-
Notifications
You must be signed in to change notification settings - Fork 2
/
bootstrap_makeradialtexdistr.py~
926 lines (801 loc) · 37.4 KB
/
bootstrap_makeradialtexdistr.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
from astropy.io import fits
import numpy as np
import astropy.units as u
import math
import matplotlib.pyplot as plt
import matplotlib as mpl
from astropy import visualization
import os
import pdb
from scipy.optimize import curve_fit as cf
from astropy.modeling import powerlaws, fitting
from operator import add,sub,truediv
from matplotlib import gridspec
from astropy.table import QTable, vstack, hstack
import radio_beam
import sys
import regions
from astropy.wcs import WCS
mpl.interactive(True)
plt.close('all')
mu=2.8*u.Dalton
def circle(data,ycenter,xcenter,rad):
edgex=[]
edgey=[]
for i in range(np.shape(data)[0]):
for j in range(np.shape(data)[1]):
if (j-xcenter)**2+(i-ycenter)**2==rad**2:
edgex.append(j)
edgey.append(i)
return np.vstack((edgex,edgey))
def submid_profile(r):
n=0.75
c=powerlawpair[0]*(powerlawpair[1]/pixtophysicalsize)**n
return c*((r/pixtophysicalsize)**-n)
def sublinear_profile(r):
n=0.5
c=powerlawpair[0]*(powerlawpair[1]/pixtophysicalsize)**n
return c*((r/pixtophysicalsize)**-n)
def linear_profile(r):
n=1
c=powerlawpair[0]*(powerlawpair[1]/pixtophysicalsize)**n
return c*((r/pixtophysicalsize)**-n)
def quadratic_profile(r):
n=1.25
c=powerlawpair[0]*(powerlawpair[1]/pixtophysicalsize)**n
return c*((r/pixtophysicalsize)**-n)
def powerlaw_profile(x,a,n):
return a*((x/pixtophysicalsize.value)**-n)
def round_to_1(x):
return round(x, -int(math.floor(math.log10(abs(x)))))
source=os.getenv('SOURCE')#'SgrB2S'
fielddict={'SgrB2S':1,'DSi':10,'DSii':10,'DSiii':10,'DSiv':10,'DSv':10,'DSVI':2,'DSVII':3,'DSVIII':3,'DSIX':7}
fnum=fielddict[source]
print(f'Source: {source}')
base=f'/blue/adamginsburg/d.jeff/SgrB2DSreorg/field{fnum}/CH3OH/{source}/'
homedict={'SgrB2S':'/nov2022continuumsanitycheck_limitvt1lines_centeronlinepeak_repline20-20/','DSi':'/nov2022continuumsanitycheck/','DSii':'/nov2022continuumsanitycheck/','DSiii':'/nov2022continuumsanitycheck/','DSiv':'/nov2022contniuumsanitycheck/','DSv':f'/nov2022contniuumsanitycheck/','DSVI':'/nov2022continuumsanitycheck/','DSVII':f'/nov2022contniuumsanitycheck/','DSVIII':f'/nov2022contniuumsanitycheck/','DSIX':f'/nov2022contniuumsanitycheck/'}#{'SgrB2S':"new_testingstdfixandontheflyrepstuff_K_OctReimage_restfreqfix_newvelmask_newpeakamp/",'DSi':"Kfield10originals_trial7_field10errors_newexclusion_matchslabwidthtorep/",'DSii':"Kfield10originals_noexclusions/",'DSiii':"Kfield10originals_noexclusions/",'DSiv':"Kfield10originals_noexclusions/",'DSv':"Kfield10originals_noexclusions_include4-3_150K_trial2/",'DSVI':"Kfield2originals_trial3_8_6-8_7excluded/",'DSVII':'Kfield3originals_200K_trial1_noexclusions/','DSVIII':'Kfield3originals_175K_trial1_noexclusions/','DSIX':'Kfield7originals_150K_trial1_noexclusions/'}#base+'field10originals_z0_000186431_5-6mhzwidth_stdfixes/'
home=base+homedict[source]
fighome=f'/blue/adamginsburg/d.jeff/repos/CH3OHTemps/figures/{source}/'
figpath=fighome+homedict[source]
if not os.path.exists(figpath):
os.makedirs(figpath)
print(f'Creating figpath {figpath}')
else:
print(f'Figpath {figpath} already exists.')
