You can run RESOLVE right after SOLVE (using solve.mtz as input), or you can run it using an mtz-format file written by another program.
Usually if you have MAD/SAD/MIR data, you will want to (1) edit and run one of the standard SOLVE scripts( to solve your structure and calculate an initial map, and (2) edit and run the RESOLVE_BUILD script to density modify the map and build an atomic model. With fast model-building, the whole process only takes a few hours for a small protein.
If you have an MR model and FOBS data, you will want to run the RESOLVE_BUILD script to remove model bias and build a new atomic model.
If you have non-crystallographic symmetry, you will want to include that in your RESOLVE scripts, either by specifying the NCS matrices (see Keywords for resolve) or by specifying the coordinates of some of the atoms in each monomer with a PDB file "ha.pdb" (this can be the heavy-atom file written by SOLVE for MIR/MAD/SAD data, or a file you create from some of the CA atoms in your starting PDB file for your MR solution).
It is really easy to run RESOLVE right after SOLVE.
Just go to the directory where you ran SOLVE and type (or put in a command
file):
#!/bin/csh # Here is a very minimal script to run RESOLVE: # Set CCP4 variables for symmetry information and # for file handling: setenv SYMOP /usr/local/lib/solve/symop.lib setenv SYMINFO /usr/local/lib/solve/syminfo.lib setenv CCP4_OPEN UNKNOWN # Now run RESOLVE: resolve<<EOD solvent_content 0.4 ! your solvent content goes here. ! Next line is protein sequence file seq_file protein.seq EOD # Now "resolve.mtz" has the output amplitudes, weighted F, phases, # figure of merit and HL-coeffs in columns labelled: FP PHIM FOMM HLAM HLBM HLCM HLDM # Also resolve.pdb contains your model and the heavy-atom sites from SOLVE. # |
That's it! (Sure, there are a few other keywords, but usually you don't need them.) (More sample scripts are available too.)