the National Natural Science Foundation of China(NSFC,Grant Nos.11921003,12233011,and 12373002)。
It was hypothesized in the literature that some physical parameters may be time-evolving and the astrophysical data can serve as a probe.Recently,the James Webb Space Telescope(JWST)released its early observations.In ...
supported in part by the National Key R&D Program of China(Grant No.2021YFC2203100);the National Natural Science Foundation of China(Grant Nos.11921003,11961131007,11653002,12003029,12261131497,and 12003074);China Postdoctoral Science Foundation(Grant No.2023TQ0355);CAS Young Interdisciplinary Innovation Team(Grant No.JCTD-2022-20);111 Project for“Observational and Theoretical Research on Dark Matter and Dark Energy”(Grant No.B23042);the Fundamental Research Funds for Central Universities;the CSC Innovation Talent Funds;the CAS Project for Young Scientists in Basic Research(Grant No.YSBR-006);by the USTC Research Funds of the Double First-Class Initiative。
A group of massive galaxies at redshifts of z■7 have been recently detected by the James Webb Space Telescope(JWST),which were unexpected to form at such an early time within the standard Big Bang cosmology.In this w...
supported by the National Natural Science Foundation of China(NSFC,grant No.12075246);the Fundamental Research Funds for the Central Universities;the Fundamental Research Funds for the Central Universities(grant No.E2EG6602X2 and grant No.E2ET0209X2);supported in part by the Natural Science Foundation of Henan Province and Zhengzhou University(grant Nos.242300420231,JC23149007,35220136);the China Postdoctoral Science Foundation(grant No.2021M692942);the NSFC(grant No.11905224);the NSFC(grant No,12147103);supported by the scientific research starting grants from University of Chinese Academy of Sciences(grant No.118900M061)。
Recently,observational hints for supermassive black holes have been accumulating,prompting the question:Can primordial black holes(PBHs)be supermassive,particularly with masses M■10^(9)M_(⊙)?A supercritical bubble,c...
support of Cyrus Chun Ying Tang Foundations;supported by the National Natural Science Foundation of China(Grant Nos.11921003,and 12233011);the Chinese Academy of Sciences via the Key Research Program of Frontier Sciences(Grant No.QYZDJ-SSWSYS024)。
Studies have proposed that there is evidence for cosmological coupling of black holes(BHs)with an index of k≈3;hence,BHs serve as the astrophysical source of dark energy.However,the data sample is limited for the red...
M.S.thanks DMRC for support;D.S.thanks the compeers of GD Goenka University for continuing assistance.
Gamma-ray bursts(GRBs) are among the brightest objects in the Universe and, hence, can be observed up to a very high redshift. Properly calibrated empirical correlations between intensity and spectral correlations of ...
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 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...
The Hubble constant(H_0),which represents the expansion rate of the universe,is one of the most important cosmological parameters.The recent measurements of H0using the distance ladder methods such as type Ia supernov...
This paper predicts the average luminous mass of galaxies that will be detected by JWST space telescope at redshift z ≈ 10 - 20. The prediction, derived in the paper, is based on holographic analysis, developed from ...
supported by the National Key R&D Program of China(Nos.2018YFE0202900 and 2022YFA1602901);the NSFC grant(Nos.11988101,11873051 and 12125302);NSFC grant(No.12033008);CAS Project for Young Scientists in Basic Research Grant(No.YSBR-062);the K.C.Wong Education Foundation;the National Key Research and Development of China(No.2018YFA0404503);the support by the National Natural Science Foundation of China(Nos.12047569 and 12147217);the science research grants from the China Manned Space Project with Nos.CMSCSST-2021-A03 and CMS-CSST-2021-A07;by the Natural Science Foundation of Jilin Province,China(No.20180101228JC)。
The observational data of high redshift galaxies become increasingly abundant,especially since the operation of the James Webb Space Telescope,which allows us to verify and optimize the galaxy formation model at high ...