#notransmask=['DSv','DSVI','DSVII','DSVIII','DSIX']
#if source == 'SgrB2S':
texmap=home+"bootstrap_texmap_3sigma_allspw_withnans_weighted.fits"
#else:
#texmap=home+"texmap_5transmask_3sigma_allspw_withnans_weighted.fits"
texerrmap=home+'error_trot_boostrap1000_nonegativeslope.fits'#"texmap_error_allspw_withnans_weighted.fits"
#snrmap=home+"texmap_snr_allspw_weighted.fits"
abunmap=home+'bootstrap_ch3ohabundance_3sigma_ntotintercept_bolocamfeather_smoothedtobolocam.fits'
abunsnrmap=home+'bootstrap_ch3ohabundance_snr_ntotintercept_bolocamfeather_smoothedtobolocam.fits'
nh2map=home+'bootstrap_nh2map_3sigma_bolocamfeather_smoothedtobolocam.fits'
nh2errormap=home+'bootstrap_nh2map_error_bolocamfeather_smoothedtobolocam.fits'
lummap=home+'bootstrap_boltzmannlum_3sigma_bolocamfeather_smoothedtobolocam.fits'
lumerrmap=home+'bootstrap_boltzmannlum_error_bolocamfeather_smoothedtobolocam.fits'
ntotmap=home+'bootstrap_smoothed_ntot_to_bolocamfeathercont_3sigma.fits'
ntoterrmap=home+'bootstrap_smoothed_ntot_err.fits'
h2massmap=home+'bootstrap_h2massmap_3sigma_bolocamfeather_smoothedtobolocam.fits'
h2masserrmap=home+'bootstrap_h2massmap_error_bolocamfeather_smoothedtobolocam.fits'
smoothedtroterrmap=home+'bootstrap_smoothed_trot_err.fits'
smoothedtrotmap=home+'bootstrap_smoothed_trot_to_bolocamfeathercont.fits'
texmap=fits.open(texmap)
texmapdata=texmap[0].data*u.K
texerrdata=np.squeeze(fits.getdata(texerrmap))*u.K
snrs=(texmapdata/texerrdata).value#fits.getdata(snrmap)
abunds=fits.getdata(abunmap)
snr_abund=fits.getdata(abunsnrmap)
nh2s=fits.getdata(nh2map)*u.cm**-2
nh2s_error=fits.getdata(nh2errormap)*u.cm**-2
lums=fits.getdata(lummap)*u.solLum
lumserr=fits.getdata(lumerrmap)*u.solLum
ntots=fits.getdata(ntotmap)*u.cm**-2
ntoterr=np.squeeze(fits.getdata(ntoterrmap))*u.cm**-2
h2mass=fits.getdata(h2massmap)*u.solMass
h2masserr=fits.getdata(h2masserrmap)*u.solMass
smooth_trotfits=fits.open(smoothedtrotmap)
smooth_trot=smooth_trotfits[0].data*u.K
smooth_trot_err=fits.getdata(smoothedtroterrmap)*u.K
if source == 'SgrB2S':
wcsobj=WCS(smooth_trotfits[0].header)
regs = regions.Regions.read('/blue/adamginsburg/d.jeff/imaging_results/regfiles/roughsgrb2smassregion_ignoresHIIregion.reg')
pixreg = regs[0].to_pixel(wcsobj)
pixmask = pixreg.to_mask()
texmapdata=pixmask.cutout(texmapdata,fill_value=np.nan)
'''
texmask=np.ma.masked_where(texmapdata > 1000, texmapdata)
texmapdata=texmask.filled()
'''
texerrdata=pixmask.cutout(texerrdata,fill_value=np.nan)
snrs=np.squeeze(texmapdata/texerrdata)
abunds=pixmask.cutout(abunds,fill_value=np.nan)
snr_abund=pixmask.cutout(snr_abund,fill_value=np.nan)
nh2s=pixmask.cutout(nh2s,fill_value=np.nan)
nh2s_error=pixmask.cutout(nh2s_error,fill_value=np.nan)
lums=pixmask.cutout(lums,fill_value=np.nan)
lumserr=pixmask.cutout(lumserr,fill_value=np.nan)
ntots=pixmask.cutout(ntots,fill_value=np.nan)
ntoterr=pixmask.cutout(ntoterr,fill_value=np.nan)
h2mass=pixmask.cutout(h2mass,fill_value=np.nan)
h2masserr=pixmask.cutout(h2masserr,fill_value=np.nan)
smooth_trot=pixmask.cutout(smooth_trot,fill_value=np.nan)
smooth_trot_err=pixmask.cutout(smooth_trot_err,fill_value=np.nan)
dGC=8.34*u.kpc#per Meng et al. 2019 https://www.aanda.org/articles/aa/pdf/2019/10/aa35920-19.pdf
cntmbeam=radio_beam.Beam.from_fits_header(smooth_trotfits[0].header)
trotbeam=radio_beam.Beam.from_fits_header(texmap[0].header)
cellsize=(np.abs(texmap[0].header['CDELT1']*u.deg)).to('arcsec')
pixperbeam=(cntmbeam.sr/((cellsize**2).to('sr'))).value
pixtophysicalsize=(np.tan(cellsize)*dGC).to('AU')
print(pixtophysicalsize)
bmaj=trotbeam.major#texmap[0].header['BMAJ']*u.deg
bmajpix=round((bmaj/cellsize).value)
bmin=trotbeam.minor#texmap[0].header['BMIN']*u.deg
bminpix=round((bmin/cellsize).value)
beamarea_sr=trotbeam.sr#bmaj*bmin
beamarea_sqdeg=beamarea_sr.to('deg2')
bmajtophyssize=(np.tan(bmaj)*dGC).to('AU')
bmintophyssize=(np.tan(bmin)*dGC).to('AU')
'''Can probably simplify beamarea_phys to d(np.tan(bmaj)*np.tan(bmin))'''
beamarea_phys=trotbeam.beam_projected_area(dGC)#np.pi*bmajtophyssize*bmintophyssize
#pdb.set_trace()
cntmbmaj=cntmbeam.major#3.629587176773e-05*u.deg
cntmbmajtoAU=(np.tan(cntmbmaj)*dGC).to('AU')
pixdict={'SgrB2S':(26,14),'DSi':(36,42),'DSii':(22,24),'DSiii':(24,24),'DSiv':(32,31),'DSv':(19,19),'DSVI':(62,62),'DSVII':(75,75),'DSVIII':(50,50),'DSIX':(34,35)}#y,x; DSiii was 24,24;S was 73,54 - contfix S was 69,58
sgrb2scentralpix=(25,25)#contfix pix, prefinal was (66,70)
#SgrB2S tpeak is 73,54
#nh2dict={'DSiii':(27,27)}
#ntotdict={'SgrB2S':(63,71)'}
texpeakpix=pixdict[source]
#nh2peakpix=nh2dict[source]
#(36,43)#DSi hotspot
#texpeakpix=(73,56)#SgrB2S hotspot
#x-1, y-1 from DS9
