Provided by: vienna-rna_2.4.17+dfsg-2build2_amd64 bug

NAME

       RNAplfold - manual page for RNAplfold 2.4.17

SYNOPSIS

       RNAplfold [OPTION]...

DESCRIPTION

       RNAplfold 2.4.17

       calculate locally stable secondary structure - pair probabilities

       Computes local pair probabilities for base pairs with a maximal span of L. The probabilities are averaged
       over all windows of size L that contain the base pair. For a sequence of length n and a window size of  L
       the  algorithm uses only O(n+L*L) memory and O(n*L*L) CPU time. Thus it is practical to "scan" very large
       genomes for short stable RNA structures.

       Output consists of a dot plot in postscript file, where the averaged pair  probabilities  can  easily  be
       parsed and visually inspected.

       The  -u option makes i possible to compute the probability that a stretch of x consequtive nucleotides is
       unpaired, which is useful for predicting possible binding sites. Again this probability is averaged  over
       all windows containing the region.

       WARNING! Output format changed!!

       The output is a plain text matrix containing on each line a position i followed by the probability that i
       is unpaired, [i-1..i] is unpaired [i-2..i] is unpaired and so on to the probability  that  [i-x+1..i]  is
       unpaired.

       -h, --help
              Print help and exit

       --detailed-help
              Print help, including all details and hidden options, and exit

       --full-help
              Print help, including hidden options, and exit

       -V, --version
              Print version and exit

   General Options:
              Command line options which alter the general behavior of this program

       -v, --verbose
              Be verbose.  (default=off)

       -W, --winsize=size
              Average the pair probabilities over windows of given size.  (default=`70')

       -L, --span=size
              Set the maximum allowed separation of a base pair to span.

              By  setting the maximum base pair span no pairs (i,j) with j-i > span will be allowed. Defaults to
              winsize if parameter is omitted.

       -c, --cutoff=FLOAT
              Report only base pairs with an average probability > cutoff in the dot plot.  (default=`0.01')

       -o, --print_onthefly
              Save memory by printing out everything during computation.  (default=off)

              NOTE: activated per default for sequences over 1M bp.

       -u, --ulength=length
              Compute the  mean  probability  that  regions  of  length  1  to  a  given  length  are  unpaired.
              (default=`31')

              Output is saved in a _lunp file.

       -O, --opening_energies
              Switch output from probabilities to their logarithms.  (default=off)

              This  is  NOT exactly the mean energies needed to unfold the respective stretch of bases! (implies
              --ulength option).

       --plex_output
              Create additional output files for RNAplex.  (default=off)

       --noconv
              Do not automatically substitude nucleotide "T" with "U".  (default=off)

       --auto-id
              Automatically generate an ID for each sequence.  (default=off)

              The default mode of RNAplfold is to automatically determine an ID from the input sequence data  if
              the  input  file  format  allows to do that. Sequence IDs are usually given in the FASTA header of
              input sequences. If this flag is active, RNAplfold ignores any IDs retrieved from  the  input  and
              automatically  generates  an  ID for each sequence. This ID consists of a prefix and an increasing
              number. This flag can also be used to add a FASTA header to the output even if the input has none.

       --id-prefix=prefix
              Prefix for automatically generated IDs (as used in output file names).  (default=`sequence')

              If this parameter is set, each sequences' FASTA id will be  prefixed  with  the  provided  string.
              FASTA  ids  then take the form ">prefix_xxxx" where xxxx is the sequence number. Hence, the output
              files will obey the following naming scheme:  "prefix_xxxx_dp.ps"  (dot-plot),  "prefix_xxxx_lunp"
              (unpaired probabilities), etc. Note: Setting this parameter implies --auto-id.

       --id-delim=STRING
              Change the delimiter between prefix and increasing number for automatically generated IDs (as used
              in output file names).  (default=`_')

              This parameter can be used to change the default delimiter "_" between

              the prefix string and the increasing number for automatically generated ID.

       --id-digits=INT
              Specify  the  number  of  digits  of  the  counter  in  automatically  generated  alignment   IDs.
              (default=`4')

              When  alignments IDs are automatically generated, they receive an increasing number, starting with
              1. This number will always be left-padded by leading zeros,  such  that  the  number  takes  up  a
              certain  width.  Using  this  parameter,  the  width  can be specified to the users need. We allow
              numbers in the range [1:18]. This option implies --auto-id.

