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Title: Unveiling the Role of the Magnetic Field at 
       the Smallest Scales of Star Formation 
Authors: Hull C.L.H., Mocz P., Burkhart B., Goodman A.A., Girart J.M., 
         Cortes P.C., Hernquist L., Springel V., Li Z.-Y., Lai S.-P. 
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Description of contents: 

  Variables:

  Pc = polarized intensity (debiased)
  sigma_pol = the rms noise in the Stokes Q and U maps

  Files:
  
  FITS: Serpens_Emb8_cont_image_I.pbcor.fits
                -Cleaned map of total intensity (Stokes I) dust emission
  
  FITS: Serpens_Emb8_cont_image_Q.pbcor.fits
                -Cleaned map of Stokes Q dust emission
        
  FITS: Serpens_Emb8_cont_image_U.pbcor.fits
                -Cleaned map of Stokes U dust emission
  
  FITS: Serpens_Emb8_cont_image.pa.fits
        -Map of the position angle of the true dust polarization 
         (not the magnetic field)
                -Results are masked where Pc < 3*sigma_pol

  FITS: Serpens_Emb8_cont_image.pol.fits
                -Map of total debiased polarized dust emission
                -Results are masked where Pc < 3*sigma_pol

System requirements: A FITS reader is required to read the FITS files; 
  no other special programs are required.  

Additional comments:
  
  Note that the raw ALMA data are not included here, but will available in 
  from the ALMA archive once the proprietary period has ended.  
  Reduced/calibrated data are also available from the lead author (C. Hull).  
  All raw data are in CASA format, and thus require an installation of CASA.
  
  The URL of the ALMA data archive is:
  https://almascience.nrao.edu/alma-data/archive
  
  To access the data used in this paper, one must query for the project code
  2013.1.00726.S.

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