Mercurial > repos > galaxyp > openms
comparison peak_picker_hi_res.xml @ 0:ba86fd127f5a draft
Uploaded
author | galaxyp |
---|---|
date | Wed, 19 Dec 2012 00:32:25 -0500 |
parents | |
children | cf0d72c7b482 |
comparison
equal
deleted
inserted
replaced
-1:000000000000 | 0:ba86fd127f5a |
---|---|
1 <tool id="openms_peak_picker_hi_res" version="0.1" name="Peak Peaker (Hi Res)"> | |
2 <description> | |
3 </description> | |
4 <requirements> | |
5 <requirement type="package">openms</requirement> | |
6 </requirements> | |
7 <command> | |
8 openms_wrapper.py --executable 'PeakPickerHiRes' --config $config | |
9 </command> | |
10 <configfiles> | |
11 <configfile name="config">[simple_options] | |
12 in=${input} | |
13 out=${out} | |
14 algorithm!signal_to_noise=${signal_to_noise} | |
15 algorithm!ms1_only=${ms1_only} | |
16 </configfile> | |
17 </configfiles> | |
18 <inputs> | |
19 <param format="mzML" name="input" type="data" label="Input profile peak list"/> | |
20 <param type="float" name="signal_to_noise" value="1" label="Signal-to-noise ratio" help="Minimal signal-to-noise ratio for a peak to be picked (0.0 disables SNT estimation!)" /> | |
21 <param type="boolean" name="ms1_only" label="MS1 Only" help="If checked, peak picking is only applied to MS1 scans. Other scans are copied to the output without changes." /> | |
22 </inputs> | |
23 <outputs> | |
24 <data format="mzML" name="out" /> | |
25 </outputs> | |
26 <help> | |
27 **What it does** | |
28 | |
29 This peak-picking algorithm detects ion signals in raw data and reconstructs the corresponding peak shape by cubic spline interpolation. Signal detection depends on the signal-to-noise ratio which is adjustable by the user (see parameter signal_to_noise). A picked peak's m/z and intensity value is given by the maximum of the underlying peak spline. Please notice that this method is still experimental since it has not been tested thoroughly yet. | |
30 | |
31 The algorithm used by this tool is best suited for high-resolution MS data (FT-ICR-MS, Orbitrap). In high-resolution data, the signals of ions with similar mass-to-charge ratios (m/z) exhibit little or no overlapping and therefore allow for a clear separation. Furthermore, ion signals tend to show well-defined peak shapes with narrow peak width. These properties faciliate a fast computation of picked peaks so that even large data sets can be processed very quickly. | |
32 | |
33 **Citation** | |
34 | |
35 For the underlying tool, please cite ``Marc Sturm, Andreas Bertsch, Clemens Gröpl, Andreas Hildebrandt, Rene Hussong, Eva Lange, Nico Pfeifer, Ole Schulz-Trieglaff, Alexandra Zerck, Knut Reinert, and Oliver Kohlbacher, 2008. OpenMS – an Open-Source Software Framework for Mass Spectrometry. BMC Bioinformatics 9: 163. doi:10.1186/1471-2105-9-163.`` | |
36 | |
37 If you use this tool in Galaxy, please cite Chilton J, et al. https://bitbucket.org/galaxyp/galaxyp-toolshed-openms | |
38 </help> | |
39 </tool> |