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

* gal1_monomer_wt *

CA distance fluctuations for 2405021233474105405

--- normal mode 8 ---

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
GLY 1066 0.98 ALA 1001 -0.34 ILE 1128

ASN 1039 1.10 SER 1002 -0.40 LYS 1127

SER 1038 0.62 GLY 1003 -0.31 LEU 1004

SER 1038 0.40 LEU 1004 -0.31 GLY 1003

LYS 1129 0.32 VAL 1005 -0.33 HIS 1052

CYS 1130 0.30 ALA 1006 -0.26 HIS 1052

SER 1002 0.26 SER 1007 -0.24 HIS 1052

SER 1002 0.20 ASN 1008 -0.19 HIS 1052

GLY 1103 0.14 LEU 1009 -0.16 HIS 1052

SER 1002 0.16 ASN 1010 -0.12 HIS 1052

SER 1002 0.12 LEU 1011 -0.14 ARG 1018

SER 1002 0.14 LYS 1012 -0.19 ARG 1018

SER 1002 0.14 PRO 1013 -0.23 ARG 1018

LYS 1107 0.14 GLY 1014 -0.29 ARG 1018

THR 1097 0.16 GLU 1015 -0.31 ARG 1018

GLY 1103 0.21 LEU 1017 -0.25 ARG 1018

GLY 1103 0.25 ARG 1018 -0.31 GLU 1015

ALA 1121 0.23 VAL 1019 -0.20 GLU 1015

ALA 1121 0.26 ARG 1020 -0.22 GLY 1014

SER 1038 0.31 GLY 1021 -0.24 SER 1002

ASN 1039 0.32 GLU 1022 -0.26 SER 1002

GLY 1066 0.35 VAL 1023 -0.25 SER 1002

GLY 1066 0.43 ALA 1024 -0.28 SER 1002

GLY 1066 0.40 PRO 1025 -0.24 ASP 1102

GLY 1066 0.43 ASP 1026 -0.25 SER 1002

GLY 1066 0.44 ALA 1027 -0.29 SER 1002

GLY 1066 0.42 LYS 1028 -0.30 SER 1002

GLY 1066 0.40 SER 1029 -0.30 GLY 1124

GLY 1066 0.42 PHE 1030 -0.29 GLY 1124

GLY 1066 0.36 VAL 1031 -0.27 HIS 1052

ASN 1039 0.28 LEU 1032 -0.21 HIS 1052

SER 1002 0.36 ASN 1033 -0.23 HIS 1052

SER 1002 0.36 LEU 1034 -0.15 HIS 1052

SER 1002 0.49 GLY 1035 -0.11 HIS 1052

SER 1002 0.57 LYS 1036 -0.13 ASN 1008

SER 1002 0.77 ASP 1037 -0.18 ASN 1008

SER 1002 1.08 SER 1038 -0.18 HIS 1052

SER 1002 1.10 ASN 1039 -0.13 TRP 1068

SER 1002 0.79 ASN 1040 -0.12 ASN 1008

SER 1002 0.61 LEU 1041 -0.11 ASN 1008

SER 1002 0.43 CYS 1042 -0.08 PHE 1106

SER 1002 0.33 LEU 1043 -0.07 GLY 1035

SER 1002 0.33 HIS 1044 -0.13 ASN 1033

ALA 1001 0.15 PHE 1045 -0.11 VAL 1005

GLY 1066 0.22 ASN 1046 -0.17 VAL 1005

GLY 1066 0.20 PRO 1047 -0.16 GLY 1124

GLY 1066 0.20 ARG 1048 -0.23 GLY 1124

GLY 1066 0.23 PHE 1049 -0.23 SER 1002

ALA 1067 0.22 ASN 1050 -0.27 SER 1002

ALA 1067 0.26 ALA 1051 -0.29 GLY 1124

THR 1070 0.25 HIS 1052 -0.33 VAL 1005

ALA 1075 0.15 GLY 1053 -0.26 VAL 1005

ALA 1075 0.14 ASP 1054 -0.20 VAL 1005

GLN 1080 0.12 ALA 1055 -0.20 SER 1002

GLY 1066 0.11 ASN 1056 -0.17 GLY 1124

VAL 1076 0.09 THR 1057 -0.14 GLY 1124

ASP 1134 0.07 ILE 1058 -0.10 GLY 1124

LYS 1107 0.13 VAL 1059 -0.14 VAL 1005

ALA 1001 0.20 CYS 1060 -0.11 VAL 1005

ALA 1001 0.34 ASN 1061 -0.12 GLN 1072

SER 1002 0.47 SER 1062 -0.11 PHE 1106

SER 1002 0.69 LYS 1063 -0.12 GLN 1072

SER 1002 0.73 ASP 1064 -0.16 ARG 1111

SER 1002 0.89 ASP 1065 -0.19 LEU 1112

SER 1002 1.01 GLY 1066 -0.10 ASN 1008

ALA 1001 0.81 ALA 1067 -0.13 THR 1070

