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--- pegasus:overview [02/09/2023 13:25] – lipatov
+++ pegasus:overview [02/09/2023 13:39] – lipatov
@@ Line 75: / Line 75: @@
 | JH'2013 set 1 (CCFM)  |  2  |  4  |  200  |  [[https://arxiv.org/abs/1312.7875|F. Hautmann, H. Jung]]  |
 | JH'2013 set 2 (CCFM)  |  2  |  4  |  200  |  [[https://arxiv.org/abs/1312.7875|F. Hautmann, H. Jung]]  |
-| KMR (MMHT'2014)  |  1  |  5  |  211  |  [[https://arxiv.org/abs/hep-ph/9911379|M.A. Kimber, A.D. Martin, M.G. Ryskin]] \\ [[https://arxiv.org/abs/hep-ph/0306169|G. Watt, A.D. Martin, M.G. Ryskin]]   |
+| KLSZ'2020 (KMR)  |  1  |  4  |  143  |  [[https://arxiv.org/abs/1911.01445|A.V. Kotikov, A.V. Lipatov, B.G. Shaikhatdenov, P. Zhang]]   |
-| KMR (NNPDF3.1)  |  1  |  5  |  167  |  [[https://arxiv.org/abs/hep-ph/9911379|M.A. Kimber, A.D. Martin, M.G. Ryskin]] \\ [[https://arxiv.org/abs/hep-ph/0306169|G. Watt, A.D. Martin, M.G. Ryskin]]   |
-| KMR (DAS set 1)  |  1  |  4  |  143  |  [[https://arxiv.org/abs/1911.01445|A.V. Kotikov, A.V. Lipatov, B.G. Shaikhatdenov, P. Zhang]]   |
-| KMR (DAS set 2)  |  1  |  4  |  143  |  [[https://arxiv.org/abs/1911.01445|A.V. Kotikov, A.V. Lipatov, B.G. Shaikhatdenov, P. Zhang]]   |
 | PB NLO set 1  |  2  |  4  |  118  |  [[https://arxiv.org/abs/1704.01757|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]   |
 | PB NLO set 2  |  2  |  4  |  118  |  [[https://arxiv.org/abs/1704.01757|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]   |
@@ Line 84: / Line 81: @@
 The A0+, A0-, B0+, B0-, JH'2013 set 1(2)+ and JH'2013 set 1(2)- distributions, needed
 to estimate the scale uncertainties of the CCFM-based calculations, are not shown in the Table.
+Additionally, any other TMD gluon density in a proton could be used:
+one just have to upload it from the separate data file (prepared in the standard uPDFEvolve format).
 ===== Strong coupling and masses of particles =====