We present the first hydrodynamical cosmological simulations in the νHDM framework
based on Milgromian dynamics (MOND) with light (11 eV) sterile neutrinos. νHDM can …

We present a physical model of the mass accretion histories (MAH) of haloes in
concordance with the observed cosmic star formation rate density (CSFRD). We model the …

In this paper, we set out to construct a set of reference mock galaxy redshift surveys
(MGRSs) for the future Chinese Space-station Survey Telescope (CSST) observation, where …

More precise measurements of galaxy clustering will be provided by the next generation of
galaxy surveys, such as DESI, WALLABY, and the Square Kilometre Array. To utilize this …

Based on the DECaLS shear catalog, we study the scaling relations between halo mass (M
h) and various proxies for Sloan Digital Sky Survey central galaxies, including stellar mass …

Cluster cosmology depends critically on how optical clusters are selected from imaging
surveys. We compare the conditional luminosity function (CLF) and weak-lensing (WL) halo …

We present a tentative constraint on cosmological parameters Ω m and σ 8 from a joint
analysis of galaxy clustering and galaxy-galaxy lensing from DESI Legacy Imaging Surveys …

As a key driver of the secular evolution of disc galaxies, bar formation is potentially linked to
the surrounding tidal field. We systematically investigate the dependence of bars on both the …

The Jiao Tong University Spectroscopic Telescope (JUST) is a 4.4-meter f/6.0
segmentedmirror telescope dedicated to spectroscopic observations. The JUST primary …

Tele-correlation refers to the correlation of galaxy shapes with large angular separations
(eg, $> 100$ degrees). Since there are no astrophysical reasons causing such a correlation …