Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Malikov, E. and Y. Sun | 2017 | 6 | 3 | 9.0 | 0.066 | 1.000 | 100% |
| 2 | Gupta, A (self) | 2018 | 4 | 3 | 6.0 | 0.044 | 0.928 | 100% |
| 3 | Pinkse, J., M. E. Slade, and C. Brett | 2002 | 4 | 3 | 6.0 | 0.044 | 0.928 | 100% |
| 4 | Kelejian, H. H. and I. R. Prucha | 2007 | 11 | 6 | 16.5 | 0.121 | 0.899 | 73% |
| 5 | Sun, Y., H. Yan, W. Zhang, and Z. Lu (self) | 2014 | 7 | 2 | 11.0 | 0.077 | 0.874 | 100% |
| 6 | Li, Q., C. J. Huang, D. Li, and T.-T. Fu | 2002 | 7 | 2 | 13.0 | 0.077 | 0.874 | 100% |
| 7 | Kelejian, H. H. and I. R. Prucha | 1998 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 8 | Lee, L. F | 2004 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 9 | Sun, Y | 2016 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 10 | Sun, Y. and E. Malikov | 2018 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 11 | Sun, Y | 2024 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 12 | Robinson, P. M. and S. Thawornkaiwong | 2012 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 13 | Hong, Y. and H. White | 1995 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 14 | Harrison Jr, D. and D. L. Rubinfeld | 1978 | 2 | 2 | 3.0 | 0.022 | 0.644 | 100% |
| 15 | Delgado, M. and P. M. Robinson | 2015 | 2 | 2 | 4.0 | 0.022 | 0.644 | 100% |
| 16 | Helmers, C. and M. Patnam | 2014 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 17 | Hsieh, C.-S. and H. van Kippersluis | 2018 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 18 | Cliff, A. D. and J. K. Ord | 1981 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 19 | Anselin, L | 1988 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 20 | Kuersteiner, G. M. and I. R. Prucha | 2020 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 21 | Fan, J. and W. Zhang (self) | 1999 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 22 | Fan, J. and W. Zhang (self) | 2008 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 23 | Su, L. and S. Jin | 2010 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 24 | Su, L | 2012 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 25 | Zhang, Z (self) | 2013 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 26 | Ackerberg, D., X. Chen, and J. Hahn | 2012 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 27 | Korolev, I | 2019 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 28 | Ahmad, I., S. Leelahanon, and Q. Li | 2005 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 29 | de Jong, R. M. and H. J. Bierens | 1994 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 30 | Gupta, A. and M. H. Seo (self) | 2023 | 1 | 1 | 1.0 | 0.011 | 0.406 | 100% |
| 31 | Huber, P. J | 1973 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 32 | Le Cam, L | 1960 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 33 | Andrews, D. W. K | 1985 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 34 | Koenker, R. and J. A. F. Machado | 1999 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 35 | Cattaneo, M. D., M. Jansson, and W. K. Newey | 2018 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 36 | Gupta, A. and P. M. Robinson (self) | 2015 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 37 | Chen, X | 2007 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 38 | Robinson, P. M | 2011 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 39 | Hidalgo, J. and M. Schafgans | 2017 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 40 | Conley, T. G., S. Gon\ccalves, M. S. Kim, and B. P... | 2023 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 41 | Gupta, A. and X. Qu (self) | 2024 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 42 | Ackerberg, D. A., K. Caves, and G. Frazer | 2015 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 43 | Basu, S. and B. Bundick | 2017 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 44 | Attanasio, O., S. Cattan, E. Fitzsimons, C. Meghir... | 2020 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 45 | Combes, P.-P., G. Duranton, and L. Gobillon | 2021 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 46 | Iyoha, E | 2023 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 47 | Murakami, N., D. Liu, and K. Otsuka | 1994 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 48 | Li, D.-K., C.-L. Mei, and N. Wang | 2019 | 1 | 1 | 2.0 | 0.011 | 0.406 | 100% |
| 49 | Scott, D. J | 1973 | 1 | 1 | 0.5 | 0.011 | 0.087 | 0% |