Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Wasserman, L., A. Ramdas, and S. Balakrishnan | 2020 | 11 | 7 | 14.5 | 0.099 | 0.935 | 82% |
| 2 | Kaido, H. and Y. Zhang (self) | 2019 | 5 | 3 | 6.5 | 0.045 | 0.928 | 80% |
| 3 | Philippe, F., G. Debs, and J.-Y. Jaffray | 1999 | 4 | 3 | 6.5 | 0.036 | 0.843 | 75% |
| 4 | Bresnahan, T. F. and P. C. Reiss | 1990 | 3 | 3 | 3.5 | 0.027 | 0.737 | 67% |
| 5 | Chesher, A., A. M. Rosen, and Y. Zhang (self) | 2024 | 3 | 2 | 5.0 | 0.027 | 0.737 | 100% |
| 6 | Barseghyan, L., M. Coughlin, F. Molinari, and J. C... | 2021 | 3 | 2 | 4.0 | 0.027 | 0.737 | 100% |
| 7 | Chernozhukov, V., S. Lee, and A. M. Rosen | 2013 | 3 | 2 | 4.5 | 0.027 | 0.737 | 100% |
| 8 | Kaido, H. and F. Molinari (self) | 2024 | 3 | 2 | 3.0 | 0.027 | 0.737 | 100% |
| 9 | Bugni, F., I. Canay, and X. Shi | 2017 | 3 | 2 | 4.5 | 0.027 | 0.737 | 100% |
| 10 | Honore, B. E. and E. Tamer | 2006 | 2 | 2 | 3.0 | 0.018 | 0.644 | 100% |
| 11 | Chesher, A. and A. M. Rosen | 2017 | 2 | 2 | 1.5 | 0.018 | 0.644 | 100% |
| 12 | Haile, P. A. and E. Tamer | 2003 | 2 | 2 | 3.0 | 0.018 | 0.644 | 100% |
| 13 | Fack, G., J. Grenet, and Y. He | 2019 | 2 | 2 | 3.0 | 0.018 | 0.644 | 100% |
| 14 | Chernozhukov, V., H. Hong, and E. Tamer | 2007 | 2 | 2 | 3.0 | 0.018 | 0.644 | 100% |
| 15 | Epstein, L. G., H. Kaido, and K. Seo (self) | 2016 | 2 | 2 | 1.5 | 0.018 | 0.644 | 100% |
| 16 | Tamer, E. | 2003 | 2 | 2 | 2.5 | 0.018 | 0.644 | 100% |
| 17 | Galichon, A. and M. Henry | 2011 | 2 | 2 | 2.5 | 0.018 | 0.644 | 100% |
| 18 | Beresteanu, A., I. Molchanov, and F. Molinari | 2011 | 2 | 2 | 2.5 | 0.018 | 0.644 | 100% |
| 19 | Andrews, D. W. and X. Shi | 2013 | 2 | 2 | 2.5 | 0.018 | 0.644 | 100% |
| 20 | Han, S. and H. Kaido (self) | 2024 | 2 | 2 | 4.0 | 0.018 | 0.644 | 100% |
| 21 | Li, L. and M. Henry | 2022 | 2 | 1 | 1.0 | 0.018 | 0.511 | 100% |
| 22 | Canay, I. A. and A. M. Shaikh | 2017 | 2 | 1 | 1.0 | 0.018 | 0.511 | 100% |
| 23 | Cox, G. and X. Shi | 2022 | 2 | 1 | 1.0 | 0.018 | 0.511 | 100% |
| 24 | Andrews, I., J. Roth, and A. Pakes | 2023 | 2 | 1 | 1.0 | 0.018 | 0.511 | 100% |
| 25 | Ciliberto, F. and E. Tamer | 2009 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 26 | Berry, S. T. and G. Compiani | 2022 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 27 | Miyauchi, Y. | 2016 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 28 | Sheng, S. | 2020 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 29 | Eizenberg, A. | 2014 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 30 | Dickstein, M. J. and E. Morales | 2018 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 31 | Bjorn, P. A. and Q. H. Vuong | 1984 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 32 | Bajari, P., H. Hong, and S. P. Ryan | 2010 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 33 | Andrews, D. W. and G. Soares | 2010 | 1 | 1 | 1.0 | 0.009 | 0.406 | 100% |
| 34 | Wald, A. | 1950 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 35 | Jovanovic, B. | 1989 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 36 | Horowitz, J. L. and S. Lee | 2023 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 37 | Kaido, H., F. Molinari, and J. Stoye (self) | 2019 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 38 | Hahn, J. and H. R. Moon | 2010 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 39 | Epstein, L. and K. Seo | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% | |
| 40 | Powell, J. L. | 1994 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 41 | Chen, X., E. T. Tamer, and A. Torgovitsky | 2011 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 42 | Chen, X., T. M. Christensen, and E. Tamer | 2018 | 1 | 1 | 0.5 | 0.009 | 0.406 | 100% |
| 43 | Artstein, Z. | 1983 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 44 | Molchanov, I. and F. Molinari | 2018 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 45 | Manski, C. F. and E. Tamer | 2002 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 46 | ---\hspace-.1pt---\hspace-.1pt--- | 1991 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 47 | Khan, S., M. Ponomareva, and E. Tamer | 2023 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 48 | Andrews, D. W. and W. Ploberger | 1994 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 49 | Elliott, G., U. K. Muller, and M. W. Watson | 2015 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 50 | Luo, Y., K. Ponomarev, and H. Wang | 2024 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 51 | Berry, S. and E. Tamer | 2006 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 52 | Lehmann, E. L. and J. P. Romano | 2006 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 53 | Choquet, G. | 1954 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 54 | Molchanov, I. | 2006 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 55 | Huber, P. J. | 1981 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 56 | Dempster, A. P. | 1967 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 57 | Shafer, G. | 1982 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 58 | Gul, F. and W. Pesendorfer | 2014 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 59 | Epstein, L. G. and K. Seo | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% | |
| 60 | Huber, P. J. and V. Strassen | 1973 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 61 | ---\hspace-.1pt---\hspace-.1pt--- | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% | |
| 62 | Montes, I., E. Miranda, and P. Vicig | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% | |
| 63 | Ritzwoller, D. M. and J. P. Romano | 2024 | 1 | 1 | 2.0 | 0.009 | 0.406 | 100% |
| 64 | 1 | 1 | 1.0 | 0.009 | 0.087 | 0% | ||
| 65 | Denneberg, D. | 1994 | 1 | 1 | 0.5 | 0.009 | 0.087 | 0% |
| 66 | Schmeidler, D. | 1986 | 1 | 1 | 0.5 | 0.009 | 0.087 | 0% |
| 67 | Berry, S. T. | 1992 | 1 | 1 | 0.5 | 0.009 | 0.087 | 0% |