We have examined most of the astrophysical properties of the two star clusters, FSR-163 and Majaess 215, using the third data release of the Gaia space mission(Gaia DR3). We utilized the py UPMASK method to allocate t...
We presented the first photometric analysis of the V1961 Cyg and V0890 Lyr binary systems.We observed and analyzed these systems at an observatory in France as part of the Binary Systems of South and North (BSN)Projec...
supported by the Beijing Natural Science Foundation(No.L221003).
The construction of high-precision urban rail maps is crucial for the safe and efficient operation of railway transportation systems.However,the repetitive features and sparse textures in urban rail environments pose ...
The early time observations of Type Ia supernovae(SNe Ia)play a crucial role in investigating and resolving longstanding questions about progenitor stars and the explosion mechanisms of these events.Colors of supernov...
supported by the National Key R&D Program of China(Grant Nos.2022YFF0503400 and 2022YFF0503401);China Manned Space Program(Grant Nos.CMS-CSST-2021-B01,CMS-CSST-2021-B04,and CMS-CSST2021-A12);Science Program of Beijing Academy of Science and Technology(Grant No.24CD014);National Natural Science Foundation of China(Grant Nos.12288102 and 12033003);Tencent Xplorer Prize。
The China Space Station Telescope(CSST,also known as Xuntian)is a serviceable two-meter-aperture wide-field telescope operating in the same orbit as the China Space Station.The CSST plans to survey a sky area of 17,50...
The ATLAS project is primarily funded to search for near-earth asteroids through NASA grants NN12AR55G,80NSSC18K0284,and 80NSSC18K1575;funded by Kepler/K2 grant J1944/80NSSC19K0112 and HST GO-15889,and STFC grants ST/T000198/1 and ST/S006109/1。
This work analyzes the photometric data of the Oort spike comets C/2019 L3(ATLAS)and C/2019 O3(Palomar)obtained between 2016 and 2023 by the ATLAS network and the Belgian Olmen Observatory.The comets Palomar and ATLAS...
supported by the National Natural Science Foundation of China(grant No.12173062)。
The image quality of a large field survey telescope with a fast focal ratio of the primary mirror is high sensitivity to the optical elements’misalignments and the primary mirror’s deformations.To maintain good opti...
supported by the Natural Science Foundation of Xinjiang Uygur Autonomous Region of China(grant No.2021D01B112);Tianshan Talent Training Program through the grant 2023TSYCCX0101。
In this work,we report observations of three comets:38P/Stephan-Oterma,64P/Swift-Gehrels,and C/2017 M4(ATLAS),conducted with the Nanshan one-meter wide-field telescope in 2018 August and November,and 2019January.We ex...
Funding for the TESS mission is provided by the NASA Explorer Program;support of the National Natural Science Foundation of China(NSFC,grant Nos.U2031204,12373038,12163005,and 12288102);the science research grants from the China Manned Space Project with No.CMSCSST-2021-A10;the Natural Science Foundation of Xinjiang Nos.2022D01D85 and 2022TSYCLJ0006。
We analyze the frequencies of three known roAp stars,TIC 96315731,TIC 72392575,and TIC 318007796,using the light curves from the Transiting Exoplanet Survey Satellite.For TIC 96315731,the rotational and pulsational fr...
support from the SRF INSPIRE(IF 170314)fellowship program,Government of India;financial support from the SERB Core Research Grant project,the Government of India。
Contact binaries at various stages of evolution unveil various operating mechanisms that drive them.We report the photometric and period variation analysis of two contact binaries EV Cnc and AH Cnc in open cluster M67...