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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 total intensity images 
 shown in Figure 2.

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

System requirements: Any FITS capable reader.

Additional comments: The brightest region near 
 the coronagraphic spot is the stellar PSF and can appear elongated due to 
 strong wind shaking the telescope during the observations. The bright spots 
 in the four corners of each image are satellite spots. These appear at radii 
 of 1.0'' in H-band, and secondary satellite spots appear at 1.0'' in J-b
 and and 1.5'' in H-band. Companion candidates are visible around FU Ori, 
 MWC 789, and Hen 3-365, with their locations given in Table 6. Other faint 
 visible features include the arm to the north-west of MWC 789, the arm to 
 the immediate east of the spot in FU Ori, and the arm to the north west of 
 the spot in Hen 3-365. 

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