Knowledge

SigSpec

Source πŸ“

669: 262: 664:{\displaystyle \tan 2\theta _{0}={\frac {K\sum _{k=0}^{K-1}\sin 2\omega t_{k}-2\left(\sum _{k=0}^{K-1}\cos \omega t_{k}\right)\left(\sum _{k=0}^{K-1}\sin \omega t_{k}\right)}{K\sum _{k=0}^{K-1}\cos 2\omega t_{k}-{\big (}\sum _{k=0}^{K-1}\cos \omega t_{k}{\big )}^{2}+{\big (}\sum _{k=0}^{K-1}\sin \omega t_{k}{\big )}^{2}}},} 1442: 2183:
M. Gruberbauer; K. Kolenberg; J. F. Rowe; D. Huber; J. M. Matthews; P. Reegen; R. Kuschnig; C. Cameron; T. Kallinger; W. W. Weiss; D. B. Guenther; A. F. J. Moffat; S. M. Rucinski; D. Sasselov; G. A. H. Walker (2007). "MOST photometry of the RRdLyrae variable AQLeo: two radial modes, 32 combination
904: 1139: 1834: 2247:
M. Gruberbauer; H. Saio; D. Huber; T. Kallinger; W. W. Weiss; D. B. Guenther; R. Kuschnig; J. M. Matthews; A. F. J. Moffat; S. M. Rucinski; D. Sasselov; G. A. H. Walker (2008). "MOST photometry and modeling of the rapidly oscillating (roAp) star γ Equulei".
2669:
K. Zwintz; T. Kallinger; D. B. Guenther; M. Gruberbauer; D. Huber; J. Rowe; R. Kuschnig; W. W. Weiss; J. M. Matthews; A. F. J. Moffat; S. M. Rucinski; D. Sasselov; G. A. H. Walker; M. P. Casey (2009). "MOST photometry of the enigmatic PMS pulsator HD 142666".
2374:
D. Huber; H. Saio; M. Gruberbauer; W. W. Weiss; J. F. Rowe; M. Hareter; T. Kallinger; P. Reegen; J. M. Matthews; R. Kuschnig; D. B. Guenther; A. F. J. Moffat; S. M. Rucinski; D. Sasselov; G. A. H. Walker (2008). "MOST photometry of the roAp star 10 Aquilae".
1297: 1933: 1974:
and to classify stellar pulsation (see references below). The fact that this method incorporates the properties of the time-domain sampling appropriately makes it a valuable tool for typical astronomical measurements containing data gaps.
2422:
T. Kallinger; D. B. Guenther; J. M. Matthews; W. W. Weiss; D. Huber; R. Kuschnig; A. F. J. Moffat; S. M. Rucinski; D. Sasselov (2008). "Nonradial p-modes in the G9.5 giant ε Ophiuchi? Pulsation model fits to MOST photometry".
1308: 2717:
K. Zwintz; M. Hareter; R. Kuschnig; P. J. Amado; N. Nesvacil; E. Rodriguez; D. Diaz-Fraile; W. W. Weiss; T. Pribulla; D. B. Guenther; J. M. Matthews; A. F. J. Moffat; S. M. Rucinski; D. Sasselov; G. A. H. Walker (2009).
677: 912: 73:, appropriately incorporating a time series to be averaged to zero before applying the DFT, which is done in many practical applications. When a zero-mean corrected dataset has to be statistically compared to a 1622: 1732: 1170: 1845: 1658: 157: 254: 200: 2186: 227: 1162: 1692: 1956: 1724: 111: 1437:{\displaystyle \phi (A)={\frac {KA\cdot \operatorname {sock} }{2<x^{2}>}}\exp \left(-{\frac {KA^{2}}{4<x^{2}>}}\cdot \operatorname {sock} \right),} 62:. It represents the answer to the question, β€œWhat would be the chance to obtain an amplitude like the measured one or higher, if the analysed time series were 2295:
D. B. Guenther; T. Kallinger; P. Reegen; W. W. Weiss; J. M. Matthews; R. Kuschnig; A. F. J. Moffat; S. M. Rucinski; D. Sasselov; G. A. H. Walker (2007).
2622:
M. Zechmeister; M. Kuerster (2009). "The gemeralised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms".
899:{\displaystyle \alpha _{0}={\sqrt {{\frac {2}{K^{2}}}\left(K\sum _{k=0}^{K-1}\cos ^{2}\left(\omega t_{k}-\theta _{0}\right)-\left^{2}\right)}},} 2782: 2239: 1134:{\displaystyle \beta _{0}={\sqrt {{\frac {2}{K^{2}}}\left(K\sum _{k=0}^{K-1}\sin ^{2}\left(\omega t_{k}-\theta _{0}\right)-\left^{2}\right)}}.} 2102:
J. D. Scargle (1982). "Studies in astronomical time series analysis. II. Statistical aspects of spectral analysis of unevenly spaced data".
