/
SingleLensFitter.py
1203 lines (815 loc) · 30.8 KB
/
SingleLensFitter.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
import numpy as np
from scipy import linalg
from scipy import optimize
import emcee
import george
from george import kernels
import matplotlib as mpl
mpl.use("Agg")
import matplotlib.pyplot as plt
from matplotlib import gridspec
from matplotlib.ticker import MaxNLocator
from pylab import subplots_adjust
import corner
from astropy.stats import mad_std
from scipy.interpolate import interp1d
from scipy.optimize import minimize
class SingleLensFitter():
"""Class definition for single microlens event fitter."""
def __init__(self,data,initial_parameters,eigen_lightcurves=None,reference_source=None,ZP=28.0):
"""Initialise the SingleLensFitter.
inputs:
data: A dictionary with each key being a data set name string and each
value being a tuple of (date, flux, flux_err) each being numpy
arrays.
initial_parameters: A numpy array of starting guess values for u_0, t_0, t_E.
eigen_lightcurves: If defined, this should be a dictionary with the same keys as data,
and each value being an n x m numpy array of n lightcurves each
with m data values corresponding to the dates of the input data.
These lightcurves (detrend vectors) are fitted linearly to the data
at the same time as the magnification and flux parameters. An
eigen_lightucrves dictionary entry can be defined for any subset
of data sources, and different data sources can have different
numbers of eigenlightcurves.
"""
self.data = data
self.eigen_lightcurves = eigen_lightcurves
self.initial_parameters = initial_parameters
self.p = initial_parameters
self.ZP = ZP
if reference_source is None:
self.reference_source = self.data.keys()[0]
print 'Using',self.reference_source,'as reference.'
else:
if reference_source in self.data:
self.reference_source = reference_source
else:
self.reference_source = self.data.keys()[0]
print 'Warning:',reference_source,'is not a valid data source.'
print 'Using',self.reference_source,'as reference.'
self.parameter_labels = [r"$u_0$",r"$t_0$",r"$t_E$"]
self.ndim = 3
self.use_finite_source = False
self.use_limb_darkening = False
self.use_source_variability = False
self.use_blend_variability = False
self.marginalise_linear_parameters = True
self.fit_blended = True
self.u0_limits = (0.0,1.3)
self.tE_limits = (0.5,200)
self.t0_limits = None
self.lrho_limits = (-6,0)
self.use_gaussian_process_model = False
self.GP_default_params = (1.0,-2.0)
self.ln_a_limits = (-5,15)
self.ln_tau_limits = (-5.5, 7.0)
self.ln_a = {}
self.ln_tau = {}
self.cov = {}
self.use_mixture_model = False
self.mixture_default_params = (0.0001,1.0e8,0.0)
self.P_b_limits = (0.0,0.05)
self.V_b_limits = (0.0,1.0e12)
self.Y_b_limits = (-1.e5,1.e5)
self.P_b = {}
self.V_b = {}
self.Y_b = {}
self.use_finite_source = False
self.nwalkers = 50
self.nsteps = 50
self.nsteps_production = 500
self.thresh_std = 0.1
self.thresh_mean = 0.05
self.max_burnin_iterations = 200
self.emcee_lnp_convergence_threshold = 0.5
self.emcee_mean_convergence_threshold = 0.1
self.emcee_std_convergence_threshold = 0.1
self.plotprefix = 'single_lens_fit'
self.samples = None
self.n_plot_samples = 30
