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STAR model

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988:. Chan and Tong (1986) rigorously proved that the family of STAR models includes the SETAR model as a limiting case by showing the uniform boundedness and equicontinuity with respect to the switching parameter. Without this proof, to say that STAR models nest the SETAR model lacks justification. Unfortunately, whether one should use a SETAR model or a STAR model for one's data has been a matter of subjective judgement, taste and inclination in much of the literature. Fortunately, the test procedure, based on David Cox's test of separate family of hypotheses and developed by Gao, Ling and Tong (2018, Statistica Sinica, volume 28, 2857-2883) is now available to address this issue. Such a test is important before adopting a STAR model because, among other issues, the parameter controlling its rate of switching is notoriously data-hungry. 1850: 864: 1299: 24: 977:
STAR models were introduced and comprehensively developed by Kung-sik Chan and Howell Tong in 1986 (esp. p. 187), in which the same acronym was used. It originally stands for Smooth Threshold AutoRegressive. For some background history, see Tong (2011, 2012). The models can be thought of in
353: 1110: 1797: 481: 1494: 1625: 849: 672: 774: 561: 1225: 202: 118:, the STAR model is a tool for understanding and, perhaps, predicting future values in this series, assuming that the behaviour of the series changes depending on the value of the 1275: 387: 997: 1879: 695: 1347: 912: 72: 1327: 966: 939: 892: 52: 1638: 1974:"Threshold models in time series analysis—30 years on (with discussions by P. Whittle, M. Rosenblatt, B. E. Hansen, P. Brockwell, N. I. Samia & F. Battaglia)" 1808: 1290:
of regimes. In both cases the presence of the transition function is the defining feature of the model as it allows for changes in values of the parameters.
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part. Most popular transition function include exponential function and first and second-order logistic functions. They give rise to Logistic STAR (
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terms of extension of autoregressive models discussed above, allowing for changes in the model parameters according to the value of a
1901: 1121: 1823: 1862: 2074: 1872: 1866: 1858: 2069: 1883: 1350: 348:{\displaystyle y_{t}=\gamma _{0}+\gamma _{1}y_{t-1}+\gamma _{2}y_{t-2}+...+\gamma _{p}y_{t-p}+\epsilon _{t}.\,} 1828: 863: 1232: 1105:{\displaystyle y_{t}=\mathbf {X_{t}} +G(z_{t},\zeta ,c)\mathbf {X_{t}} +\sigma ^{(j)}\epsilon _{t}\,} 398: 364: 1813: 1286:
They can be understood as two-regime SETAR model with smooth transition between regimes, or as
679: 1792:{\displaystyle G(z_{t},\zeta ,c)=(1+exp(-\zeta (z_{t}-c_{1})(z_{t}-c_{2})))^{-1},\zeta >0} 2048: 2018: 1988: 1958: 1950: 1925: 1332: 897: 57: 1305: 1298: 944: 917: 870: 30: 23: 2033: 1929: 1818: 157: 144:(AR) parts linked by the transition function. The model is usually referred to as the 141: 99: 2003: 2063: 1833: 131: 152:) models proceeded by the letter describing the transition function (see below) and 1916:
Chan, K. S.; Tong, H. (1986). "On Estimating Thresholds in Autoregressive Models".
102:, in order to allow for higher degree of flexibility in model parameters through a 476:{\displaystyle \epsilon _{t}{\stackrel {\mathit {iid}}{\sim }}WN(0;\sigma ^{2})\,} 852: 484: 186: 95: 17: 2052: 2023: 1993: 79: 1489:{\displaystyle G(z_{t},\zeta ,c)=(1+exp(-\zeta (z_{t}-c)))^{-1},\zeta >0} 1954: 1939:"Smooth Transition Autoregressive Models—A Survey of Recent Developments" 1620:{\displaystyle G(z_{t},\zeta ,c)=1-exp(-\zeta (z_{t}-c)^{2}),\zeta >0} 856: 488: 844:{\displaystyle \epsilon _{t}{\stackrel {\mathit {iid}}{\sim }}WN(0;1)\,} 1356:
Three basic transition functions and the name of resulting models are:
667:{\displaystyle \mathbf {X_{t}} =(1,y_{t-1},y_{t-2},\ldots ,y_{t-p})\,} 1963: 769:{\displaystyle \gamma _{0},\gamma _{1},\gamma _{2},...,\gamma _{p}\,} 556:{\displaystyle y_{t}=\mathbf {X_{t}\gamma } +\sigma \epsilon _{t}.\,} 1938: 1843: 991:
Defined in this way, STAR model can be presented as follows:
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first order logistic function - results in Logistic STAR (
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Exponential transition function for the ESTAR model with
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Exponential transition function for the ESTAR model with
1220:{\displaystyle X_{t}=(1,y_{t-1},y_{t-2},...,y_{t-p})\,} 1302:
Logistic transition function for the ESTAR model with
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Van Dijk, D.; Teräsvirta, T.; Franses, P. H. (2002).