2470:
T. Kallinger; P. Reegen; W. W. Weiss (2008). "A heuristic derivation of the uncertainty for frequency determination in time series data".
2540:
P. Reegen; M. Gruberbauer; L. Schneider; W. W. Weiss (2008). "Cinderella - Comparison of INDEpendent RELative Least-squares Amplitudes".
1665: 2792: 2530: 78: 1453: 26:) is a statistical technique to provide the reliability of periodicities in a measured (noisy and not necessarily equidistant) 1829:{\displaystyle \Phi _{\operatorname {FA} }(A)=\exp \left(-{\frac {KA^{2}}{4<x^{2}>}}\cdot \operatorname {sock} \right).} 160: 1984: 2006: 35: 2331: 2787: 70: 1292:{\displaystyle \tan \theta ={\frac {\sum _{k=0}^{K-1}\sin \omega t_{k}}{\sum _{k=0}^{K-1}\cos \omega t_{k}}},} 1928:{\displaystyle \operatorname {sig} (A)={\frac {KA^{2}\log e}{4<x^{2}>}}\cdot \operatorname {sock} .} 2233: 1938:
It returns the number of random time series one would have to examine to obtain one amplitude exceeding
2767: 2731: 2689: 2641: 2600: 2559: 2489: 2442: 2394: 2346: 2308: 2267: 2205: 2155: 2111: 2068: 2025: 1630: 116: 2749: 2705: 2679: 2657: 2631: 2575: 2549: 2505: 2479: 2458: 2432: 2410: 2384: 2362: 2283: 2257: 2221: 2195: 2171: 2145: 2084: 2041: 2015: 232: 178: 205: 2526: 2004:
P. Reegen (2007). "SigSpec - I. Frequency- and phase-resolved significance in Fourier space".
1839:
The sig is defined as the negative logarithm of the false-alarm probability and evaluates to
1147: 2739: 2735: 2697: 2693: 2649: 2645: 2608: 2567: 2563: 2497: 2493: 2450: 2446: 2402: 2398: 2354: 2316: 2275: 2271: 2213: 2163: 2119: 2076: 2072: 2033: 2029: 1967: 31: 1670: 2517:
P. Reegen (2005). ""SigSpec - reliable computation of significance in Fourier space", in
2604: 2350: 2312: 2209: 2159: 2115: 1941: 1709: 96: 2776: 2753: 2217: 2175: 1971: 172: 164: 74: 2709: 2661: 2579: 2509: 2462: 2366: 2287: 2225: 2045: 2414: 2136:
M. Breger; S. M. Rucinski; P. Reegen (2007). "The Pulsation of EE Camelopardalis".
2088: 59: 2744: 2719: 2701: 2653: 1702:
Integration of the pdf yields the false-alarm probability that white noise in the
2571: 2501: 2454: 2406: 2279: 2037: 2297:"Searching for p-modes in η Bootis & Procyon using MOST satellite data" 2059:
N. R. Lomb (1976). "Least-squares frequency analysis of unequally spaced data".
1703: 55: 27: 168: 51: 47: 54:
measure of the probability that the given amplitude level would be seen in
1661: 2330:
D. B. Guenther; T. Kallinger; K. Zwintz; W. W. Weiss; J. Tanner (2007).
2020: 2080: 2613: 2588: 2321: 2296: 63: 2358: 2167: 2123: 2684: 2636: 2554: 2484: 2437: 2389: 2262: 2200: 2150: 89:
Probability density function (pdf) of white noise in Fourier space
82: 2525:. Cambridge, UK: Cambridge University Press. pp. 791–798. 2768:
Website with further information on SigSpec calculation, etc.
