id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
x346d22079m	Ali Snedden	Evolution of Baryons in Cosmic Large Scale Structure	2015		.txt	text/plain	280	13	59	z = 3 occurs in low contrast regions of filaments, but as the density contrast increases at lower redshift, star formation switches to high contrast regions or the inner parts of filaments. Since filaments bridge between void and cluster regions, this suggests that the majority of star formation occurs in galaxies in intermediate density regions prior to the accretion onto poor clusters.	cache/x346d22079m.txt	txt/x346d22079m.txt