- Loading the packages
- Simple linear model (
*aka*a regression) - A linear model with a categorical predictor
- All with one function
- References

This vignette can be referred to by citing the package:

- Makowski, D., Ben-Shachar, M. S., & Lüdecke, D. (2019).
*bayestestR: Describing Effects and their Uncertainty, Existence and Significance within the Bayesian Framework*. Journal of Open Source Software, 4(40), 1541. https://doi.org/10.21105/joss.01541

Now that you’ve read the **Get started** section, let’s dive in the **subtleties of Bayesian modelling using R**.

Once you’ve installed the necessary packages, we can load `rstanarm`

(to fit the models), `bayestestR`

(to compute useful indices) and `insight`

(to access the parameters).

We will begin by conducting a simple linear regression to test the relationship between `Petal.Length`

(our predictor, or *independent*, variable) and `Sepal.Length`

(our response, or *dependent*, variable) from the `iris`

dataset which is included by default in R.

Let’s start by fitting the **frequentist** version of the model, just to have a reference point:

```
>
> Call:
> lm(formula = Sepal.Length ~ Petal.Length, data = iris)
>
> Residuals:
> Min 1Q Median 3Q Max
> -1.2468 -0.2966 -0.0152 0.2768 1.0027
>
> Coefficients:
> Estimate Std. Error t value Pr(>|t|)
> (Intercept) 4.3066 0.0784 54.9 <2e-16 ***
> Petal.Length 0.4089 0.0189 21.6 <2e-16 ***
> ---
> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
>
> Residual standard error: 0.41 on 148 degrees of freedom
> Multiple R-squared: 0.76, Adjusted R-squared: 0.758
> F-statistic: 469 on 1 and 148 DF, p-value: <2e-16
```

In this model, the linear relationship between `Petal.Length`

and `Sepal.Length`

is **positive and significant** (beta = 0.41, *t*(148) = 21.6, *p* < .001). This means that for each one-unit increase in `Petal.Length`

(the predictor), you can expect `Sepal.Length`

(the response) to increase by **0.41**. This effect can be visualized by plotting the predictor values on the `x`

axis and the response values as `y`

using the `ggplot2`

package:

```
library(ggplot2) # Load the package
# The ggplot function takes the data as argument, and then the variables
# related to aesthetic features such as the x and y axes.
ggplot(iris, aes(x=Petal.Length, y=Sepal.Length)) +
geom_point() + # This adds the points
geom_smooth(method="lm") # This adds a regression line
```

Now let’s fit a **Bayesian version** of the model by using the `stan_glm`

function in the `rstanarm`

package:

You can see the sampling algorithm being run.

Once it is done, let us extract the parameters (*i.e.*, coefficients) of the model.

```
> (Intercept) Petal.Length
> 1 4.4 0.40
> 2 4.5 0.37
> 3 4.3 0.41
> 4 4.4 0.40
> 5 4.3 0.41
> 6 4.3 0.42
```

As we can see, the parameters take the form of a lengthy dataframe with two columns, corresponding to the `intercept`

and the effect of `Petal.Length`

. These columns contain the **posterior distributions** of these two parameters. In simple terms, the posterior distribution is a set of different plausible values for each parameter.

Let’s look at the length of the posteriors.

```
> [1] 4000
```

Why is the size 4000, and not more or less?

First of all, these observations (the rows) are usually referred to as **posterior draws**. The underlying idea is that the Bayesian sampling algorithm (*e.g.*, **Monte Carlo Markov Chains - MCMC**) will *draw* from the hidden true posterior distribution. Thus, it is through these posterior draws that we can estimate the underlying true posterior distribution. **Therefore, the more draws you have, the better your estimation of the posterior distribution**. However, increased draws also means longer computation time.

