Occultations by small non-spherical trans-neptunian objects. I. A new event simulator for TAOS II

The TAOS II Collaboration

研究成果: 雜誌貢獻期刊論文同行評審

5 引文 斯高帕斯(Scopus)

摘要

We present a new occultation event simulator for the Trans-Neptunian Automated Occultation Survey (TAOS II). We have developed a method to compute occultation shadows by small objects with non-circular apparent shapes (as may result from an intrinsic morphology or from the projection of a contact binary). The new simulator calculates diffraction features in the occultation shadows, as well as resulting light curves as would be measured by the TAOS?II survey system. We include effects such as the spectral type and finite angular size of the occulted star. We find that occultation events, especially by Trans-Neptunian Objects with diameters ~3 km may be misidentified or mischaracterized when not taking non-spherical shapes into account.

原文???core.languages.en_GB???
文章編號064401
期刊Publications of the Astronomical Society of the Pacific
131
發行號1000
DOIs
出版狀態已出版 - 6月 2019

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