1617:{\displaystyle \operatorname {sock} (\omega ,\theta )=\left} 2521:, eds. J. Zverko, J. Ziznovsky, S.J. Adelman, W.W. Weiss". 93:
Considering a time series to be represented by a set of
2720:"MOST observations of the young open cluster NGC 2264" 1944: 1848: 1735: 1712: 1673: 1633: 1456: 1311: 1173: 1150: 915: 680: 265: 235: 208: 181: 175:
angle may be described in terms of three parameters,
119: 99: 69:
SigSpec may be considered a formal extension to the
2523:
The A-Star Puzzle, Proceedings of IAU Symposium 224
2332:"Seismology of Pre-Main-Sequence Stars in NGC 6530" 1950: 1927: 1828: 1718: 1686: 1652: 1616: 1436: 1302:the probability density of amplitudes is given by 1291: 1156: 1133: 898: 663: 248: 221: 194: 151: 105: 2589:"A new slowly pulsating subdwarf-B star: HD 4539" 2187:Monthly Notices of the Royal Astronomical Society 1698:False-alarm probability and spectral significance 256:, defining the β€œsampling profile”, according to 1144:In terms of the phase angle in Fourier space, 644: 590: 574: 520: 8: 2519:The A-Star Puzzle, Proceedings IAU Symp. 224 2743: 2683: 2635: 2612: 2553: 2483: 2436: 2388: 2320: 2261: 2199: 2149: 2019: 1943: 1904: 1877: 1867: 1847: 1800: 1782: 1772: 1740: 1734: 1711: 1678: 1672: 1641: 1632: 1601: 1596: 1580: 1556: 1549: 1538: 1533: 1517: 1493: 1486: 1455: 1408: 1390: 1380: 1354: 1327: 1310: 1277: 1252: 1241: 1229: 1204: 1193: 1186: 1172: 1149: 1115: 1099: 1086: 1056: 1045: 1021: 1008: 987: 971: 960: 940: 931: 929: 920: 914: 880: 864: 851: 821: 810: 786: 773: 752: 736: 725: 705: 696: 694: 685: 679: 649: 643: 642: 635: 610: 599: 589: 588: 579: 573: 572: 565: 540: 529: 519: 518: 509: 481: 470: 450: 425: 414: 394: 369: 358: 337: 309: 298: 288: 279: 264: 240: 234: 213: 207: 186: 180: 140: 127: 118: 98: 2587:C. Schoenaers; A. E. Lynas-Gray (2007). 38:(DFT) and assigns a quantity called the 1996: 2231: 1447:where the sock function is defined by 7: 2593:Communications in Asteroseismology 2301:Communications in Asteroseismology 2238:: CS1 maint: unflagged free DOI ( 1958:at the given frequency and phase. 1737: 1706:produces an amplitude of at least 14: 2218:10.1111/j.1365-2966.2007.12042.x 2061:Astrophysics and Space Science 1861: 1855: 1752: 1746: 1475: 1463: 1321: 1315: 146: 120: 1: 2783:Statistical signal processing 1966:SigSpec is primarily used in 1653:{\displaystyle <x^{2}>} 152:{\displaystyle (t_{k},x_{k})} 30:. It relies on the amplitude 42:(frequently abbreviated by β€œ 2745:10.1051/0004-6361/200911863 2702:10.1051/0004-6361:200811116 2654:10.1051/0004-6361:200811296 1985:Spectral density estimation 249:{\displaystyle \theta _{0}} 195:{\displaystyle \alpha _{0}} 2809: 2724:Astronomy and Astrophysics 2672:Astronomy and Astrophysics 2624:Astronomy and Astrophysics 2572:10.1051/0004-6361:20078855 2542:Astronomy and Astrophysics 2502:10.1051/0004-6361:20077559 2472:Astronomy and Astrophysics 2455:10.1051/0004-6361:20078171 2425:Astronomy and Astrophysics 2407:10.1051/0004-6361:20079220 2377:Astronomy and Astrophysics 2280:10.1051/0004-6361:20078830 2250:Astronomy and Astrophysics 2038:10.1051/0004-6361:20066597 2007:Astronomy and Astrophysics 222:{\displaystyle \beta _{0}} 36:Discrete Fourier transform 2793:Digital signal processing 2339:The Astrophysical Journal 2184:frequencies and beyond". 