Input data
QSMxT reads BIDS datasets. If you convert your
DICOMs with qsmxt dicom-convert
the layout is handled for you, and this page is mostly reference. If you are
assembling a dataset by hand, or wondering why an output did not appear, start
here.
Checking a dataset
Section titled “Checking a dataset”qsmxt validate study/bidsThis reports every run it discovers, the echo times and field strength it read, and which outputs your data can support. Run it before a long job:
sub-01_acq-gre_MEGRE Echoes: 4 Echo times: [0.004, 0.012, 0.02, 0.028] s Field strength: 3.0 T Magnitude: present MESE (spin-echo): not found Capabilities: QSM reconstruction: yes R2*/T2* mapping: yes SWI: yesExpected layout
Section titled “Expected layout”The pipeline discovers a run from its phase images:
sub-*/[ses-*/]anat/*_part-phase_*.nii[.gz]with matching JSON sidecars containing EchoTime and MagneticFieldStrength.
Multi-echo data uses the BIDS echo-<N> entity. Magnitude images sit alongside
as *_part-mag_*, and are optional for a basic QSM run but required by most
other outputs.
Two further acquisitions are recognised when present:
| Pattern | Provides |
|---|---|
sub-*/[ses-*/]anat/*_part-mag_*.nii[.gz] |
magnitude, for R2*/T2*, SWI and masking |
sub-*/[ses-*/]anat/*_echo-*_MESE.nii[.gz] |
multi-echo spin-echo, for R2 and hence R2’ |
A MESE acquisition needs at least three echoes to fit R2. Fewer are ignored.
What each output needs
Section titled “What each output needs”Phase is what a run is discovered from, so it is present for everything below. This table lists what each output needs in addition to it.
| Output | Also requires |
|---|---|
| QSM | nothing, though magnitude is recommended and some masking options need it |
SWI (--do-swi) |
magnitude |
R2*/T2* (--do-r2starmap, --do-t2starmap) |
magnitude, at least 3 echoes |
R2 (--do-r2map) |
a MESE acquisition, at least 3 echoes |
R2’ (--do-r2primemap) |
magnitude and a MESE acquisition, for R2* and R2 |
Source separation
(--do-chisep) splits into two groups. The r2star-qsm and decompose methods
work from multi-echo GRE magnitude alone. The other six are based on R2’, so they
need a MESE acquisition as well.
Bringing your own inputs
Section titled “Bringing your own inputs”QSMxT will use maps produced by other tools from <bids>/derivatives/<TOOL>/,
following the same sub-*/[ses-*/]anat/ layout:
| Option | Supplies | Filename |
|---|---|---|
--use-custom-masks [TOOL] |
brain mask | *_mask.nii* |
--use-custom-qsm <TOOL> |
susceptibility map | *_Chimap.nii* |
--use-custom-r2 <TOOL> |
R2 map | *_R2map.nii* |
--use-custom-r2prime <TOOL> |
R2’ map | *_R2primemap.nii* |
Supplying R2’ directly removes the MESE requirement for source separation, since
R2 is only needed to compute it. qsmxt validate lists the derivative tools it
can see for each run.