print(f'Center p: {texmapdata[texpeakpix[0],texpeakpix[1]]}')
#r=35 #for 15,000 AU
#pixradius=math.ceil((0.08*u.pc/pixtophysicalsize).to(''))
rdict={'SgrB2S':10000*u.AU,'DSi':7500*u.AU,'DSii':8700*u.AU,'DSiii':6000*u.AU,'DSiv':8000*u.AU,'DSv':3500*u.AU,'DSVII':6000*u.AU,'DSVIII':5700*u.AU,'DSIX':5000*u.AU}#1-6400,4-8500,5-4000,7-6600,S-12000
rdictkeys=rdict.keys()
if source not in rdictkeys:
r_phys=10000*u.AU
else:
r_phys=rdict[source]#r*pixtophysicalsize.to('pc')
r=math.ceil((r_phys/pixtophysicalsize).to(''))
print(f'physical radius: {r_phys}')
xpixs=np.arange(texpeakpix[0],(texpeakpix[0]+r))
texinradius=[]
xinradius=[]
yinradius=[]
centrtopix=[]
snrsinradius=[]
abundinradius=[]
abundsnrinradius=[]
nh2inradius=[]
lumsinradius=[]
massinradius=[]
ntotsinradius=[]
lookformax=[]
yy,xx=np.indices(texmapdata.shape)
rr=((xx-texpeakpix[1])**2+(yy-texpeakpix[0])**2)**0.5
mask=rr<r
yy2,xx2=np.indices(smooth_trot.shape)# These are all for the abundances, since the abundance peak in SgrB2S isn't at the temperature peak
rr2=((xx2-texpeakpix[1])**2+(yy2-texpeakpix[0])**2)**0.5
S_rr=((xx2-sgrb2scentralpix[1])**2+(yy2-sgrb2scentralpix[0])**2)**0.5# I may need to try using this on the abundance vs radius plot instead of the rr2
mask2=rr2<r
S_mask=S_rr<r
centrtopix=(rr[mask]*pixtophysicalsize).value
yinradius=rr[0]
xinradius=rr[1]
texinradius=texmapdata[rr<r].value
texerrinradius=texerrdata[rr<r].value
snrsinradius=snrs[rr<r]/5
abundinradius=abunds[rr2<r]
abundsnrinradius=snr_abund[rr2<r]
nh2inradius=nh2s[rr2<r].value
nh2errorinradius=nh2s_error[rr2<r].value
nh2snrinradius=(nh2inradius/nh2errorinradius)
lumsinradius=lums[rr2<r].value
lumerrinradius=lumserr[rr2<r].value
ntotsinradius=ntots[rr2<r].value
massinradius=h2mass[rr2<r].value#(nh2s[rr<r]*mu*beamarea_phys).to('solMass').value
masserrinradius=h2masserr[rr2<r].value#(nh2s_error[rr<r]*mu*beamarea_phys).to('solMass').value
S_massinradius=h2mass[S_rr<r].value
S_masserrinradius=h2masserr[S_rr<r].value
#pdb.set_trace()
lookformax=texmapdata[rr<10**0.5].value
lookformax_err=texerrdata[rr<10**0.5].value
teststack=np.stack((centrtopix,massinradius,snrsinradius,lumsinradius,nh2inradius,nh2errorinradius,texinradius,lumerrinradius,masserrinradius,abundinradius),axis=1)
teststack=teststack[teststack[:,0].argsort()]
set_centrtopix=set(teststack[:,0])
listordered_centrtopix=list(set_centrtopix)
listordered_centrtopix.sort()
avglist=[]
radialdensitylist=[]
err_radialdens=[]
mrcubedlist=[]
avgtexlist=[]
avgtexerrlist=[]
avginversesigma=[]
radialmaxtex=[]
radialmintex=[]
radialmasserr=[]
radialabun=[]
onlymassinteriorandradius=False
massinterior_radius=[]
totalmass=np.nansum(teststack[:,1])
sanitycheckmass=0
edge=None
localminmass=False
trad=180
for bin in listordered_centrtopix:
tempmass=[]
tempsnr=[]
tempmasssnr=[]
temptex=[]
temptexerr=[]
tempinvsig=[]
massesinterior=[]
masserrinterior=[]
tempmasserr=[]
tempabun=[]
for data in teststack:
#print(f'Bin: {bin} AU')
if bin == data[0]:
if np.isnan(data[1]):
#print(f'Nan present in bin {data[0]}')
continue
else:
tempmass.append(data[1])
tempmasssnr.append(data[1]/data[8])
tempmasserr.append(data[8])
tempabun.append(data[9])
if np.isnan(data[6])==False:
if np.isinf(data[2])==False:
truesnr=data[2]*5
temptex.append(data[6])
temptexerr.append(data[6]/truesnr)
tempinvsig.append(truesnr/data[6])
tempsnr.append(truesnr)
if bin >= data[0]:
massesinterior.append(data[1])
masserrinterior.append(data[8])
else:
pass
if len(tempmass)==0:
avglist.append(0)
else:
avg=np.average(tempmass,weights=tempmasssnr)
massinbin=np.nansum(tempmass)*u.solMass
masserrinbin=np.sqrt(np.sum(np.square(tempmasserr)))*np.sqrt(pixperbeam)
binvolume=(4/3)*np.pi*(bin*u.AU)**3
massinteriorsum=np.nansum(massesinterior)*u.solMass
masserrinteriorsum=np.sqrt(np.nansum(np.square(masserrinterior)))*u.solMass*np.sqrt(pixperbeam)
rawdensityinbin=massinteriorsum/binvolume
err_binrawdensity=np.sqrt(masserrinteriorsum/binvolume)**2#np.sqrt(binvolume**-1*masserrinbin*u.solMass)**2
numberdensityinbin=(rawdensityinbin/mu).to('cm-3')
err_binnumberdensity=(np.sqrt(mu**-1*err_binrawdensity)**2).to('cm-3')
mrcubed=((massinbin/mu).to(''))/((bin*u.AU).to('cm'))**3
if len(temptex)==0:
print(f'Problem radius: {bin}')
pdb.set_trace()
else:
pass
avgtex=np.average(temptex,weights=tempsnr)
#if np.isnan(avgtex):
# pdb.set_trace()
#if len(avgtexterr)==0:
# avgtexerr=np.nan
#else:
avgtexerr=np.sqrt(np.sum(np.square(temptexerr)))#np.average(temptexerr)
#pdb.set_trace()
avginvsig=np.average(tempinvsig)
if bin == 0:
tempmaxtex=temptex[0]+temptexerr[0]
tempmintex=temptex[0]-temptexerr[0]
#pdb.set_trace()
else:
tempmaxtex=np.nanmax(temptex)
tempmintex=np.nanmin(temptex)
