• DOI:10.1088/0004-6256/148/5/100
• Corpus ID: 119254807

First Lunar Occultation Results from the 2.4 m Thai National Telescope equipped with ULTRASPEC

@article{Richichi2014FirstLO,
  title={First Lunar Occultation Results from the 2.4 m Thai National Telescope equipped with ULTRASPEC},
  author={A Richichi and P. Irawati and Boonrucksar Soonthornthum and Vik S. Dhillon and Thomas R. Marsh},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2014}
}

• A. Richichi, P. Irawati, +2 authors T. Marsh
• Published 1 August 2014
• Physics
• arXiv: Solar and Stellar Astrophysics

The recently inaugurated 2.4\,m Thai National Telescope (TNT) is equipped, among other instruments, with the ULTRASPEC low-noise, frame-transfer EMCCD camera. At the end of its first official observing season, we report on the use of this facility to record high time resolution imaging using small detector subarrays with sampling as fast as several $10^2$\,Hz. In particular, we have recorded lunar occultations of several stars which represent the first contribution to this area of research made from South-East Asia with a telescope of this class. Among the results, we discuss an accurate measurement of $\alpha $~Cnc, which has been reported previously as a suspected close binary. Attempts to resolve this star by several authors have so far met with a lack of unambiguous confirmation. With our observation we are able to place stringent limits on the projected angular separation ($ 5$) of a putative companion. We also present a measurement of the binary {HR~7072}, which extends considerably the time coverage available for its yet undetermined orbit. We discuss our precise determination of the flux ratio and projected separation in the context of other available data. We conclude by providing an estimate of the performance of ULTRASPEC at TNT for lunar occultation work. This facility can help to extend the lunar occultation technique in a geographical area where no comparable resources were available until now.