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Article

Bayesian Sensitivity Analysis for VaR and CVaR Employing Distorted Band Priors

by
José Pablo Arias-Nicolás
1,†,
María Isabel Parra
1,†,
Mario M. Pizarro
2,*,† and
Eva L. Sanjuán
1,†
1
Department of Mathematics, University of Extremadura, 06006 Badajoz, Spain
2
Department of Economics and Statistics, University of León, 24071 León, Spain
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Axioms 2024, 13(2), 77; https://doi.org/10.3390/axioms13020077
Submission received: 21 December 2023 / Revised: 16 January 2024 / Accepted: 22 January 2024 / Published: 24 January 2024
(This article belongs to the Special Issue Computational Statistics and Its Applications)

Abstract

:
In the context of robust Bayesian analysis, studies mainly focus on computing the range of some quantities of interest when the prior distribution varies in a class. We use the concept of distorted bands to introduce a family of priors on the shape parameter of the Generalized Pareto distribution. We show how certain properties of the likelihood ratio order allow us to propose novel sensitivity measures for Value at Risk and Conditional Value at Risk, which are the most useful and reliable risk measures. Although we focus on the Generalized Pareto distribution, which is essential in Extreme Value Theory, the new sensitivity measures could be employed for all the distributions that verify certain conditions related to likelihood ratio order. A thorough simulation study was carried out to perform a sensitivity analysis, and two illustrative examples are also provided.

1. Introduction

In Bayesian analysis, the choice of a prior distribution is a crucial issue. Without the expert’s information, we can only implement the process at our own will (using Jeffreys’ prior and other uninformative priors). The considerations of classes of priors and loss functions is the starting point for many developments in Bayesian sensitivity analysis, also called robust Bayesian analysis. Bayesian sensitivity analysis aims to quantify and model the uncertainty induced by the choice of the prior, likelihood, or loss [1,2]. Excellent surveys of Bayesian sensitivity analysis with respect to the prior are found in [3,4], whereas sensitivity regarding the loss function was considered in [5,6,7,8,9], among others. Some interesting applications can be found in [10,11].
In order to model the uncertainty of the prior information, a class of prior distributions is generally employed. Therefore, parametric classes, ϵ -contaminated classes [1], band classes, or quantile classes have been defined (see [2,12] for a general revision).
Distorted band classes were defined in [13] and were employed to define a class of priors in [14], which was called distorted band priors. Later, Ref. [15] applied them to insurance problems and [16] employed them in a collective risk model for insurance claims. More recently, Ref. [17] extended the concept of distorted bands to the multivariate case.
In this work, we employ distorted bands for prior distribution in order to make a Bayesian sensitivity analysis for the most useful and reliable risk measures employed in Extreme Value Theory.
Extreme Value Theory (EVT) is the science that studies rare events and employs statistical tools to model and predict them. It has been widely developed in Finance and Insurance, when the interest is focused on observations that differ significantly from the majority of data [18,19,20,21]. EVT provides statistical models to compute extreme risk measures, such as Value at Risk (VaR), Conditional Value at Risk (CVaR), and Return Level. Some other ways of measuring extreme risk were proposed by [22]. They are used, for example, to study the behavior of extreme returns on investment portfolios [23,24] and involve extreme quantiles estimation. There are several reasons why it is important to compute accurate estimates for the most employed risk measures, VaR and CVaR. From an economic point of view, underestimation of risk could obviously cause immense problems for banks and other participants in financial markets. On the other hand, an overestimation of risk may cause one to allocate too much capital as a cushion for risk exposures, having a negative effect on profits. Therefore, precise estimates of risk measures are obviously desirable.
A distribution of probability that plays an essential role in EVT is the Generalized Pareto distribution (GPD). Loosely speaking, Refs. [25,26] showed that, when we consider the distribution of data above a certain threshold u, it can usually be approximated by a properly scaled GPD as u tends to the endpoint of the distribution. Several methods have been developed for inferring the parameters of the GPD [27,28]. From a Bayesian point of view, Refs. [29,30] employed Markov chain Monte Carlo methods, Ref. [31] employed Jeffrey’s prior and the Metropolis–Hastings algorithm, and ref. [32] employed GPD itself as prior distribution. Mixture models were first proposed by [33], and afterwards, Ref. [34] studied an additive mixture model, where one of the components is the GPD, to make Bayesian inference on extreme quantiles. In addition, Ref. [35] defined a combination of mixture of Gamma below the threshold and a GPD above it. Afterwards, Ref. [36] also used a mixture model and focused on estimating the threshold. More recently, Ref. [37] employed all the data available to make estimations, using relations between the parameters of the baseline distribution and the parameters of the limit GPD distribution, following a similar idea developed in [38] for the Gumbel distribution. For both works, considered priors were highly informative.
The main novelty of this work is the proposal of sensitivity and relative sensitivity measures for VaR and CVaR, by introducing distorted bands for prior distributions. We focus on GPD distribution, because of its importance in EVT, and make use of properties related to the likelihood ratio order to define the sensitivity measures. The distorted band prior is defined on the shape parameter of the GPD. The measures of sensitivity and relative sensitivity are valid for all the distributions that fulfill condition (10) from Proposition 1, like Gamma or Weibull distributions.
In Section 2, we introduce the concept of distorted bands and show how we can use them to define bands for priors on the shape parameter of a GPD and the properties associated with them. In Section 3, we provide the definitions of VaR and CVaR and an essential result that allows us to define the new sensitivity measures for VaR and CVaR.
In Section 4, we describe a thorough simulation study in which we performed a sensitivity analysis employing the new sensitivity measures.
Finally, in Section 5, we provide two illustrative examples with real-life applications in two different fields, in order to show the usefulness of the sensitivity measures.