self.make_plots = True
self.plot_colours = ['#FF0000', '#000000', '#008000', '#800080', '#FFA500', '#A52A2A', '#ff9999', '#999999', \
'#4c804c', '#804d80', '#ffdb98', '#a56262', '#CCFF66', '#CC9900', '#9966FF', '#FF3366']
return
def add_finite_source(self,lrho=None):
from mpmath import ellipe
self.use_finite_source = True
self.finite_source_index = self.ndim
if lrho is not None:
self.lrho = lrho
else:
self.lrho = -3.0
self.p = np.hstack((self.p,self.lrho))
self.parameter_labels.append(r"$log_{10} \rho$")
self.ndim += 1
self.finite_source_integration_subintervals = 50
# lz = np.arange(-5,10,0.01)
# fsz = 10.0**lz
# ell = np.zeros_like(fsz)
# rsz = np.arcsin(1.0/fsz)
# p2 = np.pi/2.0
# for zi in range(len(lz)):
# if fsz[zi] < 1.0:
# ell[zi] = ellipe(p2,fsz[zi])
# else:
# ell[zi] = ellipe(rsz[zi],fsz[zi])
#self._ellipe_interpolator = interp1d(fsz,ell)
def add_limb_darkening(self,gamma=None,lrho=None):
if not self.use_finite_source:
self.add_finite_source(lrho=lrho)
self.use_limb_darkening = True
self.limb_darkening_index = self.ndim
if gamma is not None:
self.gamma = gamma
else:
self.gamma = 0.1
self.p = np.hstack((self.p,self.gamma))
self.parameter_labels.append(r"$\Gamma$")
self.ndim += 1
# Set up 2d Simpsons Rule matrix
n = self.finite_source_integration_subintervals
x = np.ones(n+1)
c2 = np.arange(n/2-1)*2 + 2
c4 = np.arange(n/2)*2 + 1
x[c2] = 2
x[c4] = 4
xx, yy = np.meshgrid(x,x)
self.simpson_matrix = xx*yy
def add_source_variability(self,params=None):
self.use_source_variability = True
self.source_variability_index = self.ndim
if params is not None:
self.source_variability_amplitude = params[0]
self.source_variability_frequency = params[1]
self.source_variability_phase = params[2]
else:
self.source_variability_amplitude = 0.001
self.source_variability_frequency = np.pi
self.source_variability_phase = 0.0
self.p = np.hstack((self.p,self.source_variability_amplitude,self.source_variability_frequency,self.source_variability_phase))
self.parameter_labels.append(r"$K$")
self.parameter_labels.append(r"$\omega$")
self.parameter_labels.append(r"$phi$")
self.ndim += 3
def add_blend_variability(self,params=None):
self.use_blend_variability = True
self.blend_variability_index = self.ndim
if params is not None:
self.blend_variability_amplitude = params[0]
self.blend_variability_frequency = params[1]
self.blend_variability_phase = params[2]
else:
self.blend_variability_amplitude = 0.001
self.blend_variability_frequency = np.pi
self.blend_variability_phase = 0.0
self.p = np.hstack((self.p,self.blend_variability_amplitude,self.blend_variability_frequency,self.blend_variability_phase))
self.parameter_labels.append(r"$K$")
self.parameter_labels.append(r"$\omega$")
self.parameter_labels.append(r"$phi$")
self.ndim += 3
def add_mixture_model(self):
self.use_mixture_model = True
self.mixture_index = self.ndim
for site in self.data.keys():
self.p = np.hstack((self.p, self.mixture_default_params))
self.ndim += 3
self.parameter_labels.append(site+'_P_b')
self.parameter_labels.append(site+'_V_b')
self.parameter_labels.append(site+'_Y_b')
def add_gaussian_process_model(self,common=True):
self.use_gaussian_process_model = True
