| Literature DB >> 32548268 |
Casey W Miller1, Benjamin M Zwickl2, Julie R Posselt3, Rachel T Silvestrini4, Theodore Hodapp5.
Abstract
We provide statistical measures and additional analyses showing that our original analyses were sound. We use a generalized linear mixed model to account for program-to-program differences with program as a random effect without stratifying with tier and found the GRE-P (Graduate Record Examination physics test) effect is not different from our previous findings, thereby alleviating concern of collider bias. Variance inflation factors for each variable were low, showing that multicollinearity was not a concern. We show that range restriction is not an issue for GRE-P or GRE-V (GRE verbal), and only a minor issue for GRE-Q (GRE quantitative). Last, we use statistical measures of model quality to show that our published models are better than or equivalent to several alternates.Entities:
Year: 2020 PMID: 32548268 PMCID: PMC7274790 DOI: 10.1126/sciadv.aba4647
Source DB: PubMed Journal: Sci Adv ISSN: 2375-2548 Impact factor: 14.136
Fig. 1Ph.D. completion for U.S. men and women by program in our dataset as a function of GRE physics percentile score.
Fig. 2Ph.D. completion for U.S. men and women in our dataset as a function of mean-centered GRE physics percentile score.
Fit parameters from the generalized linear mixed model excluding tier as a parameter and using random effects to account for program-level variations.
| Intercept | 1.36 | 0.17 | 3.00 × 10−15 |
| GRE-P | 0.0058 | 0.0031 | 0.06 |
| Female | −0.32 | 0.12 | 0.007 |
Generalized variance inflation factors for each of the models in Table 2 of our Science Advances article.
| All students | ug.GPA | 1.14 | 1 | 1.07 |
| GRE.Q | 1.56 | 1 | 1.25 | |
| GRE-V | 1.30 | 1 | 1.14 | |
| GRE-P | 2.02 | 1 | 1.42 | |
| Gender | 1.07 | 1 | 1.03 | |
| Tier | 1.30 | 2 | 1.07 | |
| Race | 1.93 | 7 | 1.05 | |
| Start year | 1.11 | 10 | 1.01 | |
| U.S. only | ug.GPA | 1.16 | 1 | 1.08 |
| GRE-Q | 1.56 | 1 | 1.25 | |
| GRE-V | 1.20 | 1 | 1.09 | |
| GRE-P | 1.71 | 1 | 1.31 | |
| Gender | 1.09 | 1 | 1.04 | |
| Tier | 1.55 | 2 | 1.12 | |
| Race | 1.38 | 6 | 1.03 | |
| Start year | 1.12 | 10 | 1.01 | |
| U.S. male | ug.GPA | 1.17 | 1 | 1.08 |
| GRE-Q | 1.51 | 1 | 1.23 | |
| GRE-V | 1.18 | 1 | 1.09 | |
| GRE-P | 1.65 | 1 | 1.28 | |
| Tier | 1.60 | 2 | 1.12 | |
| Race | 1.40 | 6 | 1.03 | |
| Start year | 1.13 | 10 | 1.01 | |
| U.S. female | ug.GPA | 1.21 | 1 | 1.10 |
| GRE-Q | 1.81 | 1 | 1.35 | |
| GRE-V | 1.31 | 1 | 1.15 | |
| GRE-P | 1.71 | 1 | 1.31 | |
| Tier | 1.55 | 2 | 1.12 | |
| Race | 1.58 | 6 | 1.04 | |
| Start year | 1.37 | 10 | 1.02 |
Correlation coefficients (Spearman’s rank order correlation) among the four quantitative admissions metrics within each of the four analytic samples, averaged across 40 imputations of missing data.
| All | ug.GPA | 1 | 0.18 | 0.18 | 0.18 |
| GRE-Q | 1 | 0.23 | 0.55 | ||
| GRE-V | 1 | 0.14 | |||
| GRE-P | 1 | ||||
| U.S. only | ug.GPA | 1 | 0.26 | 0.18 | 0.28 |
| GRE-Q | 1 | 0.35 | 0.55 | ||
| GRE-V | 1 | 0.33 | |||
| GRE-P | 1 | ||||
| U.S. male | ug.GPA | 1 | 0.24 | 0.16 | 0.36 |
| GRE-Q | 1 | 0.34 | 0.54 | ||
| GRE-V | 1 | 0.34 | |||
| GRE-P | 1 | ||||
| U.S. female | ug.GPA | 1 | 0.26 | 0.22 | 0.24 |
| GRE-Q | 1 | 0.45 | 0.61 | ||
| GRE-V | 1 | 0.42 | |||
| GRE-P | 1 |
Correlation coefficients (Spearman’s rank order correlation) among the fit parameters within each of the four analytic samples, averaged across 40 imputations of missing data.