2. Distorted Band Priors

We recall the definition of the likelihood ratio order for two random variables and the concept of distortion function.
Let X and Y be absolutely continuous random variables with probability density functions (pdfs) f X and f Y , respectively. X is said to be smaller than Y in the likelihood ratio order, and we denote it by X l r Y (or f X l r f Y ), if the ratio
f Y ( t ) f X ( t )
increases over the union of the supports of the two pdfs.
A distortion function is a non-decreasing continuous function h : 0 , 1 0 , 1 such that h ( 0 ) = 0 and h ( 1 ) = 1 .
Definition 1.
Given a random variable X and a distortion function h, we call X distorted by h, and we denote it as X h ; the random variable has the distribution function
F X h ( x ) = h F X ( x ) = h F X x .
If F X h is differentiable, then, taking the derivative in Equation (2), we obtain the distorted density function of X h
f X h ( x ) = h F X ( x ) f X ( x ) .
In a Bayesian framework, let π denote a prior distribution over the set of states Θ , with pdf π ( θ ) , where θ represents the unknown parameter. After taking into account the observed data x, let π x denote the posterior distribution. Let π h and π h , x denote the distorted distributions π and π x by h, respectively.
In addition, let Y π x denote the random variable of the posterior predictive distribution associated with π x , with the density function
f π x ( y | x ) = Θ f ( y | θ ) π x ( θ ) d θ ,
and Y π h , x denote the random variable of the posterior predictive distribution associated with  π h , x .
Although priors can be distorted according to different criteria, Ref. [14] were in favor of the use of convex and concave distortion functions because of their desirable properties when we compare the original prior with the distorted one. That is, if h 1 and h 2 are distortion functions, with h 1 being concave and h 2 convex, it follows from Lemma 1 in [14] that
π h 1 l r π l r π h 2 .
Inspired by this last property, Ref. [14] defined the distorted band as follows:
Definition 2.
The distorted band  Γ h 1 , h 2 , π  associated with π based on h 1 and h 2 , a concave distortion function and a convex distortion function, respectively, is defined as
Γ h 1 , h 2 , π = { π : π h 1 l r π l r π h 2 } .
As an immediate consequence, it was shown by [14] that the distorted posterior distributions π h 1 , x and π h 2 , x are also lower and upper bounds for the class of all posteriors π x because they interit the likelihood ratio order, i.e., for all π Γ h 1 , h 2 , π ; then,
π h 1 , x l r π x l r π h 2 , x .
Due to the fact that Definition 2 is based on h 1 and h 2 , we can provide many possible bands just considering different concave and convex distortion functions. Of course, the choice of those functions cannot be arbitrary and should represent the uncertainty about the prior belief in each problem. For example, a convex (concave) distortion function will give more (less) weight to larger values.
A typical way of measuring a distortion is given by the classical power functions
h 1 ( x ) = 1 ( 1 x ) α   and   h 2 ( x ) = x α , α > 1 ,
where it is well known that if we take α = n N in Equation (8), then π h 1 and π h 2 can be interpreted as the minimum and the maximum, respectively, of an independent and identically distributed sample of size n that comes from the basis prior distribution π . Therefore, let Γ α be the distorted band associated with π and h 1 and h 2 given by (8), for a fixed α > 1 .
As we commented in the Introduction, the Generalized Pareto distribution (GPD) is essential in Extreme Value Theory. We will deduce some properties about the likelihood ratio order and distorted bands for the GPD.
Definition 3.
Given a random variable X, we say that it follows a GPD with parameters θ, σ, X G P D ( θ , σ ) , if its distribution function is
G ( x | θ , σ ) = 1 1 x σ 1 / θ ,
with support 0 x σ , θ > 0 , where θ and σ are the shape and scale parameters, respectively.
An interesting property of the GPD that allows us to establish an order is the following.
Proposition 1.
Let X θ be a random variable that follows a GPD with shape parameter θ. If X θ 1 , X θ 2 follow GPD with the same scale σ, then
X θ 1 l r X θ 2 , f o r a l l 0 < θ 1 < θ 2 .
Proof. 
If X θ 1 GPD ( θ 1 , σ ) and X θ 2 GPD ( θ 2 , σ ) , then
f X θ 2 ( t ) f X θ 1 ( t ) = θ 1 θ 2 1 t σ 1 θ 2 1 θ 1 ,
where 0 t σ . For all 0 < θ 1 < θ 2 , it is easy to prove that this ratio increases over the support ( 0 , σ ) . Therefore, X θ 1 l r X θ 2 .    □
Proposition 2.
Let Y GPD ( θ , σ ) be a random variable with uncertainty in the shape parameter θ (conditionally independent with x under θ), and let the scale parameter σ be fixed. Let π be a prior distribution and Γ α a distorted band associated with π based on h 1 and h 2 . For all sample x and for all π Γ α
Y π h 1 , x l r Y π x l r Y π h 2 , x .
Proof. 
Let Y θ , x and Y θ , x be two GPDs with shape parameters θ , θ Θ , such that θ < θ . Then, by Proposition 1, Y θ , x l r Y θ , x .
For all π Γ α , it is verified that π h 1 , x l r π x l r π h 2 , x ; then, for posterior predictive distributions,
Y π h 1 , x l r Y π x l r Y π h 2 , x
due to Theorem 10 in [39].    □
It is clear that all the families of random variables X θ verifying that X θ 1 l r X θ 2 when θ 1 < θ 2 will also verify (11) from Proposition 2 for a distorted band prior Γ α . Examples of these distributions are Gamma on parameter α and Weibull on both parameters. Therefore, the following results could also be developed for the cited distributions.

