supported by National Natural Science Foundation of China(NSFC,Grant Nos.U1831209 and U2031144);the research fund of Ankara University(BAP)through the project 18A0759001。
We report the confirmation of a sub-Saturn-size exoplanet,TOI-1194 b,with a mass of about 0.456+0.055-0.051M_(J),and a very low mass companion star with a mass of about 96.5±1.5 MJ,TOI-1251 B.Exoplanet candidates pro...
financial support from the SERB Core Research Grant project,the Government of India;support from the SRF INSPIRE(IF 170314)fellowship program,Government of India。
Marginal short-period contact binaries are important to understand as they pose a different physical scenario than the predicted theoretical model based on the thermal relaxation oscillation mechanism due to their sha...
support from the National Natural Science Foundation of China(NSFC)(Nos.12005124 and 12147215);support from the Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi(STIP)(No.2020L0528);the Applied Basic Research Programs of Natural Science Foundation of Shanxi Province(No.202103021223320)。
In this work,the pulsation analysis is performed on 83 high-amplitudeδScuti stars(HADS),which have been observed by the Transiting Exoplanet Survey Satellite.The results show that 49 of these HADS show single-mode pu...
supported by Canakkale Onsekiz Mart University,The Scientific Research Coordination Unit,Project number:2022-FBA-3851。
We present the first detailed investigation of six eclipsing binary systems in the TESS field.The TESS light curves of the targets are analyzed by determining the initial effective temperatures via SED fits.The absolu...