Provided by: vienna-rna_2.6.4+dfsg-1build2_amd64 bug

NAME

       RNAsubopt - manual page for RNAsubopt 2.6.4

SYNOPSIS

       RNAsubopt [OPTION]...

DESCRIPTION

       RNAsubopt 2.6.4

       calculate suboptimal secondary structures of RNAs

       Reads  RNA  sequences  from  stdin  and  (in  the  default  -e  mode) calculates all suboptimal secondary
       structures within a user defined energy range  above  the  minimum  free  energy  (mfe).  It  prints  the
       suboptimal  structures  in dot-bracket notation followed by the energy in kcal/mol to stdout. Be careful,
       the number of structures returned grows exponentially with both sequence length and energy range.

       Alternatively, when used with the -p option, RNAsubopt produces Boltzmann weighted samples  of  secondary
       structures.

       -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

       -v, --verbose
              Be verbose.

              (default=off)

   I/O Options:
              Command line options for input and output (pre-)processing

       -i, --infile=filename
              Read a file instead of reading from stdin.

              The  default  behavior of RNAsubopt is to read input from stdin. Using this parameter the user can
              specify an input file name where data is read from.

       -o, --outfile[=filename]
              Print output to file instead of stdout.

              This option may be used to write all output to output files rather than printing  to  stdout.  The
              default filename is "RNAsubopt_output.sub" if no FASTA header precedes the input sequences and the
              --auto-id feature is inactive. Otherwise, output files with the scheme "prefix.sub" are generated,
              where  the  "prefix" is taken from the sequence id. The user may specify a single output file name
              for all data generated from the input  by  supplying  an  optional  string  as  argument  to  this
              parameter. In case a file with the same filename already exists, any output of the program will be
              appended  to  it.  Note:  Any  special characters in the filename will be replaced by the filename
              delimiter, hence there is no way to pass an entire directory path through this  option  yet.  (See
              also the "--filename-delim" parameter)

       --noconv
              Do not automatically substitute nucleotide "T" with "U".

              (default=off)

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

              The  default mode of RNAsubopt 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, RNAsubopt 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=STRING
              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. Note: Setting  this
              parameter implies --auto-id.

       --id-delim=CHAR
              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 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=CHAR
              Change the delimiting character used in 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.sub".  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).

   Algorithms:
              Select the algorithms which should be applied to the given RNA sequence(s).

       -e, --deltaEnergy=range
              Compute suboptimal structures with energy in a certain range of the optimum (kcal/mol).

              Default is calculation of mfe structure only.

       --deltaEnergyPost=range
              Only print structures with energy within range of the mfe after post reevaluation of energies.

              Useful in conjunction with -logML, -d1 or -d3: while the -e  option  specifies  the  range  before
              energies are re-evaluated, this option specifies the maximum energy after re-evaluation.

       -s, --sorted
              Sort the suboptimal structures by energy and lexicographical order.

              (default=off)

              Structures  are  first  sorted  by  energy  in  ascending order. Within groups of the same energy,
              structures are then sorted in ascending in lexicographical order of  their  dot-bracket  notation.
              See  the  --en-only flag to deactivate this second step. Note that sorting is done in memory, thus
              it can easily lead to exhaution of RAM! This is  especially  true  if  the  number  of  structures
              produced  becomes  large  or the RNA sequence is rather long. In such cases better use an external
              sort method, such as UNIX "sort".

       --en-only
              Only sort structures by free energy.  (default=off)

              In combination with --sorted,  this  flag  deactivates  the  second  sorting  criteria  and  sorts
              structures  solely  by their free energy instead of additionally sorting by lexicographic order in
              each energy band. This might save some  time  during  the  sorting  process  in  situations  where
              lexicographic order is not required.

       -p, --stochBT=number
              Randomly draw structures according to their probability in the Boltzmann ensemble.

              Instead  of  producing  all  suboptimals in an energy range, produce a random sample of suboptimal
              structures, drawn with probabilities equal to their Boltzmann weights via stochastic  backtracking
              in the partition function. The -e and -p options are mutually exclusive.

       --stochBT_en=number
              Same as "--stochBT" but also print free energies and probabilities of the backtraced structures.

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

              The  argument  provided  with  this  option  is used to scale the thermodynamic temperature in the
              Boltzmann factors independently from the temperature of the individual loop energy  contributions.
              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.

       -N, --nonRedundant
              Enable non-redundant sampling strategy.

              (default=off)

       -S, --pfScale=DOUBLE
              In the calculation of the pf use scale*mfe as an estimate for the ensemble free  energy  (used  to
              avoid overflows).

              (default=`1.07')

              The default is 1.07, useful values are 1.0 to 1.2. Occasionally needed for long sequences.

       -c, --circ
              Assume a circular (instead of linear) RNA molecule.

              (default=off)

       -D, --dos
              Compute density of states instead of secondary structures.

              (default=off)

              This  option  enables the evaluation of the number of secondary structures in certain energy bands
              around the MFE.

       -z, --zuker
              Compute Zuker suboptimals instead of all suboptimal structures within an energy  band  around  the
              MFE.

              (default=off)

       -g, --gquad
              Incoorporate G-Quadruplex formation.  (default=off)

              No  support  of  G-quadruplex  prediction  for stochastic backtracking and Zuker-style suboptimals
              yet).

   Structure Constraints:
              Command line options to interact with the structure constraints feature of this program

       --maxBPspan=INT
              Set the maximum base pair span.