3. Bayesian Sensitivity Analysis for VaR and CVaR

As we mentioned in the Introduction, we are going to focus on two important risk measures that are widely employed: Value at Risk (VaR) and Conditional Value at Risk (CVaR).
Definition 4.
Let X be a random variable representing loss. Given a parameter 0 < p < 1 , the Value-at-Risk ( V a R p ) of X is the p-quantile of the distribution X
V a R p ( X ) = inf { x : P ( X x ) p } ,
and the Conditional Value-at-Risk ( C V a R p ) of X is
C V a R p ( X ) = E X | X V a R p ( X ) .
VaR p ( X ) is understood as the minimum loss that will not be exceeded with probability p, and we can understand it as the highest loss in the p · 100 % best cases. CVaR p ( X ) is the expected loss, conditioned on the fact that the loss exceeds the VaR p ( X ) at the given confidence level p · 100 % . It is an alternate measure to VaR p ( X ) , more sensitive to the shape of the tail of the loss distribution.
Proposition 3.
If Y G P D ( θ , σ ) , then
V a R p ( Y π h 1 , x ) V a R p ( Y π x ) V a R p ( Y π h 2 , x ) ,
C V a R p ( Y π h 1 , x ) C V a R p ( Y π x ) C V a R p ( Y π h 2 , x ) ,
for all π Γ α .
Proof. 
Due to Proposition 2, if Y GPD ( θ , σ ) ,
Y π h 1 , x l r Y π x l r Y π h 2 , x ,
for all sample x and π Γ α . In addition, we have to apply the properties
X l r Y VaR p ( X ) VaR p ( Y ) ,
X l r Y CVaR p ( X ) CVaR p ( Y ) .
They can be easily deduced taking into account that, if X l r Y , then F Y ( x ) F X ( x ) , for all x in the union of the supports. Therefore,
VaR p ( X ) = inf { F X ( x ) p } inf { F Y ( x ) p } = VaR p ( Y ) ,
and
CVaR p ( X ) = E X | X VaR p ( X ) E Y | Y VaR p ( Y ) = CVaR p ( Y ) .
   □
Corollary 1.
For all 0 < p < 1 and for the prior distribution π , which belong to a distorted band associated to π, Γ α , it is verified that
sup π Γ α V a R p ( Y π x ) = V a R p ( Y π h 2 , x ) ,
inf π Γ α V a R p ( Y π x ) = V a R p ( Y π h 1 , x ) ,
sup π Γ α C V a R p ( Y π x ) = C V a R p ( Y π h 2 , x ) ,
inf π Γ α C V a R p ( Y π x ) = C V a R p ( Y π h 1 , x ) .
Proof. 
It is a direct consequence of Proposition 3.    □
The sensitivity analysis is essential in Bayesian analysis and decision theory. The main differences among works in Bayesian sensitivity are about the choice of the classes and the sensitivity measures. In most papers about Bayesian robustness, the range of the posterior expectation of a quantity of interest g ( θ ) , with priors varying in a class Γ ,
sup π Γ E π x [ g ( θ ) ] inf π Γ E π x [ g ( θ ) ] ,
has been proposed as measure of sensitivity (global robustness).
The range is the most important sensitivity measure in global robustness. It has a simple interpretation: when Γ reasonably reflects the uncertainty in the prior, a “small” range indicates robustness. On the other hand, a “large” range is an indication that there is lack of robustness, and we should obtain more information.
We have shown that considering the distorted band, both the VaR and CVaR for the posterior predictive distributions are ordered too. This means that the range of these measures can be computed determining only VaR and CVaR of the posterior predictive distortion distributions. If we compute this range with respect to the VaR and CVaR, we will have a relative sensitivity measure. Consequently, we can define two sensitivity measures for VaR and CVaR of posterior predictive distributions, when the prior distribution belongs to a class of prior distributions associated with π , Γ α .
