File size: 48,850 Bytes
8de7e09
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
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
1001
1002
1003
1004
1005
1006
1007
1008
1009
1010
1011
1012
1013
1014
1015
1016
1017
1018
1019
1020
1021
1022
1023
1024
1025
1026
1027
1028
1029
1030
1031
1032
1033
1034
1035
1036
1037
1038
1039
1040
1041
1042
1043
1044
1045
1046
1047
1048
1049
1050
1051
1052
1053
1054
1055
1056
1057
1058
1059
1060
1061
1062
1063
1064
1065
1066
1067
1068
1069
1070
1071
1072
1073
1074
1075
1076
1077
1078
1079
1080
1081
1082
1083
1084
1085
1086
1087
1088
1089
1090
1091
1092
1093
1094
1095
1096
1097
1098
1099
1100
1101
1102
1103
1104
1105
1106
1107
1108
1109
1110
1111
1112
1113
1114
1115
1116
1117
1118
1119
1120
1121
1122
1123
1124
1125
1126
1127
1128
1129
1130
1131
1132
1133
1134
1135
1136
1137
1138
1139
1140
1141
1142
1143
1144
1145
1146
1147
1148
1149
1150
1151
1152
1153
1154
1155
1156
1157
1158
1159
1160
1161
1162
1163
1164
1165
1166
1167
1168
1169
1170
1171
1172
1173
1174
1175
1176
1177
1178
1179
1180
1181
1182
1183
1184
1185
1186
1187
1188
1189
1190
1191
1192
1193
1194
1195
1196
1197
1198
1199
1200
1201
1202
1203
1204
1205
1206
1207
1208
1209
1210
1211
1212
1213
1214
1215
1216
1217
1218
1219
1220
1221
1222
1223
1224
1225
1226
1227
1228
1229
1230
1231
1232
1233
1234
1235
1236
1237
1238
1239
1240
1241
1242
1243
1244
1245
1246
1247
1248
1249
1250
1251
1252
1253
1254
1255
1256
1257
1258
1259
1260
1261
1262
1263
1264
1265
1266
1267
1268
1269
1270
1271
1272
1273
1274
1275
1276
1277
1278
1279
1280
1281
1282
1283
1284
1285
1286
1287
1288
1289
1290
1291
1292
1293
1294
1295
1296
1297
1298
1299
1300
1301
1302
1303
1304
1305
1306
1307
1308
1309
1310
1311
1312
1313
1314
1315
1316
1317
1318
1319
1320
1321
1322
1323
1324
1325
1326
1327
1328
1329
1330
1331
1332
1333
1334
1335
1336
1337
1338
1339
1340
1341
1342
1343
1344
1345
1346
1347
1348
1349
1350
1351
1352
1353
1354
1355
1356
1357
1358
1359
1360
1361
1362
1363
1364
1365
1366
1367
1368
1369
1370
1371
1372
1373
1374
1375
1376
1377
1378
1379
1380
1381
1382
1383
1384
1385
1386
1387
1388
1389
1390
1391
1392
1393
1394
1395
1396
1397
1398
1399
1400
1401
1402
1403
1404
1405
1406
1407
1408
1409
1410
1411
1412
1413
1414
1415
1416
1417
1418
1419
1420
1421
1422
1423
1424
1425
1426
1427
1428
1429
1430
1431
1432
1433
1434
1435
1436
1437
1438
1439
1440
1441
1442
1443
1444
1445
1446
1447
1448
1449
1450
1451
1452
1453
1454
1455
1456
1457
1458
1459
1460
1461
1462
1463
1464
1465
1466
1467
1468
1469
1470
1471
1472
1473
1474
1475
1476
1477
1478
1479
1480
1481
1482
1483
1484
1485
1486
1487
1488
1489
1490
1491
1492
1493
1494
1495
1496
1497
1498
1499
1500
1501
1502
1503
1504
1505
1506
1507
1508
1509
1510
1511
1512
1513
1514
1515
1516
1517
1518
1519
1520
1521
1522
1523
1524
1525
1526
1527
1528
1529
1530
1531
1532
1533
1534
1535
1536
1537
1538
1539
1540
1541
1542
1543
1544
1545
1546
1547
1548
1549
1550
1551
1552
1553
1554
1555
1556
1557
1558
1559
1560
1561
1562
1563
1564
1565
1566
1567
1568
1569
1570
1571
1572
1573
1574
1575
1576
1577
1578
1579
1580
1581
1582
1583
1584
1585
1586
1587
1588
1589
1590
1591
1592
1593
1594
1595
1596
1597
1598
1599
1600
1601
1602
1603
1604
1605
1606
1607
1608
1609
1610
1611
1612
1613
1614
1615
1616
1617
1618
1619
1620
1621
1622
1623
1624
1625
1626
1627
1628
1629
1630
1631
1632
1633
1634
1635
1636
1637
1638
1639
1640
1641
1642
1643
1644
1645
1646
1647
1648
1649
1650
1651
1652
1653
1654
1655
1656
1657
1658
1659
1660
1661
1662
1663
1664
1665
1666
1667
1668
1669
1670
1671
1672
1673
1674
1675
1676
1677
1678
1679
1680
1681
1682
1683
1684
1685
1686
1687
1688
1689
1690
1691
1692
1693
1694
1695
1696
1697
1698
1699
1700
1701
1702
1703
1704
1705
1706
1707
1708
1709
1710
1711
1712
1713
1714
1715
1716
1717
1718
1719
1720
1721
1722
1723
1724
1725
1726
1727
1728
1729
1730
1731
1732
1733
1734
1735
1736
1737
1738
1739
1740
1741
1742
1743
1744
1745
1746
1747
1748
1749
1750
1751
1752
1753
1754
1755
1756
1757
1758
1759
1760
1761
1762
1763
1764
1765
1766
1767
1768
1769
1770
1771
1772
1773
1774
1775
1776
1777
1778
1779
1780
1781
1782
1783
1784
1785
1786
1787
1788
1789
1790
1791
1792
1793
1794
1795
1796
1797
1798
1799
1800
1801
1802
1803
1804
1805
1806
1807
1808
1809
1810
1811
1812
1813
1814
1815
1816
1817
1818
1819
1820
1821
1822
1823
1824
1825
1826
1827
1828
1829
1830
1831
1832
1833
1834
1835
1836
1837
1838
1839
1840
1841
1842
1843
1844
1845
1846
1847
1848
1849
1850
1851
1852
1853
1854
1855
1856
1857
1858
1859
1860
1861
1862
1863
1864
1865
1866
1867
1868
1869
1870
1871
1872
1873
1874
1875
1876
1877
1878
1879
1880
1881
1882
1883
1884
1885
1886
1887
1888
1889
1890
1891
1892
1893
1894
1895
1896
1897
1898
1899
1900
1901
1902
1903
1904
1905
1906
1907
1908
1909
1910
1911
1912
1913
1914
1915
1916
1917
1918
1919
1920
1921
1922
1923
1924
1925
1926
1927
1928
1929
1930
1931
1932
1933
1934
1935
1936
1937
1938
1939
1940
1941
1942
1943
1944
1945
1946
1947
1948
1949
1950
1951
1952
1953
1954
1955
1956
1957
1958
1959
1960
1961
1962
1963
1964
1965
1966
1967
1968
1969
1970
1971
1972
1973
1974
1975
1976
1977
1978
1979
1980
1981
1982
1983
1984
1985
1986
1987
1988
1989
1990
1991
1992
1993
1994
1995
1996
1997
1998
1999
2000
2001
2002
2003
2004
2005
2006
2007
2008
2009
2010
2011
2012
2013
2014
2015
2016
2017
2018
2019
2020
2021
2022
2023
2024
2025
2026
2027
2028
2029
2030
2031
2032
2033
2034
2035
2036
2037
2038
2039
2040
2041
2042
2043
2044
2045
2046
2047
2048
2049
2050
2051
2052
2053
2054
2055
2056
2057
2058
2059
2060
2061
2062
2063
2064
2065
2066
2067
2068
2069
2070
2071
2072
2073
2074
2075
2076
2077
2078
2079
2080
2081
2082
2083
2084
2085
2086
2087
2088
2089
2090
2091
2092
2093
2094
2095
2096
2097
2098
2099
2100
2101
2102
2103
2104
2105
2106
2107
2108
2109
2110
2111
2112
2113
2114
2115
2116
2117
2118
2119
2120
2121
2122
2123
2124
2125
2126
2127
2128
2129
2130
2131
2132
2133
2134
2135
2136
2137
2138
2139
2140
2141
2142
2143
2144
2145
2146
2147
2148
2149
2150
2151
2152
2153
2154
2155
2156
2157
2158
2159
2160
2161
2162
2163
2164
2165
2166
2167
2168
2169
2170
2171
2172
2173
2174
2175
2176
2177
2178
2179
2180
2181
2182
2183
2184
2185
2186
2187
2188
2189
2190
2191
2192
2193
2194
2195
2196
2197
2198
2199
2200
2201
2202
2203
2204
2205
2206
2207
2208
2209
2210
2211
2212
2213
2214
2215
2216
2217
2218
2219
2220
2221
2222
2223
2224
2225
2226
2227
2228
2229
2230
2231
2232
2233
2234
2235
2236
2237
2238
2239
2240
2241
2242
2243
2244
2245
2246
2247
2248
2249
2250
2251
2252
2253
2254
2255
2256
2257
2258
2259
2260
2261
2262
2263
2264
2265
2266
2267
2268
2269
2270
2271
2272
2273
2274
2275
2276
2277
2278
2279
2280
2281
2282
2283
2284
2285
2286
2287
2288
2289
2290
2291
2292
2293
2294
2295
2296
2297
2298
2299
2300
2301
2302
2303
2304
2305
2306
2307
2308
2309
2310
2311
2312
2313
2314
2315
2316
2317
2318
2319
2320
2321
2322
2323
2324
2325
2326
2327
2328
2329
2330
2331
2332
2333
2334
2335
2336
2337
2338
2339
2340
2341
2342
2343
2344
2345
2346
2347
2348
2349
2350
2351
2352
2353
2354
2355
2356
2357
2358
2359
2360
2361
2362
2363
2364
2365
2366
2367
2368
2369
2370
2371
2372
2373
2374
2375
2376
2377
2378
2379
2380
2381
2382
2383
2384
2385
2386
2387
2388
2389
2390
2391
2392
2393
2394
2395
2396
2397
2398
2399
2400
2401
2402
2403
2404
2405
2406
2407
2408
2409
2410
2411
2412
2413
2414
2415
2416
2417
2418
2419
2420
2421
2422
2423
2424
2425
1
00:00:08,370 --> 00:00:13,950
Today, inshallah, we'll start chapter six. Chapter

