Supported in part by the the National Natural Science Foundation of China(12105191,12275183,12275184,11875196)。
This study investigates the observational signatures of traversable Simpson-Visser wormholes illuminated by luminous celestial spheres and orbiting hot spots.We demonstrate that when light sources and observers are on...
supported by the National Key R&D Program of China(grant No.2022YFE0116800);the National Natural Science Foundation of China(NSFC,grant No.12203019);the Natural Science Foundation of Jiangxi Province(grant No.20242BAB20033);the NSFC(grant Nos.11873026 and11273014);the China Manned Space Project(grant No.CMS-CSST-2021-B08);the Joint Research Fund in Astronomy(grant No.U1431227)。
Geometric distortion(GD)critically constrains the precision of astrometry.Using well-established methods to correct GD requires calibration observations,which can only be obtained using a special dithering strategy du...
supported by the National Key Research and Development Program of China(2021YFA0715101);the National Natural Science Foundation of China(NSFC,grant Nos.12033009 and 12103087);the Strategic Priority Research Program of the Chinese Academy of Sciences(XDA0350300);the International Partnership Program of Chinese Academy of Sciences(020GJHZ2022034FN);the Yunnan Fundamental Research Projects(202201AU070225,202301AT070328,202401AT070141);the Young Talent Project of Yunnan Revitalization Talent Support Program。
High-precision ephemerides not only support space missions,but can also be used to study the origin and future of celestial bodies.In this paper,a coupled orbit-rotation dynamics model that fully takes into account th...
supported by the National Natural Science Foundation of China(No.12373073,U2031104,No.12173015);Guangdong Basic and Applied Basic Research Foundation(No.2023A1515011340)。
Obtaining high precision is an important consideration for astrometric studies using images from the Narrow Angle Camera(NAC)of the Cassini Imaging Science Subsystem(ISS).Selecting the best centering algorithm is key ...
supported by the National Natural Science Foundation of China (Nos. 61873196 and 62373030);the Innovation Program for Quantum Science and Technology(No. 2021ZD0303400)。
In the two-dimensional positioning method of pulsars, the grid method is used to provide non-sensitive direction and positional estimates. However, the grid method has a high computational load and low accuracy due to...
supported by the National Natural Science Foundation of China(NSFC)under grant No.42304044;the Natural Science Foundation of Henan,China under grant No.222300420385。
High-precision polar motion prediction is of great significance for deep space exploration and satellite navigation.Polar motion is affected by a variety of excitation factors,and nonlinear prediction methods are more...
generously supported by the National Natural Science Foundation of China(NSFC,Grant Nos.12073047 and 12273077);the National Key Research and Development(Grant No.2022YFF0711500)。
In this study,we conducted simulations to find the geometric aberrations expected for images taken by the Main Survey Camera of the Chinese Space Station Telescope(CSST)due to its motion.As anticipated by previous wor...
funded by the science research grants from the China Manned Space Project with NO.CMS-CSST-2021-A11and NO.CMS-CSST-2021-B10;the National Natural Science Foundation of China(NSFC)under grant No.12373074。
The multi-color imaging sky survey conducted by the China Space Station Telescope(CSST)holds significant promise for advancing the development of the celestial reference frame.In this study,we focus on assessing the a...
funded by the National Natural Science Foundation of China(NSFC,Grant Nos.12203104 and 11933011);the Natural Science Foundation of Jiangsu Province(grants No.BK20210999);the National SKA Program of China(grant No.2022SKA0120103);the Entrepreneurship and Innovation Program of Jiangsu Province;the Key Laboratory for Radio Astronomy,CAS。
The next generation of very long baseline interferometry(VLBI)is stepping into the era of microarcsecond(μas)astronomy,and pushing astronomy,especially astrometry,to new heights.VLBI with the Square Kilometre Array(S...
funded by the National Key R&D Program of China(grant No.2022YFE0116800);the National Natural Science Foundation of China(NSFC,grant No.12173085);the West Light Foundation of The Chinese Academy of Sciences Key scientific research projects of colleges and universities in Henan Province(grant No.23B16001)。
This study details an astrometric observation campaign of the Near-Earth Asteroid 1998 HH49,conducted with the aim of refining our understanding of its physical characteristics.Utilizing the 50 cm telescope located at...