supported by the National Key R&D Program of China No.2018YFE0120800;the National Natural Science Foundation of China grant No.11973047;the National Key R&D Program of China No.2022YFF0504300;the National SKA Program of China Nos.2020SKA0110401,and 2020SKA0110402。
Observations are beginning to constrain the history of the epoch of reionization(EoR).Modeling the reionization process is indispensable to interpret the observations,to infer the properties of ionizing sources,and to...
supported by the National SKA Program of China(Grant No.2020SKA0110401);NSFC(Grant Nos.12103044,11821303 and 11850410429);National Key R&D Program of China(Grant No.2018YFA0404502);supported in part by grants from Yunnan University。
The bubble size distribution of ionized hydrogen regions probes information about the morphology of HⅡbubbles during reionization.Conventionally,the HⅡbubble size distribution can be derived from the tomographic ima...
supported by the Key Projects of Frontier Science of Chinese Academy of Sciences(Grant No.QYZDY-SSW-SLH022);the Strategic Priority Research Program of Chinese Academy of Sciences(Grant No.XDB23000000);the National Key R&D Program of China(Grant No.2018YFA0404601)。
We present a conceptual design study of external calibrators in the 21 cm experiment towards detecting the globally averaged radiation of the epoch of reionization(EoR).Employment of external calibrator instead of int...
supported by the National Natural Science Foundation of China(Grant Nos.11988101,11890694);National Key R&D Program of China(No.2019YFA0405502);China Scholarship Council。
Estimating ages for a large number of giants is of great importance for studying Galactic evolution.In this work,we determine stellar ages and masses for 556007 giants from LAMOST Data Release 5(DR5)with empirical rel...
supported by the National Key R&D Program of China(No.2017YFB0203300);and the Key Program of the National Natural Science Foundation of China(NFSC,Grant No.11733010);W.S.Z.acknowledges support from the NSFC(Grant No.11673077);F.L.L.is supported by the NSFC(Grant No.11333008);the State Key Development Program for Basic Research of China(2015CB857000)。
The thermal history of cosmic gas in the dark ages remains largely unknown.It is important to quantify the impact of relevant physics on the IGM temperature between z=10 and z^30,in order to interpret recent and oncom...
supported by the Ministry of Science and Technology(2016YFE0100300);the National Natural Science Foundation of China(Grant Nos.11473044,U1501501,U1631118 and 11633004);the Chinese Academy of Sciences(QYZDJ-SSW-SLH017);support by the CSC Cai Yuanpei grant
Extracting the neutral hydrogen (HI) signal is a great challenge for cosmological 21 cm experiments; both the astrophysical foregrounds and receiver noise are typically several orders of magnitude greater than the 2...
supported by the National Natural Science Foundation of China(Grant Nos.11473031,11261140641 and 11173028);the 973 Program(Grant No.2013CB837900)
The cross-correlation between the high-redshift 21 cm background and the Soft X-ray Background (SXB) of the Universe may provide an additional probe of the Epoch of Reionization. Here we use semi-numerical simulatio...
partially supported by the National Natural Science Foundation of China(Grant No.11433002);support by a Marsden Fund grant in New Zealand
Detection and mitigation of radio frequency interference (RFI) is the first and also the key step for data processing in radio observations, especially for ongoing low frequency radio experiments towards the detecti...
The possibility to estimate ages and masses of Young Stellar Objects (YSOs) from their location in the Hertzsprnng-Russell diagram (HRD) or a color- magnitude diagram provides a very important tool for the investi...
supported by the Program for New Century Excellent Talents in University(NCET);the National Natural Science Foundation of China (Grant Nos.10878010,10221001 and 10633040);the National Basic Research Program (973 program No. 2007CB815405);supported by the Brazilian agencies CNPq, CAPES and FAPESP ;by the France-Brazil CAPES/Cofecub program
Stellar ages and metallicities are crucial for understanding the formation and evolution of elliptical galaxies. However, due to the age-metallicity degeneracy, it is hard to measure these two parameters accurately wi...