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NAMERNAparconv - manual page for RNAparconv 2.5.0SYNOPSISRNAparconv [options] [<input file>] [<output file>]DESCRIPTIONRNAparconv 2.5.0Convert energy parameter files from ViennaRNA 1.8.4 to 2.0 format Converts energy parameter files from "old" ViennaRNAPackage 1.8.4 format to the new format used since ViennaRNAPackage 2.0. The Program reads a valid energy parameter file or valid energy parameters from stdin and prints the converted energy parameters to stdout or a specified output file. Per default, the converted output file contains the whole set of energy parameters used throughout ViennaRNAPackage 1.8.4. The user can specify sets of energy parameters that should not be included in the output.
REFERENCESIf you use this program in your work you might want to cite:R. Lorenz, S.H. Bernhart, C. Hoener zu Siederdissen, H. Tafer, C. Flamm, P.F. Stadler and I.L. Hofacker (2011), "ViennaRNA Package 2.0", Algorithms for Molecular Biology: 6:26 I.L. Hofacker, W. Fontana, P.F. Stadler, S. Bonhoeffer, M. Tacker, P. Schuster (1994), "Fast Folding and Comparison of RNA Secondary Structures", Monatshefte f. Chemie: 125, pp 167-188 R. Lorenz, I.L. Hofacker, P.F. Stadler (2016), "RNA folding with hard and soft constraints", Algorithms for Molecular Biology 11:1 pp 1-13 The energy parameters are taken from: D.H. Mathews, M.D. Disney, D. Matthew, J.L. Childs, S.J. Schroeder, J. Susan, M. Zuker, D.H. Turner (2004), "Incorporating chemical modification constraints into a dynamic programming algorithm for prediction of RNA secondary structure", Proc. Natl. Acad. Sci. USA: 101, pp 7287-7292 D.H Turner, D.H. Mathews (2009), "NNDB: The nearest neighbor parameter database for predicting stability of nucleic acid secondary structure", Nucleic Acids Research: 38, pp 280-282 AUTHORRonny LorenzREPORTING BUGSIf in doubt our program is right, nature is at fault. Comments should be sent to rna@tbi.univie.ac.at.
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