Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Gu and Koenker | 2017 | 5 | 3 | 10.0 | 0.079 | 1.000 | 100% |
| 2 | Kiefer and Wolfowitz | 1956 | 4 | 3 | 5.5 | 0.063 | 0.843 | 75% |
| 3 | Yan, Wang, and Rigollet | 2024 | 3 | 2 | 5.0 | 0.048 | 0.737 | 100% |
| 4 | Robbins | 1956 | 2 | 2 | 3.0 | 0.032 | 0.644 | 100% |
| 5 | Walters | 2024 | 2 | 2 | 3.0 | 0.032 | 0.644 | 100% |
| 6 | Adusumilli, Gu, and Tao | 2025 | 2 | 2 | 3.0 | 0.032 | 0.644 | 100% |
| 7 | Shen and Wu | 2025 | 2 | 2 | 4.0 | 0.032 | 0.644 | 100% |
| 8 | Bruni and Koch | 1985 | 6 | 2 | 6.0 | 0.095 | 0.606 | 33% |
| 9 | Zhang, Cui, Sen, and Toh | 2024 | 2 | 1 | 4.0 | 0.032 | 0.511 | 100% |
| 10 | Efron | 2014 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 11 | Koenker and Gu | 2024 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 12 | Koenker and Gu | 2025 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 13 | Chen | 2024 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 14 | Kwon | 2025 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 15 | Cheng, Ho, and Schorfheide | 2025 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 16 | Gaillac | 2024 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 17 | Stein | 1956 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 18 | James and Stein | 1961 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 19 | Efron and Morris | 1973 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 20 | Liu, Moon, and Schorfheide | 2020 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 21 | Pastorino | 2024 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 22 | Bunting, Diegert, and Maurel | 2024 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 23 | de Paula, Gualdani, Pastorino, and Salgado | 2025 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 24 | Compiani and Kitamura | 2016 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 25 | Song, Lee, and Ng (self) | 2026 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 26 | Zhang | 1997 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 27 | Polyanskiy and Sellke | 2025 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 28 | Jiang and Zhang | 2009 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 29 | Koenker and Mizera | 2014 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 30 | Kim, Carbonetto, Stephens, and Anitescu | 2020 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 31 | Wang, Ibrahim, and Mazumder | 2025 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 32 | Altonji, Hynsjö, and Vidangos | 2023 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 33 | Browning and Ejrnaes | 2013 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 34 | Chamberlain and Hirano | 1999 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 35 | Geweke and Keane | 2000 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 36 | Hirano | 2002 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 37 | Giacomini, Lee, and Sarpietro (self) | 2025 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 38 | Moon, Schorfheide, and Zhang | 2023 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 39 | Meghir and Pistaferri | 2004 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 40 | Mincer | 1974 | 1 | 1 | 2.0 | 0.016 | 0.406 | 100% |
| 41 | Armstrong, Kolesár, and Plagborg-Møller | 2022 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 42 | Ignatiadis and Wager | 2022 | 1 | 1 | 1.0 | 0.016 | 0.406 | 100% |
| 43 | 2 | 1 | 2.0 | 0.032 | 0.110 | 0% |