Between Dec 22, 2025 and Jan 5, 2026, items can be submitted to the UDC and DRUM, but will not be processed until after the break. Staff will not be available to answer email during this period, and will not be able to provide DOIs for datasets until after Jan 5. If you are in need of a DOI during this period, consider Figshare, Zenodo, Open Science Framework, Harvard Dataverse or OpenICPSR.

Implications of three causal models for the measurement of halo error

Loading...
Thumbnail Image

View/Download File

Persistent link to this item

Statistics
View Statistics

Journal Title

Journal ISSN

Volume Title

Published Date

Publisher

Abstract

The appropriateness of a traditional correlational measure of halo error (the difference between dimensional rating intercorrelations and dimensional true score intercorrelations) is reexamined in the context of three causal models of halo error. Mathematical derivations indicate that the traditional correlational measure typically will underestimate halo error in ratings and can suggest no halo error or even "negative" halo error when positive halo error actually occurs. A corrected correlational measure is derived that avoids these problems, and the traditional and corrected measures are compared empirically. Results suggest that use of the traditional correlational measure of halo error be discontinued. Index terms: halo, halo effect, halo error, performance ratings, rating accuracy, rating errors.

Keywords

Description

Related to

Replaces

License

Series/Report Number

Funding information

Isbn identifier

Doi identifier

Previously Published Citation

Fisicaro, Sebastiano A & Lance, Charles E. (1990). Implications of three causal models for the measurement of halo error. Applied Psychological Measurement, 14, 419-429. doi:10.1177/014662169001400407

Other identifiers

doi:10.1177/014662169001400407

Suggested citation

Fisicaro, Sebastiano A.; Lance, Charles E.. (1990). Implications of three causal models for the measurement of halo error. Retrieved from the University Digital Conservancy, https://hdl.handle.net/11299/113941.

Content distributed via the University Digital Conservancy may be subject to additional license and use restrictions applied by the depositor. By using these files, users agree to the Terms of Use. Materials in the UDC may contain content that is disturbing and/or harmful. For more information, please see our statement on harmful content in digital repositories.