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exponential function - results in Exponential STAR (
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is the transition function bounded between 0 and 1.
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The transition might depend on the 7: 2041:Statistical Methods and Applications 495:written in a following vector form: 1930:10.1111/j.1467-9892.1986.tb00501.x 697:is the vector of parameters : 14: 1270:{\displaystyle G(z_{t},\zeta ,c)} 1848: 1349:- from 0 to 1. Calculated using 1227:is a column vector of variables; 1066: 1062: 1020: 1016: 674:is a column vector of variables; 582: 578: 524: 520: 84:Smooth Transition Autoregressive 1918:Journal of Time Series Analysis 1631:second order logistic function: 2080:Nonlinear time series analysis 1765: 1761: 1758: 1732: 1729: 1703: 1694: 1676: 1670: 1645: 1602: 1593: 1573: 1564: 1543: 1518: 1462: 1458: 1455: 1436: 1427: 1409: 1403: 1378: 1264: 1239: 1213: 1138: 1086: 1080: 1057: 1032: 837: 825: 660: 591: 469: 450: 1: 1824:Generalised logistic function 382:{\displaystyle \gamma _{i}\,} 2011:Statistics and Its Interface 1981:Statistics and Its Interface 1329:varying from -10 to +10 and 109:Given a time series of data 54:varying from -10 to +10 and 134:), or exogenous variables. 2096: 15: 2053:10.1007/s10260-012-0196-1 2024:10.4310/sii.2011.v4.n2.a4 1994:10.4310/SII.2011.v4.n2.a1 894:varying from -10 to +10, 855:error term with constant 690:{\displaystyle \gamma \,} 487:error term with constant 94:are typically applied to 1857:This article includes a 164:) and Exponential STAR ( 98:data as an extension of 16:Not to be confused with 1886:more precise citations. 130:series (similar to the 2002:Hansen, B. E. (2011). 1793: 1621: 1490: 1353: 1343: 1342:{\displaystyle \zeta } 1323: 1271: 1221: 1106: 969: 962: 935: 908: 907:{\displaystyle \zeta } 888: 845: 770: 691: 668: 557: 477: 383: 349: 137:The model consists of 75: 68: 67:{\displaystyle \zeta } 48: 1955:10.1081/ETC-120008723 1829:Logistic distribution 1794: 1622: 1491: 1344: 1324: 1322:{\displaystyle z_{t}} 1301: 1272: 1222: 1107: 968:) equal to -7 and +3. 963: 961:{\displaystyle c_{2}} 936: 934:{\displaystyle c_{1}} 909: 889: 887:{\displaystyle z_{t}} 866: 846: 771: 692: 669: 558: 478: 384: 350: 181:Consider a simple AR( 177:AutoRegressive Models 100:autoregressive models 69: 49: 47:{\displaystyle z_{t}} 26: 1639: 1512: 1372: 1333: 1306: 1233: 1122: 998: 945: 918: 898: 871: 782: 701: 680: 573: 502: 407: 365: 203: 156:is the order of the 58: 31: 1943:Econometric Reviews 1294:Transition Function 980:transition variable 120:transition variable 2075:Time series models 1859:list of references 1814:Exponential growth 1789: 1617: 1486: 1354: 1339: 1319: 1267: 1217: 1102: 970: 958: 931: 904: 884: 841: 766: 687: 664: 553: 473: 379: 345: 76: 64: 44: 2070:Nonlinear systems 2032:Tong, H. (2012). 