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Clinical evaluation of the MPS 9000 Macular Pigment Screener
Hannah E Bartlett, Louise A Stainer, Sandip Singh, Frank Eperjesi, Olivia Howells

Clinical evaluation of the MPS 9000 Macular Pigment Screener

Science & Mathematics Published 2010 Verification Pending

Overview & Synopsis

Background/aims The MPS 9000 uses a psychophysical technique known as heterochromatic flicker photometry to measure macular pigment optical density (MPOD). Our aim was to determine the measurement variability (noise) of the MPS 9000. Methods Forty normally sighted participants who ranged in age from 18 to 50 years (25.4 Β± 8.2 years) were recruited from staff and students of Aston University. Data were collected by two operators, LS and SS, in two sessions separated by one week in order to assess test repeatability and reproducibility. Results The overall mean MPOD for the cohort was 0.35 Β± 0.14. There was no significant negative correlation between MPS 9000 MPOD readings and age (r = -0.192, p = 0.236). Coefficients were 0.33 and 0.28 for repeatability, and 0.25 and 0.26 for reproducibility. There was no significant correlation between mean and difference MPOD values for any of the four pairs of results. Conclusions If MPOD is being monitored over time then any change less than 0.33 units should not be considered clinically significant as it is very likely to be due to measurement noise. The size of the coefficient appears to be positively correlated with MPOD.

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Document Information

Document Title Clinical evaluation of the MPS 9000 Macular Pigment Screener
Author / Organization Hannah E Bartlett, Louise A Stainer, Sandip Singh, Frank Eperjesi, Olivia Howells
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2010
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-72027
Original Source Link Visit Source Page on hal.science »