# FIESTA: Fast IdEntification of State-of-The-Art models using adaptive   bandit algorithms

**Authors:** Henry B. Moss, Andrew Moore, David S. Leslie, Paul Rayson

arXiv: 1906.12230 · 2019-07-01

## TL;DR

FIESTA is a model selection method that uses adaptive bandit algorithms to efficiently identify the best models with fewer evaluations by focusing resources on promising candidates and providing confidence guarantees.

## Contribution

It introduces an adaptive bandit-based approach for model selection that reduces computational costs and improves reliability over traditional methods.

## Key findings

- Significantly fewer evaluations needed to select top models.
- Reliable model selection with confidence guarantees.
- Effective in sentiment analysis model comparison.

## Abstract

We present FIESTA, a model selection approach that significantly reduces the computational resources required to reliably identify state-of-the-art performance from large collections of candidate models. Despite being known to produce unreliable comparisons, it is still common practice to compare model evaluations based on single choices of random seeds. We show that reliable model selection also requires evaluations based on multiple train-test splits (contrary to common practice in many shared tasks). Using bandit theory from the statistics literature, we are able to adaptively determine appropriate numbers of data splits and random seeds used to evaluate each model, focusing computational resources on the evaluation of promising models whilst avoiding wasting evaluations on models with lower performance. Furthermore, our user-friendly Python implementation produces confidence guarantees of correctly selecting the optimal model. We evaluate our algorithms by selecting between 8 target-dependent sentiment analysis methods using dramatically fewer model evaluations than current model selection approaches.

## Full text

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## Figures

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## References

43 references — full list in the complete paper: https://tomesphere.com/paper/1906.12230/full.md

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Source: https://tomesphere.com/paper/1906.12230