#!/bin/csh -f
glrf <<EOF
title DHFR, Cross Rotation, origin kept
!
print cross.prt
!
!
! conventions
!
polar xyk
euler zyz
orthogonalization axabz
!
!
!locsymmetry 80. 90. 180.0 2 P
!locexpand true
!
!
acell 100 100 100 90 90 90
asymm x, y, z
aobsfile work/t1.cal
aformat 3i4, f8.2, 8x, f8.2
acutoff 1 1 0
apower 2
origin false
!
bcell 41.580 74.180 59.180 90.00 99.26
90.00
bsymmetry P21
bobsfile work/r1rb3sf.fin
bformat (3i4, 2f8.2)
bcutoff 2.0 1.0 0.0
bpower 2
!
cutoff 1.5
!
resolution 9 2.5
radius 25.0
!
self false
cross true
fast true
!
sangle euler
slimit 1 0 360 5
slimit 2 0 90 5
slimit 3 0 360 5
!
mapfile cross.map
peak 2.0 50
oangle polar xyk
!
cntfile cross.ps
cntlevel 450 1000 50
section 213
cntsection 1 37
!
stop
EOF |
Call the program "glrf" to read the following script
cross.prt is the log file. It will contain a list of
the peaks found in this cross rotation function.
Use these conventions; they are consistent with those
used by CCP4 programs.
If the self rotation function indicates NCS
rotational symmetry, you can specify the angle here. Top solutions
in the cross rotation will be constrained to maintain these relationships.
Remove the "!" to uncomment. In this example, (80, 90, 180) corresponds
to phi, psi, and kappa. "2" specifies a 2-fold axis. "P" specifies
that you are using polar angle conventions here.
unit cell parameters used to calculate
structure factors from the model (in sfcal.com).
asymm x,y,z refers to the symmetry operators
used in
sfcal.com (P1 is x,y,z).
aobs-file. Name of the file containing
structure factors calculated from your model's coordinates (see sfcal.com,
step 1 above).
aformat refers to the format of the model
structure factors. These will be correct for output from sfcal.com.
unit cell parameters of your crystal.
bsymm -space group of your crystal.
bobsfile -structure factors of your crystal.
(here in .fin format)
format of your structure factor file (here
in .fin format)
bpower- 2 if structure factors, 1 if intensities
resolution. You should experiment with
the resolution range. (e.g. 9-3, 9-5, 8-4, etc.) If your model is relatively
poor, peaks in the RF may only be seen at lower resolution.
radius of integration. Again, experiment
with this parameter. Use values between the radius and diameter of your protein
molecule.
slimits. Let theta1, theta2, and theta3
vary over the asymmetric unit of rotational space. Use 5 degree intervals.
If you dont know the limits of the asymmetric unit in rotation space, see
Rao
et al., Acta Cryst. A36, 878-884 (1980).
mapfile. The output map containing
the cross rotation function.
peak. Show top 50 peaks with a height
greater than 2.0
cntlevel. Contour all peaks above the 450 level, where
the highest peak is scaled to the 1000 level. Show intervals of 50.
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