Definition 5.
Given a distorted band Γ α with α > 1 , we define the following sensitivity measures for the VaR and CVaR of the posterior predictive distributions as
S V a R p ( Γ α ) = V a R p ( Y π h 2 , x ) V a R p ( Y π h 1 , x ) ,
S C V a R p ( Γ α ) = C V a R p ( Y π h 2 , x ) C V a R p ( Y π h 1 , x ) .
To provide more information on the sensitivity analysis, we will also define relative sensitivity measures over the VaR and CVaR, based on the relative measures proposed by [9].
Definition 6.
Relative Sensitivity measures are defined as
R S V a R p ( Γ α ) = S V a R p ( Γ α ) V a R p ( Y π x ) ,
R S C V a R p ( Γ α ) = S C V a R p ( Γ α ) C V a R p ( Y π x ) .
If these sensitivity measures are small, we will say the distorted band class is robust. Otherwise, a more precise distorted band class or another reference prior should be chosen.

4. Simulations

We considered a sample of size n of a random variable X GPD ( θ , σ ) with fixed scale parameter σ = 1 and three prior distributions for the shape parameter θ , π ( θ ) : an inverse gamma, Inv Γ ( a , b ) , an inverse χ 2 ( k ) , and a Pareto distribution, Pareto ( c , x m ) . Let Γ α be the distorted prior band for α > 1 .
For all the priors, the posterior distribution is an inverse gamma with hyperparameters γ + n and β + T n ,
π x Inv Γ ( γ + n , β + T n ) , with T n = i = 1 n ln 1 x i σ ,
where γ = a , k / 2 , c and β = b , 1 / 2 , 0 .
Then, we fixed γ = 3 , β = 0.5 , and considered three representative values of α , α = 1.5 , 3 , 6 , and samples of size n = 1 , 10 , 100 . For all the combinations of these hyperparameters, 100,000 values of the random variable Y π x GPD ( θ , σ ) were generated. We conducted 100 replications, in order to determine the sensitivity measures for VaR and CVaR, taking the mean of each measure.
In addition, we took different values of θ = 0.01 , 0.04 , 0.16 , 0.32 , 0.64 , 1.28 , 2.56 . Figure 1, Figure 2, Figure 3 and Figure 4 show sensitivity measures for different values of p, taking different sizes of sample (columns) and distortion values (rows). In each figure, the blue lines correspond to θ = 0.01 , the red lines represent θ = 2.56 , and the dashed black lines between them are ordered by the values of θ = 0.04 , 0.16 , 0.32 , 0.64 , 1.28 .
We can notice the interaction between the values of θ and p in Figure 2 and Figure 3. For the different values of the shape parameter θ , we can see the different behaviors of the variations in the sensitivity measures when the values of p change.
Differences in both measures are larger when the distortion (given by α ) increases and also for large sizes of the dataset (n). Notice that for each size of the dataset n, the shape of the curves associated with θ is similar, and the maximum value of the sensitivity measure becomes smaller when n is larger.
However, the interaction between θ and p disappears when we plot the relative sensitivity measures (see Figure 3 and Figure 4). In this case, the measures are ordered by the values of θ ; they are larger for small datasets ( n = 1 ) and smaller if we have many data ( n = 100 ). As in the previous measures, larger distortion also produces larger values of the measures.