ALA 1001 0.62 TRP 1068 -0.15 GLU 1071

ALA 1001 0.50 GLY 1069 -0.15 GLN 1072

ALA 1001 0.37 THR 1070 -0.18 ALA 1075

ALA 1001 0.25 GLU 1071 -0.15 ARG 1073

ALA 1001 0.18 GLN 1072 -0.17 GLU 1074

LYS 1107 0.19 ARG 1073 -0.15 GLU 1071

GLY 1053 0.13 GLU 1074 -0.17 GLN 1072

ASP 1134 0.15 ALA 1075 -0.18 THR 1070

ASP 1134 0.15 VAL 1076 -0.14 GLN 1080

GLU 1086 0.12 PHE 1077 -0.13 GLU 1074

GLU 1086 0.12 PRO 1078 -0.28 GLN 1080

GLY 1066 0.17 PHE 1079 -0.23 PRO 1078

GLY 1066 0.23 GLN 1080 -0.31 ASP 1102

GLY 1066 0.31 PRO 1081 -0.28 ASP 1102

GLY 1066 0.33 GLY 1082 -0.29 ASP 1102

GLY 1066 0.26 SER 1083 -0.33 ASP 1102

ASN 1039 0.25 VAL 1084 -0.20 PRO 1101

ASN 1039 0.20 ALA 1085 -0.20 LYS 1099

ALA 1121 0.21 GLU 1086 -0.22 THR 1090

ALA 1121 0.17 VAL 1087 -0.20 THR 1090

PHE 1133 0.22 CYS 1088 -0.26 THR 1090

ASP 1134 0.22 ILE 1089 -0.16 ALA 1085

ASP 1134 0.23 THR 1090 -0.26 CYS 1088

SER 1002 0.15 PHE 1091 -0.24 ARG 1018

SER 1002 0.16 ASP 1092 -0.21 ARG 1018

SER 1002 0.23 GLN 1093 -0.17 ARG 1018

SER 1002 0.23 ALA 1094 -0.17 LYS 1099

SER 1002 0.20 ASN 1095 -0.16 THR 1097

SER 1002 0.16 LEU 1096 -0.16 CYS 1088

ASP 1134 0.22 THR 1097 -0.17 ALA 1085

ASP 1134 0.22 VAL 1098 -0.17 ALA 1085

ASP 1134 0.26 LYS 1099 -0.21 SER 1083

ARG 1018 0.19 LEU 1100 -0.23 SER 1083

ARG 1018 0.19 PRO 1101 -0.31 SER 1083

ARG 1018 0.22 ASP 1102 -0.33 SER 1083

ASP 1134 0.28 GLY 1103 -0.27 SER 1083

ASP 1134 0.26 TYR 1104 -0.21 SER 1083

ASP 1134 0.28 GLU 1105 -0.20 SER 1083

ASP 1134 0.22 PHE 1106 -0.20 PRO 1109

ARG 1073 0.19 LYS 1107 -0.19 PRO 1109

SER 1002 0.19 PHE 1108 -0.18 PHE 1106

SER 1002 0.26 PRO 1109 -0.20 PHE 1106

SER 1002 0.32 ASN 1110 -0.14 ASP 1065

SER 1002 0.40 ARG 1111 -0.17 PHE 1106

SER 1002 0.48 LEU 1112 -0.19 ASP 1065

SER 1002 0.40 ASN 1113 -0.17 ASP 1065

SER 1002 0.39 LEU 1114 -0.17 ASP 1065

SER 1002 0.31 GLU 1115 -0.14 ASP 1065

SER 1002 0.28 ALA 1116 -0.13 ASP 1065

SER 1002 0.29 ILE 1117 -0.09 ARG 1018

SER 1002 0.32 ASN 1118 -0.15 HIS 1052

SER 1002 0.40 TYR 1119 -0.20 HIS 1052

SER 1002 0.27 MET 1120 -0.23 HIS 1052

LYS 1127 0.36 ALA 1121 -0.31 HIS 1052

SER 1038 0.46 ALA 1122 -0.28 HIS 1052

ASN 1039 0.65 ASP 1123 -0.28 HIS 1052

GLY 1066 0.63 GLY 1124 -0.30 SER 1029

GLY 1066 0.53 ASP 1125 -0.38 SER 1002

GLY 1066 0.42 PHE 1126 -0.34 SER 1002

SER 1038 0.45 LYS 1127 -0.40 SER 1002

SER 1038 0.35 ILE 1128 -0.36 SER 1002

VAL 1005 0.32 LYS 1129 -0.33 ALA 1001

ALA 1006 0.30 CYS 1130 -0.30 ALA 1001

ALA 1006 0.22 VAL 1131 -0.27 ALA 1001

GLY 1103 0.24 ALA 1132 -0.25 CYS 1130

GLY 1103 0.25 PHE 1133 -0.20 GLY 1003

GLY 1103 0.28 ASP 1134 -0.24 CYS 1130

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 8 ---

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

* gal1_monomer_wt *