       --id-start=LONG
              Specify the first number in automatically generated alignment IDs.  (default=`1')

              When sequence IDs are automatically generated, they receive an increasing number, usually starting
              with  1.  Using this parameter, the first number can be specified to the users requirements. Note:
              negative numbers are not allowed.   Note:  Setting  this  parameter  implies  to  ignore  any  IDs
              retrieved from the input data, i.e. it activates the --auto-id flag.

       --filename-delim=STRING
              Change the delimiting character that is used for sanitized filenames.  (default=`ID-delimiter')

              This  parameter  can  be  used to change the delimiting character used while sanitizing filenames,
              i.e. replacing invalid characters. Note, that the default delimiter ALWAYS is the first  character
              of  the "ID delimiter" as supplied through the --id-delim option. If the delimiter is a whitespace
              character or empty, invalid characters will be simply removed rather than substituted.  Currently,
              we  regard  the  following  characters  as illegal for use in filenames: backslash '\', slash '/',
              question mark '?', percent sign '%', asterisk '*', colon ':', pipe symbol '|', double  quote  '"',
              triangular brackets '<' and '>'.

       --filename-full
              Use full FASTA header to create filenames.  (default=off)

              This  parameter can be used to deactivate the default behavior of limiting output filenames to the
              first word of the sequence ID.  Consider  the  following  example:  An  input  with  FASTA  header
              ">NM_0001  Homo Sapiens some gene" usually produces output files with the prefix "NM_0001" without
              the additional data available in the FASTA header, e.g. "NM_0001_dp.ps". With this  flag  set,  no
              truncation  of  the  output  filenames is performed, i.e.  output filenames receive the full FASTA
              header data as prefixes. Note, however, that invalid  characters  (such  as  whitespace)  will  be
              substituted  by  a  delimiting  character  or  simply  removed,  (see  also  the  parameter option
              --filename-delim).

       --shape=<filename>
              Use SHAPE reactivity data to guide structure predictions.

       --shapeMethod=STRING
              Specify the  method  how  to  convert  SHAPE  reactivity  data  to  pseudo  energy  contributions.
              (default=`D')

              The following methods can be used to convert SHAPE reactivities into pseudo energy contributions.

              'D':  Convert  by  using  a  linear equation according to Deigan et al 2009. The calculated pseudo
              energies will be applied for  every  nucleotide  involved  in  a  stacked  pair.  This  method  is
              recognized  by  a  capital  'D'  in the provided parameter, i.e.: --shapeMethod="D" is the default
              setting. The slope 'm' and the intercept 'b' can be set  to  a  non-default  value  if  necessary,
              otherwise  m=1.8  and  b=-0.6.  To  alter these parameters, e.g. m=1.9 and b=-0.7, use a parameter
              string like this: --shapeMethod="Dm1.9b-0.7". You may also provide only one of the two  parameters
              like: --shapeMethod="Dm1.9" or --shapeMethod="Db-0.7".

              'Z':  Convert  SHAPE  reactivities  to pseudo energies according to Zarringhalam et al 2012. SHAPE
              reactivities will be converted to pairing probabilities by using linear mapping.  Aberration  from
              the  observed  pairing probabilities will be penalized during the folding recursion. The magnitude
              of the penalties can affected by adjusting the factor beta (e.g. --shapeMethod="Zb0.8").

              'W': Apply a given vector of perturbation energies to unpaired nucleotides according  to  Washietl
              et al 2012. Perturbation vectors can be calculated by using RNApvmin.

       --shapeConversion=STRING
              Specify  the  method  used  to  convert SHAPE reactivities to pairing probabilities when using the
              SHAPE approach of Zarringhalam et al.  (default=`O')

              The following methods can be used to convert SHAPE reactivities into the probability for a certain
              nucleotide to be unpaired.

              'M': Use linear mapping according to Zarringhalam et al.

              'C': Use a cutoff-approach to divide into paired and unpaired nucleotides (e.g. "C0.25")

              'S':  Skip  the  normalizing  step since the input data already represents probabilities for being
              unpaired rather than raw reactivity values

              'L': Use a linear model to convert the reactivity into a  probability  for  being  unpaired  (e.g.
              "Ls0.68i0.2" to use a slope of 0.68 and an intercept of 0.2)

              'O': Use a linear model to convert the log of the reactivity into a probability for being unpaired
              (e.g. "Os1.6i-2.29" to use a slope of 1.6 and an intercept of -2.29)

       --commands=<filename>
              Read additional commands from file.