2104:The Astrophysical Journal 2138:The Astronomical Journal 71:Lomb-Scargle periodogram 2736:2009A&A...502..239Z 2694:2009A&A...494.1031Z 2646:2009A&A...496..577Z 2564:2008A&A...484..601R 2494:2008A&A...481..571K 2447:2008A&A...478..497K 2399:2008A&A...483..239H 2272:2008A&A...480..223G 2073:1976Ap&SS..39..447L 2030:2007A&A...467.1353R 1157:{\displaystyle \theta } 1952: 1929: 1830: 1720: 1688: 1654: 1618: 1438: 1293: 1263: 1215: 1158: 1135: 1067: 982: 900: 832: 747: 665: 621: 551: 492: 436: 380: 320: 250: 223: 196: 153: 107: 85:only) has to be zero. 1953: 1930: 1831: 1721: 1689: 1687:{\displaystyle x_{k}} 1655: 1619: 1439: 1294: 1237: 1189: 1159: 1136: 1041: 956: 901: 806: 721: 666: 595: 525: 466: 410: 354: 294: 251: 224: 197: 154: 108: 50:. This quantity is a 40:spectral significance 24:SIGnificance SPECtrum 16:Statistical technique 1942: 1846: 1733: 1710: 1671: 1631: 1454: 1309: 1171: 1148: 913: 678: 263: 233: 206: 179: 117: 97: 58:, in the sense of a 2605:2007CoAst.151...67S 2351:2007ApJ...671..581G 2313:2007CoAst.151....5G 2210:2007MNRAS.379.1498G 2160:2007AJ....134.1994B 2116:1982ApJ...263..835S 1606: 1543: 2081:10.1007/BF00648343 1948: 1925: 1826: 1716: 1684: 1666:dependent variable 1650: 1614: 1592: 1529: 1434: 1289: 1154: 1131: 896: 661: 246: 219: 192: 163:of white noise in 149: 103: 2614:10.1553/cia151s67 1951:{\displaystyle A} 1914: 1810: 1719:{\displaystyle A} 1607: 1544: 1418: 1364: 1284: 1126: 946: 891: 711: 656: 106:{\displaystyle K} 81:(rather than the 2800: 2788:Fourier analysis 2757: 2747: 2713: 2687: 2678:(3): 1031–1040. 2665: 2639: 2618: 2616: 2583: 2557: 2536: 2513: 2487: 2466: 2440: 2418: 2392: 2370: 2336: 2326: 2324: 2322:10.1553/cia151s5 2291: 2265: 2243: 2237: 2229: 2203: 2194:(4): 1498–1506. 2179: 2153: 2144:(5): 1994–1998. 2128: 2127: 2099: 2093: 2092: 2056: 2050: 2049: 2023: 2014:(3): 1353–1371. 2001: 1968:asteroseismology 1957: 1955: 1954: 1949: 1934: 1932: 1931: 1926: 1915: 1913: 1909: 1908: 1892: 1882: 1881: 1868: 1835: 1833: 1832: 1827: 1822: 1818: 1811: 1809: 1805: 1804: 1788: 1787: 1786: 1773: 1745: 1744: 1725: 1723: 1722: 1717: 1693: 1691: 1690: 1685: 1683: 1682: 1659: 1657: 1656: 1651: 1646: 1645: 1623: 1621: 1620: 1615: 1613: 1609: 1608: 1605: 1600: 1591: 1590: 1586: 1585: 1584: 1561: 1560: 1550: 1545: 1542: 1537: 1528: 1527: 1523: 1522: 1521: 1498: 1497: 1487: 1443: 1441: 1440: 1435: 1430: 1426: 1419: 1417: 1413: 1412: 1396: 1395: 1394: 1381: 1365: 1363: 1359: 1358: 1342: 1328: 1298: 1296: 1295: 1290: 1285: 1283: 1282: 1281: 1262: 1251: 1235: 1234: 1233: 1214: 1203: 1187: 1163: 1161: 1160: 1155: 1140: 1138: 1137: 1132: 1127: 1125: 1121: 1120: 1119: 1114: 1110: 1109: 1105: 1104: 1103: 1091: 1090: 1066: 1055: 1031: 1027: 1026: 1025: 1013: 1012: 992: 991: 981: 970: 947: 945: 944: 932: 930: 925: 924: 905: 903: 902: 897: 892: 890: 886: 885: 884: 879: 875: 874: 870: 869: 868: 856: 855: 831: 820: 796: 792: 791: 790: 778: 777: 757: 756: 746: 735: 712: 710: 709: 697: 695: 690: 689: 670: 668: 667: 662: 657: 655: 654: 653: 648: 647: 640: 639: 620: 609: 594: 593: 584: 583: 578: 577: 570: 569: 550: 539: 524: 523: 514: 513: 491: 480: 461: 460: 456: 455: 454: 435: 424: 404: 400: 399: 398: 379: 368: 342: 341: 319: 308: 289: 284: 283: 255: 253: 252: 247: 245: 244: 228: 226: 225: 220: 218: 217: 201: 199: 198: 193: 191: 190: 159:, the amplitude 158: 156: 155: 150: 145: 144: 132: 131: 112: 110: 109: 104: 34:obtained by the 2808: 2807: 2803: 2802: 2801: 2799: 2798: 2797: 2773: 2772: 2764: 2730:(1): 1239–252. 