if avgtex<=150:#massinteriorsum >= 0.5*totalmass:
if edge == None:
#if source == 'DSii' or source == 'DSVI':
# sanitycheckmass=massinteriorsum
# localminmass=True
#else:
edge=bin
sanitycheckmass=massinteriorsum
else:
pass
else:
pass
avgabuninrad=np.nanmean(tempabun)
avglist.append(avg)
avgtexlist.append(avgtex)
avgtexerrlist.append(avgtexerr)
avginversesigma.append(avginvsig)
radialmaxtex.append(tempmaxtex)
radialmintex.append(tempmintex)
radialdensitylist.append(numberdensityinbin.value)
mrcubedlist.append(mrcubed.value)
err_radialdens.append(err_binnumberdensity.value)
radialabun.append(avgabuninrad)
massinterior_radius.append((massinteriorsum.value,masserrinteriorsum.value,bin))
#pdb.set_trace()
if onlymassinteriorandradius:
outlist=np.array(massinterior_radius)
np.savetxt(f'{source}_massinterior_radius.txt',outlist)
sys.exit()
if edge == None:#for hot sources where T never falls below 150 K
mintemp=np.nanmin(avgtexlist)
pix_mintemp=np.where(avgtexlist==mintemp)[0]
edge=listordered_centrtopix[pix_mintemp[0]]
#pdb.set_trace()
fillwidth=np.copy(avgtexerrlist)#[x/2 for x in avgtexerrlist]
upperfill=radialmaxtex#list( map(add,avgtexlist,fillwidth))#radialmaxtex
lowerfill=radialmintex#list( map(sub,avgtexlist,fillwidth))#radialmintex#
massestosum=[]
masserrtoprop=[]
lumstosum=[]
lumerrtoprop=[]
nh2tomean=[]
nh2errortomean=[]
#pdb.set_trace()
if source == 'SgrB2S':#Selects masses,luminosities, nh2s, distances, and temperatures for use in radial plot
#wcsobj=WCS(smooth_trotfits[0].header)
#regs = regions.Regions.read('/blue/adamginsburg/d.jeff/imaging_results/regfiles/roughsgrb2smassregion_ignoresHIIregion.reg')
#pixreg = regs[0].to_pixel(wcsobj)
#pixmask = pixreg.to_mask()
#err_mdata = pixmask.cutout(h2masserr)
#dat_mdata=pixmask.cutout(h2mass)
#masserrtoprop.append(pixmask.get_values(h2masserr))#propmasserr=np.sqrt(np.nansum(np.square(pixmask.get_values(h2masserrmap))))
#massestosum.append(pixmask.get_values(h2mass))#sgrb2smass=np.nansum(pixmask.get_values(h2massmap))
#lumstosum.append(pixmask.get_values(lums))
#lumerrtoprop.append(pixmask.get_values(lumserr))
#nh2tomean.append(pixmask.get_values(nh2s.value))
#nh2errortomean.append(pixmask.get_values(nh2s_error))
#nh2snrinradius=list(pixmask.get_values(nh2s/nh2s_error))
#premask_tex=np.copy(texinradius)
#texinradius=list(pixmask.get_values(texmapdata.value))
rr2_sgrb2s=centrtopix#(rr2*pixtophysicalsize).value#list(pixmask.get_values(rr2*pixtophysicalsize).value)#rr2 and not rr here?
'''
xx_sgrb2s=[]
yy_sgrb2s=[]
for why in yinradius:
for ex in xinradius:
if regions.PixCoord(why,ex) in pixreg:
xx_sgrb2s.append(ex)
yy_sgrb2s.append(why)
else:
pass
'''
#premask_abuns=np.copy(abundinradius)
#abundinradius=list(pixmask.get_values(abunds))
#abundsnrinradius=list(pixmask.get_values(snr_abund))
trotsforabunds=texinradius#list(pixmask.get_values(texmapdata.value))
#pdb.set_trace()
#print(f'New error: {propmasserr}')
#else:
onlytexabund=False
if onlytexabund:
if source == 'SgrB2S':
np.savetxt(f'contfix_{source}_abuns.txt',abundinradius)
np.savetxt(f'contfix_{source}_errabuns.txt',(np.array(abundinradius)/np.array(abundsnrinradius)))
np.savetxt(f'contfix_{source}_tex.txt',trotsforabunds)
np.savetxt(f'contfix_{source}_errtex.txt',(texerrinradius))
print('Done')
sys.exit()
else:
np.savetxt(f'contfix_{source}_abuns.txt',abundinradius)
np.savetxt(f'contfix_{source}_errabuns.txt',(np.array(abundinradius)/np.array(abundsnrinradius)))
np.savetxt(f'contfix_{source}_tex.txt',texinradius)
np.savetxt(f'contfix_{source}_errtex.txt',(texerrinradius))
print('Done')
sys.exit()
for data2 in teststack:
if data2[0] <= edge:
massestosum.append(data2[1])
masserrtoprop.append(data2[8])
lumstosum.append(data2[3])
lumerrtoprop.append(data2[7])
nh2tomean.append(data2[4])
nh2errortomean.append(data2[5])
else:
break
masssum=np.nansum(massestosum)
propmasserr=np.sqrt(np.nansum(np.square(masserrtoprop)))*np.sqrt(pixperbeam)#np.sum(masserrtoprop)
lumsum=np.nansum(lumstosum)
proplumerr=np.sqrt(np.nansum(np.square(lumerrtoprop)))*np.sqrt(pixperbeam)#np.sum(lumerrtoprop)
nh2mean=np.nanmean(nh2tomean)
nh2errormean=np.nanmean(nh2errortomean)
powerlaw_normpairs={'SgrB2S':(275,3500),'DSi':(210,3500),'DSii':(130,5000),'DSiii':(150,3000),'DSiv':(150,4500),'DSv':(160,2000),'DSVI':(130,4000),'DSVII':(200,2000),'DSVIII':(75,5000),'DSIX':(160,2500)}#7-75,4000
powerlawpair=powerlaw_normpairs[source]
fiducial_index=0.75
fiducial_norm=powerlawpair[0]*(powerlawpair[1]/pixtophysicalsize)**fiducial_index
lowerbound_initialguess={'SgrB2S':0.25,'DSi':0.25,'DSii':0.1,'DSiii':0.25,'DSiv':0.25,'DSv':0.25,'DSVI':0.25,'DSVII':0.25,'DSVIII':0.25,'DSIX':0.25}