1972:Tong, H. 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1423: 1420: 1417: 1414: 1411: 1408: 1405: 1402: 1399: 1396: 1393: 1388: 1384: 1380: 1377: 1366: 1365: 1351:GNU R package. 1338: 1316: 1312: 1295: 1292: 1283: 1280: 1279: 1278: 1266: 1263: 1260: 1257: 1254: 1249: 1245: 1241: 1238: 1228: 1215: 1210: 1207: 1204: 1200: 1196: 1193: 1190: 1187: 1184: 1179: 1176: 1173: 1169: 1165: 1160: 1157: 1154: 1150: 1146: 1143: 1140: 1137: 1132: 1128: 1113: 1112: 1098: 1094: 1088: 1085: 1082: 1078: 1074: 1068: 1064: 1059: 1056: 1053: 1050: 1047: 1042: 1038: 1034: 1031: 1028: 1022: 1018: 1013: 1008: 1004: 984: 974: 971: 955: 951: 928: 924: 903: 881: 877: 861: 860: 839: 836: 833: 830: 827: 824: 821: 813: 810: 807: 801: 792: 788: 777: 762: 758: 754: 751: 748: 745: 742: 737: 733: 729: 724: 720: 716: 711: 707: 685: 675: 662: 657: 654: 651: 647: 643: 640: 637: 632: 629: 626: 622: 618: 613: 610: 607: 603: 599: 596: 593: 590: 584: 580: 564: 563: 551: 546: 542: 538: 535: 531: 526: 522: 517: 512: 508: 493: 492: 471: 466: 462: 458: 455: 452: 449: 446: 438: 435: 432: 426: 417: 413: 402: 399:autoregressive 375: 371: 356: 355: 343: 338: 334: 330: 325: 322: 319: 315: 309: 305: 301: 298: 295: 292: 289: 284: 281: 278: 274: 268: 264: 260: 255: 252: 249: 245: 239: 235: 231: 226: 222: 218: 213: 209: 192: 185:) model for a 178: 175: 173: 170: 158:autoregressive 142:autoregressive 113: 74:- from 0 to 1. 63: 41: 37: 13: 10: 9: 6: 4: 3: 2: 2092: 2081: 2078: 2076: 2073: 2071: 2068: 2067: 2065: 2054: 2050: 2046: 2042: 2035: 2030: 2025: 2020: 2016: 2012: 2005: 2000: 1995: 1990: 1986: 1982: 1975: 1970: 1965: 1960: 1956: 1952: 1948: 1944: 1940: 1935: 1931: 1927: 1923: 1919: 1914: 1913: 1906: 1903: 1895: 1885: 1881: 1875: 1874: 1868: 1864: 1860: 1855: 1846: 1845: 1839: 1835: 1834:SETAR (model) 1832: 1830: 1827: 1825: 1822: 1820: 1817: 1815: 1812: 1810: 1807: 1806: 1802: 1786: 1783: 1780: 1777: 1772: 1769: 1753: 1749: 1745: 1740: 1736: 1724: 1720: 1716: 1711: 1707: 1700: 1697: 1691: 1688: 1685: 1682: 1679: 1673: 1667: 1664: 1661: 1658: 1653: 1649: 1642: 1635: 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96:time series 18:Star schema 2064:Categories 1840:References 172:Definition 168:) models. 