_image.gmix2image(self.obj0_gmix,self['dims'],
# nsub=self.nsub)
self.image0=None
def add_image_stats(self):
self['cen_uw'] = self.obj0_gmix.get_cen()
res = admom.admom(self.image, self['cen'][0],self['cen'][1],
guess=self['Ttrue']/2.)
cov_admom = array([res['Irr'],res['Irc'],res['Icc']])
cen_admom = array([res['wrow'], res['wcol']])
self['cov_admom'] = cov_admom
self['cen_admom'] = cen_admom
self['a4'] = res['a4']
self['e1_admom'] = res['e1']
self['e2_admom'] = res['e2']
def add_psf_stats(self):
self['cen_psf'] = self.psf_gmix.get_cen()
self['cen_psf_uw'] = self['cen_psf']
res = admom.admom(self.psf,self['cen_psf'][0],self['cen_psf'][1],
guess=self['Ttrue_psf']/2.)
cov_admom = array([res['Irr'],res['Irc'],res['Icc']])
cen_admom = array([res['wrow'], res['wcol']])
self['cov_psf_admom'] = cov_admom
self['cen_psf_admom'] = cen_admom
self['a4_psf'] = res['a4']
def trim(self, fluxfrac=0.997):
im = self.image
row,col=ogrid[0:im.shape[0],
0:im.shape[1]]
rm = array(row - self['cen'][0], dtype='f8')
cm = array(col - self['cen'][1], dtype='f8')
radm = sqrt(rm**2 + cm**2)
radii = numpy.arange(1,im.shape[0]/2)
cnts=numpy.zeros(radii.size)
for ir,r in enumerate(radii):
w=where(radm <= r)
if w[0].size > 0:
cnts[ir] = im[w].sum()
cnts /= cnts.max()
w,=where(cnts > fluxfrac)
if w.size > 0:
rad = radii[w[0]]
rmin = self['cen'][0]-rad
rmax = self['cen'][0]+rad
cmin = self['cen'][1]-rad
cmax = self['cen'][1]+rad
if rmin < 0:
rmin=0
if rmax > (im.shape[0]-1):
rmax = (im.shape[0]-1)
if cmin < 0:
cmin=0
if cmax > (im.shape[1]-1):
cmax = (im.shape[1]-1)
self.image = self.image[rmin:rmax, cmin:cmax]
self.psf = self.psf[rmin:rmax, cmin:cmax]
# reset dims and centers
self['dims'] = self.image.shape
cen = [self['cen'][0]-rmin, self['cen'][0]-cmin]
self['cen']=cen
self.psf_gmix.set_cen(cen[0],cen[1])
self.obj_gmix.set_cen(cen[0],cen[1])
self.obj0_gmix.set_cen(cen[0],cen[1])
self.add_image_stats()
self.add_psf_stats()