2
00:00:13,950 --> 00:00:20,350
six talks about the normal distribution. In this

3
00:00:20,350 --> 00:00:24,810
chapter, there are mainly two objectives. The

4
00:00:24,810 --> 00:00:30,470
first objective is to compute probabilities from

5
00:00:30,470 --> 00:00:34,530
normal distribution. And mainly we'll focus on

6
00:00:34,530 --> 00:00:37,270
objective number one. So we are going to use

7
00:00:37,270 --> 00:00:40,290
normal distribution in this chapter. And we'll

8
00:00:40,290 --> 00:00:43,830
know how can we compute probabilities if the data

9
00:00:43,830 --> 00:00:46,810
set is normally distributed. You know many times

10
00:00:46,810 --> 00:00:50,690
you talked about extreme points or outliers. So

11
00:00:50,690 --> 00:00:54,490
that means if the data has outliers, that is the

12
00:00:54,490 --> 00:00:57,290
distribution is not normally distributed. Now in

13
00:00:57,290 --> 00:01:01,090
this case, If the distribution is normal, how can

14
00:01:01,090 --> 00:01:04,350
we compute probabilities underneath the normal

15
00:01:04,350 --> 00:01:10,030
curve? The second objective is to use the normal

16
00:01:10,030 --> 00:01:13,210
probability plot to determine whether a set of

17
00:01:13,210 --> 00:01:18,150
data is approximately normally distributed. I mean

18
00:01:18,150 --> 00:01:25,550
beside box plots we discussed before. Beside this

19
00:01:25,550 --> 00:01:30,190
score, how can we tell if the data point or

20
00:01:30,190 --> 00:01:35,350
actually the entire distribution is approximately

21
00:01:35,350 --> 00:01:39,410
normally distributed or not. Before we learn if

22
00:01:39,410 --> 00:01:44,110
the point is outlier by using backsplot and this

23
00:01:44,110 --> 00:01:46,750
score. In this chapter we'll know how can we

24
00:01:46,750 --> 00:01:51,630
determine if the entire distribution is

25
00:01:51,630 --> 00:01:54,770
approximately normal distributed. So there are two

26
00:01:54,770 --> 00:01:56,710
objectives. One is to compute probabilities

27
00:01:56,710 --> 00:01:59,370
underneath the normal curve. The other, how can we

28
00:01:59,370 --> 00:02:05,310
tell if the data set is out or not? If you

29
00:02:05,310 --> 00:02:09,330
remember, first class, we mentioned something

30
00:02:09,330 --> 00:02:13,130
about data types. And we said data has mainly two

31
00:02:13,130 --> 00:02:17,930
types. Numerical data, I mean quantitative data.

32
00:02:18,690 --> 00:02:22,630
and categorical data, qualitative. For numerical

33
00:02:22,630 --> 00:02:26,190
data also it has two types, continuous and

34
00:02:26,190 --> 00:02:30,430
discrete. And discrete takes only integers such as

35
00:02:30,430 --> 00:02:35,310
number of students who take this class or number

36
00:02:35,310 --> 00:02:40,190
of accidents and so on. But if you are talking

37
00:02:40,190 --> 00:02:45,320
about Age, weight, scores, temperature, and so on.

38
00:02:45,560 --> 00:02:49,260
It's continuous distribution. For this type of

39
00:02:49,260 --> 00:02:53,320
variable, I mean for continuous distribution, how

40
00:02:53,320 --> 00:02:56,300
can we compute the probabilities underneath the

41
00:02:56,300 --> 00:02:59,640
normal? So normal distribution maybe is the most

42
00:02:59,640 --> 00:03:02,380
common distribution in statistics, and it's type

43
00:03:02,380 --> 00:03:07,820
of continuous distribution. So first, let's define

44
00:03:07,820 --> 00:03:12,010
continuous random variable. maybe because for

45
00:03:12,010 --> 00:03:15,230
multiple choice problem you should know the

46
00:03:15,230 --> 00:03:19,110
definition of continuous random variable is a

47
00:03:19,110 --> 00:03:22,070
variable that can assume any value on a continuous

48
00:03:23,380 --> 00:03:27,020
it can assume any uncountable number of values. So

49
00:03:27,020 --> 00:03:31,080
it could be any number in an interval. For

50
00:03:31,080 --> 00:03:35,720
example, suppose your ages range between 18 years

51
00:03:35,720 --> 00:03:39,580
and 20 years. So maybe someone of you, their age

52
00:03:39,580 --> 00:03:44,000
is about 18 years, three months. Or maybe your

53
00:03:44,000 --> 00:03:47,580
weight is 70 kilogram point five, and so on. So

54
00:03:47,580 --> 00:03:49,780
it's continuous on the variable. Other examples

55
00:03:49,780 --> 00:03:53,140
for continuous, thickness of an item. For example,

56
00:03:53,740 --> 00:03:54,440
the thickness.

57
00:03:58,260 --> 00:04:02,490
This one is called thickness. Now, the thickness

58
00:04:02,490 --> 00:04:05,930
may be 2 centimeters or 3 centimeters and so on,

59
00:04:06,210 --> 00:04:09,730
but it might be 2.5 centimeters. For example, for

60
00:04:09,730 --> 00:04:13,030
this remote, the thickness is 2.5 centimeters or 2

61
00:04:13,030 --> 00:04:16,510
.6, not exactly 2 or 3. So it could be any value.

62
00:04:16,650 --> 00:04:19,450
Range is, for example, between 2 centimeters and 3

63
00:04:19,450 --> 00:04:23,010
centimeters. So from 2 to 3 is a big range because

64
00:04:23,010 --> 00:04:25,670
it can take anywhere from 2.1 to 2.15 and so on.

