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--- pegasus:overview [02/09/2023 13:25] – lipatov
+++ pegasus:overview [02/09/2023 14:36] – 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.
+In principle, 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 [[https://arxiv.org/abs/1407.5935|uPDFevolv]] routine format.
 ===== Strong coupling and masses of particles =====
@@ Line 131: / Line 130: @@
 Contributions to the physics in PEGASUS were provided by Anatoly Kotikov (JINR, Dubna) and
-Nizami Abdulov (MSU, Moscow). We thank Vladimir Lyubushkin (JINR, Dubna), Gennady Lykasov (JINR, Dubna)
+Gennady Lykasov (JINR, Dubna). We thank Vladimir Lyubushkin (JINR, Dubna) and Alsu Bagdatova (LPI, Moscow), who contributed significantly to the functionality and stability of PEGASUS.
-and Andrey Prokhorov (MSU, Moscow & JINR, Dubna), who contributed significantly to the functionality and stability of PEGASUS.
 We are especially grateful to Nikolai Zotov, who guided and supervised our first steps in High Energy Physics,
 who encouraged our progress in k<sub>t</sub>-factorization and whose enthusiasm consolidated our group. Nikolai Zotov passed away on January 2016. Our work is dedicated to his memory.