Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | ---\hspace-.1pt---\hspace-.1pt--- | 5 | 3 | 7.0 | 0.077 | 1.000 | 100% | |
| 2 | Tan, Z. | 2006 | 7 | 4 | 10.0 | 0.108 | 0.950 | 86% |
| 3 | Dorn, J., K. Guo, and N. Kallus | 2024 | 4 | 4 | 5.5 | 0.062 | 0.928 | 100% |
| 4 | Fan, Y. and S. S. Park | 2010 | 6 | 3 | 9.0 | 0.092 | 0.874 | 67% |
| 5 | Dorn, J. and K. Guo | 2023 | 3 | 3 | 4.5 | 0.046 | 0.843 | 100% |
| 6 | Rambachan, A., A. Coston, and E. Kennedy | 2023 | 3 | 2 | 3.0 | 0.046 | 0.737 | 100% |
| 7 | Kallus, N. and A. Zhou | 2018 | 2 | 2 | 2.5 | 0.031 | 0.644 | 100% |
| 8 | ---\hspace-.1pt---\hspace-.1pt--- | 2020 | 2 | 2 | 2.5 | 0.031 | 0.644 | 100% |
| 9 | Zhao, Q., D. S. Small, and B. B. Bhattacharya | 2019 | 2 | 1 | 1.0 | 0.031 | 0.511 | 100% |
| 10 | Imbens, G. W. and D. B. Rubin | 2015 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 11 | ---\hspace-.1pt---\hspace-.1pt--- | 2024 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 12 | Masten, M. A. and A. Poirier (self) | 2016 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 13 | Bonvini, M. and E. H. Kennedy | 2022 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 14 | Huang, M. and S. D. Pimentel | 2025 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 15 | Ding, P. and T. J. VanderWeele | 2016 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 16 | VanderWeele, T. J. and P. Ding | 2017 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 17 | Sjolander, A. | 2024 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 18 | Dorn, J. and L. Yap | 2024 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 19 | Torgovitsky, A. | 2019 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 20 | Gu, J., T. Russell, and T. Stringham | 2024 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 21 | Duarte, G. | 2024 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 22 | ---\hspace-.1pt---\hspace-.1pt--- | 2023 | 1 | 1 | 0.5 | 0.015 | 0.406 | 100% |
| 23 | Sklar, M. | 1959 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 24 | Chernozhukov, V., I. Fernandez-Val, and Y. Luo | 2018 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 25 | Masten, M. A., A. Poirier, and L. Zhang (self) | 2024 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 26 | Heckman, J. J., J. Smith, and N. Clements | 1997 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 27 | Manski, C. F. | 1997 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 28 | ---\hspace-.1pt---\hspace-.1pt--- | 2003 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 29 | Stoye, J. | 2010 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 30 | Makarov, G. | 1982 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 31 | Williamson, R. C. and T. Downs | 1990 | 1 | 1 | 2.0 | 0.015 | 0.406 | 100% |
| 32 | ---\hspace-.1pt---\hspace-.1pt--- | 1 | 1 | 1.0 | 0.015 | 0.406 | 100% | |
| 33 | Billingsley, P. | 1995 | 3 | 2 | 1.5 | 0.046 | 0.159 | 0% |
| 34 | Royden, H. and P. M. Fitzpatrick | 2010 | 2 | 1 | 1.0 | 0.031 | 0.110 | 0% |
| 35 | van der Vaart, A. W. | 2000 | 1 | 1 | 0.5 | 0.015 | 0.087 | 0% |
| 36 | Nelsen, R. B. | 2006 | 1 | 1 | 0.5 | 0.015 | 0.087 | 0% |
| 37 | Ash, R. B. and C. A. Doleans-Dade | 2000 | 1 | 1 | 0.5 | 0.015 | 0.087 | 0% |