If we look at the documentation (`?sampling`

) for the rstanarm `"sampling"`

algorithm used by default in the model above, we can see several parameters that influence the number of posterior draws. By default, there are **4** `chains`

(you can see it as distinct sampling runs), that each create **2000** `iter`

(draws). However, only half of these iterations are kept, as half are used for `warm-up`

(the convergence of the algorithm). Thus, the total is ** 4 chains * (2000 iterations - 1000 warm-up) = 4000** posterior draws. We can change that, for instance:

```
model <- stan_glm(Sepal.Length ~ Petal.Length, data=iris, chains = 2, iter = 1000, warmup = 250)
nrow(insight::get_parameters(model)) # Size (number of rows)
```

```
[1] 1500
```

In this case, as would be expected, we have ** 2 chains * (1000 iterations - 250 warm-up) = 1500** posterior draws. But let’s keep our first model with the default setup (as it has more draws).

Now that we’ve understood where these values come from, let’s look at them. We will start by visualizing the posterior distribution of our parameter of interest, the effect of `Petal.Length`

.

This distribution represents the probability (the y axis) of different effects (the x axis). The central values are more probable than the extreme values. As you can see, this distribution ranges from about **0.35 to 0.50**, with the bulk of it being at around **0.41**.

Congrats! You’ve just described your posterior distribution.

And this is at the heart of Bayesian analysis. We don’t need *p*-values, *t*-values or degrees of freedom: **everything is there**, within this posterior distribution.

Our description above is consistent with the values obtained from the frequentist regression (which resulted in a beta of **0.41**). This is reassuring! Indeed, **in most cases a Bayesian analysis does not drastically change the results** or their interpretation. Rather, it makes the results more interpretable and intuitive, and easier to understand and describe.

We can now go ahead and **precisely characterize** this posterior distribution.

Unfortunately, it is often not practical to report the whole posterior distributions as graphs. We need to find a **concise way to summarize it**. We recommend to describe the posterior distribution with **3 elements**:

- A
**point-estimate**which is a one-value summary (similar to the*beta*in frequentist regressions). - A
**credible interval**representing the associated uncertainty. - Some
**indices of significance**, giving information about the relative importance of this effect.

**What single value can best represent my posterior distribution?**

Centrality indices, such as the *mean*, the *median* or the *mode* are usually used as point-estimates - but what’s the difference between them? Let’s answer this by first inspecting the **mean**:

```
> [1] 0.41
```

This is close to the frequentist beta. But as we know, the mean is quite sensitive to outliers or extremes values. Maybe the **median** could be more robust?

```
> [1] 0.41
```

Well, this is **very close to the mean** (and identical when rounding the values). Maybe we could take the **mode**, that is, the *peak* of the posterior distribution? In the Bayesian framework, this value is called the **Maximum A Posteriori (MAP)**. Let’s see:

```
> MAP = 0.41
```

**They are all very close!** Let’s visualize these values on the posterior distribution:

```
ggplot(posteriors, aes(x = Petal.Length)) +
geom_density(fill = "orange") +
# The mean in blue
geom_vline(xintercept=mean(posteriors$Petal.Length), color="blue", size=1) +
# The median in red
geom_vline(xintercept=median(posteriors$Petal.Length), color="red", size=1) +
# The MAP in purple
geom_vline(xintercept=map_estimate(posteriors$Petal.Length), color="purple", size=1)
```

Well, all these values give very similar results. Thus, **we will choose the median**, as this value has a direct meaning from a probabilistic perspective: **there is 50% chance that the true effect is higher and 50% chance that the effect is lower** (as it divides the distribution in two equal parts).

Now that the have a point-estimate, we have to **describe the uncertainty**. We could compute the range:

```
> [1] 0.35 0.48
```

But does it make sense to include all these extreme values? Probably not. Thus, we will compute a **credible interval**. Long story short, it’s kind of similar to a frequentist **confidence interval**, but easier to interpret and easier to compute — *and it makes more sense*.