2716: 2668: 2621: 2586: 2539: 2533: 2516: 2469: 2421: 2373: 2334: 2329: 2294: 2246: 2230: 2182: 2135: 2132: 2131: 2101: 2100: 2096: 2058: 2057: 2053: 2021:physics/0703160 2003: 2002: 1998: 1993: 1981: 1964: 1940: 1939: 1900: 1893: 1873: 1869: 1844: 1843: 1796: 1789: 1778: 1774: 1768: 1764: 1736: 1731: 1730: 1708: 1707: 1700: 1674: 1669: 1668: 1637: 1629: 1628: 1576: 1569: 1565: 1552: 1551: 1513: 1506: 1502: 1489: 1488: 1485: 1481: 1452: 1451: 1404: 1397: 1386: 1382: 1376: 1372: 1350: 1343: 1329: 1307: 1306: 1273: 1236: 1225: 1188: 1169: 1168: 1146: 1145: 1095: 1082: 1078: 1074: 1040: 1036: 1035: 1017: 1004: 1000: 996: 983: 952: 948: 936: 916: 911: 910: 860: 847: 843: 839: 805: 801: 800: 782: 769: 765: 761: 748: 717: 713: 701: 681: 676: 675: 641: 631: 571: 561: 505: 462: 446: 409: 405: 390: 353: 349: 333: 290: 275: 261: 260: 236: 231: 230: 209: 204: 203: 182: 177: 176: 167:, depending on 136: 123: 115: 114: 95: 94: 91: 83:population mean 17: 12: 11: 5: 2806: 2804: 2796: 2795: 2790: 2785: 2775: 2774: 2771: 2770: 2763: 2762:External links 2760: 2759: 2758: 2714: 2666: 2630:(2): 577–584. 2619: 2584: 2548:(2): 601–608. 2537: 2531: 2514: 2478:(2): 571–574. 2467: 2431:(2): 497–505. 2419: 2383:(1): 239–248. 2371: 2359:10.1086/522880 2345:(1): 581–591. 2327: 2292: 2256:(1): 223–232. 2244: 2180: 2168:10.1086/522795 2130: 2129: 2124:10.1086/160554 2094: 2067:(2): 447–462. 2051: 1995: 1994: 1992: 1989: 1988: 1987: 1980: 1977: 1972:variable stars 1963: 1960: 1947: 1936: 1935: 1924: 1921: 1918: 1912: 1907: 1903: 1899: 1896: 1891: 1888: 1885: 1880: 1876: 1872: 1866: 1863: 1860: 1857: 1854: 1851: 1837: 1836: 1825: 1821: 1817: 1814: 1808: 1803: 1799: 1795: 1792: 1785: 1781: 1777: 1771: 1767: 1763: 1760: 1757: 1754: 1751: 1748: 1743: 1739: 1715: 1699: 1696: 1681: 1677: 1649: 1644: 1640: 1636: 1625: 1624: 1612: 1604: 1599: 1595: 1589: 1583: 1579: 1575: 1572: 1568: 1564: 1559: 1555: 1548: 1541: 1536: 1532: 1526: 1520: 1516: 1512: 1509: 1505: 1501: 1496: 1492: 1484: 1480: 1477: 1474: 1471: 1468: 1465: 1462: 1459: 1445: 1444: 1433: 1429: 1425: 1422: 1416: 1411: 1407: 1403: 1400: 1393: 1389: 1385: 1379: 1375: 1371: 1368: 1362: 1357: 1353: 1349: 1346: 1341: 1338: 1335: 1332: 1326: 1323: 1320: 1317: 1314: 1300: 1299: 1288: 1280: 1276: 1272: 1269: 1266: 1261: 1258: 1255: 1250: 1247: 1244: 1240: 1232: 1228: 1224: 1221: 1218: 1213: 1210: 1207: 1202: 1199: 1196: 1192: 1185: 1182: 1179: 1176: 1153: 1142: 1141: 1130: 1124: 1118: 1113: 1108: 1102: 1098: 1094: 1089: 1085: 1081: 1077: 1073: 1070: 1065: 1062: 1059: 1054: 1051: 1048: 1044: 1039: 1034: 1030: 1024: 1020: 1016: 1011: 1007: 1003: 999: 995: 990: 986: 980: 977: 974: 969: 966: 963: 959: 955: 951: 943: 939: 935: 928: 923: 919: 907: 906: 895: 889: 883: 878: 873: 867: 863: 859: 854: 850: 846: 842: 838: 835: 830: 827: 824: 819: 816: 813: 809: 804: 799: 795: 789: 785: 781: 776: 772: 768: 764: 760: 755: 751: 745: 742: 739: 734: 