Demographic factors (race, citizenship, and gender), tier, and start year fixed effect were also calculated but are not shown here.
| All students | (Intercept) | 1 | −0.71 | −0.49 | −0.03 | 0.22 |
| ug.GPA | 1 | −0.14 | −0.08 | −0.06 | ||
| GRE-Q | 1 | −0.16 | −0.42 | |||
| GRE-V | 1 | −0.17 | ||||
| GRE-P | 1 | |||||
| U.S. only | (Intercept) | 1 | −0.74 | −0.37 | −0.10 | 0.18 |
| ug.GPA | 1 | −0.18 | −0.06 | −0.04 | ||
| GRE-Q | 1 | −0.20 | −0.42 | |||
| GRE-V | 1 | −0.13 | ||||
| GRE-P | 1 | |||||
| U.S. male | (Intercept) | 1 | −0.74 | −0.38 | −0.12 | 0.20 |
| ug.GPA | 1 | −0.17 | −0.05 | −0.06 | ||
| GRE-Q | 1 | −0.17 | −0.41 | |||
| GRE-V | 1 | −0.15 | ||||
| GRE-P | 1 | |||||
| U.S. female | (Intercept) | 1 | −0.75 | −0.35 | −0.04 | 0.15 |
| ug.GPA | 1 | −0.19 | −0.08 | 0.04 | ||
| GRE-Q | 1 | −0.27 | −0.43 | |||
| GRE-V | 1 | −0.06 | ||||
| GRE-P | 1 |
AICc analysis for the four analytic samples analyzed through a variety of models.
The rows for the four analytic samples indicate the difference between the AICc for each model relative to the minimum among these models. Models with AICc differences of two or less are considered equivalent.
| As published | ug.GPA, GRE-Q, | 0.0 | 1.5 | 1.7 | 4.5 | |
| a | ug.GPA, GRE-V, and | GRE-Q | 4.1 | 1.7 | 1.1 | 3.0 |
| b | ug.GPA, GRE-Q, and | GRE-P | 0.3 | 2.1 | 1.7 | 2.9 |
| c | GRE-Q | ug.GPA, GRE-V, and | 2.6 | 9.8 | 4.5 | 3.8 |
| d | GRE-P | ug.GPA, GRE-Q, and | 7.9 | 11.4 | 4.9 | 5.2 |
| e | ug.GPA, | 0.4 | 0.0 | 0.0 | 2.6 | |
| f | ug.GPA | GRE-Q, GRE-V, and | 7.6 | 3.8 | 1.6 | 0.0 |
Data showing the interquartile range (IQR) for different groups of test takers for the indicated tests.
| GRE-P | Physicists | 26 | 51 | 75 | 49 |
| Our sample: physicists | 42 | 65 | 85 | 43 | |
| U.S. physicists | 28 | 40 | 63 | 35 | |
| Our sample: U.S. physicists | 35 | 55 | 71 | 36 | |
| U.S. male physicists | 21 | 42 | 67 | 46 | |
| Our sample: U.S. male physicists | 39 | 57 | 73 | 34 | |
| U.S. female physicists | 13 | 26 | 47 | 34 | |
| Our sample: U.S. female physicists | 21 | 37 | 57 | 36 | |
| GRE-Q | Physicists | 69 | 81 | 91 | 22 |
| Our sample: physicists | 81 | 89 | 91 | 10 | |
| United States | 20 | 38 | 59 | ||
| U.S. physicists | 62 | 78 | 87 | 25 | |
| Our sample: U.S. physicists | 79 | 87 | 91 | 12 | |
| U.S. male | 27 | 51 | 69 | ||
| U.S. male physicists | 66 | 78 | 89 | 23 | |
| Our sample: U.S. male physicists | 79 | 87 | 91 | 12 | |
| U.S. female | 17 | 30 | 51 | ||
| U.S. female physicists | 59 | 73 | 84 | 25 | |
| Our sample: U.S. female physicists | 75 | 83 | 91 | 16 | |
| GRE-V | Physicists | 35 | 65 | 86 | 51 |
| Our sample: physicists | 57 | 77 | 89 | 32 | |
| United States | 39 | 61 | 80 | ||
| U.S. physicists | 65 | 83 | 93 | 28 | |
| Our sample: U.S. physicists | 68 | 81 | 91 | 23 | |
| U.S. male | 43 | 69 | 86 | ||
| U.S. male physicists | 65 | 80 | 93 | 28 | |
| Our sample: U.S. male physicists | 68 | 81 | 91 | 23 | |
| U.S. female | 35 | 56 | 76 | ||
| U.S. female physicists | 69 | 83 | 93 | 24 | |
| Our sample: U.S. female physicists | 70 | 83 | 93 | 23 |
Fig. 3GRE physics (blue) and GRE quantitative (orange) score distributions for U.S. physicists, plotted as percentile or scaled score.
The symbols are bins of width 1 SE error of measure for score differences for each test, decreasing from a perfect score.