Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Li, X. and P. Ding | 2017 | 5 | 4 | 8.5 | 0.078 | 1.000 | 100% |
| 2 | Liu, R. Y. et al | 1988 | 5 | 3 | 10.0 | 0.078 | 1.000 | 100% |
| 3 | Behaghel, L., B. Crepon, and M. Gurgand | 2014 | 15 | 8 | 27.0 | 0.234 | 0.977 | 93% |
| 4 | Walters, C. R | 2015 | 3 | 3 | 3.5 | 0.047 | 0.843 | 100% |
| 5 | Morris, C. N | 1983 | 2 | 2 | 3.0 | 0.031 | 0.644 | 100% |
| 6 | Kline, P., R. Saggio, and M. S\olvsten | 2020 | 2 | 2 | 2.5 | 0.031 | 0.644 | 100% |
| 7 | Imbens, G. W. and D. B. Rubin | 2015 | 2 | 2 | 4.0 | 0.031 | 0.644 | 100% |
| 8 | Loh, P.-L. and M. J. Wainwright | 2011 | 2 | 1 | 4.0 | 0.031 | 0.511 | 100% |
| 9 | De Chaisemartin, C. and X. d’Haultfoeuille (self) | 2018 | 2 | 1 | 4.0 | 0.031 | 0.511 | 100% |
| 10 | Hotz, V. J., G. W. Imbens, and J. H. Mortimer | 2005 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 11 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% | ||
| 12 | Angrist, J. D. and J.-S. Pischke | 2008 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 13 | Hoerl, A. E. and R. W. Kennard | 1970 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 14 | Wager, S. and S. Athey | 2018 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 15 | Kline, P., E. K. Rose, and C. R. Walters | 2022 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 16 | Deeb, A (self) | 2021 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 17 | Raudenbush, S. W. and H. S. Bloom | 2015 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 18 | Rose, E. K., J. T. Schellenberg, and Y. Shem-Tov | 2022 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 19 | Deaton, A | 1985 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 20 | Menzel, K | 2023 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 21 | Stanley, T. D. and H. Doucouliagos | 2012 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 22 | Adusumilli, K., F. Agostinelli, and E. Borghesan | 2024 | 1 | 1 | 0.5 | 0.016 | 0.406 | 100% |
| 23 | Angrist, J. D., G. W. Imbens, and D. B. Rubin | 1996 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 24 | Neyman, J | 1923 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 25 | Imbens, G. W. and J. D. Angrist | 1994 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 26 | Eicker, F. et al | 1963 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 27 | Huber, P. J. et al | 1967 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 28 | White, H. et al | 1980 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 29 | Golub, G. H., M. Heath, and G. Wahba | 1979 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 30 | Santosa, F. and W. W. Symes | 1986 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 31 | Tibshirani, R | 1996 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 32 | S\orensen, \O., A. Frigessi, and M. Thoresen | 2015 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 33 | Datta, A. and H. Zou | 2017 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 34 | Athey, S., N. Keleher, and J. Spiess | 2023 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 35 | Roy, A. D | 1951 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |