Empirical examination of stability under summability

3. Empirical examination of stability under summability

It is a remarkable feature of simulated realizations from near-IGARCH pro- cesses driven by fat-tailed innovations that they tend to exhibit SuS. GK demon- strated this property by estimating the tail index a of simulated GARCH and IGARCH observations for several values of S, the number of consecutive non- overlapping summed observations. In their subsequent note, Groenendijk et al. Ž . 1995 provided some theoretical insight explaining this phenomenon. It should be noted that, rather than using a general tail estimator, GK adopted that of Ž . McCulloch 1986 , which is specifically designed to estimate the tail index for Ž . iid stable Paretian data. Specifically, GK make the following observations. First, for a normal-GARCH Ž process, the closer the model comes to being IGARCH i.e., the closer c qd is 1 1 . to one , the higher the value of S has to be before the majority of estimated stable tail index values reach two. Second, they find that not only does the sum c qd 1 1 influence the convergence towards two, but also the values themselves, with, for a given value of sum c qd , larger values of c corresponding to slower conver- 1 1 1 Ž . gence i.e., higher S . Finally, using Student’s t innovations with 5 df, in short, Ž . t 5 , they show that these results still hold, but convergence is, compared to Ž . normal innovations, much slower. In fact, for t 5 -IGARCH models, evidence from their Table 2 and their further Monte Carlo runs suggests that the estimated stable tail index does not converge at all as S increases. It seems safe to say that Ž . this is not a phenomenon of just the t 5 distribution, but rather of general violation of normality, in particular, a Afattening of the tailsB. We now consider to what extent such results hold for the stable Paretian A-PARCH model using parameter values similar to ones estimated using real financial data. In particular, for each of the 24 combinations resulting from using c s0.1, 0.3, gs0, y0.50, d such that V s0.95, 0.99, and as1.6, 1.8, 2 1 1 g Ž . d Ž with constant values c s0.01, bs0 and ds1 , we generate S A-PARCH 1, a , b . 1 time series, each of length 5000. For each of these series, the stable tail index is estimated. Fig. 7 shows, separate for each of the 24 parameter constellations, the means of the estimated stable tail index for the ranges S s1, 2, . . . , 50 computed over the 100 simulated series. In comparison to GK, who used the McCulloch Ž . Ž 1986 estimator, we employ a modified Hill estimator Paolella, 1997; Mittnik . and Paolella, 1999 , which is also designed specifically for the tail index of iid stable Paretian observations, but possesses better small-sample properties than the Ž . McCulloch estimator see Appendix A . Recall that, while the innovations driving the simulated A-PARCH processes are iid stable Paretian, the observed output series are clearly not, so that the estimated stable tail index should not be expected to recover the tail index used to generate the innovations process. We would instead expect such an estimate to Ž . highly underestimate the actual tail index of the innovations, given that the GARCH effects induce a fattening of the tails in the output process. Initial Fig. 7. The means of the stable tail index estimates as a function of the summation length S over 100 1 Ž . Ž . Ž . Ž . simulated S -A-PARCH 1, 1 series, using a s2 solid , a s1.8 dashed and a s1.6 dotted . a ,0 Ž . inspection of Fig. 7 immediately verifies that i the unconditional estimate of a is Ž . indeed far below the true value; and ii the SuS phenomenon holds quite strongly d Ž . for S A-PARCH 1, 1 processes, with a near-linear downward shift accompany- a , b ing a decrease in a. Notice further that for given values of V , g and a , the g estimated stable tail index using c s0.1 is much higher than that for c s0.3, 1 1 which, for a s2, agrees with the findings of GK for their normal-IGARCH models. The main difference between the plots corresponding to V s0.95 from those g of V s0.99 is a downward shift, i.e., all things being equal, the closer V is to g g one, the lower the estimated tail index is. In addition, the variability of the estimated tail index increases with increasing V s0.99 as well as increasing c . g 1 The effect of decreasing is demonstrated by comparing the left and right panels; all other factors being equal, the estimated tail index undergoes a downward shift, which parallels the finding of GK using EGARCH models with non-zero asymme- try parameter. Note that this shift is not linear in a , with the drop being far more Ž . pronounced for large a-values near two , and minimal for smaller values of a.

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