80:statistics 1964:1765/1656 1892:June 2012 1781:ζ 1770:− 1746:− 1717:− 1701:ζ 1698:− 1662:ζ 1609:ζ 1587:− 1571:ζ 1568:− 1553:− 1535:ζ 1478:ζ 1467:− 1450:− 1434:ζ 1431:− 1395:ζ 1337:ζ 1288:continuum 1256:ζ 1206:− 1175:− 1156:− 1093:ϵ 1077:σ 1049:ζ 902:ζ 800:∼ 787:ϵ 757:γ 732:γ 719:γ 706:γ 684:γ 653:− 639:… 628:− 609:− 541:ϵ 537:σ 530:γ 461:σ 425:∼ 412:ϵ 393:=1,2,..., 370:γ 333:ϵ 321:− 304:γ 280:− 263:γ 251:− 234:γ 221:γ 62:ζ 1803:See also 1504:) model: 1364:) model: 857:variance 489:variance 1880:improve 1115:where: 566:where: 358:where: 126:of the 92:models 2037:(PDF) 2007:(PDF) 1977:(PDF) 1865:, or 1502:ESTAR 1362:LSTAR 166:ESTAR 162:LSTAR 1784:> 1612:> 1481:> 941:and 397:are 389:for 146:STAR 88:STAR 2049:doi 2019:doi 1989:doi 1959:hdl 1951:doi 1926:doi 78:In 2066:: 2045:21 2043:. 2039:. 2013:. 2009:. 1983:. 1979:. 1957:. 1947:21 1945:. 1941:. 1920:. 1869:, 1861:, 106:. 90:) 82:, 2055:. 2051:: 2027:. 2021:: 2015:4 1997:. 1991:: 1985:4 1967:. 1961:: 1953:: 1932:. 1928:: 1922:7 1905:) 1899:( 1894:) 1890:( 1876:. 1787:0 1778:, 1773:1 1766:) 1762:) 1759:) 1754:2 1750:c 1741:t 1737:z 1733:( 1730:) 1725:1 1721:c 1712:t 1708:z 1704:( 1695:( 1692:p 1689:x 1686:e 1683:+ 1680:1 1677:( 1674:= 1671:) 1668:c 1665:, 1659:, 1654:t 1650:z 1646:( 1643:G 1615:0 1606:, 1603:) 1598:2 1594:) 1590:c 1582:t 1578:z 1574:( 1565:( 1562:p 1559:x 1556:e 1550:1 1547:= 1544:) 1541:c 1538:, 1532:, 1527:t 1523:z 1519:( 1516:G 1484:0 1475:, 1470:1 1463:) 1459:) 1456:) 1453:c 1445:t 1441:z 1437:( 1428:( 1425:p 1422:x 1419:e 1416:+ 1413:1 1410:( 1407:= 1404:) 1401:c 1398:, 1392:, 1387:t 1383:z 1379:( 1376:G 1315:t 1311:z 1265:) 1262:c 1259:, 1253:, 1248:t 1244:z 1240:( 1237:G 1214:) 1209:p 1203:t 1199:y 1195:, 1192:. 1189:. 1186:. 1183:, 1178:2 1172:t 1168:y 1164:, 1159:1 1153:t 1149:y 1145:, 1142:1 1139:( 1136:= 1131:t 1127:X 1097:t 1087:) 1084:j 1081:( 1073:+ 1067:t 1063:X 1058:) 1055:c 1052:, 1046:, 1041:t 1037:z 1033:( 1030:G 1027:+ 1021:t 1017:X 1012:= 1007:t 1003:y 985:t 983:z 954:2 950:c 927:1 923:c 880:t 876:z 859:. 838:) 835:1 832:; 829:0 826:( 823:N 820:W 812:d 809:i 806:i 791:t 776:; 761:p 753:, 750:. 747:. 744:. 741:, 736:2 728:, 723:1 715:, 710:0 661:) 656:p 650:t 646:y 642:, 636:, 631:2 625:t 621:y 617:, 612:1 606:t 602:y 598:, 595:1 592:( 589:= 583:t 579:X 550:. 545:t 534:+ 525:t 521:X 516:= 511:t 507:y 491:. 470:) 465:2 457:; 454:0 451:( 448:N 445:W 437:d 434:i 431:i 416:t 395:p 391:i 374:i 342:. 337:t 329:+ 324:p 318:t 314:y 308:p 300:+ 297:. 294:. 291:. 288:+ 283:2 277:t 273:y 267:2 259:+ 254:1 248:t 244:y 238:1 230:+ 225:0 217:= 212:t 208:y 194:t 190:y 183:p 154:p 150:p 148:( 139:2 128:x 115:t 111:x 86:( 40:t 36:z 20:.

Index

Star schema

statistics
time series
autoregressive models
SETAR models
autoregressive
autoregressive
time series
autoregressive
white-noise
variance
white-noise
variance


GNU R package.
Characterizations of the exponential function
Exponential growth
Exponentiation
Generalised logistic function
Logistic distribution
SETAR (model)
list of references
related reading
external links
inline citations
improve
introducing
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