65
00:04:26,130 --> 00:04:28,810
So thickness is an example of continuous random

66
00:04:28,810 --> 00:04:31,190
variable. Another example, time required to

67
00:04:31,190 --> 00:04:36,010
complete a task. Now suppose you want to do an

68
00:04:36,010 --> 00:04:39,710
exercise. Now the time required to finish or to

69
00:04:39,710 --> 00:04:45,150
complete this task may be any value between 2

70
00:04:45,150 --> 00:04:48,730
minutes up to 3 minutes. So maybe 2 minutes 30

71
00:04:48,730 --> 00:04:52,150
seconds, 2 minutes 40 seconds and so on. So it's

72
00:04:52,150 --> 00:04:55,550
continuous random variable. Temperature of a

73
00:04:55,550 --> 00:05:00,140
solution. height, weight, ages, and so on. These

74
00:05:00,140 --> 00:05:03,720
are examples of continuous random variable. So

75
00:05:03,720 --> 00:05:08,040
these variables can potentially take on any value

76
00:05:08,040 --> 00:05:11,340
depending only on the ability to precisely and

77
00:05:11,340 --> 00:05:14,020
accurately measure. So that's the definition of

78
00:05:14,020 --> 00:05:17,320
continuous random variable. Now, if you look at

79
00:05:17,320 --> 00:05:21,810
the normal distribution, It looks like bell

80
00:05:21,810 --> 00:05:25,990
-shaped, as we discussed before. So it's bell

81
00:05:25,990 --> 00:05:31,270
-shaped, symmetrical. Symmetrical means the area

82
00:05:31,270 --> 00:05:34,390
to the right of the mean equals the area to the

83
00:05:34,390 --> 00:05:37,950
left of the mean. I mean 50% of the area above and

84
00:05:37,950 --> 00:05:41,770
50% below. So that's the meaning of symmetrical.

85
00:05:42,490 --> 00:05:46,370
The other feature of normal distribution, the

86
00:05:46,370 --> 00:05:49,510
measures of center tendency are equal or

87
00:05:49,510 --> 00:05:53,170
approximately equal. Mean, median, and mode are

88
00:05:53,170 --> 00:05:55,530
roughly equal. In reality, they are not equal,

89
00:05:55,650 --> 00:05:58,210
exactly equal, but you can say they are

90
00:05:58,210 --> 00:06:01,850
approximately equal. Now, there are two parameters

91
00:06:01,850 --> 00:06:05,750
describing the normal distribution. One is called

92
00:06:05,750 --> 00:06:10,820
the location parameter. location, or central

93
00:06:10,820 --> 00:06:13,800
tendency, as we discussed before, location is

94
00:06:13,800 --> 00:06:17,160
determined by the mean mu. So the first parameter

95
00:06:17,160 --> 00:06:20,340
for the normal distribution is the mean mu. The

96
00:06:20,340 --> 00:06:24,240
other parameter measures the spread of the data,

97
00:06:24,280 --> 00:06:27,680
or the variability of the data, and the spread is

98
00:06:27,680 --> 00:06:31,860
sigma, or the variation. So we have two

99
00:06:31,860 --> 00:06:36,770
parameters, mu and sigma. The random variable in

100
00:06:36,770 --> 00:06:39,930
this case can take any value from minus infinity

101
00:06:39,930 --> 00:06:44,270
up to infinity. So random variable in this case

102
00:06:44,270 --> 00:06:50,310
continuous ranges from minus infinity all the way

103
00:06:50,310 --> 00:06:55,100
up to infinity. I mean from this point here up to

104
00:06:55,100 --> 00:06:58,380
infinity. So the values range from minus infinity

105
00:06:58,380 --> 00:07:02,080
up to infinity. And if you look here, the mean is

106
00:07:02,080 --> 00:07:05,600
located nearly in the middle. And mean and median

107
00:07:05,600 --> 00:07:10,820
are all approximately equal. That's the features

108
00:07:10,820 --> 00:07:14,740
or the characteristics of the normal distribution.

109
00:07:16,460 --> 00:07:20,360
Now, how can we compute the probabilities under

110
00:07:20,360 --> 00:07:25,840
the normal killer? The formula that is used to

111
00:07:25,840 --> 00:07:29,220
compute the probabilities is given by this one. It

112
00:07:29,220 --> 00:07:33,560
looks complicated formula because we have to use

113
00:07:33,560 --> 00:07:36,040
calculus in order to determine the area underneath

114
00:07:36,040 --> 00:07:40,120
the cube. So we are looking for something else. So

115
00:07:40,120 --> 00:07:45,300
this formula is it seems to be complicated. It's

116
00:07:45,300 --> 00:07:49,600
not hard but it's complicated one, but we can use

117
00:07:49,600 --> 00:07:52,380
it. If we know calculus very well, we can use

118
00:07:52,380 --> 00:07:55,240
integration to create the probabilities underneath

119
00:07:55,240 --> 00:07:58,900
the curve. But for our course, we are going to

120
00:07:58,900 --> 00:08:04,460
skip this formula because this

121
00:08:04,460 --> 00:08:09,340
formula depends actually on mu and sigma. A mu can

122
00:08:09,340 --> 00:08:13,110
take any value. Sigma also can take any value.

123
00:08:13,930 --> 00:08:17,310
That means we have different normal distributions.

124
00:08:18,470 --> 00:08:23,830
Because the distribution actually depends on these

125
00:08:23,830 --> 00:08:27,610
two parameters. So by varying the parameters mu

126
00:08:27,610 --> 00:08:29,790
and sigma, we obtain different normal

127
00:08:29,790 --> 00:08:32,710
distributions. Since we have different mu and

128
00:08:32,710 --> 00:08:36,310
sigma, it means we should have different normal

129
00:08:36,310 --> 00:08:38,770
distributions. For this reason, it's very

130
00:08:38,770 --> 00:08:43,430
complicated to have tables or probability tables

131
00:08:43,430 --> 00:08:46,010
in order to determine these probabilities because

132
00:08:46,010 --> 00:08:50,130
there are infinite values of mu and sigma maybe

133
00:08:50,130 --> 00:08:57,750
your edges the mean is 19. Sigma is, for example,

134
00:08:57,910 --> 00:09:01,990
5. For weights, maybe the mean is 70 kilograms,

135
00:09:02,250 --> 00:09:04,990
the average is 10. For scores, maybe the average

136
00:09:04,990 --> 00:09:08,710
is 65, the mean is 20, sigma is 20, and so on. So

137
00:09:08,710 --> 00:09:11,090
we have different values of mu and sigma. For this

138
00:09:11,090 --> 00:09:13,650
reason, we have different normal distributions.

139
00:09:18,490 --> 00:09:25,740
Because changing mu shifts the distribution either

140
00:09:25,740 --> 00:09:29,640
left or to the right. So maybe the mean is shifted

141
00:09:29,640 --> 00:09:32,440
to the right side, or the mean maybe shifted to

142
00:09:32,440 --> 00:09:37,140
the left side. Also, changing sigma, sigma is the

143
00:09:37,140 --> 00:09:40,660
distance between the mu and the curve. The curve

144
00:09:40,660 --> 00:09:45,220
is the points, or the data values. Now this sigma

145
00:09:45,220 --> 00:09:48,380
can be increases or decreases. So if sigma

146
00:09:48,380 --> 00:09:52,860
increases, it means the spread also increases. Or

147
00:09:52,860 --> 00:09:55,780
if sigma decreases, also the spread will decrease.

148
00:09:56,200 --> 00:09:59,660
So the distribution or the normal distribution

149
00:09:59,660 --> 00:10:02,820
depends actually on these two values. For this

150
00:10:02,820 --> 00:10:05,120
reason, since we have too many values or infinite

151
00:10:05,120 --> 00:10:07,600
values of mu and sigma, then in this case we have

152
00:10:07,600 --> 00:10:14,500
different normal distributions. There is another

153
00:10:14,500 --> 00:10:16,940
distribution. It's called standardized normal.

