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RNAMULTIFOLD(1) |
User Commands |
RNAMULTIFOLD(1) |
RNAmultifold - manual page for RNAmultifold 2.5.0
RNAmultifold [OPTION]... [FILE]...
RNAmultifold 2.5.0
Compute secondary structures of multiple interacting RNAs
The program works much like RNAfold, but allows one to specify
multiple RNA sequences which are then allowed to form conncected components.
RNA sequences are read from stdin in the usual format, i.e. each line of
input corresponds to one sequence, except for lines starting with
">" which contain the name of the next sequence(s). Multiple
strands must be concatenated using the \'&\' character as separator.
RNAmultifold can compute MFE, partition function, corresponding ensemble
free energy and base pairing probabilities. These properties are either
computed for a particular arrangement (concatenation) of sequences, for the
full ensemble of the complex of input RNAs, or all complexes formed by the
input sequences up to a specified number of interacting sequences. Output
consists of a PostScript "dot plot" file containing the pair
probabilities, see the RNAfold man page for details. The program will
continue to read new sequences until a line consisting of the single
character @ or an end of file condition is encountered.
- -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
- Command line options which alter the general behavior of this program
- -v, --verbose
- Be verbose.
- (default=off)
- -j, --jobs[=number]
- Split batch input into jobs and start processing in parallel using
multiple threads. A value of 0 indicates to use as many parallel threads
as computation cores are available.
- (default=`0')
- Default processing of input data is performed in a serial fashion, i.e.
one sequence pair at a time. Using this switch, a user can instead start
the computation for many sequence pairs in the input in parallel.
RNAmultifold will create as many parallel computation slots as specified
and assigns input sequences of the input file(s) to the available slots.
Note, that this increases memory consumption since input alignments have
to be kept in memory until an empty compute slot is available and each
running job requires its own dynamic programming matrices.
- --unordered
- Do not try to keep output in order with input while parallel processing is
in place.
- (default=off)
- When parallel input processing (--jobs flag) is enabled, the order
in which input is processed depends on the host machines job scheduler.
Therefore, any output to stdout or files generated by this program will
most likely not follow the order of the corresponding input data set. The
default of RNAmultifold is to use a specialized data structure to still
keep the results output in order with the input data. However, this comes
with a trade-off in terms of memory consumption, since all output must be
kept in memory for as long as no chunks of consecutive, ordered output are
available. By setting this flag, RNAmultifold will not buffer individual
results but print them as soon as they have been computated.
- --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 RNAmultifold 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, RNAmultifold 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 sequence will be prefixed with the provided
string. Hence, the output files will obey the following naming scheme:
"prefix_xxxx_ss.ps" (secondary structure plot),
"prefix_xxxx_dp.ps" (dot-plot), "prefix_xxxx_dp2.ps"
(stack probabilities), etc. where xxxx is the sequence number. Note:
Setting this parameter implies --auto-id.
- --id-delim=delimiter
- 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=delimiter
- 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_ss.ps" for secondary structure plots. With
this flag set, no truncation of the output filenames is done, 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).
- Command line options to interact with the structure constraints feature of
this program
- --maxBPspan=INT
- Set the maximum base pair span
- (default=`-1')
- --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.
- Select additional algorithms which should be included in the calculations.
The Minimum free energy (MFE) and a structure representative are
calculated in any case.
- -p, --partfunc[=INT]
- Calculate the partition function and base pairing probability matrix in
addition to the MFE structure. Default is calculation of mfe structure
only.
- (default=`1')
- In addition to the MFE structure we print a coarse representation of the
pair probabilities in form of a pseudo bracket notation, followed by the
ensemble free energy. Note that unless you also specify -d2 or
-d0, the partition function and mfe calculations will use a
slightly different energy model. See the discussion of dangling end
options below.
- An additionally passed value to this option changes the behavior of
partition function calculation:
- In order to calculate the partition function but not the pair
probabilities
- use the -p0 option and save about
- 50% in runtime. This prints the ensemble free energy -kT
ln(Z).
- -a, --all_pf[=INT]
- Compute the partition function and free energies not only for the complex
formed by the input sequences (the "ABC... mutimer"), but also
of all complexes formed by the input sequences up to the number of input
sequences, e.g. AAA, AAB, ABB, BBB, etc.
- (default=`1')
- The output will contain the free energies for each of these species. Using
-a automatically switches on the -p option.
- -c, --concentrations
- In addition to everything listed under the -a option, read in
initial monomer concentrations and compute the expected equilibrium
concentrations of all possible species (A, B, AA, BB, AB, etc).
- (default=off)
- Start concentrations are read from stdin (unless the -f option is
used) in [mol/l], equilibrium concentrations are given realtive to the sum
of the inputs. An arbitrary number of initial concentrations can be
specified (one tuple of concentrations per line).
- -f, --concfile=filename
- Specify a file with initial concentrations for the input sequences.
- The table consits of arbitrary many lines with multiple numbers separated
by whitespace (the concentration of the input sequences A, B, C, etc.).
This option will automatically toggle the -c (and thus -a
and -p) options (see above).
- --absolute-concentrations Report absolute instead of relative
- concentrations
- (default=off)
- -S, --pfScale=scaling factor
- In the calculation of the pf use scale*mfe 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
long sequences. You can also recompile the program to use double precision
(see the README file).
- --bppmThreshold=<value>
- Set the threshold for base pair probabilities included in the postscript
output
- (default=`1e-5')
- By setting the threshold the base pair probabilities that are included in
the output can be varied. By default only those exceeding 1e-5 in
probability will be shown as squares in the dot plot. Changing the
threshold to any other value allows for increase or decrease of data.
- -g, --gquad
- Incoorporate G-Quadruplex formation into the structure prediction
algorithm.
- (default=off)
- Note, only intramolecular G-quadruplexes are considered.
- -T, --temp=DOUBLE
- Rescale energy parameters to a temperature of temp C. Default is 37C.
- -4, --noTetra
- Do not include special tabulated stabilizing energies for tri-, tetra- and
hexaloop hairpins.
- (default=off)
- Mostly for testing.
- -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)
- -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.
- --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. RNAmultifold -nsp -GA will allow GA
and AG pairs. Nonstandard pairs are given 0 stacking energy.
- -e, --energyModel=INT
- 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.
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
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
If in doubt our program is right, nature is at fault. Comments should be sent to
rna@tbi.univie.ac.at.
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