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Table 12: Fitted Logistic AR(1) Model With Free 3 Para- Estimators

in S-Estimation of Nonlinear Regression Models With Dependent and Heterogeneous Observations
by Shinichi Sakata, Halbert White 2001
"... In PAGE 39: ... Given the encouraging result from S50, we now t the logistic AR model to the data without xing 3, which is nonlinear in parameters. The tted values are reported in Table12 . The estimated standard errors... In PAGE 40: ...Table12 may not be appropriate for OLS, S10, and S30, because the estimator of the covariance matrix used in the table assumes that all parameters are identi ably unique. The S50 estimate of 3 is 1.... ..."
Cited by 1

TABLE I COMBINATIONAL MODEL-FREE FAULT DIAGNOSIS

in Fault diagnosis and logic debugging using Boolean satisfiability
by Er Smith, Student Member, Andreas Veneris Member, Moayad Fahim, Ali Student Member, Anastasios Viglas Member 2005
Cited by 10

TABLE III COMBINATIONAL MODEL-FREE LOGIC DEBUGGING

in Fault diagnosis and logic debugging using Boolean satisfiability
by Er Smith, Student Member, Andreas Veneris Member, Moayad Fahim, Ali Student Member, Anastasios Viglas Member 2005
Cited by 10

TABLE IV SEQUENTIAL MODEL-FREE FAULT DIAGNOSIS

in Fault diagnosis and logic debugging using Boolean satisfiability
by Er Smith, Student Member, Andreas Veneris Member, Moayad Fahim, Ali Student Member, Anastasios Viglas Member 2005
Cited by 10

Table 3 shows the results for the model free con- troller using two actions. Due to the more di - cult task, more runs are needed to achieve to bal- ance the pole. The resulting controller quality com- pares very well to the performance achieved with the model based approach. For nearly all start- ing positions in the working region, balancing of the pole was possible, and the majority of positions ended in a stable state.

in Aspects of Learning Neural Control
by Martin Riedmiller, Komplexitat Und Deduktionssyteme
"... In PAGE 6: ... Table3 : Results for the MFRA two-actions con- troller IV. Conclusions The paper attempts to classify controller design techniques with respect to the available a priori knowledge.... ..."

TABLE I QBF-BASED VERSUS SAT-BASED MODEL-FREE FAULT DIAGNOSIS

in Fault diagnosis using quantified boolean formulas
by Hratch Mangassarian, Andreas Veneris, Marco Benedetti 2007
Cited by 1

Table 7.1: Model-free diagnosis of single stuck-at faults.

in Diagnosis of Combinational Logic Circuits Using Boolean Satisfiability
by Alexander D. S. Smith

Table 7.3: Model-free diagnosis of single gate replacement errors.

in Diagnosis of Combinational Logic Circuits Using Boolean Satisfiability
by Alexander D. S. Smith

TABLE 6.1. Performance of model-free fault detection for various faults

in Acknowledgments
by Venkata S Vongala 2005

Table 3. Broken power{law ts with galactic and free absorption. For these datasets, the broken power-law model is statistically preferred with respect to a single power-law model (the F{tests in the last column are against the single power{law model with free absorption)

in unknown title
by unknown authors 2001
"... In PAGE 4: ... 1989). The results from the single power-law ts are reported in Table 2, while Table3 reports the broken power-law ts parame- ters. Adopting a conservative approach, we assessed the presence of a spectral break when the broken power-law model was signi cantly better, according to the F{test, even with respect to the single power{law model with free absorption.... In PAGE 5: ...rrors at 68% conf. level for 3 and 4 parameters of interest ( 2 =3:52 and 4.72 respectively). adopting an absorption value greater than the galactic one. In most cases, however, the broken power{law models with galactic absorbing columns provided even better ts (according to the F{test, see Table3 ). For 1ES 0033+595 and PKS 0548{322, instead, there is evidence for a higher column density also using the broken power{law models.... In PAGE 5: ... The spectrum is characterized by a curved shape, which is better t- ted by a broken power-law than by a single power-law model (with both xed and free absorption). The best t, however, still requires a column density in excess of the galactic value (see Table3 ), with high signi cance (F{test gt; 99:8%). The spectral indices before and after the break Fig.... In PAGE 10: ....2.7. H 2356{309 The spectrum of this source is not compatible with a sin- gle power{law model: there is clear evidence for a convex spectral shape, that is best tted by a broken power{law with high signi cance ( gt;99.9%, see Table3 ). This locates the synchrotron peak around 1.... ..."
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