154
00:10:20,330 --> 00:10:26,070
Now, we have normal distribution X, and how can we

155
00:10:26,070 --> 00:10:31,930
transform from normal distribution to standardized

156
00:10:31,930 --> 00:10:35,310
normal distribution? The reason is that the mean

157
00:10:35,310 --> 00:10:40,310
of Z, I mean, Z is used for standardized normal.

158
00:10:40,850 --> 00:10:44,490
The mean of Z is always zero, and sigma is one.

159
00:10:45,770 --> 00:10:48,150
Now it's a big difference. The first one has

160
00:10:48,150 --> 00:10:53,160
infinite values of Mu and Sigma. Now, for the

161
00:10:53,160 --> 00:10:56,200
standardized normal distribution, the mean is

162
00:10:56,200 --> 00:11:01,540
fixed value. The mean is zero, Sigma is one. So,

163
00:11:01,620 --> 00:11:04,340
the question is, how can we actually transform

164
00:11:04,340 --> 00:11:09,720
from X, which has normal distribution, to Z, which

165
00:11:09,720 --> 00:11:13,160
has standardized normal with mean zero and Sigma

166
00:11:13,160 --> 00:11:23,330
of one. Let's see. How can we translate x which

167
00:11:23,330 --> 00:11:27,510
has normal distribution to z that has standardized

168
00:11:27,510 --> 00:11:32,190
normal distribution? The idea is you have just to

169
00:11:32,190 --> 00:11:39,170
subtract mu of x, x minus mu, then divide this

170
00:11:39,170 --> 00:11:43,150
result by sigma. So we just subtract the mean of

171
00:11:43,150 --> 00:11:49,660
x. and dividing by its standard deviation now so

172
00:11:49,660 --> 00:11:52,360
if we have x which has normal distribution with

173
00:11:52,360 --> 00:11:55,940
mean mu and standard deviation sigma to transform

174
00:11:55,940 --> 00:12:00,960
or to convert to z score use this formula x minus

175
00:12:00,960 --> 00:12:05,220
the mean then divide by its standard deviation now

176
00:12:05,220 --> 00:12:09,090
all of the time we are going to use z for

177
00:12:09,090 --> 00:12:12,230
standardized normal distribution and always z has

178
00:12:12,230 --> 00:12:15,370
mean zero and all and sigma or standard deviation.

179
00:12:16,250 --> 00:12:20,170
So the z distribution always has mean of zero and

180
00:12:20,170 --> 00:12:25,490
sigma of one. So that's the story of standardizing

181
00:12:25,490 --> 00:12:33,070
the normal value. Now the Formula for this score

182
00:12:33,070 --> 00:12:37,570
becomes better than the first one, but still we

183
00:12:37,570 --> 00:12:40,570
have to use calculus in order to determine the

184
00:12:40,570 --> 00:12:45,710
probabilities under the standardized normal k. But

185
00:12:45,710 --> 00:12:49,470
this distribution has mean of zero and sigma of

186
00:12:49,470 --> 00:12:56,910
one. So we have a table on page 570. Look at page

187
00:12:56,910 --> 00:13:00,910
570. We have table or actually there are two

188
00:13:00,910 --> 00:13:05,010
tables. One for negative value of Z and the other

189
00:13:05,010 --> 00:13:08,830
for positive value of Z. So we have two tables for

190
00:13:08,830 --> 00:13:14,730
positive and negative values of Z on page 570 and

191
00:13:14,730 --> 00:13:15,470
571.

192
00:13:17,870 --> 00:13:22,770
Now the table on page 570 looks like this one. The

193
00:13:22,770 --> 00:13:26,610
table you have starts from minus 6, then minus 5,

194
00:13:26,750 --> 00:13:32,510
minus 4.5, and so on. Here we start from minus 3.4

195
00:13:32,510 --> 00:13:38,850
all the way down up to 0. Look here, all the way

196
00:13:38,850 --> 00:13:44,490
up to 0. So these scores here. Also we have 0.00,

197
00:13:44,610 --> 00:13:51,880
0.01, up to 0.09. Also, the other page, page 571,

198
00:13:52,140 --> 00:13:56,940
gives the area for positive z values. Here we have

199
00:13:56,940 --> 00:14:01,760
0.0, 0.1, 0.2, all the way down up to 3.4 and you

200
00:14:01,760 --> 00:14:05,920
have up to 6. Now let's see how can we use this

201
00:14:05,920 --> 00:14:11,020
table to compute the probabilities underneath the

202
00:14:11,020 --> 00:14:12,460
normal curve.

203
00:14:14,940 --> 00:14:19,190
First of all, you have to know that Z has mean

204
00:14:19,190 --> 00:14:23,750
zero, standard deviation of one. And the values

205
00:14:23,750 --> 00:14:26,610
could be positive or negative. Values above the

206
00:14:26,610 --> 00:14:32,850
mean, zero, have positive Z values. The other one,

207
00:14:32,910 --> 00:14:36,690
values below the mean, have negative Z values. So

208
00:14:36,690 --> 00:14:42,770
Z score can be negative or positive. Now this is

209
00:14:42,770 --> 00:14:46,530
the formula we have, z equals x minus mu divided

210
00:14:46,530 --> 00:14:46,990
by six.

211
00:14:52,810 --> 00:15:01,170
Now this value could be positive if x is above the

212
00:15:01,170 --> 00:15:04,810
mean, as we mentioned before. It could be a

213
00:15:04,810 --> 00:15:09,870
negative if x is smaller than the mean or zero.

214
00:15:13,120 --> 00:15:18,140
Now the table we have gives the area to the right,

215
00:15:18,420 --> 00:15:21,240
to the left, I'm sorry, to the left, for positive

216
00:15:21,240 --> 00:15:26,220
and negative values of z. Okay, so we have two

217
00:15:26,220 --> 00:15:32,160
tables actually, one for negative on page 570, and

218
00:15:32,160 --> 00:15:38,260
the other one for positive values of z. I think we

219
00:15:38,260 --> 00:15:41,060
discussed that before when we talked about these

220
00:15:41,060 --> 00:15:44,080
scores. We have the same formula.

221
00:15:47,120 --> 00:15:53,700
Now let's look at this, the next slide. Suppose x

222
00:15:53,700 --> 00:16:01,880
is distributed normally with mean of 100. So the

223
00:16:01,880 --> 00:16:06,470
mean of x is 100. and the standard deviation of

224
00:16:06,470 --> 00:16:11,110
50. So sigma is 50. Now let's see how can we

225
00:16:11,110 --> 00:16:17,750
compute the z-score for x equals 200. Again the

226
00:16:17,750 --> 00:16:22,790
formula is just x minus mu divided by sigma x 200

227
00:16:22,790 --> 00:16:28,330
minus 100 divided by 50 that will give 2. Now the

228
00:16:28,330 --> 00:16:33,910
sign of this value is positive That means x is

229
00:16:33,910 --> 00:16:37,950
greater than the mean, because x is 200. Now,

230
00:16:37,990 --> 00:16:42,270
what's the meaning of 2? What does this value tell

231
00:16:42,270 --> 00:16:42,410
you?

232
00:16:48,230 --> 00:16:55,430
Yeah, exactly. x equals 200 is two standard

233
00:16:55,430 --> 00:16:58,690
deviations above the mean. Because if you look at

234
00:16:58,690 --> 00:17:05,210
200, the x value, The mean is 100, sigma is 50.

235
00:17:05,730 --> 00:17:09,690
Now the difference between the score, which is

236
00:17:09,690 --> 00:17:16,810
200, and the mu, which is 100, is equal to

237
00:17:16,810 --> 00:17:18,690
standard deviations, because the difference is

238
00:17:18,690 --> 00:17:24,230
100. 2 times 50 is 100. So this says that x equals

239
00:17:24,230 --> 00:17:29,070
200 is 2 standard deviations above the mean. If z

240
00:17:29,070 --> 00:17:34,330
is negative, you can say that x is two standard

241
00:17:34,330 --> 00:17:38,710
deviations below them. Make sense? So that's how

242
00:17:38,710 --> 00:17:42,670
can we compute the z square. Now, when we

243
00:17:42,670 --> 00:17:45,970
transform from normal distribution to

244
00:17:45,970 --> 00:17:49,490
standardized, still we will have the same shape. I

245
00:17:49,490 --> 00:17:51,350
mean the distribution is still normally

246
00:17:51,350 --> 00:17:55,800
distributed. So note, the shape of the

247
00:17:55,800 --> 00:17:58,840
distribution is the same, only the scale has

248
00:17:58,840 --> 00:18:04,500
changed. So we can express the problem in original

249
00:18:04,500 --> 00:18:10,640
units, X, or in a standardized unit, Z. So when we

250
00:18:10,640 --> 00:18:16,620
have X, just use this equation to transform to

251
00:18:16,620 --> 00:18:17,160
this form.