self.gaussian_process_index = self.ndim
self.gaussian_process_common = common
if common:
self.p = np.hstack((self.p, self.GP_default_params))
self.ndim += 2
self.parameter_labels.append('ln_a')
self.parameter_labels.append('ln_tau')
else:
for site in self.data.keys():
self.p = np.hstack((self.p, self.GP_default_params))
self.ndim += 2
self.parameter_labels.append(site+'_ln_a')
self.parameter_labels.append(site+'_ln_tau')
def lnprior_GP(self,GP_params):
params = ['ln_a','ln_tau']
for i, p in enumerate(params):
prange = eval('self.'+p+'_limits')
if prange:
if GP_params[i] < prange[0] or GP_params[i] > prange[1]:
return -np.inf
return 0.0
def lnprior_mixture(self,mixture_params):
params = ['P_b','V_b','Y_b']
for i, p in enumerate(params):
prange = eval('self.'+p+'_limits')
if prange:
if mixture_params[i] < prange[0] or mixture_params[i] > prange[1]:
return -np.inf
return 0.0
def lnprior_ulens(self):
params = ['u0','t0','tE']
for p in params:
prange = eval('self.'+p+'_limits')
if prange:
param = eval('self.'+p)
if param < prange[0] or param > prange[1]:
return -np.inf
return 0.0
def lnprior_lrho(self,lrho):
if lrho < self.lrho_limits[0] or lrho > self.lrho_limits[1]:
return -np.inf
return 0.0
def lnprior_gamma(self,gamma):
if gamma < 0.0 or gamma > 1.0:
return -np.inf
return 0.0
def lnprior_source_variability(self,params):
K =params[0]
omega = params[1]
phi = params[2]
if K < 0.0 or phi < 0.0 or phi > 2.0*np.pi or omega > 4 or omega < 0.1:
return -np.inf
return 0.0
def lnprob(self,p):
self.p = p
self.u0 = p[0]
self.t0 = p[1]
self.tE = p[2]
lp = self.lnprior_ulens()
if self.use_finite_source:
lp += self.lnprior_lrho(p[self.finite_source_index])
if self.use_limb_darkening:
lp += self.lnprior_gamma(p[self.limb_darkening_index])
if self.use_source_variability:
ind = self.source_variability_index
lp += self.lnprior_source_variability(p[ind:ind+3])
if self.use_blend_variability:
ind = self.blend_variability_index
lp += self.lnprior_source_variability(p[ind:ind+3])
if self.use_mixture_model:
pi = self.mixture_index
for data_set_name in self.data.keys():
self.P_b[data_set_name] = p[pi]
self.V_b[data_set_name] = p[pi+1]
self.Y_b[data_set_name] = p[pi+2]
lp += self.lnprior_mixture(p[pi:pi+3])
pi += 3
if self.use_gaussian_process_model:
pi = self.gaussian_process_index
if self.gaussian_process_common:
self.ln_a = p[pi]
self.ln_tau = p[pi+1]
lp += self.lnprior_GP(p[pi:pi+2])
pi += 2
else:
for data_set_name in self.data.keys():
self.ln_a[data_set_name] = p[pi]
self.ln_tau[data_set_name] = p[pi+1]
lp += self.lnprior_GP(p[pi:pi+2])
pi += 2
if np.isfinite(lp):
lp += self.lnlikelihood()
else:
return -np.inf
return lp
def neglnprob(self,p):
return -self.lnprob(p)
def lnlikelihood(self):
lnprob = 0.0
for data_set_name in self.data.keys():
t, y, yerr = self.data[data_set_name]
mag = self.magnification(t)
if self.use_gaussian_process_model:
if self.gaussian_process_common:
a = np.exp(self.ln_a)
tau = np.exp(self.ln_tau)
else:
a = np.exp(self.ln_a[data_set_name])
tau = np.exp(self.ln_tau[data_set_name])
gp = george.GP(a * kernels.ExpKernel(tau))
gp.compute(t, yerr)
self.cov[data_set_name] = gp.get_matrix(t)
result, lp = self.linear_fit(data_set_name,mag)
