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Lightcurves of an occultation of a background star by Pluto observed on 15 Aug. 2018 at OAN, SPM in Baja California, México. The lightcurves were collected at a cadence of 20 Hz using two of the TAOS II telescopes, one with a commercial Andor Zyla CMOS camera (grey) and one with the TAOS II prototype CIS107 CMOS camera (blue). The spikes in the middle of occultation event, which are consistent in both light curves, are scintillation events stemming from density waves in the atmosphere of Pluto.
Pluto Occultation 2018
Lightcurves of an occultation of a background star by Pluto observed on 15 Aug. 2018 at OAN, SPM in Baja California, México. The lightcurves were collected at a cadence of 20 Hz using two of the TAOS II telescopes, one with a commercial Andor Zyla CMOS camera (grey) and one with the TAOS II prototype CIS107 CMOS camera (blue). The spikes in the middle of occultation event, which are consistent in both light curves, are scintillation events stemming from density waves in the atmosphere of Pluto.
Pluto Occultation 2018
Huang, Chung-Kai
Support Scientist
photo of Huang, Chung-Kai
Office: ASMAB 1025
TEL: +886-2-2366-5405
FAX: +886-2-2367-7849
Email: kevinhuang_replace2@_asiaa.sinica.edu.tw

Research Interests

Solar System, Trans-Neptunian Objects, Stellar Occultations, Astronomy Data Modeling, Time Domain Astronomy, Light Curves

Publications

My Publications from ADS

Journal Papers affiliated with ASIAA

  1. Huang C-K; Lehner MJ; Granados Contreras AP; Castro-Chacón JH; Chen W-P; Alcock C; Alvarez-Santana FI; Cook KH; Geary JC; Guerrero Peña CA; Hernández-Ñguila JB; Hernández-Valencia B; Karr J; Kavelaars JJ; Norton T; Nuñez JM; Ochoa D; Reyes-Ruiz M; Sánchez E; Silva JS; Szentgyorgyi A; Wang S-Y; Yen W-L; Zhang Z-W, "The TAOS II Survey: Real-time Detection and Characterization of Occultation Events" , PASP: 133(1021), id.34503 (17pp), Mar, 2021 [SCI] ( ADS | Fulltext )
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