Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | 5 | 4 | 8.0 | 0.053 | 1.000 | 100% | ||
| 2 | Abadie, A. | 2021 | 4 | 4 | 7.0 | 0.042 | 0.928 | 100% |
| 3 | Ferman, B. | 2021 | 4 | 3 | 7.0 | 0.042 | 0.928 | 100% |
| 4 | Ferman, B. and C. Pinto | 2021 | 3 | 3 | 5.0 | 0.032 | 0.843 | 100% |
| 5 | Wainwright, M. J. | 2019 | 3 | 3 | 6.0 | 0.032 | 0.843 | 100% |
| 6 | Abadie, A., A. Diamond, and J. Hainmueller | 2010 | 4 | 2 | 6.0 | 0.042 | 0.811 | 100% |
| 7 | Hainmueller, J. | 2012 | 4 | 2 | 5.0 | 0.042 | 0.811 | 100% |
| 8 | Buhlmann, P. and S. van de Geer | 2011 | 3 | 2 | 5.0 | 0.032 | 0.737 | 100% |
| 9 | Zheng, X. and S. X. Chen (self) | 2024 | 3 | 2 | 4.0 | 0.032 | 0.737 | 100% |
| 10 | Abadie, A. and J. Gardeazabal | 2003 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 11 | Bonhomme, S. and E. Manresa | 2015 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 12 | Su, L., Z. Shi, and P. C. B. Phillips (self) | 2016 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 13 | Vogt, M. and O. Linton | 2017 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 14 | Newey, W. K. and R. J. Smith | 2004 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 15 | Owen, A. B. | 1988 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 16 | Jagannathan, R. and T. Ma | 2003 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 17 | Bonhomme, S., T. Lamadon, and E. Manresa | 2022 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 18 | Feng, G., S. Giglio, and D. Xiu | 2020 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 19 | Doudchenko, N. and G. W. Imbens | 2016 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 20 | Shi, Z. and J. Huang (self) | 2023 | 2 | 2 | 3.0 | 0.021 | 0.644 | 100% |
| 21 | Kleven, H. J., C. Landais, and E. Saez | 2013 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 22 | Bohn, S., M. Lofstrom, and S. Raphael | 2014 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 23 | Acemoglu, D., S. Johnson, A. Kermani, J. Kwak, and... | 2016 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 24 | Cunningham, S. and M. Shah | 2018 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 25 | Athey, S. and G. W. Imbens | 2017 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 26 | Giannone, D., M. Lenza, and G. E. Primiceri | 2021 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 27 | Liao, Y., X. Ma, A. Neuhierl, and Z. Shi (self) | 2024 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 28 | Kitamura, Y. | 2007 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 29 | Abadie, A. and J. L'Hour | 2021 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 30 | Arkhangelsky, D., S. Athey, D. A. Hirshberg, G. W.... | 2021 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 31 | Chernozhukov, V., K. Wuthrich, and Y. Zhu | 2021 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 32 | Bates, J. M. and C. W. J. Granger | 1969 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 33 | Diebold, F. X. and M. Shin | 2019 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 34 | Hsiao, C., S. H. Ching, and S.-K. Wan | 2012 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 35 | Li, K. T. and D. R. Bell | 2017 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 36 | Arkhangelsky, D. and D. Hirshberg | 2023 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 37 | Wang, Y. and J. R. Zubizarreta | 2020 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 38 | Chen, J. | 2023 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 39 | ---\hspace-.1pt---\hspace-.1pt--- | 2015 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 40 | Li, K. T. | 2020 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 41 | Candes, E. and T. Tao | 2007 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 42 | Stock, J. H. and M. W. Watson | 2004 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 43 | DeMiguel, V., L. Garlappi, and R. Uppal | 2009 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 44 | Tibshirani, R. | 1996 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 45 | Fan, J. and R. Li | 2001 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 46 | Bickel, P. J. and E. Levina | 2008 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 47 | Tong, C., P. R. Hansen, and I. Archakov | 2025 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 48 | He, Y., D. Liu, G. Pan, and Y. Wang | 2024 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 49 | Abadie, A., S. Athey, G. W. Imbens, and J. M. Wool... | 2023 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 50 | Chan, F. and L. L. Pauwels | 2018 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 51 | Engle, R. and B. Kelly | 2012 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 52 | Bai, J. and S. Ng | 2002 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 53 | Bai, J. | 2003 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 54 | Li, H., Q. Li, and Y. Shi (self) | 2017 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 55 | Fan, J., Y. Liao, and M. Mincheva (self) | 2013 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 56 | Tsybakov, A., P. Bickel, and Y. Ritov | 2009 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 57 | Cressie, N. and T. R. Read | 1984 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 58 | Schennach, S. M. | 2007 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 59 | Hansen, L. P., J. Heaton, and A. Yaron | 1996 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 60 | Horn, R. A. and C. R. Johnson | 2017 | 1 | 1 | 0.5 | 0.011 | 0.087 | 0% |