bpl_alpha2_initialguess={'SgrB2S':0.25,'DSi':0.5,'DSii':0.5,'DSiii':0.25,'DSiv':0.25,'DSv':0.25,'DSVI':0.25,'DSVII':0.25,'DSVIII':0.25,'DSIX':0.25}
if source == 'DSVII':
inputamp=150
elif source == 'DSIX':
inputamp=100
elif source == 'SgrB2S':
inputamp=300
#elif source == 'DSv':
# inputamp=250
else:
inputamp=100
fitter=fitting.LevMarLSQFitter()
fitter2=fitting.LevMarLSQFitter()
base_bpl=powerlaws.BrokenPowerLaw1D(amplitude=inputamp,x_break=1000,alpha_1=-1,alpha_2=bpl_alpha2_initialguess[source])#lowerbound_initialguess[source])#amp=150,xbreak=1500 for ds7
base_spl=powerlaws.PowerLaw1D(amplitude=np.mean(radialdensitylist[1:]))
if source=='DSIX':
innerradius=9
outerradius=len(listordered_centrtopix)-1#None
elif source=='DSiv':
innerradius=1
outerradius=197
elif source=='DSVII':
innerradius=1
outerradius=None
else:
innerradius=1
outerradius=None
radiustofit=listordered_centrtopix[innerradius:outerradius]
textofit=avgtexlist[innerradius:outerradius]
texerrtofit=avgtexerrlist[innerradius:outerradius]
weightstofit=avginversesigma[innerradius:outerradius]
denstofit=radialdensitylist[innerradius:outerradius]#[innerradius:outerradius]
densweightstofit=1/(np.array(err_radialdens[innerradius:outerradius]))
popt,pcov=cf(powerlaw_profile,radiustofit,textofit,sigma=texerrtofit,bounds=([0,lowerbound_initialguess[source]],[1000,1.25]))#[1:197] for ds4 (some nans may be present further out),[5:] for ds7, [9:] for ds9
fit_pl=fitter(base_bpl,radiustofit,textofit,weights=weightstofit)
perr=np.sqrt(np.diag(fitter.fit_info['param_cov']))
if source == 'DSiv'or 'DSv':
fit_dens=fitter2(base_spl,radiustofit[:(len(radiustofit)-1)],denstofit[:(len(radiustofit)-1)],weights=densweightstofit[:(len(radiustofit)-1)])
else:
fit_dens=fitter2(base_spl,radiustofit,denstofit,weights=densweightstofit)
derr=np.sqrt(np.diag(fitter2.fit_info['param_cov']))
print(f'Sum: {masssum} +/- {propmasserr} Msun')
print(f'Core radius: {edge} +/- {cntmbmajtoAU/2}')
print(f'Core luminosity: {lumsum} +/- {proplumerr} Lsun')
print(f'Average H2 column in {edge} AU radius: {nh2mean} +/- {nh2errormean}')
plottexmax=np.nanmax(lookformax)+10
maxtexindex=np.where(lookformax==np.nanmax(lookformax))
maxtexerror=lookformax_err[maxtexindex]
print(f'Max Tex: {np.max(lookformax)} +/- {float(maxtexerror)} K')
#copy_centrtopix=np.copy(centrtopix)*u.AU
copy_centrtopix=np.copy(listordered_centrtopix)#np.linspace(0,r_phys.value,num=len(avgtexlist))*u.AU
#copy_centrtopix.sort()
lineartex=[]
quadrtex=[]
sublinhalftex=[]
sublinmidtex=[]
fittedtex=[]
#pdb.set_trace()
for dist in copy_centrtopix:
lineartex.append(linear_profile(dist).value)
quadrtex.append(quadratic_profile(dist).value)
sublinhalftex.append(sublinear_profile(dist).value)
sublinmidtex.append(submid_profile(dist).value)
fittedtex.append((popt[0]*((dist/pixtophysicalsize.value)**-popt[1])))#.value)
#pdb.set_trace()
plt.rcParams["figure.dpi"]=150
sourcenamesfortable={'SgrB2S':'SgrB2S','DSi':'DS1','DSii':'DS2','DSiii':'DS3','DSiv':'DS4','DSv':'DS5','DSVI':'DS6','DSVII':'DS7','DSVIII':'DS8','DSIX':'DS9'}
densalpha=fit_dens.alpha.value
errdensalpha=round_to_1(derr[2])
onlydens=False
plt.figure()
if source == 'DSiv':
plt.errorbar(listordered_centrtopix,radialdensitylist,yerr=err_radialdens,label='Data',fmt='o')
plt.plot(listordered_centrtopix,fit_dens(listordered_centrtopix),label=f'$p$={round(densalpha,(len(str(errdensalpha))-2))} \u00B1 {errdensalpha}',zorder=5)
plt.axvline(edge,ls='--',label='$R_{core}$',color='black')
plt.yscale('log')
plt.xlabel('$r$ (AU)',fontsize=14)
plt.ylabel('$n$ (cm$^{-3}$)',fontsize=14)
plt.legend()
plt.show()
else:
plt.errorbar(listordered_centrtopix,radialdensitylist,yerr=err_radialdens,label='Data',fmt='o')
plt.plot(listordered_centrtopix,fit_dens(listordered_centrtopix),label=f'$p$={round(densalpha,(len(str(errdensalpha))-2))} \u00B1 {errdensalpha}',zorder=5)
plt.axvline(edge,ls='--',label='$R_{core}$',color='black')
plt.yscale('log')
plt.xlabel('$r$ (AU)',fontsize=14)
plt.ylabel('$n$ (cm$^{-3}$)',fontsize=14)
plt.legend()
densplotpath=figpath+'contsanitycheck_densityprofile_trotntotbootmasked.png'
print(f'\nSaving to {densplotpath}')
plt.savefig(densplotpath,overwrite=True)
plt.show()
densityslopepath='contsanitycheck_densityslopes_bootmasked.fits'
if os.path.exists(densityslopepath):
dtable=QTable.read(densityslopepath)
if densalpha in dtable['density_alpha']:
print(f'alpha value {densalpha} already exists in table.')
else:
print(f'Appending alpha {densalpha} +/- {errdensalpha} to table.')
densalpha=[densalpha,errdensalpha]
preinsert=QTable(rows=[densalpha],names=['density_alpha','err_densityalpha'])
densstack=vstack([dtable,preinsert])
print('Appending complete.')
