Test Phase of OWL-Net : Global Network of Robotic Telescopes (2017-2018)

Hong-Suh Yim, Korea Astronomy and Space Science Institute; Jang-Hyun Park, Korea Astronomy and Space Science Institute; Jung Hyun Jo, Korea Astronomy and Space Science Institute; Jin Choi, Korea Astronomy and Space Science Institute (KASI) / University of Science and Technology (UST); Dong-Goo Roh, Korea Astronomy and Space Science Institute; Myungjin Kim, Korea Astronomy and Space Science Institute; Sooyoung Kim, Korea Astronomy and Space Science Institute; Sungki Cho, Korea Astronomy and Space Science Institute; Eun-Jung Choi, Korea Astronomy and Space Science Institute; Young-Sik Park, Korea Astronomy and Space Science Institute; Hong-Kyu Moon, Korea Astronomy and Space Science Institute; Young-Jun Choi, Korea Astronomy and Space Science Institute; Jae-Mann Kyeong, Korea Astronomy and Space Science Institute; Jiwoong Yu, Korea Astronomy and Space Science Institute; Seong-Cheol Bang, Korea Astronomy and Space Science Institute; Wonyong Han, Korea Astronomy and Space Science Institute;

Keywords: optical telescope, robotic observatory, automatic observation, space situational awareness

Abstract:

OWL, which was completed in 2016, has been in test operation for two years from 2017 to 2018. During that time, we focused on stabilizing the operation of five each OWL observatories through both software enhancements and hardware reinforcement work. As of the end of 2018, the average operating rate is more than 90%. In order to be more standard system, we have also performed calibration work through standards stars and satellites with known precise orbital elements. As a result, not only satellites but also near-Earth asteroids can be included in observations of OWL-Net. In this presentation, I would like to briefly show a series of works and their results during the test period.

Date of Conference: September 17-20, 2019

Track: Space Situational Awareness

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