Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Crump, R. K., V. J. Hotz, G. W. Imbens, and O. A. ... | 2009 | 5 | 3 | 8.0 | 0.061 | 1.000 | 100% |
| 2 | Angrist, J. D | 1998 | 8 | 4 | 14.0 | 0.098 | 1.000 | 100% |
| 3 | Armstrong, T. B. and M. Kolesar | 2021 | 4 | 3 | 6.0 | 0.049 | 0.928 | 100% |
| 4 | Armstrong, T. B., M. Kolesár, and S. Kwon (self) | 2023 | 5 | 4 | 7.5 | 0.061 | 0.928 | 80% |
| 5 | Angrist, J. D. and J.-S. Pischke | 2009 | 4 | 2 | 5.0 | 0.049 | 0.811 | 100% |
| 6 | S\l oczy\'nski, T | 2022 | 3 | 2 | 4.0 | 0.037 | 0.737 | 100% |
| 7 | de Chaisemartin, C. and X. D'Haultfoeuille | 2020 | 2 | 2 | 3.0 | 0.024 | 0.644 | 100% |
| 8 | Goodman-Bacon, A | 2021 | 2 | 2 | 3.0 | 0.024 | 0.644 | 100% |
| 9 | Goldsmith-Pinkham, P., P. Hull, and M. Kolesar | 2024 | 2 | 2 | 2.0 | 0.024 | 0.644 | 100% |
| 10 | Rothe, C | 2017 | 2 | 2 | 3.0 | 0.024 | 0.644 | 100% |
| 11 | de Chaisemartin, C | 2024 | 2 | 2 | 3.0 | 0.024 | 0.644 | 100% |
| 12 | Armstrong, T. B. and M. Koles\'ar | 2018 | 3 | 2 | 4.5 | 0.037 | 0.644 | 67% |
| 13 | Sun, L. and S. Abraham (self) | 2021 | 2 | 2 | 3.0 | 0.024 | 0.644 | 100% |
| 14 | Aizer, A., S. Eli, J. Ferrie, and A. Lleras-Muney | 2016 | 3 | 1 | 6.0 | 0.037 | 0.585 | 100% |
| 15 | Donoho, D. L | 1994 | 2 | 2 | 2.5 | 0.024 | 0.511 | 50% |
| 16 | Kline, P., R. Saggio, and M. S\olvsten | 2020 | 2 | 1 | 4.0 | 0.024 | 0.511 | 100% |
| 17 | Dobkin, C., A. Finkelstein, R. Kluender, and M. J.... | 2018 | 2 | 1 | 4.0 | 0.024 | 0.511 | 100% |
| 18 | Martinez-Bravo, M | 2014 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 19 | Favara, G. and J. Imbs | 2015 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 20 | Michalopoulos, S. and E. Papaioannou | 2016 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 21 | Bobonis, G. J., L. R. Camara Fuertes, and R. Schwa... | 2016 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 22 | Xu, G | 2018 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 23 | D’Amour, A., P. Ding, A. Feller, L. Lei, and J. Se... | 2021 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 24 | Gibbons, C. E., J. C. S. Serrato, and M. B. Urbanc... | 2019 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 25 | Armstrong, T. B., P. Kline, and L. Sun (self) | 2025 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 26 | Heiler, P. and E. Kazak | 2021 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 27 | Ma, X. and J. Wang | 2020 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 28 | Sasaki, Y. and T. Ura | 2022 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 29 | Lechner, M | 2008 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 30 | Athey, S., G. W. Imbens, and S. Wager | 2018 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 31 | Manski, C. F. and J. V. Pepper | 2018 | 1 | 1 | 1.0 | 0.012 | 0.406 | 100% |
| 32 | Imbens, G. W. and J. M. Wooldridge | 2009 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 33 | Poirier, A. and T. Słoczyński | 2024 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 34 | Athey, S. and G. Imbens | 2016 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 35 | Davis, J. M. and S. B. Heller | 2017 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 36 | Bruns-Smith, D., O. Dukes, A. Feller, and E. L. Og... | 2025 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 37 | Li, K.-C | 1982 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 38 | Masten, M. A. and A. Poirier | 2020 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 39 | Li, C. and U. K. Muller | 2021 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 40 | Imbens, G. and S. Wager | 2019 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 41 | Noack, C. and C. Rothe | 2024 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 42 | Sanchez-Becerra, A | 2023 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 43 | de Chaisemartin, C. and A. Deeb | 2024 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 44 | Roth, J., P. H. Sant’Anna, A. Bilinski, and J. Poe | 2023 | 1 | 1 | 2.0 | 0.012 | 0.406 | 100% |
| 45 | Low, M. G | 1997 | 2 | 1 | 1.0 | 0.024 | 0.110 | 0% |