5. Applications

In this Section, we show the usability of the new measures of sensitivity for VaR and CVaR for very different applications, with real-life data.
In the first one, we have a small dataset related to the stock index IBEX35, while for the second example, we have a larger dataset with air pollutants PM 2.5.

5.1. Iberia Index Dataset

In Spain, the most important stock index is the Iberia Index or IBEX35. This index is equivalent to the S&P500 index. For this study, the data of IBEX35’s daily closing for year 2022 were selected [40]. The dataset comprises a sample of 257 values.
Usually, the variable of interest to compute risk measures is the daily logarithmic return of stock index, defined by
R t = ln P t P t 1 ,
where P t and P t 1 indicate the stock index on days t and t 1 , respectively.
The values that exceed the 0.9 order quantile are considered extreme values and relocated. The resulting dataset is small, with 26 values. We can see the histogram of the dataset values on Figure 5, fitted to a GPD (0.06, 15.46). The estimations for θ and σ were computed using the function gpd from evir library [41] of R.
Then, we set α = 1.5 , 3 , 6 , fixed σ = 15.46 , and took a prior distribution Inv Γ ( 1.5 , 0.5 ) for the parameter θ . To determine the sensitivity measures for VaR and CVaR, we generated 100,000 values of the random variable Y π x GPD ( θ , σ ) , taking the mean of each measure. Figure 6 shows the sensitivity measures (upper charts) and relative sensitivity (lower charts) measures of VaR and CVaR for different values of p.
As we expected, the values for all the sensitivity measures are larger for large values of α . In addition, for each measure, the curves exhibit the same behavior for all the values of α , reaching the maximum for the same value of p.

5.2. Particulate Matter 2.5 Dataset

Particulate matter (PM) is a mixture of solid particles and liquid droplets that can be inhaled and cause serious health problems. When particulate matter is less than 2.5 micrometers in diameter, it is known as PM 2.5, and it is considered to be especially dangerous for human health. In this context, studying the tail distribution of the levels of PM 2.5 and making a sensitivity analysis for VaR and CVaR can be undoubtedly useful.
We considered values of the levels of PM 2.5 measured in μ g/m3 for the Period 2011–2022 from Madrid (Spain), publicly available on the website [42]. The dataset comprises a sample of 10845 observations. As in the previous example, the values that exceed the threshold u = q 0.9 , relocated, were considered as extreme values.
The resulting dataset consists of 1028 values. We adjusted a GPD distribution with the function gpd, obtaining values for θ = 0.06 and σ = 105.72 . Figure 7 shows the histogram of the extreme dataset, together with the GPD (0.06, 105.72) density function.
We set α = 1.5 , 3 , 6 , fixed σ = 105.72 , and considered a prior distribution Inv Γ ( 1.5 , 0.5 ) for the parameter θ . To determine the sensitivity measures for VaR and CVaR, we generated 100,000 values of the random variable Y π x GPD ( θ , σ ) , taking the mean of each measure. Figure 8 shows the sensitivity measures (upper charts) and relative sensitivity (lower charts) measures of VaR and CVaR for different values of p.
As we can see in Figure 8, the graphs for the sensitivity measures are very similar to the graphs for the previous example (Figure 6): for a larger distortion α , the measures are also larger. For each measure, the curves show similar behaviors.

