Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Chernozhukov, V., S. Lee, and A. Rosen | 2013 | 8 | 4 | 13.0 | 0.070 | 1.000 | 100% |
| 2 | Kitagawa, T. and A. Tetenov | 2018b | 7 | 4 | 13.0 | 0.061 | 1.000 | 100% |
| 3 | Andrews, D. W. and G. Soares | 2010 | 6 | 5 | 8.5 | 0.052 | 0.941 | 83% |
| 4 | Luedtke, A. and M. van der Laan | 2016 | 5 | 3 | 5.5 | 0.043 | 0.928 | 80% |
| 5 | Canay, I. A. and A. M. Shaikh | 2017 | 4 | 3 | 6.0 | 0.035 | 0.928 | 100% |
| 6 | Tsybakov, A. B | 2004 | 6 | 4 | 7.0 | 0.052 | 0.874 | 67% |
| 7 | Mbakop, E. and M. Tabord-Meehan | 3 | 3 | 5.0 | 0.026 | 0.843 | 100% | |
| 8 | Athey, S. and S. Wager | 3 | 3 | 5.0 | 0.026 | 0.843 | 100% | |
| 9 | Hirano, K. and J. Porter | 2012 | 3 | 2 | 4.0 | 0.026 | 0.737 | 100% |
| 10 | Romano, J. P., A. M. Shaikh, and M. Wolf | 2014 | 3 | 2 | 4.0 | 0.026 | 0.737 | 100% |
| 11 | Hahn, J | 4 | 3 | 5.0 | 0.035 | 0.737 | 50% | |
| 12 | Mammen, E. and A. B. Tsybakov | 1999 | 2 | 2 | 2.0 | 0.017 | 0.644 | 100% |
| 13 | Bloom, H. S., L. L. Orr, S. H. Bell, G. Cave, F. D... | 1997 | 2 | 2 | 3.0 | 0.017 | 0.644 | 100% |
| 14 | Hirano, K. and J. Porter | 2009 | 2 | 2 | 3.0 | 0.017 | 0.644 | 100% |
| 15 | Levis, A. W., M. Bonvini, Z. Zeng, L. Keele, and E... | 2023 | 2 | 2 | 3.0 | 0.017 | 0.644 | 100% |
| 16 | Manski, C. F | 2004 | 2 | 1 | 2.0 | 0.017 | 0.511 | 100% |
| 17 | Chernozhukov, V., S. Lee, A. M. Rosen, and L. Sun | 2025 | 2 | 1 | 2.0 | 0.017 | 0.511 | 100% |
| 18 | Dehejia, R. H | 2005 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 19 | Stoye, J | 2009 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 20 | Chamberlain, G | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% | |
| 21 | Bhattacharya, D. and P. Dupas | 2012 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 22 | Tetenov, A | 2012 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 23 | Rai, Y | 2019 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 24 | Sun, L | 2021 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 25 | Sasaki, Y. and T. Ura | 2024 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 26 | Kitagawa, T., S. Lee, and C. Qiu | 2022 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 27 | Yata, K | 2021 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 28 | Armstrong, T. B. and S. Shen | 2023 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 29 | Moon, S | 2025 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 30 | Qian, M. and S. A. Murphy | 2011 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 31 | Murphy, S. A | 2003 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 32 | Robins, J. M | 2004 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 33 | Shi, C., A. Fan, R. Song, and W. Lu | 2018 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 34 | Andrews, I., T. Kitagawa, and A. McCloskey | 2024 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 35 | Andrews, I. and J. Chen | 2025 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 36 | Chen, Q., M. Austern, and V. Syrgkanis | 2023 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 37 | Whitehouse, J., M. Austern, and V. Syrgkanis | 2025 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 38 | Ben-Michael, E | 2025 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 39 | Ben-Michael, E., D. J. Greiner, K. Imai, and Z. Ji... | 2021 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 40 | Cui, Y. and S. Han | 2024 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 41 | Adjaho, C. and T. Christensen | 2022 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 42 | Kasy, M | 2016 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 43 | Kitagawa, T. and A. Tetenov | 2021 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 44 | Terschuur, J | 2025 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 45 | Bai, Y., A. Santos, and A. M. Shaikh | 2022 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 46 | Cox, G. F | 2024 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 47 | Ketz, P. and A. McCloskey | 2025 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 48 | Lehmann, E. L. and J. P. Romano | 2005 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 49 | Robins, J. and A. Rotnitzky | 1995 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 50 | Lehmann, E. L | 1959 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 51 | Harter, H. L | 1964 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 52 | Dumbgen, L. and Spokoiny | 2001 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 53 | Armstrong, T. B | 2015 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 54 | Berger, R. L | 1997 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 55 | Chernozhukov, V., W. K. Newey, and A. Santos | 2015 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 56 | Chernozhukov, V., H. Hong, and E. Tamer | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% | |
| 57 | Armstrong, T. B | 2014 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 58 | Kallus, N., X. Mao, and A. Zhou | 2020 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 59 | Kallus, N | 2022b | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 60 | Kallus, N | 2022a | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 61 | Semenova, V (self) | 2020 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 62 | Semenova, V (self) | 2023 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 63 | Chandrasekhar, A., V. Chernozhukov, F. Molinari, a... | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% | |
| 64 | Liu, Y. and F. Molinari | 2024 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 65 | Heckman, J., H. Ichimura, and P. Todd | 1997 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 66 | Abadie, A., J. Angrist, and G. Imbens | 2002 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 67 | Kitagawa, T. and A. Tetenov | 2018a | 2 | 1 | 1.0 | 0.017 | 0.110 | 0% |