Should you encounter any unexpected behaviour,
please let us know.

* gal1_monomer_wt *

CA distance fluctuations for 2405021233474105405

--- normal mode 11 ---

This matrix displays the maximum distance fluctuations between all pairs of CA atoms and between the two extreme conformations that were computed for this mode (DQMIN/DQMAX). Distance increases are plotted in blue and decreases in red for the strongest 10% of the residue pair distance changes. Every pixel corresponds to a single residue. Grey lines are drawn every 10 residues, yellow lines every 100 residues (counting from the upper left corner).

The following table indicates for every residue the two corresponding residues with the strongest CA distance fluctuations.

[HELP on distance fluctuations]

GD ok

largest increase ref largest decrease
ASN 1008 0.57 ALA 1001 -0.98 GLY 1053

LYS 1129 0.90 SER 1002 -0.98 HIS 1052

CYS 1130 0.90 GLY 1003 -0.68 ASP 1125

GLY 1003 0.57 LEU 1004 -0.72 ASP 1125

ALA 1001 0.32 VAL 1005 -0.57 ASP 1125

ALA 1001 0.45 ALA 1006 -0.51 LYS 1127

ALA 1001 0.50 SER 1007 -0.41 ASP 1125

ALA 1001 0.57 ASN 1008 -0.36 LYS 1127

ALA 1001 0.51 LEU 1009 -0.33 LYS 1127

ALA 1001 0.49 ASN 1010 -0.27 LYS 1127

ALA 1001 0.40 LEU 1011 -0.23 ASP 1125

ALA 1001 0.37 LYS 1012 -0.19 ASP 1125

ALA 1001 0.27 PRO 1013 -0.14 ASP 1125

GLU 1105 0.28 GLY 1014 -0.10 VAL 1031

ALA 1001 0.33 GLU 1015 -0.12 ASP 1125

GLY 1003 0.50 LEU 1017 -0.14 ASP 1125

GLY 1003 0.60 ARG 1018 -0.08 ASP 1125

GLY 1003 0.72 VAL 1019 -0.11 ASP 1125

GLY 1003 0.64 ARG 1020 -0.11 ASN 1008

SER 1002 0.52 GLY 1021 -0.25 ALA 1006

SER 1002 0.33 GLU 1022 -0.31 ALA 1006

ASP 1102 0.10 VAL 1023 -0.36 LEU 1004

ASP 1102 0.12 ALA 1024 -0.58 LEU 1004

PRO 1078 0.20 PRO 1025 -0.53 LEU 1004

PRO 1078 0.23 ASP 1026 -0.67 GLY 1003

PRO 1078 0.12 ALA 1027 -0.59 GLY 1003

PRO 1078 0.11 LYS 1028 -0.75 SER 1002

ASP 1125 0.10 SER 1029 -0.66 GLY 1124

LYS 1127 0.12 PHE 1030 -0.49 GLY 1124

LYS 1127 0.06 VAL 1031 -0.27 SER 1038

ALA 1122 0.31 LEU 1032 -0.24 ASP 1125

GLY 1003 0.15 ASN 1033 -0.34 ASP 1123

GLY 1003 0.18 LEU 1034 -0.28 ASP 1123

ALA 1001 0.15 GLY 1035 -0.34 ASP 1123

ALA 1001 0.24 LYS 1036 -0.35 ASP 1123

ALA 1001 0.23 ASP 1037 -0.44 ASP 1123

ALA 1001 0.11 SER 1038 -0.60 ASP 1123

ASN 1008 0.11 ASN 1039 -0.68 SER 1002

ASN 1008 0.10 ASN 1040 -0.47 SER 1002

MET 1120 0.08 LEU 1041 -0.38 ASP 1123

GLY 1035 0.11 CYS 1042 -0.29 ASP 1123

GLY 1003 0.12 LEU 1043 -0.24 ASP 1123

ALA 1121 0.09 HIS 1044 -0.29 ASP 1123

GLY 1003 0.14 PHE 1045 -0.19 ALA 1001

LYS 1127 0.06 ASN 1046 -0.34 ALA 1001

ASP 1026 0.09 PRO 1047 -0.45 ALA 1001

ASP 1026 0.13 ARG 1048 -0.63 ALA 1001

ASP 1026 0.20 PHE 1049 -0.75 ALA 1001

ASP 1026 0.17 ASN 1050 -0.89 ALA 1001

ASP 1026 0.10 ALA 1051 -0.95 SER 1002

ASP 1054 0.10 HIS 1052 -0.98 SER 1002

GLU 1074 0.14 GLY 1053 -0.98 ALA 1001

GLU 1074 0.17 ASP 1054 -0.89 ALA 1001

GLU 1074 0.22 ALA 1055 -0.94 ALA 1001

ASP 1026 0.21 ASN 1056 -0.77 ALA 1001

LYS 1107 0.20 THR 1057 -0.67 ALA 1001

PHE 1108 0.16 ILE 1058 -0.49 ALA 1001

PHE 1108 0.09 VAL 1059 -0.46 ALA 1001

THR 1057 0.07 CYS 1060 -0.31 ALA 1001

MET 1120 0.07 ASN 1061 -0.36 SER 1002

MET 1120 0.08 SER 1062 -0.38 SER 1002

ASN 1008 0.07 LYS 1063 -0.52 SER 1002

PRO 1109 0.08 ASP 1064 -0.51 SER 1002

ARG 1111 0.10 ASP 1065 -0.61 SER 1002

ASN 1008 0.09 GLY 1066 -0.74 SER 1002

ASN 1008 0.08 ALA 1067 -0.64 SER 1002

ASN 1008 0.07 TRP 1068 -0.58 SER 1002

THR 1070 0.08 GLY 1069 -0.44 SER 1002