model = self.compute_lightcurve(data_set_name,t)
lnprob = gp.lnlikelihood(y-model)
else:
result, lp = self.linear_fit(data_set_name,mag)
lnprob += lp
return lnprob
def linear_fit(self,data_key,mag):
t, y, yerr = self.data[data_key]
if self.use_gaussian_process_model:
C = self.cov[data_key]
else:
C = np.diag(yerr**2)
C_inv = linalg.inv(C)
if self.fit_blended:
if self.use_source_variability:
ind = self.source_variability_index
A = np.vstack((np.ones_like(mag),mag*(1.0+self.p[ind]*np.sin(self.p[ind+1]*t+self.p[ind+2]))))
elif self.use_blend_variability:
ind = self.blend_variability_index
A = np.vstack((np.ones_like(mag)*(1.0+self.p[ind]*np.sin(self.p[ind+1]*t+self.p[ind+2])),mag))
else:
A = np.vstack((np.ones_like(mag),mag))
n_params = 2
else:
if self.use_source_variability:
ind = self.source_variability_index
A = (mag*(1.0+self.p[ind]*np.sin(self.p[ind+1]*t+self.p[ind+2]))-1.0).reshape(1,len(mag))
else:
A = (mag-1.0).reshape(1,len(mag))
n_params = 1
if self.eigen_lightcurves is not None:
if data_key in self.eigen_lightcurves:
eigs = self.eigen_lightcurves[data_key]
for i in range(eigs.shape[0]):
A = np.vstack((A,eigs[i,:]))
n_params += 1
S = np.dot(A,np.dot(C_inv,A.T)).reshape(n_params,n_params)
b = np.dot(A, np.dot(C_inv,y).T)
if self.marginalise_linear_parameters:
try:
M = linalg.inv(S)
except linalg.LinAlgError:
return (0,0), -np.inf
g = np.dot(M,b)
D = y - np.dot(A.T,g)
chi2 = np.dot(D.T,np.dot(C_inv,D))
if self.use_mixture_model:
detM = linalg.det(M)
lnprob = np.log( 2*np.pi*np.sum( (1.0 - self.P_b[data_key]) * \
np.exp(-D**2/(2.0*yerr**2)) / \
np.sqrt(detM) + \
self.P_b[data_key]*np.exp(-(y-self.Y_b[data_key])**2 / \
2*(self.V_b[data_key]+yerr**2)) / \
np.sqrt(2*np.pi*(self.V_b[data_key]+yerr**2)) ))
else:
lnprob = np.log(2*np.pi) - 0.5*chi2 - 0.5*np.log(linalg.det(M))
return g, lnprob
else:
try:
a = linalg.solve(S,b)
except linalg.LinAlgError:
return (0,0), -np.inf
D = y - np.dot(A.T,a)
chi2 = np.dot(D.T,np.dot(C_inv,D))
if self.use_mixture_model:
lnprob = np.sum( np.log( (1.0 - self.P_b[data_key])*np.exp(-D**2/(2.0*yerr**2)) / \
np.sqrt(2*np.pi*yerr**2) + \
self.P_b[data_key]*np.exp(-(y-self.Y_b[data_key])**2 / \
2*(self.V_b[data_key]+yerr**2)) / \
np.sqrt(2*np.pi*(self.V_b[data_key]+yerr**2)) ))
else:
lnprob = -np.log(np.sum(np.sqrt(2*np.pi*yerr**2))) - 0.5*chi2
return a, lnprob
def magnification(self,t,p=None):
if p is None:
p = self.p
u0, t0, tE = p[:3]
if self.use_finite_source:
lrho = p[self.finite_source_index]
tau = (t-t0)/tE
u = np.sqrt(u0**2+tau**2)
A = (u**2 + 2.0)/(u*np.sqrt(u**2+4.0))
if self.use_finite_source:
rho = 10.0**lrho
#
# This is from Lee et al. (2009) ApJ, 695, 200
#
n = self.finite_source_integration_subintervals
z = np.abs(u)/rho
fs_points = np.where(z < 10.0)[0]
if self.use_limb_darkening:
epsilon = 1.0e-8
gamma = p[self.limb_darkening_index]
S = self.simpson_matrix
for q in range(len(fs_points)):
uq = u[fs_points[q]]
if uq <= rho:
theta_1d = np.arange(n+1)*np.pi/n
theta = np.broadcast_to(theta_1d,(n+1,n+1)).T
delta_theta = np.pi/n
u1 = 0.0*theta_1d
u2 = uq*np.cos(theta_1d) + np.sqrt(rho**2 - uq**2 * np.sin(theta_1d)**2) - epsilon
else:
theta_1d = np.arange(n+1)*np.pi/(2.0*n)