252
00:18:21,360 --> 00:18:23,200
Now, for example, suppose we have normal

253
00:18:23,200 --> 00:18:26,040
distribution and we are interested in the area

254
00:18:26,040 --> 00:18:32,660
between A and B. Now, the area between A and B, it

255
00:18:32,660 --> 00:18:34,700
means the probability between them. So

256
00:18:34,700 --> 00:18:39,140
statistically speaking, area means probability. So

257
00:18:39,140 --> 00:18:42,700
probability between A and B, I mean probability of

258
00:18:42,700 --> 00:18:45,380
X greater than or equal A and less than or equal B

259
00:18:45,380 --> 00:18:49,420
is the same as X greater than A or less than B.

260
00:18:50,450 --> 00:18:57,210
that means the probability of X equals A this

261
00:18:57,210 --> 00:19:02,510
probability is zero or probability of X equals B

262
00:19:02,510 --> 00:19:06,930
is also zero so in continuous distribution the

263
00:19:06,930 --> 00:19:10,630
equal sign does not matter I mean if we have equal

264
00:19:10,630 --> 00:19:15,130
sign or we don't have these probabilities are the

265
00:19:15,130 --> 00:19:19,390
same so I mean for example if we are interested

266
00:19:20,310 --> 00:19:23,450
for probability of X smaller than or equal to E.

267
00:19:24,850 --> 00:19:30,370
This probability is the same as X smaller than E.

268
00:19:31,330 --> 00:19:33,730
Or on the other hand, if you are interested in the

269
00:19:33,730 --> 00:19:39,010
area above B greater than or equal to B, it's the

270
00:19:39,010 --> 00:19:44,770
same as X smaller than E. So don't worry about the

271
00:19:44,770 --> 00:19:48,660
equal sign. Or continuous distribution, exactly.

272
00:19:49,120 --> 00:19:53,820
But for discrete, it does matter. Now, since we

273
00:19:53,820 --> 00:19:58,200
are talking about normal distribution, and as we

274
00:19:58,200 --> 00:20:01,320
mentioned, normal distribution is symmetric around

275
00:20:01,320 --> 00:20:05,900
the mean, that means the area to the right equals

276
00:20:05,900 --> 00:20:09,340
the area to the left. Now the entire area

277
00:20:09,340 --> 00:20:12,940
underneath the normal curve equals one. I mean

278
00:20:12,940 --> 00:20:16,500
probability of X ranges from minus infinity up to

279
00:20:16,500 --> 00:20:21,500
infinity equals one. So probability of X greater

280
00:20:21,500 --> 00:20:26,920
than minus infinity up to infinity is one. The

281
00:20:26,920 --> 00:20:31,480
total area is one. So the area from minus infinity

282
00:20:31,480 --> 00:20:38,080
up to the mean mu is one-half. The same as the

283
00:20:38,080 --> 00:20:42,600
area from mu up to infinity is also one-half. That

284
00:20:42,600 --> 00:20:44,760
means the probability of X greater than minus

285
00:20:44,760 --> 00:20:48,300
infinity up to mu equals the probability from mu

286
00:20:48,300 --> 00:20:52,120
up to infinity because of symmetry. I mean you

287
00:20:52,120 --> 00:20:56,160
cannot say that for any distribution. Just for

288
00:20:56,160 --> 00:20:59,000
symmetric distribution, the area below the mean

289
00:20:59,000 --> 00:21:03,780
equals one-half, which is the same as the area to

290
00:21:03,780 --> 00:21:07,110
the right of the mean. So the entire Probability

291
00:21:07,110 --> 00:21:11,330
is one. And also you have to keep in mind that the

292
00:21:11,330 --> 00:21:17,570
probability always ranges between zero and one. So

293
00:21:17,570 --> 00:21:20,030
that means the probability couldn't be negative.

294
00:21:22,870 --> 00:21:27,730
It should be positive. It shouldn't be greater

295
00:21:27,730 --> 00:21:31,710
than one. So it's between zero and one. So always

296
00:21:31,710 --> 00:21:39,020
the probability lies between zero and one. The

297
00:21:39,020 --> 00:21:44,500
tables we have on page 570 and 571 give the area

298
00:21:44,500 --> 00:21:46,040
to the left side.

299
00:21:49,420 --> 00:21:54,660
For negative or positive z's. Now for example,

300
00:21:54,940 --> 00:22:03,060
suppose we are looking for probability of z less

301
00:22:03,060 --> 00:22:08,750
than 2. How can we find this probability by using

302
00:22:08,750 --> 00:22:12,210
the normal curve? Let's go back to this normal

303
00:22:12,210 --> 00:22:16,410
distribution. In the second page, we have positive

304
00:22:16,410 --> 00:22:17,070
z-scores.

305
00:22:23,850 --> 00:22:33,390
So we ask about the probability of z less than. So

306
00:22:33,390 --> 00:22:40,690
the second page, gives positive values of z. And

307
00:22:40,690 --> 00:22:44,590
the table gives the area below. And he asked about

308
00:22:44,590 --> 00:22:49,550
here, B of z is smaller than 2. Now 2, if you

309
00:22:49,550 --> 00:22:54,910
hear, up all the way down here, 2, 0, 0. So the

310
00:22:54,910 --> 00:23:00,530
answer is 9772. So this value, so the probability

311
00:23:00,530 --> 00:23:02,130
is 9772.

312
00:23:03,990 --> 00:23:05,390
Because it's 2.

313
00:23:09,510 --> 00:23:14,650
It's 2, 0, 0. But if you ask about what's the

314
00:23:14,650 --> 00:23:20,590
probability of Z less than 2.05? So this is 2.

315
00:23:23,810 --> 00:23:30,370
Now under 5, 9, 7, 9, 8. So the answer is 9, 7.

316
00:23:34,360 --> 00:23:38,900
Because this is two, and we need five decimal

317
00:23:38,900 --> 00:23:44,820
places. So all the way up to 9798. So this value

318
00:23:44,820 --> 00:23:54,380
is 2.05. Now it's about, it's more than 1.5,

319
00:23:55,600 --> 00:23:56,880
exactly 1.5.

320
00:24:02,140 --> 00:24:04,880
1.5. This is 1.5.

321
00:24:08,800 --> 00:24:09,720
9332.

322
00:24:12,440 --> 00:24:16,300
1.5. Exactly 1.5. So 9332.

323
00:24:18,780 --> 00:24:27,990
What's about probability less than 1.35? 1.3 all

324
00:24:27,990 --> 00:24:35,250
the way to 9.115. 9.115. 9.115. 9.115. 9.115. 9

325
00:24:35,250 --> 00:24:35,650
.115. 9.115.

