论文标题
候选TOI 717.01和确认的HAT-P-3B的系外行星的研究
Studies of Exoplanets with Candidate TOI 717.01 and Confirmed HAT-P-3b
论文作者
论文摘要
从Las Cumbres天文台0.4米望远镜的W-Filter中请求系外行星TOI 717.01，卡塔尔-8 B和HAT-P-3 B的图像。在这些请求中，拍摄了TOI 717.01和HAT-P-3B的图像，并使用外部外交解释代码（异国情调）软件减少了图像，以及来自太阳兄弟姐妹管道的6个光度计算法。 HAT-P-3 B的过境中点被发现为2458907.6205，与当晚预期的中点不同20.2分钟。对于TOI 717.01，不可分割的是由于其低运输深度为0.1％。 TOI 717.01场中的一个比较恒星之一可能是可变的。
Images of the exoplanets TOI 717.01, Qatar-8 b, and HAT-P-3 b were requested in the w-filter from the Las Cumbres Observatory 0.4-meter telescopes. Of these requests, images were taken of TOI 717.01 and HAT-P-3b and were reduced using the EXOplanet Transit Interpretation Code (EXOTIC) software, as well as 6 photometric algorithms from the Our Solar Siblings pipeline. The transit midpoint for HAT-P-3 b was found to be 2458907.6205, which is 20.2 minutes different from its expected midpoint that night. For TOI 717.01, the transit was not discernible, likely due to its low transit depth of 0.1%. It is possible that one of the comparison stars in the TOI 717.01 field is variable.