theta = np.broadcast_to(theta_1d,(n+1,n+1)).T
delta_theta = np.pi/(2.0*n)
u1 = uq*np.cos(theta_1d) - np.sqrt(rho**2 - uq**2 * np.sin(theta_1d)**2) + epsilon
u2 = uq*np.cos(theta_1d) + np.sqrt(rho**2 - uq**2 * np.sin(theta_1d)**2) - epsilon
u1[theta_1d>np.arcsin(rho/uq)] = 0.0
u2[theta_1d>np.arcsin(rho/uq)] = 0.0
uu1 = np.broadcast_to(u1,(n+1,n+1)).T
uu2 = np.broadcast_to(u2,(n+1,n+1)).T
r = np.broadcast_to(np.arange(n+1),(n+1,n+1))*(uu2-uu1)/n + uu1
delta_r = np.ones_like(r)
delta_r[:,1:-1] = 0.5*(r[:,2:] - r[:,:-2])
delta_r[:,0] = 0.5*(r[:,1] - r[:,0])
delta_r[:,-1] = 0.5*(r[:,-1] - r[:,-2])
integrand = ((r**2+2.0)/np.sqrt(r**2+4.0)) * \
(1.0-gamma*(1.0-1.5*np.sqrt(1.0-(r**2-2.0*r*uq*np.cos(theta)+uq**2)/rho**2) ))
integrand[np.isnan(integrand)] = 0.0
#A[fs_points[q]] = 2.0/(np.pi*rho**2) * (delta_theta/9.0) * np.sum(S*integrand*delta_r)
A[fs_points[q]] = np.sum(S*integrand*delta_r)/np.sum(S*r*delta_r)
# if uq <= 0.7*rho:
# print 'uq',uq
# print 'rho', rho
# print 'u1', u1
# print 'u2', u2
# print 'uu1', uu1
# print 'uu2', uu2
# print 'uu2-uu1', uu2-uu1
# print 'theta', theta_1d
# print 'r', r
# print 'S', S
# print 'delta_r',delta_r
# print 'integrand', integrand
# print 'A', A[fs_points[q]]
# sys.exit()
else:
for q in range(len(fs_points)):
uq = u[fs_points[q]]
if uq <= rho:
k = np.arange(1,n)
theta = np.pi*k/n
u2 = uq*np.cos(theta) + np.sqrt(rho**2 - uq**2 * np.sin(theta)**2)
f1 = u2 * np.sqrt(u2**2 + 4.0)
k = np.arange(1,n+1)
theta = np.pi*(2.0*k - 1.0)/(2.0*n)
u2 = uq*np.cos(theta) + np.sqrt(rho**2 - uq**2 * np.sin(theta)**2)
f2 = u2 * np.sqrt(u2**2 + 4.0)
A[fs_points[q]] = (1.0/(2.0*n*rho**2)) * ( ((uq+rho)/3.0) * np.sqrt((uq+rho)**2+4.0) - \
((uq-rho)/3.0) * np.sqrt((uq-rho)**2+4.0) + \
(2.0/3.0) * np.sum(f1) + (4.0/3.0) * np.sum(f2) )
else:
k = np.arange(1,n/2)
theta = 2.0*k*np.arcsin(rho/uq)/n
u1 = uq * np.cos(theta) - np.sqrt(rho**2 - uq**2 * np.sin(theta)**2)
u2 = uq * np.cos(theta) + np.sqrt(rho**2 - uq**2 * np.sin(theta)**2)
f1 = u2 * np.sqrt(u2**2 + 4.0) - u1 * np.sqrt(u1**2 + 4.0)
k = np.arange(1,n/2+1)
theta = (2.0*k-1.0)*np.arcsin(rho/uq)/n
u1 = uq * np.cos(theta) - np.sqrt(rho**2 - uq**2 * np.sin(theta)**2)
u2 = uq * np.cos(theta) + np.sqrt(rho**2 - uq**2 * np.sin(theta)**2)
f2 = u2 * np.sqrt(u2**2 + 4.0) - u1 * np.sqrt(u1**2 + 4.0)
A[fs_points[q]] = (np.arcsin(rho/uq)/(np.pi*n*rho**2)) * \
( ((uq+rho)/3.0) * np.sqrt((uq+rho)**2+4.0) - \
((uq-rho)/3.0) * np.sqrt((uq-rho)**2+4.0) + \
(2.0/3.0) * np.sum(f1) + (4.0/3.0) * np.sum(f2) )
#
# This is from Gould (1994) ApJ, 421, L71
#
# z = np.abs(u)/rho
# fs_points = np.where(z < 50.0)[0]
# print 'fs_points', fs_points
# print 'z[fs_points]', z[fs_points]
# B0 = 4 * z[fs_points] * self._ellipe_interpolator(z[fs_points]) / np.pi
# A[fs_points] *= B0
return A
def fit(self,method='Nelder-Mead'):
if self.p is None:
raise Exception('Error in SingleLensFitter.fit(): No initial_parameters found.')
return None
print 'Initial parameters:', self.p
print 'ln Prob = ',self.lnprob(self.p)
result = minimize(self.neglnprob,self.p,method=method)
self.p = result.x
print 'Final parameters:', self.p
print 'ln Prob = ',self.lnprob(self.p)
def emcee_has_converged(self,sampler,n_steps=100):