We will compute this **credible interval** based on the Highest Density Interval (HDI). It will give us the range containing the 89% most probable effect values. **Note that we will use 89% CIs instead of 95%** CIs (as in the frequentist framework), as the 89% level gives more stable results (Kruschke, 2014) and reminds us about the arbitrarity of such conventions (McElreath, 2018).

```
> # Highest Density Interval
>
> 89% HDI
> ------------
> [0.38, 0.44]
```

Nice, so we can conclude that **the effect has 89% chance of falling within the [0.38, 0.44] range**. We have just computed the two most important pieces of information for describing our effects.

However, in many scientific fields it not sufficient to simply describe the effects. Scientists also want to know if this effect has significance in practical or statistical terms, or in other words, whether the effect is important. For instnace, is the effect different from 0? So how do we **assess the significance of an effect**. How can we do this?

Well, in this particular case, it is very eloquent: **all possible effect values ( i.e., the whole posterior distribution) are positive and over 0.35, which is already substantial evidence the effect is not zero**.

But still, we want some objective decision criterion, to say if **yes or no the effect is ‘significant’**. One approach, similar to the frequentist framework, would be to see if the **Credible Interval** contains 0. If it is not the case, that would mean that our **effect is ‘significant’**.

But this index is not very fine-grained, isn’t it? **Can we do better? Yes.**

Imagine for a moment you are interested in how the weight of chickens varies depending on two different **feed types**. For this exampe, we will start by selecting from the `chickwts`

dataset (available in base R) two feed types of interest for us (*we do have peculiar interests*): **meat meals** and **sunflowers**.

```
library(dplyr)
# We keep only rows for which feed is meatmeal or sunflower
data <- chickwts %>%
filter(feed %in% c("meatmeal", "sunflower"))
```

Let’s run another Bayesian regression to predict the **weight** with the **two types of feed type**.

```
posteriors <- insight::get_parameters(model)
ggplot(posteriors, aes(x=feedsunflower)) +
geom_density(fill = "red")
```

This represents the **posterior distribution of the difference between meatmeal and sunflowers**. Seems that the difference is rather

```
> [1] 51
```

```
> # Highest Density Interval
>
> 89% HDI
> --------------
> [13.52, 91.37]
```

It makes you fat by around 51 grams (the median). However, the uncertainty is quite high: **there is 89% chance that the difference between the two feed types is between 14 and 91.**

Is this effect different from 0?

Testing whether this distribution is different from 0 doesn’t make sense, as 0 is a single value (*and the probability that any distribution is different from a single value is infinite*).

However, one way to assess **significance** could be to define an area around 0, which will consider as *practically equivalent* to zero (*i.e.*, absence of, or negligible, effect). This is called the **Region of Practical Equivalence (ROPE)**, and is one way of testing the significance of parameters.

**How can we define this region?**

Driing driiiing

– **The easystats team speaking. How can we help?**

– **I am Prof. Sanders. An expert in chicks… I mean chickens. Just calling to let you know that based on my expert knowledge, an effect between -20 and 20 is negligible. Bye.**

Well, that’s convenient. Now we know that we can define the ROPE as the `[-20, 20]`

range. All effects within this range are considered as *null* (negligible). We can now compute the **proportion of the 89% most probable values (the 89% CI) which are not null**, *i.e.*, which are outside this range.

```
> # Proportion of samples inside the ROPE [-20.00, 20.00]:
>
> inside ROPE
> -----------
> 5.00 %
```

**5% of the 89% CI can be considered as null**. Is that a lot? Based on our **guidelines**, yes, it is too much. **Based on this particular definition of ROPE**, we conclude that this effect is not significant (the probability of being negligible is too high).

Although, to be honest, I have **some doubts about this Prof. Sanders**. I don’t really trust **his definition of ROPE**. Is there a more **objective** way of defining it?

Prof. Sanders giving default values to define the Region of Practical Equivalence (ROPE).