731: 728: 724: 720: 716: 708: 704: 700: 693: 688: 684: 672: 671: 660: 652: 646: 638: 634: 630: 627: 624: 619: 616: 613: 608: 605: 602: 598: 592: 587: 582: 576: 568: 564: 560: 557: 554: 549: 546: 543: 538: 535: 532: 528: 522: 517: 512: 508: 504: 501: 498: 495: 490: 487: 484: 479: 476: 473: 469: 465: 459: 453: 449: 445: 442: 439: 434: 431: 428: 423: 420: 417: 413: 408: 403: 397: 393: 389: 386: 383: 378: 375: 372: 367: 364: 361: 357: 352: 348: 345: 340: 336: 332: 329: 326: 323: 318: 315: 312: 307: 304: 301: 297: 293: 287: 282: 278: 274: 271: 268: 243: 239: 216: 212: 189: 185: 148: 143: 139: 135: 130: 126: 122: 102: 90: 87: 15: 13: 10: 9: 6: 4: 3: 2: 2805: 2794: 2791: 2789: 2786: 2784: 2781: 2780: 2778: 2769: 2766: 2765: 2761: 2755: 2751: 2746: 2741: 2737: 2733: 2729: 2725: 2721: 2715: 2711: 2707: 2703: 2699: 2695: 2691: 2686: 2681: 2677: 2673: 2667: 2663: 2659: 2655: 2651: 2647: 2643: 2638: 2633: 2629: 2625: 2620: 2615: 2610: 2606: 2602: 2598: 2594: 2590: 2585: 2581: 2577: 2573: 2569: 2565: 2561: 2556: 2551: 2547: 2543: 2538: 2534: 2532:0-521-85018-5 2528: 2524: 2520: 2515: 2511: 2507: 2503: 2499: 2495: 2491: 2486: 2481: 2477: 2473: 2468: 2464: 2460: 2456: 2452: 2448: 2444: 2439: 2434: 2430: 2426: 2420: 2416: 2412: 2408: 2404: 2400: 2396: 2391: 2386: 2382: 2378: 2372: 2368: 2364: 2360: 2356: 2352: 2348: 2344: 2340: 2333: 2328: 2323: 2318: 2314: 2310: 2306: 2302: 2298: 2293: 2289: 2285: 2281: 2277: 2273: 2269: 2264: 2259: 2255: 2251: 2245: 2241: 2235: 2227: 2223: 2219: 2215: 2211: 2207: 2202: 2197: 2193: 2189: 2188: 2181: 2177: 2173: 2169: 2165: 2161: 2157: 2152: 2147: 2143: 2139: 2134: 2133: 2125: 2121: 2117: 2113: 2109: 2105: 2098: 2095: 2090: 2086: 2082: 2078: 2074: 2070: 2066: 2062: 2055: 2052: 2047: 2043: 2039: 2035: 2031: 2027: 2022: 2017: 2013: 2009: 2008: 2000: 1997: 1990: 1986: 1983: 1982: 1978: 1976: 1973: 1969: 1961: 1959: 1945: 1922: 1919: 1916: 1910: 1905: 1901: 1897: 1894: 1889: 1886: 1883: 1878: 1874: 1870: 1864: 1858: 1852: 1849: 1842: 1841: 1840: 1823: 1819: 1815: 1812: 1806: 1801: 1797: 1793: 1790: 1783: 1779: 1775: 1769: 1765: 1761: 1758: 1755: 1749: 1741: 1729: 1728: 1727: 1713: 1705: 1697: 1695: 1679: 1675: 1667: 1663: 1647: 1642: 1638: 1634: 1610: 1602: 1597: 1593: 1587: 1581: 1577: 1573: 1570: 1566: 1562: 1557: 1553: 1546: 1539: 1534: 1530: 1524: 1518: 1514: 1510: 1507: 1503: 1499: 1494: 1490: 1482: 1478: 1472: 1469: 1466: 1460: 1457: 1450: 1449: 1448: 1431: 1427: 1423: 1420: 1414: 1409: 1405: 1401: 1398: 1391: 1387: 1383: 1377: 1373: 1369: 1366: 1360: 1355: 1351: 1347: 1344: 1339: 1336: 1333: 1330: 1324: 1318: 1312: 1305: 1304: 1303: 1286: 1278: 1274: 1270: 1267: 1264: 1259: 1256: 1253: 1248: 1245: 1242: 1238: 1230: 1226: 1222: 1219: 1216: 1211: 1208: 1205: 1200: 1197: 1194: 1190: 1183: 1180: 1177: 1174: 1167: 1166: 1165: 1151: 1128: 1122: 1116: 1111: 1106: 1100: 1096: 1092: 1087: 1083: 1079: 1075: 1071: 1068: 1063: 1060: 1057: 1052: 1049: 1046: 1042: 1037: 1032: 1028: 1022: 1018: 1014: 1009: 1005: 1001: 997: 993: 988: 984: 978: 975: 972: 967: 964: 961: 957: 953: 949: 941: 937: 933: 926: 921: 917: 909: 908: 893: 887: 881: 876: 871: 865: 861: 857: 852: 848: 844: 840: 836: 833: 828: 825: 822: 817: 814: 811: 807: 802: 797: 793: 787: 783: 779: 774: 