the support of the China National Key Program for Science and Technology Research and Development of China(2022YFA1602901,2023YFA1608204);the National Natural Science Foundation of China(Nos.11988101,11873051,12125302,12373011,12041305,12173016);the CAS Project for Young Scientists in Basic Research grant(No.YSBR-062)。
Accurate flux density calibration is essential for precise analysis and interpretation of observations across different observation modes and instruments.In this research,we first introduce the flux calibration model ...
supported by the National Key Research and Development Program of China(2023YFA1608100);the National Natural Science Foundation of China(NSFC,grant Nos.12090044,11833006 and 12303023);the science research grants from the China Manned Space Project including the CSST Milky Way and Nearby Galaxies Survey on Dust and Extinction Project CMS-CSST-2021-A09 and No.CMS-CSST-2021-A08.G.C.L;Hubei Provincial Natural Science Foundation with grant No.2023AFB577;the Key Laboratory Fund of Ministry of Education under grant No.QLPL2022P01;National Natural Science Foundation of China(NSFC,Grant No.U1731108)。
We present radial velocity(RV)curve templates of RR Lyrae first-overtone(RRc)stars constructed with the Mg I b triplet and Hαlines using time-domain Medium-Resolution Survey spectra of seven RRc stars from Large Sky ...
This work shows details of an evaluation of an observational system comprising a complementary metal-oxidesemiconductor detector, 60 cm telescope and filter complement. The system’s photometric precision and differen...
supported by the National Key R&D Program of China(grant No.2022YFA1602901);the Youth Innovation Promotion Association,Chinese Academy of Sciences(No.2020057);the science research grants from the China Manned Space Project,and the National Natural Science Foundation of China(NSFC,grant Nos.12090041 and 12090040);Additional support comes from the Strategic Priority Research Program of the Chinese Academy of Sciences(grant Nos.XDB0550100 and XDB0550102);the Open Project Program of the Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences。
From ∼5000 deg^(2) of the combination of the Beijing–Arizona Sky Survey and Mayall z-band Legacy Survey which is also the northern sky region of the Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Surveys...
supported by the Specialized Research Fund for State Key Laboratories under Grant 202217;the Key Laboratory of Solar Activity and Space Weather(NSSC)under Grant E26600021S。
Ground-based radio observations below 30 MHz are susceptible to the ionosphere of the Earth and the radio frequency interference.Compared with other space mission concepts,making low frequency observations using an in...
Funding for the research was provided by Cui Xiangqun’s Academician Studio;Funding for the project has been provided by the National Development and Reform Commission。
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST)has been in normal operation for more than 10 yr,and routine maintenance is performed on the fiber positioner every summer.The positioning accuracy ...
supported by the National Key R&D Program of China under grant No.2018YFA0404703;the Open Project Program of the Key Laboratory of FAST,NAOC,Chinese Academy of Sciences。
The Phased Array Feed(PAF)is considered as one of the next generation receivers for radio telescopes,which can significantly enlarge the instantaneous Field-of-View of large aperture single dish radio telescopes and e...
supported by the National Natural Science Foundation of China (Grant Nos. U1931209, 62272336);Projects of Science and Technology Cooperation and Exchange of Shanxi Province (Grant Nos. 202204041101037, 202204041101033);the central government guides local science and technology development funds (Grant No. 20201070);The Fundamental Research Program of Shanxi Province (Grant Nos. 20210302123223, 202103021224275);the Ph D Start-up Foundation of Taiyuan University of Science and Technology (20222119);Guo Shou Jing Telescope (the Large sky Area Multi-Object fiber Spectroscopic Telescope, LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission。
Large sky Area Multi-Object fiber Spectroscopic Telescope(LAMOST) has completed the observation of nearly 20 million celestial objects,including a class of spectra labeled “Unknown.” Besides low signal-to-noise rati...
the support provided for this research from Fundamental Research Grant Scheme code FRGS/1/2019/ STG02/UKM/02/7, which is funded by the Malaysian Ministry of Higher Education (MoHE)。
In this paper,we present the broadband(0.5–195 keV)X-ray spectral analysis for one of the newly detected AGNs in the Swift-BAT 105 month Hard X-ray Survey Catalog,NGC 4117.According to our ongoing research on low lum...