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Title: Irregular dust features around intermediate-mass young stars with 
       GPI: signs of youth or misaligned disks? 
Authors: Laws A.S.E., Harries T.J., Setterholm B.R., Monnier J.D., Rich E.A., 
         Aarnio A.N., Adams F.C., Andrews S., Bae J., Calvet N., Espaillat C.,
         Hartmann L., Hinkley S., Isella A., Kraus S., Wilner D., Zhu Z. 
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Description of contents: Seven .fits files of the linearly-polarized intensity 
 (LPI) images shown in Figure 2.

 GPI_FUOri-J_LPI.fits	  => panel (a)
 GPI_mwc789-H_LPI.fits    => panel (b)
 GPI_hd139614-J_LPI.fits  => panel (c)
 GPI_hd139614-H_LPI.fits  => panel (d)
 GPI_hd45677-J_LPI.fits   => panel (e)
 GPI_hd45677-H_LPI.fits   => panel (f)
 GPI_Hen3-365-J_LPI.fits  => panel (g)

System requirements: Any FITS capable reader.

Additional comments: The physical scales are the same as in Figure 2.

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