distance restraints
were obtained from NOESY spectra collected with a mixing time of 100
ms. The NOE cross-peaks were integrated with the XEASY program and
were converted into upper distance bounds using the CALIBA program
incorporated into the program package CYANA.92 (link) Only NOE-derived constraints were considered in the annealing procedures.
An ensemble of 200 structures was generated with the simulated annealing
of the program CYANA. Then, 20 structures were chosen, whose interproton
distances best fitted NOE-derived distances, and refined through successive
steps of restrained and unrestrained energy minimization calculations
using the Discover algorithm (Accelrys, San Diego, CA) and the consistent
valence force field.93 (link) The minimization
lowered the total energy of the structures; no residue was found in
the disallowed region of the Ramachandran plot. The final structures
were analyzed using the InsightII program (Accelrys, San Diego, CA).
Molecular graphics images were realized using the UCSF Chimera package.94 (link)