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Propensity score matching with clustered data. An application to the estimation of the impact of caesarean section on the Apgar score
Author(s) -
Arpino Bruno,
Cannas Massimo
Publication year - 2016
Publication title -
statistics in medicine
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.996
H-Index - 183
eISSN - 1097-0258
pISSN - 0277-6715
DOI - 10.1002/sim.6880
Subject(s) - propensity score matching , matching (statistics) , cluster (spacecraft) , confounding , computer science , caesarean section , statistics , apgar score , econometrics , mathematics , pregnancy , birth weight , biology , genetics , programming language
This article focuses on the implementation of propensity score matching for clustered data. Different approaches to reduce bias due to cluster‐level confounders are considered and compared using Monte Carlo simulations. We investigated methods that exploit the clustered structure of the data in two ways: in the estimation of the propensity score model (through the inclusion of fixed or random effects) or in the implementation of the matching algorithm. In addition to a pure within‐cluster matching, we also assessed the performance of a new approach, ‘preferential’ within‐cluster matching. This approach first searches for control units to be matched to treated units within the same cluster. If matching is not possible within‐cluster, then the algorithm searches in other clusters. All considered approaches successfully reduced the bias due to the omission of a cluster‐level confounder. The preferential within‐cluster matching approach, combining the advantages of within‐cluster and between‐cluster matching, showed a relatively good performance both in the presence of big and small clusters, and it was often the best method. An important advantage of this approach is that it reduces the number of unmatched units as compared with a pure within‐cluster matching. We applied these methods to the estimation of the effect of caesarean section on the Apgar score using birth register data. Copyright © 2016 John Wiley & Sons, Ltd.

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