6. Conclusions

  • We provided sensitivity measures for the VaR p and CVaR p of the GPD distribution when the prior distribution on the shape parameter varies on a class Γ α defined using the concept of distorted bands.
  • The definitions of the sensitivity measures SVaR p Γ α and SCVaR p Γ α and the relative sensitivity measures RSVaR p Γ α and RSCVaR p Γ α were made using a property related to likelihood ratio order on the shape parameter θ of the GPD. Therefore, it could be extended to other distributions that fulfill that property for a parameter.
  • An extensive simulation study was carried out in order to perform a sensitivity analysis, for different values of θ , sizes of the dataset n, and the distortion parameter α , when p ( 0 , 1 ) . We concluded that there is interaction between the parameters θ and p for the sensitivity measures SVaR p Γ α and SCVaR p Γ α . The relative sensitivity measures RSVaR p Γ α and RSCVaR p Γ α are not affected by such interaction. For all four measures, the values are larger when the distortion ( α ) increases and when the size of the dataset is smaller. For each value of θ , the shape of the curves for the sensitivity measures versus p are similar.
  • We illustrated the practical use of the sensitivity measures with two examples: for data from the IBEX35 index and PM2.5 air pollutants.

Author Contributions

Conceptualization, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Methodology, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Software, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Validation, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Formal analysis, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Investigation, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Resources, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Data curation, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Writing—original draft, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Writing—review & editing, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Visualization, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Supervision, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Project administration, J.P.A.-N., M.I.P., M.M.P. and E.L.S.; Funding acquisition, J.P.A.-N., M.I.P., M.M.P. and E.L.S. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by MCIN/AEI/10.13039/501100011033 and ERDF A way of making Europe as part of R&D&I Project PID2021-122209OB-C32.

Data Availability Statement

Iberia Index dataset is available on the website [40] and Particulate Matter 2.5 dataset is available on the website [42].

Conflicts of Interest

The authors declare no conflicts of interest. The funders had no role in the design of the study; in the collection, analyses, or interpretation of data; in the writing of the manuscript; or in the decision to publish the results.

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Figure 1. Sensitivity of VaR p versus p for different values of α (rows) and n (columns).
Figure 1. Sensitivity of VaR p versus p for different values of α (rows) and n (columns).
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Figure 2. Sensitivity of CVaR p versus p for different values of α (rows) and n (columns).
Figure 2. Sensitivity of CVaR p versus p for different values of α (rows) and n (columns).
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Figure 3. Relative sensitivity of VaR p versus p for different values of α (rows) and n (columns).
Figure 3. Relative sensitivity of VaR p versus p for different values of α (rows) and n (columns).
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Figure 4. Relative sensitivity of CVaR p versus p for different values of α (rows) and n (columns).
Figure 4. Relative sensitivity of CVaR p versus p for different values of α (rows) and n (columns).
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Figure 5. Histogram of IBEX35 extreme values. The red curve represents the density of the GPD ( 0.06 , 15.46 ) .
Figure 5. Histogram of IBEX35 extreme values. The red curve represents the density of the GPD ( 0.06 , 15.46 ) .
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Figure 6. Sensitivity (upper charts) and relative sensitivity (lower charts) of VaR p (left charts) and CVaR p (right charts) versus p for different values of α for Iberia index dataset.
Figure 6. Sensitivity (upper charts) and relative sensitivity (lower charts) of VaR p (left charts) and CVaR p (right charts) versus p for different values of α for Iberia index dataset.
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Figure 7. Histogram of PM 2.5 extreme values. The red curve represents the density of the GPD ( 0.06 , 105.72 ) .
Figure 7. Histogram of PM 2.5 extreme values. The red curve represents the density of the GPD ( 0.06 , 105.72 ) .
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Figure 8. Sensitivity (upper charts) and relative sensitivity (lower charts) of VaR p (left charts) and CVaR p (right charts) versus p for different values of α for PM 2.5 dataset.
Figure 8. Sensitivity (upper charts) and relative sensitivity (lower charts) of VaR p (left charts) and CVaR p (right charts) versus p for different values of α for PM 2.5 dataset.
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Arias-Nicolás, J.P.; Parra, M.I.; Pizarro, M.M.; Sanjuán, E.L. Bayesian Sensitivity Analysis for VaR and CVaR Employing Distorted Band Priors. Axioms 2024, 13, 77. https://doi.org/10.3390/axioms13020077

AMA Style

Arias-Nicolás JP, Parra MI, Pizarro MM, Sanjuán EL. Bayesian Sensitivity Analysis for VaR and CVaR Employing Distorted Band Priors. Axioms. 2024; 13(2):77. https://doi.org/10.3390/axioms13020077

Chicago/Turabian Style

Arias-Nicolás, José Pablo, María Isabel Parra, Mario M. Pizarro, and Eva L. Sanjuán. 2024. "Bayesian Sensitivity Analysis for VaR and CVaR Employing Distorted Band Priors" Axioms 13, no. 2: 77. https://doi.org/10.3390/axioms13020077

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