The discovery of massive galaxies at high redshifts,especially the passive ones,poses a big challenge for the current st......

It is well known from the Butcher-Oemler effect that galaxies in dense environment are mostly red with little star forma......

The star formation rate function(SFRF)and specific star formation rate function(sSFRF)from observations are impacted by ......

We investigate two classes of conditions for galaxy quenching at 0.5 ＜ z ＜ 2.5 based on the structural scaling relations o......

It is well known from the Butcher-Oemler effect that galaxies in dense environment are mostly red with little star forma......

The star formation rate function(SFRF) and specific star formation rate function(s SFRF) from observations are impacted ......