#pdb.set_trace()
print(f'Saving to {densityslopepath}')
densstack.write(densityslopepath,overwrite=True)
print('Done')
else:
print('No density table found')
print('Creating density table')
densalpha=[densalpha,errdensalpha]
dtable=QTable(rows=[densalpha],names=['density_alpha','err_densityalpha'])
print('Table created')
print(f'Writing to {densityslopepath}')
dtable.write(densityslopepath)
print('Done')
if onlydens:
sys.exit()
else:
pass
onlyradabun=True
if source == 'SgrB2S':
plt.figure()
plt.scatter(trotsforabunds,abundinradius,s=5,c=nh2inradius,norm=mpl.colors.LogNorm())
#plt.yscale('log')
plt.xlabel('$T_{rot}$ (K)',fontsize=14)
plt.ylabel('X(CH$_3$OH)',fontsize=14)
plt.xlim(xmax=plottexmax)
#plt.colorbar(pad=0,label='Luminosity (Lsun)')
plt.colorbar(pad=0,label='N(H$_2$) (cm$^{-2}$)')#'N(CH$_3$OH) (cm$^{-2}$)')##
figsavepath=figpath+f'texabundiag_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
#pdb.set_trace()
plt.savefig(figsavepath,bbox_inches='tight',overwrite=True)
plt.show()
plt.figure()
plt.scatter(listordered_centrtopix,radialabun,s=5,)#c=nh2inradius,norm=mpl.colors.LogNorm())#abundinradius
plt.yscale('log')
plt.xlabel('$r$ (AU)',fontsize=14)
plt.ylabel('X(CH$_3$OH)',fontsize=14)
plt.colorbar(pad=0,label='N(H$_2$) (cm$^{-2}$)')#'T$_K$ (K)')
figsavepath=figpath+f'real_radialavgabundiag_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
#pdb.set_trace()
plt.savefig(figsavepath,bbox_inches='tight',overwrite=True)
plt.show()
savetxt=np.array([listordered_centrtopix,radialabun])
np.savetxt(f'{source}_radialavgabun.txt',savetxt)
if onlyradabun:
sys.exit()
plt.figure()
plt.scatter(rr2_sgrb2s,nh2inradius,s=5,c=texinradius,vmax=plottexmax,cmap='inferno')
plt.yscale('log')
plt.xlabel('$r$ (AU)',fontsize=14)
plt.ylabel('N(H$_2$) (cm$^{-2}$)',fontsize=14)
plt.colorbar(pad=0,label='T$_{rot}$ (K)')#'T$_K$ (K)')
figsavepath=figpath+f'radialavgnh2s_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
#pdb.set_trace()
plt.savefig(figsavepath,bbox_inches='tight',overwrite=True)
plt.show()
else:
plt.figure()
plt.scatter(texinradius,abundinradius,s=5,c=nh2inradius,norm=mpl.colors.LogNorm())
plt.yscale('log')
plt.xlabel('$T_{rot}$ (K)',fontsize=14)
plt.ylabel('X(CH$_3$OH)',fontsize=14)
plt.xlim(xmax=plottexmax)
#plt.colorbar(pad=0,label='Luminosity (Lsun)')
plt.colorbar(pad=0,label='N(H$_2$) (cm$^{-2}$)')#'N(CH$_3$OH) (cm$^{-2}$)')##
figsavepath=figpath+f'texabundiag_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
plt.savefig(figsavepath,bbox_inches='tight',overwrite=True)
plt.show()
plt.figure()
plt.scatter(listordered_centrtopix,radialabun,s=5)#,c=nh2inradius,norm=mpl.colors.LogNorm())#abundinradius
plt.yscale('log')
plt.xlabel('$r$ (AU)',fontsize=14)
plt.ylabel('X(CH$_3$OH)',fontsize=14)
#plt.colorbar(pad=0,label='N(H$_2$) (cm$^{-2}$)')#'T$_K$ (K)')
figsavepath=figpath+f'real_radialavgabundiag_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
plt.savefig(figsavepath,bbox_inches='tight',overwrite=True)
plt.show()
savetxt=np.array([listordered_centrtopix,radialabun])
np.savetxt(f'{source}_radialavgabun.txt',savetxt)
if onlyradabun:
sys.exit()
plt.figure()
plt.scatter(centrtopix,nh2inradius,s=5,c=texinradius,vmax=plottexmax,cmap='inferno')
plt.yscale('log')
plt.xlabel('$r$ (AU)',fontsize=14)
plt.ylabel('N(H$_2$) (cm$^{-2}$)',fontsize=14)
plt.colorbar(pad=0,label='T$_{rot}$ (K)')#'T$_K$ (K)')
figsavepath=figpath+f'radialavgnh2s_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
plt.savefig(figsavepath,bbox_inches='tight',overwrite=True)
plt.show()
fig=plt.figure()#figsize=(14,7))
spec = gridspec.GridSpec(ncols=1, nrows=2, wspace=0.5,
hspace=.0, height_ratios=[2, 0.5])
ax0=fig.add_subplot(spec[0])
ax1=fig.add_subplot(spec[1],sharex=ax0)
residual_bpl=list( map(sub,avgtexlist,fit_pl(listordered_centrtopix)))
residual_spl=list( map(sub,avgtexlist,fittedtex))
avgsnr=np.array(list( map(truediv,avgtexlist,avgtexerrlist)))
avgsnrforplot=avgsnr/2
ax1.axhline(y=0,ls='--',color='black')
if source == 'DSiv':
ax1.plot(copy_centrtopix[:197],residual_spl[:197],color='orange',label='single')#[:197] for ds4,[1:] for ds7
ax1.plot(copy_centrtopix[:197],residual_bpl[:197],color='red',label='broken')#[:197] for ds4,
ax0.scatter(listordered_centrtopix,avgtexlist)#[:197] for ds4
ax0.fill_between(listordered_centrtopix[:197],upperfill[:197],lowerfill[:197],alpha=0.2,color='blue')#[:197] for ds
