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...
This work is supported by“the Fundamental Research Funds for the Central Universities”,111 project No.B20019;Shanghai Natural Science Foundation,grant No.19ZR1466800.
The Jiao Tong University Spectroscopic Telescope(JUST)is a 4.4-meter f/6.0 segmented-mirror telescope dedicated to spectroscopic observations.The JUST primary mirror is composed of 18 hexagonal segments,each with a di...
supported by the National Natural Science Foundation of China(Grant Nos.12002028 and 51827806);Beijing Institute of Technology Research Fund Program for Young Scholars.
In recent years,exoplanet detection has become the technological frontier in the field of astronomy,because it provides evidence of the origin of life and the future human habitable exoplanet.Deploying several satelli...
funded by the National Natural Science Foundation of China(NSFC,Grant No.11833004);funded by the Strategic Priority Research Program on Space Science,the Chinese Academy of Sciences,Grant No.XDA15020800。
For detecting exoplanets with high precision,using the angular distance between the two stars to detect the periodic motion of the star will be a better choice.This approach can avoid importing the position error of t...
The authors would like to appreciate the anonymous reviewers for giving valuable advice to help in improving the quality of the paper.This study was supported by the National Natural Science Foundation of China(Nos.11602297,11902027,and 62173334).
The dynamics and control of a tetrahedral spacecraft formation flying in the Sun-Earth L2 region is initiatively studied,based on the circular restricted three-body problem(CR3BP).Driven by the science goal of identif...
supported by the National Natural Science Foundation of China(Grant Nos.11827804,U2031210)。
The portable adaptive optics(PAO)device is a low-cost and compact system,designed for 4-meter class telescopes that have no adaptive optics(AO)system,because of the physical space limitation at the Nasmyth or Cassegra...
supported by grants from the Ministry of Science and Technology(MOST),Taiwan,China.The grant numbers are MOST 105-2119-M-007-029-MY3,MOST 1062112-M-007-006-MY3;the University Grants Commission(UGC);financial support through Major Research Project no.UGC-MRP 43-521/2014(SR);IUCCA,Pune,India for providing supports through the IUCCA Associateship Programme;financially supported by the National Natural Science Foundation of China(Grant Nos.11590782 and 11421303);supported by the B-type Strategic Priority Program of the Chinese Academy of Sciences(Grant No.XDB41000000);the National Natural Science Foundation of China(Grant No.11773081);CAS Interdisciplinary Innovation Team;Foundation of Minor Planets of the Purple Mountain Observatory。
Considering the importance of investigating the transit timing variations(TTVs)of transiting exoplanets,we present a follow-up study of HAT-P-12 b.We include six new light curves observed between2011 and 2015 from thr...
Supported by the B-type Strategic Priority Program of the Chinese Academy of Sciences(XDB41000000);the National Natural Science Foundation of China(11773081,11573073);CAS Interdisciplinary Innovation Team,Foundation of Minor Planets of the Purple Mountain Observatory and Youth Innovation Promotion Association。
Four future missions for deep space exploration and future space-based exoplanet surveys on habitable planets by 2030 are scheduled to be launched.Two Mars exploration missions are designed to investigate geological s...
sponsored by the National Natural Science Foundation of China (NSFC) (Grant Nos. 11527804, 10943002 and 11373023)
The diurnal polarization variation of the Earth, treated as an exoplanet with an unresolved disk but resolvable from its host star, is presented in three wavelength bands centered at 490 nm, 670 nm and865 nm respectiv...
Exoplanet transit timing variation is a method to find exoplanets. To understand this method better, I wrote a computer program in python to simulate the transit of exoplanets. I use my program to simulate the transit...