**Yes.** One of the practice is for instance to use the **tenth ( 1/10 = 0.1) of the standard deviation (SD)** of the response variable, which can be considered as a “negligible” effect size (Cohen, 1988).

```
> [1] -6.2 6.2
```

Let’s redefine our ROPE as the region within the `[-6.2, 6.2]`

range. **Note that this can be directly obtained by the rope_range function :)**

```
> [1] -6.2 6.2
```

Let’s recompute the **percentage in ROPE**:

```
> # Proportion of samples inside the ROPE [-6.17, 6.17]:
>
> inside ROPE
> -----------
> 0.00 %
```

With this reasonable definition of ROPE, we observe that the 89% of the posterior distribution of the effect does **not** overlap with the ROPE. Thus, we can conclude that **the effect is significant** (in the sense of *important* enough to be noted).

Maybe we are not interested in whether the effect is non-negligible. Maybe **we just want to know if this effect is positive or negative**. In this case, we can simply compute the proportion of the posterior that is positive, no matter the “size” of the effect.

```
n_positive <- posteriors %>%
filter(feedsunflower > 0) %>% # select only positive values
nrow() # Get length
n_positive / nrow(posteriors) * 100
```

```
> [1] 98
```

We can conclude that **the effect is positive with a probability of 98%**. We call this index the **Probability of Direction (pd)**. It can, in fact, be computed more easily with the following:

```
> pd = 98.15%
```

Interestingly, it so happens that **this index is usually highly correlated with the frequentist p-value**. We could almost roughly infer the corresponding

```
> [1] 0.044
```

If we ran our model in the frequentist framework, we should approximately observe an effect with a *p*-value of 0.04. **Is that true?**

```
>
> Call:
> lm(formula = weight ~ feed, data = data)
>
> Residuals:
> Min 1Q Median 3Q Max
> -123.91 -25.91 -6.92 32.09 103.09
>
> Coefficients:
> Estimate Std. Error t value Pr(>|t|)
> (Intercept) 276.9 17.2 16.10 2.7e-13 ***
> feedsunflower 52.0 23.8 2.18 0.04 *
> ---
> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
>
> Residual standard error: 57 on 21 degrees of freedom
> Multiple R-squared: 0.185, Adjusted R-squared: 0.146
> F-statistic: 4.77 on 1 and 21 DF, p-value: 0.0405
```

The frequentist model tells us that the difference is **positive and significant** (beta = 52, p = 0.04).

**Although we arrived to a similar conclusion, the Bayesian framework allowed us to develop a more profound and intuitive understanding of our effect, and of the uncertainty of its estimation.**

And yet, I agree, it was a bit **tedious** to extract and compute all the indices. **But what if I told you that we can do all of this, and more, with only one function?**

Behold,`describe_posterior`

!

This function computes all of the adored mentioned indices, and can be run directly on the model:

```
> # Description of Posterior Distributions
>
> Parameter | Median | 89% CI | pd | 89% ROPE | % in ROPE | BF | Rhat | ESS
> -----------------------------------------------------------------------------------------------------------------
> (Intercept) | 276.853 | [247.820, 305.534] | 1.000 | [-6.175, 6.175] | 0 | 2.435e+11 | 0.999 | 3536.592
> feedsunflower | 50.991 | [ 13.516, 91.371] | 0.982 | [-6.175, 6.175] | 0 | 1.575 | 1.000 | 3535.028
```

**Tada!** There we have it! The **median**, the **CI**, the **pd** and the **ROPE percentage**!

Understanding and describing posterior distributions is just one aspect of Bayesian modelling… **Are you ready for more?** **Click here** to see the next example.

Cohen, J. (1988). *Statistical power analysis for the social sciences*.

Kruschke, J. (2014). *Doing bayesian data analysis: A tutorial with r, jags, and stan*. Academic Press.

McElreath, R. (2018). *Statistical rethinking: A bayesian course with examples in r and stan*. Chapman; Hall/CRC.