ax0.plot(copy_centrtopix,fittedtex,color='orange',label=f'$\\alpha$={round(popt[1],2)} \u00B1 {round(pcov[1,1]**0.5,2)}',zorder=1)
ax0.plot(copy_centrtopix,fit_pl(copy_centrtopix),color='red',ls='-',zorder=2,label=f'$\\alpha_1$={round(fit_pl.alpha_1.value,2)} \u00B1 {round(perr[2],2)}\n$\\alpha_2$={round(fit_pl.alpha_2.value,2)} \u00B1 {round(perr[3],2)}\n$r_{{break}}$={round(fit_pl.x_break.value)} \u00B1 {round(perr[1])}')#[1:] for ds7
ax1.set_xlabel('$r$ (AU)',fontsize=14)
ax0.set_ylabel('T$_{rot}$ (K)',fontsize=14)
ax1.set_ylabel('Residuals',fontsize=10)
ax0.set_ylim(ymax=(max(upperfill)+30))
ax0.legend()
ax0.tick_params(direction='in')
ax0.tick_params(axis='x',labelcolor='w')
ax1.tick_params(axis='x',top=True,direction='in')
figsavepath=figpath+f'radialavgtex_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
plt.tight_layout()
plt.savefig(figsavepath,overwrite=True)
plt.show()
elif source == 'DSVII':
ax1.plot(copy_centrtopix[1:],residual_spl[1:],color='orange',label='single')#[:197] for ds4,[1:] for ds7
ax1.plot(copy_centrtopix[1:],residual_bpl[1:],color='red',label='broken')#[:197] for ds4
ax0.scatter(listordered_centrtopix,avgtexlist)#[:197] for ds4
ax0.fill_between(listordered_centrtopix,upperfill,lowerfill,alpha=0.2,color='blue')#[:197] for ds4
ax0.plot(copy_centrtopix,fittedtex,color='orange',label=f'$\\alpha$={round(popt[1],2)} \u00B1 {round(pcov[1,1]**0.5,2)}',zorder=1)
ax0.plot(copy_centrtopix[1:],fit_pl(copy_centrtopix)[1:],color='red',ls='-',zorder=2,label=f'$\\alpha_1$={round(fit_pl.alpha_1.value,2)} \u00B1 {round(perr[2],2)}\n$\\alpha_2$={round(fit_pl.alpha_2.value,2)} \u00B1 {round(perr[3],2)}\n$r_{{break}}$={round(fit_pl.x_break.value)} \u00B1 {round(perr[1])}')#[1:] for ds7
ax1.set_xlabel('$r$ (AU)',fontsize=14)
ax0.set_ylabel('T$_{rot}$ (K)',fontsize=14)
ax1.set_ylabel('Residuals',fontsize=10)
ax0.set_ylim(ymax=(max(upperfill)+30))
ax0.legend()
ax0.tick_params(direction='in')
ax0.tick_params(axis='x',labelcolor='w')
ax1.tick_params(axis='x',top=True,direction='in')
figsavepath=figpath+f'radialavgtex_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
plt.tight_layout()
plt.savefig(figsavepath,overwrite=True)
plt.show()
else:
ax1.plot(copy_centrtopix,residual_spl,color='orange',label='single')#[:197] for ds4,[1:] for ds7
ax1.plot(copy_centrtopix,residual_bpl,color='red',label='broken')#[:197] for ds4,
ax0.scatter(listordered_centrtopix,avgtexlist)#[:197] for ds4
ax0.fill_between(listordered_centrtopix,upperfill,lowerfill,alpha=0.2,color='blue')#[:197] for ds4
ax0.plot(copy_centrtopix,fittedtex,color='orange',label=f'$\\alpha$={round(popt[1],2)} \u00B1 {round(pcov[1,1]**0.5,2)}',zorder=1)
ax0.plot(copy_centrtopix,fit_pl(copy_centrtopix),color='red',ls='-',zorder=2,label=f'$\\alpha_1$={round(fit_pl.alpha_1.value,2)} \u00B1 {round(perr[2],2)}\n$\\alpha_2$={round(fit_pl.alpha_2.value,2)} \u00B1 {round(perr[3],2)}\n$r_{{break}}$={round(fit_pl.x_break.value)} \u00B1 {round(perr[1])}')#[1:] for ds7
ax1.set_xlabel('$r$ (AU)',fontsize=14)
ax0.set_ylabel('T$_{rot}$ (K)',fontsize=14)
ax1.set_ylabel('Residuals',fontsize=10)
if source == 'SgrB2S':
ax0.set_ylim(ymax=(800),ymin=100)#max(upperfill)+30),ymin=100)
else:
ax0.set_ylim(ymax=(max(upperfill)+30))
ax0.legend()
ax0.tick_params(direction='in')
ax0.tick_params(axis='x',labelcolor='w')
ax1.tick_params(axis='x',top=True,direction='in')
figsavepath=figpath+f'radialavgtex_contsanitycheck_r{r}px_rphys{int(pixtophysicalsize.value)}AU_smoothed.png'
plt.tight_layout()
plt.savefig(figsavepath,overwrite=True)
plt.show()
if source=='SgrB2S':
plt.figure()
plt.scatter(nh2inradius,ntotsinradius,s=5,c=texinradius,vmax=plottexmax,cmap='inferno')
'''
x=[min(nh2inradius),max(nh2inradius)]
y1=(9.5e-8*np.array(x))
y2=(1.5e-7*np.array(x))
y3=(5e-8*np.array(x))
plt.plot(x,np.transpose([y1,y2,y3]))
'''
plt.yscale('log')
plt.xscale('log')
plt.colorbar(pad=0,label='T$_{rot}$ (K)')
plt.xlabel('N(H$_2$) (cm$^{-2}$)')
plt.ylabel('N(CH$_3$OH) (cm$^{-2}$)')
figsavepath=figpath+'nch3ohvsnh2_contsanitycheck_smoothed.png'
plt.savefig(figsavepath,overwrite=True)
plt.show()
else:
plt.figure()
plt.scatter(nh2inradius,ntotsinradius,s=5,c=texinradius,cmap='inferno')
'''
x=[min(nh2inradius),max(nh2inradius)]
y1=(9.5e-8*np.array(x))
y2=(1.5e-7*np.array(x))
y3=(5e-8*np.array(x))
plt.plot(x,np.transpose([y1,y2,y3]))
'''
plt.yscale('log')
plt.xscale('log')
plt.colorbar(pad=0,label='T$_{rot}$ (K)')
plt.xlabel('N(H$_2$) (cm$^{-2}$)')
plt.ylabel('N(CH$_3$OH) (cm$^{-2}$)')