GLY 1069 0.08 THR 1070 -0.39 SER 1002

ASP 1026 0.06 GLU 1071 -0.42 ALA 1001

THR 1057 0.14 GLN 1072 -0.41 ALA 1001

PHE 1108 0.20 ARG 1073 -0.51 ALA 1001

ALA 1055 0.22 GLU 1074 -0.48 ALA 1001

LYS 1107 0.28 ALA 1075 -0.57 ALA 1001

PHE 1106 0.26 VAL 1076 -0.53 ALA 1001

PHE 1106 0.27 PHE 1077 -0.55 ALA 1001

GLN 1080 0.29 PRO 1078 -0.43 ALA 1001

ASP 1026 0.20 PHE 1079 -0.45 ALA 1001

PRO 1078 0.29 GLN 1080 -0.54 ALA 1001

PRO 1078 0.25 PRO 1081 -0.56 ALA 1001

ASP 1102 0.21 GLY 1082 -0.44 ALA 1001

ASP 1102 0.21 SER 1083 -0.32 ALA 1001

SER 1002 0.29 VAL 1084 -0.17 ALA 1006

GLY 1003 0.29 ALA 1085 -0.14 ALA 1001

GLY 1003 0.45 GLU 1086 -0.07 VAL 1031

GLY 1003 0.44 VAL 1087 -0.09 VAL 1031

GLY 1003 0.45 CYS 1088 -0.09 VAL 1031

GLY 1003 0.38 ILE 1089 -0.11 VAL 1031

GLY 1003 0.31 THR 1090 -0.12 VAL 1031

GLU 1105 0.23 PHE 1091 -0.16 VAL 1031

GLU 1105 0.24 ASP 1092 -0.14 VAL 1031

ALA 1075 0.22 GLN 1093 -0.16 ASP 1123

ALA 1075 0.26 ALA 1094 -0.15 ASP 1123

ALA 1075 0.25 ASN 1095 -0.14 ASP 1123

ALA 1075 0.19 LEU 1096 -0.14 VAL 1031

GLY 1003 0.24 THR 1097 -0.11 VAL 1031

GLY 1003 0.28 VAL 1098 -0.11 VAL 1031

GLY 1003 0.29 LYS 1099 -0.12 VAL 1031

GLY 1003 0.25 LEU 1100 -0.17 ALA 1001

GLY 1003 0.26 PRO 1101 -0.17 ALA 1001

GLN 1080 0.29 ASP 1102 -0.24 ALA 1001

GLY 1014 0.28 GLY 1103 -0.15 ALA 1001

GLY 1014 0.27 TYR 1104 -0.24 ALA 1001

GLY 1014 0.28 GLU 1105 -0.17 ALA 1001

PHE 1077 0.27 PHE 1106 -0.19 ALA 1001

ALA 1075 0.28 LYS 1107 -0.13 ALA 1001

ALA 1075 0.23 PHE 1108 -0.14 SER 1002

ALA 1075 0.23 PRO 1109 -0.18 SER 1002

ALA 1075 0.18 ASN 1110 -0.21 ASP 1123

ALA 1075 0.15 ARG 1111 -0.27 SER 1002

ALA 1075 0.12 LEU 1112 -0.29 SER 1002

ALA 1075 0.15 ASN 1113 -0.24 ASP 1123

ALA 1001 0.17 LEU 1114 -0.25 ASP 1123

ALA 1001 0.26 GLU 1115 -0.22 ASP 1123

ALA 1001 0.31 ALA 1116 -0.23 ASP 1125

ALA 1001 0.29 ILE 1117 -0.27 ASP 1125

ALA 1001 0.39 ASN 1118 -0.32 ASP 1125

ALA 1001 0.31 TYR 1119 -0.37 ASP 1125

ALA 1001 0.24 MET 1120 -0.42 ASP 1125

GLY 1003 0.22 ALA 1121 -0.51 ASP 1125

GLY 1003 0.34 ALA 1122 -0.61 ASP 1125

ILE 1128 0.49 ASP 1123 -0.60 SER 1038

LYS 1127 0.27 GLY 1124 -0.66 SER 1029

SER 1029 0.10 ASP 1125 -0.72 LEU 1004

ASP 1123 0.18 PHE 1126 -0.48 LEU 1004

SER 1002 0.50 LYS 1127 -0.52 LEU 1004

GLY 1003 0.80 ILE 1128 -0.39 ALA 1006

SER 1002 0.90 LYS 1129 -0.25 ALA 1006

GLY 1003 0.90 CYS 1130 -0.19 LYS 1129

GLY 1003 0.80 VAL 1131 -0.24 LYS 1129

GLY 1003 0.65 ALA 1132 -0.16 LYS 1129

GLY 1003 0.49 PHE 1133 -0.20 LYS 1129

ALA 1001 0.46 ASP 1134 -0.13 LYS 1129

If you find results from this site helpful for your research, please cite one of our papers:

K. Suhre & Y.H. Sanejouand, ElNemo: a normal mode web-server for protein movement analysis and the generation of templates for molecular replacement. Nucleic Acids Research, 32, W610-W614, 2004.
K. Suhre & Y.H. Sanejouand, On the potential of normal mode analysis for solving difficult molecular replacement problems. Acta Cryst. D vol.60, p796-799, 2004 © International Union of Crystallography.

elNémo is maintained by Yves-Henri Sanejouand.
It was developed by Karsten Suhre.
Between 2003 and 2014, it was hosted by IGS (Marseille).
Last modification: April 25th, 2023.

Should you encounter any unexpected behaviour, please let us know.

*** gal1_monomer_wt ***

CA distance fluctuations for 2405021233474105405

--- normal mode 11 ---

Should you encounter any unexpected behaviour,
please let us know.

* gal1_monomer_wt *