326
00:24:41,170 --> 00:24:42,430
9.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9

327
00:24:42,430 --> 00:24:42,450
.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9

328
00:24:42,450 --> 00:24:42,450
.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9

329
00:24:42,450 --> 00:24:44,050
.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9

330
00:24:44,050 --> 00:24:50,530
.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9.115. 9

331
00:24:50,530 --> 00:24:54,980
.115. 9. But here we are looking for the area to

332
00:24:54,980 --> 00:25:01,280
the right. One minus one. Now this area equals

333
00:25:01,280 --> 00:25:05,660
one minus because

334
00:25:05,660 --> 00:25:11,420
since suppose

335
00:25:11,420 --> 00:25:18,760
this is the 1.35 and we are interested in the area

336
00:25:18,760 --> 00:25:24,030
to the right or above 1.35. The table gives the

337
00:25:24,030 --> 00:25:28,230
area below. So the area above equals the total

338
00:25:28,230 --> 00:25:31,970
area underneath the curve is 1. So 1 minus this

339
00:25:31,970 --> 00:25:39,050
value, so equals 0.0885,

340
00:25:39,350 --> 00:25:42,250
and so on. So this is the way how can we compute

341
00:25:42,250 --> 00:25:47,850
the probabilities underneath the normal curve. if

342
00:25:47,850 --> 00:25:51,090
it's probability of z is smaller than then just

343
00:25:51,090 --> 00:25:55,910
use the table directly otherwise if we are talking

344
00:25:55,910 --> 00:26:00,390
about z greater than subtract from one to get the

345
00:26:00,390 --> 00:26:04,870
result that's how can we compute the probability

346
00:26:04,870 --> 00:26:13,750
of z less than or equal now

347
00:26:13,750 --> 00:26:18,890
let's see if we have x and x that has normal

348
00:26:18,890 --> 00:26:22,070
distribution with mean mu and standard deviation

349
00:26:22,070 --> 00:26:26,250
of sigma and let's see how can we compute the

350
00:26:26,250 --> 00:26:33,790
value of the probability mainly

351
00:26:33,790 --> 00:26:38,190
there are three steps to find the probability of x

352
00:26:38,190 --> 00:26:42,490
greater than a and less than b when x is

353
00:26:42,490 --> 00:26:47,000
distributed normally first step Draw normal curve

354
00:26:47,000 --> 00:26:54,880
for the problem in terms of x. So draw the normal

355
00:26:54,880 --> 00:26:58,140
curve first. Second, translate x values to z

356
00:26:58,140 --> 00:27:03,040
values by using the formula we have. z x minus mu

357
00:27:03,040 --> 00:27:06,440
divided by sigma. Then use the standardized normal

358
00:27:06,440 --> 00:27:15,140
table on page 570 and 571. For example, Let's see

359
00:27:15,140 --> 00:27:18,420
how can we find normal probabilities. Let's assume

360
00:27:18,420 --> 00:27:23,760
that X represents the time it takes to download an

361
00:27:23,760 --> 00:27:28,580
image from the internet. So suppose X, time

362
00:27:28,580 --> 00:27:33,760
required to download an image file from the

363
00:27:33,760 --> 00:27:38,460
internet. And suppose we know that the time is

364
00:27:38,460 --> 00:27:42,060
normally distributed for with mean of eight

365
00:27:42,060 --> 00:27:46,130
minutes. And standard deviation of five minutes.

366
00:27:46,490 --> 00:27:47,510
So we know the mean.

367
00:27:50,610 --> 00:27:59,670
Eight. Eight. And sigma of five minutes. And they

368
00:27:59,670 --> 00:28:03,410
ask about what's the probability of X smaller than

369
00:28:03,410 --> 00:28:07,990
eight one six. So first thing we have to compute,

370
00:28:08,170 --> 00:28:12,190
to draw the normal curve. The mean lies in the

371
00:28:12,190 --> 00:28:18,060
center. which is 8. He asked about probability of

372
00:28:18,060 --> 00:28:22,580
X smaller than 8.6. So we are interested in the

373
00:28:22,580 --> 00:28:27,920
area below 8.6. So it matched the table we have.

374
00:28:29,980 --> 00:28:34,900
Second step, we have to transform from normal

375
00:28:34,900 --> 00:28:37,280
distribution to standardized normal distribution

376
00:28:37,280 --> 00:28:42,120
by using this form, which is X minus mu divided by

377
00:28:42,120 --> 00:28:51,430
sigma. So x is 8.6 minus the mean, 8, divided by

378
00:28:51,430 --> 00:28:57,130
sigma, gives 0.12. So just straightforward

379
00:28:57,130 --> 00:29:02,890
calculation, 8.6 is your value of x. The mean is

380
00:29:02,890 --> 00:29:12,810
8, sigma is 5, so that gives 0.12. So now, the

381
00:29:12,810 --> 00:29:17,210
problem becomes, instead of asking x smaller than

382
00:29:17,210 --> 00:29:25,110
8.6, it's similar to z less than 0.12. Still, we

383
00:29:25,110 --> 00:29:26,310
have the same normal curve.

384
00:29:29,450 --> 00:29:32,990
8, the mean. Now, the mean of z is 0, as we

385
00:29:32,990 --> 00:29:39,230
mentioned. Instead of x, 8.6, the corresponding z

386
00:29:39,230 --> 00:29:43,000
value is 0.12. So instead of finding probability

387
00:29:43,000 --> 00:29:48,580
of X smaller than 8.6, smaller than 1.12, so they

388
00:29:48,580 --> 00:29:53,760
are equivalent. So we transform here from normal

389
00:29:53,760 --> 00:29:56,980
distribution to standardized normal distribution

390
00:29:56,980 --> 00:29:59,980
in order to compute the probability we are looking

391
00:29:59,980 --> 00:30:05,820
for. Now, this is just a portion of the table we

392
00:30:05,820 --> 00:30:06,100
have.

393
00:30:10,530 --> 00:30:18,530
So for positive z values. Now 0.1 is 0.1. Because

394
00:30:18,530 --> 00:30:25,670
here we are looking for z less than 0.1. So 0.1.

395
00:30:27,210 --> 00:30:32,950
Also, we have two. So move up to two decimal

396
00:30:32,950 --> 00:30:38,190
places, we get this value. So the answer is point.

397
00:30:42,120 --> 00:30:45,860
I think it's straightforward to compute the

398
00:30:45,860 --> 00:30:49,460
probability underneath the normal curve if X has

399
00:30:49,460 --> 00:30:53,160
normal distribution. So B of X is smaller than 8.6

400
00:30:53,160 --> 00:30:56,740
is the same as B of Z less than 0.12, which is

401
00:30:56,740 --> 00:31:02,680
around 55%. Makes sense because the area to the

402
00:31:02,680 --> 00:31:07,080
left of 0 equals 1 half. But we are looking for

403
00:31:07,080 --> 00:31:12,440
the area below 0.12. So greater than zero. So this

404
00:31:12,440 --> 00:31:16,600
area actually is greater than 0.5. So it makes

405
00:31:16,600 --> 00:31:20,440
sense that your result is greater than 0.5.

406
00:31:22,320 --> 00:31:22,960
Questions?

407
00:31:25,480 --> 00:31:30,780
Next, suppose we are interested of probability of

408
00:31:30,780 --> 00:31:35,380
X greater than. So that's how can we find normal

409
00:31:35,380 --> 00:31:41,980
upper tail probabilities. Again, the table we have

410
00:31:41,980 --> 00:31:46,580
gives the area to the left. In order to compute

411
00:31:46,580 --> 00:31:50,880
the area in the upper tail probabilities, I mean

412
00:31:50,880 --> 00:31:55,620
this area, since the normal distribution is

413
00:31:55,620 --> 00:32:00,160
symmetric and The total area underneath the curve

414
00:32:00,160 --> 00:32:04,680
is 1. So the probability of X greater than 8.6 is

415
00:32:04,680 --> 00:32:11,640
the same as 1 minus B of X less than 8.6. So first

416
00:32:11,640 --> 00:32:17,020
step, just find the probability we just have and

417
00:32:17,020 --> 00:32:21,680
subtract from 1. So B of X greater than 8.6, the

418
00:32:21,680 --> 00:32:25,930
same as B of Z greater than 0.12. which is the

419
00:32:25,930 --> 00:32:30,370
same as 1 minus B of Z less than 0.5. It's 1 minus

420
00:32:30,370 --> 00:32:36,230
the result we got from previous one. So this value

421
00:32:36,230 --> 00:32:39,410
1 minus this value gives 0.452.

422
00:32:41,610 --> 00:32:45,090
So for the other tail probability, just subtract 1

423
00:32:45,090 --> 00:32:47,690
from the lower tail probabilities.

424
00:32:51,930 --> 00:32:55,750
Now let's see how can we find Normal probability

425
00:32:55,750 --> 00:33:01,750
between two values. I mean if X, for example, for

426
00:33:01,750 --> 00:33:06,610
the same data we have, suppose X between 8 and 8

427
00:33:06,610 --> 00:33:13,360
.6. Now what's the area between these two? Here we

428
00:33:13,360 --> 00:33:17,220
have two values of x, x is 8 and x is 8.6.