770: 766: 762: 758: 753: 749: 743: 740: 737: 732: 729: 726: 722: 718: 714: 706: 702: 698: 691: 686: 682: 674: 673: 658: 650: 636: 632: 628: 625: 622: 617: 614: 611: 606: 603: 600: 596: 585: 580: 566: 562: 558: 555: 552: 547: 544: 541: 536: 533: 530: 526: 515: 510: 506: 502: 499: 496: 493: 488: 485: 482: 477: 474: 471: 467: 463: 457: 451: 447: 443: 440: 437: 432: 429: 426: 421: 418: 415: 411: 406: 401: 395: 391: 387: 384: 381: 376: 373: 370: 365: 362: 359: 355: 350: 346: 343: 338: 334: 330: 327: 324: 321: 316: 313: 310: 305: 302: 299: 295: 291: 285: 280: 276: 272: 269: 266: 259: 258: 257: 241: 237: 214: 210: 187: 183: 174: 170: 166: 165:Fourier space 162: 141: 137: 133: 128: 124: 100: 88: 86: 84: 80: 76: 75:random sample 72: 67: 65: 61: 57: 53: 49: 45: 41: 37: 33: 29: 25: 21: 2727: 2723: 2675: 2671: 2627: 2623: 2596: 2592: 2545: 2541: 2522: 2518: 2475: 2471: 2428: 2424: 2380: 2376: 2342: 2338: 2304: 2300: 2253: 2249: 2234:cite journal 2191: 2185: 2141: 2137: 2107: 2103: 2097: 2064: 2060: 2054: 2011: 2005: 1999: 1970:to identify 1965: 1962:Applications 1937: 1838: 1701: 1660:denotes the 1626: 1446: 1301: 1143: 92: 68: 60:type I error 43: 39: 23: 22:(acronym of 19: 18: 2110:: 835–853. 1704:time domain 79:sample mean 56:white noise 52:logarithmic 46:”) to each 28:time series 2777:Categories 1991:References 2754:123505620 2685:0812.1960 2637:0901.2573 2599:: 67–76. 2555:0710.2963 2485:0801.0683 2438:0711.0837 2390:0803.1721 2263:0801.0863 2201:0705.4603 2176:120843648 2151:0709.3393 1917:⋅ 1887:⁡ 1853:⁡ 1813:⋅ 1770:− 1762:⁡ 1738:Φ 1594:β 1578:θ 1574:− 1571:θ 1563:⁡ 1531:α 1515:θ 1511:− 1508:θ 1500:⁡ 1473:θ 1467:ω 1461:⁡ 1421:⋅ 1378:− 1370:⁡ 1337:⋅ 1313:ϕ 1271:ω 1268:⁡ 1257:− 1239:∑ 1223:ω 1220:⁡ 1209:− 1191:∑ 1181:θ 1178:⁡ 1152:θ 1097:θ 1093:− 1080:ω 1072:⁡ 1061:− 1043:∑ 1033:− 1019:θ 1015:− 1002:ω 994:⁡ 976:− 958:∑ 918:β 862:θ 858:− 845:ω 837:⁡ 826:− 808:∑ 798:− 784:θ 780:− 767:ω 759:⁡ 741:− 723:∑ 683:α 629:ω 626:⁡ 615:− 597:∑ 559:ω 556:⁡ 545:− 527:∑ 516:− 503:ω 497:⁡ 486:− 468:∑ 444:ω 441:⁡ 430:− 412:∑ 388:ω 385:⁡ 374:− 356:∑ 344:− 331:ω 325:⁡ 314:− 296:∑ 277:θ 270:⁡ 238:θ 211:β 184:α 169:frequency 48:amplitude 2710:54503935 2662:10408194 2580:11390524 2510:18481860 2463:18201762 2367:54866017 2307:: 5–25. 2288:54726017 2226:55678660 2046:15076973 1979:See also 1662:variance 32:spectrum 2732:Bibcode 2690:Bibcode 2642:Bibcode 2601:Bibcode 2560:Bibcode 2490:Bibcode 2443:Bibcode 2415:3032930 2395:Bibcode 2347:Bibcode 2309:Bibcode 2268:Bibcode 2206:Bibcode 2156:Bibcode 2112:Bibcode 2089:2671466 2069:Bibcode 2026:Bibcode 1664:of the 1164:, with 20:SigSpec 2752:  2708:  2660:  2578:  2529:  2508:  2461:  2413:  2365:  2286:  2224:  2174:  2087:  2044:  113:pairs 77:, the 64:random 2750:S2CID 2706:S2CID 2680:arXiv 2658:S2CID 2632:arXiv 2576:S2CID 2550:arXiv 2506:S2CID 2480:arXiv 2459:S2CID 2433:arXiv 2411:S2CID 2385:arXiv 2363:S2CID 2335:(PDF) 2284:S2CID 2258:arXiv 2222:S2CID 2196:arXiv 2172:S2CID 2146:arXiv 2085:S2CID 2042:S2CID 2016:arXiv 173:phase 2527:ISBN 2240:link 1920:sock 1911:> 1898:< 1816:sock 1807:> 1794:< 1648:> 1635:< 1627:and 1458:sock 1424:sock 1415:> 1402:< 1361:> 1348:< 1340:sock 171:and 2740:doi 2728:502 2698:doi 2676:494 2650:doi 2628:496 2609:doi 2597:151 2568:doi 2546:484 2498:doi 2476:481 2451:doi 2429:478 2403:doi 2381:483 2355:doi 2343:671 2317:doi 2305:151 2276:doi 2254:480 2214:doi 2192:379 2164:doi 2142:134 2120:doi 2108:263 2077:doi 2034:doi 2012:467 1884:log 1850:sig 1759:exp 1554:sin 1491:cos 1367:exp 1265:cos 1217:sin 1175:tan 1069:sin 985:sin 834:cos 750:cos 623:sin 553:cos 494:cos 438:sin 382:cos 322:sin 267:tan 161:pdf 66:?” 