Physical properties of the trans-neptunian object (38628) huya from a multi-chord stellar occultation

HIGHLIGHTS

• who: Santos-Sanz P. et al. from the in Ukraine and u00c7ukurova University Observatory in Turkey) are listed in Table, . Basic information about the , telescopes that participated in this campaign and their locations is shown in the online Table A.2. Aperture photometry for each data set was obtained, from which we derived the light curves (flux of the star normalized to the mean value before the occultation versus the time). The light curves from the , positive observations at , sites (see Table A.1) showed drops in flux caused by the occultation. Light curves from the other . . .
  

   

  

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