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financial support provided by the National Natural Science Foundation of China(NSFC,grant Nos.12173027,11973028,11933001,1803012,12150009,and 12173062);the National Key R&D Program of China(2019YFA0706601);the Major Key Project of PCL;the science research grants received from the China Manned Space Project with Nos.CMS-CSST-2021-B12,CMS-CSST-2021-B09 and CMS-CSST-2021-A01;the Square Kilometre Array(SKA)Project with No.2020SKA0110102;the Civil Aerospace Technology Research Project(D050105)。
The China Space Station Telescope(CSST)is a telescope with 2 m diameter,obtaining images with high quality through wide-field observations.In its first observation cycle,to capture time-domain observation data,the CSS...
supported by the National Natural Science Foundation of China(NSFC)No.11873055 and No.11933003;sponsored(in part)by the Chinese Academy of Sciences(CAS)through a grant to the CAS South America Center for Astronomy(CASSACA);support from project PID2020-114414GB-100,financed by MCIN/AEI/10.13039/501100011033;the Junta de Andaluciaía(Spain)grant FQM108;support by the National Key R&D Program of China No.2017YFA0402600;the National Natural Science Foundation of China(NSFC)grant Nos.11890692,12133008,and 12221003;China Manned Space Project No.CMS-CSST2021-A04。
We present a study of star-forming galaxies (SFGs) with pseudobulges (bulges with Sérsic index n<2) in a loca close major-merger galaxy pair sample (H-KPAIR).With data from new aperture photometries in the optical an...
the science research grants from the China Manned Space Project with No.CMS-CSST-2021-A08.Y.H;the science research grants from the China Manned Space Project with No.CMS-CSST-2021-B05;the NSFC for grant Nos.11903027 and11833006;the NSFC for grant Nos.11973001,12090040,and 12090044;the National Key R&D Program of China for grant No.2019YFA0405503.H.W.Z;the National Key R&D Program of China for grant No.2019YFA0405504。
Deriving atmospheric parameters of a large sample of stars is of vital importance to understand the formation and evolution of the Milky Way.Photometric surveys,especially those with near-ultraviolet filters,can offer...
supported by the National Key R&D Program of China(2022YFF0503401);the National Natural Science Foundation of China(12203047,12025303,11890693,12003031);the science research grants from the China Manned Space Project with NO.CMSCSST-2021-A06;the Fundamental Research Funds for the Central Universities(WK3440000006,WK2030000057)。
The Wide Field Survey Telescope(WFST)is a dedicated time-domain multi-band(u,g,r,i,and z)photometric survey facility under construction.In this paper,we present a preliminary study that assesses the quality of photome...
supported by China Manned Space Program through its Space Application System;the National Natural Science Foundation of China(NSFC,grant Nos.11973022 and U1811464);the Natural Science Foundation of Guangdong Province(No.2020A1515010710)。
Machine learning has become a crucial technique for classifying the morphology of galaxies as a result of the meteoric development of galactic data.Unfortunately,traditional supervised learning has significant learnin...
the financial support from the Council of Scientific&Industrial Research (CSIR),Government of India。
We use the recently discovered simple photometric parameter Central Intensity Ratio(CIR)determined for a sample of 57 nearby(z<0.02)Seyfert galaxies to explore the central features of galaxies and their possible conne...
supported by the fund for the Youth Project of Basic Research Program of Yunnan Province (202001BB050012);the Joint Foundation of Department of Science and Technology of Yunnan Province and Yunnan University (202201BF070001-020);funded by the“Yunnan University Development Plan for World-Class Astronomy Discipline”。
3C 66A is one of our first batches of photometric monitoring objects with the 1 m optical telescope at Yunnan University Astronomical Observatory.In the present work,the observational campaign was performed from 2021 ...
supported by the National Key R&D Program of China with No. 2021YFA1600404;the National Natural Science Foundation of China (NSFC, grant Nos. 11991051, Y911080201, 12073068, 11673062, 11703077, 11703078);the CAS “Light of West China” Program, the Yunnan Province Foundation (2019FB004, 202001AT070069);Yunnan Province Youth Top Talent Project (YNWR-QNBJ-2020-116);the science research grants from the China Manned Space Project with NO. CMS-CSST-2021-A06 and CMS-CSST2021-A05。
In order to study the physical properties of the γ-ray emitting narrow-line Seyfert 1(NLS1) galaxy population,photometric and spectral observations of the γ-ray emitting NLS1 PMN J0948+0022 were made with the Lijian...
supported by the National Natural Science Foundation of China(NSFC,Grant No.12120101003);Beijing Municipal Natural Science Foundation under grant 1222028;the China Manned Space Project with Nos.CMS-CSST-2021-A02 and CMS-CSST-2021-A04;supported by NSFC under grants 11890691,11890693,11873053,12073035,12133010,11733007;the National Key R&D Program of China under grant 2019YFA0405501。
Photometric redshift(photoz)is a fundamental parameter for multi-wavelength photometric surveys,while galaxy clusters are important cosmological probes and ideal objects for exploring the dense environmental impact on...
funded in part by the National Science Foundation(NSF 1517474,1909109);the National Aeronautics and Space Administration(NASA 17-ADAP17-68)。
The first multi-color light curve analysis of the AH Mic binary system is presented.This system has very few past observations from the southern hemisphere.We extracted the minima times from the light curves based on ...