44:sig 2779:: 2748:. 2738:. 2726:. 2722:. 2704:. 2696:. 2688:. 2674:. 2656:. 2648:. 2640:. 2626:. 2607:. 2595:. 2591:. 2574:. 2566:. 2558:. 2544:. 2504:. 2496:. 2488:. 2474:. 2457:. 2449:. 2441:. 2427:. 2409:. 2401:. 2393:. 2379:. 2361:. 2353:. 2341:. 2337:. 2315:. 2303:. 2299:. 2282:. 2274:. 2266:. 2252:. 2236:}} 2232:{{ 2220:. 2212:. 2204:. 2190:. 2170:. 2162:. 2154:. 2140:. 2118:. 2106:. 2083:. 2075:. 2065:39 2063:. 2040:. 2032:. 2024:. 2010:. 1742:FA 1726:, 1694:. 229:, 202:, 2756:. 2742:: 2734:: 2712:. 2700:: 2692:: 2682:: 2664:. 2652:: 2644:: 2634:: 2617:. 2611:: 2603:: 2582:. 2570:: 2562:: 2552:: 2535:. 2512:. 2500:: 2492:: 2482:: 2465:. 2453:: 2445:: 2435:: 2417:. 2405:: 2397:: 2387:: 2369:. 2357:: 2349:: 2325:. 2319:: 2311:: 2290:. 2278:: 2270:: 2260:: 2242:) 2228:. 2216:: 2208:: 2198:: 2178:. 2166:: 2158:: 2148:: 2126:. 2122:: 2114:: 2091:. 2079:: 2071:: 2048:. 2036:: 2028:: 2018:: 1946:A 1923:. 1906:2 1902:x 1895:4 1890:e 1879:2 1875:A 1871:K 1865:= 1862:) 1859:A 1856:( 1824:. 1820:) 1802:2 1798:x 1791:4 1784:2 1780:A 1776:K 1766:( 1756:= 1753:) 1750:A 1747:( 1714:A 1680:k 1676:x 1643:2 1639:x 1611:] 1603:2 1598:0 1588:) 1582:0 1567:( 1558:2 1547:+ 1540:2 1535:0 1525:) 1519:0 1504:( 1495:2 1483:[ 1479:= 1476:) 1470:, 1464:( 1432:, 1428:) 1410:2 1406:x 1399:4 1392:2 1388:A 1384:K 1374:( 1356:2 1352:x 1345:2 1334:A 1331:K 1325:= 1322:) 1319:A 1316:( 1287:, 1279:k 1275:t 1260:1 1254:K 1249:0 1246:= 1243:k 1231:k 1227:t 1212:1 1206:K 1201:0 1198:= 1195:k 1184:= 1129:. 1123:) 1117:2 1112:] 1107:) 1101:0 1088:k 1084:t 1076:( 1064:1 1058:K 1053:0 1050:= 1047:l 1038:[ 1029:) 1023:0 1010:k 1006:t 998:( 989:2 979:1 973:K 968:0 965:= 962:k 954:K 950:( 942:2 938:K 934:2 927:= 922:0 894:, 888:) 882:2 877:] 872:) 866:0 853:k 849:t 841:( 829:1 823:K 818:0 815:= 812:l 803:[ 794:) 788:0 775:k 771:t 763:( 754:2 744:1 738:K 733:0 730:= 727:k 719:K 715:( 707:2 703:K 699:2 692:= 687:0 659:, 651:2 645:) 637:k 633:t 618:1 612:K 607:0 604:= 601:k 591:( 586:+ 581:2 575:) 567:k 563:t 548:1 542:K 537:0 534:= 531:k 521:( 511:k 507:t 500:2 489:1 483:K 478:0 475:= 472:k 464:K 458:) 452:k 448:t 433:1 427:K 422:0 419:= 416:k 407:( 402:) 396:k 392:t 377:1 371:K 366:0 363:= 360:k 351:( 347:2 339:k 335:t 328:2 317:1 311:K 306:0 303:= 300:k 292:K 286:= 281:0 273:2 242:0 215:0 188:0 147:) 142:k 138:x 134:, 129:k 125:t 121:( 101:K

Index

time series
spectrum
Discrete Fourier transform
amplitude
logarithmic
white noise
type I error
random
Lomb-Scargle periodogram
random sample
sample mean
population mean
pdf
Fourier space
frequency
phase
variance
dependent variable
time domain
asteroseismology
variable stars
Spectral density estimation
Astronomy and Astrophysics
arXiv
physics/0703160
Bibcode
2007A&A...467.1353R
doi
10.1051/0004-6361:20066597
S2CID

Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.

↑