Ordered by composite index (descending). Higher values indicate more intensive citation.
| # | Reference | Year | Mentions | Breadth | Sec. Wtd | Share | Composite | Main % |
|---|---|---|---|---|---|---|---|---|
| 1 | Sucarrat, G., Gr\onneberg, S., and Escribano, A | 2016 | 5 | 3 | 9.0 | 0.051 | 1.000 | 100% |
| 2 | Otto, P., Do\ugan, O., and Ta\csp\inar, S (self) | 2022 | 7 | 2 | 10.0 | 0.071 | 0.874 | 100% |
| 3 | Zhou, J., Li, D., Pan, R., and Wang, H | 2020 | 5 | 2 | 7.0 | 0.051 | 0.874 | 100% |
| 4 | Hansen, P. R., Lunde, A., and Nason, J. M | 2011 | 3 | 3 | 5.0 | 0.031 | 0.843 | 100% |
| 5 | Diebold, F. X. and Mariano, R. S | 2002 | 4 | 2 | 8.0 | 0.041 | 0.811 | 100% |
| 6 | Geweke, J | 1986 | 2 | 2 | 3.0 | 0.020 | 0.644 | 100% |
| 7 | Fulle, M. J. and Otto, P (self) | 2022 | 2 | 2 | 3.0 | 0.020 | 0.644 | 100% |
| 8 | Maharaj, E. A., D'Urso, P., and Caiado, J | 2019 | 2 | 2 | 3.0 | 0.020 | 0.644 | 100% |
| 9 | Caporin, M. and Paruolo, P | 2015 | 3 | 1 | 3.0 | 0.031 | 0.585 | 100% |
| 10 | Billio, M., Caporin, M., Frattarolo, L., and Peliz... | 2021 | 3 | 1 | 3.0 | 0.031 | 0.585 | 100% |
| 11 | Piccolo, D | 1990 | 3 | 1 | 6.0 | 0.031 | 0.585 | 100% |
| 12 | Mantegna, R. N | 1999 | 2 | 1 | 4.0 | 0.020 | 0.511 | 100% |
| 13 | Bollerslev, T | 1986 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 14 | Andersen, T. G. and Bollerslev, T | 1998 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 15 | Francq, C. and Zakoian, J.-M | 2019 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 16 | Otto, P., Schmid, W., and Garthoff, R (self) | 2018 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 17 | Otto, P., Schmid, W., and Garthoff, R (self) | 2021 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 18 | Sato, T. and Matsuda, Y | 2017 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 19 | Sato, T. and Matsuda, Y | 2021 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 20 | Otto, P. and Schmid, W (self) | 2022 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 21 | Sahu, S. K. and Bohning, D | 2022 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 22 | Mattera, R (self) | 2022 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 23 | Huang, W., Wang, K., Jay Breidt, F., and Davis, R.... | 2011 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 24 | Cameletti, M., Gomez-Rubio, V., and Blangiardo, M | 2019 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 25 | Piter, A., Otto, P., and Alkhatib, H (self) | 2022 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 26 | Fasso, A., Maranzano, P., and Otto, P (self) | 2022 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 27 | Holly, S., Pesaran, M. H., and Yamagata, T | 2010 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 28 | Baltagi, B. H. and Li, J | 2014 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 29 | Otto, P. and Schmid, W (self) | 2018 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 30 | Pirinsky, C. and Wang, Q | 2006 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 31 | Barker, D. and Loughran, T | 2007 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 32 | Eckel, S., Loffler, G., Maurer, A., and Schmidt, V | 2011 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 33 | Asgharian, H., Hess, W., and Liu, L | 2013 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 34 | Fernandez-Aviles, G., Montero, J.-M., and Orlov, A... | 2012 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 35 | Diebold, F. X. and Y\ilmaz, K | 2014 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 36 | Demiris, N., Kypraios, T., and Smith, L. V | 2014 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 37 | Barigozzi, M. and Hallin, M | 2017 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 38 | Vinciotti, V., Tosetti, E., Moscone, F., and Lycet... | 2019 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 39 | Betancourt, B., Rodr\'\iguez, A., and Boyd, N | 2020 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 40 | Liu, S., Caporin, M., and Paterlini, S | 2021 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 41 | Zhou, Y., Chen, Z., and Liu, Z | 2023 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 42 | Wu, J., Xu, K., Chen, X., Li, S., and Zhao, J | 2022 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 43 | Huang, D., Hu, W., Jing, B., and Zhang, B | 2023 | 1 | 1 | 1.0 | 0.010 | 0.406 | 100% |
| 44 | Bauwens, L. and Sucarrat, G | 2010 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 45 | Sucarrat, G. and Escribano, A | 2012 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 46 | Duan, N | 1983 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 47 | Francq, C. and Sucarrat, G | 2018 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 48 | Francq, C. and Sucarrat, G | 2017 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 49 | Donaldson, R. G. and Kamstra, M | 1997 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 50 | Kristjanpoller, W. and Minutolo, M. C | 2015 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 51 | Lee, L.-f | 2007 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 52 | Lee, L.-f. L. and Yu, J | 2014 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 53 | Tumminello, M., Lillo, F., and Mantegna, R. N | 2010 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 54 | D’Urso, P. and Maharaj, E. A | 2009 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 55 | Caiado, J., Crato, N., and Pena, D | 2006 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 56 | Caiado, J., Crato, N., and Poncela, P | 2020 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 57 | Lahmiri, S | 2016 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 58 | Cerqueti, R. and Mattera, R (self) | 2023 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 59 | Otranto, E | 2008 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 60 | D'Urso, P., De Giovanni, L., and Massari, R | 2016 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 61 | Gallo, G. M., Lacava, D., and Otranto, E | 2021 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 62 | Cerqueti, R., Giacalone, M., and Mattera, R (self) | 2021 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 63 | Cerqueti, R., D’Urso, P., De Giovanni, L., Giacalo... (self) | 2022 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 64 | Proietti, T. and Giovannelli, A | 2021 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 65 | Tollenaar, N. and van der Heijden, P. G | 2013 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 66 | Deb, S. and Deb, S | 2022 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 67 | Di Narzo, A. and Cocchi, D | 2010 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 68 | Becker, R. and Clements, A. E | 2008 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |
| 69 | Timmermann, A | 2006 | 1 | 1 | 2.0 | 0.010 | 0.406 | 100% |