# Emcee convergence testing is not easy. The method we will adopt
# is to test whether the parameter means and standard deviations, and ln_p, have
# stabilised, comparing the last n steps, with the previous n steps.
#std_threshold = 0.01
#mean_threshold = 0.01
n_test = sampler.chain.shape[0]*n_steps
lnp = sampler.lnprobability.T.ravel()
if len(lnp) < 2*n_test:
return False
converged = True
steps = sampler.chain.shape[1]
with open(self.plotprefix+'_lnp','a') as fid:
fid.write("After %d steps, parameter means, standard deviations, convergence metrics and ln_P:\n"%steps)
for k in range(sampler.chain.shape[2]):
samples = sampler.chain[:,:,k].T.ravel()
mean2 = np.mean(samples[-2*n_test:-n_test])
mean1 = np.mean(samples[-n_test:])
std2 = np.std(samples[-2*n_test:-n_test:])
std1 = np.std(samples[-n_test:])
delta_param = np.abs(mean1 - mean2)/std1
delta_std = np.abs(std2-std1)/std2
fid.write("%g %g %g %g\n"%(mean1,std1,delta_param,delta_std))
if delta_param > self.emcee_mean_convergence_threshold:
converged = False
if delta_std > self.emcee_std_convergence_threshold:
converged = False
lnp_delta = np.mean(lnp[-n_test:]) - np.mean(lnp[-2*n_test:-n_test])
if lnp_delta > self.emcee_lnp_convergence_threshold:
converged = False
fid.write("delta lnp: %10.4f %d\n"%(lnp_delta,converged))
return converged
def sample(self,optimize_first=False):
if self.p is None:
raise Exception('Error in SingleLensFitter.fit(): No initial_parameters found.')
return None
print 'Initial parameters:', self.p
print 'ln Prob = ',self.lnprob(self.p)
ndim = self.ndim
if optimize_first:
print 'Optimising...'
minimize(self.neglnprob,self.p,method='Nelder-Mead')
print 'Optimized parameters:', self.p
print 'ln Prob = ',self.lnprob(self.p)
print ndim, len(self.p), self.nwalkers
self.state = [self.p + 1e-8 * np.random.randn(ndim) \
for i in xrange(self.nwalkers)]
sampler = emcee.EnsembleSampler(self.nwalkers, ndim, self.lnprob)
print("Running burn-in...")
iteration = 0
converged = False
steps = 0
self.count = 0
print 'ndim, walkers, nsteps, max_iterations:', ndim, self.nwalkers, self.nsteps, self.max_burnin_iterations
while not converged and iteration < self.max_burnin_iterations:
self.state, lnp , _ = sampler.run_mcmc(self.state, self.nsteps)
iteration += 1
print 'iteration', iteration, 'completed'
kmax = np.argmax(sampler.flatlnprobability)
self.p = sampler.flatchain[kmax,:]
np.save(self.plotprefix+'-state-burnin',np.asarray(self.state))
if self.make_plots:
self.plot_chain(sampler,suffix='-burnin.png')
# ind = 3
# if self.use_finite_source:
# ind += 1
# npar = 0
# if self.use_mixture_model:
# npar += 3
# if self.use_gaussian_process_model:
# npar += 2
# if npar > 0:
# for data_set_name in self.data.keys():
# self.plot_chain(sampler,index=range(ind,npar+ind), \
# suffix='-burnin-'+data_set_name+'.png', \
# labels=self.parameter_labels[ind:ind+npar])
# ind += npar
# if self.gaussian_process_common:
# ind -= 2
self.plot_combined_lightcurves()
converged = self.emcee_has_converged(sampler,n_steps=self.nsteps)
print("Running production...")
sampler.reset()
self.state, lnp, _ = sampler.run_mcmc(self.state, self.nsteps_production)
self.samples = sampler.flatchain
params = map(lambda v: (v[1], v[2]-v[1], v[1]-v[0]), \
zip(*np.percentile(self.samples[:,:], \
[16, 50, 84], axis=0)))
self.p = np.asarray(params)[:,0]
self.u0 = self.p[0]
self.t0 = self.p[1]
self.tE = self.p[2]
if self.use_finite_source:
self.rho = self.p[self.finite_source_index]
if self.use_limb_darkening:
self.gamma = self.p[self.limb_darkening_index]
if self.make_plots:
self.plot_chain(sampler,suffix='-final.png')