429
00:33:24,280 --> 00:33:33,780
Exactly, so below 8.6 minus below 8 and below 8 is

430
00:33:33,780 --> 00:33:40,840
1 half. So the probability of x between 8

431
00:33:40,840 --> 00:33:47,340
and And 8.2 and 8.6. You can find z-score for the

432
00:33:47,340 --> 00:33:52,480
first value, which is zero. Also compute the z

433
00:33:52,480 --> 00:33:55,540
-score for the other value, which as we computed

434
00:33:55,540 --> 00:34:01,580
before, 0.12. Now this problem becomes z between

435
00:34:01,580 --> 00:34:04,540
zero and 0.5.

436
00:34:07,480 --> 00:34:15,120
So B of x. Greater than 8 and smaller than 8.6 is

437
00:34:15,120 --> 00:34:20,800
the same as z between 0 and 0.12. Now this area

438
00:34:20,800 --> 00:34:25,320
equals b of z smaller than 0.12 minus the area

439
00:34:25,320 --> 00:34:26,520
below z which is 1.5.

440
00:34:31,100 --> 00:34:37,380
So again, b of z between 0 and 1.5 equal b of z

441
00:34:37,380 --> 00:34:42,840
small. larger than 0.12 minus b of z less than

442
00:34:42,840 --> 00:34:46,520
zero. Now, b of z less than 0.12 gives this

443
00:34:46,520 --> 00:34:53,060
result, 0.5478. The probability below zero is one

444
00:34:53,060 --> 00:34:56,160
-half because we know that the area to the left is

445
00:34:56,160 --> 00:34:59,320
zero, same as to the right is one-half. So the

446
00:34:59,320 --> 00:35:04,240
answer is going to be 0.478. So that's how can we

447
00:35:04,240 --> 00:35:07,540
compute the probabilities for lower 10 directly

448
00:35:07,540 --> 00:35:12,230
from the table. upper tail is just one minus lower

449
00:35:12,230 --> 00:35:18,990
tail and between two values just subtracts the

450
00:35:18,990 --> 00:35:21,970
larger one minus smaller one because he was

451
00:35:21,970 --> 00:35:26,310
subtracted bz less than point one minus bz less

452
00:35:26,310 --> 00:35:29,430
than or equal to zero that will give the normal

453
00:35:29,430 --> 00:35:36,850
probability another example suppose we are looking

454
00:35:36,850 --> 00:35:49,350
for X between 7.4 and 8. Now, 7.4 lies below the

455
00:35:49,350 --> 00:35:55,270
mean. So here, this value, we have to compute the

456
00:35:55,270 --> 00:36:00,130
z-score for 7.4 and also the z-score for 8, which

457
00:36:00,130 --> 00:36:04,090
is zero. And that will give, again,

458
00:36:07,050 --> 00:36:13,710
7.4, if you just use this equation, minus

459
00:36:13,710 --> 00:36:17,690
the mean, divided by sigma, negative 0.6 divided

460
00:36:17,690 --> 00:36:21,150
by 5, which is negative 0.12.

461
00:36:22,730 --> 00:36:31,410
So it gives B of z between minus 0.12 and 0. And

462
00:36:31,410 --> 00:36:35,700
that again is B of z less than 0. minus P of Z

463
00:36:35,700 --> 00:36:40,140
less than negative 0.12. Is it clear? Now here we

464
00:36:40,140 --> 00:36:42,260
converted or we transformed from normal

465
00:36:42,260 --> 00:36:45,960
distribution to standardized. So instead of X

466
00:36:45,960 --> 00:36:52,100
between 7.4 and 8, we have now Z between minus 0

467
00:36:52,100 --> 00:36:57,480
.12 and 0. So this area actually is the red one,

468
00:36:57,620 --> 00:37:03,740
the red area is one-half. Total area below z is

469
00:37:03,740 --> 00:37:10,700
one-half, below zero, and minus z below minus 0

470
00:37:10,700 --> 00:37:17,820
.12. So B of z less than zero minus negative 0.12.

471
00:37:18,340 --> 00:37:21,940
That will give the area between minus 0.12 and

472
00:37:21,940 --> 00:37:28,860
zero. This is one-half. Now, B of z less than

473
00:37:28,860 --> 00:37:33,270
negative 0.12. look you go back to the normal

474
00:37:33,270 --> 00:37:37,650
curve to the normal table but for the negative

475
00:37:37,650 --> 00:37:42,310
values of z negative point one two negative point

476
00:37:42,310 --> 00:37:53,290
one two four five two two it's four five point

477
00:37:53,290 --> 00:37:56,630
five minus point four five two two will give the

478
00:37:56,630 --> 00:37:58,370
result we are looking for

479
00:38:01,570 --> 00:38:06,370
So B of Z less than 0 is 0.5. B of Z less than

480
00:38:06,370 --> 00:38:12,650
negative 0.12 equals minus 0.4522. That will give

481
00:38:12,650 --> 00:38:14,290
0 forcibility.

482
00:38:16,790 --> 00:38:23,590
Now, by symmetric, you can see that this

483
00:38:23,590 --> 00:38:28,470
probability between

484
00:38:28,470 --> 00:38:38,300
Z between minus 0.12 and 0 is the same as the

485
00:38:38,300 --> 00:38:43,340
other side from 0.12 I mean this area the red one

486
00:38:43,340 --> 00:38:46,200
is the same up to 8.6

487
00:38:55,600 --> 00:38:58,840
So the area between minus 0.12 up to 0 is the same

488
00:38:58,840 --> 00:39:04,920
as from 0 up to 0.12. Because of symmetric, since

489
00:39:04,920 --> 00:39:09,680
this area equals the same for the other part. So

490
00:39:09,680 --> 00:39:15,660
from 0 up to 0.12 is the same as minus 0.12 up to

491
00:39:15,660 --> 00:39:19,100
0. So equal, so the normal distribution is

492
00:39:19,100 --> 00:39:23,200
symmetric. So this probability is the same as B of

493
00:39:23,200 --> 00:39:27,980
Z between 0 and 0.12. Any question?

494
00:39:34,520 --> 00:39:36,620
Again, the equal sign does not matter.

495
00:39:42,120 --> 00:39:45,000
Because here we have the complement. The

496
00:39:45,000 --> 00:39:49,250
complement. If this one, I mean, complement of z

497
00:39:49,250 --> 00:39:53,350
less than, greater than 0.12, the complement is B

498
00:39:53,350 --> 00:39:56,350
of z less than or equal to minus 0.12. So we

499
00:39:56,350 --> 00:40:00,070
should have just permutation, the equality. But it

500
00:40:00,070 --> 00:40:04,830
doesn't matter. If in the problem we don't have

501
00:40:04,830 --> 00:40:07,470
equal sign in the complement, we should have equal

502
00:40:07,470 --> 00:40:11,430
sign. But it doesn't matter actually if we have

503
00:40:11,430 --> 00:40:14,510
equal sign or not. For example, if we are looking

504
00:40:14,510 --> 00:40:19,430
for B of X greater than A. Now what's the

505
00:40:19,430 --> 00:40:25,950
complement of that? 1 minus less

506
00:40:25,950 --> 00:40:32,450
than or equal to A. But if X is greater than or

507
00:40:32,450 --> 00:40:37,870
equal to A, the complement is without equal sign.

508
00:40:38,310 --> 00:40:40,970
But in continuous distribution, the equal sign

509
00:40:40,970 --> 00:40:44,990
does not matter. Any question?

510
00:40:52,190 --> 00:40:58,130
comments. Let's move to the next topic which talks

511
00:40:58,130 --> 00:41:05,510
about the empirical rule. If you remember before

512
00:41:05,510 --> 00:41:16,750
we said there is an empirical rule for 68, 95, 95,

513
00:41:17,420 --> 00:41:23,060
99.71. Now let's see the exact meaning of this

514
00:41:23,060 --> 00:41:23,320
rule.

