Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Arellano and Bond | 1991 | 5 | 4 | 9.0 | 0.031 | 1.000 | 100% |
| 2 | Chamberlain | 2022 | 8 | 5 | 15.0 | 0.050 | 1.000 | 100% |
| 3 | Bonhomme (self) | 2012 | 5 | 3 | 9.0 | 0.031 | 1.000 | 100% |
| 4 | Bonhomme, Dano, and Graham (self) | 2023 | 7 | 4 | 13.0 | 0.043 | 1.000 | 100% |
| 5 | Alvarez and Arellano | 2003 | 8 | 3 | 16.0 | 0.050 | 1.000 | 100% |
| 6 | Bonhomme (self) | 2025 | 4 | 3 | 7.0 | 0.025 | 0.928 | 100% |
| 7 | Ghanem, Sant'Anna, and Wuthrich | 2022 | 4 | 4 | 8.0 | 0.025 | 0.928 | 100% |
| 8 | Bonhomme, Dano, and Graham (self) | 2025 | 5 | 2 | 9.0 | 0.031 | 0.874 | 100% |
| 9 | Abadie | 2005 | 3 | 3 | 5.0 | 0.019 | 0.843 | 100% |
| 10 | Arellano | 2003 | 3 | 3 | 5.0 | 0.019 | 0.843 | 100% |
| 11 | Marx, Tamer, and Tang | 2024 | 3 | 3 | 5.0 | 0.019 | 0.843 | 100% |
| 12 | Robins | 1986 | 3 | 3 | 6.0 | 0.019 | 0.843 | 100% |
| 13 | Lee | 2020 | 4 | 2 | 7.0 | 0.025 | 0.811 | 100% |
| 14 | Chamberlain | 1992 | 3 | 2 | 5.0 | 0.019 | 0.737 | 100% |
| 15 | Arellano and Bover | 1995 | 3 | 2 | 6.0 | 0.019 | 0.737 | 100% |
| 16 | Arellano and Bonhomme (self) | 2012 | 3 | 2 | 6.0 | 0.019 | 0.737 | 100% |
| 17 | Goodman-Bacon | 2021 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 18 | Blundell and Bond | 1998 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 19 | De Chaisemartin and d’Haultfoeuille | 2020 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 20 | Sun and Abraham | 2021 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 21 | Callaway and Sant’Anna | 2021 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 22 | Borusyak, Jaravel, and Spiess | 2024 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 23 | Honore and Tamer | 2006 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 24 | Abowd, Kramarz, and Margolis | 1999 | 2 | 2 | 3.0 | 0.012 | 0.644 | 100% |
| 25 | Ashenfelter and Card | 1985 | 2 | 2 | 4.0 | 0.012 | 0.644 | 100% |
| 26 | Marx, Tamer, and Tang | 2024 | 2 | 2 | 4.0 | 0.012 | 0.644 | 100% |
| 27 | Chamberlain | 1992 | 2 | 2 | 4.0 | 0.012 | 0.644 | 100% |
| 28 | Chesher, Rosen, and Zhang | 2024 | 2 | 2 | 4.0 | 0.012 | 0.644 | 100% |
| 29 | Botosaru, Loh, and Muris | 2024 | 2 | 2 | 4.0 | 0.012 | 0.644 | 100% |
| 30 | Hayashi | 2011 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 31 | Acemoglu, Naidu, Restrepo, and Robinson | 2019 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 32 | Alvarez and Arellano | 2004 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 33 | Moral-Benito | 2013 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 34 | Hahn and Kuersteiner | 2002 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 35 | Graham and Powell | 2012 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 36 | Kuersteiner and Prucha | 2020 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 37 | Bonhomme, Lamadon, and Manresa (self) | 2019 | 2 | 1 | 4.0 | 0.012 | 0.511 | 100% |
| 38 | Imbens and Angrist | 1994 | 1 | 1 | 1.0 | 0.006 | 0.406 | 100% |
| 39 | Hendry | 1995 | 1 | 1 | 1.0 | 0.006 | 0.406 | 100% |
| 40 | Engle, Hendry, and Richard | 1983 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 41 | Torgovitsky | 2019 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 42 | Chamberlain | 1982 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 43 | Rust | 1987 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 44 | Keane and Wolpin | 1997 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 45 | Chabe-Ferret | 2015 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 46 | de Chaisemartin and d'Haultfoeuille | 2022 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 47 | Mikusheva and S\olvsten | 2023 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 48 | Nickell | 1981 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 49 | Roth | 2022 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 50 | Freyaldenhoven, Hansen, and Shapiro | 2019 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 51 | Rambachan and Roth | 2023 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 52 | LaLonde | 1986 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 53 | Klosin | 2024 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 54 | Holtz-Eakin, Newey, and Rosen | 1988 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 55 | Wooldridge | 2010 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 56 | Kiviet | 1995 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 57 | Ahn and Schmidt | 1995 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 58 | Hsiao, Pesaran, and Tahmiscioglu | 2002 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 59 | Mundlak | 1978 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 60 | Moral-Benito, Allison, and Williams | 2019 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 61 | Bun, Carree, and Juodis | 2017 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 62 | Arellano and Hahn | 2007 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 63 | Dhaene and Jochmans | 2015 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 64 | Bun and Carree | 2005 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 65 | Bonhomme and Denis (self) | 2025 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 66 | Botosaru and Liu | 2025 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 67 | de Chaisemartin and D'Haultfoeuille | 2025 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 68 | Arkhangelsky and Imbens | 2024 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 69 | Azriel and Schwartzman | 2020 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 70 | Fernandez-Val and Lee | 2013 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 71 | Arellano and Honore | 2001 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 72 | Blundell, Griffith, and Windmeijer | 2002 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 73 | Wooldridge | 1997 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 74 | Al-Sadoon, Li, and Pesaran | 2017 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 75 | Woutersen | 2000 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 76 | Rasch | 1960 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 77 | Chamberlain | 2023 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 78 | Honore and Weidner | 2024 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 79 | Honore, Muris, and Weidner | 2025 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 80 | Dano | 2023 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 81 | Arellano and Bonhomme (self) | 2016 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 82 | Hu and Schennach | 2008 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 83 | Hu and Shum | 2012 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 84 | Di Addario, Kline, Saggio, and S\olvsten | 2023 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |
| 85 | Mikusheva, S\olvsten, and Jing | 2025 | 1 | 1 | 2.0 | 0.006 | 0.406 | 100% |