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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: One .fits files of the radial Stokes Q_phi_ image
 shown in Figure 9.

 GPI_hd139614-J_Qphi-r2.fits	=> panel (a)

System requirements: Any FITS capable reader.

Additional comments: Spiral arms in HD 139614 (Q_phi_, J-band, normalized 
 by distance from the image center r by multiplying by r^2^). These data were 
 taken without the use of a coronagraph, resulting in saturation in the image 
 center. The saturated area appears as a stripe centered at (0.0,0.0'') of 
 position angle ~30 degrees and extent ~0.3''. 

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