515
00:41:37,580 --> 00:41:40,460
Now we have to apply the empirical rule not to

516
00:41:40,460 --> 00:41:43,020
Chebyshev's inequality because the distribution is

517
00:41:43,020 --> 00:41:48,670
normal. Chebyshev's is applied for skewed

518
00:41:48,670 --> 00:41:52,630
distributions. For symmetric, we have to apply the

519
00:41:52,630 --> 00:41:55,630
empirical rule. Here, we assume the distribution

520
00:41:55,630 --> 00:41:58,390
is normal. And today, we are talking about normal

521
00:41:58,390 --> 00:42:01,330
distribution. So we have to use the empirical

522
00:42:01,330 --> 00:42:02,410
rules.

523
00:42:07,910 --> 00:42:13,530
Now, the mean is the value in the middle. Suppose

524
00:42:13,530 --> 00:42:16,900
we are far away. from the mean by one standard

525
00:42:16,900 --> 00:42:22,720
deviation either below or above and we are

526
00:42:22,720 --> 00:42:27,040
interested in the area between this value which is

527
00:42:27,040 --> 00:42:33,040
mu minus sigma so we are looking for mu minus

528
00:42:33,040 --> 00:42:36,360
sigma and mu plus sigma

529
00:42:53,270 --> 00:42:59,890
Last time we said there's a rule 68% of the data

530
00:42:59,890 --> 00:43:06,790
lies one standard deviation within the mean. Now

531
00:43:06,790 --> 00:43:10,550
let's see how can we compute the exact area, area

532
00:43:10,550 --> 00:43:15,250
not just say 68%. Now X has normal distribution

533
00:43:15,250 --> 00:43:18,390
with mean mu and standard deviation sigma. So

534
00:43:18,390 --> 00:43:25,280
let's compare it from normal distribution to

535
00:43:25,280 --> 00:43:29,700
standardized. So this is the first value here. Now

536
00:43:29,700 --> 00:43:34,940
the z-score, the general formula is x minus the

537
00:43:34,940 --> 00:43:40,120
mean divided by sigma. Now the first quantity is

538
00:43:40,120 --> 00:43:45,660
mu minus sigma. So instead of x here, so first z

539
00:43:45,660 --> 00:43:49,820
is, now this x should be replaced by mu minus

540
00:43:49,820 --> 00:43:55,040
sigma. So mu minus sigma. So that's my x value,

541
00:43:55,560 --> 00:44:00,240
minus the mean of that, which is mu, divided by

542
00:44:00,240 --> 00:44:07,900
sigma. Mu minus sigma minus mu mu cancels, so plus

543
00:44:07,900 --> 00:44:13,520
one. And let's see how can we compute that area. I

544
00:44:13,520 --> 00:44:16,980
mean between minus one and plus one. In this case,

545
00:44:17,040 --> 00:44:23,180
we are interested or we are looking for the area

546
00:44:23,180 --> 00:44:28,300
between minus one and plus one this area now the

547
00:44:28,300 --> 00:44:31,360
dashed area i mean the area between minus one and

548
00:44:31,360 --> 00:44:39,460
plus one equals the area below one this area minus

549
00:44:39,460 --> 00:44:44,980
the area below minus one that will give the area

550
00:44:44,980 --> 00:44:48,200
between minus one and plus one now go back to the

551
00:44:48,200 --> 00:44:52,500
normal table you have and look at the value of one

552
00:44:52,500 --> 00:45:02,620
z and one under zero what's your answer one point

553
00:45:02,620 --> 00:45:11,520
one point now without using the table can you tell

554
00:45:11,520 --> 00:45:17,360
the area below minus one one minus this one

555
00:45:17,360 --> 00:45:17,840
because

556
00:45:23,430 --> 00:45:29,870
Now the area below, this is 1. The area below 1 is

557
00:45:29,870 --> 00:45:31,310
0.3413.

558
00:45:34,430 --> 00:45:37,590
Okay, now the area below minus 1.

559
00:45:40,770 --> 00:45:42,050
This is minus 1.

560
00:45:46,810 --> 00:45:49,550
Now, the area below minus 1 is the same as above

561
00:45:49,550 --> 00:45:50,510
1.

562
00:45:54,310 --> 00:45:58,810
These are the two areas here are equal. So the

563
00:45:58,810 --> 00:46:03,110
area below minus 1, I mean b of z less than minus

564
00:46:03,110 --> 00:46:09,130
1 is the same as b of z greater than 1. And b of z

565
00:46:09,130 --> 00:46:12,650
greater than 1 is the same as 1 minus b of z

566
00:46:12,650 --> 00:46:17,310
smaller than 1. So b of z less than 1 here. You

567
00:46:17,310 --> 00:46:19,710
shouldn't need to look again to the table. Just

568
00:46:19,710 --> 00:46:26,770
subtract 1 from this value. Make sense? Here we

569
00:46:26,770 --> 00:46:30,490
compute the value of B of Z less than 1, which is

570
00:46:30,490 --> 00:46:35,430
0.8413. We are looking for B of Z less than minus

571
00:46:35,430 --> 00:46:39,770
1, which is the same as B of Z greater than 1.

572
00:46:40,750 --> 00:46:43,850
Now, greater than means our tail. It's 1 minus the

573
00:46:43,850 --> 00:46:48,700
lower tail probability. So this is 1 minus. So the

574
00:46:48,700 --> 00:46:52,240
answer again is 1 minus 0.8413.

575
00:46:54,280 --> 00:47:00,040
So 8413 minus 0.1587.

576
00:47:11,380 --> 00:47:17,030
So 8413. minus 1.1587.

577
00:47:21,630 --> 00:47:27,570
Okay, so that gives 0.6826.

578
00:47:29,090 --> 00:47:37,550
Multiply this one by 100, we get 68.1826.

579
00:47:38,750 --> 00:47:44,010
So roughly 60-80% of the observations lie between

580
00:47:44,010 --> 00:47:50,470
one standard deviation around the mean. So this is

581
00:47:50,470 --> 00:47:53,850
the way how can we compute the area below one

582
00:47:53,850 --> 00:47:57,250
standard deviation or above one standard deviation

583
00:47:57,250 --> 00:48:03,790
of the mean. Do the same for not mu minus sigma,

584
00:48:05,230 --> 00:48:11,540
mu plus minus two sigma and mu plus two sigma. The

585
00:48:11,540 --> 00:48:14,600
only difference is that this one is going to be

586
00:48:14,600 --> 00:48:17,280
minus 2 and do the same.

587
00:48:20,620 --> 00:48:23,080
That's the empirical rule we discussed in chapter

588
00:48:23,080 --> 00:48:28,980
3. So here we can find any probability, not just

589
00:48:28,980 --> 00:48:33,660
95 or 68 or 99.7. We can use the normal table to

590
00:48:33,660 --> 00:48:36,900
give or to find or to compute any probability.

591
00:48:48,270 --> 00:48:53,090
So again, for the other one, mu plus or minus two

592
00:48:53,090 --> 00:49:00,190
sigma, it covers about 95% of the axis. For mu

593
00:49:00,190 --> 00:49:03,750
plus or minus three sigma, it covers around all

594
00:49:03,750 --> 00:49:08,450
the data, 99.7. So just do it at home, you will

595
00:49:08,450 --> 00:49:14,210
see that the exact area is 95.44 instead of 95.

596
00:49:14,840 --> 00:49:18,520
And the other one is 99.73. So that's the

597
00:49:18,520 --> 00:49:23,520
empirical rule we discussed in chapter three. I'm

598
00:49:23,520 --> 00:49:32,560
going to stop at this point, which is the x value

599
00:49:32,560 --> 00:49:38,400
for the normal probability. Now, what we discussed

600
00:49:38,400 --> 00:49:43,560
so far, we computed the probability. I mean,

601
00:49:43,740 --> 00:49:49,120
what's the probability of X smaller than E? Now,

602
00:49:49,200 --> 00:49:56,240
suppose this probability is known. How can we

603
00:49:56,240 --> 00:50:01,500
compute this value? Later, we'll talk about that.

604
00:50:06,300 --> 00:50:09,820
It's backward calculations. It's inverse or

605
00:50:09,820 --> 00:50:11,420
backward calculation.

606
00:50:13,300 --> 00:50:14,460
for next time inshallah.