C. Jiang

TL;DR: In this article, the bias is a multivariate function of halo properties that falls into three regimes: early-forming, low-mass and late-forming haloes, and the bias depends sensitively on the recent mass accretion history.

TL;DR: In this article, the authors used a high-resolution N-body/SPH cosmological simulation to find an accurate scaling relation between galaxy pair counts and merger rates down to a stellar mass ratio of about 1:30.

TL;DR: In this paper, an accurate scaling relation between galaxy pair counts and merger rates down to a stellar mass ratio of about 1:30 was found, which explicitly accounts for the dependence on redshift (or time), on pair separation, and on mass of the two galaxies in a pair.

TL;DR: In this article, the Lyman Alpha Galaxies at Epoch of Reionization (LAGER) survey was used to measure the luminosity functions of the H$\alpha, [OIII], and [OII] galaxies in a single 3 deg$2$ CTIO/Blanco DECam pointing of the COSMOS field.

TL;DR: In this paper, the authors investigated how H$\alpha$ equivalent width (EW) correlated with galaxy properties and how selection biases could alter such correlations using a $z = 0.47$ narrowband-selected sample of 1572 H$α$ emitters from the Ly$\α$ Galaxies in the Epoch of Reionization (LAGER) survey.