COMPARATIVE ANALYSIS OF OBSERVATIONS OF THE SELECTED EXOPLANET TRANSITS OBTAINED AT THE KYIV COMET STATION WITH THE DATABASE OF THE ORBITAL TELESCOPES TESS AND KEPLER

M. Lobodenko, Y. Pavlenko, I. Kulyk, A. Nahurna, M. Solomakha, O. Baransky
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Abstract

We present a comparative analysis of observations of the selected exoplanet transits obtained at the Kyiv Comet station with the database of the TESS (Transiting Exoplanet Survey Satellite) and Kepler space telescopes. The light curves obtained by the TESS and Kepler orbital telescopes were processed using a program based on the Python package Lightcurve 2.3v which is freely available in the MUST archive (Barbara A. Mikulski Archive for Space Telescopes). The ground based observations were carried out with the 70-cm telescope AZT- 8 (Lisnyky). Photometric processing of the ground based observation was performed by using the Muniwin program. The light curves and parameters of the observed transits as well as the exoplanet orbital parameters obtained from ground based observations were published in the ETD (Exoplanet Transit Database). Determined transit parameters were compared with the results of the TESS command, which are stored in the MUST archive. Here we presents a comparison of the parameters of transit phenomena (period, depth, transit duration) and some orbital parameters obtained from two independent sets of observations, terrestrial and orbital, performed in different epochs.
基辅彗星站获得的选定系外行星凌日观测数据与Tess和Kepler轨道望远镜数据库的对比分析
我们对基辅彗星站获得的选定系外行星凌日观测结果与TESS(凌日系外行星调查卫星)和开普勒太空望远镜的数据库进行了比较分析。TESS和开普勒轨道望远镜获得的光曲线是使用基于Python包Lightcurve 2.3v的程序处理的,该程序可在MUST档案(Barbara a.Mikulski太空望远镜档案)中免费获得。地面观测是用70厘米的AZT-8(利斯尼基)望远镜进行的。地面观测的光度处理是使用穆尼温程序进行的。观测到的凌日的光曲线和参数以及从地面观测中获得的系外行星轨道参数发表在ETD(外行星凌日数据库)中。将确定的运输参数与TESS命令的结果进行比较,TESS命令存储在MUST档案中。在这里,我们对凌日现象的参数(周期、深度、凌日持续时间)和从不同时期进行的两组独立的陆地和轨道观测中获得的一些轨道参数进行了比较。
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