              Commands include hard and soft constraints, but also structure  motifs  in  hairpin  and  interior
              loops  that  need to be treeted differently. Furthermore, commands can be set for unstructured and
              structured domains.

   Model Details:
       -T, --temp=DOUBLE
              Rescale energy parameters to a temperature in degrees centigrade.  (default=`37.0')

       -4, --noTetra
              Do not include special tabulated stabilizing energies for  tri-,  tetra-  and  hexaloop  hairpins.
              (default=off)

              Mostly for testing.

       -d, --dangles=INT
              Specify  "dangling  end"  model  for  bases  adjacent  to  helices  in  free ends and multi-loops.
              (default=`2')

              With -d2 dangling energies will be added for the bases adjacent to a helix on both  sides  in  any
              case while -d0 ignores dangling ends altogether (mostly for debugging).

       --noLP Produce structures without lonely pairs (helices of length 1).  (default=off)

              For partition function folding this only disallows pairs that can only occur isolated. Other pairs
              may still occasionally occur as helices of length 1.

       --noGU Do not allow GU pairs.  (default=off)

       --noClosingGU
              Do not allow GU pairs at the end of helices.  (default=off)

       -P, --paramFile=paramfile
              Read energy parameters from paramfile, instead of using the default parameter set.

              Different sets of energy parameters for RNA and DNA should accompany your distribution.   See  the
              RNAlib documentation for details on the file format. When passing the placeholder file name "DNA",
              DNA parameters are loaded without the need to actually specify any input file.

       -S, --pfScale=DOUBLE
              Set scaling factor for Boltzmann factors to prevent under/overflows.

              In the calculation of the partition function use pfScale * average_free_energy as an estimate  for
              the  ensemble free energy (used to avoid overflows). The default is 1.07, useful values are 1.0 to
              1.2.  Occasionally needed for longer folding windows.

       -b, --binaries
              Output accessibility profiles in binary format.  (default=off)

              The binary files produced by RNAplfold do not need to be parsed by RNAplex,

              so that they are directly loaded into memory. This is useful  when  large  sequences  have  to  be
              searched  for putative hybridization sites. Another advantage of the binary format is the 50% file
              size decrease.

       --nsp=STRING
              Allow other pairs in addition to the usual AU,GC,and GU pairs.

              Its argument is a comma separated list of additionally allowed pairs. If the first character is  a
              "-" then AB will imply that AB and BA are allowed pairs.  e.g. RNAfold -nsp -GA  will allow GA and
              AG pairs. Nonstandard pairs are given 0 stacking energy.

       -e, --energyModel=INT
              Set energy model.

              Rarely used option to fold sequences from the artificial ABCD... alphabet, where A  pairs  B,  C-D
              etc.  Use the energy parameters for GC (-e 1) or AU (-e 2) pairs.

       --betaScale=DOUBLE
              Set the scaling of the Boltzmann factors.  (default=`1.')

              The  argument provided with this option enables to scale the thermodynamic temperature used in the
              Boltzmann factors  independently  from  the  temperature  used  to  scale  the  individual  energy
              contributions of the loop types. The Boltzmann factors then become exp(-dG/(kT*betaScale)) where k
              is the Boltzmann constant, dG the free energy  contribution  of  the  state  and  T  the  absolute
              temperature.

REFERENCES

       If 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

       S. H. Bernhart, U. Mueckstein, and I.L. Hofacker (2011), "RNA Accessibility in  cubic  time",  Algorithms
       Mol Biol. 6: 3.

       S. H. Bernhart, I.L. Hofacker, and P.F. Stadler (2006), "Local Base Pairing Probabilities in Large RNAs",
       Bioinformatics: 22, pp 614-615

       A.F. Bompfuenewerer, R. Backofen, S.H. Bernhart, J. Hertel, I.L. Hofacker, P.F. Stadler, S. Will  (2007),
       "Variations on RNA Folding and Alignment: Lessons from Benasque", J. Math. Biol.

       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

AUTHOR

       Stephan H Bernhart, Ivo L Hofacker, Peter F Stadler, Ronny Lorenz

REPORTING BUGS

       If in doubt our program is right, nature is at fault.  Comments should be sent to rna@tbi.univie.ac.at.

SEE ALSO

       RNALfold(1)