@@ -556,7 +556,7 @@ information, to be defined below.
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556 | 556 | However, you should be aware that these "unconditional" moments do depend on |
557 | 557 | the initial distribution $N(\mu_0, \Sigma_0)$. |
558 | 558 | |
559 | | -#### Moments of the Observations |
| 559 | +#### Moments of the Observables |
560 | 560 | |
561 | 561 | Using linearity of expectations again we have |
562 | 562 | |
@@ -585,9 +585,8 @@ is not quite as good as knowing the full distribution.
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585 | 585 | However, there are some situations where these moments alone tell us all we |
586 | 586 | need to know. |
587 | 587 | |
588 | | -These are situations in which the mean vector and covariance matrix are **sufficient statistics** for the population distribution. |
| 588 | +These are situations in which the mean vector and covariance matrix are all of the **parameters** that pin down the population distribution. |
589 | 589 | |
590 | | -(Sufficient statistics form a list of objects that characterize a population distribution) |
591 | 590 | |
592 | 591 | One such situation is when the vector in question is Gaussian (i.e., normally |
593 | 592 | distributed). |
@@ -753,8 +752,7 @@ The black line is the population density of $y_T$ calculated from {eq}`lss_mgs_y
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753 | 752 | The histogram and population distribution are close, as expected. |
754 | 753 | |
755 | 754 | By looking at the figures and experimenting with parameters, you will gain a |
756 | | -feel for how the population distribution depends on the model primitives {ref}`listed above <lss_pgs>`, as intermediated by |
757 | | -the distribution's sufficient statistics. |
| 755 | +feel for how the population distribution depends on the model primitives {ref}`listed above <lss_pgs>`, as intermediated by the distribution's parameters. |
758 | 756 | |
759 | 757 | #### Ensemble Means |
760 | 758 | |
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