# ind = 3
# if self.use_finite_source:
# ind += 1
# if npar > 0:
# for data_set_name in self.data.keys():
# self.plot_chain(sampler,index=range(ind,npar+ind), \
# suffix='-final-'+data_set_name+'.png', \
# labels=self.parameter_labels[ind:ind+npar])
# if not self.gaussian_process_common:
# ind += npar
# ind += npar
self.plot_lightcurves()
self.plot_chain_corner()
print 'Results:'
# print 'u0', params[0]
# print 't0', params[1]
# print 'tE', params[2]
# if self.use_finite_source:
# print 'rho', params[self.finite_source_index]
with open(self.plotprefix+'.fit_results','w') as fid:
for i in range(self.ndim):
fid.write('%s %f %f %f\n'%(self.parameter_labels[i],params[i][0],params[i][1],params[i][2]))
print '%s %f %f %f\n'%(self.parameter_labels[i],params[i][0],params[i][1],params[i][2])
# fid.write('u0 %f %f %f\n'%(params[0][0],params[0][1],params[0][2]))
# fid.write('t0 %f %f %f\n'%(params[1][0],params[1][1],params[1][2]))
# fid.write('tE %f %f %f\n'%(params[2][0],params[2][1],params[2][2]))
# if self.use_finite_source:
# pi = self.finite_source_index
# fid.write('rho %f %f %f\n'%(params[pi][0],params[pi][1],params[pi][2]))
# if self.use_limb_darkening:
# pi = self.limb_darkening_index
# fid.write('gamma %f %f %f\n'%(params[pi][0],params[pi][1],params[pi][2]))
np.save(self.plotprefix+'-state-production',np.asarray(self.state))
np.save(self.plotprefix+'-min_chi2-production',np.asarray(sampler.flatchain[np.argmax(sampler.flatlnprobability)]))
return
def plot_chain(self,s,index=None,plot_lnprob=True,suffix='',labels=None):
if index is None:
index = range(self.ndim)
if labels is None:
labels = self.parameter_labels
ndim = len(index)
plt.figure(figsize=(8,11))
subplots_adjust(hspace=0.0001)
for i in range(ndim):
if i == 0:
plt.subplot(ndim+plot_lnprob,1,i+1)
ax1 = plt.gca()
else:
plt.subplot(ndim+plot_lnprob,1,i+1,sharex=ax1)
plt.plot(s.chain[:,:,index[i]].T, '-', color='k', alpha=0.3)
if labels:
plt.ylabel(labels[i])
ax = plt.gca()
if i < ndim-1+plot_lnprob:
plt.setp(ax.get_xticklabels(), visible=False)
ax.yaxis.set_major_locator(MaxNLocator(prune='lower'))
ax.locator_params(axis='y',nbins=4)
if plot_lnprob:
plt.subplot(ndim+plot_lnprob,1,ndim+plot_lnprob,sharex=ax1)
plt.plot(s.lnprobability.T, '-', color='r', alpha=0.3)
plt.ylabel(r"$ln P$")
ax = plt.gca()
ax.yaxis.set_major_locator(MaxNLocator(prune='lower'))
ax.locator_params(axis='y',nbins=4)
plt.savefig(self.plotprefix+suffix)
plt.close()
def compute_lightcurve(self,data_key, x, params=None):
t, _, _ = self.data[data_key]
coeffs, _ = self.linear_fit(data_key,self.magnification(t,params))
if self.fit_blended:
if self.use_source_variability:
ind = self.source_variability_index
fx = coeffs[0]+coeffs[1]*self.magnification(x,params)*(1.0+self.p[ind]*np.sin(self.p[ind+1]*x+self.p[ind+2]))
elif self.use_blend_variability:
ind = self.blend_variability_index
fx = coeffs[0]*(1.0+self.p[ind]*np.sin(self.p[ind+1]*x+self.p[ind+2]))+coeffs[1]*self.magnification(x,params)
else:
fx = coeffs[0]+coeffs[1]*self.magnification(x,params)
else:
if self.use_source_variability:
ind = self.source_variability_index
fx = coeffs[0]*(self.magnification(x,params)*(1.0+self.p[ind]*np.sin(self.p[ind+1]*x+self.p[ind+2]))-1)
else:
fx = coeffs[0]*(self.magnification(x,params)-1)
return fx
def plot_combined_lightcurves(self,t_range=None,y_range=None):
plt.figure(figsize=(8,11))
colour = iter(plt.cm.jet(np.linspace(0,1,len(self.data))))
if t_range is None:
t_min = self.p[1]-4*self.p[2]
t_max = self.p[1]+4*self.p[2]
for site in self.data.keys():
if np.min(self.data[site][0]) < t_min:
t_min = np.min(self.data[site][0])
if np.max(self.data[site][0]) > t_max:
t_max = np.max(self.data[site][0])
else:
t_min, t_max = t_range
n_data = len(self.data)
gs = gridspec.GridSpec(2,1,height_ratios=(3,1))
# Main lightcurve plot
ax0 = plt.subplot(gs[0])