              (default=`-1')

       -C, --constraint[=filename]
              Calculate structures subject to constraints.  (default=`')

              The program reads first the sequence, then  a  string  containing  constraints  on  the  structure
              encoded with the symbols:

              '.' (no constraint for this base)

              '|' (the corresponding base has to be paired

              'x' (the base is unpaired)

              '<' (base i is paired with a base j>i)

              '>' (base i is paired with a base j<i)

              and matching brackets '(' ')' (base i pairs base j)

              With  the  exception  of '|', constraints will disallow all pairs conflicting with the constraint.
              This is usually sufficient to enforce the constraint, but occasionally a base may stay unpaired in
              spite of constraints. PF folding ignores constraints of type '|'.

       --batch
              Use constraints for multiple sequences.  (default=off)

              Usually, constraints provided from input file only apply to a single  input  sequence.  Therefore,
              RNAsubopt  will  stop its computation and quit after the first input sequence was processed. Using
              this  switch,  RNAsubopt  processes  multiple  input  sequences  and  applies  the  same  provided
              constraints to each of them.

       --canonicalBPonly
              Remove non-canonical base pairs from the structure constraint.

              (default=off)

       --enforceConstraint
              Enforce base pairs given by round brackets '(' ')' in structure constraint.

              (default=off)

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

       --shapeMethod=method
              Select SHAPE reactivity data incorporation strategy.

              (default=`D')

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

              'D': Convert by using the linear equation according to Deigan et al 2009.

              Derived  pseudo energy terms 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=method
              Select method for SHAPE reactivity conversion.

              (default=`O')

              This  parameter  is  useful when dealing with the SHAPE incorporation according to Zarringhalam et
              al. 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.

   Energy Parameters:
              Energy parameter sets can be adapted or loaded from user-provided input files

       -T, --temp=DOUBLE
              Rescale energy parameters to a temperature of temp C. Default is 37C.

              (default=`37.0')

       -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. The placeholder file name 'DNA' can  be  used
              to load DNA parameters without the need to actually specify any input file.

       -4, --noTetra
              Do not include special tabulated stabilizing energies for tri-, tetra- and hexaloop hairpins.

              (default=off)

              Mostly for testing.

       --salt=DOUBLE
              Set salt concentration in molar (M). Default is 1.021M.

       -m, --modifications[=STRING]
              Allow for modified bases within the RNA sequence string.

              (default=`7I6P9D')

              Treat  modified  bases  within  the  RNA  sequence  differently,  i.e.  use  corresponding  energy
              corrections and/or pairing partner rules if available.  For that, the modified bases in the  input
              sequence  must  be  marked  by their corresponding one-letter code. If no additional arguments are
              supplied, all available corrections are performed. Otherwise, the user may limit the modifications
              to a particular subset of modifications, resp. one-letter codes, e.g. -mP6 will only  correct  for
              pseudouridine and m6A bases.

              Currently supported one-letter codes and energy corrections are:

              '7': 7-deaza-adenonsine (7DA)

              'I': Inosine

              '6': N6-methyladenosine (m6A)

              'P': Pseudouridine

              '9': Purine (a.k.a. nebularine)

              'D': Dihydrouridine

       --mod-file=STRING
              Use additional modified base data from JSON file.

   Model Details:
              Tweak the energy model and pairing rules additionally using the following parameters

       -d, --dangles=INT
              How to treat "dangling end" energies for bases adjacent to helices in free ends and multi-loops.

              (default=`2')

              With  -d1 only unpaired bases can participate in at most one dangling end.  With -d2 this check is
              ignored, dangling energies will be added for the bases adjacent to a helix on both  sides  in  any
              case;  this  is  the  default for mfe and partition function folding (-p).  The option -d0 ignores
              dangling ends altogether (mostly for debugging).  With -d3 mfe folding will allow coaxial stacking
              of adjacent helices in multi-loops. At the  moment  the  implementation  will  not  allow  coaxial
              stacking of the two interior pairs in a loop of degree 3 and works only for mfe folding.

              Note  that  with  -d1 and -d3 only the MFE computations will be using this setting while partition
              function uses -d2 setting, i.e. dangling ends will be treated differently.

       --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)

       --logML
              Recompute energies of structures using  a  logarithmic  energy  function  for  multi-loops  before
              output.  (default=off)

              This  option  does  not effect structure generation, only the energies that are printed out. Since
              logML lowers energies somewhat, some structures may be missing.

       --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. --nsp="-GA"  will allow GA and AG
              pairs. Nonstandard pairs are given 0 stacking energy.

       --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.

       --helical-rise=FLOAT
              Set the helical rise of the helix in units of Angstrom.

              (default=`2.8')

              Use with caution! This value will be re-set automatically to 3.4 in case DNA parameters are loaded
              via -P DNA and no further value is provided.

       --backbone-length=FLOAT
              Set the average backbone length for looped regions in units of Angstrom.

              (default=`6.0')

              Use  with  caution!  This  value  will  be re-set automatically to 6.76 in case DNA parameters are
              loaded via -P DNA and no further value is provided.

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. Wuchty, W. Fontana, I. L. Hofacker and P. Schuster (1999), "Complete Suboptimal Folding of RNA and the
       Stability of Secondary Structures", Biopolymers: 49, pp 145-165

       M. Zuker (1989), "On Finding All Suboptimal Foldings of an RNA Molecule", Science 244.4900, pp 48-52

       Y.  Ding,  and  C.E.  Lawrence  (2003),  "A  statistical  sampling  algorithm for RNA secondary structure
       prediction", Nucleic Acids Research 31.24, pp 7280-7301

       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

       Ivo L Hofacker, Stefan Wuchty, Walter Fontana, 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.

RNAsubopt 2.6.4                                   January 2025                                      RNASUBOPT(1)