figsavepath=figpath+'nch3ohvsnh2_contsanitycheck_smoothed.png'
plt.savefig(figsavepath,overwrite=True)
plt.show()
'''
print(f'Norm initial guess: {fiducial_norm}')
print(f'norm error: {pcov[0,0]**0.5}')
print(f'index initial guess: {lowerbound_initialguess[source]}')
print(f'index error: {pcov[1,1]**0.5}')
'''
onlypowerlaw=True
powerlawpath='/blue/adamginsburg/d.jeff/imaging_results/SgrB2DS-CH3OH/contsanitycheck_powerlawtable_bootmasked.fits'
pwrlwprams=[(round(fit_pl.alpha_1.value,2)*u.dimensionless_unscaled),(round(perr[2],2)*u.dimensionless_unscaled),(round(fit_pl.alpha_2.value,2)*u.dimensionless_unscaled),(round(perr[3],2)*u.dimensionless_unscaled),(round(fit_pl.x_break.value)*u.AU),(round(perr[1])*u.AU)]
powerlawparams=QTable(rows=[pwrlwprams],names=['alpha_1','alpha_1 error','alpha_2','alpha_2 error','x_break','x_break error'])
if os.path.exists(powerlawpath):
print('\nStart power law table procedure')
print(f'Power law table already exists at {powerlawpath}')
pwrlwtable=QTable.read(powerlawpath)
if pwrlwprams[4] in pwrlwtable['x_break']:
print('Current parameter set already exists in table.')
#print('Exiting...')
#sys.exit()
else:
print('Appending new values')
pwrlwstack=vstack([pwrlwtable,powerlawparams])
print(f'Saving composite table to {powerlawpath}')
pwrlwstack.write(powerlawpath,overwrite=True)
print('Power law table update complete\n')
else:
print('No power law table in current directory')
if source != 'DSi':
print('Please change source to DS1 to ensure proper stack')
pdb.set_trace()
else:
print('Creating new power law table')
powerlawparams.write(powerlawpath)
print('New power law table created\n')
if onlypowerlaw:
print('Only power law parameters requested.')
print('Exiting...')
sys.exit()
else:
pass
sumtablepath=f'contsanitycheck_hotcoresummarytable_postreprojsmooth_t{trad}radius_bootmasked.fits'
if os.path.exists(sumtablepath):
print('\nUpdating summary table with new values')
sumtable=QTable.read(sumtablepath)
if sourcenamesfortable[source] in sumtable['Source']:
print(f'Data for source {source} already exists.')
sourceindex=int(np.where(sumtable['Source']==sourcenamesfortable[source])[0])
print(sumtable[sourceindex])
update=input('Overwrite? [y/n]\n')
if update=='y':
props=[sourcenamesfortable[source],(float(lookformax[maxtexindex])*u.K),(float(maxtexerror)*u.K),(nh2mean*u.cm**-2),(nh2errormean*u.cm**-2),
(masssum*u.solMass),(propmasserr*u.solMass),(lumsum*u.solLum),(proplumerr*u.solLum),(edge*u.AU),(cntmbmajtoAU/2)]
sumtable[sourceindex]=tuple(props)
print(f'{source} source properties updated.')
print(f'\nSaving at {sumtablepath}')
sumtable.write(sumtablepath,overwrite=True)
print('Update complete')
else:
print(f'{source} source properties unchanged.')
else:
print(f'Adding new source {source} to summary table.')
props=[sourcenamesfortable[source],(float(lookformax[maxtexindex])*u.K),(float(maxtexerror)*u.K),(nh2mean*u.cm**-2),(nh2errormean*u.cm**-2),
(masssum*u.solMass),(propmasserr*u.solMass),(lumsum*u.solLum),(proplumerr*u.solLum),(edge*u.AU),(cntmbmajtoAU/2)]
tempqtable=QTable(rows=[props],names=['Source','T_max','T_max_error','N(H_2) avg)','N(H_2) error','H_2 Mass','H_2 Mass error','Luminosity','Luminosity_error','Radius','Radius_error'])
outtable=vstack([sumtable,tempqtable])
print(f'{source} source properties added to table.')
print(f'\nSaving at {sumtablepath}')
outtable.write(sumtablepath,overwrite=True)
print('Update complete')
else:
newsumtable=input('Create new summary table? (y/n): ')
if 'y' == newsumtable:
print(f'Creating new summary table with {source} data')
props=[sourcenamesfortable[source],(float(lookformax[maxtexindex])*u.K),(float(maxtexerror)*u.K),(nh2mean*u.cm**-2),(nh2errormean*u.cm**-2),
(masssum*u.solMass),(propmasserr*u.solMass),(lumsum*u.solLum),(proplumerr*u.solLum),(edge*u.AU),(cntmbmajtoAU/2)]
tempqtable=QTable(rows=[props],names=['Source','T_max','T_max_error','N(H_2) avg)','N(H_2) error','H_2 Mass','H_2 Mass error','Luminosity','Luminosity_error','Radius','Radius_error'])
print(f'\nSaving at {sumtablepath}')
outtable=tempqtable
outtable.write(sumtablepath,overwrite=True)
print('New summary table created')
else:
print(f'Source {source} results not saved')
'''
edgepoints=circle(texmapdata,texpeakpix[0],texpeakpix[1],r)
plt.imshow(texmapdata.value,origin='lower',vmax=550,vmin=10)
plt.scatter(edgepoints[0],edgepoints[1],color='orange')
#plt.scatter(xinradius,yinradius,color='orange')
plt.show()
'''