Data supporting Liu et al. 2026

The files are the data supporting the article "The dominance of turbulence over magnetism in the formation of massive star cluster seeds". The Zip file RAMSES_output_example.tar.gz contains an example of the RAMSES output. Due to the upload limit, we are unable to upload all the RAMSES simulation results to the repository. The Zip file POLARIS_output.zip contains the synthetic Stokes I, Q, and U images from the POLARIS output. The CSV files contain the parameters of the condensations identified (by getsf and astrodendro) in the ALMA dust continuum maps. --------- region: source region. RA: in units of degrees. DEC: in units of degrees. major_FWHM: major FWHM of condensation in units of arcsec. minor_FWHM: minor FWHM of condensation in units of arcsec. PA_source: position angle of the condensation elongation orientation in units of degrees, following IAU convention. PA_B: position angle of condensation-averaged magnetic field orientation in units of degrees, following IAU convention. Ipeak_pbcor: peak intensity of condensation in units of Jy/beam. After primary beam correction. Fint_pbcor: integrated flux of condensation in units of Jy. After primary beam correction.